<?xml version="1.0" encoding="UTF-8"?>
<?xml-stylesheet type='text/xsl' href='/oai.xsl' ?>
<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/"
         xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
         xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/
         http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd">
<responseDate>2026-05-15T08:05:44Z</responseDate>
<request metadataPrefix="oai_dc" verb="ListRecords">http://oai-pmh.copernicus.org/oai.php</request>
 <ListRecords>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:wesd140740</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>wesd</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 generalised Gaussian wake model based on extended actuator disc theory]]></dc:title>
      <dc:creator>Fei, Zheni</dc:creator>
      <dc:creator>Nishino, Takafumi</dc:creator>
      <dc:creator>Vogel, Christopher R.</dc:creator>
      <dc:description><![CDATA[As both the turbine and the wind farm sizes grow, the local blockage effect and the robustness of the wake model become increasingly important for wind farm design. One of the main challenges that affects the generality of conventional wake models is to find the start of the far wake region where the velocity field can be assumed to be self-similar. This work derives a wake model based on the actuator disc theory that considers the local blockage effect by considering the global mass conservation and predicts the start of the far wake with a mathematical condition. We define that the far wake starts around the point where the divergence of the Reynolds shear stresses is equal to its streamwise integration. The model is validated against a series of Reynolds-averaged Navier-Stokes (RANS) simulations. The proposed condition for the start of far wake applies to a wide range of turbine thrust coefficients, blockage ratios and inflow turbulence intensities, except for low turbulence intensity around 1 % for the cases examined in this study. The velocity increase induced by the blockage effect becomes non-negligible at 5 % for the examined cases, which can be lower than that induced by the real atmosphere. Thus, the blockage effect should be considered in the wake modelling for large turbines.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/wes-2026-76</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/preprints/wes-2026-76/]]></dc:identifier>
      <dc:source>eISSN: 2366-7451</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:wes136536</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>wes</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[Design and simulation of a continuously variable hydraulic power-split drivetrain for wind turbines]]></dc:title>
      <dc:creator>Seifermann, Pascal</dc:creator>
      <dc:creator>Schaaf, Jonathan</dc:creator>
      <dc:creator>Störtenbecker, Sven</dc:creator>
      <dc:creator>Dam, Alexander</dc:creator>
      <dc:creator>Dalhoff, Peter</dc:creator>
      <dc:description><![CDATA[<p>This paper presents the development and analysis of a novel drivetrain concept for large-scale wind turbines. The proposed concept builds on a predominantly mechanical transmission, with a small fraction of power transferred by a hydraulic system. The hydraulic power path, an adjustable hydrostatic transmission with a pump and a motor, enables full rotational speed variability while transmitting only a limited portion of the total power. As a result, a higher overall efficiency can be achieved compared to fully hydrostatic drivetrains. Furthermore, it is possible to couple the generator directly to the grid, thus omitting the frequency converter which contributes to system complexity, losses, and failure susceptibility.</p>        <p>A simulation model incorporating component-level loss representations is developed to evaluate different transmission layouts and design variants. It is investigated whether a hydromechanical power-split drivetrain can achieve efficiency and energy yield levels comparable to conventional geared drivetrains while referring to the characteristics of currently available hydraulic components.</p>        <p>The results show that the drivetrain efficiency strongly depends on the transmission layout and the site-specific wind conditions. While lower efficiencies are observed for sites with low mean annual wind speeds, specific design configurations achieve high efficiencies and energy yields comparable to those of a conventional geared reference drivetrain at sites with higher mean annual wind speeds. Overall, this paper extends previous research by minimizing the rated power of the hydraulic power path, estimating efficiencies for different drivetrain configurations, and looking into a mechanical design.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/wes-11-1733-2026</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/articles/11/1733/2026/]]></dc:identifier>
      <dc:source>eISSN: 2366-7451</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:os137510</identifier>
    <datestamp>2026-05-13</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[Determination of the height of deep-sea mooring lines above seafloor using turbulence measurements]]></dc:title>
      <dc:creator>Haren, Hans</dc:creator>
      <dc:description><![CDATA[<p>Height variations O(1) m of closely spaced moored oceanographic instrumentation are difficult to measure in the deep sea, requiring high-accuracy pressure sensors preferably on all instruments in a mooring-array. In this paper, an alternative method for relative height determination is presented using 2 m spaced high-resolution temperature sensors moored on multiple 9.5 m-spaced lines in the deep Western Mediterranean Sea. While it was anticipated that height variations between lines could be detected under near-homogeneous conditions via adiabatic lapse rate O(10<span class="inline-formula"><sup>−4</sup></span> °C m<span class="inline-formula"><sup>−1</sup></span>) by the 3 <span class="inline-formula">×</span> 10<span class="inline-formula"><sup>−5</sup></span> °C-noise-level sensors, such was prevented by the impossibility of properly correcting for short-term bias due to electronic drift. Instead, a satisfactory height determination was achieved during a period of relatively strong stratification and large turbulence activity. By band-pass filtering data of the highest-resolved turbulent motions across the strongest temperature gradient, significant height variations were detectable to within <span class="inline-formula">±</span>0.2 m.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-1501-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/1501/2026/]]></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:os135992</identifier>
    <datestamp>2026-05-13</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[High-latitude eddy statistics from SWOT  compared with in situ observations]]></dc:title>
      <dc:creator>Marez, Charly</dc:creator>
      <dc:creator>Bendinger, Arne</dc:creator>
      <dc:creator>Dilmahamod, Ahmad Fehmi</dc:creator>
      <dc:description><![CDATA[<p>Mesoscale eddies play a key role in the transport of heat, salt, and momentum in the ocean, yet their statistical characterization at high latitudes has remained elusive due to the coarse resolution of conventional satellite altimetry. Here we present a statistical description of the mesoscale eddies in the Labrador Sea at an unprecedented resolution, using observations from the Surface Water and Ocean Topography (SWOT) mission, significantly extending previous estimates derived from lower-resolution altimetry products. We apply an eddy-detection algorithm directly to the native 2 km SWOT swaths, without gridding or assimilation, and validate the detections against in situ measurements from shipboard current profiler data from one cruise in 2024, as well as against a statistically derived shipboard current-profiler-based eddy census. The comparison demonstrates good agreement in eddy size and intensity, confirming SWOT's ability to resolve high-latitude mesoscale structures previously undetectable or distorted in gridded altimetry. The SWOT-derived eddy census based on two full calendar years reveals a predominance of energetic anticyclones (Irminger Rings) in the basin interior and smaller cyclones along the continental slopes, with clear seasonal variability linked to boundary current instability. These findings provide the first observational benchmark for mesoscale activity in the Labrador Sea and illustrate SWOT’s potential to extend eddy statistics to high-latitude and ice-influenced regions, opening the way for a global assessment of mesoscale variability.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-1515-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/1515/2026/]]></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:nhess134286</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>nhess</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[Monitoring diffuse volcanic degassing with seismic ambient noise]]></dc:title>
      <dc:creator>Seivane, Helena</dc:creator>
      <dc:creator>Schimmel, Martin</dc:creator>
      <dc:description><![CDATA[<p>Diffuse volcanic degassing is a persistent and often underestimated natural hazard, with potential impacts on air quality, ecosystem health, and volcanic risk management. Detecting and monitoring this process is challenging, especially in volcanoes lacking visible fumarolic activity, where the final stage of gas migration is jointly modulated by the shallow subsurface structure and natural pressure forcings.  We present a continuous monitoring approach based on Rayleigh wave ellipticity from ambient seismic noise to track pressure-driven gas transport in the uppermost soil layers. Applied to Cumbre Vieja Volcano (La Palma, Canary Islands), the method detects subdaily seismic velocity variations linked to periodic pressure oscillations, consistent with natural forcings such as atmospheric and solid earth tides. In this work, we focus on the terdiurnal cycle, the only subdaily band at La Palma Island that reflects purely atmospheric pressure forcing. Its temporal evolution reveals long-term fluctuations that broadly coincide with reported <span class="inline-formula">CO<sub>2</sub></span> emission trends, despite differences in spatial and temporal resolution between both estimates. In addition, we identify a clear semiannual cycle in the long-term ellipticity response at the terdiurnal frequency. This seasonality coincides with the modulation by solid Earth tides and confirms their role in controlling permeability in the upper vadose zone and in the enhancement of barometric pumping efficiency across all stations analyzed. Prior to the 2021 eruption, the terdiurnal cycle reveals contrasting station responses, with TBT exhibiting the earliest and most sustained increase. Together, these observations point to the usefulness of this approach as a complementary tool in the assessment of diffuse degassing and volcanic unrest. This seismic-noise-based approach offers a cost-effective and resilient strategy for detecting hazardous gas migration, supporting early warning and mitigation efforts in volcanic regions.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-2249-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/2249/2026/]]></dc:identifier>
      <dc:source>eISSN: 1684-9981</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:nhess128861</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>nhess</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[Seismo-acoustic and GNSS observations of a record-breaking  Black Sea storm: repurposing geophysical sensors for  environmental monitoring]]></dc:title>
      <dc:creator>Petrescu, Laura</dc:creator>
      <dc:creator>Antonescu, Bogdan</dc:creator>
      <dc:creator>Nistor, Sorin</dc:creator>
      <dc:creator>Floroiu, Iustin</dc:creator>
      <dc:creator>Ene, Dragoş</dc:creator>
      <dc:creator>Ghica, Daniela</dc:creator>
      <dc:creator>Ionescu, Constantin</dc:creator>
      <dc:creator>Anghel, Andrei</dc:creator>
      <dc:creator>Datcu, Mihai</dc:creator>
      <dc:description><![CDATA[<p>In August 2024, a devastating storm struck Romania's Black Sea coast, setting new precipitation records and marking an unusual change relative to historical climate observations. To investigate this extraordinary event, we integrated non-conventional sensors (seismic, GNSS, infrasound, and satellite data) with ERA5 meteorological reanalysis to monitor storm dynamics. High-frequency (<span class="inline-formula">&gt;30</span> Hz) seismic signals captured precipitation, while microseismic bands (0.1–1 Hz) reflected wave-induced ground motion. Analysis of infrasound data via unsupervised learning delineated periods of acoustic quiescence from storm-related activity. The temporal evolution of these infrasound states coincided with distinct patterns in seismic ground motion, suggesting a shared origin in the storm's atmospheric dynamics. The infrasound array also detected over 1100 signals in the 0.6–7 Hz band, matching lightning discharges observed by geostationary satellites. GNSS data recorded a buildup of precipitable water vapor that peaked concurrently with intense rainfall, following a multi-day increase that preceded the main storm phase. This study highlights the value of integrating diverse, non-traditional datasets to enhance the resolution and depth of storm analysis. Their combined use offers a more holistic understanding of storm evolution and supports future research on the potential role of multi-sensor observations in improving early-warning systems in vulnerable coastal regions.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-2227-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/2227/2026/]]></dc:identifier>
      <dc:source>eISSN: 1684-9981</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:jm137420</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>jm</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[Palynofacies and lacustrine sequence stratigraphy:  a case example from the Jurassic Cañadón Asfalto Formation, Cañadón Asfalto Basin,  Extra-Andean Patagonia, Argentina]]></dc:title>
      <dc:creator>Olivera, Daniela Elizabeth</dc:creator>
      <dc:creator>Zavala, Carlos</dc:creator>
      <dc:creator>Quattrocchio, Mirta Elena</dc:creator>
      <dc:creator>Soreda, María Eugenia</dc:creator>
      <dc:creator>Scasso, Roberto</dc:creator>
      <dc:creator>Yang, Renchao</dc:creator>
      <dc:description><![CDATA[<p>This study presents a detailed palynofacies analysis integrated with lacustrine sequence stratigraphy to evaluate the role of climate-driven hydrological balance on basin infill and its impact on the organic matter accumulation in the Jurassic Cañadón Asfalto Formation, Cerro Cóndor depocentre, Extra-Andean Patagonia, Argentina. It provides valuable insights into the changes in the nature and taphonomic history of the organic matter throughout the different stages of a lacustrine system's evolution based on the analysis of 51 outcrop samples from the Cañadón Lahuincó “A” section. Two depositional sequences are recognised. Sequence I documents the evolution from underfilled to balanced-fill/overfilled lake stages. Underfilled conditions are characterised by extreme lake-level variability, while the transition to balanced-fill/overfilled conditions is marked by stacked coarsening-upward successions. Sequence II is bounded by an abrupt accommodation increase and initially records renewed underfilled conditions, followed by the establishment of a fully overfilled lake stage characterised by persistent progradational stacking patterns. The most conspicuous feature of the Cañadón Asfalto Formation's organic matter is the overall dominance of land-derived fraction. The variations between the allochthonous and autochthonous (algae and algal-derived amorphous organic matter) material suggests variable climatic conditions, with the alternation of wetter and drier periods at least during the Sequence I and part of the Sequence II. Four palynofacies types (PT-A to PT-D) were defined recording variations in depositional energy, redox conditions, and sediment–water balance. PT-A and PT-D indicate wetter periods, while PT-B indicates relatively drier intervals. PT-C shows the changes between these two opposite situations. The underfilled stage is characterised by the dominance of reworked terrestrial phytoclasts (indicating high-energy inflow events) and poor sporomorph preservation. Conversely, the balanced-fill stage shows sporomorph-rich palynofacies. In both lake stages, blooms of well-preserved strong fluorescence <i>Botryococcus</i> colonies (chlorophytic algae) are registered during drier periods. The overfilled conditions are characterised by the lack of palynomorphs. Kerogen<span id="page336"/> varies from Type III (PT-A) to mixed Type I/III in algae-rich intervals (PT-B, PTC), confirming hydrological balance as the control on organic matter preservation.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/jm-45-335-2026</dc:identifier>
      <dc:identifier><![CDATA[https://jm.copernicus.org/articles/45/335/2026/]]></dc:identifier>
      <dc:source>eISSN: 2041-4978</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:soil133858</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>soil</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[Estimating soil carbon sequestration potential with mid-IR spectroscopy and explainable machine learning]]></dc:title>
      <dc:creator>Hu, Yang</dc:creator>
      <dc:creator>Viscarra Rossel, Raphael A.</dc:creator>
      <dc:description><![CDATA[<p>Soil carbon sequestration refers to the process of capturing atmospheric carbon through plant photosynthesis and storing it in soil as organic carbon. The primary mechanism for carbon sequestration is the adsorption of organic carbon molecules onto the mineral surfaces of the soil's fine fraction (clay <span class="inline-formula">+</span> silt <span class="inline-formula">≤</span> 20 <span class="inline-formula">µ</span>m), forming mineral-associated organic carbon (MAOC). Soil has a finite capacity to stabilise and sequester organic carbon, known as carbon saturation capacity, which depends on the proportion of reactive minerals in the soil. The difference between the current MAOC content and the carbon saturation capacity is referred to as the organic carbon saturation deficit (<span class="inline-formula"><i>C</i><sub>def</sub></span>) or sequestration potential. Fourier-transformed (FTIR) mid-infrared (mid-IR) spectroscopy can simultaneously measure soil properties relevant to carbon stabilisation: organic carbon functional groups, clay and iron-oxide mineralogy and particle size. Therefore, we hypothesise that mid-IR spectroscopy can effectively and accurately estimate <span class="inline-formula"><i>C</i><sub>def</sub></span>. Here, we aim to (i) develop spectroscopic models to estimate the MAOC and <span class="inline-formula"><i>C</i><sub>def</sub></span> of 482 Australian topsoil samples, (ii) model MAOC and <span class="inline-formula"><i>C</i><sub>def</sub></span> using mid-IR spectra and an interpretable machine learning  algorithm, and (iii) further interpret the MAOC and <span class="inline-formula"><i>C</i><sub>def</sub></span> models using SHapley Additive exPlanations (SHAP). Using frontier line analysis, we fitted a function to the upper envelope of the MAOC vs. clay <span class="inline-formula">+</span> silt relationship to derive <span class="inline-formula"><i>C</i><sub>def</sub></span>. We recorded mid-IR spectra of the samples and used the regression trees method CUBIST to model MAOC content and <span class="inline-formula"><i>C</i><sub>def</sub></span>. We interpreted these models by examining the regression trees and using SHAP. The models were unbiased and estimated MAOC content with <span class="inline-formula"><i>R</i><sup>2</sup></span> of 0.86 and RMSE of 2.77 (g kg soil<span class="inline-formula"><sup>−1</sup></span>), and <span class="inline-formula"><i>C</i><sub>def</sub></span> with <span class="inline-formula"><i>R</i><sup>2</sup></span> of 0.89 and RMSE of 3.72 (g kg soil<span class="inline-formula"><sup>−1</sup></span>). Model interpretation showed that <span class="inline-formula"><i>C</i><sub>def</sub></span> estimates relied on negative interactions with absorptions from organic matter functional groups and positive interactions with absorptions from clay minerals. Our results demonstrate that mid-IR spectra can effectively estimate MAOC and soil <span class="inline-formula"><i>C</i><sub>def</sub></span>, providing a rapid, cost-effective method for assessing and monitoring this critical soil function.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/soil-12-619-2026</dc:identifier>
      <dc:identifier><![CDATA[https://soil.copernicus.org/articles/12/619/2026/]]></dc:identifier>
      <dc:source>eISSN: 2199-398X</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:hess134994</identifier>
    <datestamp>2026-05-13</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[From soil to stream: modeling the catchment-scale hydrological effects of increased soil organic carbon]]></dc:title>
      <dc:creator>Heinz, Malve</dc:creator>
      <dc:creator>Holzkämper, Annelie</dc:creator>
      <dc:creator>Kumar, Rohini</dc:creator>
      <dc:creator>Ledain, Sélène</dc:creator>
      <dc:creator>Horton, Pascal</dc:creator>
      <dc:creator>Schaefli, Bettina</dc:creator>
      <dc:description><![CDATA[<p>Droughts are increasingly threatening agricultural productivity. One potential adaptation is to increase the soil water retention capacity, which can be achieved by increasing soil organic carbon (SOC) through agricultural management. We investigated how increasing SOC affected catchment-scale hydrology including extremes. SOC increases were implemented via adjustments to soil hydraulic parameters (<span class="inline-formula"><i>ρ</i><sub>b</sub></span>, <span class="inline-formula"><i>θ</i><sub>PWP</sub></span>, <span class="inline-formula"><i>θ</i><sub>FC</sub></span>, <span class="inline-formula"><i>θ</i><sub>Sat</sub></span>, <span class="inline-formula"><i>K</i><sub>sat</sub></span>) in a mesoscale hydrologic modeling (mHM) framework, following literature-reported effects. Our analysis focuses on the medium-sized, agriculturally dominated Broye catchment in Western Switzerland and four nested subcatchments, where we evaluated five SOC increase scenarios of varying depth and magnitude. At the catchment scale, increment of SOC resulted in higher soil water content (1.43 %–3.75 %) and slightly higher evapotranspiration (0.15 %–0.38 %), while subsurface runoff was reduced (0.27 %–0.70 % across all scenarios). These values represent overall net changes over 2016–2022; while at shorter timescales, the magnitude and even direction of effects varied seasonally and by subcatchment. Increased water retention meant more soil water was available for evapotranspiration and less for groundwater recharge and streamflow. Consequently, streamflows were slightly reduced, peak flows modestly attenuated while low flow responses depended on catchment characteristics and timing. In warmer and drier subcatchments, low flow frequency increased in some years, whereas in cooler and wetter subcatchments, conditions in spring and early summer produced a beneficial effect, slightly reducing low flow frequency. Overall, our analysis suggests that large-scale increases in SOC can provide hydrological benefits such as enhanced agricultural productivity and reduced peak flows, but may involve trade-offs through reduced groundwater recharge and thus water availability.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-2879-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/2879/2026/]]></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:gmd132321</identifier>
    <datestamp>2026-05-13</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[SWEpy: an open-source GPU-accelerated solver for near-field inundation and far-field tsunami modeling]]></dc:title>
      <dc:creator>Fuenzalida, Juan</dc:creator>
      <dc:creator>Kusanovic, Danilo</dc:creator>
      <dc:creator>Meza, Joaquín</dc:creator>
      <dc:creator>Meneses, Rodrigo</dc:creator>
      <dc:creator>Catalán, Patricio A.</dc:creator>
