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    <identifier>oai:publications.copernicus.org:wcd129324</identifier>
    <datestamp>2026-03-06</datestamp>
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      <dc:title><![CDATA[Concurrent heat waves and their linkage to large-scale meridional heat transports through planetary-scale waves]]></dc:title>
      <dc:creator>Lembo, Valerio</dc:creator>
      <dc:creator>Messori, Gabriele</dc:creator>
      <dc:creator>Faranda, Davide</dc:creator>
      <dc:creator>Galfi, Vera Melinda</dc:creator>
      <dc:creator>Graversen, Rune Grand</dc:creator>
      <dc:creator>Pons, Flavio Emanuele</dc:creator>
      <dc:description><![CDATA[<p>We investigate concurrent heatwaves across the Northern Hemisphere through the linkage between extremes in Meridional Heat Transport (MHT) and in hemispheric land surface temperature (LST). MHT provides fundamental insight on how large-scale thermodynamics links to atmospheric large-scale dynamics, especially through the action of the eddy planetary-scale circulation in the mid-latitudes. The phase and amplitude of these waves can in fact favor the simultaneous occurrence of heatwaves in remote regions, but how this relates to the amount of heat carried by them has not yet been discussed. In this work, we find that the conditional occurrence of extremely weak MHT and extremely warm hemispheric LSTs is significantly more frequent than other conditional occurrences, both in Summer (JJA) and in Winter (DJF). We argue that the combination of extremely weak, in some cases equatorward, MHTs and warm LSTs in JJA are associated with the reversal of the MHT contribution by zonal wavenumber 3, which is in turn associated with the frequency of atmospheric blocking in western Eurasia and the intensity of blockings and jet stream over the Northwestern Pacific. In DJF, the weak, albeit never equatorward, MHT – warm LST events are characterized by a suppression of the climatologically dominant wavenumber 2, which weakens the overall MHT. The flow is anomalously zonal across much of North America and Eurasia, with reduced frequency of atmospheric blockings and downstream displacement of the jet stream, advecting moist and mild air eastward into the continents. Overall, such dynamical pattern correspond to abnormally warm and widespread temperatures in North America, Eastern Europe, and China. The conditional occurrence of extremely weak MHTs and warm hemispheric LSTs is found to be related to between 30 % and over 40 % of extremely warm hemispheric LST days in both seasons.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/wcd-7-453-2026</dc:identifier>
      <dc:identifier><![CDATA[https://wcd.copernicus.org/articles/7/453/2026/]]></dc:identifier>
      <dc:source>eISSN: 2698-4016</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:mrd139120</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>mrd</setSpec>
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      <dc:title><![CDATA[An Order of Magnitude Signal-to-Noise Improvement of Magnetic Resonance Spectra using a Segmented-Overlap Fourier-Filtering and Averaging (SOFFA) Approach]]></dc:title>
      <dc:creator>Sidabras, Jason W.</dc:creator>
      <dc:description><![CDATA[Segmented-Overlap Fourier-Filtering and Averaging (SOFFA) data acquisition method is described in detail for magnetic resonance spectroscopy. In this work the four processes that encompass the SOFFA data acquisition method are detailed: (i) oversampling spectral segments, (ii) Fourier block-filtering, (iii) segment-overlap averaging, and (iv) decimation. Three experimental examples are shown. Conventional Continuous Wave (CW) Electron Paramagnetic Resonance (EPR) is compared to SOFFA-CW of a single reduced [4Fe-4S]<sup>+</sup> (S=1/2) at concentrations of 1 mM, 100 &micro;M, and 10 &micro;M showing an average increase in concentration sensitivity by a factor of 5.6. Experimental comparison of CW and SOFFA nonadiabatic rapid scan (SOFFA-NARS) data with similar filter parameters and field-modulation amplitude demonstrates a factor of 10.3 in signal-to-noise improvement for a 150 &micro;M sitedirected spin-labeled Hemoglobin in 82 % glycerol at 18 &deg;C. The signal-to-noise improvements were made for the same data acquisition times on standard commercial instruments. This method can be implemented to perform real-time segmented processing and, combined with more sophisticated averaging methods, will push the state-of-the-art sensitivity in magnetic resonance spectroscopy.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/mr-2026-6</dc:identifier>
      <dc:identifier><![CDATA[https://mr.copernicus.org/preprints/mr-2026-6/]]></dc:identifier>
      <dc:source>eISSN: 2699-0016</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:gmd130849</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Assessing seasonal climate predictability using  a deep learning application: NN4CAST]]></dc:title>
      <dc:creator>Galván Fraile, Víctor</dc:creator>
      <dc:creator>Rodríguez-Fonseca, Belén</dc:creator>
      <dc:creator>Polo, Irene</dc:creator>
      <dc:creator>Martín-Rey, Marta</dc:creator>
      <dc:creator>Moreno-García, María N.</dc:creator>
      <dc:description><![CDATA[<p>Seasonal climate predictions are essential for climate services, with changes in tropical sea surface temperature (SST) representing the most influential oceanic drivers. SST anomalies can affect the climate in remote regions through various atmospheric teleconnection mechanisms, and the persistence/evolution of those SST anomalies can give seasonal predictability to atmospheric signals. Dynamical models often struggle with biases and low signal-to-noise ratios, making statistical methods a valuable alternative. Deep learning models are currently providing accurate predictions, mainly in short-range weather forecasts. Nevertheless, the black-box nature of this methodology makes it necessary to ensure its explainability. In this context, we present NN4CAST (Neural Network foreCAST), a Python deep learning pipeline designed to assess seasonal predictability, with built-in tools for evaluating model skill and performing basic spatial diagnostics based on empirical orthogonal functions. Starting from the raw datasets, NN4CAST performs all methodological steps: preprocessing, training and evaluation, enabling researchers to rapidly explore the predictability of a target variable and identify its main potential drivers. This flexible framework allows for the quick testing of predictive skill from different sources of predictability, making it a valuable asset for climate services. Although NN4CAST can use different variables to feed the model, we illustrate its application to reproduce tropical and extratropical teleconnections by training the model with Pacific SST anomalies. We show that NN4CAST can provide skilful predictions across timescales, from modelling variables at lag 0 that capture observed relationships to producing seasonal forecasts at longer leads, both in regions with linear SST-atmosphere coupling (tropics) and in highly non-linear remote regions (such as Europe). Two key examples are the prediction of SST anomalies in the tropical Atlantic region during boreal spring from previous winter SSTs, and the modelling  of precipitation anomalies over the European continent in boreal fall from the contemporaneous Pacific SSTs. The former exemplifies a predominantly linear ENSO-Tropical North Atlantic teleconnection, whereas the latter involves a highly non-linear and non-stationary ENSO-Euro-Atlantic teleconnection. Our results demonstrates NN4CAST's potential to determine and quantify the influence of specific potential drivers on a target variable, offering a useful tool for improving climate predictability assessments. NN4CAST enables the attribution of predictions to specific input features, helping to identify the relative importance of different sources of predictability over time and space. In summary, NN4CAST offers a powerful framework to better characterize and understand the complex, non-linear and non-stationary remote climate interactions.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-1917-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/1917/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:essdd138997</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[UK-Flow15 Part 1: Development of a coherent national-scale 15-min flow dataset]]></dc:title>
      <dc:creator>Fileni, Felipe</dc:creator>
      <dc:creator>Fowler, Hayley J.</dc:creator>
      <dc:creator>Lewis, Elizabeth</dc:creator>
      <dc:creator>Fry, Matt</dc:creator>
      <dc:creator>Cooper, Hollie</dc:creator>
      <dc:creator>Swain, Ollie</dc:creator>
      <dc:creator>McLay, Fiona</dc:creator>
      <dc:creator>Coxon, Gemma</dc:creator>
      <dc:creator>Bruce, Emma</dc:creator>
      <dc:creator>Yang, Longzhi</dc:creator>
      <dc:creator>Archer, David</dc:creator>
      <dc:description><![CDATA[High-resolution river flow data is essential for modelling flood dynamics and assessing hydrological change. In the UK, there are a wealth of sub-daily flow records that have been collected for more than 70 years. However, they remain scattered across multiple agencies and lack consistent quality assurance, limiting their use for large-sample and national-scale analysis. This paper presents UK-Flow15, a quality-controlled, 15-min, national scale, flow dataset for the UK, based on records from over 1,300 gauging stations and more than 1.8 billion observations. Data were collected via APIs and in conjunction with UK measuring authorities, then compiled into a single national dataset. Duplicate timestamps and inconsistencies in temporal resolution were systematically identified and resolved using a combination of automated filters and manual review. A comprehensive quality-control framework, specifically tailored for the dataset, was then applied to identify and document data anomalies; the full methodological development and evaluation of this framework are presented in the companion paper of this series. The final dataset is accompanied by transparent documentation of flagged issues and a suite of metadata files detailing data resolution, QC outcomes, and all processing decisions to support traceability and user interpretation. We demonstrate the dataset&rsquo;s utility through a practical case study by systematic removal of unreliable data, interpolation of anomalous spikes, and manual verification of significant high-flow and truncation events. These steps illustrate how the dataset can be effectively curated for detailed hydrological research and operational applications. This publicly accessible, robust, and transparent dataset significantly enhances capabilities for sub-daily hydrological research in the UK, offering essential resources for improved flood prediction, management strategies, and policymaking.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-152</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-152/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:cp131019</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>cp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Wine must yields as indicators of May to July climate in Central Europe, 1416–1988]]></dc:title>
      <dc:creator>Pfister, Christian</dc:creator>
      <dc:creator>Brönnimann, Stefan</dc:creator>
      <dc:creator>Litzenburger, Laurent</dc:creator>
      <dc:creator>Thejll, Peter</dc:creator>
      <dc:creator>Altwegg, Andres</dc:creator>
      <dc:creator>Brázdil, Rudolf</dc:creator>
      <dc:creator>Kiss, Andrea</dc:creator>
      <dc:creator>Landsteiner, Erich</dc:creator>
      <dc:creator>Ljungqvist, Fredrik Charpentier</dc:creator>
      <dc:creator>Pliemon, Thomas</dc:creator>
      <dc:description><![CDATA[<p>The paper explores to which extent narrative documentary records on wine production in Central Europe can be used as a proxy for summer temperatures. Here, we compiled 11 regional series spanning from the early 15th century to 1988. We detrended the data to adjust for long-term biases such as warfare-related population decline. The homogenised regional series were subsequently merged into three supra-regional series: (1) the Mosel series, starting in 1416 and consisting of data from the former city-republic of Metz (France) and the Grand Duchy of Luxembourg; (2) the series for Germany, starting in 1511 and mainly originating from the former city-state of Heilbronn; and (3) the third series, starting in 1529 and representing production on the Swiss Plateau. The residuals of the supra-regional yield series were averaged, divided into seven classes, and multiplied by five quality classes. Yield quality indices (YQI) varying between 35 (large and excellent) and 1 (small and undrinkable) significantly correlated with temperatures between May and July. Regression analysis of the composite series revealed that yield and quality primarily depend on the climate conditions from May to July as well as on those in June of the previous year. Crops with a YQI <span class="inline-formula">&gt;</span> 28 (rated “good” by traditional winegrowers) were related to above-average May–July temperatures, early grape harvest dates and high tree-ring maximum latewood density values resulting from frequent anticyclonic weather situations. Crops with YQI <span class="inline-formula">&gt;</span> 10 could not be uncritically assigned to cold summers since severe winter conditions, and spring frosts sometimes substantially reduced yields without affecting quality, particularly during the Little Ice Age in the marginal Mosel and German areas. Extreme yield fluctuations challenged winegrowing communities. Overproduction induced wastefulness, while crop failures sometimes triggered witch hunts.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/cp-22-541-2026</dc:identifier>
      <dc:identifier><![CDATA[https://cp.copernicus.org/articles/22/541/2026/]]></dc:identifier>
      <dc:source>eISSN: 1814-9332</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:os129145</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>os</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Tracking marine debris in Northwest Spain: assessing wind influence with a Lagrangian transport model]]></dc:title>
      <dc:creator>Rial-Osorio, Martiño</dc:creator>
      <dc:creator>Pérez-Muñuzuri, Vicente</dc:creator>
      <dc:creator>Cloux, Sara</dc:creator>
      <dc:description><![CDATA[<p>Marine debris is responsible for major problems in our oceans, causing serious environmental degradation, detrimental health effects and economic losses in sectors related to the marine environment. In this work, we examine how plastics released by the Ulla river at the estuary's extreme affect the transport, accumulation, and beaching of floating particles in the Ría de Arousa, an estuary on the northwest coast of the Iberian Peninsula, as a result of wind force. Using Lagrangian simulations of particle tracking under different wind drag coefficients (1 %, 3 % and 5 %), we evaluate the spatial and seasonal patterns of particle concentration, residence time and deposition on the coast. Our results show that wind plays a crucial role in modulating particle behavior. Low wind-driven conditions favor greater near-shore accumulation and longer residence times, especially in the northern and inner regions of the estuary. As wind influence increases, particle dispersion intensifies, leading to lower overall accumulation and weakening of correlations between river discharge and coastal deposition. Seasonal differences are also studied, with higher concentrations observed in the north during winter and in the south during summer.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-777-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/777/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:os133225</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>os</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Iron isotope insights into equatorial Pacific biogeochemistry]]></dc:title>
      <dc:creator>Camin, Capucine</dc:creator>
      <dc:creator>Labatut, Marie</dc:creator>
      <dc:creator>Pradoux, Catherine</dc:creator>
      <dc:creator>Murray, James W.</dc:creator>
      <dc:creator>Lacan, François</dc:creator>
      <dc:description><![CDATA[<p>The EUCFe cruise (RV <i>Kilo Moana</i>, 2006) was designed to characterize sources of Fe to the western equatorial Pacific and its transport by the Equatorial Undercurrent (EUC), a narrow and fast eastward current flowing along the equator, to the eastern equatorial Pacific High Nutrient Low Chlorophyll (HNLC) region. This study presents seawater dissolved (DFe) and particulate (PFe) iron concentrations and isotopic compositions (<span class="inline-formula"><i>δ</i><sup>56</sup></span>DFe and <span class="inline-formula"><i>δ</i><sup>56</sup></span>PFe) from 15 stations in the equatorial band (2° N–2° S) between Papua New Guinea and 140° W, over more than 8500 km along the equator and in the upper 1000 m of the water column.</p>        <p><span class="inline-formula"><i>δ</i><sup>56</sup></span>DFe and <span class="inline-formula"><i>δ</i><sup>56</sup></span>PFe ranged from <span class="inline-formula">−0.22</span> ‰ to <span class="inline-formula">+</span>0.79 <span class="inline-formula">±</span> 0.07 ‰ and from <span class="inline-formula">−0.52</span> ‰ to <span class="inline-formula">+</span>0.43 <span class="inline-formula">±</span> 0.07 ‰, respectively (relative to IRMM-14, 95 % confidence interval). Source signatures, biogeochemical processes and transport all contribute to these observations. Two distinct areas, one under continental influence (the western equatorial Pacific) and an open ocean region (the central equatorial Pacific), emerged from the data. In the area under continental influence, high PFe concentrations along with <span class="inline-formula"><i>δ</i><sup>56</sup></span>DFe values systematically heavier than that of <span class="inline-formula"><i>δ</i><sup>56</sup></span>PFe indicated an equilibrium fractionation and the co-occurrence of chemical fluxes from both phases toward the other. This exchange occurs through non-reductive processes, as previously proposed from three of the eight stations of this area (Labatut et al., 2014) and extends up to 1200 km from the coast. In the open ocean area, preservation of a DFe isotopic signature of <span class="inline-formula">∼</span> <span class="inline-formula">+</span>0.36 ‰ within the EUC, from Papua New Guinea to the central equatorial Pacific (7800 km), confirmed the origin of the DFe carried within this current toward the HNLC region. At the same depth, bordering the EUC at 2° N and 2° S at 140° W, light isotopic signatures suggested that iron was originating from the eastern Pacific oxygen minimum zones. These light signatures were also observed in deeper central waters, between 200 and 500 m. Our data did not allow conclusions about fractionation during uptake by phytoplankton, but indicated that any fractionation, if present, must be small, no larger than a few tenths of a per mil.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-791-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/791/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:soil134347</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>soil</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Modelling long-term soil organic carbon sequestration under varying environmental drivers and internal protection mechanisms – towards a digital twin]]></dc:title>
      <dc:creator>Meij, W. Marijn</dc:creator>
      <dc:creator>Finke, Peter</dc:creator>
      <dc:description><![CDATA[<p>Soil organic carbon (SOC) plays a large role in sustainable soil management and climate change mitigation. To understand the potential of soils to sequester additional carbon requires detailed knowledge of the underlying processes and drivers. In this study, we use soil evolution model SoilGen3.8.2 to assess the effects of environmental drivers (bioclimate, erosion level and land use) and four protection mechanisms on long-term SOC dynamics.</p>        <p>The protection mechanisms (aggregation, clay mineralogy, microporosity and metal oxyhydroxides, MOOHs) showed large differences with different temporal patterns, where aggregation and clay mineralogy dominated during 10 <span class="inline-formula">ka</span> of pedogenesis and MOOHs had a negligible effect. Ranking internal and external controls on SOC stocks revealed a decreasing influence of bioclimate <span class="inline-formula">&gt;</span> protection mechanism <span class="inline-formula">&gt;</span> erosion rate <span class="inline-formula">&gt;</span> land use <span class="inline-formula">&gt;</span> time.</p>        <p>Topsoil and subsoil SOC recovery after agricultural use revealed different dynamics, controlled by the history of environmental drivers and pedogenesis. Natural SOC recovery showed lowest rates for subsoils and highest rates for topsoils, with a strong control of erosion and pedogenetic history. The addition of ground rock of different mineralogies to enhance SOC sequestration had some effect, mainly for goethite, montmorillonite and a temporary effect of calcite. Our simulations demonstrate how SoilGen can improve understanding of soil processes, while also highlighting knowledge gaps, such as missing experimental insights in key SOC stabilization mechanisms.</p>        <p>Our study shows that soil models such as SoilGen cannot act as digital twins of a soil that represent the entire soil, as not all processes and parameters of the complex soil system are represented. These models can, however, form the basis of topical digital twins that target specific processes or properties. We provide a roadmap for developing such topical digital twins and recommend to start from a complex model that accounts for pedogenetic history.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/soil-12-165-2026</dc:identifier>
      <dc:identifier><![CDATA[https://soil.copernicus.org/articles/12/165/2026/]]></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:egusphere137554</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Simulated temporal scaling dependencies in sub-daily precipitation]]></dc:title>
      <dc:creator>Dobler, Andreas</dc:creator>
      <dc:creator>Benestad, Rasmus</dc:creator>
      <dc:creator>Lutz, Julia</dc:creator>
      <dc:creator>Parding, Kajsa Maria</dc:creator>
