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    <identifier>oai:publications.copernicus.org:tc139769</identifier>
    <datestamp>2026-09-25</datestamp>
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      <dc:title><![CDATA[Variability of internal snow properties over Antarctic late summer sea ice on different spatial scales]]></dc:title>
      <dc:creator>Paul, Daria</dc:creator>
      <dc:creator>Caus, Danu</dc:creator>
      <dc:creator>Keil, Paul</dc:creator>
      <dc:creator>Kadow, Christopher</dc:creator>
      <dc:creator>Arndt, Stefanie</dc:creator>
      <dc:description><![CDATA[<p>Snow on Antarctic sea ice strongly affects thermodynamic processes, sea ice mass balance, and microwave remote sensing, yet its spatial variability and characteristic length scales remain poorly quantified. The aim of this study is to provide a spatially extensive, layer-resolved characterization of Antarctic late-summer snow on sea ice and, for the first time, to quantify the variability of snow properties and their horizontal correlation length scales on first-year (FYI) and multi-year ice (MYI). We use a unique combination of manual snow pit observations and more than 900 SnowMicroPen (SMP) profiles collected along meter-scale transects during three expeditions in the Weddell Sea between 2018 and 2021. Snow stratigraphy and microstructural classes were derived from SMP force data using a supervised one-dimensional convolutional neural network trained on manually classified SMP profiles. Across both sea-ice regimes, intrinsic properties of individual snow types, including density and specific surface area, were broadly similar. Differences between FYI and MYI instead arise from contrasting snowpack structure, snow type fractions, and spatial coherence, with MYI characterized by a higher prevalence of dense melt-freeze layers and enhanced vertical heterogeneity. Spatial autocorrelation analyses reveal pronounced scale-dependent variability, with snow properties on FYI decorrelating over short distances, while MYI exhibits substantially higher spatial coherence. Individual ice floes capture only about 50 % of the snow density variability characteristic of their respective ice regime, underscoring fundamental limits to the representativeness of point measurements. A hierarchy of variability emerges, in which snow type fractions and layer thickness dominate snowpack heterogeneity, while bulk snow density is comparatively homogeneous across spatial scales. These results demonstrate that Antarctic summer snow variability is governed primarily by stratigraphic composition and ice-regime-dependent snowpack evolution rather than bulk-integrated properties. These findings emphasize the need for spatially distributed observations and stratigraphy-aware parameterizations to improve the representation of snow on Antarctic sea ice in remote-sensing applications and sea ice and climate models. In particular, the relative consistency of specific surface area within snow types across ice regimes provides observational constraints that can be evaluated for future microwave-emission and radiative-transfer modeling studies.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/tc-20-5491-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/5491/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:os140699</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>os</setSpec>
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      <dc:title><![CDATA[LETKF-based Ocean Research Analysis version 2.0 for a quasi-global domain (LORA-QG): validation and intercomparison with eddy-permitting global ocean reanalysis datasets]]></dc:title>
      <dc:creator>Ohishi, Shun</dc:creator>
      <dc:creator>Miyoshi, Takemasa</dc:creator>
      <dc:creator>Kachi, Misako</dc:creator>
      <dc:description><![CDATA[<p>We previously produced the local ensemble transform Kalman filter (LETKF)-based Ocean Research Analysis (LORA) version 1.0 datasets for the western North Pacific and Maritime Continent regions (LORA-WNP and LORA-MC, respectively) during the period from August 2015 to January 2024. However, these limited domains and periods constrain their applicability. Therefore, we developed a new eddy-permitting LETKF-based ocean data assimilation system and produced LORA version 2.0 for a quasi-global domain (LORA-QG) from June 2002, when the Advanced Microwave Scanning Radiometer (AMSR) series, a series of space-borne microwave imagers, began providing sea surface temperature observations and the Argo program substantially expanded in situ temperature and salinity measurements. We validated LORA-QG using observations from surface drifter buoys, tide gauges, and ocean climate stations, and compared the results with those of three eddy-permitting global ocean reanalysis datasets (GLORYS2V4, ORAS5, and C-GLORSv7). Although these observations are independent of LORA-QG, ORAS5, and C-GLORSv7, they are not entirely independent of GLORYS2V4. The validation results show that LORA-QG agrees well with the observations and has the second-highest accuracy among the four datasets in terms of overall root-mean-square deviations relative to the observations, thus achieving sufficient accuracy for geoscientific research and practical applications. LORA-QG provides features unavailable in conventional global reanalysis products, including ensemble-based uncertainty estimates and individual terms of the heat and salinity budget equations. These features make LORA-QG a valuable dataset for ensemble-based ocean forecasting and process-based studies. However, room for improvement remains, as LORA-QG exhibits significant warm biases in the tropics, particularly in the western tropical Pacific, and its sea surface salinity representation is likely limited due to relatively strong salinity nudging toward a climatological dataset in the mixed layer.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/os-22-2915-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/2915/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:os138560</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>os</setSpec>
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      <dc:title><![CDATA[North Atlantic sea level budget revisited]]></dc:title>
      <dc:creator>Song, Zhe</dc:creator>
      <dc:creator>Cazenave, Anny</dc:creator>
      <dc:creator>Llovel, William</dc:creator>
      <dc:creator>Storto, Andrea</dc:creator>
      <dc:creator>Bouih, Marie</dc:creator>
      <dc:description><![CDATA[<p>Based on satellite altimetry, GRACE space gravimetry and Argo-based steric data down to 2000 m, recent studies have shown that the North Atlantic sea level budget (i.e., altimetry-based sea level minus sum of components) of the past two decades is not closed, with strong regional residuals in the North Atlantic. In this study, we revisit the North Atlantic sea level budget, using satellite altimetry, GRACE and GRACE-FO data, different Argo products and an ocean reanalysis (CIGAR) over the 2004–2022 time span. The ocean reanalysis is used to estimate the manometric contribution, an alternative to using GRACE data, as well as the deep ocean contribution to the sea level budget, not yet fully sampled by Argo. Analyzing different data sets allows us to assess their impact on the previously reported non-closure of the North Atlantic sea level budget. We first find that using the CIGAR ocean reanalysis-based manometric component significantly reduces the residuals of the North Atlantic sea level budget compared to GRACE. We also find that accounting for the deep ocean (below 2000 m) thermal expansion (using the CIGAR reanalysis) allows for reducing 90 % the North Atlantic budget residuals when using CIGAR for the manometric component. The budget can be closed within the data uncertainties when CIGAR manometric and full depth steric sea level are included.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/os-22-2903-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/2903/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:hess142110</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>hess</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Freeze–thaw processes influence shallow groundwater recharge sources and pathways in the Qinghai Lake Basin: insights from water isotopes]]></dc:title>
      <dc:creator>Zhang, Wenhao</dc:creator>
      <dc:creator>Li, Xiaoyan</dc:creator>
      <dc:creator>Deng, Yuanhong</dc:creator>
      <dc:creator>Hu, Guangrong</dc:creator>
      <dc:creator>Shi, Fangzhong</dc:creator>
      <dc:description><![CDATA[<p>Groundwater plays a crucial role in maintaining baseflow in rivers and ensuring water supply, particularly in alpine regions where the freeze–thaw (FT) cycle exerts a strong influence on hydrological processes. However, a systematic understanding is still lacking regarding how FT processes affect the composition of groundwater recharge sources and the transitions among recharge pathways. This study takes the Qinghai Lake basin (QLB) as a case study and combines water isotope and hydrometeorological data to quantify the dynamic characteristics of groundwater recharge sources and pathways during the FT periods. The study found that soil water (57.0 %–76.3 %) was the dominant source of groundwater recharge during the FT periods, followed by rainfall (13.8 %–26.1 %) and snowmelt (7.9 %–22.0 %). The thawing process enhances the vertical connectivity of the soil profile, facilitating the recharge of groundwater from snowmelt and the 60–90 cm soil layer. Furthermore, the lc-excess value of groundwater gradually shifts from values closer to soil water to those closer to precipitation, indicating that piston flow gradually weakens during the process of groundwater recharge by soil water, while preferential flow intensifies, resulting in a pattern where piston flow and preferential flow coexist. Spatially, in the middle and upper regions dominated by permafrost, groundwater is primarily recharged by water from the 0–60 cm soil layer traveling along longer hydrological pathways, whereas in the downstream regions of the basin dominated by seasonal frozen ground, groundwater is primarily recharged by rapid infiltration from the 30–90 cm soil layer. Our research demonstrates that in alpine permafrost regions, freeze–thaw processes regulate water storage and transport, thereby further influencing the recharge sources and pathways of shallow groundwater.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-6039-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/6039/2026/]]></dc:identifier>
      <dc:source>eISSN: 1607-7938</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:hess136344</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>hess</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Integrating coupled surface–subsurface modelling and field measurements in a degraded fen: water-balance dynamics and a framework for evaluating rewetting measures]]></dc:title>
      <dc:creator>Mahmoodi, Nariman</dc:creator>
      <dc:creator>Merz, Christoph</dc:creator>
      <dc:creator>Pickert, Jürgen</dc:creator>
      <dc:creator>Dietrich, Ottfried</dc:creator>
      <dc:description><![CDATA[<p>Peatlands play a crucial role in regional water balance and carbon dynamics but are often degraded due to drainage and agricultural use. In Germany, many drained peatlands have shifted from carbon sinks to CO<span class="inline-formula"><sub>2</sub></span> sources. Rewetting these ecosystems is therefore essential to restore their ecological functions and mitigate greenhouse gas emissions. However, effective rewetting requires a detailed understanding of peatland hydrology and its response to climatic and management conditions. To address this need, this study employs a fully coupled surface–subsurface hydrological model (HydroGeoSphere) to analyze the complex hydrological functioning of a typical degraded fen peatland site (11.6 ha) in Brandenburg, Germany. The model-based quantification of hydrological fluxes is basis for assessing peatland vulnerability to climate variability and land use while providing a hydrological baseline for future evaluation of rewetting strategies. The studied peatland is connected to a regional aquifer and intensively drained by a system of ditches. Simulations used daily meteorological inputs and detailed field measurements from 2015 to 2023. Evapotranspiration (ET) was parameterized using field-measured vegetation dynamics (seasonal leaf area index and management schedules), while measured ditch water levels served as hydraulic boundary conditions. The site was spatially divided into different management units with distinct vegetation parameters. The peat profile was represented by two layers (a 0.3 m highly degraded surface peat overlying a 0.7 m less degraded layer) overlying sand (aquifer) and till (aquifer base). The model was evaluated from different angles against eddy covariance ET and groundwater table dynamics during a calibration period (2016–2020) and a validation period (2021–2023) using a multi-metric approach. The model successfully reproduced seasonal water-table fluctuations and ditch–peatland interactions, including ET-driven hydraulic gradient dynamics between summer and winter. Simulated ET closely matched eddy covariance measurements, with RMSE values of 64 mm yr<span class="inline-formula"><sup>−1</sup></span>, 10.2 mm month<span class="inline-formula"><sup>−1</sup></span>, and 1.01 mm d<span class="inline-formula"><sup>−1</sup></span>, and showed only minor biases during dry conditions, while over the year seasonal dynamics of ET were also well captured by the model. The model reproduced groundwater variations with sufficient accuracy, achieving KGE values of 0.80–0.85, NSE of 0.83–0.86, and RMSE of 0.15 m during calibration and validation. The analysis of seasonal and interannual water-storage changes showed pronounced shifts between hydrological surplus and deficit, demonstrating that drained fens are highly sensitive to evapotranspiration demand and prolonged drought. The modeling approach captured key hydrological processes with high robustness. The modelling framework provides a hydrological baseline and a basis for future assessment of peatland rewetting measures. These findings support ongoing restoration initiatives on drained peatlands in Europe.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-6019-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/6019/2026/]]></dc:identifier>
      <dc:source>eISSN: 1607-7938</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:esd138613</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Assessing Earth system responses in mitigation scenarios with activity-driven simulation of carbon dioxide removal]]></dc:title>
      <dc:creator>Schwinger, Jörg</dc:creator>
      <dc:creator>Merfort, Leon</dc:creator>
      <dc:creator>Bauer, Nico</dc:creator>
      <dc:creator>Bernardello, Raffaele</dc:creator>
      <dc:creator>Butenschön, Momme</dc:creator>
      <dc:creator>Bourgeois, Timothée</dc:creator>
      <dc:creator>Gidden, Matthew J.</dc:creator>
      <dc:creator>Gupta, Shraddha</dc:creator>
      <dc:creator>Lee, Hanna</dc:creator>
      <dc:creator>Mengis, Nadine</dc:creator>
      <dc:creator>Moustakis, Yiannis</dc:creator>
      <dc:creator>Muri, Helene</dc:creator>
      <dc:creator>Nieradzik, Lars</dc:creator>
      <dc:creator>Peano, Daniele</dc:creator>
      <dc:creator>Pongratz, Julia</dc:creator>
      <dc:creator>Sauer, Pascal</dc:creator>
      <dc:creator>Tourigny, Etienne</dc:creator>
      <dc:creator>Wårlind, David</dc:creator>