      <dc:description><![CDATA[<p>We present <code>SWEpy</code>, an open-source Python finite volume (FV) software for solving the shallow water equations (SWEs) on unstructured triangular meshes. The framework combines flexibility and high performance through GPU acceleration and a well-balanced, positivity-preserving, higher-order central-upwind (CU) scheme. These features are required for simulation of hydrodynamic phenomena such as tsunami propagation, flooding, and dam-break flows in complex and large geometries.</p>        <p>To reduce numerical diffusion, a phenomenon commonly encountered in FV methods, <code>SWEpy</code> incorporates a second-order WENO reconstruction together with a third-order strong stability-preserving Runge–Kutta time integration scheme. These numerical components are particularly well-suited for far-field tsunami modeling, where minimizing artificial diffusion is essential to accurately preserve wave amplitude, phase, and dispersion over long propagation distances.</p>        <p>The performance, stability, and accuracy of <code>SWEpy</code> are validated using canonical benchmarks, including Synolakis’ conical island and Bryson’s flow over a Gaussian bump. Its capabilities are further demonstrated through large-scale simulations of the 1959 Malpasset Dam failure and the 2010 Maule tsunami, highlighting its effectiveness in realistic scenarios. Overall, these results show that <code>SWEpy</code> framework delivers high-resolution solutions on consumer-grade hardware, providing a user-friendly and computationally efficient platform for both research applications and operational forecasting.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-3953-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/3953/2026/]]></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:gmd132768</identifier>
    <datestamp>2026-05-13</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[Two-tier MOM6 regional modelling suite of the East Australian Current system]]></dc:title>
      <dc:creator>Reilly, John A.</dc:creator>
      <dc:creator>Chapman, Christopher C.</dc:creator>
      <dc:creator>Quinn, Courtney</dc:creator>
      <dc:creator>Kajtar, Jules B.</dc:creator>
      <dc:creator>Barnes, Ashley J.</dc:creator>
      <dc:creator>Holbrook, Neil J.</dc:creator>
      <dc:description><![CDATA[<p>We present a new ultra-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">30</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="27pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="dc49814963aca0c62140aa9a3b56a981"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gmd-19-3853-2026-ie00001.svg" width="27pt" height="14pt" src="gmd-19-3853-2026-ie00001.png"/></svg:svg></span></span>° (<span class="inline-formula">∼</span> 3 km) regional ocean model of the eastern Australian region and evaluate the performance of this model against two <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">10</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="27pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="12db55596f36ad3d61d5560c9bad12c7"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gmd-19-3853-2026-ie00002.svg" width="27pt" height="14pt" src="gmd-19-3853-2026-ie00002.png"/></svg:svg></span></span>° (<span class="inline-formula">∼</span> 10 km) models as well as a suite of satellite and in situ observations. We evaluate model biases in the context of (i) submesoscale-permitting (<span class="inline-formula">∼</span> 3 km) vs. mesoscale-permitting (<span class="inline-formula">∼</span> 10 km) horizontal resolution and (ii) differences between version 5 and version 6 of the Modular Ocean Model (MOM5 vs. MOM6) to assess the added value in each case and determine the suitability of our higher resolution model for scientific research. There are some consistent biases shared by the two regional MOM6 configurations, and also in the higher resolution configuration that are not seen in the lower resolution models. These biases are further investigated with two sets of sensitivity experiments to understand the effect of submesoscale eddy parameterization and imposed dynamic viscosity at a submesoscale-permitting resolution. The high-resolution simulation has much higher variance compared to the lower resolution simulations across all evaluation metrics, indicating that the greater spectrum of length scales also manifests in more variability in the temporal domain. The two MOM6 regional configurations of differing resolution appear to be more aligned than the regional (MOM6) and global (MOM5) <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">10</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="27pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="50cc10563f4975718db6fa900ec33e58"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gmd-19-3853-2026-ie00003.svg" width="27pt" height="14pt" src="gmd-19-3853-2026-ie00003.png"/></svg:svg></span></span>° configurations in most results, reflecting the substantial changes made to the MOM between version 5 and version 6. Importantly, we also show that higher resolution is not a panacea: in regions where key dynamics are quasi-linear and well-captured captured by coarser grids (e.g., the EAC jet), further refinement may offer limited benefit – and actually degrade the performance if parameterizations are not appropriately tuned.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-3853-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/3853/2026/]]></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:gmd131564</identifier>
    <datestamp>2026-05-13</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[darcyInterTransportFoam v1.0: an open-source, fully-coupled 3D solver for simulating surface water – saturated groundwater processes and exchanges]]></dc:title>
      <dc:creator>Pardo-Álvarez, Álvaro</dc:creator>
      <dc:creator>Fleckenstein, Jan H.</dc:creator>
      <dc:creator>Koutantou, Kalliopi</dc:creator>
      <dc:creator>Brunner, Philip</dc:creator>
      <dc:description><![CDATA[<p>Fully-coupled solvers have proven to be suitable and computationally efficient tools for studying surface water–groundwater (SW-GW) interactions. Most existing fully-coupled codes use the two-dimensional, depth-averaged shallow water equations for surface flows. As a result, three-dimensional (3D) flow dynamics are ignored in the surface domain, including phenomena important for the SW-GW exchange such as turbulence. Computational Fluid Dynamics (CFD) solvers allow to capture 3D information on the surface turbulent flow by solving the full Navier-Stokes equations. Consequently, they are well-suited for the study of the actual exchange flows of water and solutes across the sediment-water interface. Among the available CFD software, the open-source toolbox OpenFOAM provides a flexible modelling framework to implement user-defined, fully-coupled models for the detailed investigation of SW-GW interaction processes. Based on this CFD platform, Lee et al. (2021) developed hyporheicScalarInterFoam, a fully-coupled 3D solver capable of solving the flow and transport processes in both surface and subsurface domains as well as the interactions across their interface. Despite the potential of this new code to tackle SW-GW interactions, its application to real-world hydrogeological scenarios is constrained by limitations in boundary conditions, parameter heterogeneity and key hydrodynamic and transport processes, among others, which hinder the accurate representation of the complex characteristics of natural systems. To overcome this, an updated and extended version of hyporheicScalarInterFoam, called darcyInterTransportFoam, is presented in this paper. The new fully-coupled solver enhances the applicability of the original by introducing novel simulation features. These include internal solver updates, such as the definition of heterogeneous and anisotropic subsurface fields and the simulation of heat transfer in both domains, as well as newly implemented add-ons, including pre- and post-processing utilities and additional boundary conditions. A complete description of all the new features is provided in this paper. Moreover, the utility of darcyInterTransportFoam is demonstrated in a test case, where the SW-GW flow, solute transport and heat transfer processes are simulated in a highly conductive river-aquifer system.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-3923-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/3923/2026/]]></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:gmd127354</identifier>
    <datestamp>2026-05-13</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[psit 1.0: a system to compress Lagrangian flows]]></dc:title>
      <dc:creator>Pietak, Alexander</dc:creator>
      <dc:creator>Huang, Langwen</dc:creator>
      <dc:creator>Fusco, Luigi</dc:creator>
      <dc:creator>Sprenger, Michael</dc:creator>
      <dc:creator>Schemm, Sebastian</dc:creator>
      <dc:creator>Hoefler, Torsten</dc:creator>
      <dc:description><![CDATA[<p>Meteorological simulations produce large amounts of data, which can represent a challenge when trying to store, share, and analyze it. As weather and climate models increasingly simulate the atmosphere at higher spatio-temporal resolution, it becomes imperative to compress the data effectively. While compression algorithms exist for weather data stored in a gridded Eulerian frame, there are, to date, no specialized alternatives for data stored in the Lagrangian frame. In this study, we present psit, a system to compress weather data stored in the Lagrangian frame. The system works by mapping the trajectories to a grid structure, performing additional encodings on these, and passing them to either the JPEG 2000 image compression algorithm or SZ3. The specialty of the algorithm is the mapping phase and the following encodings, which generate the grids in a way that allows the aforementioned compression algorithms to perform well. To gauge the performance of psit, we test a variety of metrics. We demonstrate that in the majority of cases, equivalent or superior compression performance is attained through the utilization of psit as opposed to naive compression with ZFP or SZ3. We also compare compression with measurement inaccuracies. Here, we show that the density of <span class="inline-formula">168</span> hour long trajectories compressed with a ratio in the range of <span class="inline-formula">30</span> to <span class="inline-formula">40</span> behaves similarly to trajectories calculated from uncompressed wind fields with additional random perturbations with magnitude of <span class="inline-formula">0.1</span> m s<span class="inline-formula"><sup>−1</sup></span> in the horizontal and around <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">6</mn><mo>×</mo><msup><mn mathvariant="normal">10</mn><mrow><mo>-</mo><mn mathvariant="normal">3</mn></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="42pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="80811ea2898db14d9b4474c3d81fc171"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gmd-19-3893-2026-ie00001.svg" width="42pt" height="14pt" src="gmd-19-3893-2026-ie00001.png"/></svg:svg></span></span> Pa s<span class="inline-formula"><sup>−1</sup></span> in the vertical component. Additionally, we conduct two case studies in which we discuss the impact of compression on the study of warm conveyor belts associated with extratropical cyclones and the impact of compression on the radioactive plume prediction of the Fukushima incident in 2011.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-3893-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/3893/2026/]]></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:essdd141086</identifier>
    <datestamp>2026-05-13</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[Daily Global Sea Surface Ageostrophic Current Dataset from 1993&ndash;2023 via Physics-Informed Deep Learning]]></dc:title>
      <dc:creator>Cui, Guangxi</dc:creator>
      <dc:creator>Yuen, Ka-Veng</dc:creator>
      <dc:creator>Chen, Ying</dc:creator>
      <dc:creator>Liu, Zhiqiang</dc:creator>
      <dc:creator>Yang, Dingqi</dc:creator>
      <dc:creator>Liu, Guangliang</dc:creator>
      <dc:creator>Cai, Zhongya</dc:creator>
      <dc:description><![CDATA[Surface ocean circulation shapes climate, air-sea exchange, and the transport of heat, carbon, and other tracers, yet most long-term satellite-based global datasets rely primarily on geostrophic balance and therefore miss important ageostrophic motions. Here, we reconstruct global daily sea surface circulation at 0.25&deg; resolution from 1993 to 2023 using a physics-informed deep learning framework that integrates satellite altimetry with momentum constraints from geostrophic balance, wind stress, and nonlinear advection. The resulting dataset is dynamically consistent, with a mean momentum-balance error below 1.5 %, and reduces the median velocity error against independent mooring observations to 0.07 m s⁻&sup1;, compared with 0.20 m s⁻&sup1; for geostrophic currents and 0.10 m s⁻&sup1; for Ekman-corrected currents. We show that geostrophic flow sets the large-scale circulation, whereas Ekman and nonlinear contributions are smaller but comparable in magnitude to each other. Although nonlinear advection contributes little to relative vorticity, it strongly shapes surface divergence and the fine-scale structure of eddy kinetic energy. Our results show that nonlinear ageostrophic flow is an essential component of global surface circulation and that neglecting it limits our ability to resolve surface transport and variability on climatically relevant scales.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-341</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-341/]]></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:essdd139884</identifier>
    <datestamp>2026-05-13</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[PROMICE: Greenland ice velocity maps v2026]]></dc:title>
      <dc:creator>Solgaard, Anne</dc:creator>
      <dc:creator>Kusk, Anders</dc:creator>
      <dc:creator>Merryman Boncori, John Peter</dc:creator>
      <dc:creator>Dall, Jørgen</dc:creator>
      <dc:creator>Ahlstrøm, Andreas P.</dc:creator>
      <dc:creator>Andersen, Signe B.</dc:creator>
      <dc:creator>Citterio, Michele</dc:creator>
      <dc:creator>How, Penelope</dc:creator>
      <dc:creator>Karlsson, Nanna B.</dc:creator>
      <dc:creator>Kjeldsen, Kristian K.</dc:creator>
      <dc:creator>Larsen, Signe H.</dc:creator>
      <dc:creator>Lund, Mads C.</dc:creator>
      <dc:creator>Løkkegaard, Anja</dc:creator>
      <dc:creator>Lüthi, Martin P.</dc:creator>
      <dc:creator>Mejia, Jessica</dc:creator>
      <dc:creator>Mankoff, Kenneth D.</dc:creator>
      <dc:creator>As, Dirk</dc:creator>
      <dc:creator>Sugiyama, Shin</dc:creator>
      <dc:creator>Fausto, Robert S.</dc:creator>
      <dc:description><![CDATA[We present an updated version of the Programme for Monitoring of the Greenland Ice Sheet (PROMICE) ice velocity product (<a href="https://doi.org/10.22008/FK2/K70OPK" target="_blank" rel="noopener">https://doi.org/10.22008/FK2/K70OPK</a>; Solgaard and Kusk (2026)), providing a continuous time series of Greenland Ice Sheet velocity mosaics from January 2016 to the present. The product is derived from Sentinel-1 synthetic aperture radar (SAR) data, gridded at 200 m spatial resolution and updated every 12 days using data spanning two consecutive Sentinel-1 repeat cycles (24 days). Data are typically released within 10 days of the final acquisition and include all valid 6- and 12-day image pairs within the 24-day window.</p> <p>This update includes several important improvements to the processing chain. The spatial resolution has been refined from 500 m to 200 m, justified by the implementation of an adaptive correlation template size approach for offset tracking, improving velocity retrievals and enhancing delineation of narrow outlet glaciers. We further implement a new mosaicking strategy, which reduces noise associated with ionospheric disturbances. Additional improvements include enhanced error handling and outlier rejection. The full processing workflow is described, including data selection, mosaicking, uncertainty estimation, and filtering procedures.</p> <p>Validation against in-situ GNSS measurements over the full time series shows that the standard deviation of the differences between satellite- and GNSS-derived velocities (with corresponding bias) is 22 m/yr (-0.3 m/yr) and 38 m/yr (-0.4 m/yr) for the easting and northing components, respectively. These values fall within expected ranges, although a substantial fraction of the discrepancy likely reflects uncertainty in the GNSS measurements. This interpretation is supported by validation over stable terrain, where substantially lower values are obtained: 9 m/yr (0.1 m/yr) and 15 m/yr (-0.1 m/yr) for the easting and northing components, respectively. Compared to the previous product version, uncertainties are higher due to a prolonged period when only one Sentinel-1 satellite was operational, resulting in increased noise and reduced temporal sampling. We quantify the impact of these conditions on spatial coverage.</p> <p>Overall, coverage is highest during winter, when radar coherence is strong and acquisitions are most comprehensive, whereas summer coverage is reduced due to surface melt. Despite these seasonal and mission-related constraints, the PROMICE ice velocity product provides consistent temporal sampling and broad spatial coverage, supporting investigations of ice-sheet-wide and glacier-specific dynamics and ice discharge on seasonal to multi-year timescales.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-221</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-221/]]></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:essdd138438</identifier>
    <datestamp>2026-05-13</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[A Comprehensive Global Aquatic N2O Emission Database (GANED): Unravelling N2O Emission Patterns from Different Water Bodies]]></dc:title>
      <dc:creator>Nazir, Muhammad Junaid</dc:creator>
      <dc:creator>Yu, Longfei</dc:creator>
      <dc:creator>Zhang, Yunjie</dc:creator>
      <dc:creator>Zou, Jing</dc:creator>
      <dc:creator>Yuan, Wenping</dc:creator>
      <dc:creator>Wei, Jing</dc:creator>
      <dc:description><![CDATA[Nitrous oxide (N<sub>2</sub>O) is not only one of the main potent greenhouse gases, but also currently the dominant ozone-depleting substance. The quantification of N<sub>2</sub>O emissions from aquatic ecosystems, despite their global importance, is hindered by fragmented observations, inconsistent data reporting, and pronounced spatiotemporal variability. In this study, to improve accessibility, we introduce the Global Aquatic N<sub>2</sub>O Emission Database (GANED; <a href="https://doi.org/10.6073/pasta/4a086e49a4f308679b951293b380e7b9" target="_blank" rel="noopener">https://doi.org/10.6073/pasta/4a086e49a4f308679b951293b380e7b9</a>, Nazir et al., 2026), a consolidated dataset comprising 5130 N<sub>2</sub>O concentration records and 7386 N<sub>2</sub>O flux measurements from 3002 sites across diverse aquatic systems, including rivers, streams, lakes, reservoirs, ponds, estuaries, coastal waters, and open seas. The dataset integrates information on aquatic N<sub>2</sub>O emission from 426 peer-reviewed publications across 8 continents, covering the period 1980&ndash;2023. While the number of observations has increased substantially since 2000, spatial coverage remains uneven, with significant gaps across Africa and parts of high-latitude regions, including Antarctica and South America. Our dataset revealed a highly skewed distribution of N<sub>2</sub>O concentration and flux across aquatic ecosystems, with rivers and streams exhibiting the most significant variability and functioning as emission hotspots. Lakes and estuaries showed moderate variability and emission levels, whereas seas and coastal waters were characterized by consistently lower values. Pearson correlation coefficient revealed a strong positive relationship of N<sub>2</sub>O fluxes with ammonium (NH<sub>4</sub><sup>+</sup>; R = 0.943, <em>p</em> &lt; 0.001), nitrate (NO<sub>3</sub><sup>-</sup>; R = 0.691, <em>p</em> &lt; 0.001), and nitrite (NO<sub>2</sub><sup>-</sup>; R = 0.807, <em>p</em> &lt; 0.001). Significant negative correlations were found with dissolved oxygen (DO; R = -0.205, <em>p</em> &lt; 0.05), dissolved organic carbon (DOC; R = -0.977, <em>p</em> &lt; 0.05), and salinity (R = -0.636, <em>p</em> = 0.005), while non-significant associations were observed for water temperature, total nitrogen (TN), and total phosphorus (TP). The GANED dataset facilitates improved quantification of global aquatic N<sub>2</sub>O inventories by providing comprehensive N<sub>2</sub>O concentrations and fluxes in water bodies, as well as metadata describing sampling location, aquatic system type, and associated environmental parameters. The magnitude and patterns of N<sub>2</sub>O emissions from water bodies provided by the GANED database are essential in defining how these aquatic ecosystems shape our climate, refining emission estimates, identifying drivers, and guiding mitigation strategies.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-109</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-109/]]></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:essd134923</identifier>
    <datestamp>2026-05-13</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[Global Carbon Budget 2025]]></dc:title>
      <dc:creator>Friedlingstein, Pierre</dc:creator>
      <dc:creator>O'Sullivan, Michael</dc:creator>
      <dc:creator>Jones, Matthew W.</dc:creator>
      <dc:creator>Andrew, Robbie M.</dc:creator>
      <dc:creator>Bakker, Dorothee C. E.</dc:creator>
      <dc:creator>Hauck, Judith</dc:creator>
      <dc:creator>Landschützer, Peter</dc:creator>
      <dc:creator>Quéré, Corinne</dc:creator>
      <dc:creator>Li, Hongmei</dc:creator>
      <dc:creator>Luijkx, Ingrid T.</dc:creator>
      <dc:creator>Peters, Glen P.</dc:creator>
      <dc:creator>Peters, Wouter</dc:creator>
      <dc:creator>Pongratz, Julia</dc:creator>
      <dc:creator>Schwingshackl, Clemens</dc:creator>
      <dc:creator>Sitch, Stephen</dc:creator>
      <dc:creator>Canadell, Josep G.</dc:creator>
      <dc:creator>Ciais, Philippe</dc:creator>
      <dc:creator>Aas, Kjetil</dc:creator>
      <dc:creator>Alin, Simone R.</dc:creator>
      <dc:creator>Anthoni, Peter</dc:creator>
      <dc:creator>Barbero, Leticia</dc:creator>
      <dc:creator>Bates, Nicholas R.</dc:creator>
      <dc:creator>Bellouin, Nicolas</dc:creator>
      <dc:creator>Benoit-Cattin, Alice</dc:creator>
      <dc:creator>Berghoff, Carla F.</dc:creator>
      <dc:creator>Bernardello, Raffaele</dc:creator>
      <dc:creator>Bopp, Laurent</dc:creator>
      <dc:creator>Brasika, Ida Bagus Mandhara</dc:creator>
      <dc:creator>Chamberlain, Matthew A.</dc:creator>
      <dc:creator>Chandra, Naveen</dc:creator>
      <dc:creator>Chevallier, Frédéric</dc:creator>
      <dc:creator>Chini, Louise P.</dc:creator>
      <dc:creator>Collier, Nathan O.</dc:creator>
      <dc:creator>Colligan, Thomas H.</dc:creator>
      <dc:creator>Cronin, Margot</dc:creator>
      <dc:creator>Djeutchouang, Laique M.</dc:creator>
      <dc:creator>Dou, Xinyu</dc:creator>
      <dc:creator>Enright, Matt P.</dc:creator>
      <dc:creator>Enyo, Kazutaka</dc:creator>
      <dc:creator>Erb, Michael</dc:creator>
      <dc:creator>Evans, Wiley</dc:creator>
      <dc:creator>Feely, Richard A.</dc:creator>
      <dc:creator>Feng, Liang</dc:creator>
      <dc:creator>Ford, Daniel J.</dc:creator>
      <dc:creator>Foster, Adrianna</dc:creator>
      <dc:creator>Fransner, Filippa</dc:creator>
      <dc:creator>Gasser, Thomas</dc:creator>
      <dc:creator>Gehlen, Marion</dc:creator>
      <dc:creator>Gkritzalis, Thanos</dc:creator>
      <dc:creator>Goncalves De Souza, Jefferson</dc:creator>
      <dc:creator>Grassi, Giacomo</dc:creator>
      <dc:creator>Gregor, Luke</dc:creator>
      <dc:creator>Gruber, Nicolas</dc:creator>
      <dc:creator>Guenet, Bertrand</dc:creator>
      <dc:creator>Gürses, Özgür</dc:creator>
      <dc:creator>Harrington, Kirsty</dc:creator>
      <dc:creator>Harris, Ian</dc:creator>
      <dc:creator>Heinke, Jens</dc:creator>
      <dc:creator>Hurtt, George C.</dc:creator>
      <dc:creator>Iida, Yosuke</dc:creator>
      <dc:creator>Ilyina, Tatiana</dc:creator>
      <dc:creator>Ito, Akihiko</dc:creator>
      <dc:creator>Jacobson, Andrew R.</dc:creator>
      <dc:creator>Jain, Atul K.</dc:creator>
      <dc:creator>Jarníková, Tereza</dc:creator>
      <dc:creator>Jersild, Annika</dc:creator>
      <dc:creator>Jiang, Fei</dc:creator>
      <dc:creator>Jones, Steve D.</dc:creator>
      <dc:creator>Kato, Etsushi</dc:creator>