      <dc:description><![CDATA[Rainfall intensity-duration-frequency (IDF) curves are an essential tool in water management, for instance in urban stormwater handling. They are commonly derived by fitting generalised extreme value distributions to observed annual maximum rainfall values, a process that requires long-term, high temporal resolution (sub-daily) observations of precipitation to ensure robust estimates. Alternatively, IDF curves can be approximated with simplified parametric mathematical expressions fitted to empirical data, providing a possibility to avoid the challenging data requirements. In this case, the parametric expression can be based on two key parameters that specify the shape of the curves: the wet-spell mean precipitation <em>&mu;</em> and the wet-spell frequency <em>f<sub>w</sub></em>. For these two parameters, robust estimates are easier to obtain.</p> <p>The resulting parametric IDF curves exhibit a fractal dimension and the present study takes a step towards better understanding the conditions influencing this fractal dimension and its spatial and temporal variability. To this end, we explore the dependencies across different timescales, using hourly precipitation data from convection-permitting (3 km) regional climate model simulations carried out with the HCLIM model over northern Europe. The analysis is applied to HCLIM simulations driven by boundary conditions from the ERA-Interim reanalysis, as well as from the EC-Earth and GFDL-CM3 global climate models for current and future climates following the RCP8.5 scenario.</p> <p>We find that the relationship between wet-spell mean precipitation for different durations, and hence the sub-daily fractal dimension, is influenced by geographical conditions, as is also the wet-spell frequency. The results are consistent across different boundary conditions representing current climate conditions (reanalysis and global climate models), and showed little sensitivity to the driving model, indicating that different meteorological phenomena prevail in different regions and that these are well represented in the models. Future climate projections show changes in the fractal dimension and wet-spell frequency ratios with a general north-south gradient. Overall, the models indicate a shift towards fewer, but more intense wet-hours per wet day.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-207</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-207/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138978</identifier>
    <datestamp>2026-03-06</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 ability of LSTM to model snowmelt versus rainfall generated floods]]></dc:title>
      <dc:creator>Bakke, Sigrid Jørgensen</dc:creator>
      <dc:creator>Barna, Danielle Marie</dc:creator>
      <dc:creator>Engeland, Kolbjørn</dc:creator>
      <dc:creator>Kolberg, Sjur Anders</dc:creator>
      <dc:creator>Nordeide, Sunniva</dc:creator>
      <dc:description><![CDATA[One of the most important skills of hydrological models is to simulate timing and magnitude of flood events. Long Short-Term Memory (LSTM) networks are currently among the most successful models for streamflow and flood prediction over large regions. In snow-influenced catchments, which typically comprise a minority in large-scale studies, floods are generated by two distinctly different processes, snowmelt and rainfall. The applicability of hydrological models in such regions is therefore dependent on their ability to represent both types of floods. Nevertheless, flood evaluations of LSTM taking different flood-generating processes into account are currently lacking. This study fills this gap by evaluating the ability of LSTM to model flood peak characteristics separately for snowmelt and rainfall generated floods. The trained LSTM model successfully simulated streamflow time series across the 103 evaluated catchments, with average NSE of 0.85 and average KGE of 0.87 over the unseen evaluation period. LSTM exhibited better performance in the majority of the catchments in terms of flood peak timing and magnitude for both rainfall and snowfall generated floods when compared to the operational hydrological model in the region (HBV) used as a benchmark. Both models had a 24 pp higher percentage of correctly simulated peak days for rainfall generated floods as compared to snowmelt generated floods. LSTM outperformed HBV for a larger proportion of the catchments in terms of peak timing of rainfall generated events (83 %) as compared to snowmelt generated events (64 %). On the other hand, a larger proportion of the catchments were improved by LSTM for snowmelt generated events as compared to rainfall generated events when considering peak magnitudes. The largest improvements in peak magnitudes were found for rainfall generated events, in particular for catchments where HBV exhibited high (&gt; 40 %) absolute errors. Overall, our findings bring confidence that LSTM can improve hydrological services in regions subject to both snowmelt and rainfall generated floods.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1056</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1056/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138677</identifier>
    <datestamp>2026-03-06</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[Ammonium and nitrite oxidation in the upper euphotic zone of the oligotrophic Red Sea]]></dc:title>
      <dc:creator>Rahav, Eyal</dc:creator>
      <dc:creator>Wankel, Scott D.</dc:creator>
      <dc:creator>Paytan, Adina</dc:creator>
      <dc:description><![CDATA[Nitrification is widely understood to be inhibited by light in the surface ocean, however, increasing evidence indicates its occurrence at low levels at many sites. The extent to which nitrification remains active in the euphotic zone could have important implications to new production calculations, yet it remains understudied. Here, we quantified ammonium and nitrite oxidation rates in the euphotic zone of the Gulf of Aqaba (Northern Red Sea) from late spring to late summer and examined environmental controls and implications for dark carbon fixation (chemoautotrophy) and new production. Both ammonium and nitrite oxidation were detectable throughout the euphotic zone (~0.1&ndash;0.8 nmol N L<sup>-1</sup> d<sup>-1</sup>). Overall, rates increased with depth and were strongly suppressed in the highest irradiance surface waters. Integrated rates over the entire euphotic zone (24&ndash;56 &micro;mol N m<sup>-2</sup> d<sup>-1</sup>) were among the lowest reported for oligotrophic regions globally. This reflects extremely low substrate concentrations and intense, though not complete, photoinhibition. Ammonium and nitrite oxidation together supported &lt;2 % of chemoautotrophic activity, suggesting other processes, not accounted for, such as anaplerosis may be important. Depth-resolved correlations with environmental parameters highlight light, temperature, and substrate availability as key regulators of both processes. Our results show that nitrification in the Gulf of Aqaba operates at the lower bounds of global euphotic zone rates and is loosely coupled to carbon cycling. These findings underscore the need to better resolve nitrification dynamics in ultra-oligotrophic, rapidly warming, seas to refine estimates of new production and chemoautotrophic carbon assimilation under future ocean conditions.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-855</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-855/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138722</identifier>
    <datestamp>2026-03-06</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 process-based modeling of soil organic matter physical properties for land surface models &ndash; Part 2 : Global land surface simulations and mineral soil compaction adjustment]]></dc:title>
      <dc:creator>Decharme, Bertrand</dc:creator>
      <dc:creator>Tzanos, Diane</dc:creator>
      <dc:creator>Hardouin, Lucas</dc:creator>
      <dc:creator>Boone, Aaron</dc:creator>
      <dc:creator>Minvielle, Marie</dc:creator>
      <dc:creator>Moigne, Patrick</dc:creator>
      <dc:creator>Gaillard, Rémi</dc:creator>
      <dc:description><![CDATA[In the companion paper, Decharme (2025) developed a process-based framework using soil mixture theory to represent the effects of soil organic matter on soil physical properties in land surface models. The present study extends this work by testing the framework in global land surface simulations with the ISBA-CTRIP land surface modeling system. The approach derives the volumetric organic matter fraction and phase-specific densities from soil organic carbon and bulk density using mass volume relationships, and computes hydraulic and thermal parameters using mixing rules consistent with the model physics. We also introduce an optional mineral soil compaction adjustment, under the assumption that texture-based pedotransfer functions are calibrated on weakly compacted samples, whereas gridded bulk density products mostly reflect in situ conditions that include varying degrees of compaction. We examine the effects of both developments in multidecadal global offline simulations forced by a standard meteorological dataset and driven by SoilGrids soil inputs. Four configurations are compared, a mineral-only control, a previous empirical scheme, the new process-based scheme, and its compaction-adjusted variant. The evaluation combines site-scale constraints on porosity and hydraulic behavior with large-scale benchmarks of the terrestrial water and energy cycles, including terrestrial water storage variations, river discharge, evapotranspiration, soil temperature, and active layer thickness. Overall, the global experiments suggest that the new process-based scheme produces more consistent large-scale hydrothermal responses than the previous empirical scheme, whereas the compaction adjustment plays a secondary role and mainly acts as a local modulator.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-860</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-860/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138936</identifier>
    <datestamp>2026-03-06</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[Alluvial river-channel width: transient adjustment and dynamic equilibrium]]></dc:title>
      <dc:creator>Wickert, Andrew D.</dc:creator>
      <dc:creator>Jones, Jabari C.</dc:creator>
      <dc:creator>Libby, Devon</dc:creator>
      <dc:creator>Larson, Phillip H.</dc:creator>
      <dc:creator>Barnhart, Katherine R.</dc:creator>
      <dc:creator>Wyk de Vries, Maximillian S.</dc:creator>
      <dc:creator>Schildgen, Taylor F.</dc:creator>
      <dc:description><![CDATA[Alluvial river channels naturally widen and narrow as large floods scour banks and smaller ones supply sediments that help build bars and channel margins. Despite substantial advances into the controls on the equilibrium width of river channels, relatively little theory underpins our knowledge on transient river-channel-width evolution. Such a knowledge gap inhibits us from predicting the impacts of present-day nonstationary hydrology on river-channel stability and geomorphic change. Here we present a unified approach to model transient channel widening, via erosion of cohesive banks and mobilization of noncohesive clasts, and narrowing, via lateral diffusion of sediment that attaches to the banks. The resultant model can take a full hydrograph as input, allowing the hydraulic geometry and associated "geomorphically effective" water discharge to emerge dynamically. Stable widths develop via the inverse relationship between channel width and flow depth, and therefore, shear stress on the channel margins. Equilibrium solutions closely approximate data and theory on channels with both gravel and mud banks, and we compare transient solutions to the rapidly widening Minnesota and Cannon Rivers (Minnesota, USA) and the narrowing Green River and Diamond Fork (Utah, USA). Documented Python source code to run these computations is available from GitHub and Zenodo via the "OTTAR" package, and may be installed via pip from PyPI.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1018</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1018/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138599</identifier>
    <datestamp>2026-03-06</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[Integrating total water level data and visual evidence to assess coastal flooding in San Diego County]]></dc:title>
      <dc:creator>Pinto, Denali M.</dc:creator>
      <dc:creator>Catanzarite, Antonio</dc:creator>
      <dc:creator>Govindu, Anshul</dc:creator>
      <dc:creator>Engeman, Laura</dc:creator>
      <dc:creator>Corringham, Thomas W.</dc:creator>
      <dc:creator>Fiedler, Julia</dc:creator>
      <dc:creator>Gershunov, Alexander</dc:creator>
      <dc:creator>Merrifield, Mark</dc:creator>
      <dc:description><![CDATA[Coastal flooding in Southern California poses a growing threat to communities and infrastructure, exacerbated by climate change and sea level rise. Total water level (TWL), the combination of sea level, tides, and wave runup, is increasingly used to forecast coastal flooding, but validating the thresholds at which flood impacts occur remains a challenge. This study examines the relationship between modeled TWL and photographic or video evidence of flooding in San Diego County from 2010 to 2024. We integrate model output from the Coastal Data Information Program with visual records from community monitoring programs to assess spatial and seasonal variations in flood occurrence. We also evaluate the influence of atmospheric rivers and El Ni&ntilde;o conditions. Atmospheric river days were associated with an increase in the likelihood of observed flooding, and El Ni&ntilde;o winters showed a positive but weaker correlation. Overall results demonstrate a robust but imprecise correlation between modeled TWL and observed flood impacts, with uncertainty driven largely by convenience sampling in the visual dataset. Despite these limitations, modeled TWL is shown to be a useful proxy for flood risk. Our findings underscore the need for systematic flood impact documentation to refine threshold estimates and improve flood forecasting and coastal management.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-820</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-820/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138923</identifier>
    <datestamp>2026-03-06</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[Drivers of Ecosystem Stability Differ with the Intensity of Extreme Climatic Events]]></dc:title>
      <dc:creator>Yanagawa, Aki</dc:creator>
      <dc:creator>Ueda, Rina</dc:creator>
      <dc:creator>Yoshikawa, Sayaka</dc:creator>
      <dc:creator>Iseri, Yoshihiko</dc:creator>
      <dc:creator>Kanae, Shinjiro</dc:creator>
      <dc:description><![CDATA[This study investigates how the dominant drivers of ecosystem stability metrics vary across gradients of hydroclimatic extremity. While previous studies have documented the impacts of droughts and heavy rainfall on ecosystem functioning and resilience inferred from stochastic fluctuations, less attention has been given to whether the relative importance of climatic, biotic, and landscape controls changes systematically under different levels of climatic stress. To address this question, we quantified vegetation resistance and event-scale recovery responses and compared the contributions of meteorological, biodiversity, and topographic factors across a global range of hydroclimatic conditions. We find that under normal to moderately dry conditions, vegetation stability metrics are primarily associated with meteorological variables, particularly temperature and precipitation, consistent with earlier global assessments. Under severe and extreme drought conditions, resistance decreases markedly across most regions, whereas recovery responses exhibit weaker and more spatially heterogeneous changes. Importantly, in sparsely vegetated ecosystems such as grasslands and open shrublands, the relative dominance of drivers shifts from climatic to biodiversity and topographic factors under intensified drought stress, indicating context-dependent regulation of ecosystem stability. Deciduous needle-leaf forests show consistently low resistance and recovery capacity across climatic regimes, suggesting elevated sensitivity to hydroclimatic variability. Overall, our findings demonstrate that ecosystem stability under climatic extremes cannot be explained solely by meteorological forcing and highlight the increasing importance of biodiversity and landscape heterogeneity in shaping stability responses under intensifying climate variability.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1007</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1007/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138821</identifier>
    <datestamp>2026-03-06</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[Atmospheric circulation and boundary layer processes modulating aerosol and cloud characteristics over the coastal Northeast Pacific during April to October of ARM EPCAPE field campaign]]></dc:title>
      <dc:creator>Chellappan, Seethala</dc:creator>
      <dc:creator>Painemal, David</dc:creator>
      <dc:creator>Thieman, Mandana</dc:creator>
      <dc:creator>Pelayo, Christian</dc:creator>
      <dc:creator>Smith Jr., William L.</dc:creator>
      <dc:creator>Russell, Lynn M.</dc:creator>
      <dc:description><![CDATA[Observations from the ARM Eastern Pacific Cloud Aerosol Precipitation Experiment (EPCAPE) spanning April to October 2023 at Scripps Pier, La Jolla, California (32.8663&deg; N, 117.2546&deg; W) were used to investigate the regional-scale atmospheric factors that control the variability of marine low clouds and aerosols in the coastal boundary layer (BL). Using Self-Organizing Maps applied to ERA5 sea level pressure and near-surface winds, we classify the synoptic evolution of the subtropical anticyclone into 9 regimes, which includes: 1) patterns with a weakened subtropical anticyclone south of Scripps Pier and a midlatitude cyclone further north, 2) regimes that capture the evolution of anticyclone in terms of magnitude (strong vs weak) and location (coastal vs offshore), with their corresponding transitions in BL wind strengthening and large-scale subsidence, 3) a regime characterized by an anticyclone with its core at the northwestern edge of the domain, and 4) a regime that captures anomalies that minimally depart from the climatological mean. GOES-18 cloud retrievals reveal that regimes associated with anticyclone cores closer to Scripps Pier produce reduced low-cloud fraction, shallower clouds, and low liquid water path (LWP); whereas regimes with a west/north-westward-displaced anticyclone support extensive stratocumulus with higher LWP and elevated cloud tops. Regimes with a weak anticyclone centered adjacent to the Pier feature highest concentrations of smaller-sized particles, associated with a stable BL and stagnation under weak winds. Regimes with anticyclonic strengthening farther-offshore have lower aerosol concentrations. Partial inconsistency between cloud droplet number concentration (N<sub>d</sub>) and aerosol concentration indicates BL turbulence critically influences aerosol activation into N<sub>d</sub>.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-933</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-933/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138875</identifier>
    <datestamp>2026-03-06</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[Compound Drivers and Spatial Connectivity led to the Devastating Debris Flood in the Village of La B&eacute;rarde, June 2024, French Alps]]></dc:title>
      <dc:creator>Filhol, Simon</dc:creator>
      <dc:creator>Misset, Clément</dc:creator>
      <dc:creator>Bontemps, Noélie</dc:creator>
      <dc:creator>Cusicanqui, Diego</dc:creator>
      <dc:creator>Paquet, Emmanuel</dc:creator>
      <dc:creator>Dumont, Marie</dc:creator>
      <dc:creator>Gagliardini, Olivier</dc:creator>
      <dc:creator>Lacroix, Pascal</dc:creator>
      <dc:creator>Gascoin, Simon</dc:creator>
      <dc:creator>Thirel, Guillaume</dc:creator>
      <dc:creator>Brondex, Julien</dc:creator>
      <dc:creator>Hagenmuller, Pascal</dc:creator>
      <dc:creator>Larose, Eric</dc:creator>
      <dc:creator>Schoeneich, Philipp</dc:creator>
      <dc:creator>Roy, Denis</dc:creator>
      <dc:creator>Thibert, Emmanuel</dc:creator>
      <dc:creator>Eckert, Nicolas</dc:creator>
      <dc:creator>Montety, Félix</dc:creator>
      <dc:creator>Mainieri, Robin</dc:creator>
      <dc:creator>Hauet, Alexandre</dc:creator>
      <dc:creator>Gottardi, Frédéric</dc:creator>
      <dc:creator>Berthet, Johan</dc:creator>
      <dc:creator>Baratier, Alexandre</dc:creator>
      <dc:creator>Liébault, Frédéric</dc:creator>
      <dc:creator>Chmiel, Małgorzata</dc:creator>
      <dc:creator>Piton, Guillaume</dc:creator>
      <dc:creator>Chambon, Guillaume</dc:creator>
      <dc:creator>James, Guillaume</dc:creator>
      <dc:creator>Frey, Philippe</dc:creator>
      <dc:creator>Deline, Philip</dc:creator>
      <dc:creator>Astrade, Laurent</dc:creator>
      <dc:creator>Vincent, Christian</dc:creator>
      <dc:creator>Laigle, Dominique</dc:creator>
      <dc:creator>Recking, Alain</dc:creator>
      <dc:creator>Karbou, Fatima</dc:creator>
      <dc:creator>Mauss, Adrien</dc:creator>
      <dc:creator>Bonnefoy-Demongeot, Mylène</dc:creator>
      <dc:creator>Fontaine, Firmin</dc:creator>
      <dc:creator>Langlais, Mickael</dc:creator>
      <dc:creator>Berthier, Etienne</dc:creator>
      <dc:creator>Blanc, Antoine</dc:creator>
      <dc:description><![CDATA[On the evening of June 21, 2024, a debris flood inundated the village of La B&eacute;rarde, located at the heart of the &Eacute;crins mountain range in the French Alps. More than 200&thinsp;000 m<sup>3</sup> of materials were deposited in place of the village. People were evacuated on time but many buildings were destroyed and buried. The event was understood to be driven by a 10-year return period rain alongside to a 20-year snowmelt, the drainage of a supra-glacial lake, with potentially more internal water storage in the Bonne Pierre glacier. While we do not have direct observation of the supraglacial lake drainage, we found a number of evidences pointing to the role it likely had in destabilizing and triggering sediment transport from the Bonne Pierre fan. This work required an interdisciplinary approach to establish the set of scientific elements to reconstruct the event's chronology and rarity. We found that the combination of moderate magnitude drivers is not sufficient to explain the impacts observed. The location of the village on an alluvial fan directly connected to the source of sediments, was also key to understand the magnitude of the impacts. This event took place in a region particularly sensitive to climate change, where physical processes of the cryosphere at play are subject to alteration in a changing climate (<em>e.g.</em> precipitation amount and phase). The recent paradigm of compound events helps reconsidering the nature of this event and suggests possible approaches in anticipating new up-coming compound events in an era in which the Alps are entering a new paraglacial adjustments. Nevertheless, compound events remain difficult to forecast as they may be generated by diverse set of combination of low to moderate magnitude hazards associated to specific geographical, geomorphological, cryospheric, and meteorological onsets.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-971</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-971/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138993</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Heavy Precipitation Events of Various Durations Across Germany: A Station-Based Assessment of Spatial and Temporal Variability Using the Block Maxima Method]]></dc:title>