      <dc:description><![CDATA[<p>Assessing Earth system responses arising from carbon dioxide removal (CDR) requires developing and simulating pairs of scenarios – a mitigation scenario with deployment of CDR and a corresponding no-CDR baseline. The latter describes a world where no CDR is deployed, such that net carbon emissions are higher and a given temperature target may be missed. While over the past years a rich literature on mitigation scenarios with CDR has been emerging, no-CDR baselines have mostly been explored in stylized Earth system model (ESM) experiments. In such simulations, a no-CDR baseline simply assumes that CDR is “switched off”, while socio-economic constraints are not considered. However, the deployment of CDR in mitigation scenarios, created by integrated assessment models (IAMs), is embedded in a consistent socio-economic description of plausible futures, and disallowing CDR may affect climate drivers due to changes in the energy system and in land-use dynamics. Particularly, when moving towards an activity-driven representation of CDR in emission-driven ESMs, where the activity that draws down <span class="inline-formula">CO<sub>2</sub></span> from the atmosphere is explicitly modelled, the creation of no-CDR baselines comes with challenges and trade-offs. Here, we conceptualize a framework for emission-driven ESM simulations of IAM scenarios that allows us to determine carbon-cycle feedbacks and biogeophysical effects of CDR deployment using no-CDR baselines. We show that different options exist for the creation of no-CDR baselines, which offer different insights and have their specific advantages and limitations. We also demonstrate that internal variability of the climate system inherently limits our ability to detect the small signals related to CDR deployment and its feedbacks. Hence, unless a sufficiently large initial conditions ensemble is employed, stylized modelling approaches may remain preferable for some applications, e.g., the quantification of regional biogeophysical effects of CDR deployment. Both, the efficiency of CDR (defined as <span class="inline-formula">CO<sub>2</sub></span> removed per unit of resources employed) as well as related carbon-cycle feedbacks and biogeophysical effects are expected<span id="page1342"/> to be scenario- and model-dependent. Our simulation design of concentration- and emission-driven no-CDR baselines, together with an improved representation of CDR in the IAM – ESM modelling chain, opens an avenue towards estimating CDR efficiencies and their uncertainties under various future scenarios in upcoming model intercomparison activities.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-1341-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/1341/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:esd141092</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
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       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Everyday weather in a warmer world]]></dc:title>
      <dc:creator>Thomas, Rhidian</dc:creator>
      <dc:creator>Compo, Gilbert P.</dc:creator>
      <dc:creator>George, Steve</dc:creator>
      <dc:creator>Hegerl, Gabriele C.</dc:creator>
      <dc:creator>Schurer, Andrew</dc:creator>
      <dc:creator>Shepherd, Theodore G.</dc:creator>
      <dc:creator>Slivinski, Laura C.</dc:creator>
      <dc:creator>Thompson, Vikki</dc:creator>
      <dc:creator>Hawkins, Ed</dc:creator>
      <dc:description><![CDATA[<p>How would the weather of a year from history be experienced in a warmer world? We reconstruct the weather of 1903 using a reanalysis system that assimilates only surface pressure observations (20CRv3) with observed SSTs, and then reconstruct it again with increased SSTs and atmospheric <span class="inline-formula">CO<sub>2</sub></span> levels. By assimilating the same pressure observations, the reanalysis experiments produce the same weather patterns, and so we translate the weather of 1903 into a warmer context. We focus on changes in the everyday weather of four regions with a high density of historical pressure observations, where the circulation is constrained and differences between the experiments are due to the thermodynamic component of climate change. In these regions, nearly all days are warmer in the warmer world experiments, but the largest increases occur on cold days (below freezing) and hot days (above 20 °C). Daily rainfall becomes more variable, even in regions where total rainfall is reduced. Fewer days experience light rain while more days experience heavy rain, and rainfall only increases on less than 1 d in 10. This single year pair of reanalysis experiments also recovers common patterns of observed and projected long-term changes. For example, Western Mediterranean precipitation declines outside winter, but shows a small increase in winter in the absence of storm track shifts. By anchoring our analysis in weather patterns that have actually occurred, the reanalysis experiments point to how our day-to-day experience of the same weather patterns may change in a warmer world, even if the weather patterns themselves do not.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-1365-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/1365/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:eo140575</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>eo</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[Brief communication: InSAR Svalbard Ground Motion Service – observing surface displacements in the High Arctic]]></dc:title>
      <dc:creator>Bredal, Marie</dc:creator>
      <dc:creator>Rouyet, Line</dc:creator>
      <dc:creator>Wendt, Lotte</dc:creator>
      <dc:creator>Hindberg, Heidi</dc:creator>
      <dc:creator>Stødle, Daniel</dc:creator>
      <dc:creator>Lauknes, Tom Rune</dc:creator>
      <dc:creator>Oostveen, Jelte</dc:creator>
      <dc:creator>Larsen, Yngvar</dc:creator>
      <dc:creator>Aslan, Gökhan</dc:creator>
      <dc:creator>Hauglin, Emma</dc:creator>
      <dc:creator>Dehls, John</dc:creator>
      <dc:creator>Sundal, Anja</dc:creator>
      <dc:creator>Odh, Anna</dc:creator>
      <dc:creator>Moldestad, Dag Anders</dc:creator>
      <dc:description><![CDATA[<p>The InSAR Svalbard Ground Motion Service (GMS) provides open-access surface displacement maps and time series in the Svalbard archipelago, derived from Sentinel-1 Interferometric Synthetic Aperture Radar (InSAR). The service provides seasonal products capturing short-term 2016–2024 displacements and interannual products documenting long-term 2018–2024 velocity trends. InSAR Svalbard covers five areas on Spitsbergen Island (Longyearbyen, Ny-Ålesund, Svea, Hornsund and Kapp Linné). The service consists in a web-based visualisation tool at <span class="uri">https://svalbard.insar.no/</span> (release date: 2 February 2026, last access: 22 September 2026). The products are also distributed at <a href="https://doi.org/10.5281/zenodo.18442696">https://doi.org/10.5281/zenodo.18442696</a> (Bredal et al., 2026a). InSAR Svalbard establishes a foundation for geohazard assessment in Arctic regions and interdisciplinary research on permafrost dynamics, ground stability, and environmental changes.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/eo-1-121-2026</dc:identifier>
      <dc:identifier><![CDATA[https://eo.copernicus.org/articles/1/121/2026/]]></dc:identifier>
      <dc:source>eISSN: 3054-1786</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd135993</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Simulating SAR altimeter echoes from cryospheric surfaces with the Snow Microwave Radiative Transfer (SMRT) model version 1.7]]></dc:title>
      <dc:creator>Picard, Ghislain</dc:creator>
      <dc:creator>Murfitt, Justin</dc:creator>
      <dc:creator>Zakharova, Elena</dc:creator>
      <dc:creator>Zeiger, Pierre</dc:creator>
      <dc:creator>Arnaud, Laurent</dc:creator>
      <dc:creator>Aublanc, Jeremie</dc:creator>
      <dc:creator>Landy, Jack C.</dc:creator>
      <dc:creator>Scagliola, Michele</dc:creator>
      <dc:creator>Duguay, Claude</dc:creator>
      <dc:description><![CDATA[<p>Radar altimeters are essential tools for observing the cryosphere, especially for estimating ice-sheet elevation change and sea-ice thickness. However, retrieving these quantities remains challenging, and progress depends on physically based numerical simulations of the recorded waveforms to understand their sensitivity to the geophysical parameters of the medium. Such models can also guide the design of future satellite missions. Accurate simulations require a balanced combination of a realistic description of the medium, precise calculation of wave–medium interactions, and an accurate representation of the altimeter measurement process, including downstream processing. The Snow Microwave Radiative Transfer (SMRT) model has addressed the first two aspects for a decade and includes an altimetric Low Resolution Mode (LRM) module, but has, until now, lacked a delay-Doppler (SAR) altimetric capability used by most modern sensors. This study introduces the new SMRT SAR altimetry module, which operates in three steps. First, it calculates the backscatter of all layers and interfaces using existing SMRT modules. Next, it models the waveforms of each layer and interface using a delay-Doppler approach. Finally, these components are combined to produce the final waveform. The user selects the delay-Doppler model from one of eight formulations reviewed, implemented, and compared in the literature. The validation first assesses these models under simple conditions, confirming they produce consistent results but differ in computational efficiency and flexibility. Subsequently, the new module is compared with external models to confirm its accuracy. Finally, it is applied to Antarctic conditions, where the simulations reproduce observed Sentinel-3 waveform variability linked to surface roughness. The open-source module, equipped with the eight options, now enables a wide range of numerical experiments, from studying penetration bias to exploring the potential for snow retrieval on sea ice and lake ice thickness.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9103-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9103/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd145385</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[MOISE station: Monthly environmental monitoring in the Southwestern lagoon of New Caledonia]]></dc:title>
      <dc:creator>Domergue, Salomé</dc:creator>
      <dc:creator>Rodier, Martine</dc:creator>
      <dc:creator>Dupouy, Cécile</dc:creator>
      <dc:creator>Duphil, Maxime</dc:creator>
      <dc:creator>Varillon, David</dc:creator>
      <dc:creator>Delepierre, Amandine</dc:creator>
      <dc:creator>Desnues, Anne</dc:creator>
      <dc:creator>Fiat, Sylvie</dc:creator>
      <dc:creator>Menkes, Christophe</dc:creator>
      <dc:description><![CDATA[From July 2012 to December 2024, in the Southwestern lagoon of New Caledonia, the MOISE station (<a href="https://www.mio.osupytheas.fr/fr/moise-mouillage-lagonaire-instrumente-suivi-biogeochimique/">https://www.mio.osupytheas.fr/fr/moise-mouillage-lagonaire-instrumente-suivi-biogeochimique/</a>, last access 26/08/2025) was surveyed with moored instruments and monthly visits providing unique long time series of hydrological and biogeochemical measurements in approximately 10m depth. The MOISE program objective was to characterize lagoon environmental variability across monthly, seasonal, and interannual timescales at a site potentially impacted by river outputs. Here we provided a 13-year quality-controlled dataset with vertical profiles of temperature, salinity, and chlorophyll-adjusted fluorescence from CTDs and continuous currents from a moored 600 kHz Acoustic Doppler Current Profile (ADCP).<br />This site represents the unique location in New Caledonia lagoon to deliver an extended multi-parameter time series of &nbsp;long-term monitoring of the lagoon&rsquo;s environmental state and circulation dynamics. The length of the time series allowed the depiction of the ENSO impact (El Ni&ntilde;o-Southern Oscillation) on the interannual variability. A clear seasonal cycle was also observed, with higher chlorophyll during austral summer when temperatures are highest, salinity lowest and wind-driven currents strongest and predominantly directed toward the west-northwest. MOISE data further highlight the strong influence of extreme events such as tropical cyclones, tropical depressions and heavy rainfall, on the lagoon, which can induce temporary stratification of the water column that is otherwise generally homogeneous.&nbsp;<br />The dataset was post processed, quality controlled and is available in netcdf on SEANOE in open access (SEA ScieNtific Open data Edition) at the following DOI : <a href="https://doi.org/10.17882/98821">https://doi.org/10.17882/98821</a>.&nbsp;]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-653</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-653/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd138431</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[META4.0: a new global mesoscale eddy  network atlas derived from altimetry]]></dc:title>
      <dc:creator>Gamot, Juliette</dc:creator>
      <dc:creator>Delepoulle, Antoine</dc:creator>
      <dc:creator>Nencioli, Francesco</dc:creator>
      <dc:creator>Pujol, Marie-Isabelle</dc:creator>
      <dc:creator>Dibarboure, Gerald</dc:creator>
      <dc:description><![CDATA[<p>This study introduces the new global Mesoscale Eddy Trajectory Atlases, META4.0 available in an AVISO repository at <a href="https://doi.org/10.24400/527896/a01-2026.001">https://doi.org/10.24400/527896/a01-2026.001</a> <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx16">CLS and CNES</a>, <a href="#bib1.bibx16">2026</a>)</span>. META4.0 provides eddy detections, trajectories, and interaction networks derived from satellite altimetry. Eddy detection relies on the <code>pyeddytracker</code> (PET) algorithm <span class="cit" id="xref_paren.2">(<a href="#bib1.bibx42">Mason et al.</a>, <a href="#bib1.bibx42">2014</a>)</span>, further optimized by <span class="cit" id="xref_text.3"><a href="#bib1.bibx48">Pegliasco et al.</a> (<a href="#bib1.bibx48">2022</a>)</span>, and represents a substantial improvement over the previous META3.2 product (SSALTO/DUACS, distributed by AVISO<span class="inline-formula">+</span> with CNES support).</p>        <p>The main advance of META4.0 is the explicit identification of eddy merging and splitting events. By combining grouping, which links detections across consecutive days, and segmentation, which tracks continuity through interaction events, trajectories are organized into networks of interconnected eddies. This network-based representation complements the single-trajectory view of eddy life cycles by explicitly accounting for eddy interactions.</p>        <p>The paper presents both diagnostic tools designed to explore individual eddy networks (e.g., timelines, spatial trajectories, and eddy properties such as effective radius or shape error) and the results of a global statistical analysis over more than three decades. These tools and analyses offer new diagnostics for investigating network properties, eddy lifetimes, and the spatial and temporal distribution of merging and splitting events of the META4.0 atlas. Clustering analyses reveal recurrent interaction patterns and identify regions where eddy networks are particularly active. An independent dataset of surface chlorophyll concentration is used for qualitative validation of selected events. Finally, Lagrangian advection of synthetic particles highlights coherent forward and backward transport signatures associated with interaction events, providing a physical validation of the reconstructed networks.</p>        <p>Overall, META4.0 offers a novel and physically consistent framework to characterize mesoscale eddy interactions and to better understand their role in shaping ocean dynamics.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-7043-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/7043/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd137122</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Global 30&thinsp;m annual cropland extent dynamics (2000–2024): a harmonized baseline of structural evolution and regional disparities]]></dc:title>