      <dc:creator>Keeling, Ralph F.</dc:creator>
      <dc:creator>Klein Goldewijk, Kees</dc:creator>
      <dc:creator>Knauer, Jürgen</dc:creator>
      <dc:creator>Kong, Yawen</dc:creator>
      <dc:creator>Korsbakken, Jan Ivar</dc:creator>
      <dc:creator>Koven, Charles</dc:creator>
      <dc:creator>Kunimitsu, Taro</dc:creator>
      <dc:creator>Lan, Xin</dc:creator>
      <dc:creator>Liu, Junjie</dc:creator>
      <dc:creator>Liu, Zhiqiang</dc:creator>
      <dc:creator>Liu, Zhu</dc:creator>
      <dc:creator>Monaco, Claire</dc:creator>
      <dc:creator>Ma, Lei</dc:creator>
      <dc:creator>Marland, Gregg</dc:creator>
      <dc:creator>McGuire, Patrick C.</dc:creator>
      <dc:creator>McKinley, Galen A.</dc:creator>
      <dc:creator>Melton, Joe R.</dc:creator>
      <dc:creator>Monacci, Natalie</dc:creator>
      <dc:creator>Monier, Erwan</dc:creator>
      <dc:creator>Morgan, Eric J.</dc:creator>
      <dc:creator>Munro, David R.</dc:creator>
      <dc:creator>Müller, Jens D.</dc:creator>
      <dc:creator>Nakaoka, Shin-Ichiro</dc:creator>
      <dc:creator>Nayagam, Lorna R.</dc:creator>
      <dc:creator>Niwa, Yosuke</dc:creator>
      <dc:creator>Nutzel, Tobias</dc:creator>
      <dc:creator>Olsen, Are</dc:creator>
      <dc:creator>Omar, Abdirahman M.</dc:creator>
      <dc:creator>Pan, Naiqing</dc:creator>
      <dc:creator>Pandey, Sudhanshu</dc:creator>
      <dc:creator>Pierrot, Denis</dc:creator>
      <dc:creator>Qin, Zhangcai</dc:creator>
      <dc:creator>Regnier, Pierre</dc:creator>
      <dc:creator>Rehder, Gregor</dc:creator>
      <dc:creator>Resplandy, Laure</dc:creator>
      <dc:creator>Roobaert, Alizée</dc:creator>
      <dc:creator>Rosan, Thais M.</dc:creator>
      <dc:creator>Rödenbeck, Christian</dc:creator>
      <dc:creator>Schwinger, Jörg</dc:creator>
      <dc:creator>Skjelvan, Ingunn</dc:creator>
      <dc:creator>Smallman, T. Luke</dc:creator>
      <dc:creator>Spada, Victoria</dc:creator>
      <dc:creator>Sreeush, Mohanan G.</dc:creator>
      <dc:creator>Sun, Qing</dc:creator>
      <dc:creator>Sutton, Adrienne J.</dc:creator>
      <dc:creator>Sweeney, Colm</dc:creator>
      <dc:creator>Swingedouw, Didier</dc:creator>
      <dc:creator>Séférian, Roland</dc:creator>
      <dc:creator>Takao, Shintaro</dc:creator>
      <dc:creator>Tatebe, Hiroaki</dc:creator>
      <dc:creator>Tian, Hanqin</dc:creator>
      <dc:creator>Tian, Xiangjun</dc:creator>
      <dc:creator>Tilbrook, Bronte</dc:creator>
      <dc:creator>Tsujino, Hiroyuki</dc:creator>
      <dc:creator>Tubiello, Francesco</dc:creator>
      <dc:creator>Ooijen, Erik</dc:creator>
      <dc:creator>Werf, Guido R.</dc:creator>
      <dc:creator>Velde, Sebastiaan J.</dc:creator>
      <dc:creator>Walker, Anthony P.</dc:creator>
      <dc:creator>Wanninkhof, Rik</dc:creator>
      <dc:creator>Yang, Xiaojuan</dc:creator>
      <dc:creator>Yuan, Wenping</dc:creator>
      <dc:creator>Yue, Xu</dc:creator>
      <dc:creator>Zeng, Jiye</dc:creator>
      <dc:description><![CDATA[<p>Accurate assessment of anthropogenic carbon dioxide (CO<span class="inline-formula"><sub>2</sub></span>) emissions and their redistribution among the atmosphere, ocean, and terrestrial biosphere in a changing climate is critical to better understand the global carbon cycle, support the development of climate policies, and project future climate change. Here we describe and synthesise datasets and methodologies to quantify the five major components of the global carbon budget and their uncertainties. Fossil CO<span class="inline-formula"><sub>2</sub></span> emissions (<span class="inline-formula"><i>E</i><sub>FOS</sub></span>) are based on energy and cement production data. Emissions from land-use change (<span class="inline-formula"><i>E</i><sub>LUC</sub></span>) are estimated by bookkeeping models based on land-use data. The global atmospheric CO<span class="inline-formula"><sub>2</sub></span> growth rate (<span class="inline-formula"><i>G</i><sub>ATM</sub></span>) is computed from changes in concentration measured at surface stations. The global net uptake of CO<span class="inline-formula"><sub>2</sub></span> by the ocean (<span class="inline-formula"><i>S</i><sub>OCEAN</sub></span>) is estimated with global ocean biogeochemistry models and observation-based <span class="inline-formula"><i>f</i></span>CO<span class="inline-formula"><sub>2</sub></span>-products. The global net uptake of CO<span class="inline-formula"><sub>2</sub></span> by the land (<span class="inline-formula"><i>S</i><sub>LAND</sub></span>) is estimated with dynamic global vegetation models. Additional lines of evidence are provided by atmospheric inversions, atmospheric oxygen measurements, ocean interior observation-based estimates, and Earth System Models. This year, we introduced corrections on the <span class="inline-formula"><i>E</i><sub>LUC</sub></span>, <span class="inline-formula"><i>S</i><sub>OCEAN</sub></span> and <span class="inline-formula"><i>S</i><sub>LAND</sub></span> estimates. The sum of all sources and sinks results in the carbon budget imbalance (<span class="inline-formula"><i>B</i><sub>IM</sub></span>), a measure of imperfect data and incomplete understanding of the contemporary carbon cycle. All uncertainties are reported as <span class="inline-formula">±</span> 1<span class="inline-formula"><i>σ</i></span>.</p>        <p>For the year 2024, <span class="inline-formula"><i>E</i><sub>FOS</sub></span> increased by 1.1 % relative to 2023, with fossil emissions at 10.3 <span class="inline-formula">±</span> 0.5 GtC yr<span class="inline-formula"><sup>−1</sup></span> (including the cement carbonation sink, 0.2 GtC yr<span class="inline-formula"><sup>−1</sup></span>), <span class="inline-formula"><i>E</i><sub>LUC</sub></span> was 1.3 <span class="inline-formula">±</span> 0.7 GtC yr<span class="inline-formula"><sup>−1</sup></span>, for total anthropogenic CO<span class="inline-formula"><sub>2</sub></span> emissions of 11.6 <span class="inline-formula">±</span> 0.9 GtC yr<span class="inline-formula"><sup>−1</sup></span> (42.4 <span class="inline-formula">±</span> 3.2 GtCO<span class="inline-formula"><sub>2</sub></span> yr<span class="inline-formula"><sup>−1</sup></span>). Also, for 2024, <span class="inline-formula"><i>G</i><sub>ATM</sub></span> was 7.9 <span class="inline-formula">±</span> 0.2 GtC yr<span class="inline-formula"><sup>−1</sup></span> (3.73 <span class="inline-formula">±</span> 0.1 ppm yr<span class="inline-formula"><sup>−1</sup></span>), 2.2 GtC above the 2023 growth rate. <span class="inline-formula"><i>S</i><sub>OCEAN</sub></span> was 3.4 <span class="inline-formula">±</span> 0.4 GtC yr<span class="inline-formula"><sup>−1</sup></span> and <span class="inline-formula"><i>S</i><sub>LAND</sub></span> was 1.9 <span class="inline-formula">±</span> 1.1 GtC yr<span class="inline-formula"><sup>−1</sup></span>, leaving a large negative <span class="inline-formula"><i>B</i><sub>IM</sub></span> (<span class="inline-formula">−</span>1.7 GtC yr<span class="inline-formula"><sup>−1</sup></span>), suggesting that the total sink or <span class="inline-formula"><i>G</i><sub>ATM</sub></span> is strongly overestimated in 2024. The global atmospheric CO<span class="inline-formula"><sub>2</sub></span> concentration averaged over 2024 reached 422.8 <span class="inline-formula">±</span> 0.1 ppm. Preliminary data for 2025 suggest an increase in <span class="inline-formula"><i>E</i><sub>FOS</sub></span> relative to 2024 of <span class="inline-formula">+</span>1.0 % (0.2 % to 1.7 %) globally, and atmospheric CO<span class="inline-formula"><sub>2</sub></span> concentration increasing by 2.1 ppm reaching 425.6 ppm, 53 % above the pre-industrial level (around 278 ppm in 1750). Overall, the mean and trend in the components of the global carbon budget are consistently estimated over the period 1959–2024, with a near-zero overall budget imbalance, although discrepancies of up to around 1 GtC yr<span class="inline-formula"><sup>−1</sup></span> persist for the representation of annual to decadal variability in CO<span class="inline-formula"><sub>2</sub></span> fluxes. Comparison of estimates from multiple approaches and observations shows: (1) a persistent large uncertainty in the estimate of land-use change emissions, (2) a low agreement between the different methods on the magnitude of the land CO<span class="inline-formula"><sub>2</sub></span> flux in the northern extra-tropics, and (3) a discrepancy between the different methods on the mean ocean sink.</p>        <p><span id="page3215"/>This living data update documents changes in methods and datasets applied to this most-recent global carbon budget as well as evolving community understanding of the global carbon cycle. The data presented in this work are available at <a href="https://doi.org/10.18160/GCP-2025">https://doi.org/10.18160/GCP-2025</a> (Friedlingstein et al., 2025c).</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-3211-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/3211/2026/]]></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:essd130142</identifier>
    <datestamp>2026-05-13</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[The new seismic catalog of the Gargano area (Southern Italy) after a decade of seismic monitoring by OTRIONS network]]></dc:title>
      <dc:creator>Ferreri, Andrea Pio</dc:creator>
      <dc:creator>Romeo, Annalisa</dc:creator>
      <dc:creator>Giannuzzi, Rossella</dc:creator>
      <dc:creator>Ninivaggi, Teresa</dc:creator>
      <dc:creator>Filippucci, Marilena</dc:creator>
      <dc:creator>Cecere, Gianpaolo</dc:creator>
      <dc:creator>Falco, Luigi</dc:creator>
      <dc:creator>Michele, Maddalena</dc:creator>
      <dc:creator>Selvaggi, Giulio</dc:creator>
      <dc:creator>Tallarico, Andrea</dc:creator>
      <dc:description><![CDATA[<p>The Gargano Promontory (hereafter GP) has attracted the attention of seismologists in recent years for its peculiarities regarding the high rate of low-magnitude seismicity and focal depths in the lower crust. These peculiarities have been highlighted thanks to the new data provided by the OTRIONS seismic network (hereafter OT), installed in 2013 in the GP area, consisting of 15 short-period seismometers, thanks to a fruitful collaboration between UniBa (University of Bari Aldo Moro) and INGV (Istituto Nazionale di Geofisica e Vulcanologia). The first available seismic catalog referred to the first <span class="inline-formula">7</span> years of the network operation (2013–2018) and suffered from some technological problems of the acquisition system. Thanks to improvements in the data transmission system, these problems were overcome in <span class="inline-formula">2019</span> and now the OT network data are available in real time. In order to include the most recent seismicity and to cover the temporal gaps existing in the previous catalog, we thoroughly reviewed the <span class="inline-formula">24</span> h seismic recordings, collected over the decade after the installation, by employing an automatic detect and picking software (CASP, Complete Automatic Seismic Processor). More than 7100 seismic events were initially identified. Through careful manual review, approximately 60 % were confirmed as local earthquakes, and the others were recognized as quarry blasts or false/poorly-located events. Manual review significantly improved the quality of P- and S-phase picking, and consequently led to more accurate earthquake locations, using both linearized and nonlinear algorithms. The manual review resulted in two catalogs, both released on Mendeley Data <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx8">Ferreri et al.</a>, <a href="#bib1.bibx8">2026</a>)</span> (<a href="https://doi.org/10.17632/nhfvx7ysxw.6">https://doi.org/10.17632/nhfvx7ysxw.6</a>). This study highlights the value of automatic analysis for compiling a seismic catalog, suggesting that the manual review is still necessary. The quality of the catalogs was assessed in detail using statistical parameters and a new formula for the location quality. The completeness magnitude of the new catalogs is as low as <span class="inline-formula">0.82</span>. The noise affecting the network was also evaluated. This study confirms the importance of the OT local network for seismic hazard analysis and provides a useful dataset for seismotectonic and geophysical studies in a long under-monitored region.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-3177-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/3177/2026/]]></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:asr127303</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>asr</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 damaging supercell hailstorm on 6 July 2023 in Vitoria-Gasteiz, the Basque Country]]></dc:title>
      <dc:creator>Egaña, Joseba</dc:creator>
      <dc:creator>Arrillaga, Jon Ander</dc:creator>
      <dc:creator>Gaztelumendi, Santiago</dc:creator>
      <dc:description><![CDATA[<p>We analyze a severe supercell that affected Vitoria-Gasteiz (Basque Country, northern Spain) on 6 July 2023, producing 4–5 cm hail and rainfall rates close to 30 mm h<span class="inline-formula"><sup>−1</sup></span>. The main objective of this work is to improve the forecasting and early-warning capabilities for similar high-impact storms in the Basque Country. This region lies on the northern edge of one of the most active supercell areas of the Iberian Peninsula, but remains relatively understudied. The synoptic and convective environment is examined using GFS analyses and the 1 km operational WRF configuration of Euskalmet, while the storm evolution and surface impacts are characterized through radar, rain gauge and disdrometer data. Environmental parameters were substantially above the median of Spanish very-large-hail supercells, with surface-based CAPE near 2000 J kg<span class="inline-formula"><sup>−1</sup></span>, 0–6 km bulk shear of 20–25 m s<span class="inline-formula"><sup>−1</sup></span> and 0–3 km storm-relative helicity slightly above 200 m<span class="inline-formula"><sup>2</sup></span> s<span class="inline-formula"><sup>−2</sup></span>. The storm originated from a splitting cell and rapidly intensified as a right-moving supercell, reaching cloud-top heights of 14–15 km and reflectivity values of 60–65 dB<span class="inline-formula"><i>Z</i></span>. This case also shows that convective initiation and storm splitting west of Basque Country must be monitored, as right-moving cells from these areas can affect the Basque Country when the vertical wind profile shows cyclonic curvature.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/asr-22-165-2026</dc:identifier>
      <dc:identifier><![CDATA[https://asr.copernicus.org/articles/22/165/2026/]]></dc:identifier>
      <dc:source>eISSN: 1992-0636</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:amt138596</identifier>
    <datestamp>2026-05-13</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"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Ground-based comparison of Sentinel-5P TROPOMI cloud fraction products using calibration-informed low-cost multi-spectral sensors]]></dc:title>
      <dc:creator>Schneider, Wolfgang</dc:creator>
      <dc:description><![CDATA[<p>Ground-based comparison of satellite atmospheric products is essential for ensuring data quality and algorithm performance. We present a comparison approach for Sentinel-5P TROPOspheric Monitoring Instrument (TROPOMI) cloud fraction products using a multi-spectral ground station (DG2MCM-15) located in Kempten, Bavaria, Germany. The ground observatory combines calibration-informed measurement protocols with low-cost commercial sensors, creating a citizen science comparison capability.</p>        <p>Our comparison dataset comprises 276 temporally matched observations between Sentinel-5P overpasses and ground measurements over a four-week period (11 January–8 February 2026). Ground-based cloud detection using an MLX90614 infrared pyrometer yields a Pearson correlation of <span class="inline-formula"><i>R</i>=0.879</span> (<span class="inline-formula"><i>N</i>=27</span> after quality filtering) with Sentinel-5P cloud fraction retrievals. However, this correlation is driven substantially by two high-cloud-fraction observations; the effective degrees of freedom are lower than <span class="inline-formula"><i>N</i></span> would suggest, and the method is better characterised as a three-state classifier (clear/partly cloudy/overcast) than as a continuous cloud fraction retrieval. The root mean square error of 29.1 % cloud fraction reflects a systematic positive bias from spatial scale mismatch between the ground sensor field of view and satellite pixel dimensions. The method reliably distinguishes between clear, partially cloudy, and overcast conditions, though the derived cloud fraction values exhibit clustering due to the temperature-ratio approach used. Exploratory comparison with TROPOMI aerosol index products yielded negligible correlation due to the absence of UV spectral coverage in the ground sensor, identifying a clear instrumentation requirement for future aerosol validation work.</p>        <p>Temporal matching between satellite overpasses and ground observations achieved a mean time difference of 2.7 min, with 95 % of matches within 8 min of satellite observation time. Spatial co-location analysis confirms all comparison points fall within the nominal TROPOMI pixel footprint (3.5 km <span class="inline-formula">×5.5</span> km at nadir), though the spatial scale mismatch between the ground sensor field of view and satellite pixel dimensions remains the primary source of comparison uncertainty.</p>        <p>Our results demonstrate that low-cost infrared sensors, when operated with calibration-informed measurement protocols, can provide scientifically useful satellite cloud product screening data, reliably distinguishing between clear, partially cloudy, and overcast conditions. The quasi-discrete nature of the derived cloud fraction highlights the need for improved cloud detection algorithms in future work. This approach offers a scalable pathway for expanding ground-based validation networks in regions lacking dedicated atmospheric monitoring infrastructure.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-3137-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/3137/2026/]]></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:amt137713</identifier>
    <datestamp>2026-05-13</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"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Impact of spectral aerosol radiative forcing at the Izaña observatory during the August 2023 extreme wildfires]]></dc:title>
      <dc:creator>García, Rosa D.</dc:creator>
      <dc:creator>Barreto, África</dc:creator>
      <dc:creator>Cachorro, Victoria E.</dc:creator>
      <dc:creator>González-Sicilia, Pablo</dc:creator>
      <dc:creator>Léon-Luis, Sergio</dc:creator>
      <dc:creator>Álvarez-Hernández, Ayoze</dc:creator>
      <dc:creator>Bustos, Juan José</dc:creator>
      <dc:creator>Ramos, Ramón</dc:creator>
      <dc:creator>Almansa, Fernando</dc:creator>
      <dc:creator>Álvarez-Losada, Óscar</dc:creator>
      <dc:creator>González, Yenny</dc:creator>
      <dc:creator>Rivas, Pedro Pablo</dc:creator>
      <dc:creator>Torres, Carlos Javier</dc:creator>
      <dc:description><![CDATA[<p>Extreme wildfires represent a highly variable source of atmospheric aerosols with potentially strong impacts on surface solar radiation. In August 2023, an exceptional wildfire on Tenerife (Canary Islands, Spain) reached the neighbourhoods of the Izaña Observatory (IZO, 2400 m a.s.l.). This near-source configuration enabled a rare observational characterisation of the spectral radiative effects of biomass-burning aerosols. During the most intense phases of the event (17–18 August), aerosol optical depth (AOD) at 500 nm reached extreme values of 3.63 and 2.25, respectively, with Ångström Exponent (AE) above 2, indicating a strong dominance of fine-mode smoke particles. Spectral measurements of global-horizontal, direct-normal and diffuse-horizontal solar irradiance (300–1100 nm) show a pronounced attenuation of direct and global irradiances, particularly in the visible range, together with a strong enhancement of diffuse radiation. Relative to clean-sky conditions, daily global irradiance decreased by 21 %–27 %, while direct-normal irradiance was reduced by 72 %–99 %. Spectral aerosol radiative forcing and radiative forcing efficiency at the surface were quantified using radiative transfer simulations under pristine atmospheric conditions as a reference. The integrated spectral radiative forcing (300–1100 nm) for global irradiance reached <span class="inline-formula">−395</span> and <span class="inline-formula">−299</span> W m<span class="inline-formula"><sup>−2</sup></span> on 17 and 18 August, respectively, indicating strong surface cooling dominated by scattering processes. Maximum forcing and efficiency occurred in the visible spectral range, consistent with the optical properties of freshly emitted smoke aerosols. At the same time, increases in the amount of present particles, equivalent black carbon (eBC) and greenhouse gases (CO<span class="inline-formula"><sub>2</sub></span>, CH<span class="inline-formula"><sub>4</sub></span> and CO) confirm the direct influence of the wildfire plume on atmospheric composition at IZO. These observations provide one of the few detailed spectral assessments of surface radiative forcing by extreme biomass-burning aerosols at a high-altitude site and highlight the need to accurately represent fine-mode smoke aerosols in radiative transfer and climate models.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-3151-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/3151/2026/]]></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:acp135891</identifier>
    <datestamp>2026-05-13</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[Measurement report: Chemical characterization of cloud water at Monte Cimone (Italy) – impact of air mass origin and assessment of atmospheric processes]]></dc:title>
      <dc:creator>Nibert, Pauline</dc:creator>
      <dc:creator>Wu, Yi</dc:creator>
      <dc:creator>Joly, Muriel</dc:creator>
      <dc:creator>Amato, Pierre</dc:creator>
      <dc:creator>Cristofanelli, Paolo</dc:creator>
      <dc:creator>Calzolari, Francescopiero</dc:creator>
      <dc:creator>Piro, Jean-Luc</dc:creator>
      <dc:creator>Putero, Davide</dc:creator>
      <dc:creator>Montaguti, Simonetta</dc:creator>
      <dc:creator>Renzi, Laura</dc:creator>
      <dc:creator>Vogel, Franziska</dc:creator>
      <dc:creator>Rapuano, Marco</dc:creator>
      <dc:creator>Brigante, Marcello</dc:creator>
      <dc:creator>Verhaege, Christophe</dc:creator>
      <dc:creator>Baray, Jean-Luc</dc:creator>
      <dc:creator>Deguillaume, Laurent</dc:creator>
      <dc:creator>Marinoni, Angela</dc:creator>
      <dc:creator>Zanatta, Marco</dc:creator>
      <dc:creator>Bianco, Angelica</dc:creator>
      <dc:description><![CDATA[<p>In this article, we present the results of the chemical and microbiological characterization of clouds water collected at Monte Cimone (CMN) in Italy at 2165 m a.s.l. during the MC3 (Molecular Composition of Clouds at mt. Cimone) campaign, which took place in October 2024. Twenty-six cloud samples are analyzed. Chemical analyses, including ions, oxidants, trace metals, and microbiological analyses with cell counting, are performed. The chemical characterization and back-trajectories analysis reveal that Mt. Cimone is a site under the influence of marine air masses, coming mainly from southern Europe and from the Mediterranean region. During the measurement campaign, 3 sampling periods are identified: period (1) 7–10 October, with air masses mainly originating from Spain and Atlantic Ocean with a majority of Cl<span class="inline-formula"><sup>−</sup></span> and Na<span class="inline-formula"><sup>+</sup></span> that are characteristics of marine origin; period (2) 16–18 October with air masses originating from North of Africa, impacted by a Saharan dust event with a high concentration in Ca<span class="inline-formula"><sup>2+</sup></span>; period (3) 22–23 October marked by air masses originated from southern Italy under polluted influence with a high concentration in NO<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="9pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="0723f17b5be9fc41c36a5585631feb47"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-6489-2026-ie00001.svg" width="9pt" height="16pt" src="acp-26-6489-2026-ie00001.png"/></svg:svg></span></span>. Across the campaign, DOC ranged from 1.6 to 4.3 mgC L<span class="inline-formula"><sup>−1</sup></span>, while H<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>2</sub></span> reached its maximum during period 3 (<span class="inline-formula">71.8±35.4</span> <span class="inline-formula">µ</span>mol L<span class="inline-formula"><sup>−1</sup></span>), highlighting enhanced oxidant levels under polluted conditions. This study paves the way to further scientific campaigns intended to better comprehend cloud water composition at Mt. Cimone.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-6489-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/6489/2026/]]></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:acp136072</identifier>
