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    <identifier>oai:publications.copernicus.org:tc129505</identifier>
    <datestamp>2026-06-17</datestamp>
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      <dc:title><![CDATA[Detection and attribution of the role of anthropogenic climate change in industrial-era retreat of Pine Island Glacier]]></dc:title>
      <dc:creator>Bradley, Alexander T.</dc:creator>
      <dc:creator>Bett, David T.</dc:creator>
      <dc:creator>Williams, C. Rosie</dc:creator>
      <dc:creator>Arthern, Robert J.</dc:creator>
      <dc:creator>Holland, Paul R.</dc:creator>
      <dc:creator>Byrne, James</dc:creator>
      <dc:creator>Edwards, Tamsin L.</dc:creator>
      <dc:creator>Adhikari, Mira</dc:creator>
      <dc:description><![CDATA[<p>The West Antarctic Ice Sheet (WAIS) has undergone rapid change over the satellite era, characterized by significant thinning, grounding-line retreat, and mass loss. More than a third of the ice loss from this region is from Pine Island Glacier (PIG). However, robust causal links between anthropogenic climate change and PIG ice loss have yet to be established. Here we attempt to quantify the role of anthropogenic climate change in observed retreat of PIG over the 20th century and how this may evolve up to 2200. To do so, we use an ensemble Kalman inversion data assimilation method embedded into an uncertainty quantification framework, called calibrate-emulate-sample (CES). This procedure, which assimilates observations of grounding-line retreat and ice volume, yields observationally constrained probability distributions of both model and climate forcing parameters. Our analysis suggests that it is unlikely that the extent of 20th century PIG retreat would have taken place without anthropogenically driven trends in ice-sheet forcing and that anthropogenic forcing exacerbated the extent of PIG retreat over the 20th century, by approximately 18 %. These results are, importantly, conditional on our choice of initial state. For our chosen initial state, we find that the parameter combinations compatible with these observational constraints require PIG to lose mass (but not experience grounding-line retreat) over the entire simulated period since 1750, not just after the 1940s when grounding-line retreat was initiated. This preconditioned ice mass loss introduces significant uncertainty into our quantification of 20th century forcing contributions. In simulations with no anthropogenic trend in forcing, we still observe significant retreat; this may result either from a larger-than-actual initial state, or may suggest that the earlier ice state preconditioned the industrial era retreat, possibly implicating longer term changes to WAIS in the present retreat.</p>]]></dc:description>
      <dc:date>2026-06-17</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/tc-20-3443-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/3443/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:tc137931</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>tc</setSpec>
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      <dc:title><![CDATA[Comparing calving laws at Greenland's three largest ice shelves]]></dc:title>
      <dc:creator>Barnett, Jamie</dc:creator>
      <dc:creator>Holmes, Felicity A.</dc:creator>
      <dc:creator>Greenwood, Sarah L.</dc:creator>
      <dc:creator>Morlighem, Mathieu</dc:creator>
      <dc:creator>Kirchner, Nina</dc:creator>
      <dc:creator>Jakobsson, Martin</dc:creator>
      <dc:description><![CDATA[<p>The retreat of Greenlandic glaciers through calving has major implications for the ice sheet's mass balance and future sea-level rise contributions. Despite its importance, the implementation of calving in ice sheet models remains contested, with several calving laws suggested to parametrise this process. While the performance of some of these calving laws has been tested for Antarctic ice shelves and Greenland's grounded outlet glaciers, it is unclear which calving law would best capture the observed behaviour of Greenland's ice shelves. Petermann, Ryder, and Nioghalvfjerdsbræ (79N) glaciers terminate as Greenland's three largest ice shelves, accounting for 90 % of the remaining floating ice and buttressing <span class="inline-formula">∼</span> 15 % of the ice sheet's mass. Here we build on other systematic calving studies by comparing five calving laws at Greenland's three largest ice shelves using the Ice-sheet and Sea-level System Model (ISSM). We begin by constraining the performance of each law against observed terminus fluctuations between 2008 and 2024, and continue with projections to 2300 under various climate forcings. When evaluated against observed terminus changes, we recommend the use of a von Mises or Crevasse Depth calving law owing to their consistent performance and similar tuning parameters across the three ice shelves. However, in our extended projection runs, we find that calving parametrisations have little influence on grounding line discharge rates, which are instead driven by the choice of climate forcings. Large ice shelf calving or collapse events are scarce, and only in these rare cases do we find any pronounced increase in ice discharge. Our results indicate either continued buttressing potential from Greenland's ice shelves into the coming centuries or fundamental flaws in the current set of calving laws when calibrated to contemporary ice-shelf behaviour.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/tc-20-3599-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/3599/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:tc138779</identifier>
    <datestamp>2026-06-26</datestamp>
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      <dc:title><![CDATA[Winter Arctic polynyas in CMIP6 models]]></dc:title>
      <dc:creator>Heuzé, Céline</dc:creator>
      <dc:creator>Rheinlænder, Jonathan W.</dc:creator>
      <dc:creator>Tian, Tian</dc:creator>
      <dc:creator>Wong, Carmen Hau Man</dc:creator>
      <dc:description><![CDATA[<p>Winter Arctic polynyas, openings in the pack ice, play a crucial role for the climate from sea ice production to cloud formation and are hotspots for the ecosystem and human activity. Their area has significantly increased since satellite records began. Yet their representation has yet to be evaluated in any generation of global climate models, most likely because their automatic multi-model retrieval is challenging. We here use a newly-developed machine-learning based method and evaluate polynya activity against the satellite-derived one over 1979–2024 in the 18 CMIP6 models with daily sea ice concentration available. We find that models overestimate winter Arctic polynya area but underestimate its frequency, and limit their opening to the seasonally ice-covered regions. Polynya area is increasing in most models, but the bias of these trends are inconsistent. Although the model with the highest resolution has both the highest areas and frequencies, the sea ice model component is a more robust predictor of polynya activity, with most activity in the models whose thermodynamics scheme enhances ice growth/melt. Accordingly, we found more polynyas in the models with a larger seasonal cycle, in particular those with a warmer autumn that would delay ice growth or melt early. Finally, we confirm preliminary findings that polynya activity does not seem to impact the representation of the water column; if anything, we find less-dense water at the bottom of the continental shelf following larger polynya activity. Overall, our results suggest that in the Arctic, CMIP6 models unrealistically open only sensible-heat polynyas.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/tc-20-3643-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/3643/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:tc139239</identifier>
    <datestamp>2026-06-26</datestamp>
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   <metadata>
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      <dc:title><![CDATA[The new kids on the block of Arctic coasts – formation and morphodynamics of paraglacial moraine lagoons in Svalbard]]></dc:title>
      <dc:creator>Owczarek, Zofia</dc:creator>
      <dc:creator>Kostrzewa, Oskar</dc:creator>
      <dc:creator>Piskorski, Wojciech</dc:creator>
      <dc:creator>Strzelecki, Mateusz C.</dc:creator>
      <dc:description><![CDATA[<p>As Arctic amplification accelerates glacier retreat, new dynamic landscapes are emerging at the interface of terrestrial and marine systems. This study identifies and analyses a distinct coastal landform: the Paraglacial Moraine Lagoon (PML). Formed by coastal barriers composed of terminal or lateral moraines deposited during the Little Ice Age, PMLs represent a critical yet understudied component of the glacier–climate change feedback system. Using a multi-decadal record (1936–2024) comprising aerial photography, satellite imagery, and the Digital Shoreline Analysis System (DSAS), we quantified the evolution of fourteen PML systems across the Svalbard Archipelago. Our results show that PMLs now occupy over 56 % of Svalbard's total lagoon area (ca. 83 km<span class="inline-formula"><sup>2</sup></span>), nearly triple the area they occupied in the 1930s. We identify two divergent evolutionary trajectories: (1) an erosional – fragmenting pathway (e.g., Tjuvfjordlaguna), where marine forcing leads to barrier narrowing and inlet expansion, and (2) a stabilizing – isolating pathway (e.g., Femtelaguna), where land-terminating glaciers drive rapid terrestrial sediment infilling and barrier progradation. We argue that PMLs function as essential “paraglacial sinks” trapping glaciogenic sediments and organic matter, thereby creating sheltered biodiversity hubs in otherwise harsh coastal environments. As transient features, the formation and eventual destruction of PMLs serve as a high-resolution proxy for the rapid paraglacial adjustment of polar coastlines.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/tc-20-3619-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/3619/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:nhess127184</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>nhess</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Review article: Harnessing data-driven methods for climate multi-hazard and multi-risk assessment]]></dc:title>
      <dc:creator>Ferrario, Davide Mauro</dc:creator>
      <dc:creator>Sanò, Marcello</dc:creator>
      <dc:creator>Maraschini, Margherita</dc:creator>
      <dc:creator>Critto, Andrea</dc:creator>
      <dc:creator>Torresan, Silvia</dc:creator>
      <dc:description><![CDATA[<p>In recent years, interest in data-driven methods, such as machine learning and multivariate statistics for multi-hazard and multi-risk assessment has surged, due to their ability to integrate vast amounts of data in modelling complex non-linear relationships between hazard and risk factors. This review explores data-driven methods in climate multi-hazard and risk assessment, focusing on four themes: (i) data processing and collection; (ii) hazard identification, prediction and analysis; (iii) risk assessment; and (iv) future risk scenarios under climate change. Key findings highlight the extensive use of machine learning to combine Earth observations and climate data for downscaling and land use and land cover characterisation; the application of deep learning for hazard prediction; the use of ensemble methods for risk assessment; and the growing emphasis on explainable AI frameworks. Supervised machine learning approaches trained on historical impact data to project future climate risks have also emerged as a significant research area. Future research in this area should focus on modelling multi-hazard interactions, particularly triggering and cascading effects, integrating dynamic vulnerability and exposure factors, and addressing uncertainties associated with using machine learning for extrapolation. Advancements in Earth observations and textual data integration, alongside the development of open-access disaster catalogues, will also be crucial for improving multi-risk assessments and supporting AI-driven early warning systems tailored to regional needs.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-2975-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/2975/2026/]]></dc:identifier>
      <dc:source>eISSN: 1684-9981</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:ms138878</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>ms</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Research on compliance control strategy of elbow–wrist rehabilitation robot based on information fusion]]></dc:title>
      <dc:creator>Bian, Hui</dc:creator>
      <dc:creator>Shang, Hang</dc:creator>
      <dc:creator>Li, Zihan</dc:creator>
      <dc:creator>Xu, Yifan</dc:creator>
      <dc:creator>Du, Peixuan</dc:creator>
      <dc:creator>Wang, Mingzhi</dc:creator>
      <dc:creator>Liu, Runyang</dc:creator>
      <dc:creator>Luo, Ze</dc:creator>
      <dc:description><![CDATA[<p>Compliance control is the key to human–robot physical interaction, which can improve the safety and comfort of robot-assisted rehabilitation. Aiming to address the problems of the large time delay and low compliance of the system caused by the slow speed of motion intention recognition based on the force signal, this paper integrates the force signal and the surface electromyography (sEMG) signal as the input of the elbow–wrist rehabilitation robot, which improves the responsiveness of the system. To further enhance the trajectory-tracking performance of the system, a sliding-mode controller based on the double exponential reaching law (DE-SMC) is designed. Then, the force and sEMG signal fusion experiment and the compliance control experiment were carried out. The former showed that the fused force signal would judge the subject's motion intention 102.5 ms in advance, while the latter confirmed that the compliance control strategy based on the DE-SMC controller effectively improved the compliance of elbow and radioulnar joint movement.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/ms-17-685-2026</dc:identifier>
      <dc:identifier><![CDATA[https://ms.copernicus.org/articles/17/685/2026/]]></dc:identifier>
      <dc:source>eISSN: 2191-916X</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:sd134397</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>sd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Initial results from a Trans-Amazon Drilling Project core from the Acre Basin of Brazil]]></dc:title>
      <dc:creator>Fritz, Sherilyn C.</dc:creator>
      <dc:creator>Sawakuchi, André O.</dc:creator>
      <dc:creator>Noren, Anders</dc:creator>
      <dc:creator>Baker, Paul A.</dc:creator>
      <dc:creator>Silva, Cleverson</dc:creator>
      <dc:creator>Jaramillo, Carlos</dc:creator>
      <dc:creator>Almeida, Renato Paes</dc:creator>
      <dc:creator>Janikian, Liliane</dc:creator>
      <dc:creator>Bezerra, Isaac Salém</dc:creator>
      <dc:creator>Barbosa, Marcos</dc:creator>
      <dc:creator>Bertassoli, Dailson</dc:creator>
      <dc:creator>Blankenship, Rain</dc:creator>
      <dc:creator>Chiessi, Cristiano M.</dc:creator>
      <dc:creator>Feakins, Sarah J.</dc:creator>
      <dc:creator>Garcia, Maria da Glória</dc:creator>
      <dc:creator>Gautheron, Cécile</dc:creator>
      <dc:creator>Grivna, Brian</dc:creator>
      <dc:creator>Hartmann, Gelvam</dc:creator>
      <dc:creator>Kunkel, Cindy</dc:creator>
      <dc:creator>Marconato, André</dc:creator>
      <dc:creator>Martinez, Angela</dc:creator>
      <dc:creator>Marulanda, Sebastian G.</dc:creator>
      <dc:creator>Mazoca, Carlos Eduardo M.</dc:creator>
      <dc:creator>Negri, Francisco R.</dc:creator>
      <dc:creator>Parra, Mauricio</dc:creator>
      <dc:creator>Piller, Werner E.</dc:creator>
      <dc:creator>Pupim, Fabiano N.</dc:creator>
      <dc:creator>Salgado, Victor</dc:creator>
      <dc:creator>So, Rachel T.</dc:creator>
      <dc:creator>Souza, Priscila Emerich</dc:creator>
      <dc:creator>Stiles, Elena</dc:creator>
      <dc:creator>Strömberg, Caroline A. E.</dc:creator>
      <dc:creator>Tsai, Siu Mui</dc:creator>
      <dc:creator>Wahnfried, Ingo</dc:creator>
      <dc:creator>West, Josh</dc:creator>
      <dc:creator>Adaimé, Marc-Élie</dc:creator>
      <dc:creator>Afonso, Jhon</dc:creator>
      <dc:creator>Akabane, Thomas Kenji</dc:creator>
      <dc:creator>Althaus, Camila Eliza</dc:creator>
      <dc:creator>D'Apolito, Carlos</dc:creator>
      <dc:creator>Araújo, Kleiton R.</dc:creator>
      <dc:creator>Azevedo Júnior, Roney da Silva</dc:creator>
      <dc:creator>Barcellos, Jessica</dc:creator>
      <dc:creator>Bicudo, Tacio</dc:creator>
      <dc:creator>Bogota, Giovanni</dc:creator>
      <dc:creator>Bookhagen, Bodo</dc:creator>
      <dc:creator>Breda, Caio</dc:creator>
      <dc:creator>Brito, Alderlene Pimentel</dc:creator>
      <dc:creator>Carvajal, Francy</dc:creator>
      <dc:creator>Coppi, Daniel Antunes</dc:creator>
      <dc:creator>Cruz, Carolina Barbosa Leite</dc:creator>
      <dc:creator>Figueiredo, Felipe Torres</dc:creator>
      <dc:creator>Freeman, Kate</dc:creator>
      <dc:creator>Gomes, Pedro Victor Oliveira</dc:creator>
      <dc:creator>Gross, Martin</dc:creator>
      <dc:creator>Hartke, Emma</dc:creator>
      <dc:creator>Heeschen, Katja</dc:creator>
      <dc:creator>Henrichs, William Mozart</dc:creator>
      <dc:creator>Henrique, Leonardo</dc:creator>
      <dc:creator>Hoorn, Carina</dc:creator>
      <dc:creator>Horton, Brian K.</dc:creator>
      <dc:creator>Díaz-Jamamillo, Andrés</dc:creator>
      <dc:creator>Kamrani-Mehni, Said</dc:creator>
      <dc:creator>Leite, Fatima</dc:creator>
      <dc:creator>Li, Lin</dc:creator>
      <dc:creator>Lucena, Rodrigo Ferreira</dc:creator>
      <dc:creator>Milne, Alastair</dc:creator>
      <dc:creator>Miranda, Thomás</dc:creator>
      <dc:creator>Mota, Marcelo</dc:creator>
      <dc:creator>Ochoa, Diana</dc:creator>
      <dc:creator>Lima Passos, Vinicius</dc:creator>
      <dc:creator>Lopes de Paula, Rafaela Maciel</dc:creator>
      <dc:creator>Piispa, Elisa</dc:creator>
      <dc:creator>Plata Torres, Angelo</dc:creator>
      <dc:creator>Punyasena, Surangi W.</dc:creator>
      <dc:creator>Reis, Adriano Domingos</dc:creator>
      <dc:creator>Rigsby, Catherine</dc:creator>
      <dc:creator>Salazar Rios, Andrés F.</dc:creator>
      <dc:creator>Rodrigues, Fernanda Costa Gonçalves</dc:creator>
      <dc:creator>Romão, Raquel M. M.</dc:creator>
      <dc:creator>Romero, Ingrid C.</dc:creator>
      <dc:creator>Sawakuchi, Henrique O.</dc:creator>
      <dc:creator>Schnurrenberger, Doug</dc:creator>
      <dc:creator>Shannon, Kristina Brady</dc:creator>
      <dc:creator>Silva-Caminha, Silane A. F.</dc:creator>
      <dc:creator>Sousa, Clauses</dc:creator>
      <dc:creator>Tamura, Larissa Natsumi</dc:creator>
      <dc:creator>Wiersberg, Thomas</dc:creator>
      <dc:creator>Xiang, Helanlin</dc:creator>
      <dc:creator>Zamudio, Belén</dc:creator>
      <dc:description><![CDATA[<p>The Trans-Amazon Drilling Project (TADP) is reconstructing the late Cenozoic history of Amazonian geology, climate, rivers, and forests. Drilling in the Acre Basin of western Brazil in 2023 recovered an 860 m drill core characterized by sediments that were deposited in a large paleo-river system. The overall sequence includes sandstones, siltstones, and mudstones that underwent varied degrees of weathering and pedogenesis. Here, we describe the ongoing geochronologic, geochemical, mineralogical, geophysical, and biotic analyses of the sedimentary record and present some preliminary inferences of the environmental history based on these initial results.</p>        <p>Except for the uppermost <span class="inline-formula">∼</span> 12 m, sediments from the drill core represent a single lithostratigraphic unit, assigned to the Solimões Formation, which is dominated by feldspar-rich sands of Andean origin. The pollen assemblage is quite different from Early to Middle Miocene floras that have been analyzed from a few sites elsewhere in the western Amazon. The novel pollen assemblage and new geochronological results suggest that the sequence may span the latest Miocene and all of the Pliocene Epoch, an interval that currently is not well represented in existing regional records and that is crucial for understanding the evolution of Amazonian biodiversity, as well as landscape transformations driven by Andean uplift and global climate change.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/sd-35-127-2026</dc:identifier>
      <dc:identifier><![CDATA[https://sd.copernicus.org/articles/35/127/2026/]]></dc:identifier>
      <dc:source>eISSN: 1816-3459</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:os136991</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>os</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Dynamically downscaled future projections of the Northwest Atlantic Ocean across low to high emissions scenarios]]></dc:title>
      <dc:creator>Kim, Dongmin</dc:creator>
      <dc:creator>Ross, Andrew C.</dc:creator>
      <dc:creator>Shin, Sang-Ik</dc:creator>
      <dc:creator>Gomez, Fabian A.</dc:creator>
      <dc:creator>John, Jasmin G.</dc:creator>
      <dc:creator>Volkov, Denis L.</dc:creator>
      <dc:creator>Lee, Sang-Ki</dc:creator>
      <dc:creator>Alexander, Michael A.</dc:creator>
      <dc:creator>Stock, Charles A.</dc:creator>
      <dc:description><![CDATA[<p>We used a high-resolution (1<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="1b4178c77ca0d4bfee6c9ddd864f3a43"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="os-22-1987-2026-ie00001.svg" width="8pt" height="14pt" src="os-22-1987-2026-ie00001.png"/></svg:svg></span></span>12°) Modular Ocean Model version 6 implementation for the Northwest Atlantic Ocean (MOM6-NWA12) to dynamically downscale Geophysical Fluid Dynamics Laboratory Earth System Model version 4.1 (GFDL-ESM4.1) projections for the 21st century. Simulations were conducted under four different Coupled Model Intercomparison Project Phase 6 emission scenarios. MOM6-NWA12 accurately simulates the spatial patterns of sea surface temperature, salinity, and dynamic sea surface height (SSH) during the historical period. In particular, the Gulf Stream's strength, position, recirculation, and separation from the US East Coast are significantly improved in MOM6-NWA12 compared to the coarse-resolution GFDL-ESM4.1. Projected end-of-century warming varied strongly between scenarios, from <span class="inline-formula">∼4 °C</span> under prior “worst case” emissions scenarios (SSP-585), <span class="inline-formula">2∼3 °C</span> under intermediate scenarios (SSP-245, SSP-370) more consistent with current trajectories, to <span class="inline-formula">∼1 °C</span> under aggressive mitigation (SSP-126). Consistent with a significant weakening of the Atlantic Meridional Overturning Circulation projected by GFDL-ESM4.1, MOM6-NWA12 shows a substantial volume transport reduction in the Western Boundary Current (WBC) system (i.e., Yucatan Current, Florida Current, Antilles Current, and the Deep Western Boundary Current) toward the late 21st century (between 23 % and 38 %, varying by scenario). This projected weakening of the WBC system and the associated reduction in the coastal upwelling of cold, fresh subsurface waters lead to a significant increase in ocean temperature, salinity, and dynamic SSH along the US southeast and northeast Coasts, particularly in the South Atlantic Bight.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-1987-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/1987/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:os137340</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>os</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Modulation of internal tides properties off the Vitória–Trindade ridge during contrasted seasons from altimetry and a regional ocean model]]></dc:title>
      <dc:creator>Bauchot, Perrine</dc:creator>
      <dc:creator>Koch-Larrouy, Ariane</dc:creator>
      <dc:creator>Tchilibou, Michel</dc:creator>
      <dc:creator>Carrère, Loren</dc:creator>
      <dc:creator>Hernandez, Fabrice</dc:creator>
      <dc:creator>Morvan, Guillaume</dc:creator>
      <dc:creator>Chanut, Jérôme</dc:creator>