      <dc:creator>Palarz, Angelika</dc:creator>
      <dc:creator>Junghänel, Thomas</dc:creator>
      <dc:creator>Ostermöller, Jennifer</dc:creator>
      <dc:creator>Deutschländer, Thomas</dc:creator>
      <dc:creator>Kaspar, Frank</dc:creator>
      <dc:description><![CDATA[As heavy precipitation events (HPEs) pose substantial risks to natural and human systems, a growing body of research has focused on their behaviour under ongoing climate change, hypothesising that rising air temperature can have a pronounced influence on precipitation patterns, including HPEs of various durations. Recent observational and modelling studies suggest that this influence tends to be particularly strong for short‑duration HPEs, albeit their assessment appears challenging due to limited availability of precipitation data with both high temporal resolution and long-term observational records. Therefore, in this study, we made use of recently collected, digitised, and quality‑controlled 5‑minute precipitation data from rain‑gauge stations across Germany in order to assess the spatial and temporal variability of HPEs of nine durations ranging from 5 minutes to 7 days. Using the block maxima method, we confirmed that the spatial and temporal variability of annual maximum precipitation totals (AMPTs) is strongly duration‑dependent. While the medians of short‑duration AMPTs calculated for individual stations are relatively evenly distributed across Germany, those of medium‑ and long‑duration AMPTs increasingly reflect the influence of topography. Moreover, short‑duration AMPTs exhibit higher and spatially scattered event to event variability, contrasting with the relatively consistent and regionally organised event to event variability observed for long‑duration AMPTs. The duration‑dependent nature of AMPTs is further reflected in their long‑term variability. While positive trends prevail for AMPTs with durations of 1 to 7 hours, trends for AMPTs with durations of 3 to 7 days are more balanced or even slightly negative, depending on the investigation period. Yet, statistically significant &ndash; both positive and negative &ndash; trends are relatively rare and sensitive to changes in the measurement system and investigation period.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1067</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1067/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138982</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Impacts of Cascading Check Dams on Sediment Yield in the Middle Yellow River Basin: Insights from 50 Years of Grid-cell-level Simulation]]></dc:title>
      <dc:creator>Huang, Yanzhang</dc:creator>
      <dc:creator>Gao, Guangyao</dc:creator>
      <dc:creator>Ran, Lishan</dc:creator>
      <dc:creator>Wang, Yue</dc:creator>
      <dc:creator>Zheng, Mingguo</dc:creator>
      <dc:description><![CDATA[Check dams, globally built for controlling soil erosion, form complex cascading systems that pose significant challenges for assessing spatiotemporal dynamics of sediment yield (SY) at large basin scale. This study proposed an integrative framework combining dynamic sediment trapping efficiency of cascading check dams with the Revised Universal Soil Loss Equation (RUSLE), index of connectivity (IC), and sediment delivery ratio (SDR). This model was applied to evaluate grid-cell-based distribution of SY and sediment trapped by check dams during 1970&ndash;2020 in the middle Yellow River Basin (with over 47000 check dams). The Nash-Sutcliffe efficiency of proposed model increased to 0.71 compared to model ignoring sediment trapping of check dams (0.59). Check dams reduced the multi-year average SY by 50.01 % in dam-controlled areas. Totally 3.84 &times; 10<sup>9</sup> t of sediment was trapped over the 50 years, constituting 41.49 % of designed storage capacity. The sediment reduction contribution by check dams (SRC<sub>dam</sub>) exhibited considerable spatial heterogeneity, ranging from 73.9 % to 0.9 % among sub-basins, and the proportion of accumulated sediment to storage capacity of check dams (SAR<sub>dam</sub>) varied from 78.1 % to 1.1 %. The SRC<sub>dam</sub> increased linearly with check dam density and the share of area they controlled, whereas SAR<sub>dam</sub> increased logarithmically with SY from upstream of the check dams (<em>P</em> &lt; 0.001). A trade-off between SRC<sub>dam</sub> and SAR<sub>dam</sub> in some sub-basins indicates that the number of check dams in these basins is insufficient or overmuch. This study provides a practical and data-efficient method for assessing sediment trapping and reduction by cascading check dam systems in large basins, offering valuable insights for improving soil and water conservation strategies in erosion-prone regions.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1058</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1058/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138999</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Introducing shrubs enhances the representation of high-latitude vegetation and carbon cycling in the ORCHIDEE land surface model]]></dc:title>
      <dc:creator>Kirchner, Anna</dc:creator>
      <dc:creator>López-Blanco, Efrén</dc:creator>
      <dc:creator>Bastrikov, Vladislav</dc:creator>
      <dc:creator>Luyssaert, Sebastiaan</dc:creator>
      <dc:creator>Peylin, Philippe</dc:creator>
      <dc:creator>Lansø, Anne Sofie</dc:creator>
      <dc:description><![CDATA[Arctic-Boreal terrestrial ecosystems are rapidly changing under amplified high-latitude warming, including widespread expansion of shrubs, with consequences for regional carbon and energy balances. Yet, high-latitude vegetation diversity and vegetation-climate interactions remain under-represented in many global land surface models. In ORCHIDEE, the land surface component of the IPSL Earth system model, high-latitude vegetation is represented primarily as boreal trees or grasslands, omitting explicit shrubs. Here, we implement three high-latitude shrub plant functional types (PFTs) (tall deciduous, low deciduous, and evergreen dwarf shrubs) in ORCHIDEE (revision 9269). Following literature recommendations, this classification combines phenology and stature to capture key functional contrasts while keeping the number of new PFTs limited. The implementation builds on ORCHIDEE's existing woody vegetation scheme by recalibrating a targeted set of parameters controlling allometry, carbon allocation, recruitment, mortality and phenology. Parameter values are constrained using synthesised pan-Arctic observations to obtain regionally representative shrub traits. Shrub spatial distributions are prescribed with updated PFT maps that combine ESA CCI products with Arctic and regional shrub mapping information. The resulting shrub PFTs reproduce observed ranges of shrub size and biomass allocation across the Arctic&ndash;Boreal domain. Introducing shrubs reduces simulated total aboveground biomass in the Arctic-Boreal region from 54 to 46.7 P g C (-13.5 %) and mean annual gross primary productivity from 498 to 481 g C m<sup>&minus;2</sup> yr<sup>&minus;1</sup> (-3.4 %) over the simulated period 1992-2020, with a stronger reduction in the tundra region (4.6 to 3 P g C (-34.8 %); and 334 to 289 g C m<sup>&minus;2</sup> yr<sup>&minus;1</sup> (-13.5 %)), increasing agreement with benchmarking datasets. A key strength of our implementation is its simplicity, as it builds on ORCHIDEE's existing woody vegetation framework. In addition, the use of synthesised pan-Arctic observations provides regionally representative observational constraints, making the methodological choices transferable beyond ORCHIDEE. Overall, this work provides a data-constrained shrub representation in ORCHIDEE with minimal added process complexity and establishes a foundation for future development of shrub-climate interactions and dynamic shrubification processes.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1071</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1071/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139028</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Cloud vertical structure across China from a national Ka-band cloud radar network: Thermodynamic, dynamical, and land-surface controls]]></dc:title>
      <dc:creator>Xu, Hui</dc:creator>
      <dc:creator>Guo, Jianping</dc:creator>
      <dc:creator>Deng, Jianbo</dc:creator>
      <dc:creator>Yang, Rongfang</dc:creator>
      <dc:creator>Meng, Deli</dc:creator>
      <dc:creator>Zhang, Zhen</dc:creator>
      <dc:creator>Li, Ning</dc:creator>
      <dc:creator>Sun, Yuping</dc:creator>
      <dc:creator>Jiang, Shuairu</dc:creator>
      <dc:creator>Chen, Tianmeng</dc:creator>
      <dc:creator>Chen, Juan</dc:creator>
      <dc:creator>Zeng, Liping</dc:creator>
      <dc:creator>Zhou, Yongshui</dc:creator>
      <dc:creator>Tong, Bing</dc:creator>
      <dc:description><![CDATA[<p data-start="55" data-end="678">Cloud vertical structure plays a central role in regulating Earth&rsquo;s radiation balance and hydrological cycle, yet it remains poorly represented in weather and climate models due to limited high-resolution observations. Using a newly established national network of 80 Ka-band cloud radars, we provide the first high-spatiotemporal-resolution characterization of cloud vertical structure across China for 2024 and quantify its thermodynamic, dynamical, and land-surface controls. An improved retrieval algorithm accounting for height-dependent radar sensitivity and clutter suppression is applied to derive cloud boundaries. The national annual mean cloud occurrence frequency is 56.7 %, dominated by single-layer clouds (34.7 %), followed by two-layer (14.7 %) and multi-layer clouds (7.1 %). Single-layer clouds prevail over arid northwestern China, whereas multi-layer clouds are more frequent in humid southeastern regions. Cloud base height exhibits strong seasonality, with higher values in summer and lower values in winter, and distinctly lower bases over the Tibetan Plateau. Diurnally, summer clouds show a pronounced afternoon peak between 3 and 9 km, while winter clouds are mainly confined below 3 km with a near-sunrise maximum. Thermodynamic conditions exert primary control on cloud vertical development. Higher low-level humidity favors deeper clouds and higher tops, whereas stronger lower-tropospheric stability suppresses vertical growth. Wind shear generally limits cloud depth, though moderate shear may enhance organization under unstable conditions. Land-surface characteristics further modulate cloud base height, with higher bases over barren land and lower bases over forests. These results provide national-scale observational benchmarks for improving cloud parameterizations in numerical models.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1091</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1091/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138550</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Implementation of the reduced complexity model InMAP at urban scale using a high-resolution WRF-Chem simulation]]></dc:title>
      <dc:creator>Rojas Neisa, Diego Roberto</dc:creator>
      <dc:creator>Piracoca-Mayorga, Alejandro</dc:creator>
      <dc:creator>Espitia-Cano, Sebastián</dc:creator>
      <dc:creator>Morales Betancourt, Ricardo</dc:creator>
      <dc:description><![CDATA[Most of the population globally lives in areas exceeding prior and current WHO guidelines for fine particulate matter (PM<sub>2.5</sub>), highlighting the persisting need for implementing emission reduction strategies. Given the complex transport and transformation processes that airborne species undergo in the atmosphere, chemical transport models can aid in designing and prioritizing air pollution mitigation actions. However, detailed chemical transport models often require substantial computational power and expertise. For that reason, reduced complexity models have emerged as an alternative, incorporating some of the information from chemical transport models while drastically reducing the technical complexity and computational demand. In this work, we build a local implementation of the Intervention Model For Air Pollution, InMAP, at high spatial resolution for a large urban area, in Bogot&aacute;, Colombia. As input for the reduced complexity model, we carried out a detailed 12-month simulation with the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) version 4.1. To achieve sufficiently high spatial-resolution for urban air quality, the model was configured with three nested domains of 27x27 km, 9x9 km, and 3x3 km respectively. When compared with surface station data, the modeled annual mean PM<sub>2.5</sub> showed a +3.3 % overestimation at the city-scale. Furthermore, the WRF-Chem simulation accurately captured the structure of the observed PM<sub>2.5</sub> time series at daily, weekly and seasonal time-scales. The InMAP base fields showed a slight under-prediction relative to WRF-Chem, but overall, the correlation between the WRF-Chem and InMAP modeled PM<sub>2.5</sub> fields was high, with <em>R</em><sup>2</sup> = 0.92. InMAP sensitivity was tested for three emission reduction scenarios of varying complexity, by comparing the marginal concentrations against simulations with the full chemical transport model. The scenarios ranged in complexity, from primary-PM reductions only, to scenarios exploring moderate and severe city-wide emissions reductions from diesel powered mobile sources. Although InMAP marginal PM<sub>2.5</sub> fields were linearly correlated with the corresponding WRF-Chem sensitivities, a strong overestimation in predicted PM<sub>2.5</sub> variations were shown for all emission reduction scenarios considered. For the simpler scenarios where only primary PM was reduced InMAP sensitivity was a factor of 2 that of WRF-Chem, while for the more complex emission reduction scenarios involving also reduction in gas-phase emissions, InMAP overestimated PM<sub>2.5</sub> concentrations by a factor of 5. The driver in InMAPs overestimated PM<sub>2.5</sub> sensitivity in the scenarios involving gas-phase precursors was a large overestimation of secondary organic aerosols and particulate nitrate. The results of this work suggest that InMAP can be used to scan for potential emission reduction scenarios at the urban-scale, specially when those scenarios involve mostly primary PM emission reductions. However, our analysis indicates that studies aiming to carry out assessments using the absolute reductions in concentration from InMAP should first calibrate its sensitivities against a full chemical transport model run.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-797</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-797/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139108</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Soil&ndash;atmosphere water vapor exchange in semi-arid Northwest China: New insights from fiber-optic relative humidity sensing]]></dc:title>
      <dc:creator>Guo, Junyi</dc:creator>
      <dc:creator>Sun, Mengya</dc:creator>
      <dc:creator>Zhang, Chengcheng</dc:creator>
      <dc:creator>Liu, Jie</dc:creator>
      <dc:creator>Lou, Qingnan</dc:creator>
      <dc:creator>Xu, Qiyu</dc:creator>
      <dc:creator>Shi, Bin</dc:creator>
      <dc:description><![CDATA[Soil&ndash;atmosphere water vapor exchange in arid and semi-arid regions is a key process in near-surface hydrology, reflecting the dynamic coupling of surface energy and moisture. In this study, a novel fiber-optic sensing technique was employed to measure vertical water vapor fluxes across the soil&ndash;atmosphere interface in a semi-arid region of the Loess Plateau, Yanan, China. The observations captured vapor flux dynamics across a 7-mm dry soil layer beneath the interface (hereafter referred to as Flux Layer <sub>soil</sub>) and a 10-mm molecular diffusion layer in the air above it (Flux Layer<sub> air</sub>), revealing how meteorological factors modulate near-surface vapor transport. Solar radiation enhanced vapor fluxes primarily by increasing the vapor pressure deficit (VPD), with Flux Layer <sub>soil</sub> exhibiting a slower response than Flux Layer <sub>air</sub>. This lag was most pronounced in winter, reaching up to 120 minutes. During rainfall, fluxes in both layers declined sharply as VPD dropped to near zero. Following precipitation, Flux Layer <sub>air</sub> recovered rapidly, driven by surface evaporation, while Flux Layer <sub>soil</sub> increased more gradually due to the progressive drying of subsurface moisture. Structural equation modeling based on 5657 observations revealed distinct influence pathways: Flux Layer <sub>air </sub>was more sensitive to solar radiation, air temperature, and VPD, while Flux Layer <sub>soil</sub> was predominantly governed by VPD. These findings advance the quantitative understanding of near-surface vapor transport mechanisms and improve insight into the coupled feedbacks governing soil&ndash;atmosphere interactions under variable climatic conditions.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1143</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1143/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138868</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Linking marine benthic biodiversity and ecosystem functions related to carbon cycling in a continental mud depocenter]]></dc:title>
      <dc:creator>Tung, Chueh-Chen</dc:creator>
      <dc:creator>Holtappels, Moritz</dc:creator>
      <dc:creator>Wrede, Alexa</dc:creator>
      <dc:creator>Köster, Male</dc:creator>
      <dc:creator>Sander, Lasse</dc:creator>
      <dc:creator>Beermann, Jan</dc:creator>
      <dc:creator>Sidorenko, Vera</dc:creator>
      <dc:creator>Gutow, Lars</dc:creator>
      <dc:description><![CDATA[The importance of carbon storage in continental seafloor sediments is increasingly recognized, yet the role of benthic macrofaunal biodiversity in the regulation of these processes remains poorly understood. Benthic macrofauna contributes to organic carbon cycling through respiration and secondary production, while the sediment reworking (bioturbation) and ventilation (bioirrigation) of infauna promote the redistribution and remineralization of organic matter in sediments. Here, we investigated how benthic community structure, functional traits, and the relationship between biodiversity and ecosystem functions related to carbon cycling vary along environmental gradients in muddy sediments of the southeastern North Sea. Based on 171 macrofaunal taxa collected from 50 stations, a cluster analysis revealed a clear spatial structuring of the benthic macrofauna communities across the study region. The community composition was primarily structured by bottom shear stress, salinity, and sediment characteristics. Further, a functional trait analysis showed a clear shift in community composition with water depth. Communities in the deeper sections of the study area were dominated by mobile biodiffusors and subsurface filter feeders, whereas shallower communities were characterized by less mobile, surface-modifying bivalves and polychaetes. These contrasting patterns led to pronounced differences in ecosystem functioning: bioturbation and bioirrigation potentials were significantly higher in deeper communities, whereas community secondary production and respiration were higher in shallow communities. Across all stations, community secondary production and respiration increased with taxonomic and functional diversity, while bioturbation and bioirrigation potentials were negatively related to diversity and community evenness, reflecting a dominance by key bioturbating taxa. Our findings demonstrate that environmental gradients fundamentally shape both benthic community structure and the nature of the link between biodiversity and essential ecosystem functions. These results contribute to our understanding of the role macrofauna can play in processes related to carbon sequestration in marine deposition centers with fine-grained sediment and organic matter in shelf sea systems.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-966</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-966/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138967</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[All-sky ATMS radiance data assimilation with MPAS-JEDI]]></dc:title>
      <dc:creator>Ban, Junmei</dc:creator>
      <dc:creator>Liu, Zhiquan</dc:creator>
      <dc:creator>Jung, Byoung-Joo</dc:creator>
      <dc:creator>Banos, Ivette Hernandez</dc:creator>
      <dc:creator>Ruston, Benjamin</dc:creator>
      <dc:creator>Collard, Andrew</dc:creator>
      <dc:description><![CDATA[This study extends the all-sky radiance data assimilation capability in MPAS-JEDI (data assimilation system for the Model for Prediction Across Scales-Atmosphere based upon the Joint Effort for Data assimilation Integration), previously implemented for the Advanced Microwave Sounding Unit-A (AMSU-A), to the Advanced Technology Microwave Sounder (ATMS). Compared with AMSU-A, ATMS covers a broad frequency range, including high-frequency humidity-sounding channels, in addition to the temperature-sounding and low-frequency imager channels. In contrast to the previous AMSU-A implementation, which assimilated only imaging channels under all-sky conditions, this work assimilates all ATMS channels using the all-sky approach. A situation-dependent observation error model is employed, with distinct cloud predictors over land and ocean surfaces for both temperature- and humidity-sounding channels. The analysis variables, radiance observation operator, and bias correction method are inherited from the AMSU-A all-sky assimilation. The impact of assimilating all-sky ATMS radiances is evaluated with three month-long global hybrid three-dimensional ensemble-variational (hybrid-3DEnVar) experiments: a benchmark experiment without ATMS data, an experiment assimilating only ATMS temperature-sounding channels, and an experiment assimilating all ATMS channels. The 6-hour background forecasts during the assimilation cycling and extended 5-day forecasts are verified against conventional observations, satellite radiances, and Global Forecast System (GFS) analysis. The results show that the background fits to radiosonde observations, satellite radiances, and GFS analyses have improved. Forecast verifications against GFS analyses and independent radiance observations demonstrate statistically significant improvements relative to the benchmark for up to 3 days in both ATMS experiments, across dynamic, thermodynamic, moisture, and cloud fields.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1047</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1047/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere136690</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Ice dynamics in McMurdo Sound, Antarctica, based on precise synthetic aperture radar interferometry analysis]]></dc:title>