    <datestamp>2026-05-13</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[Interpretable machine learning quantifies composition and size influences on aerosol spectral absorption]]></dc:title>
      <dc:creator>Wang, Wenfang</dc:creator>
      <dc:creator>Tian, Pengfei</dc:creator>
      <dc:creator>Zeng, Shuhua</dc:creator>
      <dc:creator>Zhang, Yifei</dc:creator>
      <dc:creator>Yu, Zeren</dc:creator>
      <dc:creator>Cui, Chen</dc:creator>
      <dc:creator>Wu, Yunfei</dc:creator>
      <dc:creator>Chen, Min</dc:creator>
      <dc:creator>Zhang, Lei</dc:creator>
      <dc:description><![CDATA[<p>The spectral dependence of aerosol absorption, characterized by the absorption Ångström exponent (AAE), strongly influences radiative effects, yet the relative importance of controlling factors remains poorly quantified. We integrate multisource observations with an interpretable machine-learning framework (Shapley Additive Explanations, SHAP) to disentangle the roles of chemical composition and particle size in predicting AAE and to evaluate radiative impacts. Field observation in Beijing reveal that near-surface AAE is predominantly influenced by higher fine mineral dust and water-soluble inorganic ions fractions. Multi-year columnar data identify dust loading as the dominant predictor, followed by carbonaceous aerosols. The fine-mode radius accounts for 29 % of size parameters cumulative importance and ranks closely with black carbon. SHAP diagnostics highlight that columnar AAE contributes to radiative forcing at the top of the atmosphere (TOA) comparably to single scattering albedo (SSA), while its impact is clearly weaker at the bottom of the atmosphere and in the atmosphere. These findings help clarify AAE determinants and reduce uncertainties in aerosol radiative effect assessments.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-6471-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/6471/2026/]]></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:acp130700</identifier>
    <datestamp>2026-05-13</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[Variability of ice supersaturated regions at flight altitudes: evaluation of ERA5 reanalysis using IAGOS in situ measurements]]></dc:title>
      <dc:creator>Hildebrandt, Katarina Grubbe</dc:creator>
      <dc:creator>Castino, Federica</dc:creator>
      <dc:creator>Meijer, Vincent</dc:creator>
      <dc:creator>Yin, Feijia</dc:creator>
      <dc:description><![CDATA[<p>Contrail cirrus is a major contributor to aviation's radiative forcing. Avoiding persistent contrail formation has been suggested as a measure to reduce the climate impact of aviation, requiring accurate forecasts of ice supersaturated conditions, where the relative humidity over ice (RHi) exceeds 100 %. Numerical weather prediction models and reanalysis products often underestimate or do not account for ice supersaturation. This study evaluates ice supersaturated regions (ISSRs) in the ECMWF ERA5 reanalysis dataset using In-service Aircraft for a Global Observing System (IAGOS) measurements over tropical and extratropical regions in the upper troposphere and lower stratosphere from 2011 to 2022. It considers seasonal and vertical differences, and how cloudy and clear-sky conditions affect ERA5’s ability to predict ISSRs. ERA5 underestimates ISSR occurrence due to a dry bias in RHi; the equitable threat score (ETS) is 0.2–0.4, indicating a weak to mediocre skill. Lowering the ERA5 RHi threshold improves ISSR prediction, with the largest improvements for RHi between 85 % and 95 %, although the optimal threshold varies with distance to the tropopause, region and season. Clear-sky conditions result in an ETS of 0.05–0.18, while the ETS is mostly below 0.1 in cloudy conditions, indicating an almost random relationship. In clear-sky conditions, lowering the threshold to 85 % increases the ETS by approximately 0.1. In cloudy conditions, lowering the threshold shows little benefit because increases in correctly predicted ISSRs are offset by increases in false positives. These findings improve our understanding of ISSR variability and has implications for accurate assessment of persistent contrail formation.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-6449-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/6449/2026/]]></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:egusphere140981</identifier>
    <datestamp>2026-05-13</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[Impact of perennial forage plants on microbial carbon use efficiency in weathered Ethiopian soils]]></dc:title>
      <dc:creator>Wickander, Niklas Jan</dc:creator>
      <dc:creator>Dörsch, Peter</dc:creator>
      <dc:description><![CDATA[<em>Aims</em>: Ethiopian soils are highly weathered and in urgent need of remediation. Increasing the soil carbon (C) pool by perennials potentially remediates soil degradation while sequestering atmospheric CO<sub>2</sub>. The soil microbial loop is thought to play an important role in soil C sequestration as it contributes significantly to the stabilization of plant litter C. The amount of stabilized litter C has been hypothesized to depend on microbial carbon use efficiency (mCUE), which is sensitive to soil nutrients and plant inputs. Here, we investigate the effect of two perennial forage crops on mCUE in four weathered Ethiopian soils.</p> <p><em>Methods</em>: We cultivated the grass <em>Urochloa</em> cv. Cayman as single stand and in mixture with the legume <em>Desmodium intortum</em> in a fully factorial greenhouse experiment with four distinct farmers&rsquo; soils from the Ethiopian Rift Valley (Amhara and Sidama). Microbial CUE was assessed after 104 days of plant growth using <sup>18</sup>O-H<sub>2</sub>O incorporation.</p> <p><em>Results</em>: Microbial CUE varied between the four soils, with Amhara soils showing lower mCUE than Sidama soils. Overall, mCUE was little affected by plant growth but increased significantly with plant dry weight (DW) in one of the two Sidama soils. Mass specific growth rates remained small in Amhara soils, indicating that factors other than plant C input inhibited microbial growth. Plant composition had no effect in Amhara soils while the <em>Urochloa</em> &times; <em>Desmodium</em> mixture tended to have lower mCUE in Sidama soils.</p> <p><em>Conclusions</em>: Perennials may improve mCUE in weathered soils, but this stimulation strongly depends on soil nutrient availability and suggests that there are critical nitrogen (N) and phosphorous (P) thresholds below under which mCUE does not respond to growing plants. This implies that highly degraded soils must be ameliorated before using perennials to stimulate nutrient cycling and restore soil health.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2488</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2488/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141013</identifier>
    <datestamp>2026-05-13</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[Observations of the multi-year variability of mixing in shelf seas]]></dc:title>
      <dc:creator>Whitwell, Chris A.</dc:creator>
      <dc:creator>Jones, Nicole L.</dc:creator>
      <dc:creator>Ivey, Greg N.</dc:creator>
      <dc:creator>Rayson, Matthew D.</dc:creator>
      <dc:description><![CDATA[We present 5-year long continuous mixing observations from four mooring locations, spanning 10&deg; degrees of latitude, on the continental shelf of North-Western Australia. The sites are subject to a diverse range of atmospheric and oceanic forcing and each has distinct local bathymetry. We estimated the diapycnal diffusivity and vertical turbulent heat flux at all sites and throughout the water column using a fine-scale mixing length model. There were four dominant peaks in the power spectrum: annual, spring-neap, diurnal, and semi-diurnal. We examined the variability in the mixing at all sites in terms of the seasonal stratification, depth, and tidal range and phase. The highest annual variability occurred at the highest latitude sites which had the greatest seasonal variation in stratification. The mixing also varied with the strength of the dominant tidal constituents (both baroclinic and barotropic). Heat flux was a more useful measure of mixing than diffusivity due to the strong seasonal variations in density stratification on the shelf. Finally, we provide guidance on the determination of the appropriate sampling period to adequately describe the mixing, and discuss the effects of short sampling periods on the ability to describe the long-term mixing.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2498</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2498/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141030</identifier>
    <datestamp>2026-05-13</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 Physically Integrated GNN Surrogate for Microbially-Mediated Kinetic Reactive Transport: PHYGNET]]></dc:title>
      <dc:creator>Wang, Jinbo</dc:creator>
      <dc:creator>Zhang, Kunfeng</dc:creator>
      <dc:creator>Illman, Walter</dc:creator>
      <dc:creator>Chen, Shuai</dc:creator>
      <dc:creator>Liu, Mingzhu</dc:creator>
      <dc:description><![CDATA[Reactive transport modelling (RTM) is essential for subsurface environmental management but is fundamentally constrained by traditional geochemical solvers. These solvers incur prohibitive computational costs and frequently suffer from numerical instabilities such as convergence failures, particularly in microbially-mediated kinetic reaction systems. While machine learning surrogates offer acceleration, they often lack physical consistency when dealing with stiff biogeochemical dynamics. Here we propose PHYGNET (Physically GNN Network), which maps microbial reaction networks into a directed graph by representing species and reactions as nodes and edges. It embeds Monod-type kinetics within a physics layer to enforce mass conservation and thermodynamic hierarchies, and incorporates a residual corrector for refinement. By successfully coupling with COMSOL, PHYGNET demonstrates the capability to execute full reactive transport simulations. Benchmark tests reveal that, in contrast to the severe super-linear time penalties faced by traditional solvers at engineering scales, PHYGNET maintains stable sub-linear scaling via tensor parallelism. At a scale of 10<sup>5</sup> grid nodes, PHYGNET achieved an acceleration (up to 3524-fold) without numerical crashes. Furthermore, its escalating speedup ratio establishes a "small-sample training, ultra-large-scale inference" paradigm that effectively offsets initial data generation costs. Overall, PHYGNET provides an efficient and physically consistent framework for accelerating Monod-type microbial reactive transport simulations, offering a practical pathway for large-scale environmental applications.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2509</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2509/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141039</identifier>
    <datestamp>2026-05-13</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[Urbanization drives coupled shifts in soil-carbon stocks, sources, and stability across natural and restored mangroves and tidal flats]]></dc:title>
      <dc:creator>Huang, Minde</dc:creator>
      <dc:creator>Guo, Fen</dc:creator>
      <dc:creator>Gao, Xueqin</dc:creator>
      <dc:creator>Ouyang, Xiaoguang</dc:creator>
      <dc:creator>Zhang, Yuan</dc:creator>
      <dc:description><![CDATA[Urbanization reshapes coastal blue carbon, but its effects on how much carbon is stored, who supplies it, and how long it persists remain poorly integrated. We investigated natural and restored mangroves and adjacent tidal flats along an urbanization gradient, and quantified soil organic carbon stocks, burial from <sup>210</sup>Pb profiles, source composition using isotope end-member mixing, and stability from turnover metrics. Our results showed a coordinated triad response to urbanization. Carbon stocks and burial declined, sources shifted away from mangrove detritus toward planktonic and algal inputs, and turnover accelerated, lowering stability. Responses were habitat dependent and nonlinear. Natural mangroves in low urbanization settings maintained the highest sequestration with mangrove-dominated inputs and slower turnover. Restored stands and tidal flats showed steeper stock losses, stronger source substitution, and faster cycling under higher urban pressure. We introduced a triad framework that treats stocks, sources, and stability as coupled state variables along the urbanization gradient and identified two reproducible system states: carbon anchors in low urbanization natural mangroves and instability fronts in restored stands and tidal flats. Shifts in sources and stability precede stock losses, providing clear early warnings of urban impact. A simple diagnostic that combines connectivity and accretion with source composition and a composite stability index guides anchor protection and stability-first restoration. These results link urban growth to blue-carbon performance and define actionable thresholds for sustaining coastal carbon.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2512</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2512/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141150</identifier>
    <datestamp>2026-05-13</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[Orbital-scale hydroclimate variations in the western Qaidam Basin during the Late Pliocene: evidence from magnetic parameters and median grain size]]></dc:title>
      <dc:creator>Luo, Zeng</dc:creator>
      <dc:creator>Wang, Hansheng</dc:creator>
      <dc:creator>Yu, Xiaoli</dc:creator>
      <dc:creator>Zhang, Zhongbao</dc:creator>
      <dc:creator>Song, Zhifen</dc:creator>
      <dc:creator>Yang, Jing</dc:creator>
      <dc:creator>Chen, Wanfeng</dc:creator>
      <dc:creator>Su, Qiangda</dc:creator>
      <dc:creator>Lu, Yang</dc:creator>
      <dc:creator>Hua, Shun</dc:creator>
      <dc:description><![CDATA[A recent study suggests that the precipitation records of the Qaidam Basin during the middle Piacenzian warm period (mPWP, 3.264&ndash;3.025 Ma) are broadly consistent with those of the monsoon influenced regions, and are highly sensitive to 20-kyr precessional cycles, implying that the East Asian summer monsoon (EASM) intensified and migrated westward into the Asian interior during this warm interval. However, it remains unclear whether such a precession-dominated pattern persisted throughout the Late Pliocene or was restricted to specific intervals. To address this question, we present new magnetic parameter and median grain size records from the Gansen (GS) section for 3.6&ndash;3.25 Ma and 2.95&ndash;1.8 Ma, and integrate them with the previously published records for 3.25&ndash;2.95 Ma to assess orbital-scale precipitation variations in the western Qaidam Basin during the Late Pliocene. The results show that EASM-related summer moisture reached the western Qaidam Basin during 3.6&ndash;3.25 Ma, although the associated precipitation was weaker than during 3.25&ndash;2.95 Ma. Spectral analysis further reveals that precipitation variations during 3.6&ndash;3.3 Ma were characterized by dominant 100&ndash;kyr cyclicity rather than the previously reported precession-dominated pattern during 3.25&ndash;2.95 Ma, suggesting a nonlinear response to insolation forcing. This contrast indicates that the precession-dominated pattern was not a persistent feature throughout the Late Pliocene in the western Qaidam Basin. Instead, our results suggest that under different climatic background states, the dominant processes controlling the westward penetration of summer moisture into the western Qaidam Basin were also different, and that the 20-kyr and 100-kyr periodicities mainly reflect these differences in forcing response. In addition, the similar phase variations between these precipitation records and the benthic oxygen isotope stack at the 40-kyr band imply that Antarctic ice sheets may have modulated hydroclimatic variations in the basin. These findings provide new insight into how background climate conditions may shape the orbital-scale response of precipitation, and more broadly hydroclimatic variations, in the Asian interior during warm periods.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2580</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2580/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141082</identifier>
    <datestamp>2026-05-13</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[Dynamic CO2 evasion and colloidal control of trace metals in the Lower Lena River]]></dc:title>
      <dc:creator>Kolesnichenko, Yuri Ya.</dc:creator>
      <dc:creator>Vorobyev, Sergey N.</dc:creator>
      <dc:creator>Nikitkin, Viktor A.</dc:creator>
      <dc:creator>Dudarev, Oleg V.</dc:creator>
      <dc:creator>Chernykh, Denis V.</dc:creator>
      <dc:creator>Spivak, Eduard A.</dc:creator>
      <dc:creator>Kurilenko, Arkadiy V.</dc:creator>
      <dc:creator>Kholodov, Vladimir A.</dc:creator>
      <dc:creator>Semiletov, Igor P.</dc:creator>
      <dc:creator>Pokrovsky, Oleg S.</dc:creator>
      <dc:description><![CDATA[Large Arctic rivers integrate carbon and element fluxes across vast permafrost-dominated landscapes, yet the lower reaches of these systems remain poorly constrained in terms of greenhouse gas (GHG) emissions and solute organization. We investigated the Low Lena River over ~800 km during the beginning of summer baseflow, combining continuous in situ pCO<sub>2</sub> measurements, floating chamber flux determinations, and analyses of major and trace elements including colloidal size fractionation. CO<sub>2</sub> concentrations exhibited pronounced short-distance variability and weak northward decrease along the main stem. Diffusive CO<sub>2</sub> fluxes (0.1&ndash;1.3 g C m<sup>&minus;2</sup> d<sup>&minus;1</sup>) were comparable to values reported for other large Siberian rivers, confirming the Lena as a persistent but moderate atmospheric CO₂ source during the open-water season. In contrast, CH<sub>4</sub> concentrations were low and spatially uniform, contributing &lt;0.5 % to total carbon emissions. Notably, bulk DOC and DIC concentrations remained remarkably stable along the transect and were consistent with long-term monitoring records and previous expeditions, indicating strong buffering of dissolved carbon pools despite dynamic CO<sub>2</sub> evasion.</p> <p>Major and trace elements segregated into two geochemical groups. Highly mobile major ions, Si, and selected oxyanion-forming trace elements were predominantly present in truly dissolved form (0&ndash;20 % colloidal fraction) and reflected groundwater connectivity and water&ndash;rock interaction. In contrast, lithogenic low-solubility elements &ndash; including trivalent and tetravalent hydrolysates &ndash; were strongly associated with Fe&ndash;Al&ndash;organic colloids (&gt;70 %), indicating surface and suprapermafrost mobilization pathways. Multivariate statistics confirmed this dual organization of solute transport. These findings reveal a functional decoupling between structurally buffered dissolved carbon pools and dynamically regulated CO<sub>2</sub> exchange, a pattern likely characteristic of large Arctic rivers. Under ongoing warming, shifts in hydrological connectivity, discharge regime, and permafrost thaw may alter this balance, with implications for pan-Arctic carbon and element export to the Arctic Ocean.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2540</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2540/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141123</identifier>
    <datestamp>2026-05-13</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[Hidden Heat: The case of 2023 Gulf of Trieste Bottom Marine Heatwave]]></dc:title>
      <dc:creator>Giordano, Fabio</dc:creator>
      <dc:creator>Ličer, Matjaž</dc:creator>
      <dc:creator>Querin, Stefano</dc:creator>
      <dc:creator>Salon, Stefano</dc:creator>
      <dc:creator>Vodopivec, Martin</dc:creator>
      <dc:description><![CDATA[In summer and autumn 2023, unusually high bottom temperatures were recorded at the Vida buoy (LTER site, 22 m depth) in the Gulf of Trieste (northern Adriatic, Mediterranean Sea). This long-term dataset enabled rare in situ observation of a bottom marine heatwave (BMHW), which began in early August and lasted over three months. At its peak, bottom temperature reached 4.3<sup>&deg;</sup>C above the 20-year average and 1.2<sup>&deg;</sup>C above the previous maximum recorded since 2002. Observations and modelling indicate that the BMHW was preconditioned by a prolonged drought starting in 2022 and continuing into 2023. This resulted in elevated surface salinity and weakened stratification, allowing unusually deep mixing that extended to the seafloor. Although 2023 was warm, heat was distributed over a thicker water column than usual, limiting sea surface warming but causing extreme temperatures at depth. The event persisted into autumn due to freshwater inflow, which re-established stratification and trapped the heat below. As surface temperatures remained moderate, the BMHW was undetectable by satellites or surface measurements. Only bottom sensors and models revealed the stress in deeper layers. Such events may therefore remain unnoticed while exerting extreme stress on the marine ecosystem. Our findings highlight reduced precipitation and deep mixing as overlooked drivers of subsurface marine heatwaves, which may become more frequent in similar shallow and stratified areas subject to increasingly frequent droughts driven by climate change.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2567</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2567/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141092</identifier>
    <datestamp>2026-05-13</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[Everyday weather in a warmer world]]></dc:title>
      <dc:creator>Thomas, Rhidian Huw</dc:creator>
      <dc:creator>Compo, Gilbert P.</dc:creator>
      <dc:creator>George, Steve</dc:creator>
      <dc:creator>Hegerl, Gabriele C.</dc:creator>
      <dc:creator>Schurer, Andrew</dc:creator>
      <dc:creator>Shepherd, Theodore G.</dc:creator>
      <dc:creator>Slivinski, Laura C.</dc:creator>
      <dc:creator>Thompson, Vikki</dc:creator>
      <dc:creator>Hawkins, Ed</dc:creator>
      <dc:description><![CDATA[How would the weather of a year from history be experienced in a warmer world? We reconstruct the weather of 1903 using a reanalysis system that assimilates only surface pressure observations (20CRv3) with observed SSTs, and then reconstruct it again with increased SSTs and atmospheric CO<sub>2</sub> levels. By assimilating the same pressure observations, the reanalysis experiments produce the same weather patterns, and so we translate the weather of 1903 into a warmer context. We focus on changes in the everyday weather of four regions with a high density of historical pressure observations, where the circulation is constrained and differences between the experiments are due to the thermodynamic component of climate change. In these regions, nearly all days are warmer in the warmer world experiments, but the largest increases occur on cold days (below freezing) and hot days (above 20 &deg;C). Daily rainfall becomes more variable, even in regions where total rainfall is reduced. Fewer days experience light rain while more days experience heavy rain, and rainfall only increases on less than one day in 10. This single year pair of reanalysis experiments also recovers common patterns of observed and projected long-term changes. For example, Western Mediterranean precipitation declines outside winter, but shows a small increase in winter in the absence of storm track shifts. By anchoring our analysis in weather patterns that have actually occurred, the reanalysis experiments point to how our day-to-day experience of the weather may change in a warmer world.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2548</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2548/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141110</identifier>