      <dc:description><![CDATA[<p>The incoherent fraction of internal tides, generated through interactions with mesoscale eddies and other transient oceanic features, remains poorly understood and challenging to predict. This limits our ability to accurately represent energy transfers and mixing induced by these waves. The Vitória–Trindade Ridge off the Brazilian shelf is a relevant natural laboratory to investigate these processes, as a hotspot for internal tides generation embedded in a region of intense mesoscale activity. To assess how seasonal stratification and mesoscale variability modulate internal tides, we compared a 27-year satellite altimetry record with a high-resolution (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">36</mn><mi mathvariant="italic">°</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="31pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="d4268fa047360fee46e06ee4f821ce16"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="os-22-2011-2026-ie00001.svg" width="31pt" height="14pt" src="os-22-2011-2026-ie00001.png"/></svg:svg></span></span>) regional simulation using NEMO v4.0.2. This joint analysis allows us to characterize the generation, propagation, and dissipation of internal tides under two contrasted regimes: austral winter (defined here from May to October) marked by a deep pycnocline, and austral summer (defined here from November to April) with a shallower and sharper seasonal pycnocline. Both model and observations depict six intense, in-phase beams of the baroclinic flux propagating southward from the ridge. The first two have a wavelength of 100 <span class="inline-formula">km</span> approximately corresponding to the mode-1 of propagation, while more distant beams are spaced by about 50 <span class="inline-formula">km</span> only, which likely corresponds to the mode-2 of propagation. Quantification from the model shows that generation rates are 5 <span class="inline-formula">%</span>–15 <span class="inline-formula">%</span> higher in summer than in winter. Dissipation occurs predominantly near the ridge (45 <span class="inline-formula">%</span>) but also extends offshore (40 <span class="inline-formula">%</span>), reaching beyond 2–3 mode-1 wavelengths. In the open ocean, dissipation is up to 40 <span class="inline-formula">%</span> stronger in winter, leading to a weaker baroclinic flux propagating on shorter distances compared to summer. Altimetry confirms seasonal variations in both wavelength and amplitude, especially for mode-2 internal tides. Finally, a representative case of interaction between internal tides and a mesoscale eddy is documented under summer conditions, showing deviation and diffraction of the baroclinic flux. This study demonstrates that mesoscale variability and seasonal stratification jointly modulate the coherence and energy pathways of internal tides. These findings are essential for improving predictions of the incoherent tide and for interpreting high-resolution altimetric observations.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-2011-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/2011/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:hess135362</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>hess</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Daily drought prediction in the Huaihe River Basin  using VMD-informer-LSTM]]></dc:title>
      <dc:creator>Li, Min</dc:creator>
      <dc:creator>Ou, Ming</dc:creator>
      <dc:creator>Yao, Yuhang</dc:creator>
      <dc:creator>Yin, Changman</dc:creator>
      <dc:description><![CDATA[<p>Accurate drought prediction is a key challenge in water resource management and agricultural planning. This study proposes a novel drought prediction framework that integrates Variational Mode Decomposition (VMD), Informer, and Long Short-Term Memory (LSTM) networks to enhance hydrological drought forecasting in the Huaihe River Basin, China. The VMD-Informer-LSTM model decomposes complex non-stationary drought sequences into multi-scale components, effectively extracting long-term trends and short-term fluctuations. Results show that the model outperforms LSTM, Transformer-LSTM, and Informer-LSTM, improving <span class="inline-formula"><i>R</i><sup>2</sup></span>, RMSE, MAE, and MAPE by 28.4 %, 46.2 %, 46.5 %, and 50.8 %, respectively, over the baseline LSTM. When the prediction period is 30 d, the VMD-Informer-LSTM achieves the highest prediction accuracy. During the 120–180 d prediction period, the prediction accuracy of all models declines, with drought intensity generally underestimated. Misclassifications are mainly concentrated in the transition zones between humid and semi-humid regions, with higher error frequency in semi-humid areas. Prediction accuracy is highest in the upstream and downstream regions, followed by the Yishuisi River Basin, while the midstream region performs poorly due to human interference. Shapley Additive Explanations (SHAP) further reveal that precipitation and temperature are the dominant meteorological drivers, jointly accounting for nearly half of the model's predictive power. These results confirm that the VMD-Informer-LSTM provides the most accurate predictions among the tested models, offering valuable support for drought risk assessment and water resource management in the Huaihe River Basin and other similar regions.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-3925-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/3925/2026/]]></dc:identifier>
      <dc:source>eISSN: 1607-7938</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd140440</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[GRIT-ADB: A Global Attribute Database for the GRIT Hydrography]]></dc:title>
      <dc:creator>Zhang, Boen</dc:creator>
      <dc:creator>Wortmann, Michel</dc:creator>
      <dc:creator>Liu, Yinxue</dc:creator>
      <dc:creator>Kratzert, Frederik</dc:creator>
      <dc:creator>Moulds, Simon</dc:creator>
      <dc:creator>Slater, Louise</dc:creator>
      <dc:description><![CDATA[Global hydro-environmental databases provide essential information for large-scale hydrological, ecological, geomorphological, and Earth system analyses. Most existing global databases are built upon convergent river representations that do not explicitly capture bifurcating, multi-channel river systems. In addition, these databases primarily characterise long-term climatological means or static representations of environmental conditions derived from earlier-generation global datasets, limiting their applicability for time-varying analyses of hydroclimatic and geomorphological processes. Here we present GRIT-ADB, a new attribute database for the vectorised Global River Topology (GRIT), a new river hydrography dataset created from a 30 m resolution river mask and terrain data that provides a topology-explicit and physically realistic representation of river networks including divergent flow pathways. GRIT-ADB provides standardised hydro-environmental information for 19.6 million km of rivers and streams. It currently comprises 64 time-varying (multi-dimensional embeddings) and 35 static variables (&gt;300 attributes), spanning five categories: hydrology, physiography, climate, land cover and use, and soils and geology. Attributes are derived by aggregating and harmonising data from state-of-the-art global datasets and are accumulated along the river network from headwaters to basin outlets, while preserving the topology of divergent and complex flow pathways. The attributes are linked to multiple GRIT scales, including hierarchically-nested subbasins, individual river reaches of up to 1 km long, and coarser-scale river segments of several kilometres long, providing a flexible framework that can accommodate future extensions of GRIT and additional attributes. By combining a standardised attribute framework with explicit representation of bifurcating river hydrography, GRIT-ADB enables improved large-scale yet high-resolution analyses of river connectivity, hydrological extremes, hydro-ecological processes, and climate impacts in complex river systems, supporting a wide range of global hydrological and environmental applications.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-279</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-279/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd136001</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Next-generation Metop ASCAT surface soil moisture datasets from EUMETSAT H SAF]]></dc:title>
      <dc:creator>Hahn, Sebastian</dc:creator>
      <dc:creator>Melzer, Thomas</dc:creator>
      <dc:creator>Wagner, Wolfgang</dc:creator>
      <dc:description><![CDATA[<p>This article presents the latest version of the Advanced Scatterometer (ASCAT) surface soil moisture (SSM) dataset provided by the Satellite Application Facility on Support to Operational Hydrology and Water Management (H SAF) lead by the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT). This new release brings the operational near real-time (NRT) product up to date with the historical offline data record. For years, the H SAF ASCAT SSM data records have benefited from successive algorithmic improvements while the H SAF ASCAT SSM NRT product has only received minor updates until its discontinuation in July 2025. A new processing chain replaces the previous service and applies the latest soil moisture retrieval algorithm to both data streams, creating a unified offline/NRT dataset and representing a major advancement for the H SAF ASCAT SSM NRT product. The H SAF ASCAT SSM climate data record (CDR) covers the time period 1 January 2007 until 31 December 2024, which is extended offline by an interim climate data record (ICDR) as well as in NRT.</p>        <p>The new release also introduces a high-resolution 6.25 km sampling H SAF ASCAT SSM dataset, alongside the standard 12.5 km sampling SSM dataset. This is achieved by customising the spatial resampling process of the ASCAT Level 1B full-resolution backscatter data. A new key development in the algorithm for ASCAT SSM concerns the estimation of the dry and wet backscatter references. Specifically, a moving-window approach is now applied to mitigate artificial trends caused by long-term land cover changes. Furthermore, a new monthly subsurface scattering flag has been added to filter out unreliable SSM measurements where backscatter and soil moisture indicate an inverted relationship.</p>        <p>Quality control of the H SAF ASCAT SSM datasets is performed by using soil moisture estimates from Noah GLDAS-2.1 and the ESA CCI Passive Soil Moisture (SM) v09.1 product, as well as in-situ observations provided by the International Soil Moisture Network (ISMN). The validation results show that both H SAF ASCAT SSM datasets have a comparable performance in terms of the Pearson correlation coefficient (H SAF ASCAT SSM 6.25 km vs ESA CCI Passive SM: 17.9 % <span class="inline-formula">&gt;</span> 0.75 and 57.8 % <span class="inline-formula">&gt;</span> 0.5; H SAF ASCAT SSM 12.5 km vs ESA CCI Passiv SM: 19.6 % <span class="inline-formula">&gt;</span> 0.75 and 59.2 % <span class="inline-formula">&gt;</span> 0.5) and signal-to-noise ratio (SNR) derived using triple collocation analysis (H SAF ASCAT SSM 6.25 km SNR: 56.0 % <span class="inline-formula">&gt;</span> 0 <span class="inline-formula">dB</span>, 35.6 % <span class="inline-formula">&gt;</span> 3 <span class="inline-formula">dB</span>, H SAF ASCAT SSM 12.5 km SNR: 58.1 % <span class="inline-formula">&gt;</span> 0 <span class="inline-formula">dB</span>, 38.6 % <span class="inline-formula">&gt;</span> 3 <span class="inline-formula">dB</span>). The best agreement can be found in regions with strong seasonal variability, including monsoonal, savanna, Mediterranean, and tropical wet-and-dry zones. A weaker consistency can be found in areas characterised by limited soil moisture variability (such as deserts), dense vegetation, pronounced topographic complexity, wetland areas, or higher latitudes (<span class="inline-formula">&gt;</span> 60<span class="inline-formula"><sup>∘</sup></span> N) experiencing longer periods of frozen soil and snow cover.</p>        <p>The H SAF ASCAT SSM CDR and ICDR datasets (6.25 km sampling: <a href="https://doi.org/10.15770/EUM_SAF_H_0012">https://doi.org/10.15770/EUM_SAF_H_0012</a>, <span class="cit" id="xref_altparen.1"><a href="#bib1.bibx72">H SAF</a>, <a href="#bib1.bibx72">2025</a><a href="#bib1.bibx72">c</a></span>, and 12.5 km sampling: <a href="https://doi.org/10.15770/EUM_SAF_H_0011">https://doi.org/10.15770/EUM_SAF_H_0011</a>, <span class="cit" id="xref_altparen.2"><a href="#bib1.bibx70">H SAF</a>, <a href="#bib1.bibx70">2025</a><a href="#bib1.bibx70">a</a></span>) are publicly available online <span class="cit" id="xref_paren.3">(<a href="#bib1.bibx70">H SAF</a>, <a href="#bib1.bibx70">2025</a><a href="#bib1.bibx70">a</a>, <a href="#bib1.bibx72">c</a>, <a href="#bib1.bibx73">d</a>, <a href="#bib1.bibx74">e</a>)</span>, while H SAF ASCAT SSM NRT datasets <span class="cit" id="xref_paren.4">(<a href="#bib1.bibx71">H SAF</a>, <a href="#bib1.bibx71">2025</a><a href="#bib1.bibx71">b</a>, <a href="#bib1.bibx75">f</a>)</span> are distributed via the broadcasting system EUMETCast.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-4393-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/4393/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd134745</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[BEACH: Barbados and Eastern Atlantic Combined High-altitude dropsonde datasets]]></dc:title>
      <dc:creator>Gloeckner, Helene Marie</dc:creator>
      <dc:creator>Mieslinger, Theresa</dc:creator>
      <dc:creator>Robbins-Blanch, Nina</dc:creator>
      <dc:creator>George, Geet</dc:creator>
      <dc:creator>Kluft, Lukas</dc:creator>
      <dc:creator>Kölling, Tobias</dc:creator>
      <dc:creator>Bony, Sandrine</dc:creator>
      <dc:creator>Windmiller, Julia Miriam</dc:creator>
      <dc:creator>Stevens, Bjorn</dc:creator>
      <dc:description><![CDATA[<p>As part of the ORCESTRA field campaign in August and September 2024, 1191 dropsondes were deployed over the Eastern and Western Atlantic ITCZ from the HALO aircraft coordinated by the PERCUSION and MAESTRO subcampaigns. Here, we describe the hierarchy and processing of the resulting Barbados and Eastern Atlantic Combined High-altitude (BEACH) dropsonde datasets. The Level 0 dataset contains measured meteorological variables, such as relative humidity (RH), temperature (<span class="inline-formula"><i>T</i></span>), pressure (<span class="inline-formula"><i>p</i></span>), eastward (<span class="inline-formula"><i>u</i></span>), and northward (<span class="inline-formula"><i>v</i></span>) wind data as output by the AVAPS system. The corresponding ASPEN quality-controlled data is called Level 1. Level 2 adds further measurement-specific quality control flags. Level 3 builds the core of BEACH including all quality controlled dropsonde profiles interpolated to a common 10 m altitude grid and concatenated into a single dataset. We further derive mesoscale vorticity, divergence, and vertical velocities from 87 circular flight patterns in Level 4 using the regression method. These area-averaged variables will guide our understanding of mesoscale processes acting within the ITCZ, one of the main goals of ORCESTRA. All data levels are openly available on IPFS, while the processing code is made public on GitHub.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-4425-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/4425/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd134172</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[CAMELS-GB v2: hydrometeorological time series and landscape attributes for 671 catchments in Great Britain]]></dc:title>
      <dc:creator>Coxon, Gemma</dc:creator>
      <dc:creator>Zheng, Yanchen</dc:creator>
      <dc:creator>Barbedo, Rafael</dc:creator>
      <dc:creator>Cooper, Hollie</dc:creator>
      <dc:creator>Fileni, Felipe</dc:creator>
      <dc:creator>Fowler, Hayley J.</dc:creator>
      <dc:creator>Fry, Matt</dc:creator>
      <dc:creator>Green, Amy</dc:creator>
      <dc:creator>Gribbin, Tom</dc:creator>
      <dc:creator>Harfoot, Helen</dc:creator>
      <dc:creator>Lewis, Elizabeth</dc:creator>
      <dc:creator>Neto, Germano Gondim Ribeiro</dc:creator>
      <dc:creator>Qiu, Xiaobin</dc:creator>
      <dc:creator>Salwey, Saskia</dc:creator>
      <dc:creator>Wendt, Doris E.</dc:creator>
      <dc:description><![CDATA[<p>Large-sample hydrological datasets containing data for tens to thousands of catchments are invaluable for hydrological process understanding and modelling. CAMELS (Catchment Attributes and MEteorology for Large-sample Studies) datasets provide hydro-meteorological timeseries, catchment attributes and catchment boundaries. Here, we present the second version of CAMELS-GB. CAMELS-GB v2 collates millions of observations from across Great Britain at hourly to monthly timescales, including quality-controlled daily river flows, catchment boundaries, and catchment characteristics from the UK National River Flow Archive. The new features include (1) extended daily hydro-meteorological timeseries from 1970–2022 including meteorological timeseries from new observed climate datasets, (2) hourly precipitation, river flow and level timeseries, (3) groundwater level timeseries and attributes for 55 groundwater wells, and (4) new catchment attributes characterising changing land cover, peak flows and human influences. These data are provided for 671 catchments across Great Britain spanning a diverse range of geophysical characteristics and human influences. CAMELS-GB v2 represents a step change for environmental and modelling analyses across Great Britain, particularly for the characterisation of sub-daily hydrological processes, and is made available as an open dataset (Coxon et al., 2025; <a href="https://doi.org/10.5285/9a46d428-958f-4ac1-86eb-94eee70c0955">https://doi.org/10.5285/9a46d428-958f-4ac1-86eb-94eee70c0955</a>).</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-4345-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/4345/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd132763</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[CropPlantHarvest: a 500&thinsp;m annual dataset of crop planting and harvesting dates (2001–2024) of the U.S. Midwest]]></dc:title>
      <dc:creator>Liu, Yin</dc:creator>
      <dc:creator>Diao, Chunyuan</dc:creator>
      <dc:description><![CDATA[<p>As key components of agricultural management, planting and harvesting schedules have strongly influenced crop production by defining the length of the crop growing season and shaping the environmental conditions crops experience. Accurate knowledge of these management data is crucial for enhancing crop yield estimates by capturing the timing of crop development relative to weather and soil conditions, assessing climate adaptation by tracking shifts in farming practices over time, and supporting agricultural carbon accounting. Yet, existing planting and harvesting date datasets are largely based on state-level statistics or rule-based calendars that overlook intra-regional variability and the influence of human decision-making. The absence of long-term, high-resolution planting and harvesting date information hinders our ability to reconstruct historical agricultural practices and assess their agronomic and environmental consequences. In this study, we introduce CropPlantHarvest, the first dataset of annual corn and soybean planting and harvesting dates across the U.S. Midwest at 500 m resolution from 2001 to 2024. Planting dates are estimated using CropSow, an integrative remotely sensed crop modeling system that aligns simulated crop growth trajectories with satellite observations to retrieve field-level planting dates. Harvesting dates are retrieved using the Normalized Harvest Phenology Index (NHPI), a novel index that integrates Normalized Difference Vegetation Index (NDVI) and near-infrared (NIR) reflectance to detect harvesting events by capturing the distinct spectral transition from senescent crops to exposed crop residues. Validation against USDA crop progress reports and field-level dataset demonstrates high accuracy of CropPlantHarvest, with a mean absolute error of approximately 5 d for both crop species. This large spatial and temporal dataset captures management-driven variability in crop season timing and duration, supporting improved modeling of crop yields, greenhouse gas emissions, and resource use. It could also serve as a benchmark for refining remote-sensing phenology products and evaluating the agro-environmental impacts of evolving crop management decisions. CropPlantHarvest is available at <a href="https://doi.org/10.5281/zenodo.16967482">https://doi.org/10.5281/zenodo.16967482</a> (Liu and Diao, 2025).</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-4373-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/4373/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:esd129877</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Regional impacts of irrigation on the  atmospheric and terrestrial water cycle of  the Iberian Peninsula in a climate model]]></dc:title>
      <dc:creator>Tiengou, Pierre</dc:creator>
      <dc:creator>Ducharne, Agnès</dc:creator>
      <dc:creator>Cheruy, Frédérique</dc:creator>
      <dc:description><![CDATA[<p>This study presents regional simulations over the Iberian Peninsula between 2010 and 2022 with the atmospheric (ICOLMDZ) and land surface (ORCHIDEE) components of the IPSL climate model  in a new limited area model configuration (25 km resolution). It uses a recently developed river routing and irrigation scheme based on a water-conservative supply-and-demand approach. Two simulations, with and without irrigation, are compared to isolate the impacts of simulated irrigation on land-atmosphere interactions and the water cycle. First, an evaluation of the simulations is conducted to characterize existing model biases in river discharge, precipitation, evapotranspiration (ET) and surface soil moisture (SSM), and assess whether they can be improved by simulating irrigation. The simulated irrigation is too low in southern Spain because of a lack of available water in the reservoirs, and likely because of the absence of representation of river dams. In northern regions such as the Ebro Valley, the simulated irrigation is more realistic and reduces the biases of river discharge and ET in summer and autumn. In general, SSM is not strongly impacted by irrigation as most additional water is evaporated. Second, atmospheric changes induced by irrigation are studied in summer (JJA). Large atmospheric responses are found over intensely irrigated areas, mainly consisting of a shift in energy partitioning between the turbulent fluxes (increase in latent heat flux and decrease in sensible heat flux, up to 50 <span class="inline-formula">W m<sup>−2</sup></span>), and a lowering of the atmospheric boundary layer (<span class="inline-formula">−100</span> m) and of the lifting condensation level (<span class="inline-formula">−250</span> m). Increases in precipitation are statistically significant only over the mountainous areas surrounding the Ebro Valley, and are closely linked to increases in convective available potential energy. Finally, atmospheric moisture recycling over the Iberian Peninsula is identified by showing that the increase in ET in the presence of irrigation exceeds the amount of water added by irrigation. This is made possible by an increase in precipitation over land, although most of this increase is located in lightly irrigated areas rather than in intensively irrigated areas. These results point to remote atmospheric effects of irrigation and motivate further investigation into land-atmosphere coupling processes in the presence of irrigation in the IPSL model.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-843-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/843/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd135507</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[A systematic atmospheric parameter optimization method to improve ENSO simulation in the ICON XPP Earth system model]]></dc:title>
      <dc:creator>Yu, Dakuan</dc:creator>
      <dc:creator>Dommenget, Dietmar</dc:creator>
      <dc:creator>Pohlmann, Holger</dc:creator>
      <dc:creator>Müller, Wolfgang A.</dc:creator>
      <dc:description><![CDATA[<p>The El Niño–Southern Oscillation (ENSO) is a dominant mode of interannual climate variability, yet accurately simulating ENSO in climate models remains a major challenge due to its complex coupled dynamics. In this study, we present a linear optimization framework and systematically adjust atmospheric parameters to improve ENSO fidelity in the Icosahedral Nonhydrostatic eXtended Predictions and Projections (ICON XPP) Earth System Model of the Max-Planck-Institute for Meteorology. The optimization approach is based on the superposition of parameter sensitivities and a Nelder–Mead algorithm that reduces the ENSO cost function. The cost function accounts for ENSO-related tropical climatology, variability, and feedbacks, which are estimated with the ENSO metric package. We first assess the sensitivity of ENSO metrics to 21 atmospheric parameters in atmosphere-only simulations. The optimization approach reduces the ENSO cost function by 30 % in the optimized atmosphere-only runs. Key improvements include reduced precipitation bias and strengthened atmospheric feedbacks such as the Bjerknes and thermal damping feedbacks. These results demonstrate the effectiveness of our method in improving ENSO metrics within the atmosphere-only configuration. Six parameters identified as most impactful from atmosphere-only tuning experiments are subsequently tuned in fully coupled simulations. The optimized fully coupled run yields moderate improvements in ENSO amplitude, cold tongue SST bias, seasonal phase-locking, ocean-atmosphere coupling and teleconnection patterns. However, isolated ENSO tuning introduces unrealistic global warming, which is further corrected by adjusting turbulence-related parameters without degrading ENSO skill. These results demonstrate that systematic ENSO tuning can yield performance gains but must be balanced with broader climate stability constraints. Our method offers a scalable, physically grounded optimization strategy, with strong potential for tuning ENSO in climate model configurations.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-5531-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/5531/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:amt139184</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>amt</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Design, operation and characterization of a mobile laboratory for hyperlocal atmospheric research]]></dc:title>