      <dc:creator>Bohn, Kallie</dc:creator>
      <dc:creator>Rack, Wolfgang</dc:creator>
      <dc:creator>Price, Daniel</dc:creator>
      <dc:creator>Sellier, Mathieu</dc:creator>
      <dc:creator>Gomez-Fell, Rodrigo</dc:creator>
      <dc:description><![CDATA[The embayment at the end of Ross Island's Hut Point Peninsula is often covered by a patch of landfast sea ice (henceforth <em>fast ice</em>), which can remain attached to the McMurdo Ice Shelf (MIS) for a few years at a time, rather than breaking out every summer. Over recent years, later fast ice formation and increased fast ice breakout have been observed, but the influence on ice shelf stability is unclear. We examined historical MIS front positions, as well as the summer 2025 fast ice breakout and MIS calving, using Landsat optical imagery and historical USGS aerial photography.</p> <p>A precise interferometric satellite analysis was conducted for spring 2024 based on ascending-descending combinations of TerraSAR-X image acquisitions. Two non-orthogonal horizontal component velocity fields were calculated, and ground-referenced with precise movement data acquired with three automated GNSS stations that had been placed on the ice. This allowed us to calibrate three simply connected subsets to each of the velocity field components: the MIS itself, the multi-year fast ice, and the first-year fast ice. These component fields then enabled us to calculate a near-complete 2D horizontal velocity field of ice motion in the area. This analysis was the basis for calculating the divergence field of the velocity as well as principal strain rate fields. The overall ice dynamics were then related to the areas where we expect a stabilizing effect of the fast ice on the ice shelf front, or where the ice shelf geometry suggests stabilizing effects.</p> <p>Once the January&ndash;February 2025 fast ice breakout was complete, the MIS front began calving almost immediately, leading to a net retreat of the MIS front to a minimum beyond any other found in the Landsat 4&ndash;9 record. The dynamics of the fast ice were largely dependent on age, with the behavior of the multi-year fast ice resembling in most ways that of the adjoining MIS rather than the first-year fast ice, due to strong coupling at the MIS&ndash;multi-year fast ice interface. The divergence of the velocity field and the principal strain rates show convergence and compression of the fast ice in the embayment, providing evidence of a stabilizing effect and possible buttressing of the MIS by fast ice.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2025-6300</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2025-6300/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139172</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Dynamical precursors to summer temperature extremes on the Antarctic Peninsula]]></dc:title>
      <dc:creator>Dow, William J.</dc:creator>
      <dc:creator>Maycock, Amanda C.</dc:creator>
      <dc:creator>Ross, Andrew N.</dc:creator>
      <dc:creator>Williams, Ryan S.</dc:creator>
      <dc:creator>Bracegirdle, Thomas J.</dc:creator>
      <dc:description><![CDATA[<span data-contrast="auto">Extreme warm summer near-surface temperatures over the Antarctic Peninsula (AP) can lead to surface melting and the disintegration of ice shelves. </span><span data-contrast="auto">While individual case studies have linked such events to anomalous large-scale circulation, a systematic assessment of the dynamical pathways leading to AP-wide extreme austral summer warm events remains limited. </span><span data-contrast="auto">This study uses ERA5 reanalysis data to investigate the large-scale dynamical precursors associated with extreme warm days over the Antarctic Peninsula. We apply k-means clustering to mean sea level pressure anomalies during high temperature extremes and identify five distinct circulation patterns with different dominant zonal wavenumbers. We investigate the spatio-temporal evolution and persistence of near-surface wind, temperature and pressure for each cluster. </span><span data-contrast="auto">Four clusters are associated with rapidly amplifying planetary-scale wave patterns, while a fifth resembles a negative Southern Annular Mode&ndash;like state with enhanced persistence prior to event onset. Despite these differing pathways, all regimes promote anomalous northerly flow toward the AP, driving strong meridional temperature advection and regional warming. </span><span data-contrast="auto">We demonstrate that extreme Antarctic Peninsula warm events arise from distinct circulation pathways, reflecting diverse dynamical states likely influenced by hemispheric-scale teleconnections and planetary wave interactions.</span>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1179</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1179/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139074</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Unified Patterns of Topological Structure of Hydrological Characteristics in Global River Networks]]></dc:title>
      <dc:creator>Zhao, Chensong</dc:creator>
      <dc:creator>Ke, Qihua</dc:creator>
      <dc:creator>Cao, Yuan</dc:creator>
      <dc:creator>Liu, Shutong</dc:creator>
      <dc:creator>Wei, Randongfang</dc:creator>
      <dc:creator>Xie, Di</dc:creator>
      <dc:creator>Wang, Jinqiang</dc:creator>
      <dc:creator>Huang, Jingwei</dc:creator>
      <dc:creator>Zhang, Qingqing</dc:creator>
      <dc:creator>Gao, Jiahui</dc:creator>
      <dc:creator>Li, Jing</dc:creator>
      <dc:creator>Wang, Guangqian</dc:creator>
      <dc:creator>Zhong, Deyu</dc:creator>
      <dc:description><![CDATA[Unravelling the coupling between river network structure and hydrological fluxes is essential for understanding basin-scale dynamics. While traditional ordering methods describe macro-scale patterns, they often obscure local functional variations. This study quantifies the universal hydrological patterns of global river networks by integrating the classical Horton&ndash;Strahler framework with a hierarchical pyramid decomposition technique. Leveraging the global HydroATLAS dataset, we analysed 228 representative basins spanning diverse hydro-climatic regimes. We extracted rigorously defined network attributes and hydrological fluxes to examine the scaling behaviours of fundamental structural components, defined here as basic units. Our results reveal a striking topological invariance in hydrological characteristics across both varying spatial scales and distinct geographic regions. Specifically, the runoff and discharge ratios of these basic units maintain robust statistical consistency regardless of basin size or climatic conditions ranging from humid to arid. This suggests that network topology functions as a dominant physical control, effectively acting as a low-pass filter that dampens high-frequency climatic variability to produce unified global scaling laws. These findings advance the theoretical understanding of fractal river networks. Furthermore, they open new avenues for prospective research, including the integration of these physics-informed topological priors into next-generation Earth system models to improve discharge predictions and water resource modelling in ungauged basins.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1128</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1128/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139048</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Two Decades of Aerosol Optical Depth evolution from CAMS Reanalysis]]></dc:title>
      <dc:creator>Moustaka, Anna</dc:creator>
      <dc:creator>Gkikas, Antonis</dc:creator>
      <dc:creator>Logothetis, Stavros-Andreas</dc:creator>
      <dc:creator>Flemming, Johannes</dc:creator>
      <dc:creator>Rémy, Samuel</dc:creator>
      <dc:creator>Ades, Melanie</dc:creator>
      <dc:creator>Benedetti, Angela</dc:creator>
      <dc:creator>Tourpali, Kleareti</dc:creator>
      <dc:creator>Amiridis, Vassilis</dc:creator>
      <dc:creator>Kazadzis, Stelios</dc:creator>
      <dc:description><![CDATA[Aerosol optical depth (AOD) is a key indicator for evaluating global climate change, and its long-term trends provide critical insights into the evolving climatic impact of atmospheric aerosols. In this study, we analyse the long-term (2003&ndash;2024) AOD record from the fourth-generation ECMWF Atmospheric Composition Reanalysis (EAC4) to investigate global and regional variability and long-term trends over the past two decades. EAC4 is evaluated against independent AERONET observations from 178 stations selected using strict data-availability criteria. The impact of satellite assimilation is explicitly quantified through comparison with a free-running control simulation (CTRL). EAC4 reproduces observed global AOD variability with high skill (R = 0.84, RMSE = 0.12, IOA = 0.90; &gt;1.6 million collocations) and shows strong agreement with AERONET-derived trends at stations exhibiting statistically significant changes (R = 0.89), correctly capturing the trend sign at 96.7 % of sites. Negative trends are generally well represented, while positive trends are more frequently underestimated. Trend analyses across 18 regions of interest reveal significant AOD declines over eastern China, North Africa, Central Europe, and the eastern United States, alongside persistent increases over South Asia and the Middle East. Decadal analyses identify pronounced transitions, including a reversal from increasing to decreasing trends over eastern China and shifts in several dust- and biomass-burning-dominated regions. Sliding-window trend diagnostics further highlight temporal variability and regime changes. By integrating long-term reanalysis data, independent validation, and component-resolved diagnostics, this study provides a consistent assessment of recent global AOD evolution.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1107</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1107/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139036</identifier>
    <datestamp>2026-03-06</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[Juice/SWI during the Lunar-Earth-Gravity-Assist. III. Observations of the Earth as Calibration Target]]></dc:title>
      <dc:creator>Jarchow, Christopher</dc:creator>
      <dc:creator>Rezac, Ladislav</dc:creator>
      <dc:creator>Hartogh, Paul</dc:creator>
      <dc:creator>Schulz-Ravanbakhsh, Ali</dc:creator>
      <dc:creator>Cavalie, Thibault</dc:creator>
      <dc:creator>Herpin, Fabrice</dc:creator>
      <dc:creator>Moreno, Raphael</dc:creator>
      <dc:creator>Murk, Axel</dc:creator>
      <dc:description><![CDATA[On August 19<sup>th</sup> and 20<sup>th</sup> 2024 the <em>Jupiter Icy Moons Explorer </em>(Juice) executed during its cruise phase towards Jupiter a combined <em>Lunar Earth Gravity Assist</em> (LEGA) maneuver. These close flybys of the Moon and the Earth provided so far the best opportunity to test the behavior, performance, and calibration of the <em>Submillimetre Wave Instrument</em> (SWI) onboard Juice. This paper shows typical data taken during the Earth Gravity Assist and the following few days. Data quality and problems resulting from unexpected behavior of the hardware are discussed.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1096</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1096/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138949</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Automated Detection of Low-altitude Isolated Mesospheric Radar Echoes Using YOLOv8: Evidence for a C-Layer Phenomenon near 60 km Altitude?]]></dc:title>
      <dc:creator>Krishnakumar, Yadu Krishnan</dc:creator>
      <dc:creator>Renkwitz, Toralf</dc:creator>
      <dc:creator>Ahrens, Andreas</dc:creator>
      <dc:description><![CDATA[The Earth's ionosphere is created by the incident solar radiation and extends from approximately 60 km to 800 km altitude. Within the ionosphere distinct regions are formed based on the number density of the dominant chemical species and their ionization by the incident solar ultraviolet radiation and X rays. The lowermost ionospheric region is called D region and expands during daytime downwards to approximately 60km. In the recent years, rather faint echoes from below the typically continuous D region have been observed during the sunlit period using a 3.17 MHz ground based radar system at polar latitudes. To our knowledge, this study might be the first evidence of such a phenomenon through consistent radar observations. Following an initial manual inspection of the raw data and the corresponding radar image spectra, an automated deep learning approach was employed to detect these isolated low-altitude echoes. We used the pattern recognition tool YOLO (You Only Look Once) to gain statistical information on the occurrence of these radar echoes over four years of radar measurements, which covered conditions ranging from minimum to maximum solar activity. The preferred altitude of these radar echoes is found to be near 58 km with typically little variability, and where the majority of detections show a rather narrow radar spectrum. Substantial annual variability was found for these parameters and the occurrence rate, essentially separating them into summer and winter. The reduced occurrence rates during the solar maximum year 2024 suggest the role of galactic cosmic rays as an ionisation source.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1030</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1030/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139161</identifier>
    <datestamp>2026-03-06</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[Climate variability in Poland (Central Europe) in the 16th century based on multiproxy data]]></dc:title>
      <dc:creator>Przybylak, Rajmund</dc:creator>
      <dc:creator>Oliński, Piotr</dc:creator>
      <dc:creator>Koprowski, Marcin</dc:creator>
      <dc:creator>Chorążyczewski, Waldemar</dc:creator>
      <dc:creator>Szychowska-Krąpiec, Elżbieta</dc:creator>
      <dc:creator>Krąpiec, Marek</dc:creator>
      <dc:creator>Pospieszyńska, Aleksandra</dc:creator>
      <dc:description><![CDATA[The article includes an overview of the current state of knowledge regarding climate in Poland (Central Europe) in the 16<sup>th</sup> century and its changes. For this purpose, we utilised all previously published reconstructions and five new quantitative reconstructions incorporating dendrochronological data and documentary evidence. New dendrochronological data were used to reconstruct the mean winter or late winter&ndash;early spring temperatures, while documentary evidence enabled the reconstruction of mean winter (DJF) and summer (JJA) temperatures. The climate of Poland in the 16th century, as reconstructed from documentary evidence, was colder than it is today (1991&ndash;2020), particularly in winter (by 3.6&thinsp;&deg;C). In summer, it was only 0.7&thinsp;&deg;C colder than today. Compared to the average for the entire 20th century, however, the summer average in the 16th century was 0.3&thinsp;&deg;C warmer, whereas the winter average was 2.5&thinsp;&deg;C colder. In both dendrochronological reconstructions of the temperature of south-eastern Poland, the temperatures in the 16th century were generally lower than those recorded today (1951&ndash;2000), particularly in the case of the reconstruction based on the fir chronology (December&ndash;March). Anomalies, however, both positive and negative, were usually of less than one standard deviation from the long-term mean. On the other hand, in northern Poland, the February&ndash;March temperatures in the 16th century were, on average, comparable to those of the present. Most available temperature reconstructions for Poland reveal cooling over the last few decades of the 16th century, particularly during the winter half-year. The climate in the 16<sup>th</sup> century was more continental than it is today.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1172</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1172/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139226</identifier>
    <datestamp>2026-03-06</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[Liquid Polymer Enhances Methanogenesis and Restructures Prokaryotic Communities in Freshwater Sediments]]></dc:title>
      <dc:creator>Feckler, Alexander</dc:creator>
      <dc:creator>Bollinger, Eric</dc:creator>
      <dc:creator>Unik, Alexandra</dc:creator>
      <dc:creator>Mueller, Peter</dc:creator>
      <dc:creator>Filker, Sabine</dc:creator>
      <dc:creator>Plicht, Christian</dc:creator>
      <dc:creator>Steinmetz, Zacharias</dc:creator>
      <dc:creator>Bundschuh, Mirco</dc:creator>
      <dc:description><![CDATA[<p style="font-weight: 400;"><span>The widespread use of synthetic hydrophilic polymers, such as polyvinylpyrrolidone (PVP), has raised concerns about their potential effects on environmental biogeochemical processes, yet their impact on sediment ecosystems remains largely unexplored. We investigated how PVP influences methane (CH<sub>4</sub>) production and prokaryotic community composition in freshwater sediments over a 56-day anoxic incubation. PVP exposure accelerated the onset of methanogenesis, increased maximum CH<sub>4</sub> production rates, and elevated maximum CH<sub>4</sub> concentrations. These functional changes were accompanied by shifts in bacterial communities, particularly an enrichment of fermentative Clostridia, which generate key substrates for methanogens (</span><span>H₂, acetate, and formate</span><span>). Nonetheless, archaeal communities, including methanogens, exhibited comparatively minor or transient responses. Mechanistically, enhanced CH<sub>4</sub> production likely resulted from a combination of increased substrate availability, altered redox microenvironments, and indirect reductions in competing electron acceptors. Our results suggest that PVP modifies sediment carbon cycling through complex microbial, biogeochemical, and physical interactions rather than direct toxicity to methanogens. These findings highlight the need to consider both chemical and physical effects of synthetic hydrophilic polymers on sediment microbial ecosystems and greenhouse gas emissions, and they underscore the importance of targeted studies to quantify these impacts in natural environments.</span>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1216</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1216/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139050</identifier>
    <datestamp>2026-03-06</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[High-resolution mapping of air quality across Europe: an ensemble machine and deep learning framework integrating multi-scale spatial predictors (CHROMAP v1.0)]]></dc:title>
      <dc:creator>Guion, Antoine</dc:creator>
      <dc:creator>Gressent, Alicia</dc:creator>
      <dc:creator>Descombes, Gaël</dc:creator>
      <dc:creator>Janati, Yassine</dc:creator>
      <dc:creator>Real, Elsa</dc:creator>
      <dc:creator>Ung, Anthony</dc:creator>
      <dc:creator>Meleux, Frédérik</dc:creator>
      <dc:creator>Schucht, Simone</dc:creator>
      <dc:creator>Colette, Augustin</dc:creator>
      <dc:description><![CDATA[This article presents a model for mapping air quality at high-resolution (called CHROMAP) based on the fusion of data from deterministic models, in-situ and satellite observations, and spatial proxies using an ensemble of ML and DL algorithms. Annual estimates of the SOMO35 indicator and the average concentrations of NO<sub>2</sub>, PM2.5, PM10, and O<sub>3</sub> are produced and evaluated for the 2013&ndash;2023 period at a spatial resolution of 500 meters over the European domain. The methodology maintains consistency across all pollutant indicators while ensuring flexibility and transferability.</p> <p>By including interpretable AI diagnostics, CHROMAP provides a quantitative assessment of the importance of the 26 features over 11 years for each air quality indicator. Integrating all types of stations into the regressions, the evaluation carried out reveals that the performance scores have been significantly improved compared to CAMS reanalyses (~10 km resolution) used for downscaling; with a reduction in RRMSE on average over the period of about -33 % for NO<sub>2</sub>, -21 % for O<sub>3</sub>, -10 % for SOMO35, -22 % for PM2.5 and -37 % for PM10, and an increase in R<sup>2</sup> of 28 %, 34 %, 18 %, 14 % and 36 %, respectively. In addition, a sensitivity analysis carried out on the static exposure of the population shows that significant differences can be found with values at high resolution, especially for NO<sub>2</sub>, thus impacting the calculation of the health impact.</p> <p>By ensuring sufficient availability of in-situ observations and concentration fields from CTMs for downscaling, this methodology could be extended to additional air quality indicators and applied at higher temporal frequency, opening new opportunities for comprehensive air quality assessment.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1109</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1109/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138364</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[On spatial scales of local aerosol production in boreal ecosystems]]></dc:title>
      <dc:creator>Ezhova, Ekaterina</dc:creator>
      <dc:creator>Rannik, Üllar</dc:creator>
      <dc:creator>Tuovinen, Santeri</dc:creator>
      <dc:creator>Garmash, Olga</dc:creator>
      <dc:creator>Peräkylä, Otso</dc:creator>
      <dc:creator>Ke, Piaopiao</dc:creator>
      <dc:creator>Laanti, Topi</dc:creator>
      <dc:creator>Lintunen, Anna</dc:creator>
      <dc:creator>Kerminen, Veli-Matti</dc:creator>
      <dc:creator>Rinne, Janne</dc:creator>
      <dc:creator>Vesala, Timo</dc:creator>