    <datestamp>2026-05-13</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[Changes in Arctic sea ice drift speed over the last 130 years]]></dc:title>
      <dc:creator>Sinnhuber, Björn-Martin</dc:creator>
      <dc:description><![CDATA[The Arctic transpolar sea ice drift speed shows a pronounced increase over past decades, one of many manifestations of Arctic climate change. However, little is known so far how the drift changed in earlier periods. Here I use data from historical drift expeditions, in particular from the <em>Fram</em> in 1893&ndash;96, the <em>Sedov</em> in 1937&ndash;40, the <em>Tara</em> in 2007&ndash;08, and the <em>Polarstern</em> during MOSAiC in 2019&ndash;20, as well as from the Soviet/Russian North Pole drift stations, to derive a 130-year record of Arctic transpolar drift speed. The transpolar drift speed already increased significantly during the early 20<sup>th</sup> century warming, followed by a period of slowing drift in the 1950s&ndash;70s and a strong increase in recent decades, closely following the evolution of Arctic mean temperatures. The observed fractal scaling of the drifts can be explained quantitatively by a Brownian motion random walk process that includes temporal auto-correlation and a mean drift term due to currents and prevailing winds. Comparisons of the sea ice drift speeds with near surface wind observations reveal that the long-term changes in drift speed are not primarily caused by changes in wind speed.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2561</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2561/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141119</identifier>
    <datestamp>2026-05-13</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[Temperature-dependent multiphase chemical kinetics can explain uniform atmospheric nanoparticle growth rates]]></dc:title>
      <dc:creator>Zhang, Zhiqiang</dc:creator>
      <dc:creator>Kang, Hyun Gu</dc:creator>
      <dc:creator>Pöschl, Ulrich</dc:creator>
      <dc:creator>Berkemeier, Thomas</dc:creator>
      <dc:description><![CDATA[Aerosols have a profound influence on climate and human health, but new particle formation in the atmosphere has remained a scientific conundrum. In particular, the growth rates of atmospheric nanoparticles are often smaller and less dependent on condensable vapor concentration than expected. Here, we take a new integrative approach to analyze observational data from field measurements and chamber experiments, which were previously unexplained and appeared inconsistent with theory and model predictions. We show that the observed growth rates can be predicted when the temperature dependence and multiphase kinetics of gas-particle partitioning are resolved. Slow surface-to-bulk transport limits the rates of vapor uptake by semi-solid particles with low diffusivity, whereas shifts in the volatility distribution following the Clausius-Clapeyron equation enhance growth rates at low temperature and concentration levels. These antagonistic effects lead to an effective buffering of the organic vapor concentration dependence of nanoparticle growth in secondary organic aerosols. Our study reveals how counteracting temperature dependencies of organic vapor oxidation, volatility and multiphase kinetics lead to a convergence of growth rates around a few nanometers per hour under widely differing atmospheric conditions.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2564</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2564/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140964</identifier>
    <datestamp>2026-05-13</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[Non-Target Analysis of Atmospheric Organic Aerosols as a Tool to Discriminate Anthropogenic Contribution in Mixed Air Masses during the ACROSS campaign]]></dc:title>
      <dc:creator>Karbach, Niklas</dc:creator>
      <dc:creator>Pouyes, Pauline</dc:creator>
      <dc:creator>Perraudin, Emilie</dc:creator>
      <dc:creator>Villenave, Eric</dc:creator>
      <dc:creator>Hoffmann, Thorsten</dc:creator>
      <dc:description><![CDATA[Organic aerosol is a major component in the particle phase of Earth&acute;s atmosphere and has influences on quality of life, health and climate. In this study, a non-target analysis of the chemical composition of atmospheric organic aerosols using liquid chromatography-Orbitrap mass spectrometry (LC-Orbitrap MS) was conducted to differentiate anthropogenic and biogenic sources through unsupervised KMeans clustering. The ACROSS campaign dataset (consisting of 36 wind-characterized samples) identified 4,916 compounds (in the range 50&ndash;400 m/z). Due to the location of the sampling site, the samples contain influences from the greater Paris area, as well as biogenic influences from the surrounding forest. K-means clustering, constrained to 2,917 compounds with strong wind-direction correlation, resolved distinct biogenic and anthropogenic clusters. Biogenic aerosols were dominated by CHO compounds (H/C: 1.2&ndash;1.7; O/C: 0.15&ndash;0.7), consistent with oxidized terpenes, while anthropogenic aerosols featured significant CHOS enrichment (H/C: 1.5&ndash;2.2; O/C: 0.2&ndash;1.0), including nitrogen-sulfur aromatics (e.g., C<sub>10</sub>H<sub>18</sub>NO<sub>8</sub>S<sup>&minus;</sup> with nitro/sulfonic groups and aromatic fragments). The approach allows to quantify anthropogenic contribution in mixed air masses, demonstrating higher amounts of anthropogenic compounds ratios during Paris-influenced periods. Results validate wind-driven source apportionment for small sample size non-target studies, providing a transferable method for aerosol characterization.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2473</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2473/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140883</identifier>
    <datestamp>2026-05-13</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[Sea ice variability and links to East Siberian permafrost carbon remobilization during the last glacial-interglacial transition]]></dc:title>
      <dc:creator>Eriksson, Albin</dc:creator>
      <dc:creator>Wu, Junjie</dc:creator>
      <dc:creator>O'Regan, Matt</dc:creator>
      <dc:creator>Gustafsson, Örjan</dc:creator>
      <dc:description><![CDATA[Sea ice in plays a central role in the polar climate system. In recent decades, the rapid decline of Arctic sea ice has triggered cascading effects the albedo effect and gas/heat transfer in polar regions. Investigations of earlier warming events, such as the Preboreal/Early Holocene (PB/EH, 11&ndash;8 kyr B.P), B&oslash;lling-Aller&oslash;d (B/A, 14.7&ndash;12.9 kyr B.P), and Dansgaard Oeschger event 3 (DO-3, 28&ndash;27.5 kyr B.P), likely hold clues on climate system responses to changes in Arctic sea ice. This study explores the history of sea ice over the Southern Lomonosov Ridge and its potential relation to permafrost carbon remobilization. Sea ice conditions over the last 27 kyrs were reconstructed through a combination of the sea ice biomarker IP<sub>25 </sub>(Ice-proxy 25) and marine phytoplankton biomarkers (brassicasterol and dinosterol) from the chronologically well-constrained core 31-PC, sampled at the Southern Lomonosov Ridge during the SWERUS-C3 expedition in 2014. The reconstruction allowed for a direct comparison with previously published terrestrial organic carbon (terrOC) remobilization history from the same core. Our findings revealed a seasonal sea ice cover between 27&ndash;26 kyr B.P after the DO-3 warm event, which likely caused more heat and moisture transport from ocean to land and strengthened permafrost thawing along the nearby coastline. A perennial sea ice cover then developed and persisted throughout the Last Glacial Maximum (LGM) to the Younger Dryas (YD), including over the entire B/A warm period. Due to sea-level rise during Meltwater Pulse 1A (MWP 1A, 14.7&ndash;13.5 kyr B.P), terrOC remobilization during B/A was rapid but its magnitude smaller when compared to PB and DO-3 in 31-PC, and other records from the Arctic. These records collectively suggest that sea-level rise, rather than sea ice conditions, exerts the primary control on coastal erosion during B/A, while we propose that the perennial sea ice cover may have limited wave-induced coastal erosion on the continental shelf bordering the southern Lomonosov Ridge. A sharp reduction and breakup of the perennial sea ice was observed from the PB to the Early Holocene. Contrary to the B/A, Meltwater Pulse 1B during PB triggered significant coastal erosion and massive terrOC remobilization concurrent with the sea ice decline. The absence of sea ice in parallel to larger coastal erosion compared to B/A implies the role of waning sea ice in enhancing permafrost carbon mobilization along the coastline in this period. In accordance with sea ice records from other Arctic seas, the Holocene record exhibited a period of gradual sea ice expansion. Taken together, these findings highlight sea ice extent as a possible factor regulating coastal permafrost carbon remobilization during the last deglaciation.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2414</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2414/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140700</identifier>
    <datestamp>2026-05-13</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[Reviews and syntheses: Microbial Carbon Fixation in Dryland: A component of Global Carbon Cycle]]></dc:title>
      <dc:creator>Correa, Sulamita Santos</dc:creator>
      <dc:creator>Schultz, Júnia</dc:creator>
      <dc:creator>Sadaiappan, Balamurugan</dc:creator>
      <dc:creator>Rosado, Alexandre Soares</dc:creator>
      <dc:creator>Mundra, Sunil</dc:creator>
      <dc:description><![CDATA[Atmospheric carbon dioxide (CO<sub>2</sub>) sequestration is commonly attributed to plant-driven processes, while the contribution of soil microorganisms remains comparatively underexplored. This imbalance is particularly relevant in dryland ecosystems, which cover over 45 % of Earth&rsquo;s land surface and store a substantial fraction of global soil organic carbon. Despite their vast extent and ecological significance, current frameworks often overlook the metabolic potential of microbial communities inhabiting these environments. In drylands, microorganisms have evolved diverse metabolic strategies to capture and store atmospheric carbon, supported by multiple carbon-fixation pathways that extend beyond the Calvin&ndash;Benson&ndash;Bassham cycle. Here, we examine microbial carbon fixation in dryland ecosystems as an underexplored component of the global carbon cycle. We highlight the diversity, metabolic flexibility, and stress adaptations of carbon-fixing microbes and discuss the dominant pathways supporting carbon assimilation under arid conditions. By integrating evidence across studies, the findings suggest that microbial processes in drylands can contribute to carbon sequestration in ways not fully captured by plant-centered perspectives. This review provides a framework for incorporating microbial metabolic diversity into current models of terrestrial carbon cycling and highlights its relevance for climate change mitigation strategies.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2278</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2278/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140671</identifier>
    <datestamp>2026-05-13</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[Mobile weather radar to provide intelligence on wildfire hazards]]></dc:title>
      <dc:creator>Guyot, Adrien</dc:creator>
      <dc:creator>McGowan, Hamish</dc:creator>
      <dc:creator>Filippi, Jean-Baptiste</dc:creator>
      <dc:creator>Alonso-Pinar, Alberto</dc:creator>
      <dc:creator>Protat, Alain</dc:creator>
      <dc:creator>McCarthy, Nicholas</dc:creator>
      <dc:creator>Webster, Simon</dc:creator>
      <dc:creator>Taylor, Amie</dc:creator>
      <dc:description><![CDATA[Extreme wildfire behaviour is increasingly associated with deep pyro-convection and pyro-cumulonimbus (pyroCb) development, posing challenges for both scientific understanding and operational wildfire management. Existing wildfire intelligence relies on a combination of aerial observations, satellite remote sensing, numerical weather prediction, and in-situ measurements, which can be limited in resolving rapidly evolving plume dynamics and near-fire wind changes. Portable weather radars represent a promising observational approach by providing high-resolution measurements of plume structure, kinematics, and microphysical properties, together with conventional radar products such as precipitation and outflow detection. However, their role within wildfire intelligence frameworks remains relatively unexplored.</p> <p>In this study, we review two decades of portable radar observations of wildfires and prescribed burns and present new analyses from a recent deployment of a mobile dual-polarization X-band radar during an extreme wildfire in Eastern Australia. Building on these observations, we introduce a set of radar-derived diagnostics relevant to wildfire intelligence, including plume depth evolution, signatures of pyro-convective dynamics, detection of low-level wind changes, and indicators associated with transitions from pyro-cumulus to deep convection. These diagnostics complement existing satellite and modelling approaches by providing information on processes that are not directly observable from current operational platforms.</p> <p>Using a Technology Readiness Level (TRL) framework, we assess the maturity of portable radar applications for wildfire monitoring. While fundamental aspects of pyrometeor scattering remain at low readiness (TRL 1&ndash;3), repeated field deployments indicate increasing maturity of plume observations (TRL 4&ndash;5), with some diagnostic products approaching pre-operational capability. These findings suggest that further progress will depend not only on technical development but also on practical considerations such as deployment logistics, integration with existing systems, and operational evaluation. Overall, portable weather radar may provide an additional component of future multi-sensor wildfire intelligence systems, helping to bridge part of the observational gap between satellite remote sensing and fireground measurements while improving understanding of fire&ndash;atmosphere interactions.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2256</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2256/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140818</identifier>
    <datestamp>2026-05-13</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[C-CWatM v1.0: A high-resolution water resources and river routing model enabling direct linkage to state-of-the-art Earth-system and land‑surface models]]></dc:title>
      <dc:creator>Greve, Peter</dc:creator>
      <dc:creator>Schmitt, Amelie U.</dc:creator>
      <dc:creator>Schreiber, Sina Jasmin</dc:creator>
      <dc:creator>Clédat, Augustin</dc:creator>
      <dc:creator>Burek, Peter</dc:creator>
      <dc:description><![CDATA[River routing and human water management are often poorly represented in many Earth-system and land-surface models, not permitting consistent assessments of human-water-climate interactions. In this work, we introduce C-CWatM v1.0 (Climate-CWatM v1.0), a land-surface-driven version of the Community Water model (CWatM) that enables online and offline simulations of river routing, water resource availability, and management. The model operates on standard land-surface output and includes an OASIS3-MCT coupling interface, enabling efficient two-way coupling with Earth-system and land-surface models. In comparison to CWatM, all modules related to land-surface and snow processes have been removed to prevent conflicts with land-surface parameterisations implemented in the coupled models. C-CWatM also offers options for reducing-forcing requirements and simple on-the-fly bias correction using predefined quantile weights. We test C-CWatM in both online and offline settings and evaluate the model performance in offline mode using REMO output across a European domain. C-CWatM reproduces large-scale discharge patterns and hydrological gradients when using non-bias-corrected forcing data without calibration of model parameters. Calibration results in moderate improvements in model performance, while quantile-mapping-based bias correction of runoff significantly enhances model skill. A reduced-forcing version of the model enables rapid simulations based on available climate model output, as demonstrated using readily available EURO-CORDEX output. C-CWatM provides a novel and flexible hydrological and water resources modelling tool for representing river routing and water management in coupled modelling systems, enabling more integrated analyses of climate-water-human interactions.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2366</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2366/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140919</identifier>
    <datestamp>2026-05-13</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[Towards ground-to-space radiative closure in the mid- to far-infrared]]></dc:title>
      <dc:creator>Pery, Benedict</dc:creator>
      <dc:creator>Brindley, Helen</dc:creator>
      <dc:creator>Murray, Jonathan</dc:creator>
      <dc:creator>Mosselmans, Sophie</dc:creator>
      <dc:creator>Panditharatne, Sanjeevani</dc:creator>
      <dc:creator>Warwick, Laura</dc:creator>
      <dc:creator>Hogan, Robin</dc:creator>
      <dc:creator>Huang, Yi</dc:creator>
      <dc:creator>Riot-Bretêcher, Benjamin</dc:creator>
      <dc:creator>Oetjen, Hilke</dc:creator>
      <dc:creator>Schuettemeyer, Dirk</dc:creator>
      <dc:creator>L'Ecuyer, Tristan</dc:creator>
      <dc:description><![CDATA[Despite containing up to half of the Earth's thermal emission to space, the far-infrared spectral region (FIR, defined here as 100&ndash;667 cm<sup>-1</sup> or 15&ndash;100 &micro;m) has seldom been observed from satellites. This has contributed to substantial uncertainties in the spectroscopy of water vapour, radiative properties of clouds, and surface spectral emissivity; these in turn limit confidence in modelled FIR energy flows. With the advent of the Polar Radiant Energy in the Far-InfraRed Experiment (PREFIRE), a step is taken towards new, systematic, spectral observations of the Earth in the FIR. Launched in 2024, the two PREFIRE CubeSats offer a new perspective of Earth's outgoing longwave energy with moderate spectral resolution. However, the observational uncertainty budget requires further consolidation.</p> <p>In this study we assess the accuracy of PREFIRE spectral measurements through a &lsquo;ground-to-space&rsquo; closure experiment. Using zenith-viewing observations from the ground-based Far INfrarEd Spectrometer for Surface Emissivity (FINESSE), we gauge the representativity of atmospheric data from in situ sensors and reanalysis. With these data we simulate PREFIRE-observed radiances for an overflight of our field site in eastern Canada. Simulations of the FINESSE radiances are in very good agreement with observations, while those from PREFIRE indicate some bias beyond the calculated uncertainties. We find that atmospheric water vapour specification, uncertain surface properties, and instrument noise dominate the uncertainties. Based on these findings, we highlight proposed techniques for closure experiments using terrestrial and satellite instruments alike. Such experiments will provide a ground-truth for validation of future FIR satellite missions.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2443</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2443/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140922</identifier>
    <datestamp>2026-05-13</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 wintertime water vapor profiling by Raman lidar at Neumayer Station III, Antarctica: Characteristics of meridional moisture transport and assessment of ERA5 reanalysis]]></dc:title>
      <dc:creator>Jakob, Friederike</dc:creator>
      <dc:creator>Radenz, Martin</dc:creator>
      <dc:creator>Baars, Holger</dc:creator>
      <dc:creator>Seifert, Patric</dc:creator>
      <dc:creator>Engelmann, Ronny</dc:creator>
      <dc:description><![CDATA[The vertical distribution of water vapor is essential for understanding moisture transport toward Antarctica, which influences the surface mass balance of the ice sheets via precipitation, sublimation and longwave radiation effects. However, high-resolution vertical water vapor observations remain limited. In this study, we present continuous water vapor mixing ratio (WVMR) profiles obtained with Raman lidar at Neumayer Station III, Antarctica during wintertime (May to August) 2023. The observations reveal a mean WVMR of 0.7 gkg<sup>&minus;1</sup> and capture an exceptional moist air intrusion in early July with WVMR values reaching up to 3.9 gkg<sup>&minus;1</sup>. Two dominant synoptic patterns driving moisture advection toward the Antarctic coast could be identified, producing distinctly different vertical moisture structures. Pattern A, with a low-pressure system northwest of Neumayer Station III seems to be more effective in transporting moisture than a low-pressure system northeast of the Station (pattern B). The lidar measurements are compared to ERA5 reanalysis humidity fields. While ERA5 generally reproduces the moisture distribution reasonably well, it exhibits a dry bias of 0.1 gkg<sup>&minus;1</sup> (&asymp; 10 %) in the lower troposphere. Potential causes of the bias were investigated. The bias shows no clear dependence on the air mass source region, but is dependent on the assimilation cycle, synoptic conditions and the surface type representation in ERA5. These findings suggest that uncertainties in boundary layer mixing processes are a major contributor to the observed dry bias. The results highlight the value of continuous high-resolution water vapor profiling in understanding Antarctic moisture transport and validating reanalysis products.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2445</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2445/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140963</identifier>
    <datestamp>2026-05-13</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[Molecular characteristics and formation pathways of organosulfur compounds: a comparative field study across contrasting atmospheric environments]]></dc:title>
      <dc:creator>Cai, Dongmei</dc:creator>
      <dc:creator>Gong, Xianda</dc:creator>
      <dc:creator>Zhang, Ruiqi</dc:creator>
      <dc:creator>Zhang, Shenyan</dc:creator>
      <dc:creator>Cheng, Yuhan</dc:creator>
      <dc:creator>Rahaman, Saidur</dc:creator>
      <dc:creator>Fang, Yin</dc:creator>
      <dc:creator>Chen, Jianmin</dc:creator>
      <dc:description><![CDATA[Organosulfur compounds (OrgSs), especially organosulfates (OSs), are ubiquitous aerosol components. However, the spatial, seasonal, and diurnal variations of OrgS formation in polluted atmospheres remain poorly understood. Here, we monitored particulate OrgSs at an urban site and a suburban site in Shanghai and examined their molecular composition and formation pathways under contrasting atmospheric conditions. A total of 1964, 1914, and 2689 OrgS molecular formulas were detected in suburban summer, urban summer, and urban winter, respectively. More than 79 % of sulfur-containing molecular formulas had (4<em>s</em> + 3<em>n</em>)/o &le; 1, indicating that OrgSs were dominated by OSs and nitrooxy-OSs (NOSs). Compared with summer, wintertime OrgSs exhibited lower O/C ratios but higher double-bond equivalence and aromaticity, suggesting a stronger influence of anthropogenic emissions and more unsaturated molecular structures. Although OrgSs were mostly present in aliphatic molecular structures, an increase in the number of aromatic OSs in winter revealed an enhanced contribution from anthropogenic sources. Isoprene/monoterpene-derived OSs peaked during the daytime due to photochemical oxidation in summer, whereas monoterpene-derived NOSs were markedly enhanced at night via nighttime NO<sub>3</sub>-initiated oxidation. Non-metric multidimensional scaling analysis further revealed that OrgS composition in summer was associated with temperature and O<sub>3</sub> during the day but shifted toward RH-driven processing at night. In winter, inorganic nitrogen and sulfur species, aerosol liquid water content, and particle acidity became more important in shaping OrgS composition, suggesting enhanced aqueous-phase and acid-catalyzed formation. These findings provide molecular-level insights into the sources and formation of atmospheric OrgSs across contrasting environments.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2472</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2472/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140862</identifier>