      <dc:creator>Cliff, Samuel J.</dc:creator>
      <dc:creator>Giordano, Michael R.</dc:creator>
      <dc:creator>McNamara Byrne, Haley</dc:creator>
      <dc:creator>Weber, Robert J.</dc:creator>
      <dc:creator>Hebert, Jude Z.</dc:creator>
      <dc:creator>Huang, Kyle</dc:creator>
      <dc:creator>Goldstein, Allen H.</dc:creator>
      <dc:creator>Apte, Joshua S.</dc:creator>
      <dc:description><![CDATA[<p>Mobile laboratories equipped with research grade instrumentation make it possible to accurately observe fine scale (<span class="inline-formula">&lt;</span> 10 m) concentration gradients driven by local emissions, chemistry and meteorology. The flexibility afforded in measurement location makes mobile monitoring well suited to local pollution source characterization and rapid response to natural and anthropogenic situations. However, constructing a platform capable of these measurements requires simultaneous consideration of many engineering challenges and previous examples are rarely documented in enough open detail for replication. Here, we present the design process and engineering decisions behind the UC Berkeley Mobile Air Pollution Laboratory (CalMAPLab). Built into a Ford Transit 250 van, the laboratory delivers extensive chemical speciation of air pollution in the gaseous and particulate phases. We characterize the performance of the electrical system, climate control and instrumentation suite for mobile measurements with over 500 h of test driving. In addition, we introduce an open-source data acquisition system with live geospatial visualization that facilitates emissions plume mapping throughout a neighborhood. Our detailed description and open design of each critical component reduces the barrier to entry for high-performance mobile monitoring in hyperlocal atmospheric research.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-4201-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/4201/2026/]]></dc:identifier>
      <dc:source>eISSN: 1867-8548</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:amt137995</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>amt</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Improving imputation of missing PM2.5 speciation data using PMF-informed source-receptor relationships]]></dc:title>
      <dc:creator>Zhu, Wubin</dc:creator>
      <dc:creator>Xie, Mingjie</dc:creator>
      <dc:creator>Dai, Qili</dc:creator>
      <dc:creator>Bi, Xiaohui</dc:creator>
      <dc:creator>Zhang, Yufen</dc:creator>
      <dc:creator>Feng, Yinchang</dc:creator>
      <dc:description><![CDATA[<p>Missing values are ubiquitous in atmospheric monitoring due to instrument drift, calibration cycles, operational interruptions, and other random malfunctions. Such gaps can undermine the reliability of subsequent analyses and introduce systematic biases. Conventional imputation methods, such as geometric mean substitution, K-nearest neighbor (KNN), Bayesian principal component analysis (BPCA), and deep learning models often rely primarily on statistical correlations, may require auxiliary inputs, and offer limited physical interpretability. To address this issue, we propose a novel source-receptor-informed Positive Matrix Factorization Reconstruction (PMFr) method that leverages PMF-derived source-receptor relationships, rather than purely statistical interpolation, to impute missing PM<span class="inline-formula"><sub>2.5</sub></span> speciation data without requiring auxiliary data. Benchmarking on a two-month dataset against commonly used imputation techniques, including KNN, BPCA, and a deep learning predictive model, demonstrates that PMFr achieves superior accuracy and robustness across real-world missing scenarios, with a mean coefficient of determination (<span class="inline-formula"><i>R</i><sup>2</sup></span>) of 0.81, index of agreement (IoA) of 0.92, and mean absolute percentage error (MAPE) of 22.8 %, reducing MAPE by 25.5 %–29.1 %, particularly for key PM<span class="inline-formula"><sub>2.5</sub></span> species. Further PMF-based validation shows that PMFr better preserves source-profile composition and source-contribution temporal features, indicating that the completed dataset retains more physically meaningful source information and is more suitable for source apportionment. These results highlight PMFr as a robust and physically interpretable approach for reconstructing reliable PM<span class="inline-formula"><sub>2.5</sub></span> speciation data.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-4219-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/4219/2026/]]></dc:identifier>
      <dc:source>eISSN: 1867-8548</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:acp135920</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>acp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Anthropogenic modulation of dust-dominated ice nucleation in an urban dryland city of China during winter and spring]]></dc:title>
      <dc:creator>Chen, Chengqing</dc:creator>
      <dc:creator>Wang, Yang</dc:creator>
      <dc:creator>Li, Jiming</dc:creator>
      <dc:creator>Feng, Lu</dc:creator>
      <dc:creator>Chai, Tianrong</dc:creator>
      <dc:creator>Ji, Zhao</dc:creator>
      <dc:creator>Wang, Jian</dc:creator>
      <dc:creator>Wang, Yuan</dc:creator>
      <dc:description><![CDATA[<p>Ice-nucleating particles (INPs) are crucial for cloud and precipitation modulation, yet their spatiotemporal variability and sources sampled from urban dryland regions remain poorly understood. While natural dust is recognized as a substantial source of INPs, its interaction and quantity with anthropogenic pollutants, as well as INP abundance of the mixtures, remain insufficiently quantified. Here, we present online observations of INPs (<span class="inline-formula">−</span>15 to <span class="inline-formula">−</span>35 °C), together with co-located aerosol size distribution and chemical composition in Lanzhou from winter 2024 to spring 2025. We show that long-range dust transport boosts INP concentrations by a factor of 15 at <span class="inline-formula">−</span>30 °C in an urban region. Elevated secondary inorganic aerosol was observed during winter pollution events and negatively correlated with INP activity (<span class="inline-formula"><i>R</i></span> <span class="inline-formula">=</span> <span class="inline-formula">−</span>0.71). We further refine an INP parameterization based on aerosol size (1–2.5 <span class="inline-formula">µ</span>m) and freezing temperature, reproducing 83 % of observations within a factor of 5. These findings underscore the need to include local aerosol heterogeneity and dust-pollution interactions in INP parameterizations for more accurate regional climate simulations.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-9017-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/9017/2026/]]></dc:identifier>
      <dc:source>eISSN: 1680-7324</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:acp132540</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>acp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Residential burning is a potentially significant source of soluble iron to the ocean]]></dc:title>
      <dc:creator>Li, Rui</dc:creator>
      <dc:creator>Plaas, Haley E.</dc:creator>
      <dc:creator>Zhang, Yifan</dc:creator>
      <dc:creator>Chen, Yizhu</dc:creator>
      <dc:creator>Zhang, Tianyu</dc:creator>
      <dc:creator>Yang, Yi</dc:creator>
      <dc:creator>Rathod, Sagar</dc:creator>
      <dc:creator>Zhang, Guohua</dc:creator>
      <dc:creator>Wang, Xinming</dc:creator>
      <dc:creator>Hamilton, Douglas S.</dc:creator>
      <dc:creator>Tang, Mingjin</dc:creator>
      <dc:description><![CDATA[<p>Understanding the physicochemical processes that supply atmospheric aerosol iron (Fe) to the ocean is crucial for understanding of global biogeochemical cycles. Anthropogenic activity contributes significant fluxes of aerosol Fe to the atmosphere, the soluble fraction of which can modulate marine primary productivity upon its deposition to the ocean surface. However, anthropogenic aerosol Fe solubility remains poorly constrained, due in part to a lack of direct measurements spanning a multitude of anthropogenic sources. We measured solubility of aerosol Fe from several distinct anthropogenic combustion processes and fuel types. The median Fe solubility varied widely by source, ranging from 0.03 % for power plant coal fly ash to 55.87 % for biofuel burning; furthermore, residential coal burning aerosol possessed much higher Fe solubility than power plant coal fly ash. Using the new Fe solubilities reported herein, we updated parameters for anthropogenic aerosol Fe within the Community Earth System Model. Anthropogenic combustion is estimated to contribute up to 20 % of the global soluble Fe flux to the ocean in the present day. Furthermore, we identified residential coal burning as a previously neglected but potentially important source with regional flux contributions ranging from <span class="inline-formula">&lt;</span> 1 % to 21 %. Our work underscores the need to further refine understanding of aerosol Fe properties from a wide variety of anthropogenic sources by increasing observations in more novel aerosol regimes, with a focus on residential coal burning. This understanding will in turn aid in characterizing the influences of anthropogenic activity on past, present, and future atmospheric nutrient inputs to marine ecosystems.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-9037-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/9037/2026/]]></dc:identifier>
      <dc:source>eISSN: 1680-7324</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:acp129664</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>acp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Assessing raindrop evaporation over northern Western Ghats from stable isotope signature of rain and vapour]]></dc:title>
      <dc:creator>Nimya, Sheena Sunil</dc:creator>
      <dc:creator>Rajaveni, Sundara Pandian</dc:creator>
      <dc:creator>Sengupta, Saikat</dc:creator>
      <dc:creator>Bhattacharya, Sourendra Kumar</dc:creator>
      <dc:creator>Ananthavel, Nandhini</dc:creator>
      <dc:description><![CDATA[<p>Stable isotopes of hydrogen and oxygen were analysed in rain and vapour samples collected simultaneously from Pune, India, during the 2019 summer monsoon. The <span class="inline-formula"><i>δ</i><sup>18</sup></span>O and <span class="inline-formula"><i>δ</i></span>D were significantly depleted in four events when the Outgoing Longwave Radiation showed a strong negative anomaly suggesting large-scale convection. The <span class="inline-formula"><i>δ</i><sup>18</sup></span>O values of the rain samples are negatively correlated with their d-excess indicating effect of drop evaporation. Isotope exchange between rain and ambient vapour and associated raindrop evaporation in the sub-cloud layer, tracked by <span class="inline-formula">Δ<i>δ</i></span>–<span class="inline-formula">Δ</span>d plot, suggest an equal share of equilibrium exchange and drop evaporation.</p>        <p>We used a one-dimensional Below Cloud Interaction Model (BCIM) to quantify sub-cloud processes affecting raindrop evolution. A Rayleigh ascent assumption in the BCIM simulations yields higher rain isotope values. Using radiosonde-based temperature and humidity profiles and constructing vapour isotope profiles from a combination of Tropospheric Emission Spectrometer data and a global circulation model (LMDZ) output, a better agreement is reached between the model and observed values. Sensitivity studies reveal that model values are strongly influenced by vapour isotope profiles, and moderately by drop size, temperature and relative humidity. Raindrop evaporation fraction estimated from the model yields daily-scale values varying from 4 % to 61 % (on average 23 %). This evaporation influences the heat budget and affects the monsoon convection. In addition, our study shows that drop evaporation reduces the rainfall amount considerably, especially in the lower range of precipitation. A precise quantification of raindrop evaporation is required for validation of the models used routinely for monsoon rainfall predictions.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-9061-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/9061/2026/]]></dc:identifier>
      <dc:source>eISSN: 1680-7324</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142663</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A Geometric Framework for Mapping Ocean Eddies Using Elliptical Streamfunction Parameterisation]]></dc:title>
      <dc:creator>Dowse, Reg Watson</dc:creator>
      <dc:creator>Keating, Shane R.</dc:creator>
      <dc:creator>Roughan, Moninya</dc:creator>
      <dc:description><![CDATA[The identification, tracking, and characterisation of ocean eddies using observational and numerical data is essential for understanding eddy dynamics and their global climate impacts. Eulerian (point-based) and Lagrangian (trajectory-based) schemes are widely used to detect and track ocean eddies. However, these methods typically do not provide information about the spatial structure of eddies or properties such as vorticity, deformation, and vertical tilt, especially when using sparse data. Here, we describe a new efficient and robust geometrical approach for mapping the three dimensional structure of ocean eddies by fitting (partial) velocity data to a simplified elliptical streamfunction model with a small number of parameters. The flexibility of the approach is demonstrated through three variants of the method adapted to different velocity sampling patterns: single and double sections (from ship transects or a numerical grid) and scattered data (e.g. from surface drifters). We validate and demonstrate these new geometric methods on idealised, axisymmetric and non-axisymmetric Gaussian eddies, as well as numerical and observational datasets. We conclude that elliptical streamfunction parametrisation offers a versatile and effective method for research into ocean eddy characteristics.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3599</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3599/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142505</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Uncertainty of Rainfall Forecasts for Impact-Based Flood Warning in the Cagayan River Basin, Philippines]]></dc:title>
      <dc:creator>Kurihara, Yuta</dc:creator>
      <dc:creator>Miyamoto, Mamoru</dc:creator>
      <dc:description><![CDATA[Effective impact-based flood early warning requires not only information on when heavy rainfall may occur, but also a calibrated estimate of the uncertainty in the resulting impacts. This study develops a framework for translating multi-centre sub-seasonal to seasonal (S2S) rainfall forecasts into probabilistic, municipality-level impact-based early-warning information for staged flood preparedness in the Cagayan River Basin, Philippines. Daily Gamma-kernel Bayesian model averaging is first applied to ensemble forecasts from ECMWF, NCEP, and UKMO to generate continuous predictive distributions of basin-mean rainfall. Leave-one-year-out verification for 2015&ndash;2025 identifies the ECMWF+NCEP+UKMO combination as the most robust tested input, with useful daily rainfall information mainly retained up to approximately lead days 5&ndash;6. The daily predictive samples are then accumulated into rolling seven-day rainfall distributions, because flood impacts in the basin are more closely related to multi-day rainfall than to isolated daily totals. Threshold-based probability recalibration improves the reliability of seven-day exceedance probabilities, raising Brier Skill Scores from &minus;0.02 to +0.08 at 100 mm per seven days and from &minus;0.07 to +0.02 at 150 mm per seven days relative to a monthly climatological baseline. The recalibrated seven-day rainfall distributions are subsequently propagated through municipality-level rainfall&ndash;damage functions to estimate probabilistic impacts on affected population, building damage, rice damage, and maize damage. An application to Typhoon Ulysses in November 2020 demonstrates how forecast-state-dependent impact intervals evolve as the event approaches and how municipalities with potentially large impacts can be prioritised. The results show that calibrated S2S rainfall probabilities can support uncertainty-aware, impact-based flood preparedness, while also highlighting limitations related to lead-time skill, basin-mean rainfall representation, upper-tail rainfall coverage, and the validation of rainfall&ndash;damage functions.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3482</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3482/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142462</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[How to Extract Lagrangian Information from Cloud Radar Doppler Spectra for Process Studies?]]></dc:title>
      <dc:creator>Ockenfuß, Paul</dc:creator>
      <dc:creator>Köcher, Gregor</dc:creator>
      <dc:creator>Petit, Isabel</dc:creator>
      <dc:creator>Kneifel, Stefan</dc:creator>
      <dc:description><![CDATA[Ground-based remote sensing instruments are often operated in a vertically pointing mode, producing time-height cross-section images (THIs) of the atmosphere. However, THIs are not Lagrangian observations: they cannot track the evolution of a single particle directly. Instead, several assumptions are required to derive the particle evolution from THI. We discuss these assumptions and show how their validity can be assessed using elevation scans. For demonstration, we analyze two intense riming cases. Since rimed particles exhibit enhanced sedimentation velocities, we first present a method to derive the vertical target velocity from scanning cloud radar observations. This method allows to study the spatial distribution of riming. The first case is comprised of several horizontally homogeneous, descending layers of rimed particles. Under these conditions, one can safely study the particle evolution in a "traditional" way by evaluating subsequent vertical profiles. The second case is more heterogeneous. For the analysis, we introduce the new spectral column vertical profile (SCVP) technique. SCVPs allow to trace the evolution of a single particle population's Doppler spectrum in space and time, thereby representing true Lagrangian observations. Our results demonstrate the value of scanning observations and show that downsides, for example regarding the use of Doppler velocity, can be overcome. Our results also raise the question whether the typically very high time resolution of THI is actually required for the common type of analyses performed on THI, and whether a combination of scanning and vertical observations could be the better observational strategy for ground-based remote sensing instruments.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3446</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3446/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142542</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[To tip or not to tip]]></dc:title>
      <dc:creator>Börner, Reyk</dc:creator>
      <dc:creator>Dijkstra, Henk A.</dc:creator>
      <dc:description><![CDATA[Tipping points have become a buzzword in Earth sciences, but ambiguous or overly narrow definitions of tipping are causing confusion around the concept. Agreeing on what tipping means, and whether a system tips or not, is important for robust science and communicating tipping risk. Based on a critical evaluation of existing tipping definitions, we propose a revised, general definition that characterizes a tipping event as a persistent nonlinear transition in forced systems. Our definition emphasizes both the phenomenology (observed time series) and cause (feedback mechanism) of a tipping event. Inspired by response theory, our proposition is compatible with more specific mathematical formulations while avoiding challenging notions such as bifurcations, equilibrium states, abruptness and irreversibility &ndash; making the definition testable also on transient dynamics in diverse complex systems under time-varying forcing. We showcase its practical use and limitations in a toy model and a case study of Earth system model data.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3507</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3507/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142428</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Technical note: Evaluation of a new cryogenic airtight vapor extraction (CRAVE) method for soil and plant water]]></dc:title>
      <dc:creator>Liu, Xiuqiang</dc:creator>
      <dc:creator>Wang, Hongxiu</dc:creator>
      <dc:creator>Chen, Xi</dc:creator>
      <dc:creator>Zhao, Ying</dc:creator>
      <dc:creator>Nehemy, Magali F.</dc:creator>
      <dc:creator>McDonnell, Jeffrey J.</dc:creator>
      <dc:description><![CDATA[Accurate extraction of soil and plant water for stable isotope analysis remains a methodological challenge in ecohydrology, particularly due to isotopic biases introduced by heating or selective pore-water extraction in conventional techniques. This study developed and evaluated a cryogenic airtight vapor extraction (CRAVE) method from soil and vegetation samples at ambient temperature within a recirculating vapor-liquid pathway. This approach avoids heating-induced non-equilibrium effects and reduces matrix-dependent artifacts and organic contamination, thereby facilitating direct comparison of isotopic compositions between soil and plant water. The results demonstrate that CRAVE-derived isotopic signatures align with both cryogenic vacuum distillation (CVD) and suction lysimeter (SL) benchmarks. However, systematic deviations were observed based on specific matrix properties. For xylem water, the d<sup>2</sup>H offset between CRAVE and CVD was strongly modulated by gravimetric water content (dry-weight basis), with CVD exhibiting greater hydrogen isotope depletion under low-moisture conditions (&lt; 0.8 g&middot;g<sup>-1</sup>). For soils, the isotopic divergence between CRAVE and CVD was driven primarily by soil texture, with offsets increasing as clay content and depth increased (<em>r</em> = 0.82&ndash;0.94), where CVD-extracted bulk water became depleted progressively in both &delta;<sup>2</sup>H and &delta;<sup>18</sup>O relative to the mobile-capillary pool captured by SL and CRAVE. The Rayleigh-based framework provides a physically grounded means to reconstruct source-water isotope values from condensate measurements; its potential use for mobile&ndash;immobile partitioning should, however, be treated as a future application pending targeted validation. Overall, CRAVE represents a promising ambient-temperature extraction method for tracing water partitioning and source-uptake dynamics within the soil&ndash;plant&ndash;atmosphere continuum.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3419</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3419/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142676</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Sensitivity of time-lapse magnetic resonance sounding to vadose zone hydrodynamic parameters: monitoring of an intense meteorological event]]></dc:title>
      <dc:creator>Gru, Guillaume</dc:creator>
      <dc:creator>Girard, Jean-François</dc:creator>
      <dc:creator>Ackerer, Philippe</dc:creator>
      <dc:creator>Lesparre, Nolwenn</dc:creator>