      <dc:creator>Liao, Yuanhong</dc:creator>
      <dc:creator>Chen, Shuang</dc:creator>
      <dc:creator>Bai, Yuqi</dc:creator>
      <dc:creator>Wang, Jie</dc:creator>
      <dc:creator>Gong, Peng</dc:creator>
      <dc:description><![CDATA[<p>Accurate annual information on cropland extent is essential for monitoring agricultural change, yet existing global products are often limited to snapshots or multiyear epochs and differ in their cropland definitions. Here we present GACED30, which, to our knowledge, is the first dedicated global 30 m annual cropland-extent dataset covering 2000–2024. The mapping framework combines gap-free SDC30 observations, spectral-semantic alignment of expert-annotated and spatially augmented samples, and rule-based spatial and temporal refinement. Independent classifiers were trained for each year using a common observation, feature, sample-construction, and modeling protocol, and the resulting annual record was used to derive pixel-level Cropping Frequency and 1 km Structural Evolution Indicators. Against independent stable-site FAST-Crop samples, GACED30 achieved an overall accuracy of 0.965 and an F<span class="inline-formula"><sub>1</sub></span> score of 0.844. Multitemporal assessments using GLAD Cropland and LUCAS reference samples showed higher recall and F<span class="inline-formula"><sub>1</sub></span> scores than GLC_FCS30D for both crop gain and crop loss, although the absolute transition scores remained modest. In a matched regional assessment in China, GACED30 achieved OA and F1 scores of 0.946 and 0.840, respectively, showing performance comparable with CACD. At the national scale, GACED30 agreed closely with definition-reconciled FAOSTAT statistics (<span class="inline-formula"><i>R</i><sup>2</sup></span>: 0.95; area-weighted direction match rate: 83.1 %). The sample-adjusted global cropland area was estimated at 1488.5 Mha in 2024, approximately 30.0 Mha higher than in 2000. Persistent expansion was concentrated in parts of Africa and South America, whereas stability and reduction were more widespread across much of the Global North. GACED30 provides a harmonized baseline for monitoring global cropland-extent dynamics and is publicly available at <a href="https://doi.org/10.5281/zenodo.18199675">https://doi.org/10.5281/zenodo.18199675</a> (Chen et al., 2026).</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-7071-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/7071/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:angeo138728</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>angeo</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[Mesoscale structure of flickering aurora from wide-field high-speed imaging]]></dc:title>
      <dc:creator>Nanjo, Sota</dc:creator>
      <dc:creator>Kurita, Satoshi</dc:creator>
      <dc:creator>Sergienko, Tima</dc:creator>
      <dc:creator>Miyoshi, Yoshizumi</dc:creator>
      <dc:creator>Kataoka, Ryuho</dc:creator>
      <dc:description><![CDATA[<p>We report wide-field observations of flickering aurora obtained with a fast sCMOS camera and a diagonal fisheye lens at Poker Flat Research Range, Alaska, on 8 February 2016. The system recorded <span class="inline-formula">512×512</span> pixel images at 80 Hz, enabling us to investigate the mesoscale organization of flickering along a discrete auroral arc over spatial scales of several hundred kilometers. Flickering occurred intermittently with dominant frequencies between 3 and 20 Hz, most commonly within a narrower band of 4–12 Hz. Spatial maps of the peak frequency reveal that regions with similar periodicities sometimes formed coherent clusters on scales of <span class="inline-formula">∼</span> 10 km, and that multiple clusters with different frequencies (e.g., <span class="inline-formula">∼8</span> and <span class="inline-formula">∼13</span> Hz) could coexist simultaneously along the same arc, separated by <span class="inline-formula">∼150</span> km. Some of these clusters moved together with the background arc, suggesting that the modulation is closely tied to the local plasma environment and inverted-V potential structures associated with discrete aurora. An automated patch detection analysis showed that, although individual events may locally suggest an inverse relationship between flickering frequency and patch size, this trend does not persist statistically. Instead, flickering at a given dominant frequency occurs over a wide range of patch sizes, with a typical apparent north–south scale of <span class="inline-formula">4.4±2.4</span> km when projected to an assumed emission altitude of 110 km. These results are consistent with generation scenarios in which electron precipitation is modulated by interference among multiple EMIC waves in the auroral acceleration region, extending previous narrow-field studies to the mesoscale and demonstrating the diagnostic value of wide-field, high-cadence imaging for wave–particle interactions in the auroral ionosphere.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/angeo-44-959-2026</dc:identifier>
      <dc:identifier><![CDATA[https://angeo.copernicus.org/articles/44/959/2026/]]></dc:identifier>
      <dc:source>eISSN: 1432-0576</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:amt139463</identifier>
    <datestamp>2026-09-25</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[Feasibility of measuring volcanic gas composition using sky-scattered sunlight and FTIR spectroscopy]]></dc:title>
      <dc:creator>Schmitt, Tobias D.</dc:creator>
      <dc:creator>Sindram, Moritz</dc:creator>
      <dc:creator>Löw, Benedikt A.</dc:creator>
      <dc:creator>Weis, Lukas</dc:creator>
      <dc:creator>Kleinschek, Ralph</dc:creator>
      <dc:creator>Bobrowski, Nicole</dc:creator>
      <dc:creator>Butz, André</dc:creator>
      <dc:description><![CDATA[<p>Monitoring volcanic emissions is essential for understanding volcanic processes and predicting eruption dynamics. Remote sensing is the only method that allows safe measurements right before, during, and after eruptions. Current monitoring relies on scattered sunlight, whose essentially unconstrained viewing geometry permits continuous and automated observation. It is, however, mostly limited to the ultraviolet and visible (UV-VIS) spectral ranges by the available sky brightness, restricting observations largely to <span class="inline-formula">SO<sub>2</sub></span>.</p>        <p>Here, we assess the feasibility of constraining volcanic emissions by passive Fourier transform infrared (FTIR) spectroscopy of sky-scattered sunlight in the near-infrared (NIR), where more gases of interest have absorption features. Combining an instrument model for the spectral signal-to-noise ratio (SNR) with an information-content analysis, and incorporating actual measurements to capture the systematic uncertainties inherent to atmospheric total column retrievals, we estimate detection limits for individual trace gas columns. The instrument model accurately reproduces the results of laboratory validation experiments. We use Mount Etna as a representative high-emission volcano. We find that <span class="inline-formula">CO<sub>2</sub></span> column measurements remain challenging: the plume enhancement is small compared to the high and variable atmospheric background, and little scattered light is available in the NIR. Even under bright skies, reaching a detection limit comparable to the expected column enhancement takes about 5 min, and up to 2.5 h under dark conditions. Plume transects, which require many such measurements at substantially better precision, are therefore out of reach, whereas individual plume-composition measurements remain conceivable. In contrast, the strongly emitted halogen species <span class="inline-formula">HCl</span> and <span class="inline-formula">HF</span>, whose atmospheric background is low, are detectable within seconds under bright skies and within a few minutes under dark conditions. For these species, a multi-instrument approach makes plume-composition measurements practical: pairing the FTIR with co-aligned UV observations of <span class="inline-formula">SO<sub>2</sub></span> yields gas ratios that, combined with established <span class="inline-formula">SO<sub>2</sub></span> flux networks, give access to the halogen emissions. For <span class="inline-formula">CO<sub>2</sub></span> this route is not excluded, but limited precision and the impact of radiative transfer errors on a background-dominated retrieval make the outcome hard to predict. Finally, this SNR and detection-limit analysis transfers to other instruments, spectral regions, target species, and emission sources.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-6145-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/6145/2026/]]></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:amt136997</identifier>
    <datestamp>2026-09-25</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[Employing smoothness of the time series of sky radiances measured in the solar aureole for cloud screening]]></dc:title>
      <dc:creator>Sinyuk, Alexander</dc:creator>
      <dc:creator>Eck, Thomas F.</dc:creator>
      <dc:creator>Slutsker, Ilya</dc:creator>
      <dc:creator>Lewis, Jasper</dc:creator>
      <dc:creator>Grigorov, Petar</dc:creator>
      <dc:creator>Smirnov, Alexander</dc:creator>
      <dc:creator>Schafer, Joel S.</dc:creator>
      <dc:creator>Sorokin, Mikhail</dc:creator>
      <dc:creator>Lind, Elena</dc:creator>
      <dc:creator>Gupta, Pawan</dc:creator>
      <dc:description><![CDATA[<p>Cloud screening algorithms have always been a critical component of Aerosol Robotic Network (AERONET) aerosol optical depth (AOD) Level 1.5 and 2.0 product. The initial cloud screening algorithm in the Version 1 and 2 database was semi-automatic and required involvement of a human analyst to finalize  the results. It became fully automatic in Version 3 (V3) due to  employing information on the angular shape of sky radiances measured in the aureole (curvature algorithm). Although efficient, the curvature algorithm is threshold based and fails to detect clouds when its parameters are beyond the corresponding pre-determined thresholds. This is especially noticeable at high latitudes where the size of ice crystals in cirrus clouds are sometimes relatively small and therefore comparable in size to aerosols. It is shown that additional information can be extracted from analysis of the smoothness of diurnal variability of sky radiances measured at the 3.3° scattering angle. This measurement is a part of the  so-called curvature scan (CCS), which takes  measurements from 3 to 7.5° scattering angle with 0.3° steps after each measurement of AOD. The analysis of the diurnal variability of CCS (3.3) for cloud-free conditions shows relatively smooth temporal dependencies, which can be fitted by polynomials with high correlation coefficients while in conditions almost completely dominated by clouds, the temporal variability is completely random. For partially cloudy days, the two main features are observed: relatively smooth aerosol signatures and irregular spikes due to clouds. The new technique is proposed that employs the smoothness of the diurnal variability of the CCS(3.3) scan as a criterion of the cloud free conditions. In the case when both features are present, the idea of the new algorithm is to remove irregular spikes due to clouds while  keeping the smooth part due to aerosols intact. The new algorithm detects spikes associated with clouds by comparing magnitudes of CCS(3.3) at neighboring time stamps through calculating their first differences (FD). This  algorithm was applied to the CCS(3.3) measurements taken at several AERONET sites. The results were analyzed in terms of net change in Angstrom exponent (AE) as well as number of AOD measurements. The analysis showed the algorithm performs satisfactorily  at AERONET sites dominated by fine mode aerosols, however at sites dominated by dust, the algorithm removes a big fraction of cloud-free observations. The issue was corrected by introducing an additional cloud screening parameter. It is based on observation of the different rates in changing  of AE with iterations for cloud-free and cloudy conditions with a much higher rate in the former case. The new parameter was selected as a slope of the linear regression between integration number and the value of AE after the corresponding iteration. The algorithm disregards FD algorithm results if the slope is smaller than certain threshold value. Finalizing  the FD algorithm threshold setting as well as evaluation of the algorithm performance is done by using independent cloud detection information available from Micro-Pulse Lidar Network (MPLNET) data. The AERONET and MPLNET data were time and space collocated with additional averaging over a one-hour period. The comparison showed that, on average, the FD algorithm outperformed V3 L1.5 by about 0.02 in Matthews Correlation Coefficient (MCC), suggesting<span id="page6126"/> consistent improvement in overall cloud detection accuracy. Additional analysis performed in terms of MCC metrics also showed  that the FD algorithm achieves a more balanced and accurate classification of clouds vs clear.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-6125-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/6125/2026/]]></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:amt135934</identifier>
    <datestamp>2026-09-25</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/
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      <dc:title><![CDATA[Global variability in the detectability of power plant NO2  plumes from space]]></dc:title>
      <dc:creator>Huang, Ruizhe</dc:creator>
      <dc:creator>Wang, Sherrie</dc:creator>
      <dc:description><![CDATA[<p>We present the first global, data-driven analysis of power plant <span class="inline-formula">NO<sub>2</sub></span> plume detectability from space. Using TROPOspheric Monitoring Instrument (TROPOMI) observations (nadir pixel size 3.5–7 <span class="inline-formula">km</span>) over 6000 of the world's highest-emitting power plants and hourly Continuous Emissions Monitoring Systems (CEMS) data for 500 US plants, we develop an automated algorithm that labels plumes and attributes them to their sources with 98 % accuracy. For the subsequent detectability analysis, we restrict to plants outside interference zones (at least 20 <span class="inline-formula">km</span> from other major power plants and 45–90 <span class="inline-formula">km</span> from cities (depending on city size)), which retains 45.0 % of US and 21.1 % of global <span class="inline-formula">NO<sub><i>x</i></sub></span> emissions in our datasets. We then train a machine learning model to predict plume detectability (the probability of detection given the observation conditions) from meteorological, environmental, sensor, and power-plant variables sampled at the single TROPOMI pixel over each plant (<span class="inline-formula">F1 score&gt;0.66</span>, <span class="inline-formula">AUC&gt;0.8</span>). Out of 25 variables, we find that <span class="inline-formula">NO<sub><i>x</i></sub></span> emission rate, surface altitude, surface albedo (<span class="inline-formula">NO<sub>2</sub></span> window), sensor zenith angle, primary fuel type, and wind speed jointly explain much of the variability in detectability. For US power plants, an hourly <span class="inline-formula">NO<sub><i>x</i></sub></span> emission rate of <span class="inline-formula">≈</span> 400 <span class="inline-formula">kg h<sup>−1</sup></span> corresponds to <span class="inline-formula">∼</span> 50 % detectability, but detectability varies from <span class="inline-formula">&lt;</span> 20 % to <span class="inline-formula">&gt;</span> 60 % under different combinations of these conditions. These results provide the first empirical quantification of the physical and environmental factors that govern <span class="inline-formula">NO<sub>2</sub></span> plume visibility in TROPOMI data, establishing a foundation for models to use similar predictors as auxiliary variables when quantifying emission rates from plume appearance.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-6099-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/6099/2026/]]></dc:identifier>