    <datestamp>2026-05-13</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[Multi-Decadal Expansion of Potentially Dangerous Glacial Lakes in Central-Eastern Nepal (1992&ndash;2024): Remote Sensing Assessment and GLOF Hazard Implications]]></dc:title>
      <dc:creator>Ghimire, Ashok</dc:creator>
      <dc:creator>Manandhar, Susa</dc:creator>
      <dc:creator>Basnet, Tribikram</dc:creator>
      <dc:creator>Aryal, Kumar</dc:creator>
      <dc:creator>Dhital, Sushant</dc:creator>
      <dc:creator>Karki, Reshu</dc:creator>
      <dc:creator>Dhakal, Aakriti</dc:creator>
      <dc:creator>Krakauer, Nir</dc:creator>
      <dc:creator>Pradhananga, Dhiraj</dc:creator>
      <dc:description><![CDATA[Glacial lakes in the Himalayan regions are expanding rapidly under ongoing climate change, intensifying the risk of Glacial Lake Outburst Floods (GLOFs). This study quantifies multi-decadal area changes (1992&ndash;2024) in four Potentially Dangerous Glacial Lakes (PDGLs), Thulagi, Lumding Tsho, Hongu 2, and Lower Barun, located in central-eastern Nepal, using Landsat 5 and Landsat 8 satellite imagery processed within the Google Earth Engine (GEE) cloud platform. Lake boundaries were delineated from post-monsoon (October&ndash;November) median composites using the Normalized Difference Water Index (NDWI; threshold = 0.3), supplemented by manual delineation where topographic shadow conditions compromised automated extractions. Area uncertainties were computed using the standard half-pixel buffer method. Non-parametric Mann-Kendall trend tests with Sen&rsquo;s slope estimator were applied to all lake area time series to evaluate the statistical significance and rate of expansion. Sub-period regression analysis was used to assess acceleration in lake growth. Empirical area-volume scaling was applied to estimate changes in impounded water volume. All four lakes exhibited statistically significant, monotonically increasing area trends over the 32-year study period (Mann-Kendall tau = 1, p &lt; 0.001 for each lake). Lower Barun exhibited the highest expansion rate (Sen&rsquo;s slope = 0.063 km<sup>2</sup> yr<sup>-1</sup>), growing from 0.77 &plusmn; 0.053 km<sup>2</sup> in 1992 to 2.76 &plusmn; 0.13 km<sup>2</sup> in 2024 (a 258 % increase), with post-2010 expansion accelerating by a factor of 1.35. Lumding Tsho showed a strongly accelerating growth trajectory (R<sup>2</sup> = 0.96) with a post-2010 rate that more than doubled. The combined estimated additional water volume stored across all four lakes since 1992 approaches 608.6 &times; 10<sup>6</sup> m<sup>3</sup>, representing a GLOF hazard of exceptional and growing scale. The approach demonstrates a scalable and reproducible framework for long-term glacial lake monitoring and hazard assessment, applicable across data-sparse high mountain environment.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2402</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2402/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140956</identifier>
    <datestamp>2026-05-13</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[Subseasonal prediction of compound heat and drought events]]></dc:title>
      <dc:creator>Wu, Rachel Wai-Ying</dc:creator>
      <dc:creator>Büeler, Dominik</dc:creator>
      <dc:creator>Pyrina, Maria</dc:creator>
      <dc:creator>Day, Jonathan</dc:creator>
      <dc:creator>Imamovic, Adel</dc:creator>
      <dc:creator>Humphrey, Vincent</dc:creator>
      <dc:creator>Domeisen, Daniela I.V.</dc:creator>
      <dc:description><![CDATA[Compound heat and drought events have severe socio-economic impacts on human health, agriculture and electricity supply. While these compound extremes are projected to intensify under climate change, our understanding of their subseasonal predictability remains limited compared to that of individual heat or drought events. In this study, we evaluate the predictability of compound heat and drought events over Europe using the subseasonal prediction system of the European Centre for Medium-Range Weather Forecasts (ECMWF). We find that the physical coupling between heat and drought contributes up to 10 % towards an increase in forecast skill when heat and drought co-occur, relative to a baseline that assumes independence between extremes. However, in regions where the physical coupling between heat and drought via land-surface interaction is misrepresented, compound skill can be lower than when drought are predicted in isolation. These findings highlight the critical role of accurately simulating land-surface feedbacks to improve the reliability of the subseasonal prediction for compound extremes.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2465</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2465/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140191</identifier>
    <datestamp>2026-05-13</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[Measurement Report: Differences in cloud optical and microphysical properties in the Arctic and Antarctic derived using thermal infrared spectroscopy]]></dc:title>
      <dc:creator>Hung, Joseph</dc:creator>
      <dc:creator>Rowe, Penny M.</dc:creator>
      <dc:creator>Cox, Christopher J.</dc:creator>
      <dc:creator>McCullough, Emily M.</dc:creator>
      <dc:creator>Kroll, Liam</dc:creator>
      <dc:creator>Ottenheimer, Raia</dc:creator>
      <dc:creator>Shupe, Matthew D.</dc:creator>
      <dc:creator>Walden, Von P.</dc:creator>
      <dc:creator>Strong, Kimberly</dc:creator>
      <dc:description><![CDATA[Climate models struggle to accurately represent polar regions, largely due to the difficulty in modeling clouds. The uncertainty budget of polar radiation is dominated by cloud and cloud-aerosol interactions, but challenges in maintaining robust field observations mean that even basic knowledge such as cloud occurrence is not well known. Measurements of the thermal emission of Earth&rsquo;s atmosphere can help close this knowledge gap due to the sensitivity of this spectral region to radiative properties of clouds. Measurements of the downwelling atmospheric emission (400 to 3000 cm<sup>&minus;1</sup>) have been collected at two polar field sites using Atmospheric Emitted Radiance Interferometer (AERI) instruments, two at the Polar Environment Atmospheric Research Laboratory (PEARL) in Eureka, Canada (80&deg; N), for which we use data from 2006 to 2022, and another at McMurdo Station (77&deg; S) in Antarctica as part of the Atmospheric Radiation Measurement (ARM) West Antarctica Radiation Experiment (AWARE) project in 2016. We analyze these spectra, with supplementary data from other instruments and models, to compare optical and microphysical properties of moderately thick clouds at Eureka and McMurdo Station, including optical depth, thermodynamic phase, liquid droplet and ice crystal effective scattering radii, and cloud boundaries. We find that the clouds sampled at McMurdo generally feature lower temperatures, smaller liquid droplets, a more concentrated distribution of ice effective radii, less seasonal variability in optical depth, and lower optical thickness because they consist of a higher proportion of ice than those at Eureka. Additionally, both locations have high occurrence rates of supercooled liquid and mixed-phase clouds and exhibit differences between single-phase and mixed-phase microphysics.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1906</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1906/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139845</identifier>
    <datestamp>2026-05-13</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[Assessment of the impact of tropical anthropogenic and biomass-burning emissions on tropospheric ozone (2007&ndash;2021) using the GEOS-Chem model constrained by satellite observations]]></dc:title>
      <dc:creator>Narivelo, Herizo</dc:creator>
      <dc:creator>Sauvage, Bastien</dc:creator>
      <dc:creator>Boersma, Klaas Folkert</dc:creator>
      <dc:creator>Smedt, Isabelle</dc:creator>
      <dc:creator>Anglou, Isidora</dc:creator>
      <dc:creator>Roozendael, Michel</dc:creator>
      <dc:creator>Flochmoën, Eric</dc:creator>
      <dc:creator>Barret, Brice</dc:creator>
      <dc:description><![CDATA[Ozone (O<sub>3</sub>) is a secondary species formed and is considered a hazardous pollutant in the troposphere. Over the recent decades, tropospheric O<sub>3 </sub>has undergone significant regional variations. This paper focuses on the impact of the evolution of anthropogenic and biomass-burning emissions in the tropics upon tropospheric and the chemical regimes of O<sub>3</sub> using numerical simulations performed of the last 15-years with the GEOS-Chem model. Satellite datasets derived from OMI (HCHO and NO<sub>2</sub>) and IASI-SOFRID (CO and O<sub>3</sub>) are used as observational constraints to ensure the most reliable representation of BB and ANT emissions. The results show that the simulation (REF) combining GFAS for BB and CAMS for ANT emission provides the best match with the selected satellite observations.</p> <p>The analysis of REF-simulation shows that positive trends in tropospheric ozone column (TOC) are observed mainly in the Northern Hemisphere, in Asia regions, Temperate North America, Europe, and some tropical regions (Equatorial Asia and Southern Hemisphere South America), driven by increased of ANT and BB emissions and favourable photochemical conditions.</p> <p>Sensitivity tests with fixing emissions in the tropical band, reveal that the increase in tropical TOC is mainly due to tropical ANT emissions, which occur in chemical regimes nd: transparent by VOC-limited. Further results highlight that effective mitigation of future increases in TOC will depend mostly on control of ANT NOx emissions in tropical regions, where chemical conditions favour high O<sub>3</sub> production, while underlying the marginal role of BB in moderating regional O<sub>3 </sub>levels.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1652</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1652/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139741</identifier>
    <datestamp>2026-05-13</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[Towards high-fidelity simulations of coastal submesoscale baroclinic instabilities with MPAS-O (vE3SM3.0.0) Part I: Idealized experiments]]></dc:title>
      <dc:creator>Hinson, Kyle E.</dc:creator>
      <dc:creator>Schlichting, Dylan R.</dc:creator>
      <dc:creator>Hetland, Robert D.</dc:creator>
      <dc:creator>Engwirda, Darren</dc:creator>
      <dc:creator>Smith, Katherine M.</dc:creator>
      <dc:creator>Petersen, Mark R.</dc:creator>
      <dc:creator>Uyeda, Kaila</dc:creator>
      <dc:description><![CDATA[Rapid advances in computational power over the past decade have enabled global, kilometer-scale simulations that realistically represent open-ocean submesoscale dynamics. However, the ability of global ocean models to represent coastal submesoscale dynamics&mdash;where flows are more heterogeneous and strongly shaped by coastlines, bathymetry, and buoyancy inputs&mdash;remains largely unexplored. This study is the first of two companion papers assessing coastal submesoscale processes in MPAS-O, an unstructured global ocean model. Here, we present the first idealized evaluation of MPAS-O&rsquo;s representation of coastal submesoscale dynamics using observed conditions in the Mississippi&ndash;Atchafalaya (M-A) River plume as a template for initial conditions, and with the previously validated structured-grid regional model ROMS serving as a benchmark. We compare statistical metrics based on flow invariants&mdash;total strain, relative vorticity, and divergence&mdash;as well as velocity gradients in frontal coordinates, across horizontal resolutions ranging from 10 km to 100 m within an idealized model domain. We find that the representation of submesoscale baroclinic instabilities is highly similar across all resolutions such that the impact of model choice is smaller than the choice of spatial grid resolution. We also compare numerical and physical mixing between models using online diagnostics based on discrete variance decay. We find that ROMS generally has more numerical mixing and less physical mixing than MPAS-O across all resolutions. Trends in numerical mixing likely arise from MPAS-O's flux-corrected transport tracer advection scheme, which is shown to be anti-diffusive relative to the MPDATA scheme used in the ROMS simulations. Trends in physical mixing likely arise from differences in each model&rsquo;s configuration of the vertical mixing scheme (the K-Profile Parameterization). A companion paper extends this idealized model-model comparison to realistic simulations of the M-A River plume.]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1566</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1566/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:cp135599</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>cp</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[Limited early-industrial warming and strong volcanic imprints in the Caucasus: the first temperature reconstruction based on maximum latewood density]]></dc:title>
      <dc:creator>Dhyani, Rupesh</dc:creator>
      <dc:creator>Martin-Benito, Dario</dc:creator>
      <dc:creator>Verschuren, Louis</dc:creator>
      <dc:creator>Matskovsky, Vladimir</dc:creator>
      <dc:creator>Bulcke, Jan</dc:creator>
      <dc:creator>Doğan, Mehmet</dc:creator>
      <dc:creator>Kvaratskhelia, Revaz</dc:creator>
      <dc:creator>Köse, Nesibe</dc:creator>
      <dc:creator>Güner, Hüseyin Tuncay</dc:creator>
      <dc:creator>Schneider, Lea</dc:creator>
      <dc:description><![CDATA[<p>The Caucasus occupies a unique climatic region influenced by European, Mediterranean, and Asian circulation systems, yet it remains underrepresented in tree ring-based Northern Hemisphere temperature proxy networks. Here, we present the first summer temperature reconstruction for the Caucasus region based on maximum latewood density (MXD). We used X-ray micro-computed tomography of tree-ring samples from <i>Pinus sylvestris</i> growing at the upper tree line in the Lesser Caucasus and an ensemble nested regression approach to develop a robust 326 year-long June–September temperature reconstruction (1697–2022). The record explains – regionally unprecedented – 72 % of temperature variance during the instrumental period (1901–2022) and captures distinct interannual and multi-decadal variability including pronounced warming since the 1990s and a strong imprint of major volcanic eruptions. Temperatures in the second half of the 19th century were not significantly colder in the Caucasus than in the second half of the 20th century. The reconstruction highlights the exceptional magnitude and pace of 21st century warming in the region, which is without analogue at least in the past three centuries. Comparison with regional and large-scale temperature reconstructions reveals strong agreement within the Caucasus but negative correlations with Central Europe, indicating distinct temperature variability patterns across Europe and western Asia. Future work should focus on the climate dynamics behind this dipole and the extension of temperature-sensitive tree-ring records in the region.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/cp-22-989-2026</dc:identifier>
      <dc:identifier><![CDATA[https://cp.copernicus.org/articles/22/989/2026/]]></dc:identifier>
      <dc:source>eISSN: 1814-9332</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:cp132789</identifier>
    <datestamp>2026-05-13</datestamp>
    <setSpec>cp</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[Spatially contrasted response of Devonian anoxia  to astronomical forcing]]></dc:title>
      <dc:creator>Gérard, Justin</dc:creator>
      <dc:creator>Pohl, Alexandre</dc:creator>
      <dc:creator>Sablon, Loïc</dc:creator>
      <dc:creator>Huygh, Jarno</dc:creator>
      <dc:creator>Silva, Anne-Christine</dc:creator>
      <dc:creator>Crucifix, Michel</dc:creator>
      <dc:description><![CDATA[<p>The Devonian period, spanning from 419 to 359 million years ago, was marked by a warmer-than-present climate and recurring ocean anoxic events, with evidence increasingly suggesting a link between these events and astronomical forcing. Here, we explore how astronomical forcing influences ocean oxygenation by modulating the continental weathering flux of phosphate within a Late Devonian climate framework. To investigate this, we performed transient simulations spanning 1.1 Myr, crossing a 2.4 Myr eccentricity node using the cGENIE Earth system model. These simulations were driven by spatially resolved fluxes of reactive phosphorus from continents, computed using the emulator developed by <span class="cit" id="xref_text.1"><a href="#bib1.bibx76">Sablon et al.</a> (<a href="#bib1.bibx76">2025</a>)</span>, trained on GEOCLIM and HadSM3 outputs. Our results provide new evidence supporting eccentricity maxima as a driver of Late Devonian anoxic events. Additionally, global analysis reveals that obliquity variations can leave an imprint on global ocean oxygen levels via their influence on biological productivity, suggesting a potential pathway for obliquity-driven anoxia under greenhouse conditions. Regional analysis revealed pronounced spatial heterogeneity in the biogeochemical response to astronomical forcing. Local ocean circulation emerged as a critical factor in shaping these patterns. The simulations indicate that astronomical forcing can, through its impact on continental weathering fluxes, exert a dominant influence on ocean oxygenation, with regional oxygen concentrations varying by up to 35 % and driving changes in regional anoxic volume of up to 19 %. Finally, these findings help explain why proxy records from different locations may show divergent expressions of astronomical signals, potentially leading to contrasting interpretations of their role in driving ocean anoxia.</p>]]></dc:description>
      <dc:date>2026-05-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/cp-22-1003-2026</dc:identifier>
      <dc:identifier><![CDATA[https://cp.copernicus.org/articles/22/1003/2026/]]></dc:identifier>
      <dc:source>eISSN: 1814-9332</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:cp125562</identifier>
    <datestamp>2026-05-12</datestamp>
    <setSpec>cp</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[Climate change drove Late Miocene to Pliocene rise and fall of C4 vegetation at the crossroads of Africa and Eurasia (Anatolia, Türkiye)]]></dc:title>
      <dc:creator>Meijers, Maud J. M.</dc:creator>
      <dc:creator>Mikes, Tamás</dc:creator>
      <dc:creator>Rojay, Bora</dc:creator>
      <dc:creator>Çubukçu, H. Evren</dc:creator>
      <dc:creator>Aydar, Erkan</dc:creator>
      <dc:creator>Lüdecke, Tina</dc:creator>
      <dc:creator>Mulch, Andreas</dc:creator>
      <dc:description><![CDATA[<p>Life on Earth has been capitalizing on the C<span class="inline-formula"><sub>3</sub></span> photosynthetic pathway for 2.8 billion years. However, in the world's grasslands that emerged since the Paleogene, C<span class="inline-formula"><sub>4</sub></span> vegetation expanded dramatically between 8 and 3 Ma in response to climatic changes. Here we present the first comprehensive Late Miocene to Holocene <span class="inline-formula"><i>δ</i><sup>13</sup></span>C soil carbonate record from the Eastern Mediterranean region (Anatolia) to reconstruct long-term geographic distributions of C<span class="inline-formula"><sub>3</sub></span> and C<span class="inline-formula"><sub>4</sub></span> plants, a region with patchy records compared to parts of Africa and Asia. Our results show a colonization of Anatolian floodplains by C<span class="inline-formula"><sub>4</sub></span> biomass by 9.9 Ma, similar to regions in NW and E Africa, followed by a transition from this mixed C<span class="inline-formula"><sub>3</sub></span>–C<span class="inline-formula"><sub>4</sub></span> vegetation to C<span class="inline-formula"><sub>4</sub></span> dominance between ca. 7.1 and 4.9 Ma. The transition to C<span class="inline-formula"><sub>4</sub></span> in Anatolia coincides with a similar shift from C<span class="inline-formula"><sub>3</sub></span> to C<span class="inline-formula"><sub>4</sub></span> vegetation in southern Asia and is generally attributed to the Late Miocene Cooling in response to decreasing atmospheric <span class="inline-formula"><i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span>. However, the Anatolian paleoecosystem patterns are unique due to a rapid and permanent return to C<span class="inline-formula"><sub>3</sub></span> dominance in the Early Pliocene, which is not observed elsewhere and occurs simultaneously with the disappearance of the open environment-adapted large mammal Pikermian chronofauna. We propose that this return to C<span class="inline-formula"><sub>3</sub></span> vegetation was caused by paleoclimatic processes that regionally shifted precipitation from the warm to the cool season, resembling the modern Mediterranean climate. In conclusion, changes in rainfall seasonality under subhumid climate, rather than increased aridity, drove the demise of C<span class="inline-formula"><sub>4</sub></span>-dominated floodplains and the open-environment adapted Pikermian chronofauna at the Eurasian-African crossroads.</p>]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/cp-22-975-2026</dc:identifier>
      <dc:identifier><![CDATA[https://cp.copernicus.org/articles/22/975/2026/]]></dc:identifier>
      <dc:source>eISSN: 1814-9332</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg135815</identifier>
    <datestamp>2026-05-12</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[Subsurface dissolution reduces the efficiency of mineral-based open-ocean alkalinity enhancement]]></dc:title>
      <dc:creator>Burger, Friedrich A.</dc:creator>
      <dc:creator>Hofmann Elizondo, Urs</dc:creator>
      <dc:creator>Grosselindemann, Hendrik</dc:creator>
      <dc:creator>Frölicher, Thomas L.</dc:creator>
      <dc:description><![CDATA[<p>Carbon dioxide removal (CDR) from the atmosphere will likely be required to offset hard-to-abate emissions and limit global warming to well below 2 <span class="inline-formula">°C</span>, in line with the Paris Agreement. Among proposed CDR strategies, ocean alkalinity enhancement (OAE) is increasingly discussed because it offers high carbon sequestration potential, long storage timescales, and potentially mitigates ocean acidification. OAE is often envisioned to occur in the open ocean through the dissolution of alkaline mineral powders, such as forsterite, the most abundant form of olivine. Fine-grained powders dissolve near the surface, where the added alkalinity can efficiently enhance oceanic carbon uptake, whereas coarser grains sink and dissolve at depth. Most modeling studies assume complete surface dissolution, leaving the impact of subsurface dissolution on ocean carbon uptake poorly understood. Here, we develop idealized vertical mineral dissolution profiles that vary with environmental conditions and grain size. These profiles are implemented in a comprehensive Earth system model to assess the capture efficiency of OAE, defined as the additional carbon taken up by the ocean per alkalinity added. We find that the efficiency is very sensitive to grain size and may decrease by more than 75 % when grain size doubles, as larger grains release the alkalinity at deeper depth. Efficiency further decreases when particles are not uniformly sized but follow a particle size distribution with the same mean particle volume. In addition, efficiency is time-dependent: it is lower in the first decades of OAE and increases as alkalinity previously released in the ocean interior eventually resurfaces, often far from deployment sites. For forsterite particles with diameter 3.4 <span class="inline-formula">µm</span>, the efficiency is less than one-fourth of that achieved with surface alkalinity addition over the first decade, less than one-third over the first 30 years, and less than half over 175 years. Our results indicate that forsterite grain sizes would need to be around 1.7 <span class="inline-formula">µm</span> to achieve effective open-ocean alkalinity enhancement and that monitoring, reporting, and verification would be challenged by delayed and spatially dispersed carbon uptake, questioning the suitability of olivine. Minerals with faster dissolution rates may present more viable alternatives when mineral particle properties are closely controlled.</p>]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-3279-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/3279/2026/]]></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:egusphere139827</identifier>