      <dc:creator>Kulmala, Markku</dc:creator>
      <dc:description><![CDATA[Quantification of the climate impact of land use is important for the development of effective climate change mitigation and adaptation practices. Ecosystems emit compounds that participate in the formation and growth of aerosol particles. Particles of few nm size can be produced locally as compared to regional aerosol growth processes at larger sizes, and in boreal environment, higher concentrations of small particles were observed over agricultural lands than over forests. The aim of this study is to provide estimates of spatial scales of an ecosystem needed to produce small particles predominantly from own emissions. Here, we consider forest and agricultural ecosystems, and distinguish situations in which aerosol production is relatively slow and vertically distributed within the well-mixed boundary layer and when it can occur quickly close to the surface. For the latter, we introduce source contribution function of local aerosol production, which is based on the concentration footprint function modified to account for aerosol growth. We quantify the contributing area for neutral stratification and a typical wind speed. For below-canopy forest, the relevant distance is at 100&ndash;500 m, whereas it is at 0.9&ndash;5.5 km in agricultural fields, depending on the growth rate and the initial size distribution. For the distribution close to measurements, the contribution of the nearby 100&ndash;500 m is approximately 30 % in agricultural fields. To improve estimates, more research is needed on the dynamics of small aerosol, including contributions of chemical compounds to aerosol growth and the impact of meteorological conditions.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-704</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-704/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere139162</identifier>
    <datestamp>2026-03-06</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[Invertebrate communities on seasonal snow patches in the European lowlands are shaped by tree canopy-derived organic inputs]]></dc:title>
      <dc:creator>Lukashanets, Dzmitry</dc:creator>
      <dc:creator>Zawierucha, Krzysztof</dc:creator>
      <dc:creator>Petkuvienė, Jolita</dc:creator>
      <dc:creator>Overlingė, Donata</dc:creator>
      <dc:creator>Vaičiūtė, Diana</dc:creator>
      <dc:creator>Kalvaitienė, Greta</dc:creator>
      <dc:creator>Kataržytė, Marija</dc:creator>
      <dc:description><![CDATA[The cryosphere encompasses a wide range of habitats that support cold-adapted communities. Seasonal snow patches (SSPs) in lowlands are underexplored cryohabitats, characterized by a short persistence period (late winter&ndash;early spring) and the presence of trees around, in contrast to large vegetation-free high-mountain and polar ecosystems. To provide the first assessment of organisms from SSPs, we focused on invertebrate diversity and densities from 40 sites in the Baltic States in relation to physicochemical parameters (i.e., suspended solids, chlorophyll a, nutrients), microalgae, and surrounding landscape features (i.e., tree canopy cover). SSPs appeared to be an important spot for bdelloid rotifers (Bdelloidea), tardigrades (Tardigrada), and nematodes (Nematoda), which together accounted for 60&ndash;100 % of all invertebrates, reaching densities &gt;7,000 ind∙m<sup>-2</sup>. Acari and Insecta were less abundant, whereas other invertebrates occurred only sporadically. The community was strongly determined by surroundings (trees), which supply snow ecosystems with organic and inorganic matter. Chlorophyll a, particulate phosphorus, total suspended solids and organic debris were strongest predictors of invertebrate distribution. The canopy cover also influenced invertebrate communities, highlighting the importance of the organic deposition from trees and also suggesting that trees may be a source of microscopic invertebrates to the snow. Results demonstrate the importance of SSPs as overlooked ephemeral habitats and can be used as a baseline for future changes in snow communities in temperate regions.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1173</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1173/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138924</identifier>
    <datestamp>2026-03-06</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[Implementing a Modern Hybrid Geology Curriculum: A Case Study from a South African University]]></dc:title>
      <dc:creator>Tibane, ﻿Lowanika Victor</dc:creator>
      <dc:creator>Ndebele, Clever</dc:creator>
      <dc:description><![CDATA[Contemporary geology education is increasingly required to advance adaptability, intellectual agility, and professional competence in response to 21<sup>st</sup> century societal and industry needs. Whilst quality assurance and accountability frameworks underscore employability, limited clarity remains regarding the alignment between university geology curricula and the evolving societal and industry demands. This study examined the implementation of a geology curriculum at a recently established university in the Northern Cape Province of South Africa using a hybrid learning model. The model incorporated conventional face to face interactive discussions with pre-recorded online learning materials leveraging smart technologies to support authentic, personalised learning. The implementation efficacy was evaluated through solicited comments from external examiners, peer reviews, institutional and industry experts, and by using students&rsquo; performance and feedback. Students&rsquo; learning was evaluated through moderated online and in person theoretical assessments, complemented by field and laboratory-based practicals, and ultimately looking at pass rates. In contrast, students&rsquo; feedback was collected anonymously using a suggestion box and by following a standardised institutional questionnaire designed for quality promotion and assurance evaluation, administered at the end of 2025. Statistical triangulation across the diverse data sources show that the hybrid delivery model can enhance students&rsquo; theoretical comprehension, practical competencies, preparedness for professional practice, and sustainable societal involvement. The study contributes empirical evidence from a resource constrained and under researched context, demonstrating how aligned hybrid curriculum design can strengthen teaching, learning, and assessment practices in geology education. These insights inform ongoing debates on curriculum innovation, quality assurance, and industry relevance in higher education.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1008</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1008/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138909</identifier>
    <datestamp>2026-03-06</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[Biogeochemical controls on nutrient fluxes in small tropical mountainous river basins: Mechanisms for P-limitation and Si-rich conditions]]></dc:title>
      <dc:creator>Badimela, Upendra</dc:creator>
      <dc:creator>Reddy, Kiran Kumar</dc:creator>
      <dc:creator>Kamaraj, Jesuraja</dc:creator>
      <dc:creator>Manohar, Ciba</dc:creator>
      <dc:creator>Suresh, Vidya</dc:creator>
      <dc:creator>Perumbully, Vinnetha</dc:creator>
      <dc:creator>Krishnan, Anoop</dc:creator>
      <dc:description><![CDATA[Small scale mountainous rivers with their quick flowing mechanisms provide a clear understanding on the nutrient flux dynamics in assessing their role in biogeochemical cycles and coastal nutrient budgets. The present study examines the spatio-temporal variability of dissolved inorganic nutrients in the Karamana River Basin (KRB) and Vamanapuram River Basin (VRB), flowing through Western Ghats, which emphasis the hydro geochemistry, segment-wise nutrient fluxes, and their biogeochemical cycle implications. The results reveal marked spatio-temporal variability in nutrient fluxes similar to the hydrochemistry, with higher fluxes generally recorded during the MON due to enhanced runoff and weathering. The segment-wise average fluxes of DIN, DIP, and DSi in the KRB were estimated at 6.84, 0.05, and 127.25 kg ha<sup>-1</sup> yr<sup>-1</sup>, respectively. In comparison, the corresponding values for the VRB were 9.44, 0.07, and 81.66 kg ha⁻&sup1; yr⁻&sup1;, respectively. A clear indication of low concentration conditions in the upstream followed by slight enrichment in the mid and downstream regions further highlight pristine environment and the role of land use and anthropogenic influence, respectively. The stagnant conditions after reaching the downstream regions with favorable tropical climate conditions promoting the consumption of nutrients through in-situ production. The DSi flux of VRB (127.25 kg ha<sup>-1</sup> yr<sup>-1</sup>) is comparable to that of large global rivers such as the Amazon (108.6 kg ha<sup>-1</sup> yr<sup>-1</sup>) and Mississippi (118.21 kg ha<sup>-1</sup> yr<sup>-1</sup>), further supports the claim of intense chemical weathering derived silica-rich conditions. Overall, the study highlights the critical role of climate and topography in regulating nutrient fluxes and confirms that nutrient inputs from these small-scale mountainous rivers have a relatively limited influence on coastal eutrophication in the receiving zones.]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-995</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-995/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:amt127402</identifier>
    <datestamp>2026-03-06</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 reflected shortwave anisotropy on satellite radiometer measurements of the Earth's energy imbalance]]></dc:title>
      <dc:creator>Hocking, Thomas</dc:creator>
      <dc:creator>Megner, Linda</dc:creator>
      <dc:creator>Hakuba, Maria</dc:creator>
      <dc:creator>Mauritsen, Thorsten</dc:creator>
      <dc:description><![CDATA[<p>The Earth's energy imbalance is the difference between incoming solar radiation and outgoing reflected and emitted radiation from the Earth, and quantifies the current ongoing accumulation of energy in the Earth's climate system. There are indications that the imbalance is growing, and it is important to be able to measure and monitor this quantity to better constrain future changes. The reflected shortwave component of the outgoing radiation depends on surface and atmospheric properties, which leads to strong directional variations associated with the angular geometry relative to the incoming sunlight and the observer. The effect of this anisotropy on global average measurements from wide-field-of-view radiometers has been the topic of some investigation in the past, and results from an earlier study suggest that this effect could potentially lead to substantial systematic biases in the context of the global mean reflected shortwave radiation. Here we simulate wide-field-of-view instruments on satellites in polar, sun-synchronous and precessing orbits, as well as constellations of these types of satellite orbits, with both Lambertian and anisotropic shortwave reflection. Reference top-of-atmosphere radiative fluxes are taken from the Clouds and the Earth's Radiant Energy System synoptic data product and combined with angular dependence models that were developed for the Earth Radiation Budget Experiment. We find that the polar regions appear brighter and the midlatitudes appear dimmer with anisotropic reflection, but both the estimated global annual mean and the estimated interannual trend only exhibit limited sensitivity to whether Lambertian or anisotropic reflection is assumed. With anisotropic reflection, the estimated global annual mean root-mean-square sampling error is at most 0.11 <span class="inline-formula">W m<sup>−2</sup></span> provided that at least two complementary satellites are used, compared with at most 0.09 <span class="inline-formula">W m<sup>−2</sup></span> in the case of Lambertian reflection. The magnitude of the difference in the estimated interannual trend is at most 0.07 <span class="inline-formula">W m<sup>−2</sup></span> per decade, and typically only <span class="inline-formula">∼</span> 0.01 <span class="inline-formula">W m<sup>−2</sup></span> per decade. Analysis of the angular sampling of these satellites reveals that the anisotropic reflection requires sufficient sampling of viewing zenith angle and relative azimuth angle, in addition to the solar zenith angle. However, we conclude that it is possible to choose satellite orbits so that the sampling error is not substantially affected by reflected shortwave anisotropy.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-1643-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/1643/2026/]]></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:amt131257</identifier>
    <datestamp>2026-03-06</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[Aerosol Composition and Extinction of the 2022 Hunga Plume Using CALIOP]]></dc:title>
      <dc:creator>Duchamp, Clair</dc:creator>
      <dc:creator>Legras, Bernard</dc:creator>
      <dc:creator>Podglajen, Aurélien</dc:creator>
      <dc:creator>Sellitto, Pasquale</dc:creator>
      <dc:creator>Bourassa, Adam E.</dc:creator>
      <dc:creator>Rozanov, Alexei</dc:creator>
      <dc:creator>Taha, Ghassan</dc:creator>
      <dc:creator>Zawada, Daniel J.</dc:creator>
      <dc:description><![CDATA[<p>We use the CALIOP (Cloud-Aerosol Lidar with Orthogonal Polarization) instrument to determine the microphysical properties of the stratospheric aerosol plume after the Hunga eruption in 2022, the largest so far after the Pinatubo in 1991.  In the early stages, low depolarization (<span class="inline-formula">&lt;2 <i>%</i></span>) is found everywhere except in patches of high depolarization (up to 35 %) detected within the plumes of sulfur compounds up to 3 d after the eruption.  As standard CALIOP L2 products are not operational in the case of the Hunga aerosol plume, we implement an iterative method of successive approximations to retrieve extinction profiles, by estimating the aerosol optical depth (AOD) and then the lidar ratio (LR). The AOD of the plume at 532 nm is between 0.5 and 1.25 on the first four days, then decreases rapidly and stabilizes at <span class="inline-formula">0.047 ± 0.011</span> for March 2022. The LR is initially between 60 and 80 sr, consistent with the early growth of sulfate aerosol particles, and then decreases to <span class="inline-formula">48 ± 6 sr</span> between late January and late March 2022.  Results are compared and validated with the solar occultation instrument SAGE III (Stratospheric Aerosol and Gas Experiment) on board the International Space Station (ISS) and Mie calculations. A comparison with limb-viewing instruments highlights significant quantitative disagreements in extinction and AOD estimates, which we attribute, in part, to the unusual size distribution of the aerosols within the Hunga plume.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-1675-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/1675/2026/]]></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:acp131789</identifier>
    <datestamp>2026-03-06</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: Observational analysis of mode-dependent fog droplet size distribution evolution and improved parameterization using segmented gamma and lognormal fitting]]></dc:title>
      <dc:creator>Zhang, Jingwen</dc:creator>
      <dc:creator>Liu, Xiaoli</dc:creator>
      <dc:creator>An, Zhenya</dc:creator>
      <dc:creator>Lv, Jingjing</dc:creator>
      <dc:creator>Xu, Dan</dc:creator>
      <dc:description><![CDATA[<p>Fog droplet size distributions (DSDs) evolve under the influence of many physical processes, yet their development through the fog lifecycle remains insufficiently understood and challenging to represent in numerical models, constraining the accuracy of fog forecasting. To improve understanding of the fog evolution, field observations under a polluted background were conducted during winters from 2006–2009 and 2017–2018 in Nanjing, China. Among the 27 observed fog events, microphysical properties including fog droplet number concentration (<span class="inline-formula"><i>N</i><sub>f</sub></span>), liquid water content (LWC), volume-mean radius (<span class="inline-formula"><i>R</i><sub>v</sub></span>), and effective radius (<span class="inline-formula"><i>R</i><sub>eff</sub></span>) varied substantially. Unimodal, bimodal, and trimodal DSDs were observed, with mode separating diameters of 2 <span class="inline-formula">µ</span>m for unimodal; 2 and 6–18 <span class="inline-formula">µ</span>m for bimodal; and 2, 6–12, and 18–26 <span class="inline-formula">µ</span>m for trimodal DSDs. Both the number of modes and the mode separating diameters vary over the fog life cycle, with more frequent and pronounced changes occurring during fog formation and dissipation or during periods of strong fluctuations in <span class="inline-formula"><i>N</i><sub>f</sub></span> and LWC. Compared with unimodal DSDs, bimodal and trimodal DSDs exhibited broader PDF distributions of LWC, <span class="inline-formula"><i>R</i><sub>v</sub></span> and <span class="inline-formula"><i>R</i><sub>eff</sub></span>. Based on these observational features, segmented gamma and lognormal fits were applied to mean DSDs using partition points at 10 and 20 <span class="inline-formula">µ</span>m. Comparisons between microphysical parameters derived from the fitted DSD and observations show that three-segment fitting improved estimates of <span class="inline-formula"><i>N</i><sub>f</sub></span> and LWC, while substantially enhanced the representation of <span class="inline-formula"><i>R</i><sub>eff</sub></span>, absorption coefficient, and optical thickness, reducing deviations from up to 90 % to within 20 %.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-3489-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/3489/2026/]]></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:acp131237</identifier>
    <datestamp>2026-03-06</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[Characterization of the annual cycle of atmospheric aerosol over Mindelo, Cabo Verde, by means of continuous multiwavelength lidar observations]]></dc:title>
      <dc:creator>Gebauer, Henriette</dc:creator>
      <dc:creator>Floutsi, Athena Augusta</dc:creator>
      <dc:creator>Hofer, Julian</dc:creator>
      <dc:creator>Haarig, Moritz</dc:creator>
      <dc:creator>Skupin, Annett</dc:creator>
      <dc:creator>Engelmann, Ronny</dc:creator>
      <dc:creator>Jimenez, Cristofer</dc:creator>
      <dc:creator>Wagner, Robert</dc:creator>
      <dc:creator>Baars, Holger</dc:creator>
      <dc:description><![CDATA[<p>This paper presents an analysis of the annual cycle of aerosol optical and geometrical properties based on multiwavelength-Raman-polarization lidar measurements for Mindelo, Cabo Verde, from July 2021 to August 2023. A quality-assured data set of more than 70 automatically-calibrated lidar profiles was manually evaluated. For the first time, a two-year time series of, e.g. layer-resolved aerosol optical depth (AOD), lidar ratio profiles, and particle depolarization profiles are presented for Cabo Verde to characterize the complete annual cycle of aerosol in the planetary boundary layer (PBL) and in the lofted aerosol layers. The aerosol conditions over Mindelo are complex with different mixing states of dust and non-dust components. A strong annual cycle was found in the overall aerosol layer top height and the geometrical extent, the AOD, and the dust fraction of the lofted layers. Furthermore, the data was used to explicitly define aerosol-related seasons. The dust season (June–September) is characterized by geometrically and optically thick lofted layers dominated by Saharan dust (up to 7 <span class="inline-formula">km</span> height) above a slightly polluted marine PBL. Seasonal mean lidar ratios at 355(532) <span class="inline-formula">nm</span> are <span class="inline-formula">34±18</span> (<span class="inline-formula">32±19</span>) <span class="inline-formula">sr</span> (PBL) and <span class="inline-formula">48±19</span> (<span class="inline-formula">39±18</span>) <span class="inline-formula">sr</span> (lofted layers). The particle depolarization ratio is <span class="inline-formula">&lt;0.05</span> (PBL) and <span class="inline-formula">0.16±0.07</span>, <span class="inline-formula">0.22±0.06</span>, and <span class="inline-formula">0.20±0.05</span> (lofted layers) at 355, 532, and 1064 <span class="inline-formula">nm</span>. The mixing season (often mixtures of Saharan dust with biomass burning aerosol, November–March) is characterized by a large variability of aerosol with mean lidar ratios of <span class="inline-formula">60±32</span> (<span class="inline-formula">48±32</span>) <span class="inline-formula">sr</span> at 355 (532) <span class="inline-formula">nm</span> and depolarization ratios of <span class="inline-formula">0.09±0.06</span>, <span class="inline-formula">0.11±0.07</span>, and <span class="inline-formula">0.16±0.08</span> at 355, 532, and 1064 <span class="inline-formula">nm</span> in the lofted layers.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-3439-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/3439/2026/]]></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:acp132903</identifier>
    <datestamp>2026-03-06</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: Three-year characteristics of sulfuric acid in urban Beijing and derivation of daytime sulfuric acid proxies applicable to inland sites]]></dc:title>
      <dc:creator>Guo, Yishuo</dc:creator>
      <dc:creator>Yan, Chao</dc:creator>
      <dc:creator>Li, Chang</dc:creator>
      <dc:creator>Deng, Chenjuan</dc:creator>
      <dc:creator>Zhang, Ying</dc:creator>
      <dc:creator>Zhou, Ying</dc:creator>
      <dc:creator>Zheng, Haotian</dc:creator>
      <dc:creator>Jiang, Yueqi</dc:creator>
      <dc:creator>Chen, Xin</dc:creator>
      <dc:creator>Ma, Wei</dc:creator>
      <dc:creator>Sarnela, Nina</dc:creator>
      <dc:creator>Lin, Zhuohui</dc:creator>
      <dc:creator>Hua, Chenjie</dc:creator>
      <dc:creator>Fan, Xiaolong</dc:creator>
      <dc:creator>Zheng, Feixue</dc:creator>
      <dc:creator>Feng, Zemin</dc:creator>
      <dc:creator>Wang, Zongcheng</dc:creator>
      <dc:creator>Zhang, Yusheng</dc:creator>
      <dc:creator>Jiang, Jingkun</dc:creator>
      <dc:creator>Zhao, Bin</dc:creator>
      <dc:creator>Kulmala, Markku</dc:creator>
      <dc:creator>Liu, Yongchun</dc:creator>