      <dc:description><![CDATA[Magnetic Resonance Sounding (MRS) is a geophysical method that provides direct information on subsurface water content and can complement traditional hydrological observations for model calibration. We develop a coupled hydrogeophysical framework by linking one-dimensional unsaturated flow with an MRS forward model to simulate a time-lapse MRS experiment during an infiltration event in the Strengbach headwater catchment in northeastern France. The geometry of the model is conditioned using insights on the porous medium thickness provided by seismic refraction tomography, in order to reduce model uncertainties related to the thickness of subsurface layers. We apply a Global Sensitivity Analysis (GSA) to quantify how uncertainty in hydrodynamic parameters affects MRS signals and their temporal evolution. The GSA combines variance-based Sobol indices with two other moment-based metrics (AMAE and AMAV) to characterize the sensitivity of both the mean and the variance of the MRS signal distributions. Using these complementary metrics provides a more robust assessment of parameter influence than Sobol indices alone. Our results identify the parameters which exert the strongest control on time-lapse MRS signals and reveal how their influence changes during the infiltration event. We also identify parameters whose uncertainties have insignificant contribution to MRS signals. These insensitive parameters are not expected to be precisely estimated with inverse modeling techniques based on MRS data. These insights clarify the potential and limitations of MRS data for constraining hydrological parameters in shallow mountain aquifers and demonstrate how the temporal evolution of MRS sensitivity can be exploited to optimize monitoring strategies during transient hydrological events.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3611</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3611/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142422</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Virtual Rain: A Unified Toolkit for High-Resolution Rainfall Simulation and Disaggregation]]></dc:title>
      <dc:creator>Cappelli, Francesco</dc:creator>
      <dc:creator>Grimaldi, Salvatore</dc:creator>
      <dc:creator>Petroselli, Andrea</dc:creator>
      <dc:creator>Santinami, Emanuele</dc:creator>
      <dc:description><![CDATA[Stochastic simulation models are essential for investigating hydrological processes and supporting water resource management. In this study, we introduce Virtual Rain, a two-step toolkit that first generates synthetic daily rainfall time series and then disaggregates them to a user-defined temporal resolution. The toolkit builds on the approaches recently proposed by some of the authors, ensuring a realistic representation of rainfall dynamics while preserving key statistical properties. The framework is implemented through a set of Python and R routines designed to facilitate practical application. In addition to providing observed rainfall time series and the scaling exponent ? (Intensity&ndash;Duration&ndash;Frequency slope), users can configure key modelling components, including the marginal distribution, autocorrelation structure, number of lags, and target temporal resolution. The routines generate both graphical and quantitative outputs, enabling direct comparison between observed and simulated series. Virtual Rain performance is evaluated through a real-world case study, demonstrating satisfactory accuracy and highlighting the robustness, flexibility, and transferability of the proposed toolbox. The toolkit is also available through an interactive web-based platform, facilitating its use by a broad range of users.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3414</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3414/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142565</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Satellite-derived management indicators improve modeling of water and greenhouse gas fluxes in Swiss agroecosystems]]></dc:title>
      <dc:creator>Jia, Aolin</dc:creator>
      <dc:creator>Aasen, Helge</dc:creator>
      <dc:creator>Hörtnagl, Lukas</dc:creator>
      <dc:creator>Feigenwinter, Iris</dc:creator>
      <dc:creator>Ledain, Sélène</dc:creator>
      <dc:creator>Lauber, Thomas</dc:creator>
      <dc:creator>Kohonen, Kukka-Maaria</dc:creator>
      <dc:creator>Tschurr, Flavian</dc:creator>
      <dc:creator>Allemann, Lorenz</dc:creator>
      <dc:creator>Turco, Fabio</dc:creator>
      <dc:creator>Buchmann, Nina</dc:creator>
      <dc:description><![CDATA[Agroecosystems regulate carbon, water, and nitrogen cycles, yet robust modeling of water and greenhouse gas (GHG) fluxes remains limited by incomplete or inaccessible information on field management practices. Although high-resolution remote sensing (RS) observations can detect management events such as mowing or harvest, their use for representing management intensity and associated impacts on ecosystem flux dynamics remains limited in existing models. Here, we developed an RS-assisted modeling framework to estimate daily latent heat flux (LE), net ecosystem CO<sub>2</sub> exchange (NEE), nitrous oxide (N<sub>2</sub>O), and methane (CH<sub>4</sub>) fluxes across six Swiss FluxNet sites (two croplands and four grasslands) between 2016 and 2025. Sentinel-2 time series were used to derive leaf area index and RS-based field management indices (RS-FMIs), detecting mowing events, quantifying defoliation intensity, and identifying crop rotation and bare soil periods. These indicators were combined with meteorological drivers to train XGBoost models for each ecosystem type and target variable separately, and driver contributions were evaluated using SHapley Additive exPlanations (SHAP) analysis.</p> <p>The RS-FMIs effectively captured <em>in situ</em> recorded management events and enabled improved reconstruction of daily flux variability. Model performances were strong for LE (R<sup>2</sup> &asymp; 0.89&ndash;0.90) and NEE (R<sup>2</sup> &asymp; 0.59&ndash;0.71), whereas N<sub>2</sub>O and CH<sub>4</sub> fluxes were reproduced with moderate accuracy (R<sup>2</sup> &asymp; 0.37&ndash;0.55). Models using RS-FMIs performed similarly to those using well-compiled <em>in situ</em> management records, supporting the ability of RS-derived vegetation and management indicators to represent management effects. LE variability was primarily energy-driven and dominated by meteorological conditions, whereas vegetation dynamics and RS-FMIs played stronger roles in shaping NEE, N<sub>2</sub>O, and CH<sub>4</sub> variability. These results demonstrate that RS-FMIs offer new opportunities to reconstruct management information and improve the representation of management effects in agroecosystem flux modeling.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3522</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3522/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142686</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The impact of the Hunga eruption on the 2023 Antarctic ozone hole: contrasting effects in the core and edge regions of the polar vortex]]></dc:title>
      <dc:creator>Heddell, Saffron Genise</dc:creator>
      <dc:creator>Chipperfield, Martyn P.</dc:creator>
      <dc:creator>Mann, Graham W.</dc:creator>
      <dc:creator>Dhomse, Sandip S.</dc:creator>
      <dc:creator>Feng, Wuhu</dc:creator>
      <dc:creator>Zhou, Xin</dc:creator>
      <dc:creator>Yoshioka, Masaru</dc:creator>
      <dc:creator>Jones, Anthony</dc:creator>
      <dc:description><![CDATA[The January 2022 Hunga eruption injected an exceptional 150 Tg of water vapour (H<sub>2</sub>O) into the stratosphere causing an enhancement not observed previously within the satellite era, with extensive and ongoing effects. From global chemical transport model simulations, we further assess the high-latitude H<sub>2</sub>O enhancement caused by the eruption, and how it influenced the 2023 Antarctic ozone depletion across two vortex regimes: the cold core and the less cold, and more insolated vortex edge region. Our simulations show the H<sub>2</sub>O chemical impacts arose mainly from the H<sub>2</sub>O enhancement promoting earlier formation of polar stratospheric clouds (PSCs), which in turn enhanced chlorine activation and subsequent ozone loss. We also show ice PSC dehydration in the vortex core limited Hunga&rsquo;s chemical effects to occur for only the first 25 % of the vortex season; consequently, the edge region experienced the largest chemical impact to ozone depletion in 2023. Overall, the H<sub>2</sub>O enhancement increased Antarctic ozone hole area by 7 % but remaining within the historical variability over the past two decades. Sensitivity simulations including the Hunga sulfate aerosol show H<sub>2</sub>O-driven heterogeneous chlorine activation on additional PSCs, dominated the chemical impacts of Hunga on polar ozone, with only minor impact from activation on volcanic sulfate aerosol. Our results highlight that while water-rich large volcanic eruptions can worsen polar ozone depletion, the magnitude of the impact is strongly influenced by stratospheric temperatures through dehydration. This suggests that less cold vortex environments, e.g. the Arctic, may experience larger relative changes in chlorine activation under similar conditions.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3619</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3619/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142699</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Eulerian and Lagrangian Assessment of Arctic Surface Current Products Using Drifter Observations]]></dc:title>
      <dc:creator>Rosquete-Estevez, Aleida</dc:creator>
      <dc:creator>Crespin, Júlia</dc:creator>
      <dc:creator>Yubero, Luis</dc:creator>
      <dc:creator>Mancho, Ana María</dc:creator>
      <dc:creator>Umbert, Marta</dc:creator>
      <dc:description><![CDATA[Accurate Arctic surface current estimates are needed to quantify freshwater redistribution, upper-ocean connectivity, and Arctic&ndash;North Atlantic exchanges, but validating them is difficult given sparse observations, sea-ice cover, and overlapping dynamical processes. This study evaluates six widely used products against drogued drifters from the Global Drifter Program (2011&ndash;2021): AVISO altimetry-derived geostrophic currents, NeurOST machine-learning reconstructions, GlobCurrent and OSCAR multi-observational/mixed-layer total currents, and the GLORYS and TOPAZ reanalyses. Skill is assessed with complementary Eulerian point-wise metrics and Lagrangian trajectory diagnostics, including a Lagrangian Uncertainty Quantification (LUQ) framework. Eulerian results show marked regional and seasonal contrasts. NeurOST and OSCAR agree best with drifter velocities, GlobCurrent and GLORYS show intermediate skill, TOPAZ has weaker near-surface speed agreement, and AVISO underestimates current intensity and variability. Products incorporating additional observational constraints, wind-driven contributions, or mixed-layer dynamics outperform altimetry-only geostrophic estimates, especially in regions shaped by mesoscale variability, bathymetry, sea ice, and narrow gateways. The Lagrangian analysis shows that good local velocity agreement does not guarantee realistic transport: small velocity differences accumulate along trajectories, producing large deviations in pathways, retention, and connectivity. LUQ diagnostics indicate part of this mismatch reflects intrinsic transport variability and initial-condition sensitivity rather than product error alone. The authors conclude that Eulerian validation must be complemented by Lagrangian, uncertainty-aware diagnostics for studies of freshwater pathways, tracer transport, and Arctic connectivity.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3629</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3629/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142610</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Separating Forced and Internal Contributions to Future Northern Hemisphere Storm Track Changes and Associated Precipitation Impacts]]></dc:title>
      <dc:creator>Helliesen, Karen E.</dc:creator>
      <dc:creator>Sheng, Bosi</dc:creator>
      <dc:creator>Bollasina, Massimo A.</dc:creator>
      <dc:description><![CDATA[Storm tracks &mdash; the preferred pathways of extratropical cyclones in the midlatitudes &mdash; are projected to shift poleward, migrate upward in the atmosphere, and change in intensity under anthropogenic climate change. These changes have important consequences for weather and climate variability across the Northern Hemisphere (NH) midlatitudes. Here we investigate future changes in NH storm track strength and position, their driving physical mechanisms, and their impacts on precipitation, using large ensemble (LE) simulations from three CMIP6 models alongside ERA5 reanalysis data. Robust projections are developed under two scenarios (SSP2-4.5 and SSP5-8.5) for both boreal winter (DJF) and summer (JJA) at end-of-century (2070&ndash;2100) relative to the present day (1984&ndash;2014). The LE approach enables a rigorous characterisation of internal variability and the separation of the forced response from sampling noise. Key results include: (i) a poleward and upward shift of winter storm tracks, driven primarily by tropical upper-tropospheric warming that enhances upper-level baroclinicity, increasing precipitation poleward of ~45&deg; N; (ii) a weakening of summer storm tracks associated with reduced static stability in the upper troposphere, leading to decreased precipitation across the midlatitudes; and (iii) substantial spread among ensemble members, particularly in DJF under SSP2-4.5, highlighting the prominent role of internal variability in shaping projected changes. The contribution of internal variability is reduced under SSP5-8.5 and during JJA, where the externally forced signal dominates. Inter-model differences, linked primarily to differing equilibrium climate sensitivities, emphasise the importance of multi-model LE frameworks for robust climate impact assessment.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3557</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3557/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142378</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Probabilistic Modelling and Prediction of Sea Level Dynamics in the Southern Baltic Sea]]></dc:title>
      <dc:creator>Pajak, Katarzyna</dc:creator>
      <dc:creator>Idzikowska, Magdalena</dc:creator>
      <dc:creator>Kowalczyk, Kamil</dc:creator>
      <dc:description><![CDATA[This paper presents a probabilistic approach to the analysis of non-stationary sea level measurement series in the southern Baltic Sea based on tide gauge data for Swinoujscie, Kolobrzeg, Ustka, Wladyslawowo and Gdansk stations. Harmonic analysis (HA), Continuous Wavelet Transform (CWT), AR(1) autoregressive model and Monte Carlo uncertainty propagation were applied to identify trends, multiscale variability and the stochastic structure of the measurement data. The results indicate a spatially consistent sea level rise trend of 1.8&ndash;2.2 mm/yr, modulated by multiscale periodic variability and short-term stochasticity. The model used allows for a probabilistic forecast of sea level changes. In addition, the analysis of extremes using the Gumbel distribution indicates an increase in the probability of extreme sea levels along the southern Baltic coast. The proposed methodology extends conventional sea level analysis by integrating probabilistic interpretation, classical uncertainty estimation, and multiscale signal analysis, thereby providing a useful tool for coastal hazard and flood risk assessment and climate change adaptation in coastal regions.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3383</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3383/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142635</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A data-driven method coupling multiple physical constraints for correcting structural errors in groundwater contaminant transport models]]></dc:title>
      <dc:creator>Tian, Jinglong</dc:creator>
      <dc:creator>Zeng, Xiankui</dc:creator>
      <dc:creator>Pan, Yue</dc:creator>
      <dc:creator>Wang, Dong</dc:creator>
      <dc:creator>Wu, Jichun</dc:creator>
      <dc:description><![CDATA[Model structural errors are pervasive in groundwater contaminant transport modeling under complex environmental conditions, hindering accurate prediction of contamination transport. Data-driven methods (DDMs) coupled with physical constraints provide an effective approach for correcting structural errors and improving prediction. However, in multicomponent reactive transport systems, multiple physical mechanisms must be satisfied simultaneously, whereas existing DDMs have limited capacity to effectively couple multiple physical constraints. To address this challenge, this study proposes a general method for correcting structural errors in groundwater models. A combined likelihood function is constructed and sub-likelihood weights are dynamically updated to effectively couple multiple physical constraints. The method is evaluated using a synthetic three-dimensional tetrachloroethylene reactive transport simulation and a cadmium-phosphate cotransport sand column experiment. These tests systematically assess the effects of coupling single versus multiple physical constraints on structural error correction and predictive performance. The results show that coupling multiple constraints can constrain parameter identification, reduce predictive uncertainty, and more comprehensively improve model predictions. Appropriate physical constraints function analogously to incorporating additional observations. Moreover, coupling multiple physical constraints results in a simpler form of structural error in the calibrated groundwater model, making it easier to characterize, thereby enhancing prediction accuracy and physical consistency. The proposed dynamic updating and stopping criterion of sub-likelihood weights maintains a balance between multiple physical constraints and observations, improving the robustness of parameter identification and constraint enforcement. Overall, the proposed DDM coupled with multiple physical constraints provides a general framework for correcting structural errors in complex groundwater contaminant transport models.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3578</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3578/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142746</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Ditches, microtopographical hotspots and hot moments drive greenhouse gas emissions from a clear-felled conifer plantation on an organic soil]]></dc:title>
      <dc:creator>Keane, Ben</dc:creator>
      <dc:creator>Blei, Emanuel</dc:creator>
      <dc:creator>Gibson-Poole, Simon</dc:creator>
      <dc:creator>Ineson, Phil</dc:creator>
      <dc:creator>Morison, James I. L.</dc:creator>
      <dc:creator>Perks, Mike</dc:creator>
      <dc:creator>Vanguelova, Elena</dc:creator>
      <dc:creator>Wilkinson, Matt</dc:creator>
      <dc:creator>Williams, Mat</dc:creator>
      <dc:creator>Xenakis, Georgios</dc:creator>
      <dc:creator>Yamulki, Sirwan</dc:creator>
      <dc:creator>Toet, Sylvia</dc:creator>
      <dc:description><![CDATA[In the United Kingdom (UK), forests on peaty gley, peaty podsol and deep peat soils contain ca. 50 % of the total forest soil C stock (Vanguelova, 2015). Many such forests were planted in the 1970s and 80s and are due for harvest, raising the question: what is the greenhouse gas (GHG) balance after felling?</p> <p>Typically, planted forests in the wetter UK uplands contain a network of ditches and ridge-with-furrows resulting in a complex mosaic of microtopographical features. Measuring GHG exchange from such a complex landscape is challenging; methane (CH<sub>4</sub>) and nitrous oxide (N<sub>2</sub>O) fluxes can vary greatly in both space and time, and ditches have been highlighted as potentially important GHG sources although they are challenging to measure.</p> <p>We used a combination of flux measurement techniques to quantify GHG fluxes and identify the drivers from the key microtopographies (ridges, hollows, ditches) within an upland forest in northern England immediately after clear felling. We deployed manual flux chambers, a SkyLine2D automated chamber system and two eddy covariance towers to measure carbon dioxide (CO<sub>2</sub>), CH<sub>4</sub>, and N<sub>2</sub>O for an intensive campaign of five weeks. We used remote sensing to estimate the proportions of microtopographies and upscaled fluxes from the chamber to the forest block scale. We investigated the contribution of brash to the GHG emissions of harvest through a litter addition experiment.</p> <p>Cumulative flux estimates based on the different techniques and the GHGs measured varied considerably. We found that CO<sub>2</sub> fluxes did not differ between microtopographies but the needle litter in harvesting residues increased CO<sub>2</sub> emissions by ca. 33 %. Soil moisture was an important driver of both CH<sub>4</sub> and N<sub>2</sub>O fluxes. Ditches were the largest source of CH<sub>4</sub> fluxes, followed by hollows and then ridges. The opposite pattern was seen for N<sub>2</sub>O fluxes, which were greatest from ridges and other drier areas within the landscape. Following heavy rainfall, emissions of all GHGs increased rapidly over the next 24 hours.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3659</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3659/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141010</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Systematic Analysis of Rain-on-Snow Events and Their Trends in the French Alps: Distinguishing All and Impactful Events across Mountain Ranges]]></dc:title>
      <dc:creator>Fournier, Paul</dc:creator>
      <dc:creator>Blanc, Antoine</dc:creator>
      <dc:creator>Blanchet, Juliette</dc:creator>
      <dc:creator>Lafaysse, Matthieu</dc:creator>
      <dc:description><![CDATA[Rain-on-snow (ROS) events are a major hydrometeorological phenomenon in mountainous regions, as the combination of liquid precipitation and snowmelt enhances flood hazard. This study provides the first systematic analysis of ROS events in the French Alps at high temporal and spatial resolution, based on the S2M reanalysis (1958&ndash;2024) with an hourly time step. By combining meteorological data with an event database of torrential floods and landslides, ROS events are explicitly linked to observed impacts. Averaged over space, 5.5 ROS events occurred per year in the French Alps over 1958&ndash;2024, with a clear contrast between the more frequently affected north-western mountain ranges and the south-eastern ones. Seasonality strongly depends on elevation, with ROS events occurring mainly in winter at lower elevations and in spring at higher elevations. Impactful ROS events, associated with torrential floods or landslides, are characterized by high cumulative rainfall and long durations. Above 76 mm of cumulative rainfall, the probability that a ROS event is impactful exceeds 50 %, defining heavy-rainfall ROS events. Trend analyses reveal a marked decline in overall ROS occurrence (-22 %) between 1959&ndash;1988 and 1995&ndash;2024, primarily in spring and early summer due to a shortening of the snow season, while increases are observed in December and January as precipitation more frequently falls as rain. Heavy-rainfall ROS events show a more moderate decrease (-9 %), with declining trends in most southern mountain ranges but increases in several northern ones. They now predominantly occur in early winter at lower elevations, which are more densely populated, making them more likely to produce damaging impacts. The next step in this systematic approach would be to create a watershed-based subdivision of the French Alps to enable comprehensive hydrological analyses of ROS events.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2497</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2497/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140927</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Aerobic and anaerobic contributions to carbon dioxide and methane emissions in a 1D peatland model: Peatland-VU v3.0]]></dc:title>
      <dc:creator>Lippmann, Tan J. R.</dc:creator>
      <dc:creator>Huissteden, Jacobus K.</dc:creator>
      <dc:creator>Velde, Ype</dc:creator>
      <dc:creator>Boon, Veronique E. N.</dc:creator>
      <dc:creator>Berg, Merit</dc:creator>
      <dc:description><![CDATA[Accurate modelling of peatland carbon dynamics is essential for understanding their role in the global carbon cycle and predicting greenhouse gas (GHG) fluxes under changing environmental and management conditions. We present PeatlandVU v3.0, an updated 1D process-based model with new representations of key above- and below-ground processes controlling peatland carbon exchange. Developments include improved vegetation phenology (leaf area index and growing degree days), alternative formulations for the temperature sensitivity of soil organic matter (SOM) decomposition, and explicit representation of anaerobic SOM mineralisation.</p> <p>Model behaviour and sensitivity were evaluated at two contrasting peatland sites in the Netherlands: a restored fen marshland (the Weerribben site) and a drained peat pasture (the Assendelft site) where model performance was evaluated against in situ flux measurements. Using ensembles of targeted perturbation experiments, we quantified sensitivity to internal parameters and environmental drivers and identified the processes and parameters that most strongly control variability in simulated CO<sub>2</sub> and CH<sub>4</sub> fluxes across contrasting peatland types. Beyond presenting new developments, this study provides a complete and consolidated sensitivity assessment of all processes and modules, not only newly implemented processes. The comprehensive evaluation provides a clear reference for future model developments, parametrisation and application to new sites.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2450</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2450/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142228</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Contrasting impacts of Asian sulfate aerosols on regional summer extreme precipitation under different climate backgrounds]]></dc:title>