      <dc:source>eISSN: 1867-8548</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:acp139798</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>acp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Assessment of aerosol iron (Fe) solubility using global dataset – Part 1: Mechanisms underlying the inverse relationship between Fe solubility and Fe concentration]]></dc:title>
      <dc:creator>Sakata, Kohei</dc:creator>
      <dc:creator>Kurisu, Minako</dc:creator>
      <dc:creator>Takahashi, Yoshio</dc:creator>
      <dc:description><![CDATA[<p>Atmospheric deposition of aerosol iron (Fe) can stimulate marine primary productivity by supplying dissolved Fe (d-Fe) to the surface ocean, thereby potentially influencing the global climate. Aerosol Fe solubility (Fe<span class="inline-formula"><sub>sol</sub></span>%) is closely linked to its bioavailability, and previous studies have shown that Fe<span class="inline-formula"><sub>sol</sub></span>% generally increases as aerosol Fe concentration decreases. However, the mechanism underlying this widely observed inverse relationship remains unresolved. In this study, aerosol observations from East Asia, the North and South Pacific, and the Atlantic were compiled, and the enrichment factor of total Fe (EF<span class="inline-formula"><sub>T-Fe</sub></span> = (T-Fe <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="57ee8123d9c9aefcf23d9c7f6463c158"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-13505-2026-ie00001.svg" width="8pt" height="14pt" src="acp-26-13505-2026-ie00001.png"/></svg:svg></span></span> T-Al)<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mtext>aerosol</mtext></msub><mo>/</mo></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="35pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="4add1ae4ced3b3e482604ba53bd21ec3"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-13505-2026-ie00002.svg" width="35pt" height="14pt" src="acp-26-13505-2026-ie00002.png"/></svg:svg></span></span> (T-Fe <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="073414a2b77546d8d5847ae97897d626"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-13505-2026-ie00003.svg" width="8pt" height="14pt" src="acp-26-13505-2026-ie00003.png"/></svg:svg></span></span> T-Al)<span class="inline-formula"><sub>crust</sub></span>) and dissolved Fe to dissolved Al ([d-Fe] <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="fb147fccdcf98a9911cf3d26a8f6dc33"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-13505-2026-ie00004.svg" width="8pt" height="14pt" src="acp-26-13505-2026-ie00004.png"/></svg:svg></span></span> [d-Al]) were used to estimate the contributions of mineral-derived and anthropogenic Fe to aerosol d-Fe, as well as the Fe<span class="inline-formula"><sub>sol</sub></span>% of each source fraction. Aerosol d-Fe was found to be derived predominantly from mineral dust in many oceanic regions. In addition, both mineral-derived Fe and anthropogenic Fe showed inverse relationships between concentration and solubility. If the inverse relationship between Fe concentration and Fe<span class="inline-formula"><sub>sol</sub></span>% were controlled mainly by simple two-component mixing between low-solubility mineral particles and highly soluble anthropogenic Fe, the Fe<span class="inline-formula"><sub>sol</sub></span>% of each source fraction would not be expected to vary systematically with concentration. Instead, the results suggest that atmospheric chemical processing, together with depositional removal during transport, progressively increases the solubility of Fe remaining in aerosol particles. The ability to estimate the sources and dissolution processes of aerosol Fe from such fundamental concentration data may help improve the parameterization of aerosol Fe dissolution in global climate models.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-13505-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/13505/2026/]]></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:acp133449</identifier>
    <datestamp>2026-09-25</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/
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      <dc:title><![CDATA[The dynamics and atmospheric impact of fire-induced circulations in idealised large-eddy simulations inspired by the Santa Coloma de Queralt fire]]></dc:title>
      <dc:creator>Roelofs, Tristan</dc:creator>
      <dc:creator>Castellnou, Marc</dc:creator>
      <dc:creator>Vilà-Guerau de Arellano, Jordi</dc:creator>
      <dc:creator>Janssens, Martin</dc:creator>
      <dc:creator>Heerwaarden, Chiel</dc:creator>
      <dc:description><![CDATA[<p>We studied the factors governing the existence of fire-induced circulations ahead of the flaming zone and the impact of these circulations on the thermodynamic structure of the atmospheric boundary layer. To study the circulation, we used MicroHH to create a high-resolution (25 <span class="inline-formula">m</span>) turbulence-resolving 3D large-eddy simulations (<span class="inline-formula">25.6 km×38.4 km</span>) of a stationary fire under realistic atmospheric conditions. The setup was inspired by field observations of fire characteristics and a radiosonde from the Santa Coloma de Queralt fire (Catalonia, Spain, 24 July 2021). The stationary fire enabled us to isolate the persistent impacts of the fire on the atmosphere.</p>        <p>Our results indicate that the existence of a fire-induced circulation is governed by the wind speed component aligned with the circulation. In our simulations, the circulation consisted of updrafts above the fire, downdrafts 2 <span class="inline-formula">km</span> ahead, and reversed surface winds between the updrafts and downdrafts. With higher wind speeds in the direction of the circulation, the reversal of the surface winds decreases. Consequently, the circulation dissipates, since the reversed winds connect the updrafts and downdrafts into a circulation. Hence, explaining why fire-induced circulations are not always present.</p>        <p>The thermodynamic impact of the circulation is driven by the updrafts and downdrafts, causing 2 <span class="inline-formula">km</span> of deepening,  followed by 2 <span class="inline-formula">km</span> of thinning of the atmospheric boundary layer ahead of the fire. Future research with non-stationary fires is required to quantify the impact of the modified thermodynamics and wind patterns on fire behaviour.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-13531-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/13531/2026/]]></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:acp131590</identifier>
    <datestamp>2026-09-25</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[Climate impact of contrail cirrus from hydrogen combustion aircraft]]></dc:title>
      <dc:creator>Pettersson, Susanne M.</dc:creator>
      <dc:creator>Azar, Christian</dc:creator>
      <dc:creator>Johansson, Daniel J. A.</dc:creator>
      <dc:description><![CDATA[<p>One possibility for reducing the climate impact of aviation is to transition to aircraft powered by hydrogen combustion. Hydrogen combustion leads to zero CO<span class="inline-formula"><sub>2</sub></span> exhaust emissions and represents a potential major step toward reduced climate impact, although the non-CO<span class="inline-formula"><sub>2</sub></span> effects (primarily contrail cirrus) remain uncertain. In this study, we simulate the climate impact, in terms of energy forcing, of contrail cirrus from hydrogen combustion aviation, using a modified version of the Contrail Cirrus Prediction model (CoCiP).</p>        <p>With no soot in the exhaust, contrail ice particles mainly form on ambient aerosols entrained into the plume and on lubrication oil droplets in the exhaust. The formation of ice particles is modelled using an emulator developed from a theoretically based microphysical contrail formation model.</p>        <p>Following the Schmidt-Appleman criterion, hydrogen combustion enables contrail formation at lower altitudes and higher temperatures than fossil jet fuel. However, we find a significant reduction in contrail energy forcing. This result holds across a wide range of assumptions, with a global average reduction of about 66 % using our base case assumptions on ambient aerosols, lubrication oil properties, droplet size distribution, emission index and energy efficiency of hydrogen aircraft. We conclude that hydrogen aircraft not only eliminate CO<span class="inline-formula"><sub>2</sub></span> emissions in the exhaust, but may also reduce the climate impact of contrail cirrus, depending on engine design for lubrication oil handling. However, we acknowledge that the modelling approach has limitations and uncertainties. Before firm conclusions can be drawn about the contrail cirrus effects of hydrogen-combustion aircraft, further studies are needed. These should include more realistic hydrogen aircraft models, alternative meteorological and microphysical models, and analyses of real-world flight patterns. In particular, measurements of lubrication-oil emissions from hydrogen aircraft under cruise conditions, as well as measurements of ice crystal number concentrations in hydrogen-aircraft contrails, would be valuable for constraining the present analysis.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-13485-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/13485/2026/]]></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:acp129418</identifier>
    <datestamp>2026-09-25</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[Simulated reductions in heterogeneous isoprene epoxydiol reactive uptake from aerosol morphology in the contiguous United States using the Community Multiscale Air Quality Model (CMAQv5.3.2)]]></dc:title>
      <dc:creator>Farrell, Sara L.</dc:creator>
      <dc:creator>Rasool, Quazi Z.</dc:creator>
      <dc:creator>Pye, Havala O. T.</dc:creator>
      <dc:creator>Zhang, Yue</dc:creator>
      <dc:creator>Li, Ying</dc:creator>
      <dc:creator>Chen, Yuzhi</dc:creator>
      <dc:creator>Wang, Chi-Tsan</dc:creator>
      <dc:creator>Zhang, Haofei</dc:creator>
      <dc:creator>Schmedding, Ryan</dc:creator>
      <dc:creator>Shiraiwa, Manabu</dc:creator>
      <dc:creator>Green, Jaime</dc:creator>
      <dc:creator>Budisulistiorini, Sri H.</dc:creator>
      <dc:creator>Jimenez, Jose L.</dc:creator>
      <dc:creator>Hu, Weiwei</dc:creator>
      <dc:creator>Surratt, Jason D.</dc:creator>
      <dc:creator>Vizuete, William</dc:creator>
      <dc:description><![CDATA[<p>Aerosol particles contain complex mixtures of polar and non-polar species that can undergo organic-inorganic phase separation. In phase-separated aerosol particles, the phase state of the outer organic coating can modulate heterogeneous chemistry. Heterogeneous chemistry leading to isoprene epoxydiol (IEPOX)-derived secondary organic aerosol (IEPOX-SOA) is encoded in the Community Multiscale Air Quality (CMAQ) model and has been the focus of previous aerosol phase separation and phase state work. In a previous study, a constant ratio of water in the organic coating (<span class="inline-formula"><i>w</i><sub>s</sub></span>) was assumed in modeling phase separation and state. Recent studies, however, have highlighted <span class="inline-formula"><i>w</i><sub>s</sub></span> as an important modulator of phase state. This work uses a later CMAQ version (version 5.3.2) with capabilities to model dynamic water uptake to the organic coating – to better predict <span class="inline-formula"><i>w</i><sub>s</sub></span> and its impact on the organic coating phase state. In addition, new parameterizations for estimating organic aerosol phase state were encoded into CMAQ, and were compared with respect to their impacts on phase state and IEPOX-SOA predictions. These evaluations were completed simulating a summertime episode over the continental United States. Simulated diurnal profiles of aerosol phase state agreed within one standard deviation of<span id="page13558"/> observationally-derived field measurements. The implementation of phase separation and phase state parameterizations resulted in times and grid cells where IEPOX reactive uptake is completely suppressed. While modelled positive bias in 2-methyltetrol concentrations were decreased with phase separation and phase state updates, modelled methyltetrol sulfates and total IEPOX-SOA concentrations further underpredicted field observations in comparison to Base CMAQ.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-13557-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/13557/2026/]]></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:egusphere146592</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The Role of Particle Size Distribution in Simulating Aerosol Transport, Radiative Effects and Surface Area of the 2019/20 Australian pyroCb Plume]]></dc:title>
      <dc:creator>Das, Sampa</dc:creator>
      <dc:creator>Colarco, Peter R.</dc:creator>
      <dc:creator>Case, Parker</dc:creator>
      <dc:creator>Steenrod, Stephen</dc:creator>
      <dc:creator>Oman, Luke D.</dc:creator>
      <dc:creator>Taha, Ghassan</dc:creator>
      <dc:description><![CDATA[The 2019/2020 Australian New Year (ANY) pyrocumulonimbus (pyroCb) events injected massive quantities of smoke into the stratosphere, significantly altering Earth's radiative balance and chemical composition. Accurately simulating these impacts in Earth System Models (ESMs) remains challenging, partly because standard bulk aerosol schemes assume particle properties based on tropospheric smoke. In this study, we leverage the NASA GEOS model coupled with the CARMA sectional microphysics module to simulate the rapid microphysical evolution of the ANY pyroCb plume. Our sectional aerosol model simulations reveal that extreme initial number densities drive rapid coagulation, producing stabilized aged particles with an effective radius (<em>R<sub>eff</sub></em>) of ~ 0.30 &micro;m, consistent with in-situ and lidar observations. Based on these results and offline Mie-theory calculations, we derive an observationally constrained configuration (<em>R</em><sub><em>eff</em></sub> = 0.30 &micro;m, &sigma; = 1.2, with moderated near-UV absorption) for the computationally efficient GOCART-2G bulk aerosol module. Compared to the finer-mode baseline, the updated configuration significantly improves simulated aerosol extinction and &Aring;ngstr&ouml;m Exponent, bringing the plume's spatial distribution and longevity into closer agreement with SAGE-III/ISS and OMPS-LP satellite records. Furthermore, pairing the larger particle size with observationally constrained absorption moderates excessive shortwave radiative heating, enabling more realistic large-scale transport. The larger particle size assumption also reduces the available aerosol Surface Area Density (SAD) by more than a factor of three. Our findings highlight a critical sensitivity to particle size assumptions in simulating large pyroCb events, demonstrating that constraining this property is essential for accurately assessing the plume's radiative impact and its role in heterogeneous chemistry.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5642</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5642/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145596</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[3D surface displacements from digital image correlation on terrain models]]></dc:title>
      <dc:creator>Oestreicher, Nicolas</dc:creator>
      <dc:creator>Denzinger, Florian</dc:creator>