      <dc:description><![CDATA[<p>Sulfuric acid (H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span>) is a key precursor in atmospheric new particle formation and cluster early growth. However, long-term measurement of it is only available at a few sites. Although several proxies for estimating H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> concentration have been proposed, they are always site-specific. Therefore, both reliable H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> measurement and proxies with wider application are highly needed. Here, we conducted a long-term H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> measurement in urban Beijing during 2019–2021, and derived three H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> proxies based entirely on its formation and loss pathways. Results show that daytime H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> concentration is 2.0–<span class="inline-formula">7.4×10<sup>6</sup></span> molec. cm<span class="inline-formula"><sup>−3</sup></span> and shows an overall decline with an average annual decrease of 14 %. This decline is mainly due to the ongoing SO<span class="inline-formula"><sub>2</sub></span> emission controls. Daytime H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> shows a clear seasonal variation that tracks UVB. Nighttime H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> concentration is 1.6–<span class="inline-formula">6.3×10<sup>5</sup></span> molec. cm<span class="inline-formula"><sup>−3</sup></span>, with higher levels in warmer seasons due to stronger sources and lower condensation sink (CS). The diurnal variations of H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> across seasons follow those of photo-oxidation-related parameters, such as UVB, OH radical, and photolysis rate of NO<span class="inline-formula"><sub>2</sub></span> (J(NO<span class="inline-formula"><sub>2</sub></span>)). All of the three proxies can reproduce H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> concentration during 10:00–14:00 LT. Importantly, they can estimate H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> concentration at a boreal forest site in Hyytiälä, Finland, suggesting their applicability to sites with diverse environments. Furthermore, the parameters used in UVB-PM<span class="inline-formula"><sub>2.5</sub></span> based proxy are available at most observational sites. Further application of this proxy could provide H<span class="inline-formula"><sub>2</sub></span>SO<span class="inline-formula"><sub>4</sub></span> concentrations covering many regions worldwide, which may further facilitate research on atmospheric nucleation and secondary aerosol growth of these sites.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-3467-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/3467/2026/]]></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:gh135143</identifier>
    <datestamp>2026-03-06</datestamp>
    <setSpec>gh</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[Between faith and nature: sacred landscapes of  South Tyrol in nineteenth-century travel accounts]]></dc:title>
      <dc:creator>Brocada, Lorenzo</dc:creator>
      <dc:description><![CDATA[<p>This paper examines how religion, landscape, and identity intersected in the nineteenth-century South Tyrol using a cultural and historical geography perspective. It primarily draws on travel writings, complemented by iconographic sources, to show how sacred inscriptions shaped spatial relations, collective identities, and mobility across the Alpine region. The analysis distinguishes between local expressions of devotion and perceptions brought by foreign travellers, revealing the interaction between lived religious practices and external representations. Treating the sacred as a spatial language mediating human–environment interactions, the study argues that sacredness is not a fixed property of place but a relational process embedded in social, symbolic, and territorial dynamics. These findings inform broader debates on the spatiality of faith and the role of religious imaginaries in forming cultural landscapes and regional identities in Europe.</p>]]></dc:description>
      <dc:date>2026-03-06</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gh-81-155-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gh.copernicus.org/articles/81/155/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-8798</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:nhess131244</identifier>
    <datestamp>2026-03-05</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[The EAWS matrix, a decision support tool to determine the regional avalanche danger level (Part B): operational testing and use]]></dc:title>
      <dc:creator>Techel, Frank</dc:creator>
      <dc:creator>Müller, Karsten</dc:creator>
      <dc:creator>Marquardt, Christopher</dc:creator>
      <dc:creator>Mitterer, Christoph</dc:creator>
      <dc:description><![CDATA[<p>To support public safety and risk management in snow-covered mountains, regional avalanche forecasts must deliver reliable information on avalanche conditions, including regional danger levels representing the avalanche danger across warning regions. To promote greater transparency and consistency in avalanche danger level assessment across European avalanche warning services, a revised version of the EAWS Matrix was developed based on expert elicitation. The Matrix, a structured decision support tool that combines the Matrix input factors snowpack stability, the frequency of snowpack stability, and avalanche size, is used to determine the regional danger level. To support the development of the Matrix described in detail in the companion paper <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx23">Müller et al.</a>, <a href="#bib1.bibx23">2025</a>)</span>, we analyzed its operational use over the first three winters following implementation by 26 European avalanche warning services. Our aim was to identify inconsistencies in Matrix application and to provide empirically based guidance for further refinement. In operational use, forecasters predominantly assigned a consistent single danger level to most Matrix input factor combinations. However, two factor combinations (<i>poor-some-size 2</i> and <i>very poor-some-size3</i>) were commonly assigned to one of two adjacent danger levels, indicating that these combinations function as transition zones between danger levels. Analyses based on finer-grained assessments of the input factors, that is, using sub-classes of the predefined coarse factor categories, revealed systematic tendencies within these classes. While application of the Matrix was relatively consistent for avalanche problems relating to dry-snow conditions, pronounced inconsistencies emerged in the classification of snowpack stability for wet-snow and gliding snow avalanche problems. These findings underscore the need for community-wide discussion and harmonization in Matrix application, particularly with respect to stability assessment practices. Assessing input factors at a finer scale shows potential for preserving important nuances in expert judgment and may enable more targeted guidance on when to assign the higher or lower of two danger levels indicated by the Matrix. However, because neither the danger level nor its input factors can be measured independently, a formal validation of Matrix logic and operational application is not possible. Despite some inconsistencies, our results suggest that European forecasters generally align with the Matrix logic, supporting its operational utility.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-1161-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/1161/2026/]]></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:nhess133070</identifier>
    <datestamp>2026-03-05</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[The 15 September 2022 floods in northern Marche (Central Italy): disaster analysis, case studies and mitigation strategies for hydro-geomorphological hazard]]></dc:title>
      <dc:creator>Bendia, Fabrizio</dc:creator>
      <dc:creator>Farabollini, Piero</dc:creator>
      <dc:creator>Materazzi, Marco</dc:creator>
      <dc:creator>Bufalini, Margherita</dc:creator>
      <dc:description><![CDATA[<p>On 15 and 16 September 2022, a large area of the Marche region in central Italy experienced an exceptionally heavy rainfall event, with nearly 420 mm of rain falling in just six hours. The intense rains, in addition to causing 13 fatalities, triggered a large number of landslides in the mountain areas and flood events, mainly concentrated along the valleys of the hydrographic basins of the Metauro, Cesano, Misa, and Esino Rivers. The physiographic setting of the territory and the poor maintenance of both the main and secondary hydrographic network, often insufficient or entirely absent, exacerbated an already exceptional event. Although extraordinary, the natural event occurred in an area already affected by intense meteoric events in the past, the most recent of which had taken place just eight years earlier, in 2014.</p>        <p>This study presents the results of the systematic and detailed surveys conducted in several sites affected by the storm, also providing detailed case studies. These surveys highlighted the critical issues detected during the disaster and identified appropriate intervention measures for reducing hydraulic risk in the Region. Many of these measures are innovative and will serve as guidelines for future land-use planning and for improving public education and awareness in flood-prone areas.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-1119-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/1119/2026/]]></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:nhess133184</identifier>
    <datestamp>2026-03-05</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[Mitigating Mazuku hazards: implementation and effectiveness of local dry-gas degassing measures in the Goma area (Virunga Volcanic Province)]]></dc:title>
      <dc:creator>Mafuko-Nyandwi, Blaise</dc:creator>
      <dc:description><![CDATA[<p>Mitigation of carbon dioxide diffuse degassing hazards remains underexplored in comparison to other volcanic hazards such as eruptions, despite their persistent and deadly impacts on communities living in active volcanic regions. This study uses a mixed-methods approach – combining quantitative surveys and qualitative interviews – to assess household perceptions of the implementation and effectiveness of risk mitigation measures against <i>mazuku</i>, a locally known hazard caused by emissions of carbon dioxide in the western part of Goma, Virunga Volcanic Province. Data were collected across three sampling zones, capturing demographic characteristics, eruption risk experiences, and perceptions regarding the implementation of mazuku risk mitigation measures.</p>        <p>Findings reveal three locally recognised categories of mitigation measures: (1) emission-limiting measures, such as blocking gas with waste materials; (2) adaptive measures, such as house ventilation or living on upper floors; and (3) awareness measures based on orally transmitted local knowledge such as avoiding mazuku zone early morning. Financial resources, gender and prior risk experience – often linked to length of residence – emerged as significant positive determinants of both motivation and perceived efficacy for the first two categories. Perceptions of awareness measures showed no significant variation across zones even between demographic profile groups. Spatial patterns in perceived implementation and perceived efficacy appear to reflect collective community mitigation implementation rather than based on individual risk mitigation assessment, with some measures perceived as effective despite limited physical evidence of reduced gas concentration.</p>        <p>The study supports the importance of co-creating mitigation strategies with local communities, adapting interventions to socio-economic realities and avoiding the importation of external mitigation measures that may lack contextual relevance. It also calls for complementary research measuring the actual effectiveness of these measures through physical monitoring of <i>mazuku</i> concentrations. These insights, grounded in a Global South context – characterised by rapid uncontrolled urbanisation, offer a valuable perspective for the development of inclusive and effective strategies of carbon dioxide diffuse degassing risk management.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-1141-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/1141/2026/]]></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:tc122862</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>tc</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 mathematical model of microbially-induced convection in sea ice]]></dc:title>
      <dc:creator>Kraitzman, Noa</dc:creator>
      <dc:creator>Grattepanche, Jean-David</dc:creator>
      <dc:creator>Sanders, Robert</dc:creator>
      <dc:creator>Klapper, Isaac</dc:creator>
      <dc:description><![CDATA[<p>Through its role as an interface between ocean and atmosphere, sea ice is important both physically and biologically. We propose here that the resident microbial community can influence the structure of sea ice, particularly near its ocean interface, by effectively lowering the local freezing point via an osmolytic mechanism. This lowered freezing point can enhance fluid flow, linking a bottom, convective ice layer with the underlying ocean, resulting in improved nutrient uptake and byproduct removal. A mathematical model based on a previously suggested abiotic one dimensional simplification of mushy ice fluid dynamics is used to illustrate, and supporting measurements of freezing point depression by lab grown sea ice-associated organisms are provided.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/tc-20-1445-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/1445/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:tc129914</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>tc</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[Greenland Monthly Accumulation Maps (1960–2022): A Statistical Semi-Empirical Bias-Adjustment Model]]></dc:title>
      <dc:creator>Lindsey-Clark, Josephine</dc:creator>
      <dc:creator>Grinsted, Aslak</dc:creator>
      <dc:creator>Vandecrux, Baptiste</dc:creator>
      <dc:creator>Schøtt Hvidberg, Christine</dc:creator>
      <dc:description><![CDATA[<p>Accurate estimates of snow accumulation over the Greenland ice-sheet are essential for reliable projections of sea-level rise. These are typically obtained from regional climate models, which carry systematic temporal and spatially variable biases, contributing to substantial uncertainties in sea-level rise projections. Here we present a novel statistical-semi-empirical model for bias-correcting gridded accumulation output from any regional climate model or reanalysis product, utilising the SUMup dataset, which provides the most comprehensive spatial and temporal coverage of surface mass balance observations to date. The method employs Empirical Orthogonal Function analysis to decompose the model accumulation output into the dominant patterns of spatial variability and their temporal evolution. Adjustment coefficients derived by fitting SUMup data enable the reconstruction of spatially complete, bias-corrected accumulation fields.</p>        <p>We apply this approach to monthly accumulation output from the HIRLAM–ECHAM Regional Climate Model (HIRHAM5; 1960–2022), the Modèle Atmosphérique Régional (MAR3.14; 1960–2022), the Regional Atmospheric Climate Model (RACMO 2.4p1; 1980–2022), and the Copernicus Arctic Regional Reanalysis (CARRA; 1991–2022). Initial mean point-wise biases of <span class="inline-formula">−</span>7.4 % (HIRHAM), <span class="inline-formula">−</span>0.5 % (MAR), 0.0 % (RACMO) and <span class="inline-formula">+</span>10.1 % (CARRA) (1991–2022), statistically significant for all models except RACMO, are reduced to <span class="inline-formula">±</span> 0.3 % following adjustment. Resulting bias-corrected mean annual accumulation rates over the ice sheet are estimated at 469 mm yr<span class="inline-formula"><sup>−1</sup></span> (HIRHAM), 412 mm yr<span class="inline-formula"><sup>−1</sup></span> (MAR), 435 mm yr<span class="inline-formula"><sup>−1</sup></span> (RACMO) and 408 mm yr<span class="inline-formula"><sup>−1</sup></span> (CARRA) between 1991–2022. Inter-model agreement improves significantly in the observation-rich accumulation zone, with a 68 % reduction in standard deviation of mean accumulation estimates, but deteriorates by 27 % in the sparsely sampled ablation zone, highlighting the need for additional observational constraints. Model bias is dominated by the southern ice sheet, with the largest statistically significant contributions from the south-east for HIRHAM (<span class="inline-formula">−</span>39 to <span class="inline-formula">−</span>54 Gt yr<span class="inline-formula"><sup>−1</sup></span>) and MAR (<span class="inline-formula">+</span>30 to <span class="inline-formula">+</span>33 Gt yr<span class="inline-formula"><sup>−1</sup></span>), and the south-west for RACMO (<span class="inline-formula">+</span>20 to <span class="inline-formula">+</span>26 Gt yr<span class="inline-formula"><sup>−1</sup></span>) and CARRA (<span class="inline-formula">+</span>34 Gt yr<span class="inline-formula"><sup>−1</sup></span>). Temporal trends and temperature sensitivities exhibit a pronounced east-west contrast, with the east dominated by strong positive responses and negative responses in the west.</p>        <p>The framework outlined in this study offers a scalable, transferable solution to improve accumulation estimates through enhanced integration of observational data, providing an improved input to ice-sheet models, with the potential to reduce uncertainties in future sea-level rise projections.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/tc-20-1463-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/1463/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:esd131319</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Dynamical system metrics and weather regimes explain the seasonally-varying link between European heatwaves and the large-scale atmospheric circulation]]></dc:title>
      <dc:creator>Dillerup, Ines</dc:creator>
      <dc:creator>Lemburg, Alexander</dc:creator>
      <dc:creator>Buschow, Sebastian</dc:creator>
      <dc:creator>Pinto, Joaquim G.</dc:creator>
      <dc:description><![CDATA[<p>Global warming is projected to increase the frequency and intensity of heatwaves in the extended summer period. To better predict heat extremes, it is important to explore the seasonal variations in their drivers. Therefore, we analyze heatwaves in Central Europe using ERA5 reanalysis data over the historical period (1950–2023) for the extended summer months (May–September). We quantify atmospheric persistence, and the link between near-surface temperatures and large-scale atmospheric circulation patterns using dynamical system metrics. This approach is further contextualized by the consideration of weather regimes, which represent the low-frequency variability of the atmosphere over the North Atlantic and Europe.</p>        <p>Our results show a maximum in atmospheric persistence in July and August, associated with higher occurrence of Scandinavian Blocking, and relative minima in spring and autumn. The relationship between the large-scale atmospheric circulation and near-surface temperatures exhibits similar seasonal characteristics. For heatwave days, we find a statistically significant anomalous strong link between large-scale atmospheric circulation and surface temperatures from June to September. This relationship is generally not attributable to the occurrence of specific weather regimes. However, heatwaves in July and August are associated with higher atmospheric persistence due to an enhanced frequency of the persistent Scandinavian and European blocking weather regimes. Beyond atmospheric circulation, additional physical drivers of daily maximum temperature during heatwaves are analyzed: While surface net solar radiation shows a particularly strong link in June and July, soil moisture exhibits an anomalously high link in July and August. These findings highlight the critical role of intra-seasonal variations in shaping heatwave dynamics.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-265-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/265/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:esd132141</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[An EOF-Based Emulator of Means and Covariances of Monthly Climate Fields]]></dc:title>
      <dc:creator>Geogdzhayev, Gosha</dc:creator>
      <dc:creator>Souza, Andre N.</dc:creator>
      <dc:creator>Flierl, Glenn R.</dc:creator>
      <dc:creator>Ferrari, Raffaele</dc:creator>
      <dc:description><![CDATA[<p>Fast emulators of comprehensive climate models are often used to explore the impact of anthropogenic emissions on future climate. A new approach to emulators is introduced that generates means and covariances of monthly averaged climate variables as a function of global mean surface temperature. The emulator is trained with output from a state-of-the-art climate model and serves as a good first-order representation for the evolution of spatially resolved climate variables and their variability. To train the emulator, data is first projected into a reduced-dimensional space; the emulator then learns the dependence of climate variables on global mean surface temperature in the projected space. To recover climate variables in physical space, an inverse transformation is applied. The resulting emulator can cheaply generate means and variances of climate fields averaged over arbitrarily defined regions and in previously unseen warming scenarios. For illustrative purposes, the emulator is applied to predict changes in the mean and variability of monthly values of both surface temperature and relative humidity as a function of global mean surface temperature changes. However, the approach can be applied to any other variable of interest on yearly, monthly or daily timescales.</p>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-235-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/235/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138925</identifier>
    <datestamp>2026-03-05</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[Extinction, Turnover, and the Reorganization of Diatom Communities Across the Eocene/Oligocene Boundary: Equatorial Atlantic Perspective]]></dc:title>
      <dc:creator>Özen, Volkan</dc:creator>
      <dc:creator>Renaudie, Johan</dc:creator>
      <dc:creator>Lazarus, David</dc:creator>