      <dc:creator>Luo, Feifei</dc:creator>
      <dc:creator>Joshi, Manoj</dc:creator>
      <dc:creator>Samset, Bjørn H.</dc:creator>
      <dc:creator>Wilcox, Laura J.</dc:creator>
      <dc:creator>Stjern, Camilla W.</dc:creator>
      <dc:creator>Allen, Robert J.</dc:creator>
      <dc:creator>Kuo, Yan-Ning</dc:creator>
      <dc:creator>Hua, Wei</dc:creator>
      <dc:creator>Li, Shuanglin</dc:creator>
      <dc:description><![CDATA[This study investigates the impact of Asian sulfate aerosols on regional summer extreme precipitation under both pre-industrial and pre-industrial +1 K climate states, using the reduced-complexity climate model Fast Ocean Rapid Troposphere Experiment version 2 (FORTE2) with Systematic Regional Aerosol Perturbations simulations. Results show that increased Asian sulfate aerosols reduce extreme precipitation, characterized by lower frequency and weaker intensity over East and South Asia in both climates, but the suppression is more pronounced over northern India in the +1 K climate. Atmospheric energy budget analysis reveals this is primarily due to enhanced dynamic effects in the warmer climate. When aerosols are added to the pre-industrial climate state, an increased horizontal dry static energy (DSE) gradient partially offsets the aerosol-induced dynamic suppression over northern India. Under the +1 K climate, higher atmospheric static stability weakens the local meridional circulation induced by aerosol forcing, reducing the meridional temperature gradient and thus diminishing the offsetting effect, making the dynamic suppression more dominant. Further analysis indicates that this difference in precipitation responses between the two climates results from the nonlinear effect between the aerosol-radiation and aerosol-cloud interactions under the +1 K climate, whereas the two effects combine approximately linearly under the pre-industrial climate. This study suggests that continued global warming alone will exacerbate Asian sulfate aerosols&rsquo; weakening of precipitation, including extremes, over northern India. This implies that future reductions in aerosol emissions may unmask or amplify extreme precipitation increases in this region.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3301</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3301/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142207</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Probing the Koillismaa Deep Intrusion in Northern Finland using Advanced Seismic Imaging]]></dc:title>
      <dc:creator>Singh, Brij</dc:creator>
      <dc:creator>Górszczyk, Andrzej</dc:creator>
      <dc:creator>Malinowski, Michał</dc:creator>
      <dc:creator>Karinen, Tuomo</dc:creator>
      <dc:description><![CDATA[The Koillismaa&ndash;N&auml;r&auml;nk&auml;vaara Layered Igneous Complex (KLIC) has been the subject of continuous studies due to its potential to host several critical raw materials, mostly of the Ni-Cu-PGE sulphide type. The KLIC is characterised by a ~50&ndash;60 km-long geophysical anomaly in which the magnetic high is followed by a shifted gravity high response, believed to be caused by the Koillismaa Deep Intrusion (KDI), but the exact origins remain unknown. A regional reflection seismic profile was acquired under the SEEMS DEEP project (2022&ndash;2025) to define the spatial geometrical architecture of the KDI. Initial processing using standard time-domain and conventional depth imaging revealed its first-order large-scale structure, indicating a funnel-shaped geometry and confirming it as a geologically complex target. In this study, we apply advanced seismic imaging methods, better suited to complex geologies, to further improve the imaging of the KDI. Ray-based (least-squares)Kirchhoff prestack depth migration and wave-equation-based reverse time migration (RTM) were used for this purpose. A high-resolution P-wave velocity model was built using acoustic full waveform inversion (FWI), while first arrival traveltime tomography was applied to build the starting model for FWI. Wave-equation-based, joint RTM-FWI workflow provided the optimum imaging of the KDI setting. A comprehensive reinterpretation of the KDI was done using the multi-method approach integrating gravity, magnetic and electromagnetic surveys. The available borehole information and common earth model for the study area were used as constraints. Shallow seismic reflectivity correlated well with the mafic dykes observed in the magnetic data. The exact origin of these dykes was earlier unknown and was attributed to the observed magnetic high in the KLIC area. Advanced seismic imaging revealed a previously unrecognized, more laterally extensive top of the KDI whose full extent was previously unknown. It is also interpreted that the denser mafic intrusion (KDI) defined by this extensive top may have increased the net vertical mass distribution in the area, because of which a shifted gravity response with respect to the magnetic high has been observed. A new hypothesis on the angular ascent of the magma towards the surface is also proposed based on the mapped seismic reflectivity associated with the mafic intrusion.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3292</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3292/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141815</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Taxon-specific coccolithophore carbonate stocks and production across a Pacific trophic gradient from oligotrophic gyre to upwelling zone]]></dc:title>
      <dc:creator>Lassus, Guillaume</dc:creator>
      <dc:creator>Beaufort, Luc</dc:creator>
      <dc:creator>Couapel, Martine</dc:creator>
      <dc:creator>Mendels, David</dc:creator>
      <dc:description><![CDATA[Coccolithophores contribute substantially to marine carbonate production, yet species-resolved estimates of coccosphere-associated CaCO₃ stocks remain scarce across large-scale trophic gradients. Here we quantify multispecific coccosphere carbonate inventories and first-order production estimates along the BIOSOPE transect across the South Pacific Gyre, one of the most strongly stratified regions of the global ocean. Estimates were obtained using an upgraded SYRACO automated recognition workflow combined with bidirectional circular polarization (BCP) imaging, allowing direct reconstruction of coccosphere calcite content at the cellular scale. Coccolithophore assemblages reproduced the major regional and vertical ecological structures previously described across the transect, including the transition from nutrient-rich surface communities near the Marquesas Archipelago and the eastern upwelling-influenced region to vertically structured assemblages in the oligotrophic gyre. At the transect scale, CaCO₃ standing stocks were primarily controlled by these large-scale trophic gradients, with maxima located in surface waters of mesotrophic regions and at depth within the deep chlorophyll maximum in the stratified gyre, indicating a vertical decoupling between coccosphere abundance and carbonate inventories under oligotrophic conditions. Taxon-specific analyses show that carbonate inventories reflect both coccosphere abundance and strong interspecific contrasts in calcite content. Isochrysidales, particularly <em>Emiliania huxleyi</em>, dominated carbonate stocks through their numerical abundance, whereas more heavily calcified taxa contributed disproportionately relative to their cell densities. Despite structuring assemblages in the lower euphotic zone, deep-dwelling taxa represented only a minor fraction of suspended carbonate stocks in the water column, contrasting with their major contribution to sedimentary assemblages in oligotrophic regions. First-order CaCO₃ production estimates followed spatial patterns similar to standing stocks, with enhanced production in mesotrophic regions and a sustained contribution from oligotrophic communities. Although uncertainties remain related to species-specific growth rates, these estimates provide the first multispecific constraints on coccolithophore calcification dynamics in the southeastern Pacific. Overall, this study demonstrates that combining automated coccosphere recognition with BCP-based carbonate measurements provides a robust framework for resolving species-level carbonate inventories across major oceanic trophic gradients and represents an important step toward quantitative assessments of coccolithophore contributions to pelagic carbonate cycling at basin scale.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3055</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3055/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141596</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A Weakly Supervised Deep Learning Framework for Estimating Above-Ground Biomass for Non-Forest Landscapes From Optical Images]]></dc:title>
      <dc:creator>Nubwimana, Rachel</dc:creator>
      <dc:creator>Brandt, Martin</dc:creator>
      <dc:creator>Ciais, Philippe</dc:creator>
      <dc:creator>Mugabowindekwe, Maurice</dc:creator>
      <dc:creator>Li, Sizhuo</dc:creator>
      <dc:creator>Davies, Andrew</dc:creator>
      <dc:creator>Gominski, Dimitri</dc:creator>
      <dc:creator>Fensholt, Rasmus</dc:creator>
      <dc:creator>Saatchi, Sassan</dc:creator>
      <dc:creator>Gieseke, Fabian</dc:creator>
      <dc:description><![CDATA[Above-ground biomass (AGB) maps are essential for carbon accounting and sustainable land management, yet AGB for non-forest landscapes remains poorly accounted for in global datasets. Here, we make use of deep learning and high-resolution PlanetScope imagery to introduce the concept of AGB contribution maps, which are high-resolution AGB predictions that capture local patterns. These maps can be predicted at any resolution from 1 to 100 m, providing insights into the spatial features included in the coarser resolution AGB maps, being essential for mapping trees outside forests. Our method employs a weakly supervised hybrid framework that transfers information from an existing 100 m global AGB map to high‑resolution optical satellite imagery, enabling the interpretation of detailed spatial patterns. We demonstrate that our map achieves detailed and spatially consistent patterns of woody vegetation in African savanna landscapes comparable to UAV-based LiDAR. Aggregated AGB values are well aligned with independent in-situ measurements (r2 = 0.71, bias 1 %), which is contrary to the original coarse AGB map used for training (r2 = 0.17, bias 48 %), indicating the capability of our approach to refine the existing map towards a higher accuracy for estimating tree biomass outside forests. This suggests that our model has learned tree-level information that is not present in the original AGB training data, providing a framework to refine existing coarse-resolution AGB maps. The granular and multi-resolution results provide no contribution to global efforts in sustainable land management of non-forest landscapes at any preferred scale and resolution.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2924</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2924/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141673</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Review article:&nbsp;The future of the physics-based NWP methodology: a critical review on applications of catastrophe theory to the atmospheric science]]></dc:title>
      <dc:creator>Liu, Chongjian</dc:creator>
      <dc:creator>Yin, Jinfang</dc:creator>
      <dc:creator>Wei, Xiaomin</dc:creator>
      <dc:creator>Sun, Xiaogong</dc:creator>
      <dc:creator>Zhu, Guofu</dc:creator>
      <dc:description><![CDATA[The physics-based NWP (Numerical Weather Prediction) methodology appears increasingly difficult to enhance the NWP model&rsquo;s forecasting capabilities. This is caused largely by catastrophe/tipping phenomena in the atmosphere as well as the multiplicity of NWP equation solutions. Classical physics from Newtonian mechanics to Einstein&rsquo;s general relativity is essentially the theory of various kinds of smooth behavior other than catastrophe phenomena (water suddenly boils, a cell doubles cancerously etc.) while catastrophe theory (CT) provides a methodology for mathematical treatment of continuous action producing a discontinuous result, and has broad application prospects in numerous subjects. Studies of catastrophe have never stopped but the closely related terminology (tipping) changed subtly, and thus similarities and differences between catastrophe and tipping as well as the rhetoric course of change and development with tipping points have been ascertained in this article with the result showing that CT itself never declines and it gets a new replacer only. Both problems of the NWP development bottleneck and the highly acclaimed AI-weather models enslaved to its knowledge quality could be basically attributed to the emergence of catastrophic/tipping points owing to the nonlinearity of model equations. In this Critical Review, via a comprehensive review and the relevant analyses, we are led to the conclusion that it would be sagacious to first determine which one is the &ldquo;physical solution&rdquo; and/or incorporate (e.g.) the second law of thermodynamics as an additional constraint into the NWP model so as to reduce the number of solutions.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2981</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2981/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141734</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Transport Efficiency of Turbulent Parcel in the Marine Boundary Layer and Its Implications for Droplet Activation in Marine Cloud Brightening]]></dc:title>
      <dc:creator>Zhao, Pan</dc:creator>
      <dc:creator>Chen, Jingyi</dc:creator>
      <dc:creator>Yang, Yang</dc:creator>
      <dc:creator>Jia, Yue</dc:creator>
      <dc:creator>Yu, Yang</dc:creator>
      <dc:description><![CDATA[Marine cloud brightening (MCB) has been proposed as a potential climate intervention strategy in which sea-salt aerosols are introduced into the marine boundary layer to enhance cloud albedo by increasing cloud droplet number concentrations (CDNC). However, whether turbulent motions can efficiently transport sea-surface-released aerosols to the cloud base remains a major uncertainty in evaluating MCB feasibility. This study investigates a stratocumulus case over the tropical Southeast Atlantic using large-eddy simulation (LES) coupled with the FLEXPART Lagrangian particle dispersion model to quantify turbulent parcel transport efficiency. Short-duration releases and high-LWP stages favor stronger transport of turbulent parcels to the cloud base. For parcels released at 00:00 UTC on 24 September, the peak instantaneous arrival rate reaches 3.39 % within 15 min in d02, whereas it decreases to 1.86 % and the peak arrival time is delayed to 17 min in d04; the corresponding cumulative arrival rate decreases from 94.16 % to 79.70 %. Although the mean in-cloud residence time decreases with increasing resolution, parcels with extremely long residence times become more frequent. Under the adopted activation parameterization, higher-resolution LES simulations yield higher activation fraction (AF) because they better resolve strong cloud-base updrafts, with AF ranging from 0.73&ndash;0.91 in d02 to 0.92&ndash;0.96 in d04. The AF is relatively insensitive to release duration but increases under high-LWP conditions. These results provide a process-level quantification of parcel transport, in-cloud residence time, and conditional activation, establishing a physical basis for evaluating aerosol delivery constraints in MCB applications.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3025</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3025/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140149</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Dynamical and Microphysical Interactions in a Coastal Bow-Echo Producing Extreme Rainfall]]></dc:title>
      <dc:creator>Jeong, Jong-Hoon</dc:creator>
      <dc:creator>Kim, Seung Hee</dc:creator>
      <dc:creator>Oh, Su-Bin</dc:creator>
      <dc:creator>Lee, Jeong-Eun</dc:creator>
      <dc:creator>Tasi, Chia-Lun</dc:creator>
      <dc:creator>Lee, Gyuwon</dc:creator>
      <dc:description><![CDATA[On 2 August 2020, a coastal bow-echo mesoscale convective system (MCS) produced severe rainfall and damaging winds over South Korea, resulting in casualties and property losses. Forecasting rapidly developing coastal bow echoes remains challenging due to limited understanding of the interactions between mesoscale dynamics and microphysical processes. Here, we analyze these interactions using improved multi-Doppler wind retrievals and polarimetric radar observations. The system evolved into a leading convective&ndash;trailing stratiform structure, reinforced by a rear-inflow jet (RIJ) that enhanced low-level convergence and shaped bowing segments. Feedbacks between RIJ-driven downdrafts, convective updrafts, and hydrometeor recycling sustained precipitation and prolonged the system&rsquo;s lifetime after landfall. In particular, mixed-phase hydrometeors in stratiform clouds were advected into the leading convective line, where they enhanced and maintained deep convection. These dynamic&ndash;microphysical interactions governed storm organization and rainfall efficiency, explaining the persistence of heavy precipitation in the coastal zone. Beyond advancing process understanding, our results highlight the role of land&ndash;sea contrasts in shaping mesoscale circulations that intensify convection and provide observational benchmarks for improving forecasts and hazard resilience in coastal regions.]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1878</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1878/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg138650</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Macroalgal influence on particulate organic matter sources and early transformation in an Arctic fjord]]></dc:title>
      <dc:creator>Jagtap, Ashok S.</dc:creator>
      <dc:creator>Singh, Archana</dc:creator>
      <dc:creator>Jain, Anand</dc:creator>
      <dc:creator>Raj, Nandini</dc:creator>
      <dc:creator>Tiwari, Manish</dc:creator>
      <dc:description><![CDATA[<p>Accelerated Arctic warming is promoting the expansion of coastal macroalgal habitats; yet their influence on pelagic organic carbon cycling remains unresolved. This study investigates the influence of macroalgal beds on the biochemical composition of surface particulate organic matter (POM) in Kongsfjorden, Svalbard, during late summer 2023. Surface waters were sampled at four macroalgal-dominated sites (MDS) and from adjacent waters (Adj-W) located 500 and 1500 <span class="inline-formula">m</span> away. A multi-proxy approach integrating elemental composition, stable isotopes, biopolymeric fractions, monosaccharides, and amino acids was used to trace macroalgal contributions and their lateral redistribution. Concentrations of particulate organic carbon, nitrogen, carbohydrates, and proteins were consistently higher at MDS than in Adj-W, indicating localized enrichment of biochemically labile organic matter within macroalgal habitats. Molecular analyses further revealed elevated concentrations of macroalgal-associated sugars (glucose, galactose, fucose, mannuronic acid) and labile amino acids (Asp, Glu, Gly, Ser, Ala) reinforcing macroalgal-derived contributions to surface POM. While <span class="inline-formula"><i>δ</i><sup>13</sup>C<sub>POC</sub></span> showed minimal spatial variation (<span class="inline-formula">−</span>26.8 ‰ to <span class="inline-formula">−</span>29.1 ‰), the biochemical and molecular signatures indicated a decreasing macroalgal contribution towards Adj-W, along with internal reorganization, suggesting lateral transport of macroalgal-derived POM with selective early-stage transformation. Overall, these findings indicate that Arctic macroalgal beds act as dynamic coastal biogeochemical hotspots, redistributing and transforming organic carbon beyond their habitat.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-4227-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/4227/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg129898</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The mirabilite microbiocosm in a Carpathian contact cave]]></dc:title>
      <dc:creator>Moldovan, Oana Teodora</dc:creator>
      <dc:creator>Theodorescu, Crin-Triandafil</dc:creator>
      <dc:creator>Levei, Erika Andrea</dc:creator>
      <dc:creator>Cadar, Oana</dc:creator>
      <dc:description><![CDATA[<p>This study examines the microbial and geochemical environment surrounding mirabilite (sodium sulfate decahydrate) deposits in Izvorul Tăușoarelor Cave, located in the Romanian Carpathians. Using a metabarcoding approach, we analysed mirabilite, sediments, dipluran insects, drip water, and moonmilk deposits to investigate the microbial communities and elemental profiles linked to mirabilite formation. Elemental analysis revealed a geochemical signature in mirabilite samples that was dominated by sodium, sulfur, and calcium. Microbial profiling revealed a unique pattern: sulfur-reducing bacteria, such as <i>Desulfobacterota,</i> were absent from mirabilite samples, whereas <i>Pseudomonas</i> dominated, suggesting an alternative sulfur cycling pathway that may involve sulfide biooxidation. The presence of ammonia-oxidising archaea (<i>Ca. Nitrocosmicus</i>) exclusively in the mirabilite area, and of bacteria (<i>Nitrococcus</i>), indicates a possible influence from a small bat colony, which contributes minimal ammonia that may support the microbial equilibrium required for mirabilite growth. <i>Actinomycetota</i>, abundant in mirabilite, may facilitate mineral crystallisation through mycelium-like structures. We propose the term “microbiocosm” to describe the interconnected network of biotic and abiotic elements surrounding the mirabilite environment and present a novel framework for investigating microbial contributions to its formation.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-4213-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/4213/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg137527</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Experimental assessment of benthic foraminifera as salinity bioindicators: Integrating morphological and eDNA approaches]]></dc:title>
      <dc:creator>Cao, Yifei</dc:creator>
      <dc:creator>Fa, Wenlong</dc:creator>
      <dc:creator>Lei, Yanli</dc:creator>
      <dc:description><![CDATA[<p>Benthic foraminifera are extensively used as bioindicators for paleoenvironmental reconstruction, and environmental DNA (eDNA) analysis provides a powerful lens to uncover their community diversity and environmental responses. Foraminifera are commonly used to assess salinity changes in estuary settings, but quantitative experimental studies of their responses to salinity gradients are scarce. Here, sediments from the intertidal zone of Qingdao Bay were subjected to a 10-week controlled culture across 13 salinity levels (0–60 Practical Salinity Units, PSU), and community dynamics were analysed using both morphological and eDNA approaches. Foraminifera exhibited broad salinity tolerance (0–60 PSU). Analyses of both morphological and molecular datasets revealed a significant increase in community diversity with salinity (<span class="inline-formula"><i>p</i>&lt;0.05</span>), accompanied by a marked decrease in the relative abundance of calcified Rotaliida (<span class="inline-formula"><i>p</i>&lt;0.01</span>). The inverse relationship for Rotaliida was quantitatively robust and well-described by a linear regression model. The eDNA analysis revealed that soft-bodied Monothalamiids, often overlooked morphologically, reached up to 76.2 % relative abundance (average 56.1 %). In contrast, the salinity-driven increase in high-Mg calcite-shelled Milioliida was observed only through morphological analysis. These results demonstrate the distinct but complementary nature of morphological and molecular methods. This study addresses the scarcity of experimental constraints on salinity responses, offering a calibrated reference for applying foraminifera in both ecological assessment and paleo-reconstruction in marginal marine environments.</p>]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-4187-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/4187/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg139162</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Invertebrate communities on seasonal snow patches in the European lowlands are shaped by tree canopy-derived organic inputs]]></dc:title>