      <dc:creator>Manconi, Andrea</dc:creator>
      <dc:description><![CDATA[We present a methodology to retrieve 3D surface displacement based on Digital Image Correlation (DIC) applied<br />to multitemporal terrain models. Our approach has been developed to overcome the DIC limitation in the vertical component<br />of the displacement field when horizontal shifts are larger than the grid sampling. To validate the performance, we applied<br />the approach to two terrain models acquired over the Brienz/Brinzauls landslide, where surface displacements affect the entire<br />slope with heterogeneous amplitudes and directions. The comparison with in-situ measurements shows that DIC can accurately<br />retrieve horizontal and vertical displacements, providing a clear representation of the spatial extent of the mass movement, as<br />well as an accurate distinction of the internal landslide compartments. Our results are in good agreement with those obtained<br />using a state-of-the-art point correlation method, but require less preprocessing and computational effort. Thus, the proposed<br />DIC strategy can be considered as a valid alternative for measuring 3D surface displacements in scenarios where multitemporal<br />terrain models are available.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5055</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5055/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145758</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[How much of a regional Coulomb stress map survives its own uncertainty? An audit with forecast-skill validation for T&uuml;rkiye]]></dc:title>
      <dc:creator>Vural, Mehmet Sait</dc:creator>
      <dc:description><![CDATA[Static Coulomb stress transfer is increasingly automated over open catalogues and fault databases rather than built by hand for single events. We ask how much of such a result survives its own inputs. For T&uuml;rkiye we resolve the stress imparted by 46 Mw &ge; 6 earthquakes between 1990 and 2026 onto 6,970 sub-segments of the mapped active-fault network, screening each across 25 parameter combinations. Three silent failure modes emerge. First, 44 records of the GEM Global Active Faults Database store a central rake 180&deg; from the circular midpoint of their own bounds; all lie in two source compilations, one being the principal North Anatolian Fault strand south of Istanbul, where it reverses the stress change from &minus;0.029 to +0.251 MPa. Second, anchoring ruptures on catalogue centroids rather than mapped traces displaces them by a median of 18.4 km; across 27 testable events this flips the sign on a median of 11.9 % of segments against 2.0 % for a rake &plusmn;15&deg; and dip &plusmn;10&deg; perturbation, and is the larger of the two in 20 of them. Third, sign stability rises from 74.3 % to 89.5 % between 1 and 50 kPa. A pseudo-prospective test against subsequent seismicity gives a segment-weighted AUC of 0.711 for Mw &lt; 7 sources, but clustering leaves an effective sample of 42, one event supplies 38 % of it, an event-equal estimate gives 0.589 &plusmn; 0.112, and distance matching leaves 0.655 with an interval spanning 0.5. Screening improves the estimate by +0.016 (95 % paired bootstrap [+0.001, +0.051]; one-sided p = 0.020). The forecast evidence is suggestive rather than strong; the two input-integrity findings do not depend on it. Coulomb maps should be published with an explicit statement of which parts are interpretable.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5171</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5171/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146417</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Precision and reproducibility of cosmogenic 10Be and 26Al measurements assessed from a multi-laboratory compilation of duplicate and reference material analyses]]></dc:title>
      <dc:creator>Wilcken, Klaus M.</dc:creator>
      <dc:creator>Fülöp, Réka-H.</dc:creator>
      <dc:creator>Simon, Krista</dc:creator>
      <dc:creator>Kotevski, Steve</dc:creator>
      <dc:creator>Codilean, Alexandru T.</dc:creator>
      <dc:creator>Rood, Anna H.</dc:creator>
      <dc:creator>Rood, Dylan H.</dc:creator>
      <dc:description><![CDATA[To quantify the reproducibility and precision of cosmogenic <sup>10</sup>Be and <sup>26</sup>Al analyses, we analysed a suite of liquid and quartz reference materials, together with duplicate preparations of unknown research samples. Comparison among these materials allows us to constrain uncertainties associated with AMS measurement, chemical extraction, and quartz purification, and to assess whether additional variability is introduced at successive stages of the analytical process. Samples were prepared in three chemistry laboratories at the Australian Nuclear Science and Technology Organisation (ANSTO), the University of Wollongong (UOW), and Imperial College London, and subsequently analysed by accelerator mass spectrometry (AMS) using the 6 MV SIRIUS accelerator at ANSTO. All three laboratories showed intra-laboratory variability below the routine 2% analytical uncertainty, while measured values were consistent with the nominal values of the reference materials. These results indicate that both methodological reproducibility and inter-laboratory variability are also within the analytical uncertainty, and provide no evidence for additional uncertainty associated with processing quartz relative to liquid reference materials. The implications for cosmogenic-nuclide research are that: (1) the reproducibility and precision of cosmogenic <sup>10</sup>Be and <sup>26</sup>Al analyses are typically 2&ndash;3% when sufficient counting statistics are achieved; (2) at lower isotope concentrations, counting statistics and/or background corrections may limit the achievable measurement uncertainty, although the resulting variability remains consistent with the reported analytical precision; and (3) precision of approximately 1% is achievable for high-concentration liquid reference materials, as demonstrated by Be-KN-5-4 and Al-KN-4-3, but has not yet been demonstrated for quartz samples.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5512</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5512/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146335</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[3-D characterization of Arctic lake ice with polarimetric SAR tomography at X- and C-band]]></dc:title>
      <dc:creator>Saporta, Paloma</dc:creator>
      <dc:creator>Pardini, Matteo</dc:creator>
      <dc:creator>Wilcox, Evan J.</dc:creator>
      <dc:creator>Boike, Julia</dc:creator>
      <dc:creator>Hajnsek, Irena</dc:creator>
      <dc:description><![CDATA[This study investigates for the first time the three-dimensional structure of Arctic lake ice based on tomographic reconstruction from a polarimetric, multi-baseline airborne&nbsp; Synthetic Aperture Radar (SAR) data set. The tomographic reconstruction indicates the presence of two strong interfaces at both X- and C-band, which can be attributed, based on field observations, to the air/ice and ice/liquid water interfaces. This means that the tomographic reconstruction is sensitive to the thickness of the ice layer of the investigated lakes. The reconstructed vertical reflectivity profiles are found to vary with polarization, therefore they can only be interpreted with a dedicated polarimetric analysis. In some lakes, we observe regions characterized by scattering with high entropy focused at the ice/water interface. We propose several hypotheses regarding the physical origin of these regions. Finally, requirements for the estimation of lake ice thickness from multi-baseline SAR are formulated to support the planning of future spaceborne SAR missions with tomographic capabilities.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5452</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5452/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146316</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Improving Reconstructed HY-1D/COCTS SST for Upwelling Events in the Gulf of Lion through Wind-Informed Cloud Detection]]></dc:title>
      <dc:creator>Li, Zhuomin</dc:creator>
      <dc:creator>Alvera-Azcárate, Aida</dc:creator>
      <dc:creator>Barth, Alexander</dc:creator>
      <dc:creator>Bensoussan, Nathaniel</dc:creator>
      <dc:creator>Guan, Lei</dc:creator>
      <dc:creator>Xu, Na</dc:creator>
      <dc:description><![CDATA[Sea surface temperature (SST) is essential for understanding ocean dynamics and air-sea interactions. SST from the Haiyang-1D (HY-1D) Chinese Ocean Color and Temperature Scanner (COCTS) has been obtained based on the algorithm derived using an atmospheric radiative transfer model. In the Gulf of Lion of the Mediterranean Sea, northwest winds prevail in summer and autumn, which favors upwelling events. This study aims to improve reconstructed HY-1D/COCTS SST for characterizing strong upwelling events in the Gulf of Lion. The study covers the period from May to November 2021(summer and autumn). The research area is 41&deg;N&ndash;44&deg;N and 3&deg;E&ndash;8&deg;E and the spatial resolution of COCTS SST is 1 km. Owing to persistent cloud cover, 61.92% of all pixels are missing. First, to better utilize COCTS SST, we apply Data Interpolating Empirical Orthogonal Functions (DINEOF) to reconstruct COCTS SST. The validation results for reconstructed COCTS SST show that DINEOF provides accurate statistical results on cloud pixels. We analyze the performance of the reconstructed COCTS SST in 8 sporadic upwelling events using the <em>in situ</em> data as reference. The hourly <em>in situ</em> data from 3 sites located in/nearby distinct upwelling areas from the Gulf of Lion (Marseille-Toulon area). The results show that the reconstructed COCTS SST characterizes most SST cooling events caused by upwelling, but not as intense as the <em>in situ</em> SST. Second, to overcome this limitation, we propose a wind-informed cloud detection procedure that takes into account wind speed and direction in order to improve the classification of upwelling-influenced pixels. The COCTS SST obtained by this improved cloud mask is subsequently reconstructed using DINEOF.&nbsp; The improved reconstructed COCTS SST has higher consistency with the <em>in situ</em> SST in the upwelling area. The results show the difficulty of cloud masking in areas with strong upwelling events and that the improved reconstructed HY-1D/COCTS SST, enabled by wind-informed cloud detection, have the potential to accurately describe such events.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5436</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5436/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146180</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Interannual variations and future changes in the soil uptake of hydrogen]]></dc:title>
      <dc:creator>Wang, Ye</dc:creator>
      <dc:creator>Wild, Oliver</dc:creator>
      <dc:creator>Hou, Xuewei</dc:creator>
      <dc:creator>Hossaini, Ryan</dc:creator>
      <dc:description><![CDATA[Hydrogen (H<sub>2</sub>) is under consideration as a green energy source for future low-carbon development pathways. However, assessment of the future climate impacts of large-scale H<sub>2</sub> use is currently limited by poor understanding of the dominant atmospheric removal process, the uptake of H<sub>2</sub> by microbial activity in soil. Here we implement a soil dry deposition scheme for H<sub>2</sub> in a global chemistry transport model and conduct a sensitivity analysis to quantify how uncertainties in soil parameters contribute to uncertainty in H<sub>2</sub> uptake. We find that soil moisture dominates the uncertainty (52 %), along with contributions from soil porosity (34 %) and the water threshold for biological activity (13 %). However, the sensitivity of uptake to soil moisture is strongly nonlinear, with increases in uptake with declining soil moisture where it is under biotic control and with increasing soil moisture where it is under diffusivity control. We show that soil uptake dominates the interannual variation in atmospheric H<sub>2</sub> abundance from 2010 to 2022, and the notable decrease in 2015, while enhanced atmospheric production drives the observed long-term increase. Our results suggest that both soil sink and source of H<sub>2 </sub>are affected by strong ENSO events driven by changes in soil moisture. Using output from 11 CMIP6 models, we project changes in H<sub>2</sub> soil uptake between 2015 and 2100 of &minus;2.5 % to +7.9 % under SSP1-2.6 and +4.1 % to +20.4 % under SSP5-8.5, suggesting an increase in soil uptake under climate change associated with future changes in soil moisture.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5371</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5371/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146434</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Cheap and accurate higher-order ice flow emulator for mountain glaciers]]></dc:title>
      <dc:creator>Rosier, Sebastian H. R.</dc:creator>
      <dc:creator>Gregov, Thomas</dc:creator>
      <dc:creator>Jouvet, Guillaume</dc:creator>
      <dc:creator>Vieli, Andreas</dc:creator>
      <dc:description><![CDATA[Numerical projections of mountain-glacier evolution increasingly rely on large ensembles that sample uncertain climate forcing, geometry, and ice-flow parameters, yet explicitly resolving higher-order ice dynamics within such ensembles remains computationally expensive. Here we take an alternative approach by training a neural network once, offline, to reproduce the velocity field of a higher-order ice-flow model, and then use the trained network in place of the ice-flow solver during transient simulations. In doing so, we retain the higher-order model's physical basis while avoiding the repeated cost of its velocity solve. The network predicts depth-dependent horizontal ice-flow velocities for land-terminating mountain glaciers directly from gridded glacier geometry and physical parameters, and its weights are then held fixed, so that no retraining is required when it is applied to a new glacier. Leveraging the computational efficiency of GPU operations together with the instructed glacier model (IGM), we generate a large synthetic training set of transient glacier states across diverse mountain topography and climate histories, and at fixed intervals we compute reference velocities from the Blatter-Pattyn ice-flow formulation. The resulting dataset contains over 300,000 higher-order velocity solutions, orders of magnitude more than the catalogues used to train earlier ice-flow emulators. We train on the misfit between the network outputs and target velocities, together with a physics term based on the same discretised ice-flow energy. Our preferred architecture, trained with this hybrid objective, accurately reproduces velocity on examples unseen during training, with a median surface-speed error of 0.71 m yr<sup>-1</sup> and a median flux-divergence error of 0.10 m yr<sup>-1</sup>. In transient simulations of two real glacier systems that lie outside the training set, the emulator tracks reference simulation ice volume through a 500-year advance-retreat cycle with maximum errors below 6%. Crucially, we find that errors do not accumulate over time. Instead, velocity biases induce geometric changes that tend to counteract them, stabilising the coupled emulator&ndash;mass-conservation system. Taken together, our results show that the expensive part of higher-order ice flow can be paid for once during training and reused indefinitely: velocity is predicted in a single forward pass rather than solved for iteratively at every time step. Higher-order ice dynamics are therefore no longer the limiting cost in mountain-glacier modelling, and become practical in large regional and global projection ensembles.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5523</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5523/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146495</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Temperature and Rainfall Effects on Rock Slope Dynamics: Evidence from Multi‑Site Monitoring in Czechia, Central Europe]]></dc:title>