    <datestamp>2026-05-12</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[Streamflow prediction in data-scarce regions with semi-supervised deep learning]]></dc:title>
      <dc:creator>Jia, Tianlong</dc:creator>
      <dc:creator>Chen, Guoding</dc:creator>
      <dc:creator>Li, Yao</dc:creator>
      <dc:creator>Chang, Xinyu</dc:creator>
      <dc:creator>Ehret, Uwe</dc:creator>
      <dc:description><![CDATA[Deep learning methods have demonstrated great performance in streamflow prediction. However, they typically require large amounts of "labeled" data for supervised learning (SL), including meteorological forcing data paired with corresponding streamflow observations. The data scarcity of streamflow observation limits application of SL models across hydrologically diverse regions worldwide. To address this issue, we propose a two-stage semi-supervised learning (SSL) for streamflow prediction in data-scarce regions, based on the Contrastive Predictive Coding (CPC) method. CPC is a self-supervised learning method, that learns data representations from "unlabeled" data (i.e., meteorological forcing time series without streamflow observations). In the first stage, CPC was used to pre-train an encoder and a Long Short-Term Memory (LSTM) network with a projection head, using a large number of meteorological sequences. In the second stage, we attached a linear layer to the pre-trained encoder and LSTM, and fine-tuned the entire model architecture for streamflow prediction, using labeled data. We developed and evaluated this approach for streamflow prediction in both regional models and single-basin models, using the CAMELS-DE dataset. We assessed the in-domain generalization performances of regional models on 1,265 basins in Germany, used to pre-train and fine-tune models. Moreover, we examined their zero-shot out-of-domain generalization performances, on additional 317 basins from CAMELS-DE, that were not involved in model training. We benchmarked our approach with a baseline SL-trained model. Our results show that the SSL regional models outperforms the SL baseline in both in-domain and zero-shot out-of-domain generalization performance for data-scarce conditions, when less than 10% of one-year labeled sequences are available. SSL models yield significant improvements in median Nash-Sutcliffe Efficiency (NSE) of 0.137 (in-domain) and 0.139 (out-of-domain), with 0.5% of one-year labeled data. Additionally, SSL enhances model ability to predict low flow and floods for data-scarce conditions, reducing the median percent bias of the bottom 30% low flow range (FLV) by 21.047 and the median Mean Absolute Percentage Error of peaks (MAPE<sub>peak</sub>) by 13.933 (out-of-domain), with 1% of one-year labeled data. This improved performance stems from the informative feature representations learned from meteorological forcing inputs though CPC pre-training, that enhances prediction ability across diverse basins under data-scarce conditions. Moreover, the advantages of SSL are more obvious for single-basin models when one-year labeled data is available. These results indicate a promising direction for leveraging SSL to develop hydrological foundation models, that have recently revolutionized artificial intelligence research. Hydrological foundation models involve pre-training on large-scale meteorological forcing datasets using self-supervised learning methods (e.g., CPC), and can be adapted to multiple hydrological tasks by model fine-tuning, e.g., simulation of water temperature and soil moisture.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1637</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1637/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139868</identifier>
    <datestamp>2026-05-12</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[Tracking organic compounds in smoke plumes using infrared satellite-based measurements]]></dc:title>
      <dc:creator>Juncosa Calahorrano, Julieta F.</dc:creator>
      <dc:creator>Millet, Dylan B.</dc:creator>
      <dc:creator>Wells, Kelley C.</dc:creator>
      <dc:creator>Hu, Chengyuan</dc:creator>
      <dc:creator>Brewer, Jared F.</dc:creator>
      <dc:creator>Payne, Vivienne H.</dc:creator>
      <dc:creator>Permar, Wade</dc:creator>
      <dc:creator>Hu, Lu</dc:creator>
      <dc:creator>Sullivan, Amy P.</dc:creator>
      <dc:creator>Ku, I.-Ting</dc:creator>
      <dc:creator>Fischer, Emily V.</dc:creator>
      <dc:creator>Selimovic, Vanessa</dc:creator>
      <dc:creator>Sekimoto, Kanako</dc:creator>
      <dc:creator>Lamplugh, Aaron</dc:creator>
      <dc:creator>Gkatzelis, Georgios</dc:creator>
      <dc:creator>Gilman, Jessica B.</dc:creator>
      <dc:creator>Coggon, Matthew</dc:creator>
      <dc:creator>Warneke, Carsten</dc:creator>
      <dc:description><![CDATA[We apply new measurements of methanol, ethene, ethyne, and HCN from the Cross-track Infrared Sounder (CrIS) to explore the quantitative use of satellite-based thermal infrared (IR) observations for fire studies. We focus analysis on the western U.S. during the 2018&ndash;2019 timeframes of two fire-focused aircraft campaigns, and use the GEOS-Chem model to guide interpretation. The CrIS data reveal large in-smoke enhancements and species:species correlations for targeted volatile organic compounds (VOCs), especially during the more active 2018 fire year. Spectral enhancements are strongest for methanol and ethene. For VOCs with similar vertical sensitivities the in-smoke correlations are height-independent and can be converted to column enhancement ratios without plume altitude information. For VOCs with dissimilar vertical sensitivities, spectral index correlations change coherently with altitude and may constrain injection or plume height changes. The mean (&plusmn; &sigma;) ethene:methanol ratio measured by CrIS across an ensemble of plumes (0.64 &plusmn; 0.24 mol/mol) matches bottom-up emission ratios (0.63 &plusmn; 0.08 mol/mol), but satellite-based and aircraft data both reveal greater variability than is predicted by GEOS-Chem. We propose that fire pyrolysis conditions are one driver of this variability and&nbsp; use in-situ data to show that near-field ethene:methanol ratios track pyrolysis conditions and hence inform the abundance of other emitted VOCs. Finally, we apply CrIS ethene:methanol ratios to estimate the high-temperature pyrolysis fraction for the same plume ensemble; the resulting fraction correlates with fire radiative power in a manner not well-captured by models.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1669</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1669/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139985</identifier>
    <datestamp>2026-05-12</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[Radar range dependent validation of spaceborne cloud profiling radar precipitation detection: lessons from CloudSat and the Canadian C band network for the EarthCARE era]]></dc:title>
      <dc:creator>Chishtie, Farrukh</dc:creator>
      <dc:description><![CDATA[Ground based validation of spaceborne precipitation detection algorithms depends critically on the quality of the reference radar observations, which degrades in a range dependent fashion due to ground clutter contamination and beam geometry effects. This study quantifies that dependence using five years (2006&ndash;2010) of coincident CloudSat Cloud Profiling Radar (CPR) overpasses and observations from the King City C band dual polarisation radar in southern Ontario, Canada, supplemented by automated and human METAR observations from twelve Environment and Climate Change Canada (ECCC) weather stations. Across 75,239 matched profiles, the CloudSat precipitation occurrence product achieves a probability of detection (POD) of 54.6 %, a critical success index (CSI) of 48.9 %, and a false alarm ratio (FAR) of 17.7 %. A systematic range bin decomposition reveals anomalously elevated Network Radar Precipitation (NRP) algorithm detection frequencies within 70 km of the King City radar, attributable to ground clutter passing the NRP 480 m vertical extent filter before Doppler discrimination becomes reliable. Excluding profiles within this range raises the POD to 66.8 % and the CSI to 56.3 %. Combining this range filter with the <em>Z</em><sub>CPR</sub> &gt; -10 dBZ threshold recommended for the Great Lakes winter precipitation regime further reduces the FAR to 13.8 % (CSI = 58.7 %). The 519 independent METAR comparisons yield a POD of 55.8 % and a low FAR of 9.2 %, confirming the radar based findings through a fully instrument independent pathway and demonstrating that the dominant CloudSat error mode is precipitation detection failure rather than false alarming. The performance degradation relative to the winter only benchmark of Hudak et al. (2008) is shown to arise primarily from near range clutter contamination and year round sampling rather than from algorithmic limitations. Critically, the 70 km threshold is governed by antenna beam geometry rather than radar wavelength and is therefore transferable to validation frameworks employing the new Canadian S band dual polarisation network. Implications for the design of ground validation campaigns for the recently launched EarthCARE Cloud Profiling Radar are discussed.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1753</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1753/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139974</identifier>
    <datestamp>2026-05-12</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[Molecular-Level Characterization of Urban Aerosol Analogues in Controlled Atmospheric Simulations]]></dc:title>
      <dc:creator>Marj, Elie</dc:creator>
      <dc:creator>Delater, Ambre</dc:creator>
      <dc:creator>Gratien, Aline</dc:creator>
      <dc:creator>Torrijos, Marie Line</dc:creator>
      <dc:creator>Macias Rodriguez, Juan Camilo</dc:creator>
      <dc:creator>Cazaunau, Mathieu</dc:creator>
      <dc:creator>Pangui, Edouard</dc:creator>
      <dc:creator>Bergé, Antonin</dc:creator>
      <dc:creator>Gaimoz, Cécile</dc:creator>
      <dc:creator>Bertin, Thomas</dc:creator>
      <dc:creator>Mebold, Emmanuelle</dc:creator>
      <dc:creator>Picquet-Varrault, Bénédicte</dc:creator>
      <dc:creator>Doussin, Jean-François</dc:creator>
      <dc:creator>Buissot, Clément</dc:creator>
      <dc:creator>Lanone, Sophie</dc:creator>
      <dc:creator>Coll, Patrice</dc:creator>
      <dc:description><![CDATA[Urban air pollution involves complex mixtures of gases and particulate matter whose molecular-level composition and gas-particle partitioning remain poorly characterized, limiting our understanding of secondary organic aerosol (SOA) formation. We address this gap using controlled atmospheric simulations combined with detailed molecular characterization.</p> <p>Two distinct urban atmospheric scenarios were simulated in the CESAM smog chamber: a standard urban (traffic emissions and biogenic precursors) and a biomass burning enhanced. Both scenarios were aged under controlled irradiation with NOx to simulate tropospheric photochemistry.</p> <p>PM<sub>1</sub> concentrations reached 15 &plusmn; 7 &micro;g.m<sup>-3</sup> for the standard scenario and 63 &plusmn; 24 &micro;g.m<sup>-3</sup> for the biomass burning scenario, with organic aerosol fractions of approximately 17 % and 40 %, respectively. Gas-phase analysis via proton-transfer-reaction time-of-flight mass spectrometry (PTR-TOF-MS) identified 23 volatile organic compounds (VOCs), dominated by oxygenated species (74&ndash;77 %). Particle-phase molecular analysis using ultrahigh-performance liquid chromatography electrospray ionization ion mobility quadrupole time-of-flight mass spectrometry (UPLC/ESI-IMS-QTOFMS) revealed 32 distinct compounds. The biomass burning scenario showed elevated source-specific tracers, including a levoglucosan isomer, nitrophenolic compounds (e.g., 3-methyl-4-nitrocatechol, 4-nitroguaiacol), and oxidized aromatics. Volatility distributions estimated via group contribution methods placed most compounds in the semi-volatile, low-volatility, and extremely low-volatility organic compound ranges (C* &lt; 300 &micro;g m<sup>-3</sup>), indicating substantial functionalization and partitioning.</p> <p>These results demonstrate the capacity of simulation chambers to generate reproducible urban aerosol analogues with distinct source-specific molecular signatures and well-characterized volatility distributions. This detailed molecular speciation provides a robust basis for process-oriented model evaluation and opens perspectives for systematic investigations of SOA formation pathways under controlled urban photochemical conditions.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1743</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1743/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140900</identifier>
    <datestamp>2026-05-12</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[Mineral dust concentration controlling convective cirrus structure and persistence: a large-eddy simulation study with observational constraints]]></dc:title>
      <dc:creator>Juurikkala, Kasper</dc:creator>
      <dc:creator>Raatikainen, Tomi</dc:creator>
      <dc:creator>Krämer, Martina</dc:creator>
      <dc:creator>Williamson, Christina J.</dc:creator>
      <dc:creator>Laaksonen, Ari</dc:creator>
      <dc:description><![CDATA[Dusty cirrus clouds are optically thick, convectively organized ice clouds that occur during intense mineral dust outbreaks. Previous modeling studies have found a link between mineral dust and convectively generated cirrus, but have been unable to explicitly resolve the associated convective dynamics due to limited spatial resolution. Here, we investigate the evolution and persistence of dusty cirrus using large-eddy simulations constrained by in-situ aircraft observations from the ML-CIRRUS 2014 campaign and complementary remote sensing data.<br />The simulations indicate that sustained convective cirrus requires mineral dust concentrations exceeding climatological values by approximately one to two orders of magnitude, corresponding to number concentrations on the order of N<sub>d </sub>&sim; 1 cm<sup>-3</sup>. Under these conditions, heterogeneous freezing on mineral dust dominates ice formation and maintains sufficiently high ice crystal number concentrations to sustain strong longwave cooling at cloud top and preserve convective overturning under shortwave radiative warming. In contrast, homogeneous freezing remains largely suppressed across a wide range of simulated conditions. The direct radiative effect of mineral dust is comparatively weak relative to cloud radiative feedbacks and does not significantly influence cirrus evolution.<br />The simulated cirrus is also highly sensitive to the choice of deposition ice nucleation parameterization, highlighting a major source of uncertainty in representing dust&ndash;ice interactions. Overall, the results identify mineral dust availability as the primary control on dusty cirrus persistence and emphasize the need for improved representation of heterogeneous ice nucleation in atmospheric models.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2427</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2427/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140796</identifier>
    <datestamp>2026-05-12</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[Reducing False Alarms in Small-Scale Slope Early Warning Systems via Deep Learning-Driven Asynchronous Displacement and Rainfall Data Fusion]]></dc:title>
      <dc:creator>Ouyang, Shubing</dc:creator>
      <dc:creator>Li, Daichao</dc:creator>
      <dc:creator>Liu, Minjiang</dc:creator>
      <dc:creator>Ge, Fengjian</dc:creator>
      <dc:creator>Zheng, Xia</dc:creator>
      <dc:creator>Li, Yuan</dc:creator>
      <dc:creator>Wu, Sheng</dc:creator>
      <dc:description><![CDATA[Real-time crackmeter-based warning systems for rainfall-induced small-scale slope failures suffer from prohibitively high false alarm rates. Across diverse geological settings, existing approaches relying on fixed thresholds or isolated rainfall&ndash;displacement relationships are highly sensitive to noise, lacking the robustness to reliably distinguish genuine deformation signals from spurious measurements. To address this operational bottleneck, this study reframes the early warning paradigm from a traditional fixed-threshold alerting process reliant on manual discrimination to an automated alert truth verification problem, proposing a real-time binary classification framework to isolate true early warnings from sensor-triggered false alarms. Utilizing a multi-source dataset of crackmeter displacement and rainfall measurements from diverse monitored slopes in Fujian Province, China, all true early warning instances were rigorously calibrated via field investigations. A patch-based dual-branch temporally-aware Transformer model was developed to explicitly address asynchronous multi-rate data fusion, strict temporal causality between rainfall and displacement, and stringent real-time decision constraints. By simultaneously capturing long-term rainfall-displacement interactions and high-resolution displacement dynamics, the model outperforms competitive baselines, achieving a precision of 90.91 %, a recall of 93.53 %, and an F2-score of 92.99 % in identifying true early warnings. Interpretability analysis reveals the model&rsquo;s decisions are primarily driven by localized displacement trends and relative rainfall intensity, aligning with expert judgment. The proposed framework significantly curtails false alarms without compromising reliability, acting as a robust decision-support layer to enhance automated slope hazard monitoring. Future work will fuse additional sensor types to suppress false alarms via cross-validation of multi-physical responses.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2352</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2352/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140870</identifier>
    <datestamp>2026-05-12</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[Statistical Assessment of the Representative Elementary Area for Areal Fracture Intensity (P21) in Digital Outcrop Models]]></dc:title>
      <dc:creator>Casiraghi, Stefano</dc:creator>
      <dc:creator>Bertacchi, Daniela</dc:creator>
      <dc:creator>Benedetti, Gabriele</dc:creator>
      <dc:creator>Mittempergher, Silvia</dc:creator>
      <dc:creator>Agliardi, Federico</dc:creator>
      <dc:creator>Martinelli, Mattia</dc:creator>
      <dc:creator>Bigoni, Francesco</dc:creator>
      <dc:creator>Albertini, Cristian</dc:creator>
      <dc:creator>Bistacchi, Andrea</dc:creator>
      <dc:description><![CDATA[The definition of a representative elementary volume (REV) or area (REA) for a target parameter is a fundamental step toward the upscaling of fracture network properties generated by discrete fracture network models (DFN) to an equivalent continuous medium for in situ applications in engineering geology, hydrogeology, and structural geology. The target parameter of this work is the areal fracture intensity (<em>P</em><sub>21</sub>), a key metric often used as a stopping criterion in stochastic DFN simulations, that is derived directly from surface data collected at natural outcrops. We propose a novel approach to define the REA as a range bounded by a lower and an upper limit. The upper limit, often overlooked but nonetheless theorized, identifies the largest representative domain, which is crucial for optimizing computational efficiency. We evaluate the REA range based on three statistical parameters, namely: the shape, mean, and variance of the <em>P</em><sub>21</sub> distributions obtained with progressively increasing scan area sizes. Each statistical parameter is assessed by combining formal statistical tests and diagnostic plots. Within a multi-parametric framework, the method enables a detailed analysis of the statistical behaviour of the dataset, supporting informed decisions in defining the REA range. The methodology is tested on two fractured limestone outcrops with markedly different characteristics: (i) an abandoned quarry in the Murge Plateau (Puglia, Italy) and (ii) the Lilstock Benches in the southern Bristol Channel basin.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2409</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2409/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140669</identifier>
    <datestamp>2026-05-12</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[Invited perspectives: Uncertainties in natural systems may be uncomfortable, but ignoring them would be absurd]]></dc:title>
      <dc:creator>Marzocchi, Warner</dc:creator>
      <dc:creator>Montanari, Alberto</dc:creator>
      <dc:creator>the RETURN-uncertainty task force</dc:creator>
      <dc:description><![CDATA[Uncertainties in natural systems are pervasive, varied, and unavoidable due to inherent open system complexity and limited knowledge. Therefore, the evolution of a natural system cannot be predicted deterministically and probabilistic forecasts are commonly used to account for these uncertainties. As the Voltaire-inspired title suggests, representing and quantifying all uncertainties in hazard and risk forecasting is difficult yet essential for an effective risk-cycle management and for a meaningful scientific evaluation of forecasting models. Although this paper focuses on hazard forecasting, we argue that the discussion and treatment of uncertainty apply equally to vulnerability and, therefore, to risk assessment. These challenges are reflected in the current absence of a common hierarchy of uncertainties, of a shared quantitative procedure to include all uncertainties in a forecast, and of effective communication and decision-making protocols, across different hazards and risks. Deepening the understanding of these distinct challenges has been the main goal of a dedicated task force of scientists from different disciplines, experts in communication, and decision-makers in the framework of a large Italian project on multirisk under NextGenEU funds &ndash; the RETURN project (<a href="https://www.fondazionereturn.it/en/" target="_blank" rel="noopener">https://www.fondazionereturn.it/en/</a>) &ndash; which includes eighteen Italian universities and research centers, the Italian Civil Protection Department, Italian State Railways, Assicurazioni Generali, other profit entities, and one Italian River Basin Authority. Within this initiative, we examined several examples of natural hazard forecasting and projections, from the perspectives of experts in various fields and/or users of these forecasts. The task force found that different hazards share key features and challenges regarding uncertainty understanding, quantification and communication, which may be embedded in a common framework. Such a framework would include a similar hierarchy of uncertainties that defines a complete hazard forecast, which is essential to properly evaluate forecasting models. This work categorizes the common key scientific and communication challenges, propose potential solutions, and intend to stimulate a deeper reflection on these issues.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2254</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2254/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140609</identifier>
    <datestamp>2026-05-12</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[Frequent occurrence of newly formed aerosol particles over wide geographical areas in the Arctic free troposphere and atmospheric boundary layer]]></dc:title>