      <dc:creator>Lukashanets, Dzmitry</dc:creator>
      <dc:creator>Zawierucha, Krzysztof</dc:creator>
      <dc:creator>Petkuvienė, Jolita</dc:creator>
      <dc:creator>Overlingė, Donata</dc:creator>
      <dc:creator>Vaičiūtė, Diana</dc:creator>
      <dc:creator>Kalvaitienė, Greta</dc:creator>
      <dc:creator>Kataržytė, Marija</dc:creator>
      <dc:description><![CDATA[<p>The cryosphere encompasses a wide range of habitats that support cold-adapted communities. Seasonal snow patches (SSPs) in lowlands are underexplored cryohabitats, characterised by a short persistence period (late winter–early spring) and the presence of trees around, in contrast to large vegetation-free high-mountain and polar ecosystems. To provide the first assessment of organisms from SSPs, we focused on invertebrate diversity and densities from 40 sites in the Baltic States in relation to physicochemical parameters (i.e., suspended solids, chlorophyll <span class="inline-formula"><i>a</i></span>, nutrients), microalgae, and surrounding landscape features (i.e., tree canopy cover). SSPs appeared to be an important spot for bdelloid rotifers (Bdelloidea), tardigrades (Tardigrada), and nematodes (Nematoda), which together accounted for 60 %–100 % of all invertebrates, reaching densities <span class="inline-formula">&gt;7000</span> <span class="inline-formula">ind m<sup>−2</sup></span>. Acari and Insecta were less abundant, whereas other invertebrates occurred only sporadically. The community was strongly determined by surroundings (trees), which supply snow ecosystems with organic and inorganic matter. Chlorophyll <span class="inline-formula"><i>a</i></span>, particulate phosphorus, total suspended solids and organic debris were strongest predictors of invertebrate distribution. The canopy cover also influenced invertebrate communities, highlighting the importance of the organic deposition from trees and also suggesting that trees may be a source of microscopic invertebrates to the snow. Results demonstrate the importance of SSPs as overlooked ephemeral habitats and can be used as a baseline for future changes in snow communities in temperate regions.</p>]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-4199-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/4199/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139159</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Observing formation and early evolution of contrails formed by IAGOS aircraft using high-resolution LEO satellite imagery]]></dc:title>
      <dc:creator>Woldhuis, Thymen</dc:creator>
      <dc:creator>Engberg, Zebediah</dc:creator>
      <dc:creator>Rohs, Susanne</dc:creator>
      <dc:creator>Meijer, Vincent</dc:creator>
      <dc:description><![CDATA[Persistent contrails and contrail cirrus are estimated to be a major contributor to the climate impact of aviation. The mitigation of these impacts by means of technological or operational changes benefits from the ability to skillfully model the formation, evolution, and impacts of contrails. Although these models can be evaluated and improved by use of observations of contrails obtained from remote sensing instruments, these comparisons are hindered by uncertainty in the required meteorological data (such as relative humidity) and limitations in the method of observation (such as younger contrails not being observable in geostationary satellite imagery). To address these challenges, we collocate aircraft equipped with in-situ humidity sensors from the IAGOS fleet in high-resolution (10&ndash;30 m) satellite imagery obtained by instruments aboard the low Earth orbit Sentinel-2 and Landsat missions. The resulting dataset consists of 543 IAGOS aircraft found in satellite imagery (51 % of which form contrails), which we use to evaluate predictions of contrail formation by the Schmidt-Appleman criterion (SAC) as well as predictions of contrail growth by the CoCiP model. When accounting for uncertainty in the IAGOS measurements of humidity and temperature, we find that the SAC correctly explains 98.3 % of the observations. Disagreement between predictions and observation increases when using meteorological data from the ERA5 reanalysis, with only 92.1 % of the observations being explained correctly. Out of the 195 annotated contrails, 48.2 % of these contrails were found to persist for longer than 10 s (approximately the jet phase) and 8.7 % longer than 120 s (approximately the vortex phase). The relative humidity with respect to ice is found to correlate most strongly with observed contrail lifetime, exhibiting an R<sup>2</sup> value of 0.49 with the logarithm of contrail age. The observed horizontal growth during the jet and vortex phases is consistent with previous observations and contrail model results. Although the limited lifetimes of the annotated contrails prevent robust statistical conclusions for the dispersion phase, three example cases show horizontal growth rates consistent with simulations by CoCiP and that of observations in literature. Overall, this study demonstrates the potential of high-resolution LEO satellites to create observational datasets for evaluating and improving models of contrail formation and early evolution.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1171</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1171/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142538</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Summer oxygen dynamics in the bottom waters of a wide, temperate shelf sea]]></dc:title>
      <dc:creator>Meng, Xin</dc:creator>
      <dc:creator>Mahaffey, Claire</dc:creator>
      <dc:creator>Wihsgott, Juliane</dc:creator>
      <dc:creator>Sharples, Jonathan</dc:creator>
      <dc:description><![CDATA[Seasonal depletion of dissolved oxygen (DO) in stratified shelf seas has important consequences for benthic and pelagic ecosystems and biogeochemical cycling. There is a need to understand the importance of different processes contributing to the bottom water oxygen budget, and how those processes might change in a warmer ocean. Using CTD observations from the UK Shelf Sea Biogeochemistry programme, we construct a summer DO budget for the bottom waters of the Celtic Sea and use the budget to assess how bottom water DO might change in a warmer climate. Across the shelf, bottom water DO concentration declined during summer stratification, with greater losses in shallow northern waters and slower depletion in deeper southern regions. At a well-sampled site in the central Celtic Sea, the bottom water shows a consistent net DO loss of &ndash;44 &plusmn; 4 mmol m⁻&sup2; d⁻&sup1;. Respiration and remineralization dominate this decline (&ndash;54 &plusmn; 19 mmol m⁻&sup2; d⁻&sup1;), while vertical turbulent fluxes from the subsurface chlorophyll maximum (SCM) form an important DO source (30 &plusmn; 17 mmol m<sup>-2</sup> d<sup>-1</sup>). Episodic wind events enhance DO supply from the SCM, helping to offset some of the DO consumption in the bottom water. Benthic oxygen demand and horizontal transports make minor contributions to the DO budget. A +2 &deg;C &ldquo;business as usual&rdquo; climate warming will reduce oxygen solubility and lead to a 12 mmol m<sup>-3</sup> drop in DO concentration in the bottom water over the summer stratified period. However, we find that increased microbial metabolic rates in the warmer bottom water are more important for changes in bottom water DO concentrations, potentially driving a decrease in DO concentration of about 35 &ndash; 66 mmol m<sup>-3</sup>. Combined, these effects will lead to increased oxygen deficiency in the central and northern Celtic Sea. Our results demonstrate the importance of metabolic responses to a warmer ocean, but also the need to better understand changes in winds and wind-driven mixing across the seasonal thermocline.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3505</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3505/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142536</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A Multi-Angle and Polarization-Based Retrieval Algorithm for Aerosol Layer Height of Smoke and Dust]]></dc:title>
      <dc:creator>Li, Pei</dc:creator>
      <dc:creator>Xue, Yong</dc:creator>
      <dc:creator>Dionisi, Davide</dc:creator>
      <dc:creator>Li, Huihui</dc:creator>
      <dc:creator>Wu, Shuhui</dc:creator>
      <dc:creator>Jiang, Xingxing</dc:creator>
      <dc:creator>He, Botao</dc:creator>
      <dc:creator>Wang, Peng</dc:creator>
      <dc:creator>Han, Liying</dc:creator>
      <dc:description><![CDATA[The vertical distribution of aerosols governs their interactions with solar radiation and clouds, making it a key factor in their climatic and environmental effects. Existing passive methods for retrieving aerosol layer height (ALH) largely rely on a single observational dimension, such as spectral or multi-angle information, which provides limited constraints under complex aerosol conditions. To address this, we extend conventional spectral approaches by incorporating multi-angle polarimetric observations. Leveraging the high sensitivity of polarization signals to differences between molecular Rayleigh and aerosol scattering, along with broader scattering angle sampling, sensitivity to aerosol vertical structure is significantly enhanced. Using a vector radiative transfer model and information content analysis, we evaluate the contributions of multi-angle and polarimetric information to ALH retrieval. Results show that, compared with radiance-only observations, multi-angle polarimetric measurements substantially increase the degrees of freedom for signal, thereby improving ALH accuracy. An optimal estimation method is developed using HARP2 multi-angle polarimetric observations aboard PACE. Retrieved ALH values are validated against ATLID lidar observations on EarthCARE. For all collocated samples, HARP2 retrievals achieve a root mean square error (RMSE) of 1.03 km, significantly lower than the 1.40 km from TROPOMI, with a near-zero bias (&minus;0.07 km). For smoke, the RMSE is 1.12 km, and for dust it further decreases to 0.92 km. In a typical dust transport event, 84.5 % of retrieval errors are smaller than 1 km, highlighting the marked accuracy advantage of multi-angle polarimetric observations in ALH retrieval.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3503</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3503/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142512</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Temporal variability in offshore Fe fluxes in the Peruvian oxygen minimum zone across an El Ni&ntilde;o termination]]></dc:title>
      <dc:creator>Chen, Guanghui</dc:creator>
      <dc:creator>Rapp, Insa</dc:creator>
      <dc:creator>Sieber, Matthias</dc:creator>
      <dc:creator>Achterberg, Eric P.</dc:creator>
      <dc:creator>Conway, Tim J.</dc:creator>
      <dc:creator>Gledhill, Martha</dc:creator>
      <dc:creator>Hopwood, Mark J.</dc:creator>
      <dc:creator>Xie, Ruifang C.</dc:creator>
      <dc:description><![CDATA[Offshore fluxes of Fe in the Peruvian oxygen minimum zone are sensitive to seawater redox state, and potentially modulated by the El Ni&ntilde;o-Southern Oscillation. However, observational data on what controls such temporal variation in offshore Fe fluxes remain scarce. Here, we report seawater concentrations of dissolved Fe (dFe), particulate Fe (pFe), and their isotopic compositions (&delta;<sup>56</sup>dFe and &delta;<sup>56</sup>pFe) from two transects at 12&deg; S and 14&deg; S across the Peruvian shelf. Our data show clear shelf-to-slope dFe and pFe plumes with negative &delta;<sup>56</sup>Fe signatures. Maximum Fe concentrations at 12&deg; S decreased from 13 to 4 nmol kg<sup>&minus;1</sup> (dFe) and 122 to 13 nmol kg<sup>&minus;1</sup> (pFe) over a month across an El Ni&ntilde;o event termination. We link these variations to an intensifying Peru-Chile Undercurrent which enhanced oxygen supply and thereby weakened sedimentary reductive Fe effluxes. Off shelf, elevated &delta;<sup>56</sup>dFe and low &delta;<sup>56</sup>pFe in anoxic waters are attributed to organic ligand binding and authigenic Fe formation.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3486</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3486/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142447</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Sensitivity of grounding zone melting to subglacial discharge configuration and sediment dynamics across contrasting ice shelf cavity regimes]]></dc:title>
      <dc:creator>Papapetros, Paola</dc:creator>
      <dc:creator>Galton-Fenzi, Benjamin K.</dc:creator>
      <dc:creator>Gwyther, David E.</dc:creator>
      <dc:creator>Boeira Dias, Fabio</dc:creator>
      <dc:creator>Cook, Sue</dc:creator>
      <dc:creator>Zhao, Chen</dc:creator>
      <dc:description><![CDATA[Subglacial freshwater discharge plays a critical role in modulating basal melting and ocean circulation beneath ice shelves, yet the combined influence of discharge configuration, cavity thermal state, and sediment-driven morphodynamics remains poorly constrained. Using idealised ocean simulations following the ISOMIP+ framework, we investigate how subglacial discharge location, configuration (channelised versus distributed), and sediment load interact with contrasting warm and cold cavity regimes, and how these processes influence the circulation, melt, and seabed evolution at the grounding zone. Melt rates differ markedly between warm and cold regimes, with values in the warm cavity an order of magnitude higher than in the cold cavity. However, relative to no-discharge control experiments, subglacial discharge induces substantially greater local melt anomalies at the grounding line in the cold cavity, where localised melt rate increases up to ~955 %, compared to ~173 % in the warm regime. Discharge location and configuration further control the spatial extent of the response, with channelised inputs driving strong, localised melting, and distributed inputs producing weaker but more spatially extensive melt across the grounding zone. Sediment-laden subglacial discharge consistently reduces localised melt under channelised configurations (~13 % reduction in the warm regime and ~16 % in the cold regime), whereas its influence is negligible (&lt;1 %) when discharge is distributed. These reductions arise primarily through morphodynamic feedbacks, as sediment modifies seabed structure and circulation near the grounding zone. In the cold regime, reduced circulation promotes sediment accumulation and episodic erosion, leading to seabed and circulation changes. These results demonstrate that the impact of subglacial discharge on basal melt depends on the combined effects of cavity regime, discharge configuration, and sediment dynamics, with implications for representing grounding zone processes and basal melt parametrisations in ice-ocean models, and ultimately for ice shelves vulnerability and Antarctic Ice Sheet stability.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3435</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3435/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142503</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Analysis of inorganic chlorine chemistry in the midlatitude summer stratosphere using aircraft and satellite observations]]></dc:title>
      <dc:creator>Wilmouth, David</dc:creator>
      <dc:creator>Hare, Jennifer</dc:creator>
      <dc:creator>Howar, Laila</dc:creator>
      <dc:creator>Salawitch, Ross</dc:creator>
      <dc:creator>Hintsa, Eric</dc:creator>
      <dc:creator>Smith, Jessica</dc:creator>
      <dc:creator>Sayres, David</dc:creator>
      <dc:creator>Anderson, James</dc:creator>
      <dc:creator>Clair, Jason</dc:creator>
      <dc:creator>Delaria, Erin</dc:creator>
      <dc:creator>Hannun, Reem</dc:creator>
      <dc:creator>Hanisco, Thomas</dc:creator>
      <dc:creator>Czizco, Daniel</dc:creator>
      <dc:creator>Shen, Xiaoli</dc:creator>
      <dc:creator>Homeyer, Cameron</dc:creator>
      <dc:creator>Santee, Michelle</dc:creator>
      <dc:creator>Bui, T. Paul</dc:creator>
      <dc:creator>Newman, Paul</dc:creator>
      <dc:creator>Keutsch, Frank</dc:creator>
      <dc:creator>Bowman, Kenneth</dc:creator>
      <dc:description><![CDATA[In recent years, significant perturbations to stratospheric inorganic chlorine have been observed following wildfires or volcanic eruptions, as well as modeled in simulations with elevated water vapor from overshooting convection or organic species in biomass burning aerosol. A detailed evaluation of inorganic chlorine in the stratosphere sampled under various conditions is presented here using high precision in situ aircraft measurements of chlorine monoxide (ClO) and chlorine nitrate (ClONO<sub>2</sub>). Data were obtained over North America during the NASA Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) mission. The vertical distributions of ClO and ClONO<sub>2</sub> from all 29 research flights of the 2-year mission are found to be relatively compact and lacking substantial outliers. The peak mixing ratios are approximately 30 ppt and 400 ppt for ClO and ClONO<sub>2</sub>, respectively. No chlorine activation was observed in the lower stratosphere in the presence of low temperatures and elevated water vapor from convective injection. Steady-state calculated ClONO<sub>2</sub> is found to be in good agreement with measured values, suggesting that a reduction in the uncertainty of the recommended rate coefficient for ClONO<sub>2</sub> production is possible. HCl is calculated at high time resolution throughout the mission using satellite data, and the resulting evaluation of the inorganic chlorine budget shows excellent agreement, with the ratio of ClO + ClONO<sub>2</sub> + HCl to total inorganic chlorine equal to 0.95 for mixing ratios greater than 500 ppt. No evidence of inorganic chlorine activation was observed during DCOTSS when aerosol organic mass fraction and biomass burning fraction were elevated.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3480</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3480/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142489</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Quantifying air&ndash;sea CO2 fluxes above desert-fringing coral reefs in the northern Red Sea revealed by eddy covariance]]></dc:title>
      <dc:creator>McGowan, Hamish</dc:creator>
      <dc:creator>Abir, Shai</dc:creator>
      <dc:creator>Lensky, Nadav</dc:creator>
      <dc:creator>Shaked, Yonathan</dc:creator>
      <dc:description><![CDATA[Eddy covariance (EC) measurements of air-sea CO<sub>2</sub> exchange over desert fringing coral reefs in the Gulf of Eilat (Aqaba) (GoE), northern Red Sea, show these ecosystems are net sinks of atmospheric CO<sub>2</sub>. This result contrasts with marine productivity models and bulk formula calculations based on water chemistry that are often used methods to determine the magnitude and direction of the CO<sub>2</sub> flux with the atmosphere over coral reefs. These studies have often concluded that coral reefs are net sources of CO<sub>2</sub> to the atmosphere with only rare cases finding otherwise. Our EC measurements find coral reefs in the GoE may absorb around 4.5 times more carbon from the atmosphere than other marine and terrestrial ecosystems and only slightly less than some tropical rainforests. This highlights the need for further direct measurements of air-sea CO<sub>2</sub> exchanges over coral reefs in different environmental settings so their role in the global carbon cycle can be accurately quantified.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3467</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3467/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142466</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[QBO-induced anomalous transport in the Northern Hemisphere stratosphere: the exceptional 2018/2019 late boreal winter]]></dc:title>
      <dc:creator>Minganti, Daniele</dc:creator>
      <dc:creator>Chabrillat, Simon</dc:creator>
      <dc:creator>Davis, Sean</dc:creator>
      <dc:creator>Errera, Quentin</dc:creator>
      <dc:creator>beeck, Marc</dc:creator>
      <dc:creator>Ray, Eric</dc:creator>
      <dc:creator>Vervalcke, Sarah</dc:creator>
      <dc:creator>Wargan, Krzysztof</dc:creator>
      <dc:creator>Wespes, Catherine</dc:creator>
      <dc:description><![CDATA[Large positive anomalies of nitrous oxide (N<sub>2</sub>O) were observed in the northern hemisphere lower stratosphere in the late 2018/2019 boreal winter. Thanks to its long lifetime in the lower stratosphere, N<sub>2</sub>O is a robust tracer for stratospheric transport. This study investigates the magnitude, vertical structure, and dynamical origin of the late 2018/2019 boreal winter N<sub>2</sub>O anomaly using multiple chemical transport model simulations, chemical reanalyses, a specified-dynamics chemistry-climate model, and merged satellite observations. All datasets consistently show pronounced N<sub>2</sub>O positive anomalies in February 2019 in the northern mid-latitudes at 50 hPa. The N<sub>2</sub>O Transformed Eulerian Mean budget indicates that the N<sub>2</sub>O anomalies are primarily driven by enhanced meridional residual advection, which is in turn determined by enhanced planetary wave forcing. The extratropical effects of the quasi-biennial oscillation (QBO) determine these transport anomalies: the poleward QBO secondary circulation was unusually strong in the late 2018/2019 boreal winter, and a marked northward displacement of the zero wind line induced the enhanced planetary wave forcing. The combined strengthening of both the northward QBO secondary circulation and the planetary wave forcing led to unusually strong poleward advection in the northern lower stratosphere, which ultimately built up the N<sub>2</sub>O positive anomalies. These results indicate the value of long-lived stratospheric tracers such as N<sub>2</sub>O for diagnosing dynamically driven extreme events and for disentangling the contributions of different transport processes. We highlight the importance of the QBO teleconnections, particularly as a warming climate may change the frequency and intensity of extreme events thereby impacting these teleconnections.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3449</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3449/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142456</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Advancing meteorite impact chronology with in situ mica Rb-Sr dating]]></dc:title>
      <dc:creator>Ribeiro, Bruno</dc:creator>
      <dc:creator>Squire, Jayden</dc:creator>
      <dc:creator>Kirkland, Chris</dc:creator>
      <dc:creator>Farkas, Juraj</dc:creator>
      <dc:creator>Loyola, Cecilia</dc:creator>
      <dc:creator>Cousins, Victoria</dc:creator>
      <dc:creator>Gostin, Victor</dc:creator>
      <dc:creator>Verdel, Charles</dc:creator>
      <dc:description><![CDATA[Meteorite impacts are highly energetic processes that drives deformation on Earth under extreme pressure and temperature conditions, far exceeding those of typical crustal processes. Consequently, it may promote environmental perturbations, blossoming/extinction of life and even produce suitable conditions for the formation of mineral resources. Thus, constraining the timing of impacts is pivotal to shedding light on its role in Earth&rsquo;s biogeodynamics, yet less than ~20 % of the impacts worldwide are precisely dated. Here, we present novel in situ mica Rb&ndash;Sr isotopes from the Australian Acraman and Gosses Bluff impact sites collected via LA-ICP-MS/MS, including single- and multi-collector instruments to expand the chronological toolbox for dating meteorite impacts. Whilst monazite (980 &plusmn; 28 Ma) and apatite (1448 &plusmn; 79 Ma) yield older ages compared to the expected Acraman impact age of 588 &plusmn; 35 Ma, in situ Rb&ndash;Sr from muscovite-bearing domains from the Acraman ejecta layer (580 &plusmn; 8 Ma; multi-collector age) and associated fine-grained zircon (598 &plusmn; 16 Ma) are consistent with the expected impact age. Similarly, apatite (132 &plusmn; 14 Ma) and mica-bearing domains (137 &plusmn; 9 Ma; multi-collector age) are comparable to the proposed impact age of 133 &plusmn; 3 Ma, whilst zircon yields mostly discordant data. The Rb&ndash;Sr results comparison between single- and multi-collector ICP-MS/MS has shown that the latter yielded significantly more precise Sr measurements, likely due to measurement of St isotopes with high resistor Faraday cups (10<sup>13</sup> &Omega;) resulting in improved signal-to-noise ratio, consequently yielding more precise isotopic ratios and isochron ages. Our findings show that in situ Rb&ndash;Sr dating of micas formed during impact metamorphism offers the means for determining the timing of meteorite impact events. This approach effectively addresses the textural complexities commonly present in impact-related rocks, which are often overlooked by bulk isotope-dilution techniques, and delivers accuracy sufficient to establish the age of impacts. The effectiveness of in situ Rb&ndash;Sr dating of impact-related micas may be attributed to their higher resistance to hydrothermal alteration compared to Ar isotopes, which often yield complex degassing spectra and younger apparent ages such as for the Acraman impact. This study shows that in situ Rb&ndash;Sr isotopes of newly grown micas in impact-related rocks refines the chronology of impacts, with potential to increase the number of dated impacts globally with a low-cost, speedy technique with minimum sample preparation. Such task is crucial for understanding the role of meteorite impacts, including their potential influence on environmental crises, mass extinctions, and the emergence of life.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3441</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3441/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142441</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A low-dimensional framework for interpreting Northern Hemisphere winter extratropical precipitation trends]]></dc:title>