      <dc:creator>Racek, Ondřej</dc:creator>
      <dc:creator>Loche, Marco</dc:creator>
      <dc:creator>Hartvich, Filip</dc:creator>
      <dc:creator>Blahůt, Jan</dc:creator>
      <dc:description><![CDATA[Rock slopes are dynamic geomorphic systems whose stability is influenced by an interplay between geological structures and environmental forcing. Among these, meteorological variables, particularly temperature and precipitation, are recognised as key drivers of both long-term slope evolution and short to medium-term joint deformation expressed through diurnal and annual displacement cycles. However, their influence on block scale displacement remains poorly explored.</p> <p>This study investigates meteorologically driven rock slope surficial dynamics using high-resolution crack meter measurements of blocks ranging in volume from 0.3 to 150 m<sup>3</sup> and environmental monitoring data collected from four instrumented sites in Czechia, Central Europe. Each site comprises unique geological and morphological conditions and is equipped with joint displacement sensors, a weather station, and an in-depth thermal probe. A total of twelve representative rock blocks were monitored across the sites, capturing both thermally driven and potentially gravitationally induced displacements.</p> <p>We analysed multi-year time series data (&ge;2 years) to assess the relationships between joint movements and meteorological variables, including air temperature, in-depth rock temperature up to 3 m and rainfall. Statistical observations revealed distinct seasonal and diurnal cycles in joint dilation linked to thermal forcing. Moreover, several blocks exhibited signs of compound kinematics, with joint displacements influenced by thermal cycles, rainfall and irreversible gravitational destabilisation trends.</p> <p>This study provides new insights into the temporal dynamics of rock slope instability in temperate climates. The observed thermal sensitivity highlights the importance of temperature variations in driving short-term reversible joint deformation and potentially contributing to progressive rock-slope destabilization. This study demonstrates the value of long-term, high-frequency monitoring for quantifying weather&ndash;rock mass interactions and supports the integration of kinematical interpretations into future monitoring system designs.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5565</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5565/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146577</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Using 1 second LEO clock corrections for the Fengyun-3E radio occultation retrievals]]></dc:title>
      <dc:creator>Zhang, Xinyu</dc:creator>
      <dc:creator>Ding, Wenwu</dc:creator>
      <dc:creator>Meng, Xiangguang</dc:creator>
      <dc:creator>Li, Ying</dc:creator>
      <dc:creator>Liu, Yan</dc:creator>
      <dc:creator>Yuan, Yunbin</dc:creator>
      <dc:description><![CDATA[<span>Clock offset constitutes a major error source for Global Navigation Satellite System (GNSS) radio occultation (RO) products, particularly for stratospheric observations. The adoption of high-rate clock correction strategy can effectively mitigate clock offset induced err</span>o<span>rs. In this study, high-rate (1-s) undifferenc</span>ed<span> (UD) Low Earth Orbit (LEO) clock corrections are used to retrieve RO observations from the Fengyun</span>-<span>3E (FY-</span>3E<span>) satellite. The retrieval results are compared with those derived from the conventional 30</span>-<span>s clock correction scheme and the single-difference (SD) scheme currently adopted in the official data processing. The results demonstrate that the 1-s LEO clock correction scheme improves the overall quality of FY-</span>3E<span> RO retrievals. For bending angle, the most prominent improvements are found in the altitude range of 40-60 km. Globally, its systematic difference is roughly 3% smaller than that of the 30-s scheme and 1% smaller than the SD scheme. Such superiority further propagates downward to refractivity and dry temperature. For refractivity, </span>the <span>largest improvements are also found in the altitude range of 40-60 km with systematic differences for the 1-s UD scheme reduced by approximately 0.5% relative to the other two schemes. Standard deviations of the 1-s scheme remain consistently smaller across the complete height range. Standard deviations of dry temperature are also improved with standard deviations about 0.5% smaller than SD and 1% to 2% smaller than the 30-s scheme in the altitude range from 0-40 km. The results in this study demonstrate the capability of using 1-s clock correction scheme for further promoting Fengyun GNSS Occultation Sounder</span>-II (<span>GNOS-II</span>)<span> RO observations. The results here can provide support for future operational processing and archive reprocessing of all Fengyun GNSS occultation datasets.</span>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5629</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5629/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146539</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[A mid-cost automated floating chamber system for high-frequency CO2 and CH4 flux measurements: design, calibration, and comparison with infrequent measurement strategies]]></dc:title>
      <dc:creator>Aben, Ralf C. H.</dc:creator>
      <dc:creator>Knaap, Judith</dc:creator>
      <dc:creator>Hahn, Floris</dc:creator>
      <dc:creator>Wulterkens, Gerben</dc:creator>
      <dc:creator>Szalas-Motesiczky, Dániel</dc:creator>
      <dc:creator>Vissers, Emiel</dc:creator>
      <dc:creator>Engels, Arno</dc:creator>
      <dc:creator>Kleine, Arjan</dc:creator>
      <dc:creator>Fritz, Christian</dc:creator>
      <dc:creator>Kosten, Sarian</dc:creator>
      <dc:description><![CDATA[Small inland waters are important greenhouse gas (GHG) sources; however, most field campaigns rely on daytime-only measurements collected at multi-week intervals, potentially biasing flux estimates. We present the Buoyant Emission Recorder for Temporal High-Frequency Analyses (BERTHA), a mid-cost automated floating chamber system for high-frequency measurements of CO<sub>2</sub> and CH<sub>4</sub> fluxes on multiple spatial scales. We describe the system&rsquo;s design and test how empirically derived pressure and water vapour correction factors for the mid-cost CO<sub>2</sub> and CH<sub>4</sub> sensors increase the accuracy of reported concentrations and derived flux estimates. Here, we found a 17&ndash;37 % (CO<sub>2</sub>) and 4&ndash;9 % (CH<sub>4</sub>) higher mean flux estimate with pressure compensation during the 97-day measuring period. Compensation for water vapour resulted in much smaller differences (~1&ndash;2 % increase). Additionally, we calculated the mean CO<sub>2</sub> and CH<sub>4</sub> emission using high-frequency measurements during 97 days and simulated alternative measurement scenarios based on the full dataset and evaluated how well these &lsquo;reference means&rsquo; could be approached by 1) single, daytime-only chamber flux measurements at daily to monthly intervals, and 2) short-term (2&ndash;3 days) automated chamber deployments every two&ndash;three weeks combined with machine learning-based gap-filling. Results of the simulation analysis showed that daytime-only measurements consistently and strongly underestimated the reference CO<sub>2</sub> mean. CH<sub>4</sub> emissions matched the reference mean well for daily, but not for monthly measurements (&gt;90 % and ~23 % of simulations deviated &lt;20 % of the reference mean, respectively). Short-term automated chamber campaigns, gap-filled using machine learning closely reproduced the CO<sub>2</sub> reference mean, with 89 % and 48 % of means being within &plusmn;20 % of the reference mean, for campaign intervals of two and three weeks, respectively. We conclude that high-frequency chamber measurements using mid-cost GHG analysers combined with empirical pressure corrections provide accurate emission estimates, a robust benchmark for evaluating reduced measurements strategies and gap-filling approaches, and potential for improved process-based understanding of GHG fluxes when combined with ancillary high-frequency measurements.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5600</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5600/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145533</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Using soil-compaction rates by the European Ground Motion Service (PS-InSAR) to estimate, at high spatial resolution, the site conditions of the Grenoble basin (French Alps) for its response to earthquakes]]></dc:title>
      <dc:creator>Schindelholz, Valentin</dc:creator>
      <dc:creator>Cheaib, Aya</dc:creator>
      <dc:creator>Maufroy, Emeline</dc:creator>
      <dc:creator>Cornou, Cécile</dc:creator>
      <dc:creator>Pathier, Erwan</dc:creator>
      <dc:description><![CDATA[In the basin of Grenoble (France), we explore the potential of the compaction rates of Quaternary sediments as measured by PS-InSAR, and freely delivered by the Copernicus service EGMS, to serve as a new proxy for mapping site-condition parameters used in seismic-hazard assessment (fundamental resonance period T<sub>0</sub> of the soil and sediment thickness H<sub>bed </sub>). The Grenoble basin is known for its strong site effect that largely amplifies seismic waves emitted by earthquakes. We develop a specific processing protocol of the EGMS data to account for its high inherent noise (involving adequate spatial smoothing, and quality filtering of the measurements considered), and propose a statistical referencing so the developed models are fully independent of the EGMS dataset chosen as input. The models are applicable in Grenoble in high spatial resolution and result in over 100 000 new estimation points of the site conditions in the entire basin area. This work highlights the huge potential of satellite imagery to complement site-characterisation and microzonation studies specifically in urbanized valleys.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5011</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5011/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143060</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Linear tomographic retrieval characterisation and performance estimation for the ESA Earth Explorer 11 candidate CAIRT (Changing Atmosphere Infra-Red Tomography explorer)]]></dc:title>
      <dc:creator>Funke, Bernd</dc:creator>
      <dc:creator>Höpfner, Michael</dc:creator>
      <dc:creator>Bender, Stefan</dc:creator>
      <dc:creator>Errera, Quentin</dc:creator>
      <dc:creator>Grabowski, Udo</dc:creator>
      <dc:creator>Hoffmann, Alex</dc:creator>
      <dc:creator>Liu, Han-Li</dc:creator>
      <dc:creator>Pedatella, Nick M.</dc:creator>
      <dc:creator>Raspollini, Piera</dc:creator>
      <dc:creator>Ungermann, Jörn</dc:creator>
      <dc:creator>Sinnhuber, Björn-Martin</dc:creator>
      <dc:description><![CDATA[The Changing-Atmosphere Infra-Red Tomography Explorer (CAIRT) was proposed as a candidate for the European Space Agency&rsquo;s eleventh Earth Explorer mission to address critical knowledge gaps in middle atmosphere dynamics and composition. Utilizing an innovative Imaging Fourier Transform Spectrometer (IFTS) in a limb-sounding geometry, CAIRT is designed to provide high-resolution, three-dimensional (3D) tomographic observations of the atmosphere from the free troposphere (5 km) to the lower thermosphere (115 km). To support the scientific evaluation and requirement consolidation of the mission, this paper introduces two computationally efficient performance modeling tools: the Linear Performance Estimator (LPE) and the Fast L2 Simulator (FL2S).</p> <p>The Linear Performance Estimator (LPE) serves as a diagnostic tool that applies linear retrieval theory to quantify spatial resolution and retrieval uncertainties for atmospheric targets like temperature and trace gas concentrations. It features a novel extension to 2D tomographic retrievals, enabling the assessment of how instrument characteristics and uncertainties propagate into final Level-2 (L2) geophysical data products. The Fast Level-2 Simulator (FL2S) complements this by utilizing LPE-derived metrics to project high-resolution atmospheric model data fields onto a simulated CAIRT measurement grid, generating synthetic L2 data products that mimic the full retrieval chain. This allows for a streamlined assessment of how CAIRT&rsquo;s spatial resolution and uncertainties affect specific scientific use cases.</p> <p>Applying these tools to the CAIRT instrument characteristics, we demonstrate the mission&rsquo;s capability to meet specified L2 and science performance requirements. The results confirm that the modular end-to-end simulation framework effectively translates instrument specifications into robust scientific performance metrics, providing a mature basis for possible future implementations of limb-imaging space missions.&nbsp;]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3881</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3881/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144487</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Towards the European Tephra Hazard Map: Methodology and Catalogue of Footprints]]></dc:title>
      <dc:creator>Folch, Arnau</dc:creator>
      <dc:creator>Sandri, Laura</dc:creator>
      <dc:creator>Barsotti, Sara</dc:creator>
      <dc:creator>Aguiar, Simone</dc:creator>
      <dc:creator>Martínez Montesinos, Beatriz</dc:creator>
      <dc:creator>Guerrero, Alejandra</dc:creator>
      <dc:creator>Tierz, Pablo</dc:creator>
      <dc:creator>Pascual, Heribert</dc:creator>
      <dc:creator>Hernandez, Eva</dc:creator>
      <dc:creator>Mingari, Leonardo</dc:creator>
      <dc:creator>Costa, Antonio</dc:creator>
      <dc:description><![CDATA[Many parts of Europe are exposed to tephra hazards that jeopardise regions around volcanoes and the continental airspace. Quantifying and mapping the impacts from future eruptions is relevant to aviation stakeholders and to national and regional civil protection administrations and agencies. This paper presents a novel methodology for long- and short-term Probabilistic Volcano Hazard Assessment (PVHA) from tephra based on a large catalogue of footprints and associated metadata, each footprint representing a single-scenario model realisation. The methodology is used to generate a first version of the European Tephra Hazard Map (ETHM), a collaborative initiative aiming at providing single- and multi-volcano mappings consistent and homogeneous across spatiotemporal scales and volcanoes. More than 53,000 footprints from 12 European volcanoes were computed by running the FALL3D atmospheric dispersal model on the accelerated partition of the MareNostrum-5 supercomputer. In regional model nests (2 km model grid resolution), footprints identify areas prone to hazardous tephra fallout. At European scale (10 km model grid resolution), footprints delineate hazardous airspace regions in terms of ash concentration at critical flight-level layers. The catalogue of footprints is stored in a Simulation Data Lake (SDL@CINECA) to ensure accessibility and re-usability, as well as to ease the addition of footprints from other volcanoes in the future. In parallel, a lightweight service facilitates downstream hazard mapping and dynamic update of hazard based on user-given Probability Density Functions (PDFs), decoupling the computational workload of simulating the physical process from the actual hazard quantification.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4485</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4485/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142494</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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      <dc:title><![CDATA[Development and evaluation of the GRIMs&ndash;NEMO fully coupled model v1.0 for simulating the East Asian Summer Monsoon]]></dc:title>