      <dc:creator>Simon, David J.</dc:creator>
      <dc:creator>Schaefer, Jonas</dc:creator>
      <dc:creator>Hartmann, Jörg</dc:creator>
      <dc:creator>Kirbus, Benjamin</dc:creator>
      <dc:creator>Müller, Joshua</dc:creator>
      <dc:creator>Hartmann, Markus</dc:creator>
      <dc:creator>Wetzel, Bruno</dc:creator>
      <dc:creator>Köhler, Laura</dc:creator>
      <dc:creator>Jörss, Anna-Marie</dc:creator>
      <dc:creator>Weinhold, Kay</dc:creator>
      <dc:creator>Herber, Andreas</dc:creator>
      <dc:creator>Jurányi, Zsófia</dc:creator>
      <dc:creator>Henning, Silvia</dc:creator>
      <dc:creator>Roberts, Gregory C.</dc:creator>
      <dc:creator>Wendisch, Manfred</dc:creator>
      <dc:creator>Pöhlker, Mira L.</dc:creator>
      <dc:creator>Stratmann, Frank</dc:creator>
      <dc:description><![CDATA[New particle formation (NPF) can impact the Arctic radiative energy budget since this region is particularly sensitive to changes in aerosol particle and cloud condensation nuclei concentrations. Prior studies have predominantly investigated NPF in the Arctic atmospheric boundary layer (ABL), concluding that this phenomenon primarily takes place close to the surface. However, this study shows that NPF may take place throughout the entire lower Arctic troposphere. We have reached this conclusion by analyzing particle number size distribution data collected during a springtime aircraft campaign in the vicinity of Svalbard, the Fram Strait, and northern Greenland. We detected newly formed aerosol particles at various altitudes ranging from about 60 m to 3900 m and identified three atmospheric scenarios for their occurrence: newly formed particles in the free troposphere, in the ABL over sea ice, and in the vicinity of clouds. Our results suggest that regional Arctic atmospheric processes as well as long-range transport play key roles in the formation of new particles. Based on our data, we furthermore conclude that NPF may be a frequent and geographically extended phenomenon in the Arctic free troposphere.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2215</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2215/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140887</identifier>
    <datestamp>2026-05-12</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[Improved Dating of Landslides in Zimbabwe by Combining Satellite Multispectral and Synthetic Aperture Radar Observations]]></dc:title>
      <dc:creator>Noyes, Joanna</dc:creator>
      <dc:creator>Palmer, Steven</dc:creator>
      <dc:creator>Bennett, Georgina</dc:creator>
      <dc:creator>Kolusu, Seshagirirao</dc:creator>
      <dc:creator>Bain, Caroline</dc:creator>
      <dc:description><![CDATA[Accurate dating of landslides is essential for understanding triggering mechanisms and improving hazard analysis, yet many inventories lack precise event timing. This study presents a two-step methodology for dating existing inventories using multi-sensor satellite data and automated change-point detection implemented with the Ruptures Python package. In Step 1, extended time series of Sentinel-2 optical NDVI and the Bare Soil Index are analysed to estimate the approximate dates of landslides. Step 2 refines these estimates using Sentinel-1 SAR VV backscatter data within a six-month window centred on the results from Step 1. The approach is tested using a landslide inventory from Zimbabwe associated with Storm Idai in March 2019. Using the results from Step 2, 52.8 % of the dataset is dated, with 84.6 % accuracy (events correctly dated during the triggering storm event) and an average precision of 12.8 days (the dates between which the event occurred). The results demonstrate that combining optical and SAR satellite observations with automated change-point detection provides an effective method for retroactively dating landslides. This approach enables inventories to be dated with minimal prior knowledge of event timing or geometry, while avoiding the need for large datasets and high-performance computing resources. The code is made available in Google Earth Engine, allowing for wide application.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2418</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2418/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140586</identifier>
    <datestamp>2026-05-12</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[Permafrost conditions in peatlands govern riverine flushing of dissolved organic carbon, methylmercury, and nutrients]]></dc:title>
      <dc:creator>Mandour, Fares</dc:creator>
      <dc:creator>Greyeyes-Howell, Jazmin</dc:creator>
      <dc:creator>Shewan, Renae</dc:creator>
      <dc:creator>Thompson, Lauren</dc:creator>
      <dc:creator>Graham, Irene</dc:creator>
      <dc:creator>Low, Mike</dc:creator>
      <dc:creator>Munson, Matthew</dc:creator>
      <dc:creator>Connon, Ryan</dc:creator>
      <dc:creator>Cunada, Christopher</dc:creator>
      <dc:creator>Emmerton, Craig</dc:creator>
      <dc:creator>Olefeldt, David</dc:creator>
      <dc:description><![CDATA[Permafrost thaw and intensified droughts and floods threaten to alter the mobilization of dissolved organic carbon (DOC), nutrients and methylmercury (MeHg) from boreal peatlands, with cascading impacts on aquatic ecosystem functions and traditional food sources. Here we monitored 27 peatland-dominated (&gt;30 %) catchments in western Canada (150 to 52,000 km<sup>2</sup>) over a five-year period (2020 &ndash; 2024) which captured extreme hydroclimatic conditions. These catchments spanned a climatic and permafrost gradient (mean annual temperature -0.2 to -2.8 &deg;C), which provided a space-for-time framework to assess impacts of continued thaw and warming. Our results demonstrated that catchment climate, and thus permafrost conditions, strongly controlled the hydrological response of solute concentrations. Warmer catchments showed a pronounced flushing response where DOC and MeHg concentrations increased by 50 % and 80 %, respectively, as discharge increased from the 10th to 90th percentile. In contrast, colder catchments maintained a chemostatic response, where concentrations remained stable and low despite hydrological variability. Similar climate-hydrology interactions were found for total nitrogen, total phosphorous, and inorganic phosphorous, but not for inorganic nitrogen. It is likely that permafrost conditions in peatlands affect both the production of solutes and their hydrological connectivity to the stream network. The presence of permafrost in peatlands may act to both ensure connectivity during droughts but also preclude full connectivity during floods, yielding the observed patterns. Our findings suggest that ongoing peatland permafrost thaw will increase mobilization MeHg, DOC, and nutrients during high flow periods. This shift necessitates further monitoring to understand the long-term consequences for aquatic ecosystems and northern communities.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2199</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2199/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140508</identifier>
    <datestamp>2026-05-12</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[Development and Characterization of an Advanced Holographic Instrument for Atmospheric Research]]></dc:title>
      <dc:creator>Glienke, Susanne</dc:creator>
      <dc:creator>Bertschinger, Kevin L.</dc:creator>
      <dc:creator>Mei, Fan</dc:creator>
      <dc:creator>Shilling, John E.</dc:creator>
      <dc:description><![CDATA[In this study, we develop and characterize an advanced holographic instrument &mdash; HOLODROPS (HOLOgraphic DROPlet Sensor) &mdash; along with a complementary event-based Particle Image Velocimetry (ePIV) system. HOLODROPS operates in two configurations: (1) HOLODROPS, designed for long-term, high-precision measurements of cloud droplet size distributions, and (2) HOLODROPS-TRACK, designed for short-interval particle tracking to study turbulence and collision-coalescence processes. Unlike traditional optical scattering or imaging probes, both configurations can simultaneously capture the size, shape, and three-dimensional position of multiple droplets and ice crystals larger than 8.8 &micro;m within a sample volume, eliminating the need for multiple instruments and yielding more accurate and cohesive data. However, the detailed three-dimensional particle tracking provided by HOLODROPS-TRACK requires significant computational resources for hologram reconstruction and data processing, limiting its use over extended measurement periods. To address this challenge, we developed the ePIV system, which leverages an event-based camera to assess key cloud motion features in real time with substantially lower data volume and processing. By rapidly characterizing the flow conditions, ePIV identifies optimal measurement windows and informs targeted deployment of HOLODROPS-TRACK, paving the road for efficient, high-resolution particle tracking when conditions are most scientifically valuable. All three systems have been successfully characterized and validated in the laboratory. Additionally, we tested HOLODROPS successfully in an outdoor setting with a drizzle event.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2141</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2141/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140478</identifier>
    <datestamp>2026-05-12</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[Effect of vibration on the elastic modulus of compacted Antarctic snow near Zhongshan Station]]></dc:title>
      <dc:creator>Zhang, Fan</dc:creator>
      <dc:creator>Han, Tong</dc:creator>
      <dc:creator>Zhang, Qiming</dc:creator>
      <dc:creator>Wang, Hao</dc:creator>
      <dc:creator>Yin, Zhenxuan</dc:creator>
      <dc:creator>Wang, Yihe</dc:creator>
      <dc:creator>Hu, Biao</dc:creator>
      <dc:creator>Tang, Xueyuan</dc:creator>
      <dc:creator>Sun, Bo</dc:creator>
      <dc:creator>Xiao, Enzhao</dc:creator>
      <dc:description><![CDATA[As one of the fundamental mechanical properties of snow, the elastic modulus is critical to the design and construction of Antarctic snow runways and roads. While previous studies measured and investigated snow&rsquo;s elastic modulus through various experimental methods, the effects of vibratory treatment, a construction measure proven to enhance snow hardness, on the elastic modulus and the underlying mesoscale mechanism remain unexamined. This study investigates the vibration-induced effect on elastic modulus of compacted Antarctic snow near Zhongshan Station and the corresponding mesoscale mechanism. P-wave propagation experiments were conducted to measure the elastic modulus of vibrated and non-vibrated compacted Antarctic snow, and X-ray tomography imaging was employed to obtain the microstructures of vibrated and non-vibrated snow samples. Results show that for isothermal sintering of 48 hours at -10 &deg;C, vibratory treatment increases the elastic modulus by 83.13 % while maintaining the snow density of 0.6 g/cm&sup3; unchanged. At the mesoscale, vibratory treatment effectively homogenizes the pore space distribution within the ice matrix. Quantitative analysis revealed the following microstructural modifications: a 7.14 % decrease in the mean structure thickness accompanied by a 12.41 % reduction in the standard deviation, a 13.68 % decrease in the mean pore thickness with a more pronounced 30.43 % decline in the standard deviation, an 18.82 % elevation in the minimum cut density, and a 2.09 % enhancement in the directional connectivity. The findings provide theoretical support for rapid construction techniques of Antarctic snow runways and roads.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2115</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2115/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140402</identifier>
    <datestamp>2026-05-12</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[Influence of synoptic patterns (NAO vs. WeMO) on rainfall isotopic composition in SE Iberia: A machine learning approach]]></dc:title>
      <dc:creator>Stachnik, Artur</dc:creator>
      <dc:creator>Gázquez, Fernando</dc:creator>
      <dc:creator>Morales-González, Antonio Lope</dc:creator>
      <dc:creator>Morellón, Mario</dc:creator>
      <dc:creator>González-Ramón, Antonio</dc:creator>
      <dc:creator>Moral-Martos, Francisco</dc:creator>
      <dc:creator>Jiménez-Espinosa, Rosario</dc:creator>
      <dc:creator>Martín-Chivelet, Javier</dc:creator>
      <dc:description><![CDATA[Atmospheric circulation controls moisture transport across the western Mediterranean, but its seasonally resolved imprint on precipitation isotopes in many areas remains poorly understood, limiting the integration of circulation diagnostics with modern isotope monitoring. Southeastern Iberia constitutes an outstanding natural laboratory to identify and quantify the roles and isotopic footprint of the main modes of atmospheric variability in the region (i.e., the Western Mediterranean Oscillation (WeMO) and the North Atlantic Oscillation (NAO)) and other local factors, such as altitude and precipitation amount. Here, we combine a multi-altitude (560&ndash;1800 m a.s.l.) precipitation-isotope network in Sierra de Segura, a mountain range located in SE Spain with explainable machine-learning methods to quantify how large-scale circulation and precipitation regime control rainfall isotopic composition.</p> <p>First we extend the WeMO index forward from 2020, when instrumental measurements end, to 2025 using a physically constrained XGBoost reconstruction based on regional sea-level pressure predictors from San Fernando (Spain) and multiple northern Italian stations, reproducing the published index over 2010&ndash;2020 with robust cross-validated performance (R&sup2; = 0.85 &plusmn; 0.05; RMSE = 0.41 &plusmn; 0.07, n = 129 months). Then we analyze 448 rainwater samples collected between 2017 and 2023, aggregated into 154 precipitation-weighted monthly observations of &delta;&sup1;⁸O, &delta;&sup2;H and &delta;&sup1;⁷O, together with d-excess and &sup1;⁷O-excess. Bulk isotope ratios co-vary strongly (&rho; &gt; 0.95), allowing &delta;&sup1;⁸O to represent the dominant network-scale signal.</p> <p>Random Forest models interpreted using SHAP reveal a clear seasonal reorganization of controls. During the wet season (October&ndash;March), &delta;&sup1;⁸O variability is primarily circulation-driven, with the North Atlantic Oscillation acting as the dominant control and the WeMO providing a consistent secondary modulation. In contrast, during the dry season (April&ndash;September), &delta;&sup1;⁸O is governed by precipitation regime, with precipitation amount overwhelmingly predominating over circulation indices and exhibiting a strongly non-linear, amount-effect response. Back-trajectory clustering of regionally coherent isotope-sampling events supports these contrasting seasonal influences, indicating a small number of recurrent synoptic transport regimes in winter and weaker synoptic organization in summer.</p> <p>Overall, these results provide a transferable, seasonally calibration that links synoptic circulation and precipitation regime to rainfall &delta;&sup1;⁸O (and excess parameters) in southeastern Iberia. This innovative framework enables robust interpretation of Mediterranean isotope-based paleoclimate archives by distinguishing circulation-driven wet-season signals from precipitation-regime-driven dry-season variability. It is readily applicable to other climatically complex areas influenced by multiple modes of atmospheric variability and pronounced seasonal contrasts. Furthermore, our results provide a basis for assessing the sensitivity of cave and lake systems to future changes in circulation persistence and rainfall intermittency under ongoing climate change.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2058</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2058/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140333</identifier>
    <datestamp>2026-05-12</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 2024 cascading glacial lake outburst flood in the Thame Valley of Everest region, Nepal: process, impacts and implications]]></dc:title>
      <dc:creator>Khadka, Nitesh</dc:creator>
      <dc:creator>Pandey, Vishnu Prasad</dc:creator>
      <dc:creator>Watson, C. Scott</dc:creator>
      <dc:creator>Zheng, Guoxiong</dc:creator>
      <dc:creator>Wu, Tianpei</dc:creator>
      <dc:creator>Sharma, Keshab</dc:creator>
      <dc:creator>Rawlins, Lauren D.</dc:creator>
      <dc:creator>Allen, Simon</dc:creator>
      <dc:creator>Gouli, Manish Raj</dc:creator>
      <dc:creator>Shrestha, Dibas</dc:creator>
      <dc:description><![CDATA[On the afternoon of 16 August 2024, a catastrophic flood devastated Thame Village in the Everest region of Nepal. This event resulted from a cascading glacial lake outburst flood (GLOF), where the outburst of an upstream glacial lake triggered the failure of a downstream lake in the headwaters&mdash;a complex hazard chain often-overlooked in conventional risk assessments. By integrating multi-source satellite imagery, field data, climatic data, empirical estimations, and numerical modelling, we analyse the triggers, processes, and consequences of the cascading failure. We find that the upper lake, which formed in the late 2000s, expanded rapidly to 0.11 km&sup2; prior to its outburst, while the lower lake grew by 20 % between 1989 and 2024. The hydrological tipping point for the upper lake was driven by intense glacier melt and calving from extreme temperatures and precipitation. Its overtopping triggered a cascade, causing the breach of the lower lake&rsquo;s moraine dam and releasing a combined water volume of approximately 6 (&plusmn; 0.65) &times;10⁵ m&sup3;. Multi-phase mass flow modelling reconstructing two possible scenarios indicates that the flood wave, with an initial peak discharge exceeding 800 m&sup3;/s, reached Thame Village within 22 to 32 minutes. The socio-economic impact was severe, with losses estimated at 6.18 million USD within the Khumbu Pasang Lhamu Rural Municipality alone, and flood effects traced over 50 km downstream. This event demonstrates that small, rapidly evolving glacial lakes, conditioned by climate-induced glacier retreat, can generate devastatingly powerful GLOFs. This underscores a critical need to broaden GLOF risk assessments to include such small lakes and to prioritize reducing exposure and vulnerability in dynamic high-mountain communities over solely engineering-based hazard control.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2011</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2011/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140304</identifier>
    <datestamp>2026-05-12</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[Equation discovery for climate impact: emulating impact models for unexplored climate scenario with interpretable symbolic regression]]></dc:title>
      <dc:creator>Roux, Erwan</dc:creator>
      <dc:creator>Tandeo, Pierre</dc:creator>
      <dc:creator>Granero Belinchon, Carlos</dc:creator>
      <dc:creator>Baklouti, Melika</dc:creator>
      <dc:creator>Sommer, Julien</dc:creator>
      <dc:creator>Sevault, Florence</dc:creator>
      <dc:creator>Somot, Samuel</dc:creator>
      <dc:creator>Doury, Antoine</dc:creator>
      <dc:creator>Najar, Mahmoud</dc:creator>
      <dc:description><![CDATA[Projected impacts of climate change are assessed with impact models, such as ecological or hydrological models, driven by climate projections. Uncertainties of projected impacts are estimated by driving impact models with a large ensemble of plausible future climate projections. However, most of the time, this is not possible for practical reasons: computing time, data availability. To fix this issue, we propose an approach that links climate projections to impacts with an interpretable equation. First, this equation is discovered based on simulations of the impact model and their corresponding climate projections. Then, we consider that this equation can be used to emulate the impact model for other climate projections. Specifically, the discovered equation maps each year climate indicators, i.e. a list of yearly and seasonally-averaged climate model variables, to a yearly-averaged impact indicator, i.e. a variable computed from the impact model outputs. In our application, the impact indicator is the annual mean Net Primary Production (NPP) of a risk-relevant regional oceanic area located in the North-Western Mediterranean basin. It is computed from the outputs of a biogeochemical model of the Mediterranean Sea, which is driven by climate projections of a coupled regional climate model of the Mediterranean area. In our methodology, we run nine validation schemes each one providing one equation to predict this impact indicator. Our results show that all discovered equations are linear, even though non-linearity is allowed, and that most of them contain four climate indicators that can be interpreted physically: the sea surface temperatures in winter and spring, the sea surface salinity in spring, and the net downward shortwave flux in winter. Based on these four indicators, we fit a linear equation on the historical period (1986&ndash;2005) and the scenario RCP8.5 (2006&ndash;2099) that reproduces well the trend and the year-to-year correlation of the impact indicator for the scenario RCP4.5 (2006&ndash;2099), which was not used for the fit. The predictions of the linear equation however underestimate the interannual variance of NPP. As a perspective, this equation allows us to approximate the impact indicator at a neglected computational cost, i.e. without running the costly biogeochemical impact model, for any regional climate model outputs available.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1991</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1991/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140291</identifier>
    <datestamp>2026-05-12</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[Physically Anchored Multi-Resolution Neural Operator Framework for Flood Inundation Prediction]]></dc:title>
      <dc:creator>Behroozi, Abdolmehdi</dc:creator>
      <dc:creator>Lawson, Kathryn</dc:creator>
      <dc:creator>Shen, Chaopeng</dc:creator>
      <dc:description><![CDATA[Accurate flood inundation modeling using high-resolution hydrodynamic simulations is computationally demanding, limiting their use for large-scale analysis and rapid scenario evaluation. Although machine learning surrogates have been developed, many struggle to reproduce the full spatiotemporal evolution of flood dynamics while maintaining physical consistency across spatial scales. In particular, simultaneously capturing basin-scale wave propagation and fine-scale inundation boundaries remains challenging. This study presents a multi-resolution deep learning framework for dynamic flood prediction. The approach combines a coarse-resolution neural operator that captures large-scale hydrodynamic behavior with a terrain-aware refinement module that reconstructs a fine-scale boundary structure. The framework is trained on high-fidelity two-dimensional shallow-water simulations and evaluated across riverine, dam-break, and complex floodplain systems, including tests under structured bathymetric uncertainty. Results demonstrate accurate reconstruction of continuous water depth fields, wet-dry delineation, and peak flow magnitude and timing. The model preserves the evolution of domain-integrated water volume over time, ensuring physically consistent mass dynamics rather than purely geometric agreement, and maintains probabilistic consistency when input topography is uncertain. The framework, therefore, provides high-resolution flood predictions at substantially reduced computational cost relative to direct high-resolution simulation. These findings show that multi-resolution deep learning can approximate hydrodynamic flood processes with strong physical fidelity and robustness to geometric uncertainty, supporting scalable flood hazard assessment and rapid predictive modeling.]]></dc:description>
      <dc:date>2026-05-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1982</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1982/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <resumptionToken expirationDate="%2026-%05-%16GMT%GMT0" completeListSize="129608" cursor="0">69175258</resumptionToken>
 </ListRecords>
</OAI-PMH>