      <dc:creator>Kim, Ha-Rim</dc:creator>
      <dc:creator>Yoo, Changhyun</dc:creator>
      <dc:creator>Seo, Hyodae</dc:creator>
      <dc:creator>Kim, Baek-Min</dc:creator>
      <dc:description><![CDATA[Extratropical precipitation trends are strongly affected by changes in large-scale circulation, but the relevant dynamic signals are often difficult to isolate in climate models. Here, we introduce a low-dimensional framework that reconstructs Northern Hemisphere winter precipitation trends from leading modes of 500-hPa geopotential-height variability. The framework decomposes circulation variability into transient, stationary, and interaction components, and links their EOF modes to precipitation using ERA5 and CMIP6 historical and SSP5-8.5 simulations. In ERA5, the leading circulation modes reproduce much of the observed precipitation redistribution, with drying in the subtropics and wetting in the midlatitudes. The transient storm-track component dominates the reconstruction, with shift and sharpening modes accounting for most of the circulation-linked precipitation trend. CMIP6 models capture the broad meridional structure of this response but underestimate its amplitude. The weak multi-model mean response results from large intermodel spread and sign cancellation in the pulsing and shift modes, while the sharpening mode remains more coherent across models. Under SSP5-8.5, circulation-induced precipitation trends become weaker relative to total precipitation trends, consistent with an increasing role of thermodynamic moistening. Nevertheless, the spatial structure of precipitation change remains strongly tied to storm-track variability. These results suggest that uncertainty in future extratropical precipitation redistribution depends not only on the magnitude of warming but also on how models represent the modal structure of storm-track change and its coupling to precipitation.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3431</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3431/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142431</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Simulated Antarctic iceberg melting occurs primarily within the Southern Ocean mixed layer]]></dc:title>
      <dc:creator>Olivé Abelló, Anna</dc:creator>
      <dc:creator>Mathiot, Pierre</dc:creator>
      <dc:creator>Jourdain, Nicolas C.</dc:creator>
      <dc:creator>Kostov, Yavor</dc:creator>
      <dc:creator>Holland, Paul R.</dc:creator>
      <dc:description><![CDATA[Although iceberg meltwater accounts for nearly half of the freshwater release from the Antarctic ice sheet, most ocean models do not represent the vertical distribution of this meltwater in a realistic way. Here, we investigate the importance of distributing the iceberg meltwater vertically in an ocean model that represents icebergs as Lagrangian particles. For more robust estimates, we update the iceberg melting laws: (i) we extend the three-equation formulation used for ice shelf melting to the iceberg basal melt parameterisation, (ii) we adopt a new formulation of lateral iceberg melt in which the buoyant plumes are fed by basal melt, and (iii) we improve the physical consistency of wave-induced ablation in our equations. The updated formulations produce a substantial increase in average lateral melt and a slight reduction in wave-induced ablation and basal melt compared to the pre-existing configuration. Seasonally, lateral melting becomes a major summer contributor, exceeding basal melting in magnitude, and all iceberg melting components decrease in winter. The enhanced sensitivity of wave-induced ablation to sea-ice concentration suppresses iceberg melting near the Antarctic margin, promoting longer iceberg lifetimes. Sensitivity simulations show that even when meltwater is evenly distributed in the vertical down to the iceberg keel depth, 76 % to 87 % of the iceberg meltwater remains injected into the surface mixed layer. Freshwater injection at depth promotes warming and salinification of the Amundsen Sea near the seabed, and freshens and cools the East Antarctic and western Ross Sea continental shelves, but all these changes have a small magnitude. Also, it leads to thinner sea ice and locally enhanced sea-ice production, especially in the southwestern Weddell Sea. Overall, these results imply that, for Southern Ocean-scale responses, modelling studies to date that release iceberg meltwater at the surface can still be considered reliable.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3422</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3422/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142419</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Deep-learning prediction of high-frequency sea-level oscillations in the Adriatic Sea]]></dc:title>
      <dc:creator>Međugorac, Iva</dc:creator>
      <dc:creator>Metličić, Nikola</dc:creator>
      <dc:creator>Šepić, Jadranka</dc:creator>
      <dc:creator>Rus, Marko</dc:creator>
      <dc:creator>Čupić, Srđan</dc:creator>
      <dc:creator>Kristan, Matej</dc:creator>
      <dc:creator>Ličer, Matjaž</dc:creator>
      <dc:description><![CDATA[The eastern Adriatic coast is a known hotspot of strong meteorologically induced high-frequency sea-level oscillations, occurring at periods shorter than 1 hour and reaching wave heights of several metres. When highest, these oscillations are termed meteotsunamis. In this study, we test deep-learning methods for predicting maximum daily amplitudes of high-frequency (T &lt; 1 hour) sea-level oscillations at two Adriatic locations, Bakar and Ploče, using convolutional neural networks driven by past sea-level observations and atmospheric predictors from the ERA5 and CERRA reanalyses. We evaluate two deep-learning architectures designed to test different approaches to representing sea-level and atmospheric forcing. The first architecture, HFNet, is based on the HIDRA family of models, a general low-frequency sea-level forecasting framework that has been extensively evaluated in the Adriatic and shown to provide a credible baseline for sea-level prediction. The second architecture, HFNet<sub>JE</sub>, extends this approach through joint encoding of atmospheric predictors and a more extensive processing of past sea-level information, with the aim of improving the representation of processes associated with high-frequency sea-level oscillations. Analysis of more than 20 years of data shows that high-frequency sea-level extremes are larger in Bakar (&gt; 60 cm) than in Ploče (&lt; 35 cm), occur ~6 times per year, and are most common during the warm season. Both architectures reproduce the observed variability, with higher skill for typical than for extreme events. HFNet<sub>JE</sub> performs best overall and under typical amplitude conditions, whereas HFNet more effectively captures extreme events, although these remain systematically underestimated in both architectures. Model performance is higher at Ploče, likely because of its smaller sea-level range and simpler response to atmospheric forcing. Models forced with ERA5 consistently outperform those using the higher-resolution CERRA in predicting extremes, suggesting limited added value from increased spatial resolution. Ablation experiments indicate that several predictors are redundant for average forecasting performance, whereas extreme-event prediction generally benefits from the full predictor set. Overall, the results demonstrate the potential of deep learning for prediction of high-frequency sea-level oscillations in the Adriatic, but also highlight persistent limitations in forecasting rare high-amplitude events.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3411</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3411/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140754</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[On combining climate models into weighted ensembles]]></dc:title>
      <dc:creator>Grusdt, Britta</dc:creator>
      <dc:creator>Perrette, Mahé</dc:creator>
      <dc:creator>Robinson, Alexander</dc:creator>
      <dc:description><![CDATA[Several methods have been proposed and used to refine estimates of future climate change based on combined output from comprehensive climate models. While previously the so-called model democracy approach was used to combine model predictions, where every model is given equal weight, it is now widely accepted that using model weights that account for model performance and model independence is necessary to obtain more reliable results. However, most existing approaches rely, implicitly or explicitly, on a similar statistical basis, while describing things in different ways. Here we distinguish between approaches that are based on the performance of individual models (individual performance weighting) and approaches that are based on the performance of the weighted ensemble as a whole (ensemble performance weighting). At the same time, we formulate both in probabilistic Bayesian terms to make their application and comparison straightforward. Using simple constructed examples, we demonstrate that the ensemble performance weighting approach implicitly accounts for co-dependencies among models, which arguably makes the computation of independence weights for the purpose of model weighting obsolete. We also show that a set of weighted models within the ensemble weighting approach will naturally tend to artificially reduce uncertainty and that this is strongly influenced by the choice of the prior distribution over weight vectors. The distinction between individual and ensemble performance weighting is both methodological and conceptual. Formulating both approaches in general probabilistic Bayesian terms as done here, can serve as a common basis for future developments with regard to ensemble model weighting in Earth system science.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2320</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2320/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141362</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[ENSO Modulation of PM2.5 air pollution in Central Kalimantan, Indonesia revealed by a dense network of Purple Air sensors]]></dc:title>
      <dc:creator>Graham, Ailish M.</dc:creator>
      <dc:creator>Spracklen, Dominick V.</dc:creator>
      <dc:creator>McQuaid, James B.</dc:creator>
      <dc:creator>Rigby, Richard</dc:creator>
      <dc:creator>Nurrahmawati, Hanun</dc:creator>
      <dc:creator>Ayona, Devina</dc:creator>
      <dc:creator>Salmayenti, Resti</dc:creator>
      <dc:creator>Kusin, Kitso</dc:creator>
      <dc:creator>Jaya, Adi</dc:creator>
      <dc:creator>Smith, Thomas E. L.</dc:creator>
      <dc:creator>Alifindira, Annisa</dc:creator>
      <dc:creator>Banna Choiruzzad, Shofwan</dc:creator>
      <dc:creator>Pope, Richard</dc:creator>
      <dc:description><![CDATA[Peatland fires in Indonesia drive severe air pollution. Studies have focused on El Ni&ntilde;o years, therefore neutral and La Ni&ntilde;a years remain uncharacterised. We deploy a dense network of PM<sub>2.5</sub> sensors across Central Kalimantan peatlands between August 2023 and October 2025 to quantify how El Ni&ntilde;o&ndash;Southern Oscillation (ENSO) modulates the magnitude and spatial variability in dry season PM<sub>2.5</sub> concentrations. Sensors were installed at urban, rural, and remote locations, spanning El Ni&ntilde;o (2023), neutral (2024), and La Ni&ntilde;a (2025) dry seasons. During the 2023 El Ni&ntilde;o dry season, low rainfall and deep water tables enhanced peatland flammability and supported extensive peat fires. Urban and rural sites exceeded the WHO 24‑hour PM<sub>2.5</sub> guideline on 99 % and 97 % of days. A remote site exceeded these guidelines on 85 % and 24 % of days, with fire smoke influence confirmed by low spatial variability and a dual‑peak diurnal cycle across sites, indicating regional pollution rather than local sources. As ENSO conditions shifted to neutral (2024) and La Ni&ntilde;a (2025), increased rainfall and shallower water tables reduced fire activity and PM<sub>2.5</sub> concentrations. In 2024, WHO guideline exceedances fell to 41 % and 12 % at urban and rural sites. Our results indicate that even across non-El Ni&ntilde;o years, dry season PM<sub>2.5</sub> is influenced by regional fire emissions, but the magnitude and spatial variability is modulated by ENSO-phase. Our results demonstrate that dense sensor networks can distinguish regional fire smoke from local pollution, enabling early detection of fire‑driven air quality degradation. Reducing peatland fires through restoration and fire management would deliver consistent air quality benefits.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2746</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2746/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142283</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Ensemble reconstruction of the Greenland Ice Sheet evolution through the last deglaciation]]></dc:title>
      <dc:creator>Gutiérrez-González, Lucía</dc:creator>
      <dc:creator>Tabone, Ilaria</dc:creator>
      <dc:creator>Robinson, Alexander</dc:creator>
      <dc:creator>Álvarez-Solas, Jorge</dc:creator>
      <dc:creator>Swierczek-Jereczek, Jan</dc:creator>
      <dc:creator>Grusdt, Britta</dc:creator>
      <dc:creator>Montoya, Marisa</dc:creator>
      <dc:description><![CDATA[The last deglaciation offers valuable insights into ice-climate interactions, as extensive paleoclimatic records document the retreat of ice sheets through a period of major climate changes. During this interval, the Greenland Ice Sheet (GrIS) retreated from its extensive Last Glacial Maximum (LGM) configuration to its present state, passing through the Holocene Thermal Maximum (HTM), when temperatures exceeded present-day values. Despite the large amount of paleoclimatic data available, ice-sheet models struggle to reproduce key aspects of the observational record, and the magnitude of the GrIS contribution to sea level throughout this period, in particular during the LGM and the HTM, remains highly uncertain. In this study, we evaluate an ensemble of 3,000 simulations of the GrIS performed with the Yelmo ice-sheet model against different observational constraints. These include: (1) the LGM ice-sheet extent, (2) ice-core-derived surface elevations, (3) an ice-extent retreat chronology based on the recent PaleoGrIS dataset, and (4) the present-day ice-sheet configuration (ice thickness, ice cover, ice-surface velocity, and bedrock elevation). We characterize the impact of the parameters perturbed along the ensemble on the GrIS evolution using an emulator based on the XGBoost algorithm combined with the SHAP (SHapley Additive exPlanations) framework. This analysis reveals that the climatic parameters (surface melting corrections and ocean thermal sensitivity) dominate the impact. By identifying the simulation that best matches these observables, we provide a constrained reconstruction of the GrIS during the last deglaciation that substantially improves upon previous reconstructions. We obtain a GrIS contribution to global sea level with respect to present of -5.75 m of sea-level equivalent (SLE) at the LGM (with an uncertainty range of -3.93 to -6.31 m) and +0.45 m after the HTM warming (with an uncertainty range of 0.43 to 1.18 m). This is in the upper range of previously existing estimates, indicating a comparatively mid-to-high GrIS sensitivity to climate changes over the last deglaciation.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3331</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3331/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142070</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Continuous Microstructural Characterization of a shallow East Antarctic Ice Core Using Machine Learning Super-Resolution and Micro-CT Imaging]]></dc:title>
      <dc:creator>Bagherzadeh, Faramarz</dc:creator>
      <dc:creator>Freitag, Johannes</dc:creator>
      <dc:creator>Frese, Udo</dc:creator>
      <dc:creator>Wilhelms, Frank</dc:creator>
      <dc:description><![CDATA[This study presents a continuous, high-resolution (60 <em>&mu;m</em>) microstructural analysis of a 130 <em>m</em> long ice core B40 drilled in Austral summer 2012/13 at the German Research station Kohnen on the East Antarctic plateau using artificial intelligence (AI)-enhanced micro-computed tomography (micro-CT) imaging and pore network modeling. Antarctic ice cores serve as valuable archives of past climate and environmental conditions. They consist of a sequence of compacted layers with varying density, ice and pore space structure, which are shaped differently depending on the climatic and environmental conditions during deposition and subsequent compaction. The in-depth development of microstructural features provides insights into the densification and pore closure processes as well as climate trends during the formation of the firn column.</p> <p>However, traditional micro-CT imaging techniques applied to full core samples, although effective, often lack the necessary resolution to capture the intricate microstructure of ice samples fully. To address this limitation, we applied AI-driven super-resolution enhancement methods to improve the clarity and detail of micro-CT images, enabling a more precise quantification of ice core properties. Following AI enhancement, the study performed a comprehensive microstructure analysis on the full firn column, including geometrical, morphological, topological, and transport-related properties. The obtained metrics, including mean intercept length (MIL), cluster size, porosity (density), tortuosity, permeability, etc., can characterize the microstructural evolution of the ice column from snow to bubbly ice across different depths. The results reveal a systematic evolution in pore geometry, connectivity, and transport efficiency with depth, capturing the snow-to-ice transition with high fidelity. Fine and coarse layers were distinguished using the K-means clustering method, and anisotropy was detected in both the ice matrix and the pore space. Principal component analysis (PCA) showed that densification is influenced by multiple factors; in particular, during the pore close-off stage, variations in coordination number and throat dimensions led to distinct densification behaviors among the samples. These findings could contribute to the improvement of densification and air transport models by providing highly accurate data on the microstructure of ice cores and even enabling the definition of new microstructure-related climate proxy parameters.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3185</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3185/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142068</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Current Dynamics, Drivers, and Vertical Thermal Structure around Sir Bu Nair Island (Arabian/Persian Gulf)]]></dc:title>
      <dc:creator>Cavalcante, Geórgenes H.</dc:creator>
      <dc:creator>Vieira, Filipe</dc:creator>
      <dc:creator>Bento, Rita</dc:creator>
      <dc:creator>Bartholomew, Aaron</dc:creator>
      <dc:creator>Burt, John A.</dc:creator>
      <dc:description><![CDATA[Sir Bu Nair Island (SBN) in the central Arabian Gulf is one of the last locations in the UAE&rsquo;s Gulf waters to retain extensive and well developed coral reefs, whereas many nearshore environments have experienced severe degradation following recurrent marine heatwaves. Although tides, winds and subtidal circulation are thought to influence reef-level thermal conditions at SBN, the local physical processes governing circulation and temperature variability have not previously been resolved from in situ observations. Here, we analyse a 17-month record (May 2021&ndash;October 2022) of currents, sea level, and temperature from bottom-mounted ADCPs and multi-depth temperature moorings, complemented by reanalysis of winds. Currents at SBN are strongly anisotropic and aligned along a dominant principal axis, reflecting topographic steering around the island. At the more exposed northwest site, upper-layer along-axis velocities commonly reach ~0.6 m s<sup>&minus;1</sup>, with episodic peaks approaching 0.8&ndash;1.0 m s<sup>&minus;1</sup>, while at the southern site, flows are weaker, with typical upper-layer velocities of ~0.3 m s<sup>&minus;1</sup> and peaks of ~0.5&ndash;0.7 m s<sup>&minus;1</sup>. Tidal forcing dominates the instantaneous flow, explaining up to ~80 % of the along-axis current variance at the northwest site but substantially less in the cross-axis direction and at the southern site, leaving significant subtidal variability. Wind&ndash;current coupling is strongest at subtidal timescales, with rapid (0&ndash;2 h) responses consistent with local barotropic adjustment to wind forcing. Temperature observations reveal pronounced seasonal variability, with summer surface temperatures exceeding 35 &deg;C and annual excursions of more than 15 &deg;C across the water column. A persistent seasonal thermocline develops during late spring and summer, with vertical temperature differences of 2&ndash;4 &deg;C. This stratification is repeatedly disrupted by rapid mixing events lasting 2&ndash;3 days, during which the water column becomes nearly homogeneous. Spectral and variance analyses show that stratification variability is dominated by diurnal processes, with additional modulation at synoptic (2&ndash;4 day) timescales. The results indicate that tidal mixing alone is insufficient to suppress stratification and that episodic destratification arises from the combined influence of wind forcing and subtidal variability acting on a preconditioned water column. These findings provide the first integrated observational description of circulation and thermal structure at SBN, demonstrating how topographic control, tides, winds, and subtidal variability interact to regulate stratification, vertical exchange and transport processes around an isolated reef system in the central Gulf.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3183</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3183/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142025</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Evolution of aerosol composition and optical properties in the Paris urban plume from coordinated airborne and ground-based observations]]></dc:title>
      <dc:creator>Yu, Chenjie</dc:creator>
      <dc:creator>Antonio, Ludovico</dc:creator>
      <dc:creator>DeCarlo, Peter F.</dc:creator>
      <dc:creator>Nault, Benjamin A.</dc:creator>
      <dc:creator>Velazquez-Garcia, Alejandra</dc:creator>
      <dc:creator>Aruffo, Eleonora</dc:creator>
      <dc:creator>Carlo, Piero</dc:creator>
      <dc:creator>Denjean, Cyrielle</dc:creator>
      <dc:creator>Tinorua, Sarah</dc:creator>
      <dc:creator>Bourrianne, Thierry</dc:creator>
      <dc:creator>Pereira, Diana L.</dc:creator>
      <dc:creator>Tu, Kevin</dc:creator>
      <dc:creator>Pangui, Edouard</dc:creator>
      <dc:creator>Cazaunau, Mathieu</dc:creator>
      <dc:creator>Bauville, Astrid</dc:creator>
      <dc:creator>Grand, Noël</dc:creator>
      <dc:creator>Bergé, Antonin</dc:creator>
      <dc:creator>Biagio, Claudia</dc:creator>
      <dc:creator>Gratien, Aline</dc:creator>
      <dc:creator>Beekmann, Matthias</dc:creator>
      <dc:creator>Siour, Guillaume</dc:creator>
      <dc:creator>Foret, Gilles</dc:creator>
      <dc:creator>D'Anna, Barbara</dc:creator>
      <dc:creator>Kammer, Julien</dc:creator>
      <dc:creator>Wu, Huihui</dc:creator>
      <dc:creator>Cantrell, Christopher</dc:creator>
      <dc:creator>Formenti, Paola</dc:creator>
      <dc:creator>Michoud, Vincent</dc:creator>