      <dc:creator>Yoo, Soojin</dc:creator>
      <dc:creator>Chang, Eun-Chul</dc:creator>
      <dc:creator>Lee, Johan</dc:creator>
      <dc:description><![CDATA[This study introduces the newly developed GRIMs&ndash;NEMO fully coupled model version 1.0 for the first time and assesses its capability to simulate the boreal summer climate, with a particular focus on the East Asian summer monsoon (EASM). The model couples the GRIMs atmospheric model, NEMO ocean, and SI3 sea ice models through OASIS3-MCT, providing a computationally efficient framework for climate simulation. Benchmark experiments show that GRIMs&ndash;NEMO requires substantially fewer computational resources than does CESM2, suggesting its potential utility for long-term integrations and ensemble-based studies. The model reasonably reproduces the large-scale features of precipitation, atmospheric circulation, and temperature, and its precipitation skill is broadly comparable to those of CMIP5 and CMIP6 models. Nevertheless, several systematic biases are identified during boreal summer, including excessive rainfall over the equatorial western Pacific, cold surface temperature biases, weakened Tibetan Plateau heating, and circulation errors over the western North Pacific. The model also captures key modes of climate variability associated with the EASM, including the El Ni&ntilde;o&ndash;Southern Oscillation, the Pacific&ndash;Japan pattern, and the boreal summer intraseasonal oscillation, despite remaining biases in their spatial structure, amplitude, and periodicity. A comparison between the coupled and atmosphere-only simulations indicates that air&ndash;sea coupling improves sea surface temperature&ndash;precipitation feedbacks and the seasonal evolution of the EASM rainband. Overall, GRIMs&ndash;NEMO shows reasonable capability as a computationally efficient, fully coupled climate model, while the identified biases highlight the need for further improvements in atmospheric physical parameterizations and the ocean model component.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3472</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3472/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:ard146363</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>ard</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 metrological calibration facility for particle number counters used in emission measurements]]></dc:title>
      <dc:creator>Waheed, Anza</dc:creator>
      <dc:creator>Saturno, Jorge</dc:creator>
      <dc:creator>Malik, Arpit</dc:creator>
      <dc:creator>Rosahl, Johannes</dc:creator>
      <dc:creator>Pratzler, Sonja</dc:creator>
      <dc:creator>Nowak, Andreas</dc:creator>
      <dc:description><![CDATA[A metrological calibration facility for particle number counters (PNCs) has been developed at the Physikalisch-Technische Bundesanstalt (PTB) as a primary reference standard for this metric required in the quantification of solid soot emission as described in national and European regulatory frameworks. This study describes the calibration of a Condensation Particle Counter (CPC) using PTB&rsquo;s primary aerosol number standard, a Faraday Cup Aerosol Electrometer (FCAE). The calibration facility enables high accuracy determination of CPC counting efficiency for particles with mobility diameters between 17 and 200 nm, as well as linearity measurements of particle number concentrations ranging from 1 cm⁻&sup3; to 20 000 cm⁻&sup3;. Soot aerosol particles were generated using a miniCAST 5303 and subsequently treating them in a Catalytic Stripper to remove volatile components before homogenisation in an integrated mixing unit. The aerosol flow was distributed via a ten-port manifold, allowing simultaneous evaluation of up to eight CPCs and a FCAE connected to two different ports simultaneously. The results demonstrate that the facility provides state-of-the-art metrological capabilities for CPC calibration, supporting improved reliability and comparability of particle number measurements in emission control applications.]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/ar-2026-33</dc:identifier>
      <dc:identifier><![CDATA[https://ar.copernicus.org/preprints/ar-2026-33/]]></dc:identifier>
      <dc:source>eISSN: 2940-3391</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:cp134506</identifier>
    <datestamp>2026-09-25</datestamp>
    <setSpec>cp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Middle to late Holocene cooling and increased zonal asymmetry in the mid-latitude North Atlantic]]></dc:title>
      <dc:creator>Si, Weimin</dc:creator>
      <dc:creator>Herbert, Timothy</dc:creator>
      <dc:creator>Toggweiler, John R.</dc:creator>
      <dc:description><![CDATA[<p>Sea Surface Temperature reconstructions derived from alkenone biomarker (SST-alk) reveal a cooling trend in the North Atlantic during the late Holocene (the last 5000 years), contrary to the warming simulated by transient climate models driven by 20 ppm increase in greenhouse gas concentrations. In this study, we present new SST-alk time series from the inter-gyre region of the North Atlantic. Our results, together with existing data, indicate that late Holocene cooling is marked by an increasing zonal SST gradient across the mid-latitude North Atlantic, with more pronounced cooling in the west than in the east. Complementary planktonic foraminifera assemblage data, interpreted alongside other circulation proxies, suggest that a late Holocene reorganization of inter-gyre ocean circulation as a likely driver of this zonal asymmetry. Finally, we compare these proxy-based reconstructions with transient climate model simulations (TraCE-21k), and find that models do not reproduce the observed zonally asymmetric cooling and the inferred circulation changes. This misrepresentation of spatial and temporal variability likely explains the data-model discrepancy in the mid-latitude North Atlantic.</p>]]></dc:description>
      <dc:date>2026-09-25</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/cp-22-1729-2026</dc:identifier>
      <dc:identifier><![CDATA[https://cp.copernicus.org/articles/22/1729/2026/]]></dc:identifier>
      <dc:source>eISSN: 1814-9332</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg140502</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Exploratory characterization of bacterial communities and predicted functional profiles in six water samples from four Colombian Andean lakes using 16S rRNA gene amplicon sequencing]]></dc:title>
      <dc:creator>Gómez-Palacio, Andrés</dc:creator>
      <dc:creator>Marín-Suarez, Johana</dc:creator>
      <dc:creator>Pedroza-Ramos, Adriana</dc:creator>
      <dc:creator>Aranguren-Riaño, Nelson</dc:creator>
      <dc:description><![CDATA[<p>Northern Andean highland lakes support agriculture, water provision, and local livelihoods, but their bacterial communities remain insufficiently characterized. We conducted an exploratory survey of bacterial community composition and predicted functional potential in six water samples from four freshwater lakes in the Eastern Cordillera of Colombia: Fúquene, Tota, Calderona, and Colorado. Five samples collected in 2019 comprised the primary dataset, while a previously published Tota sample collected in December 2018 was reprocessed as a historical reference. Bacterial communities were characterized using 16S rRNA gene amplicon sequencing, and functional profiles were inferred using PICRUSt2. After sequence processing and taxonomic filtering, 3153 amplicon sequence variants were retained. Actinobacteria, Proteobacteria, Bacteroidetes, Cyanobacteria, and Verrucomicrobia were the predominant bacterial phyla. Coverage-standardized richness and diversity varied descriptively among samples, with Colorado showing the lowest estimated ASV richness. Taxonomic composition and Bray–Curtis dissimilarities also varied among samples, reflecting differences in dominant bacterial groups. <i>Mycobacterium</i>-assigned ASVs were detected in Fúquene and Tota, <i>Leptospira</i>-assigned ASVs occurred in these same lakes at relative abundances of 0.01 %–0.36 %, and <i>Legionella</i>-assigned ASVs occurred in all six samples at 0.11 %–4.60 %. These genus-level assignments do not establish pathogenic species, viability, transmission, or risks to aquatic animals or humans. PICRUSt2 predicted variation in functional profiles, including pathways associated with naphthalene degradation, bacterial chemotaxis, biofilm formation, bacterial secretion systems, and pyrimidine and folate metabolism. Bray–Curtis ordination of predicted pathway profiles showed sample-level separation, and weighted NSTI values ranged from 0.160 to 0.181. These predictions represent inferred genomic potential rather than direct evidence of gene presence, expression, or metabolic activity. Because sampling was limited and unbalanced and lacked concurrent environmental measurements, the observed patterns cannot be attributed to specific environmental drivers. This study provides an initial descriptive baseline for bacterial communities in four Colombian Andean lakes and identifies patterns for evaluation through replicated sampling, physicochemical measurements, metagenomics, and targeted validation.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-6725-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/6725/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg140085</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[High nitrous oxide isotopic variability during denitrification by Pseudomonas species bearing NirK and NirS]]></dc:title>
      <dc:creator>Chénier, Noémy</dc:creator>
      <dc:creator>Magyar, Paul M.</dc:creator>
      <dc:creator>Zopfi, Jakob</dc:creator>
      <dc:creator>Frey, Claudia</dc:creator>
      <dc:creator>Kuhn, Thomas</dc:creator>
      <dc:creator>Lehmann, Moritz F.</dc:creator>
      <dc:creator>Mohn, Joachim</dc:creator>
      <dc:description><![CDATA[<p>Nitrous oxide (N<span class="inline-formula"><sub>2</sub></span>O) isotopocules provide key insights into microbial nitrogen cycling, but their interpretation requires well-constrained values for both oxygen isotope signatures (<span class="inline-formula"><i>δ</i><sup>18</sup></span>O–N<span class="inline-formula"><sub>2</sub></span>O) and intramolecular <span class="inline-formula"><sup>15</sup></span>N site preference (SP) associated with N<span class="inline-formula"><sub>2</sub></span>O production pathways. Site preference is widely used to distinguish N<span class="inline-formula"><sub>2</sub></span>O formation pathways because bacterial denitrification is generally assumed to yield SP values near 0 ‰ through canonical NorB-mediated NO reduction. However, the extent to which SP remains stable across physiological states and changing NO reduction pathways remains poorly constrained. Likewise, interpretation of <span class="inline-formula"><i>δ</i><sup>18</sup></span>O–N<span class="inline-formula"><sub>2</sub></span>O associated with denitrification requires understanding the relative contributions of branching kinetic isotope effects and oxygen atom exchange between nitrite and water during N<span class="inline-formula"><sub>2</sub></span>O formation.</p>        <p>Here, we investigated N<span class="inline-formula"><sub>2</sub></span>O isotopic signatures during denitrification by <i>Pseudomonas aureofaciens</i> (NirK-bearing) and <i>Pseudomonas chlororaphis</i> (NirS-bearing) under active-growth and resuspension conditions using quantum cascade laser absorption spectroscopy (QCLAS) and isotope ratio mass spectrometry (IRMS). SP tracked canonical NorB-mediated NO reduction but transiently increased above <span class="inline-formula">+</span>10 ‰ during early N<span class="inline-formula"><sub>2</sub></span>O production, suggesting temporary activity of alternative NO reductases. These dynamics were only resolved through continuous QCLAS measurements, highlighting the importance of time-resolved isotopic observations. While SP remains a useful indicator of NO reduction mechanisms, these results show that even within denitrification, shifts between NO reduction pathways may lead to variable SP signatures.</p>        <p>In parallel, we quantified oxygen atom exchange between nitrite and water using incubations prepared in natural-abundance and <span class="inline-formula"><sup>18</sup></span>O-enriched water. Contrary to expectations from denitrifier-method studies, <i>P. aureofaciens</i> exhibited substantial and highly variable oxygen-atom exchange (38 %–100 %), far exceeding previously reported values (<span class="inline-formula">&lt;9</span> %). In contrast, <i>P. chlororaphis</i> showed consistently high but less variable exchange (<span class="inline-formula">∼</span> 66 %). Resuspension experiments reproduced the characteristic low- and high-exchange behavior reported for these strains under denitrifier-method conditions, demonstrating that these exchange values are specific to the methodological framework and not representative of actively growing systems. These results show that oxygen atom exchange is not governed solely by nitrite reductase identity (NirS vs. NirK) but is strongly modulated by physiological state and metabolic context, including active growth versus stationary-phase resuspension and differences in nitrite turnover. As a result, <span class="inline-formula"><i>δ</i><sup>18</sup></span>O–N<span class="inline-formula"><sub>2</sub></span>O cannot be interpreted as a fixed tracer of denitrification pathways outside the constrained conditions of the denitrifier method.</p>        <p>Together, these findings suggest that denitrifying bacteria may generate N<span class="inline-formula"><sub>2</sub></span>O with a broader range of <span class="inline-formula"><i>δ</i><sup>18</sup></span>O–N<span class="inline-formula"><sub>2</sub></span>O and SP than previously assumed. This calls for a reassessment of N<span class="inline-formula"><sub>2</sub></span>O isotopocule interpretations and emphasizes the need to integrate isotopic measurements with physiological and biochemical constraints.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-6705-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/6705/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg139325</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Balancing nitrogen use efficiency, losses and soil nitrogen depletion to evaluate national scale agri-environmental performance over 40 years]]></dc:title>
      <dc:creator>Jiang, Jize</dc:creator>
      <dc:creator>Winkel, Lenny H. E.</dc:creator>
      <dc:creator>Wüst-Galley, Chloé</dc:creator>
      <dc:creator>Bretscher, Daniel</dc:creator>
      <dc:creator>Necpalova, Magdalena</dc:creator>
      <dc:creator>Stenke, Andrea</dc:creator>
      <dc:creator>Six, Johan</dc:creator>