      <dc:description><![CDATA[<span>Marine diatoms couple the global carbon and silicon cycles, and their fossil record tracks oceanographic and climatic changes in deep-time. The Eocene/Oligocene Transition (EOT) marks the onset of Antarctic glaciation and major ocean reorganization and is a key interval in diatom evolutionary history. Although high-latitude plankton responses to polar cooling are extensively studied, it remains challenging to determine how cooling-driven changes in circulation, stratification and nutrient supply propagated and shaped low-latitude assemblages. Here we reconstruct species-level diatom diversity from exhaustive full-assemblage counts and integrate these data with diatom and radiolarian productivity from Deep Sea Drilling Project (DSDP) Site 366 (Sierra Leone Rise, equatorial Atlantic) spanning 38&ndash;32 Ma. Diatom diversity at DSDP 366 varies in step with Southern Ocean diversity records across the same interval. Extinction rates and community-structure metrics indicate a major reorganization of tropical diatom communities that is consistent with changes in upper-ocean stratification. We identify a sharp shift in community structure at ~33.5 Ma, pointing to a rapid ecological response in the earliest Oligocene.</span>]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1009</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1009/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere137424</identifier>
    <datestamp>2026-03-05</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[Good performance of low-cost carbon dioxide sensor based on intercomparisons with the standard eddy-covariance system]]></dc:title>
      <dc:creator>Rannik, Üllar</dc:creator>
      <dc:creator>Mammarella, Ivan</dc:creator>
      <dc:creator>Vesala, Timo</dc:creator>
      <dc:creator>Väkimies, Pirkko</dc:creator>
      <dc:creator>Heiskari-Tuohiniemi, Hilkka</dc:creator>
      <dc:creator>Korkiakoski, Mika</dc:creator>
      <dc:description><![CDATA[Flux measurements have started to play an important role outside academia in assessing carbon sinks of different ecosystems and land-use types. If natural carbon solutions are to be deployed and monetized in carbon markets, more low-powered and low-cost flux systems should be deployed. There is a growing need for low-cost sensors that still fulfil the requirements for scientific applications. We present a case study where Vaisala company and the University of Helsinki joined their industrial and academic competencies to create an inexpensive yet precise fast-response carbon dioxide (CO<sub>2</sub>) and water vapour (H<sub>2</sub>O) sensor. A working prototype was developed and field-tested against a scientific reference eddy covariance (EC) setup. Special attention was paid to response time, lowered sampling frequency, and auto-calibration related to the temperature. The results at the end of the project were very promising. The enclosed-path EC prototype had a CO<sub>2</sub> response time of 0.18 sec and a noise level of 1 ppm at a 5 Hz sampling rate. The internal auto-calibration procedure was continuously improved such that CO<sub>2</sub> signal drifting was avoided and the instrument was capable of measuring CO<sub>2</sub> fluxes with high correlation relative to the reference EC setup (R<sup>2</sup> = 0.98).]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-144</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-144/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138901</identifier>
    <datestamp>2026-03-05</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[Validation of ceilometer aerosol profile retrievals using sun&ndash;sky photometer and balloon-borne in situ measurements]]></dc:title>
      <dc:creator>Muñiz-Rosado, Jorge</dc:creator>
      <dc:creator>Cazorla, Alberto</dc:creator>
      <dc:creator>Sauvageat, Eric</dc:creator>
      <dc:creator>Haefele, Alexander</dc:creator>
      <dc:creator>Herrero del Barrio, Celia</dc:creator>
      <dc:creator>González, Ramiro</dc:creator>
      <dc:creator>Román, Roberto</dc:creator>
      <dc:creator>Molina-Molero, Pedro Luis</dc:creator>
      <dc:creator>Díaz-Zurita, Arlett</dc:creator>
      <dc:creator>Naval-Hernández, Victor Manuel</dc:creator>
      <dc:creator>Rodríguez, Onel</dc:creator>
      <dc:creator>Granados-Muñoz, María José</dc:creator>
      <dc:creator>Bravo-Aranda, Juan Antonio</dc:creator>
      <dc:creator>Herrera, Milagros</dc:creator>
      <dc:creator>Pérez-Ramírez, Daniel</dc:creator>
      <dc:creator>Doppler, Lionel</dc:creator>
      <dc:creator>Alados-Arboledas, Lucas</dc:creator>
      <dc:creator>Navas-Guzman, Francisco</dc:creator>
      <dc:description><![CDATA[This study evaluates two approaches for retrieving aerosol properties from ceilometer observations, using aerosol optical depth (AOD) from AERONET and synergistic aerosol profiles obtained by combining AERONET sun&ndash;sky photometer and ceilometer measurements through the GRASP<sub>pac</sub> algorithm as reference. The two retrieval techniques considered for the ceilometer retrievals are the traditional Klett-Fernald backward inversion and a forward iterative method including an independent calibration procedure. Observations collected at three European stations (Granada, Spain; Payerne, Switzerland; and Lindenberg, Germany) during 2019&ndash;2020 are analyzed to assess the performance of both approaches under a wide range of aerosol conditions. The results show that the forward iterative method systematically outperforms the Klett-Fernald backward approach. Under high aerosol load conditions, particularly during coarse-mode-dominated events, the forward retrieval reduces AOD uncertainties by ~50 % and achieves root-mean-square errors comparable to those reported in previous validation studies. Vertical comparisons against GRASP<sub>pac</sub> profiles indicate that the forward method maintains consistent accuracy throughout the troposphere, whereas the backward approach exhibits altitude-dependent biases, especially within dust layers. Additional evaluations using COBALD balloon-borne backscatter measurements confirm that the forward retrieval reproduces observed aerosol structures within 10&ndash;30~% deviation. These results demonstrate the significant performance gains achieved by operational ceilometer networks when applying forward retrievals with independent calibration under favorable atmospheric conditions.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-990</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-990/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138336</identifier>
    <datestamp>2026-03-05</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[Isotopic Evidence for Ice Growth by Riming in Precipitation]]></dc:title>
      <dc:creator>Aggarwal, Pradeep K.</dc:creator>
      <dc:creator>Schumacher, Courtney</dc:creator>
      <dc:creator>Longstaffe, Frederick J.</dc:creator>
      <dc:creator>Funk, Aaron</dc:creator>
      <dc:creator>Shupe, Matthew D.</dc:creator>
      <dc:description><![CDATA[In this study, we investigate the impact of riming on the relative composition of oxygen and hydrogen isotopes or d-excess in precipitation. Riming, where supercooled liquid droplets freeze directly on ice particles, is an important process of precipitation formation in mixed-phase clouds but has long been assumed to occur without isotopic fractionation. We used an independent indicator of riming, the terminal fall velocity of snow particles, and correlated it with the d-excess of snow or rain precipitation (ranging from &ndash;23 to +45 &permil;) in polar (Arctic, Antarctic), mid-latitude and tropical regions. Our results show an inverse correlation of d-excess with terminal fall velocity, which increases with riming, indicating that lower d-excess reflects variable extents of riming during precipitation formation. The lower d-excess of rimed ice results from a partial loss of the accreted liquid by evaporation, and possibly splashing and shedding, before freezing is complete. This contrasts with a higher d-excess of ice that grows by the vapor deposition process. We conclude that low d-excess from riming can explain the spatial variations of Greenland and Antarctica surface snow that were previously attributed to changes in source moisture origin. Our results also help to explain the wide range of d-excess observed in daily precipitation compared to a much narrower range in surface snow or ice cores. Further, spatial or temporal differences in d-excess would allow for the estimation of variations in the rimed mass fraction, which, in turn, can be used as observational constraints for improving microphysics schemes in climate models.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-687</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-687/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138151</identifier>
    <datestamp>2026-03-05</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[Design and evaluation of a catalytic stripper with a plate electrical aerosol classifier]]></dc:title>
      <dc:creator>Guo, Chengxiang</dc:creator>
      <dc:creator>Yu, Tongzhu</dc:creator>
      <dc:creator>Yang, Yixin</dc:creator>
      <dc:creator>Gui, Huaqiao</dc:creator>
      <dc:creator>Ji, Zhe</dc:creator>
      <dc:creator>Wang, Jian</dc:creator>
      <dc:creator>Liu, Jianguo</dc:creator>
      <dc:creator>Liu, Wenqing</dc:creator>
      <dc:description><![CDATA[The catalytic stripper (CS) for removing volatile particles is a critical unit within the measurement system. However, the penetration efficiency of small size particles is currently significantly lower than large particles in CS. Therefore, further improving the penetration efficiency of small size particles is of significant research interest. This study aims to enhance the penetration efficiency of small size particles by reducing the thermophoretic loss. For this purpose, a CS equipped with a plate-type electrical aerosol classifier (EAC) was designed and developed, and its performance was evaluated. The particles are prevented from depositing on the tube wall by applying an electric field force to them in the opposite direction to the thermophoretic force they are subjected to, which ultimately serves the purpose of further improving the particle penetration efficiency. The experimental results demonstrated that the CS achieved a removal efficiency (RE) higher than 99.9 % at a flow rate of 1.5 L/min or lower. At a sample flow of 0.3 L/min and a temperature of 350 &deg;C, the penetration efficiency of CS+EAC without voltage was evaluated. Combined with the CS+EAC voltage-penetration efficiency curve, applying -112 V on the EAC, the penetration efficiency was further improved under the same experimental conditions, and the smaller the particle size, the greater the improvement. Compared to the 0 V, the improvement rate for 15 nm at -112 V was 24.4 %, while that for 23 nm was 18.9 %. Further experimental results show that the EAC can remove particles smaller than 10 or 23 nm by further increasing the voltage. This capability enables rapid particle classification and facilitates high temporal resolution measurements of particle number concentrations across different size intervals.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-565</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-565/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138890</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The Impact of NaOH, CaO, and HCO3&ndash;+ Ca+2 Addition on PIC and POC Formation in Los Angeles Harbor Waters]]></dc:title>
      <dc:creator>Wani, Rucha P.</dc:creator>
      <dc:creator>Roper, Devan</dc:creator>
      <dc:creator>Agrawal, Ria</dc:creator>
      <dc:creator>Lim, Esther J.</dc:creator>
      <dc:creator>Rollins, Nick E.</dc:creator>
      <dc:creator>Berelson, William M.</dc:creator>
      <dc:description><![CDATA[Negative CO<sub>2</sub> emission technologies such as ocean alkalinity enhancement (OAE), in tandem with emissions reduction are necessary to keep the climate system below a critical tipping point. While the biogeochemical consequences of OAE remain poorly constrained, field deployment is accelerating in the commercial sector, leaving questions of ecosystem impact in the wake. In this study we conduct alkalinity perturbation experiments to capture the resultant impact to the organic carbon and calcium carbonate pools. We quantify shifts in dissolved/particulate inorganic (DIC, PIC) and organic (DOC, POC) carbon after the addition of three alkalinity sources &ndash; NaOH, CaO, and NaHCO<sub>3</sub> + CaCl<sub>2</sub> (to simulate dissolved limestone). These experiments are conducted with coastal sea water with enhancements of +500&ndash;1000 &micro;mol kg<sup>&ndash;1</sup> alkalinity, and incubated in situ, to elucidate their impact over the short term, 0&ndash;4 days. Select experiments are also completely isolated from the light via bottle shading. With most treatments, there is no statistically significant CaCO<sub>3</sub> precipitation after OAE nor changes in organic matter production or consumption, relative to the untreated controls. One exception is when CaO addition enriches the water by 1000 &micro;mol kg<sup>&ndash;1</sup>, here we find a significant decline in POC production. <sup>13</sup>C isotope spikes were added to trace C partitioning throughout the experiment. The seawater used in these experiments had a wide range of initial ambient PIC and POC, and within this wide range, a +500 &micro;mol kg<sup>&ndash;1</sup> alkalinity in the form of NaOH, CaO or NaHCO<sub>3</sub> + CaCl<sub>2</sub> addition did not change the production or consumption of carbon in these waters.&nbsp;]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-982</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-982/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138915</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[How Does Assimilating a Large Commercial GNSS RO Dataset Impact HAFS Hurricane Forecasts? An Evaluation in Support of the ROMEX Experiment]]></dc:title>
      <dc:creator>Miller, William J.</dc:creator>
      <dc:creator>Chen, Yong</dc:creator>
      <dc:creator>Ho, Shu-Peng</dc:creator>
      <dc:creator>Shao, Xi</dc:creator>
      <dc:description><![CDATA[<p style="font-weight: 400;"><span>While </span>Global Navigation Satellite System (GNSS) radio occultation (RO) data assimilation <span>improves </span>tropical cyclone (TC) intensity<span> forecasts</span>, <span>the scaling of </span>these impacts with RO observation volume <span>remains unclear</span>. This observing system experiment (OSE) study evaluates the impact of assimilating <span>the large </span>commercial GNSS RO profile dataset from the Radio Occultation Modeling Experiment (ROMEX) on 84 Hurricane Analysis and Forecast System (HAFS) model forecasts of four 2022 Atlantic hurricanes. The ROMEX dataset contains about 20,000 daily global Spire and PlanetiQ profiles, which is roughly triple the volume of government-provided RO data that the National Centers for Environmental Prediction (NCEP) assimilated operational<span>ly</span> in 2022. Compared to a Control experiment that uses only operational<span>&nbsp;</span>RO data, assimilating ROMEX data together with operational RO profiles in HAFS yields ~ 5<span>&ndash;</span>15 % relative skill improvement in minimum central sea-level pressure (<em>P<sub>MIN</sub></em>)<em><sub> </sub></em>absolute intensity forecast errors in short-range forecasts<span>,</span> and it nearly eliminates a ~ 2<span>&ndash;</span>3 hPa <em>P<sub>MIN</sub></em> over-intensification bias in medium-to-long range forecasts. Additionally, ROMEX commercial RO data assimilation reduces HAFS temperature and water vapor errors in the middle-to-upper troposphere. A sensitivity experiment shows that <span>lower-tropospheric</span> RO data assimilated below the 5-km impact height provide a substantial contribution to ROMEX forecast improvements <span>relative to</span> Control. These results demonstrate that quadrupling the volume of assimilated GNSS RO data yield<span>s</span> a meaningful positive impact on regional <span>model TC forecasts</span>.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1000</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1000/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138839</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Winter fluxes determine the annual carbon balance of an unmanaged subarctic drained peatland]]></dc:title>
      <dc:creator>Salimi, Asra</dc:creator>
      <dc:creator>Sigurðsson, Bjarni Diðrik</dc:creator>
      <dc:creator>Bjarnadóttir, Brynhildur</dc:creator>
      <dc:creator>Feng, Chenxin</dc:creator>
      <dc:creator>Óskarsson, Hlynur</dc:creator>
      <dc:creator>Mammarella, Ivan</dc:creator>
      <dc:description><![CDATA[Peatlands are critical components of the global carbon (C) cycle, storing large amounts of soil organic carbon (SOC). However, drainage substantially alters their carbon exchange and hydrological functioning, often converting them into net carbon dioxide (CO<sub>2</sub>) sources. This study presents the first year-round, ecosystem-scale Eddy Covariance (EC) assessment of CO<sub>2</sub> dynamics from an unmanaged drained peatland in western Iceland, originally drained in the early 1960s. Two years of continuous EC measurements were collected alongside high-resolution environmental data, including solar radiation, air and soil temperatures, soil water content, and groundwater level. Several multispectral drone flights were also conducted during the study period, which provided seasonal NDVI-based estimates of canopy greenness. The two study years differed markedly in annual weather during the growing season (GS), with 2023 GS being unusually warm and dry, while 2024 GS was cold and wet. Despite these contrasts, annual net ecosystem exchange (NEE) remained similar between the two years. The annual NEE was dominated by non-growing-season (NGS) respiration, which highlighted the necessity for year-round measurements. Overall, the site remained a persistent CO<sub>2</sub> source, emitting 4.1&ndash;4.4 t CO<sub>2</sub>-C ha<sup>&minus;1</sup> yr<sup>&minus;1</sup> nearly 60 years after drainage. Temperature exerted the strongest control on ecosystem respiration (R<sub>eco</sub>), while gross primary production (GPP) responded primarily to seasonal irradiance and NDVI. A compensatory mechanism was observed during the warm year (2023) at this relatively cool site, where warming-induced increases in R<sub>eco</sub> were offset by an enhanced GPP, resulting in a relatively stable annual NEE despite meteorological contrasts. Soil moisture and vapor pressure deficit played only minor roles under these cool and moist conditions. These findings highlight the need for continued monitoring of unmanaged drained peatlands to better quantify their contribution to regional greenhouse gas budgets.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-945</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-945/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere134277</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Suspended sediment dynamics in an urban, mountain catchment in Nepal]]></dc:title>
      <dc:creator>Prajapati, Rajaram</dc:creator>
      <dc:creator>Karki, Saroj</dc:creator>
      <dc:creator>Thapa, Saraswati</dc:creator>
      <dc:creator>Lakhe, Hanik</dc:creator>
      <dc:creator>Bain, Daniel</dc:creator>
      <dc:creator>Gardner, John</dc:creator>
      <dc:description><![CDATA[Urban mountain catchments are highly vulnerable to erosion and sedimentation due to steep terrain, intense rainfall, and rapid land-use change at the urban fringe. However, event-scale sediment transport remains poorly understood in these regions, particularly in data-scarce areas such as the Himalayas. This study presents the first high-frequency, event-based analysis of suspended sediment transport in the Nakkhu River, a rapidly urbanizing catchment in Kathmandu Valley, Nepal. Using optical backscatter sensors and targeted field sampling during the 2023 monsoon, we analysed how rainfall, antecedent moisture, and human disturbance shaped sediment responses. Sediment transport was highly episodic, with two extreme storms accounting for nearly half of the seasonal suspended sediment load. Analysis of SSC&ndash;discharge hysteresis patterns revealed event-specific variability shaped by rainfall intensity, antecedent conditions, and hydrologic connectivity. Peak SSC often lagged peak discharge during low-flow events, suggesting upstream sediment sources. In contrast, high-intensity storms produced rapid sediment delivery, likely from hillslopes, mining zones, and in-channel deposits. Low-frequency (daily) monitoring underestimated sediment loads by approximately 30 % compared to 30-minutes interval data. This study provides the first 30-minute interval event-scale analysis of suspended sediment transport in Kathmandu Valley, revealing how sediment responses vary across the monsoon season in relation to rainfall intensity, discharge dynamics, and antecedent conditions. These insights, including lagged sediment peaks during low-flow events and rapid sediment flushing during intense storms, highlight the value of sub-hourly monitoring for capturing within-event variability and identifying short-lived sediment sources in urban mountain watersheds.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2025-5026</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2025-5026/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere137723</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Top-Down Benchmark of U.S. Methane Inventories Reveals Regional Discrepancies in Activity-Based Estimates]]></dc:title>
      <dc:creator>Worden, John</dc:creator>
      <dc:creator>Pandey, Sudhanshu</dc:creator>
      <dc:creator>Nesser, Hannah</dc:creator>
      <dc:creator>Bowman, Kevin</dc:creator>
      <dc:creator>Harkins, Colin</dc:creator>
      <dc:creator>Lyu, Congmeng</dc:creator>
      <dc:creator>Maasakkers, Joannes D.</dc:creator>
      <dc:creator>Gordon, Deborah</dc:creator>
      <dc:creator>Jacob, Daniel</dc:creator>
      <dc:creator>Estrada, Lucas</dc:creator>
      <dc:creator>Varon, Daniel J.</dc:creator>
      <dc:creator>East, James D.</dc:creator>
      <dc:creator>Schmeisser, Lauren</dc:creator>
      <dc:creator>Qu, Zhen</dc:creator>