      <dc:description><![CDATA[Aerosols play a critical role in Earth&rsquo;s climate, but substantial evolution in their physicochemical properties after emission introduces uncertainties in predicting their climate impacts. Observational constraints on how aging modifies aerosol properties remain limited. Here, we investigate the effects of ~2&ndash;6 h of aging on aerosol physicochemical properties using coordinated airborne and ground-based measurements in Paris and its downwind regions. Urban plumes contributed modestly to particle number concentrations in the 80&ndash;200 nm size range and resulted in a moderate enhancement of submicron particle (PM<sub>1</sub>) mass relative to out-plume background levels. Organic aerosol (Org) dominated PM<sub>1</sub> mass both near the urban source and downwind. Aircraft observations showed enhanced Org and non-refractory PM<sub>1</sub> relative to excess CO (CO above surrounding background) in downwind plumes, indicating net secondary organic aerosol production during aging. Aerosol optical properties evolved concurrently. Downwind plume-average single-scattering albedo (SSA) at 450 and 630 nm was higher than near-source values. Consistently, the complex refractive index shifted from lower real (~1.35&ndash;1.40) and higher imaginary (~0.03&ndash;0.08) components near source to higher real (~1.45&ndash;1.50) and lower imaginary (~0.015&ndash;0.02) components downwind. The absorption &Aring;ngstr&ouml;m exponent also increased, indicating a greater fractional contribution of brown carbon to light absorption. These results demonstrate that urban plume aging alters aerosol composition and optical properties and highlight the need to represent evolving aerosol characteristics in atmospheric models and remote-sensing retrievals.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3147</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3147/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142185</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Leveraging leaf-level optimality processes with explicit acclimation improves global GPP representation in an individual-based DGVM (LPJ-GUESS v4.1.1)]]></dc:title>
      <dc:creator>Forrest, Matthew</dc:creator>
      <dc:creator>Dantas de Paula, Mateus</dc:creator>
      <dc:creator>Gomes de Almeida, Filipe</dc:creator>
      <dc:creator>Harrison, Sandy P.</dc:creator>
      <dc:creator>Prentice, I. Colin</dc:creator>
      <dc:creator>Hickler, Thomas</dc:creator>
      <dc:description><![CDATA[Vegetation models are indispensable tools for investigating and projecting the terrestrial carbon cycle, both as standalone models and embedded in global climate models. However, current models vary widely in their representation of ecosystem processes and consequently in their projected future carbon dynamics. Eco-evolutionary optimality (EEO) approaches, which derive and test hypotheses about optimal plant behaviour under specific environmental conditions as a consequence of natural selection, have been proposed as a means to improve the reliability of vegetation models and the robustness of their future projections. Here we embed EEO-derived models for photosynthesis and leaf dark respiration, and their acclimation to changing conditions, into the widely used LPJ-GUESS vegetation model. We evaluated the simulated gross primary production (GPP) patterns against remotely-sensed GPP derived from sun-induced fluorescence and found that the EEO configurations improved the spatial distributions (a mean reduction in error of 15 % across gridcells) and global interannual variability (a mean reduction in error of 32 % after accounting for differences in global totals) compared to the standard version of LPJ-GUESS. Evaluation against GPP fluxes from eddy flux covariance measurements also showed improved performance, the <em>R<sup>2</sup></em> of 5-day GPP increased from 0.45 to 0.48 (averaged across 147 sites). The simulated global carbon pools, fluxes, burnt area and biome distributions were not impacted substantially. The improvements were achieved with no alteration to processes except photosynthesis, respiration and plant water uptake, and with no recalibration or tuning. The EEO configuration also reduced model run time and eliminated the need for poorly-constrained PFT-dependent parameters governing the temperature response of photosynthesis. As well as being a tangible improvement to LPJ-GUESS, this study further confirms the usefulness of EEO approaches to improve global vegetation models.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3273</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3273/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142027</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Impacts of mesh refinement on the simulation of a long-range transported extreme dust storm over East Asia in the global variable-resolution model (iAMAS v2.6.3)]]></dc:title>
      <dc:creator>Xue, Yibo</dc:creator>
      <dc:creator>Zhao, Chun</dc:creator>
      <dc:creator>Feng, Jiawang</dc:creator>
      <dc:creator>Qu, Xin</dc:creator>
      <dc:creator>Xia, Zihan</dc:creator>
      <dc:creator>Yang, Zining</dc:creator>
      <dc:creator>Zhang, Xiaoxiao</dc:creator>
      <dc:creator>Yang, Qike</dc:creator>
      <dc:creator>Li, Gudongze</dc:creator>
      <dc:creator>Zhang, Ziyu</dc:creator>
      <dc:creator>Zhang, Jianxi</dc:creator>
      <dc:description><![CDATA[Long-range transported dust storms challenge regional high-resolution models because lateral boundary conditions constrain the consistent representation of dust emission, transport, and deposition. Here we use the integrated Atmospheric Model Across Scales (iAMAS v2.6.3), a global variable-resolution physics-chemistry coupled model, to simulate the extreme East Asian dust storm from 13 to 18 March 2021. Three experiments adopt a globally quasi-uniform 50 km mesh (U50 km) and two source-refined meshes at 16&ndash;50 km (V16 km) and 4&ndash;50 km (V4 km). Evaluated against reanalysis and ground-based observations, the simulations reproduce the large-scale synoptic evolution, while mesh refinement captures more detailed near-surface dynamical features and terrain-channeled winds through improved topographic representation. The model reasonably represents 10-m wind speed, surface PM<sub>10</sub> concentrations, and aerosol optical depth. Relative to U50 km, total dust emissions over East Asia increase by 35.24 % in V16 km and 54.98 % in V4 km, as refined meshes resolve localized friction-velocity enhancement and nonlinear saltation-threshold exceedances. By altering emission evolution and its interaction with atmospheric circulation, mesh refinement also affects the spatial distribution of transported dust. The contrast between V16 km and V4 km reveals regional heterogeneity in downwind dust mass loading, with V4 km capturing localized wet-scavenging enhancement not evident in V16 km and reducing dust loading over the Yangtze River Delta by 30.49 % relative to U50 km. This research emphasizes the importance of mesh refinement for representing long-range transported dust storms and provides a basis for future evaluations of multiple dust emission schemes in global variable-resolution models.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3149</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3149/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142145</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Fog and low clouds in the Namib Desert may be more resilient than previously thought]]></dc:title>
      <dc:creator>Mass, Alexandre</dc:creator>
      <dc:creator>Cermak, Jan</dc:creator>
      <dc:creator>Knutti, Reto</dc:creator>
      <dc:creator>Merrifield, Anna L.</dc:creator>
      <dc:creator>Andersen, Hendrik</dc:creator>
      <dc:description><![CDATA[Fog and low clouds (FLCs) are essential moisture sources for Namib desert ecosystems. However, their response to climate change remains uncertain because fog processes are not resolved in climate models. Here, we apply a cloud-controlling factor framework in which FLC anomalies are expressed as a linear function of large-scale meteorological drivers, including estimated inversion strength (EIS), relative humidity at 700 hPa (R700), sea surface temperature (SST), and the eastward and northward components of 10 m wind (U10, V10). Sensitivities of FLCs to these drivers are quantified using a statistical model. By applying these sensitivities to projections of the corresponding predictors from CMIP6, we produce the first observationally constrained projections of Namib FLC occurrence. Projected trends remain uncertain and scenario-dependent; however, a robust physical signal emerges. Changes in FLCs are governed by competing influences: SST increase over the southeast Atlantic region reduces FLCs, while increased lower-tropospheric stability as well as circulation changes enhance them. Overall, these results suggest that Namib FLCs may be more resilient to climate change than previously assumed, raising the question of whether similar compensating mechanisms operate in other eastern-ocean boundary-layer upwelling systems, such as those of the Atacama Desert and California.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3242</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3242/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd137795</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[palm_csd 25.10: a processing tool for static input data  in the PALM model system]]></dc:title>
      <dc:creator>Schubert, Sebastian</dc:creator>
      <dc:creator>Anders, Julian</dc:creator>
      <dc:creator>Gronemeier, Tobias</dc:creator>
      <dc:creator>Maronga, Björn</dc:creator>
      <dc:creator>Salim, Mohamed</dc:creator>
      <dc:description><![CDATA[<p>We present palm_csd version 25.10, the current default preprocessing tool for generating the static driver for the building-resolving large-eddy simulation model PALM. The static driver defines the spatial surface characteristics of the simulation domain. This paper provides a technical description of the updated palm_csd workflow, focusing on the processing of buildings, vegetation, pavement, water bodies, terrain height and land cover in compliance with the PALM Input Data Standard (PIDS). Major extensions introduced since the previous description include the processing of georeferenced raster and vector data with automated reprojection, user-defined domain rotation and nesting, enhanced handling of building parameters, optimized generation of resolved vegetation, estimation of leaf area index from vegetation height, and the derivation of static input for non-building-resolving simulations based on Local Climate Zone classifications. We demonstrate the application of palm_csd using publicly available geodata for the city of Berlin (Germany), covering both building-resolving and LCZ-based simulation setups. Common data inconsistencies and sources of uncertainty in urban geodata are discussed. palm_csd 25.10 provides a reproducible, flexible and continuously maintained framework for transforming heterogeneous geospatial datasets into PALM-compatible static drivers to support both detailed urban morphology and coarser-scale urban climate applications.</p>]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-5515-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/5515/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd137787</identifier>
    <datestamp>2026-06-26</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Benchmarking ozone stress parameterizations in CLM5: a global mechanistic assessment of thresholds and memory effects]]></dc:title>
      <dc:creator>Zhou, Peng</dc:creator>
      <dc:creator>Chou, Jieming</dc:creator>
      <dc:creator>Dan, Li</dc:creator>
      <dc:creator>Lamarque, Jean-François</dc:creator>
      <dc:creator>Bilal, Muhammad</dc:creator>
      <dc:creator>Li, Fang</dc:creator>
      <dc:creator>Sun, Mengting</dc:creator>
      <dc:creator>Buchholz, Rebecca</dc:creator>
      <dc:creator>Murray, Desneiges</dc:creator>
      <dc:creator>Cao, Zhaoxiang</dc:creator>
      <dc:creator>Peng, Jing</dc:creator>
      <dc:creator>Li, Kai</dc:creator>
      <dc:creator>Yang, Fuqiang</dc:creator>
      <dc:creator>Pan, Wei</dc:creator>
      <dc:creator>Chen, Jinyan</dc:creator>
      <dc:creator>Xing, Liwen</dc:creator>
      <dc:description><![CDATA[<p>Tropospheric ozone remains a critical but uncertain driver of terrestrial productivity loss, and land surface models (LSMs) diverge markedly in how they represent vegetation ozone stress. We conduct a global, mechanistically consistent evaluation of three prominent ozone stress parameterization schemes, Sitch, Lombardozzi, and Li, within the Community Land Model version 5 (CLM5). Using unified meteorological and ozone forcing from CAM-chem and GSWP3.1, we designed five experiments to isolate the roles of ozone flux threshold selection and response function form. The mixed experiments using thresholds and response functions derived from the Sitch and Lombardozzi schemes were implemented without additional recalibration, allowing structural sensitivities to be evaluated consistently within the Li framework. Model output is benchmarked against MODIS and FLUXNET gross primary production (GPP) across spatial gradients, biomes, and among plant functional types (PFTs). All parameterizations capture the ozone–induced reduction in GPP relative to the ozone-free baseline, but their accuracy varies widely. The Li scheme, featuring PFT-specific thresholds and separate nonlinear responses for photosynthesis and stomatal conductance, best agrees with observed GPP patterns across scales. In contrast, the Lombardozzi scheme produces much larger reductions in high-flux regions. Analysis reveals that the structures of ozone response functions and memory-decay mechanisms primarily determine improvements in GPP simulation. Our results support a shift toward ozone parameterizations that couple stomatal flux with canopy phenology, dynamic water constraints, and regionally calibrated thresholds. These findings provide a transferable framework for quantifying ozone–carbon coupling in LSMs and highlight<span id="page5492"/> priorities for improving terrestrial biosphere models under atmospheric change.</p>]]></dc:description>
      <dc:date>2026-06-26</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-5491-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/5491/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:gh139012</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>gh</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[From destabilisation to disruption: deactivation network dynamics in an Italian fossil infrastructure conflict]]></dc:title>
      <dc:creator>Delatin Rodrigues, Daniel</dc:creator>
      <dc:creator>Calignano, Giuseppe</dc:creator>
      <dc:creator>Grasso, Marco</dc:creator>
      <dc:description><![CDATA[<p>This article introduces the deactivation network approach (DNA) to analyse conflicts in fossil fuel infrastructures as relational struggles between practices of continuity/legitimation and practices of destabilisation/disruption. The DNA is applied to Enel's power plants in Civitavecchia (Italy) across two contentious conversion cycles: an oil-to-coal project (2000–2010, realised) and a proposed coal-to-gas project (2018–2023, halted). Using an intentionally asymmetrical design, the study maps only the deactivation network and treats the fossil-support network as a structuring context shaping political opportunity structures. Event-based social network analysis, triangulated with interviews, documentary sources, and digital ethnography, compares changes in network composition, connectivity, and tie intensity across the two periods. Results show that mobilisation and activist cohesion alone did not produce disruption. Deactivation became effective when activists' destabilisation was brokered into institutional and labour arenas, enabling administrative and political interference with infrastructural continuity.</p>]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gh-81-347-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gh.copernicus.org/articles/81/347/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-8798</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd133360</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Global Ocean data set of marine aerosol properties]]></dc:title>
      <dc:creator>Quinn, Patricia K.</dc:creator>
      <dc:creator>Bates, Timothy S.</dc:creator>
      <dc:creator>Coffman, Derek J.</dc:creator>
      <dc:creator>Johnson, James E.</dc:creator>
      <dc:creator>Upchurch, Lucia M.</dc:creator>
      <dc:creator>Best, Hanna</dc:creator>
      <dc:description><![CDATA[<p>NOAA's Pacific Marine Environmental Laboratory (PMEL) has made measurements of aerosol chemical, microphysical, optical, and cloud nucleating properties onboard research cruises since 1991. The twenty-five cruises have covered all of the world's oceans – the Pacific, Atlantic, Indian, Arctic, and Southern. The result is the most comprehensive, publicly available database of aerosol properties in the marine atmosphere to date. The database also contains gas-phase species (<span class="inline-formula">O<sub>3</sub></span>, <span class="inline-formula">SO<sub>2</sub></span>), Radon, and dimethylsulfide (DMS), seawater species (DMS, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NH</mi><mn mathvariant="normal">4</mn><mo>+</mo></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="24pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="f83a9f1907f38a5589c34b239e10518b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="essd-18-4317-2026-ie00001.svg" width="24pt" height="15pt" src="essd-18-4317-2026-ie00001.png"/></svg:svg></span></span>, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="e16cba38499a6a16cb1a10e488ec56da"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="essd-18-4317-2026-ie00002.svg" width="25pt" height="16pt" src="essd-18-4317-2026-ie00002.png"/></svg:svg></span></span>, and chlorophyll <span class="inline-formula"><i>a</i></span>), and meteorological parameters. Details of the cruises (locations, dates, and objectives), parameters measured, instrumentation used, and data availability are provided here. Also included are PMEL's high-level major findings and past usage of the data by others. The goal of this paper is to promote broader awareness of the database to the atmospheric aerosol in situ measurement, satellite, and modelling communities. Data are publicly available at NOAA's National Centers for Environmental Information (NCEI) data archive (<span class="uri">https://www.ncei.noaa.gov/</span>, NOAA, 2025) (see also the list of all data sets in Table 7). Links to the Digital Object Identifiers (DOIs) for each cruise are provided herein.</p>]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-4317-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/4317/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd139584</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
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       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Flume experimental data for the study of morphological response of alpine gravel-bed rivers to flow and sediment forcing]]></dc:title>
      <dc:creator>Johannot, Adèle</dc:creator>
      <dc:creator>Recking, Alain</dc:creator>
      <dc:creator>Lopez, Arthur</dc:creator>
      <dc:creator>Bellot, Hervé</dc:creator>
      <dc:creator>Buffet, Alexis</dc:creator>
      <dc:creator>Fontaine, Firmin</dc:creator>
      <dc:creator>Bardot, Kylian</dc:creator>
      <dc:description><![CDATA[This paper presents a dataset derived from flume experiments designed to reproduce conditions typical of alpine gravel-bed streams. The experiments aim to investigate how different hydro-sedimentary forcings influence channel morphology. The flume setup is Froude-scaled based on measurements collected on a braided reach in the French Alps. Experimental runs represent daily flood peaks characteristic of the melting season, together with their associated sediment supply. The dataset includes several types of measurements: full-flume topography obtained by photogrammetry, bedload flux at the outlet measured with a force sensor, grain-size distribution of transported sediments, and flow surface velocities derived from a tracer method. Digital Elevation Models (DEMs) were generated from the photogrammetric surveys at multiple timesteps, with a spatial resolution of 0.7 mm/pixel and a mean vertical error of 1 mm. Bedload flux at the outlet can be estimated from the force sensor measurements, while the grain-size distribution of transported material was determined by sieving. For each run, the dataset includes a video of the run, DEMs of the bed at different timesteps, a video for flow velocities estimates, sediment flux and transported grain-size at the outlet, and the input liquid and solid discharges. This large dataset available at <a href="https://doi.org/10.57745/QM4ZOO" target="_blank" rel="noopener">https://doi.org/10.57745/QM4ZOO</a> comprises 115 DEMs, 35 videos for velocities estimates, 81 transported grain size distribution and videos for various input conditions. It offers strong potential for studying morphological processes at micro- to macro-scales and across various timescales, and a fabulous playground for numerical investigations.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-197</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-197/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd142510</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Coastal Atmosphere &amp; Sea Time Series (CoASTS) and Bio-Optical mapping of Marine optical Properties (BiOMaP): the hyperspectral absorption coefficients by optically significant constituents]]></dc:title>
      <dc:creator>Berthon, Jean-François</dc:creator>
      <dc:creator>Zibordi, Giuseppe</dc:creator>
      <dc:description><![CDATA[The <em>Coastal Atmosphere &amp; Sea Time Series</em> (CoASTS) and the <em>Bio-Optical mapping of Marine optical Properties</em> (BiOMaP) programs were conceived and implemented to assist ocean color applications with field measurements of apparent and inherent optical properties, and concentration of optically significant water constituents. The CoASTS program led to the creation of time-series of bio-optical measurements at the Acqua Alta Oceanographic Tower (AAOT) site the northern Adriatic Sea continued from 1995 up to 2016. The BiOMaP program supported the collection of equivalent bio-optical measurements across European Seas from 2000 up to 2022. This work focusses on CoASTS and BiOMaP hyperspectral absorption coefficients of optically significant constituents as determined applying standardized instruments, community measurement methods, extended quality control schemes and consolidated processing codes. The work, which complements a previous one by Zibordi and Berthon (2024) centred on multi-spectral data, presents the CoASTS and BiOMaP hyperspectral absorption coefficients of pigmented and non-pigmented particles in the 400&ndash;750 nm, and of colored dissolved organic matter in the 350&ndash;680 nm interval, both with a 3 nm spectral resolution at 2 nm increment.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-463</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-463/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd142280</identifier>
    <datestamp>2026-06-25</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[MacroTraits: a global trait data and information system for marine benthic ecology]]></dc:title>
      <dc:creator>Beauchard, Olivier</dc:creator>
      <dc:creator>Soetaert, Karline</dc:creator>
      <dc:description><![CDATA[For a long time, biological trait data have been a bottleneck in biodiversity research. Constraints of data unavailability and challenging analytical implementation are still obstacles to the investigation of functional biodiversity patterns. This is especially true in marine zoobenthic ecology where the use of biological traits became common much later than in terrestrial and freshwater ecology. Additionally, most of trait-based marine studies have dominantly been conducted in European waters while large gaps remain in other areas of the world. Therefore, this paper offers a framework to fill this gap by providing the most comprehensive zoobenthic trait data compilation at the global scale. Based on more than 8000 references, 1893 species of the marine macrozoobenthos are documented for life history, dwelling mode, ecosystem function, habitat and biogeography through 41 traits. Next to this compilation, the paper brings clarifications on research directions by means of these data within the dominant paradigms of modern ecology. In particular, the dichotomous expressiveness that opposes response to effect traits (i.e., fitness components versus ecosystem function) is emphasised. The data base is accessible through an R package in the repository <a href="https://doi.org/10.5281/zenodo.20555888" target="_blank" rel="noopener">https://doi.org/10.5281/zenodo.20555888</a> and that facilitates data treatment such as trait selection, cross table construction and label handling.]]></dc:description>
      <dc:date>2026-06-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-444</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-444/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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