      <dc:description><![CDATA[<p style="font-weight: 400;">Robust estimates of methane emissions are critical for understanding their impacts on atmospheric warming and air quality, and for assessing methane mitigation strategies. Gridded inventories, such as the U.S. Environmental Protection Agency&rsquo;s Greenhouse Gas Inventory (EPA GHGI), the Emissions Database for Global Atmospheric Research (EDGAR 2024), and the National Oceanic and Atmospheric Administration&rsquo;s Fossil Fuel Oil and Gas inventory (NOAA FOG), are constructed to evaluate large-scale emission patterns and support identifying emission mitigation priorities and prioritizing future measurements. However, substantial differences across inventories complicate such assessments. We benchmark EPA GHGI, EDGAR 2024, and NOAA FOG against flux estimates from an atmospheric inversion of Greenhouse Gases Observing Satellite (GOSAT) data from 2012 to 2020 over the Contiguous United States (CONUS). A key technical challenge is the heterogeneous sensitivity of satellite-derived fluxes, which depends on measurement uncertainty, coverage, and inversion model configuration. We account for this heterogeneity by applying an inversion operator to each inventory prior to comparison with the GOSAT-based estimates. The GOSAT estimates are most sensitive to oil&amp;gas and livestock emissions; oil and gas emissions are consistent with NOAA FOG (14.1 Tg CH<sub>4</sub> yr⁻&sup1; in 2015), but exceed EPA GHGI and EDGAR, particularly across Texas, Oklahoma, and Louisiana. GOSAT-based livestock emissions exceed EPA GHGI and EDGAR by 1&ndash;2 Tg CH<sub>4</sub> yr⁻&sup1;, with the largest differences in the Midwest and California. Despite these discrepancies, both activity and satellite based estimates show no observable trends from 2012 to 2020 in fossil and livestock emissions.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-313</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-313/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere136290</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[An ADCP-Based Data-Driven Framework for Proxy Sediment Transport Monitoring: From Controlled Flumes to Natural Rivers]]></dc:title>
      <dc:creator>Tuhin, Mohammd Tanvir Haque</dc:creator>
      <dc:creator>Hinkelmann, Reinhard</dc:creator>
      <dc:creator>Mudersbach, Christoph</dc:creator>
      <dc:description><![CDATA[Acoustic Doppler Current Profilers (ADCPs) provide a rich yet underutilized source for monitoring hydrodynamics and sediment transport. Accurate prediction of sediment‐related variables is critical for river engineering, morphological studies, and environmental management. Among these, Bottom-Track Velocity (BT_Vel) serves as a robust proxy for near-bed sediment dynamics and bedload activity. This study develops a machine learning (ML) and deep learning (DL) framework to predict BT_Vel from ADCP-derived hydrodynamic and acoustic features, enabling proxy estimation of sediment transport processes in both controlled flume and natural riverine environments. Two datasets were analyzed: (i) a laboratory dataset of 22,650 ensemble samples obtained under controlled flow regimes, and (ii) a field dataset of 5,900 ensemble samples collected across seven campaigns at a fixed river cross-section. A consistent benchmarking strategy was applied across Random Forest, Gradient Boosting, LightGBM, CatBoost, XGBoost, LSTM, GRU, CNN, RNN, ANN, and a hybrid LSTM+CNN, with evaluation based on both an 80/20 split and a stratified 5-fold cross-validation (CV). SHAP analysis was conducted for model interpretability. In the laboratory, Random Forest (R&sup2; = 0.804 split / 0.783 CV) and Gradient Boosting (0.787 / 0.757) achieved the best generalization, while LSTM+CNN (0.770 / 0.730) and LSTM (0.775 / 0.718) remained competitive. In the field, Random Forest again delivered the strongest results (0.573 / 0.603), followed closely by CatBoost, LightGBM, and XGBoost. Notably, LSTM improved under cross-validation (0.468 &rarr; 0.529), suggesting fold-wise diversity stabilized training under noisy, heterogeneous river data. By contrast, the Stacking Regressor consistently showed the weakest generalization across both environments. SHAP revealed a shift in feature relevance: in the laboratory, Mean water velocity (Mean_Speed) dominated predictions, while in the field, Depth and signal-to-noise ratio (SNR) emerged as stronger drivers, reflecting the influence of stage variability and acoustic quality. Overall, the study demonstrates that ADCP-derived features, coupled with explainable ML/DL models, provide robust potential for proxy sediment transport modeling. Conversion to absolute transport rates requires paired sediment measurements, while future work should expand field campaigns and explore hybrid physics&ndash;data frameworks toward operational forecasting.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2025-6190</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2025-6190/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere137566</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Soil water content and salinity regulate the temperature sensitivity of CO2 and CH4 emissions in a coastal salt-affected land]]></dc:title>
      <dc:creator>Diao, Mengmeng</dc:creator>
      <dc:creator>Sun, Wenyao</dc:creator>
      <dc:creator>Zhang, Zhaosong</dc:creator>
      <dc:creator>Chen, Yitong</dc:creator>
      <dc:creator>Zhang, Qian</dc:creator>
      <dc:creator>Ma, Xiang</dc:creator>
      <dc:creator>Sun, Juan</dc:creator>
      <dc:creator>Yang, Chao</dc:creator>
      <dc:description><![CDATA[Soil carbon emissions from coastal saline-alkaline ecosystems significantly influence the global carbon cycle, yet their responses to key environmental drivers such as soil water content and salinity remain insufficiently understood. This study employed controlled incubation experiments using soils collected from the Yellow River Delta, China, to systematically investigate the effects of varying soil water content (5 %, 15 %, 30 %, 45 %, and 60 %) and salinity levels (S1: EC=1.9 dS/m; S2: 10.8 dS/m; S3: 58.8 dS/m; S4: 66.3 dS/m; S5: 96.0 dS/m) on CO<sub>2</sub> and CH<sub>4</sub> emissions and their temperature sensitivity (Q<sub>10</sub>). The results demonstrated that under constant temperature conditions, CO<sub>2</sub> emission flux followed a unimodal pattern in response to increasing soil water content, peaking at 45 % water content, with CH<sub>4</sub> flux exhibiting a similar trend. Soil salinity significantly suppressed the fluxes of both greenhouse gases, with reductions observed across all temperature levels as salinity increased. Both soil water content and salinity played substantial regulatory roles in modulating the Q<sub>10</sub> of gas emissions. Specifically, Q<sub>10</sub> values for CO<sub>2</sub> and CH<sub>4</sub> initially decreased and then increased with rising soil water content. Along the salinity gradient, the Q<sub>10</sub> of CO<sub>2</sub> decreased from S2 to S4, whereas the Q<sub>10</sub> of CH<sub>4</sub> increased progressively from S2 to S5. These findings reveal the complex and interactive effects of soil water content and salinity on carbon cycling processes in coastal saline-alkaline lands. The study provides crucial theoretical insights for improving the prediction of carbon cycle dynamics under climate change and offers a scientific basis for the adaptive management and conservation of these vulnerable ecosystems.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-217</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-217/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138267</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Quantification of inmixing of Asian Monsoon air by multi-species classification in a match flight experiment]]></dc:title>
      <dc:creator>Kaumanns, Jan</dc:creator>
      <dc:creator>Ungermann, Jörn</dc:creator>
      <dc:creator>Vogel, Bärbel</dc:creator>
      <dc:creator>Johansson, Sören</dc:creator>
      <dc:creator>Kretschmer, Erik</dc:creator>
      <dc:creator>Plöger, Felix</dc:creator>
      <dc:creator>Preuße, Peter</dc:creator>
      <dc:creator>Woiwode, Wolfgang</dc:creator>
      <dc:creator>Riese, Martin</dc:creator>
      <dc:description><![CDATA[Mixing of air masses between different compartments of the atmosphere is one of the processes ruling atmospheric composition. The mixing process is commonly studied by using tracer-tracer correlations. Here, we generalize this approach by statistical classification methods based on a larger number of tracers to quantify mixing. From the 3-D resolution of our trace gas observations we are able to spatially resolve the observed mixing processes. This paper presents a matching flight-experiment of a filament of Asian monsoon air in the Upper Troposphere/ Lower Stratosphere (UTLS) off the North-American west coast by two flights of the High Altitude and Long Range research aircraft (HALO) conducted during the "Probing High Latitude Export of air from the Asian Summer Monsoon (PHILEAS)" campaign. In both flights the 3-D structure of the filament was revealed by tomographic observations by the Gimballed Limb Observer for Radiance Imaging of the Atmosphere (GLORIA) of five trace species (H<sub>2</sub>O, PAN, CFC &ndash; 12, O<sub>3</sub>, HNO<sub>3</sub>). The observed tracer mixing ratios show evidence for a tropopause folding in connection to a Rossby wave breaking event. We show that the strongly perturbed atmospheric situation can not be decisively described by simple tracer-tracer correlations. By using a Bayesian Gaussian mixture model to cluster our observations by similarity we identify five classes of air masses: tropospheric air (both continental and maritime), Asian Summer Monsoon outflow (ASMO), mixed air and stratospheric air. Trajectory calculations are carried out to identify air masses which are observed in both flights. A measure of the mixing strengths of the mixing between both flights follows naturally from this classification. The unique 3-D observations allow us to reveal the spatial structure of the mixing processes in high detail. In particular, the mixing of ASMO air directly with stratospheric air and into the UTLS are shown. Comparing the classification to simulated artificial surface-origin tracers in the Chemical Lagrangian Model of the Stratosphere (CLaMS), we find strong evidence for distinctly correlated air masses to originate within different source regions within the Asian monsoon region.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-650</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-650/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138275</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Quantifying national, state, and oil/gas field methane emissions and trends in the U.S. (2019&ndash;2024) through high resolution inversion of satellite observations]]></dc:title>
      <dc:creator>Estrada, Lucas A.</dc:creator>
      <dc:creator>Jacob, Daniel J.</dc:creator>
      <dc:creator>He, Megan</dc:creator>
      <dc:creator>East, James D.</dc:creator>
      <dc:creator>Varon, Daniel J.</dc:creator>
      <dc:creator>Balasus, Nicholas</dc:creator>
      <dc:creator>Hancock, Sarah E.</dc:creator>
      <dc:creator>Sulprizio, Melissa</dc:creator>
      <dc:creator>Bowman, Kevin W.</dc:creator>
      <dc:creator>Worden, John R.</dc:creator>
      <dc:creator>Reidy, Emily</dc:creator>
      <dc:creator>Runkle, Benjamin R. K.</dc:creator>
      <dc:description><![CDATA[We quantify trends of U.S. methane emissions at the national, state, and oil/gas field levels for 2019&ndash;2024 through high-resolution (up to ~25 km) analytical inversion of TROPOMI satellite observations with the open-source Integrated Methane Inversion (IMI 2.1). We find that total anthropogenic methane emissions (37 Tg a<sup>-1</sup>) are 34 % higher in magnitude than reported in the U.S. Environmental Protection Agency (EPA) Greenhouse Gas Inventory (GHGI) that provided prior estimates for the inversion. Oil/gas emissions are 64 % higher than the GHGI, consistent with previous studies. Total emissions are flat over the 2019&ndash;2024 period (0.0 &plusmn; 1.0 % a<sup>-1</sup>) but this total reflects a combination of decreasing emissions from the oil/gas (-1.1 &plusmn; 0.9 % a<sup>-1</sup>), coal (-2.3 &plusmn; 1.3 % a<sup>-1</sup>), and rice (-9.1 % &plusmn; 2.0 a<sup>-1</sup>) sectors, offset by increases in the livestock (1.8 &plusmn; 1.3 % a<sup>-1</sup>) and landfill (0.5 &plusmn; 1.4 % a<sup>-1</sup>) sectors. The methane intensity from the oil/gas sector continues its downward trend, from 2.3 % to 1.9 % over the 2019&ndash;2024 period, but unlike in previous studies we find that this trend does not simply reflect an increase in production but also a decrease in emissions, demonstrating improved emission management. Over half of total U.S. emissions originate from ten states, most dominated by fuel exploitation. Emission inventories compiled by individual states do not always improve on GHGI state estimates. Methane intensities decrease for all major oil/gas fields except those with declining production.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-655</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-655/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138522</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[GPR-derived ice thickness of the temperate Hintereisferner glacier (Austrian Alps): evaluation of thickness models]]></dc:title>
      <dc:creator>Švinka, Lelde</dc:creator>
      <dc:creator>Lamsters, Kristaps</dc:creator>
      <dc:creator>Karušs, Jānis</dc:creator>
      <dc:creator>Džeriņš, Pēteris</dc:creator>
      <dc:creator>Ješkins, Jurijs</dc:creator>
      <dc:description><![CDATA[Alpine glaciers are retreating rapidly and have a potential for near complete ice loss at the end of the 21<sup>st</sup> century thus accurate glacier evolution models are crucial for predicting the magnitude and rate of future glacier changes. Without reliable ice thickness assessments, such models lack credibility and cannot be validated, thus here we evaluate several ice thickness models and present new ground-penetrating radar (GPR) ice-thickness measurements of the Hintereisferner &ndash; a temperate glacier located in the Ötztal Alps, Austria, which despite of being one of the WGMS reference glaciers lacks up-to date measured ice thickness data.</p> <p>The GPR data is characterized by strong signal scattering, typical for temperate ice with high water content, however the glacier bed is detectable in most profiles. GPR measurements reveal a maximum ice thickness of ~160 m along the central flowline and a mean thickness of ~81 m across the surveyed area. We further select three widely used, open-source ice-thickness models, GlabTop2, OGGM, and Millan et al. (2022), and compare their output to the GPR-derived ice thickness. All models systematically overestimate ice thickness across the surveyed area, with mean positive biases of ~37&ndash;40 m for GlabTop2 and OGGM and ~59 m for the Millan model, while only minor and localized underestimation occurs along the central flowline. These results highlight the limitations of predominantly geometry-based and velocity-informed modelling approaches when applied to small, temperate valley glaciers, where ice rheology and basal conditions may have greater influence on the resulting thickness than these algorithms allow.</p> <p>The GPR data presented here is made freely available in the section &ldquo;Code and data availability&rdquo; and provides an updated ice thickness benchmark for the Hintereisferner, to be used for future model calibration and improvement for Alpine glacier evolution projections.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-783</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-783/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138233</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Sequential approach to seismotectonic zonation for South-East France]]></dc:title>
      <dc:creator>Mowbray, Victoria</dc:creator>
      <dc:creator>Mathey, Marguerite</dc:creator>
      <dc:creator>Sue, Christian</dc:creator>
      <dc:creator>Baize, Stéphane</dc:creator>
      <dc:creator>Lemoine, Anne</dc:creator>
      <dc:creator>Beauval, Céline</dc:creator>
      <dc:description><![CDATA[The south-east of France, encompassing the western Alps, the Jura Mountain range, the Rh&ocirc;ne valley and the Provence region, is the most seismically active region in metropolitan France and, consequently, one of the most extensively surveyed and studied. However, seismicity remains low to moderate (less than 10 Mw 5 and 1 Mw 6 events per century since 1300 CE) and geodetic deformation rates appear relatively low (&lt; 20 nanostrain yr<sup>-1</sup>). The resulting low-signal-to-noise ratios, together with the complex, dense fault networks inherited from a polyphased tectonic history, make this region particularly challenging for seismic hazard assessment. The geophysical and geological data available are extensive, yet inhomogeneous and insufficient to confidently characterize active faults, quantify on-fault deformation and associate seismic rates. Therefore, seismic source characterization through seismogenic area models is commonly adopted. These models are however highly sensitive to the data used to describe seismotectonic behavior. Our objective is to consider newly available geophysical data as complementary constraints to geological observations to further refine seismotectonic zonation models.</p> <p>We present an innovative sequenced zoning methodology that disaggregates seismotectonic behavior into three components (namely &ndash; crustal structure, observed seismicity and surface deformation) each analyzing several key features. We thus derive three novel, independent seismotectonic zonation models, each representing a different perspective on the seismogenic process. Additionally, we associate confidence levels with zone limits to each subsequent zonation model, by assessing feature homogeneity among neighboring zones. Afterwards, we propose a synthetic model which integrates all seismotectonic features by merging the most recurrent and highest confidence zone limits from the three independent zonation models. This approach intends to minimize zone mapping uncertainties by quantitatively assessing seismotectonic observations, and to yield reproducible and updatable models representative of the current state of seismotectonic knowledge. We subsequently compare the resulting zonation models and discuss their implications for seismic source characterization.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-623</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-623/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138927</identifier>
    <datestamp>2026-03-05</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/"
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      <dc:title><![CDATA[Juice/SWI during the Lunar-Earth-Gravity-Assist (LEGA). I. General overview]]></dc:title>
      <dc:creator>Hartogh, Paul</dc:creator>
      <dc:creator>Rezac, Ladislav</dc:creator>
      <dc:creator>Cavalié, Thibault</dc:creator>
      <dc:creator>Jarchow, Christopher</dc:creator>
      <dc:creator>Moreno, Raphael</dc:creator>
      <dc:creator>Schulz-Ravanbakhsh, Ali</dc:creator>
      <dc:creator>Carrasco Gallardo, Alberto</dc:creator>
      <dc:creator>Dabrowski, Borys</dc:creator>
      <dc:creator>Goodyear, Samuel</dc:creator>
      <dc:creator>Rengel, Miriam</dc:creator>
      <dc:creator>Herpin, Fabrice</dc:creator>
      <dc:creator>Kasai, Yasuko</dc:creator>
      <dc:creator>Kotiranta, Mikko</dc:creator>
      <dc:creator>Lellouch, Emmanuel</dc:creator>
      <dc:creator>Murk, Axel</dc:creator>
      <dc:creator>Olberg, Michael</dc:creator>
      <dc:creator>Szutowicz, Slawomira</dc:creator>
      <dc:creator>Wirström, Eva</dc:creator>
      <dc:description><![CDATA[The Jupiter Icy moons Explorer (Juice) was the first spacecraft ever that performed a combined gravity assist using 20 both the Moon and Earth in succession. The double flyby required highly precise navigation to succeed. The LEGA allowed Juice to make a shortcut through the inner solar system on its way to Jupiter, using less fuel than would have been otherwise required. On August 19, 2024, Juice had its closest approach to the Moon. This first part of the manoeuvre accelerated the spacecraft by approximately 0.9 km/s relative to the Sun. On August 20, 2024, the spacecraft swung past Earth. This second part of the manoeuvre reduced the spacecraft's speed by 4.8 km/s relative to the Sun. This was a unique opportunity for its payloads to observe the Moon and Earth from a close distance as both calibration and science targets. The Submillimetre Wave Instrument (SWI), a dual channel heterodyne spectrometer observed both targets in two far-infrared bands around 500 and 250 &mu;m wavelength in order to characterize and calibrate the overall performance of the instrument, including its receiver frontend, spectrometer backend and telescope mechanisms. In addition, the commanding pipeline and operations processes of the instrument were also tested close to its full range of flexibility using the relevant pipelines. In this paper we provide a contextual description of physical and functional characteristics of SWI, its operational principles and in-flight calibration activities during LEGA.]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1011</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1011/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere138933</identifier>
    <datestamp>2026-03-05</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The JUICE Lunar-Earth gravity assist from trajectory design, navigation and spacecraft operations perspective]]></dc:title>
      <dc:creator>Dietz, Angela</dc:creator>
      <dc:creator>Boutonnet, Arnaud</dc:creator>
      <dc:creator>Budnik, Frank</dc:creator>
      <dc:description><![CDATA[This paper describes the world&rsquo;s first-ever Lunar&ndash;Earth Gravity Assist (LEGA) performed by ESA&rsquo;s JUICE spacecraft on 19&ndash;20 August 2024 from trajectory design, navigation and spacecraft operations point of view.</p> <p>This double flyby &ndash; Moon first, Earth second &ndash; enabled a large Delta-V gain while minimizing propellant use, redirecting JUICE toward its next destination: Venus (August 2025) and ultimately Jupiter (2031). The manoeuvre was unprecedented in complexity, requiring extremely accurate navigation, rigorous preparation, and coordinated operations across engineering, flight dynamics, and science teams.</p> <p>Overall, JUICE demonstrated outstanding platform stability, navigation accuracy, and subsystem robustness during this critical milestone, validating the operational feasibility of LEGA as an enabling technique for complex interplanetary trajectories.</p> <p>This paper is an executive summary of papers published on LEGA trajectory design [Schoenmaekers et al. (2014); Boutonnet et al. (2023)], navigation [Syndercombe et al. (2025)] and spacecraft operations [Heck et al. (2025)].]]></dc:description>
      <dc:date>2026-03-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-1015</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1015/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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