      <dc:description><![CDATA[<p>Nitrogen (<span class="inline-formula">N</span>) is essential for agricultural productivity, but excessive <span class="inline-formula">N</span> inputs result in substantial losses to the environment. Conducting <span class="inline-formula">N</span> assessments at national scales is challenging because observational data are limited, especially over long time periods. Here we compiled detailed datasets and performed high-resolution biogeochemical modelling to quantify <span class="inline-formula">N</span> budgets for Switzerland's diverse agricultural ecosystems over four decades, with a focus on croplands and grasslands (i.e., permanent managed meadows used for livestock feed). Between the 1980s and the 2010s, <span class="inline-formula">N</span> use efficiency improved from 47 % to 57 % in croplands and from 63 % to 71 % in grasslands, while losses through leaching and gas emissions decreased by 24 % in croplands and 4 % in grasslands. These improvements are closely linked to the implementation of national-scale agri-environmental policies that reduced fertilizer use in the 1990s. However, despite increased efficiency, cropland soils experienced substantial <span class="inline-formula">N</span> depletion between 1995 and 2011 (<span class="inline-formula">−</span>23 <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow class="unit"><mi mathvariant="normal">kg</mi><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">N</mi><mspace width="0.125em" linebreak="nobreak"/><msup><mi mathvariant="normal">ha</mi><mrow><mo>-</mo><mn mathvariant="normal">1</mn></mrow></msup><mspace linebreak="nobreak" width="0.125em"/><msup><mi mathvariant="normal">yr</mi><mrow><mo>-</mo><mn mathvariant="normal">1</mn></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="68pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="4f73d42bc195e438a22fca77702564c9"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="bg-23-6741-2026-ie00001.svg" width="68pt" height="15pt" src="bg-23-6741-2026-ie00001.png"/></svg:svg></span></span>) in croplands. Our results demonstrate that policy reforms have improved agricultural system functioning and reduced losses, but also reveal risks associated with unbalanced soil <span class="inline-formula">N</span>, underscoring the need for integrated <span class="inline-formula">N</span> management for sustainable agriculture.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-6741-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/6741/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144747</identifier>
    <datestamp>2026-09-24</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[Design and Evaluation of a Low-Cost Horizontal Tube Radiation Shield for Temperature and Humidity Measurements in a Tropical Urban Environment]]></dc:title>
      <dc:creator>Junnaedhi, I Dewa G. A.</dc:creator>
      <dc:creator>Arkan, Muhammad</dc:creator>
      <dc:creator>Muzasyaroh, An Nur A.</dc:creator>
      <dc:creator>Nugraha, Dwina</dc:creator>
      <dc:creator>Fitriani, Rachmy</dc:creator>
      <dc:creator>Abdillah, Muhammad R.</dc:creator>
      <dc:creator>Suwarman, Rusmawan</dc:creator>
      <dc:creator>Sukendra, Sukendra</dc:creator>
      <dc:creator>Varquez, Alvin C. G.</dc:creator>
      <dc:creator>Inagaki, Atsushi</dc:creator>
      <dc:creator>Kanda, Manabu</dc:creator>
      <dc:description><![CDATA[<span>Climate change and rapid urbanization have increased the need for dense air temperature and humidity monitoring networks in tropical cities. Although low-cost sensors are widely available, the cost of radiation shields remains a major barrier to large-scale deployment. This study presents a low-cost horizontal tube radiation shield (H-Tube) constructed from commercially available pipes and fittings combined with a small number of 3D-printed components. Two versions were developed: a bright-annealed stainless-steel shield (H-Tube<sub>SS</sub>) and a PVC shield covered with aluminum foil (H-Tube<sub>PVC</sub>). Material costs were approximately USD 25 and USD 11, respectively, making them about 8 and 18 times less expensive than typical commercial radiation shields (&gt;USD 200).</span></p> <p><span>Performance was evaluated through comparative field experiments in a tropical urban environment in Bandung, Indonesia, using identical Vaisala HMP155A temperature-humidity probes. Measurements from the H-Tube were compared against a Cotton Region Shelter (CRS) reference and two commercial radiation shields: a multiplate (MP) shield and a vertical tube (V-Tube) shield. Under non-aspirated conditions, daytime temperature biases exceeded 4 &deg;C and relative humidity biases exceeded 15% during periods of strong net radiation. In contrast, aspirated operation substantially improved performance, with temperature biases generally remaining within &plusmn;1 &deg;C and relative humidity biases within &plusmn;5%, comparable to those of the commercial MP and V-Tube shields. The aspirated H-Tube<sub>SS</sub> achieved a temperature RMSE of 0.49 &deg;C relative to the CRS, comparable to the MP shield (0.53 &deg;C) and slightly lower than the H-Tube<sub>PVC</sub> (0.58 &deg;C).</span></p> <p><span>Simple bias-correction methods based on linear temperature regression and saturation-vapor-pressure adjustment for relative humidity were also developed and evaluated. For the H-Tube designs, temperature RMSE was reduced from 1.35-1.46 &deg;C to approximately 0.56 &deg;C under non-aspirated conditions and from 0.49-0.58 &deg;C to 0.30-0.35 &deg;C under aspirated conditions. Relative humidity RMSE was reduced to approximately 2.6-3.2% after correction. The correction methods also reduced temperature-measurement uncertainty, particularly for the non-aspirated configurations.</span></p> <p><span>These results demonstrate that the aspirated H-Tube provides a practical, scalable, and low-cost alternative to commercial radiation shields for distributed temperature-humidity monitoring networks in tropical urban environments.</span>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4598</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4598/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143342</identifier>
    <datestamp>2026-09-24</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[Gravity disturbance maps and updated gravity anomaly maps in French-Belgian Hainaut from recent gravity acquisitions and legacy data]]></dc:title>
      <dc:creator>Campeol, Quentin</dc:creator>
      <dc:creator>Dupont, Nicolas</dc:creator>
      <dc:creator>Kaufmann, Olivier</dc:creator>
      <dc:description><![CDATA[In Wallonia, the centre of Hainaut (SW Belgium) is considered the main area where deep geothermal resources are proven. In this region bordering France, the productive geothermal resource is located within karstified levels resulting from the dissolution of interbedded massive anhydrites in the Carboniferous limestones. To improve current knowledge of deep geological structures and to better delineate the geothermal targets, new detailed regional gravity anomaly<span> </span>and disturbance maps have been produced. These include maps of the observed gravity, free-air anomaly, refined Bouguer anomaly, gravity disturbance, topography-free gravity disturbance.</p> <p>This has involved the compilation and harmonisation of cross-border legacy and recent gravity data, combined with an homogeneous reprocessing and an interpolation using the equivalent source method. The legacy data come from the Belgian and French databases published by the ROB (Belgium) and BRGM (France) respectively, to which unpublished data from the Battaille 1967 campaign have been added after their retro-processing from Bouguer anomaly data. The new gravity data come from the recent MoreGeo 2019-2022 gravity acquisition campaign. This campaign covers an area of 820 km&sup2; with 3,784 gravity stations distributed along densely sampled lines and displays a RMSE range of 41.9 to 67.5 &micro;gal after absolute gravity referencing. The gravimetric processing works presented in this paper rely on open-source Python libraries. These include an advanced total correction budget evaluation and topographic correction up to 167 km&sup2; in extent. The resulting maps are consistent with previous ones, in particular the strong correlation between the anomaly and the thickness of the Meso-Cenozoic deposits. It also shows new anomalies that may be due to deep-seated structures. It will be used as a basis for modelling the geothermal reservoir, provided that the effect of the Meso-Cenozoic deposits is accounted for.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3978</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3978/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145953</identifier>
    <datestamp>2026-09-24</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[Dome C migration in Antarctica during the last 800,000 years]]></dc:title>
      <dc:creator>Aanderen, Victor</dc:creator>
      <dc:creator>Quiquet, Aurélien</dc:creator>
      <dc:creator>Dumas, Christophe</dc:creator>
      <dc:creator>Michel, Elisabeth</dc:creator>
      <dc:creator>Parrenin, Frederic</dc:creator>
      <dc:creator>Ritz, Catherine</dc:creator>
      <dc:creator>Jiguet-Covex, Kévin</dc:creator>
      <dc:description><![CDATA[<span>The ice core extracted as part of the Beyond EPICA project is expected to provide the longest continuous climate record, reaching back at least 1.2 million years. However, the hypothesis that Dome C has remained stable over several glacial-interglacial cycles, which is a prerequisite for establishing a reliable age-depth relationship, remains unverified. Using the GRISLI2.0 ice sheet model, we perform an ensemble of 5 high-resolution nested simulations at 10 km &times; 10 km resolution to track the evolution of Dome C position over the past 800,000 years. Our results show that Dome C undergoes substantial displacements over time, strongly controlled by grounding line dynamics in the Aurora Subglacial Basin. Using a 1D ice flow model, we further demonstrate that these dome migrations can introduce age errors of several tens of thousands of years in the age-depth relationship, with the largest uncertainties affecting the oldest and deepest ice, precisely where the Beyond EPICA record is most critical.</span>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5288</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5288/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146527</identifier>
    <datestamp>2026-09-24</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[Beyond rainfall thresholds: hydrologic controls on debris-flow initiation in alpine channels]]></dc:title>
      <dc:creator>Hrachowitz, Markus</dc:creator>
      <dc:creator>Kaitna, Roland</dc:creator>
      <dc:description><![CDATA[Debris flows are a severe natural hazard in mountain regions. As a spatially and temporally highly irregular phenomenon, meaningful quantitative description and generalization of the underlying processes in contrasting environments as well as associated robust local prediction of debris flows is hindered by a lack of sufficiently detailed observations. As a consequence, debris flows are frequently predicted based on simple regional precipitation (or rainfall) intensity-duration thresholds that lump many channels over larger spatial domains, irrespective of potentially different underlying debris flow trigger processes due to hydro-climatic or geomorphic differences between the channels. Based on long-term debris flow records of up to 18 years, hydro-climatic observations and modelled hydrological variables across three contrasting active debris flow channels (ID1-ID3) in the Austrian Alps, this study (1) analyses differences between the local debris flow regimes in these channels, based on their strength of temporal coupling with hydro-climatic and hydrological extremes, (2) quantifies differences between regional and local debris flow initiation thresholds that emerge from these differences in their temporal coupling, and (3) identifies the pairs of threshold model variables that allow the most reliable debris flow predictions in each of the three study channels. We have found that the three study channels are characterized by considerable difference in seasonal debris flow timing. In channel ID1, debris flows events are largely confined to early summer, occurring, on average, several weeks before the wettest conditions in each year, thus being only weakly coupled to hydro-meteorological extremes. In the close-by channel ID2, debris flows occur throughout summer, on average a few days after the wettest conditions of any specific year. The high debris flow frequency in this channel in addition suggests multiple cycles of sediment exhaustion and re-supply to the channel over one season. Together, this is evidence for a stronger coupling and a highly dynamic balance between the availabilities of sufficient sediment and in-stream transport capacity, respectively. Due to the geographical proximity of and thus similar hydro-climatic conditions in ID1 and ID2, the differences in debris flow regimes can largely be attributed to differences in landscape characteristics and thus geomorphic predisposition. In contrast, in channel ID3, debris flows are largely confined to late summer and temporally coincide with the wettest annual conditions, suggesting a strongly coupled debris flow regime. The differences between ID3 and the other channels arise from the combined influence of hydro-climatic and geomorphic predisposition. These differences in debris flow regimes are reflected in the differences between the individual local thresholds across the three channels and the systematically superior performance of local thresholds to detect debris flows than regional thresholds across all channels. It was further found that traditional precipitation and rainfall thresholds were consistently outperformed by thresholds that explicitly account for the sum of rainfall and snowmelt. The overall strongest thresholds were found to be the ones based on channel discharge, providing a direct descriptor of in-stream transport capacity. Together the results provide evidence for the benefit of local thresholds and explicitly accounting for hydrological variables in threshold-based debris flow prediction models.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5589</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5589/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146466</identifier>
    <datestamp>2026-09-24</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[Anti-phased steric and mass cycles and an unresolved dynamic trend in Arabian Gulf sea level]]></dc:title>
      <dc:creator>Usman, Muhammad</dc:creator>
      <dc:description><![CDATA[The Arabian Gulf is a shallow, evaporative marginal sea whose sea level has been characterised almost entirely from tide gauges and satellite altimetry; its steric and ocean-mass components have never been separated observationally, because the basin has no continuous hydrographic record. We combine DUACS satellite altimetry with CSR and JPL GRACE/GRACE-FO mascon solutions over April 2002 to December 2025 to close the Gulf sea-level budget at seasonal and multi-year timescales. The seasonal cycle of total sea level (annual amplitude 4.3 &plusmn; 0.3 cm, maximum in November) is shown to be the residual of two larger, nearly anti-phased components: an ocean-mass cycle of 3.9 &plusmn; 0.4 cm with a climatological maximum in January and a steric cycle of 7.0 &plusmn; 0.3 cm with a climatological maximum in October. The inferred steric cycle is confirmed by two further estimates: a fully independent thermal-expansion calculation from ERA5 sea-surface temperature (7.2 cm, August) and the full-column steric height from the GLORYS12 reanalysis (5.3 cm, August; halosteric contribution 0.6 cm). GLORYS12 assimilates altimetry, so it is independent for the seasonal cycle but not for the trend. These bracket the budget value and bound its systematic uncertainty at about 1.5 cm. For the long-term trend we show that regional gravimetry cannot be used directly: leakage from groundwater depletion in the adjacent Arabian Peninsula and Iran imprints &minus;2.2 &plusmn; 0.3 mm yr<sup>&minus;1</sup> on Gulf mascon cells, and the two mascon products diverge by 10&ndash;15 cm after 2021. Using instead the global barystatic rate (2.1 mm yr<sup>&minus;1</sup>) and a steric trend of 0.3&ndash;0.9 mm yr<sup>&minus;1</sup>, 2.1&ndash;3.2 mm yr<sup>&minus;1</sup> of the observed 5.2&ndash;5.6 mm yr<sup>&minus;1</sup> rise &mdash; roughly two-fifths to just over half, depending on the end date (2002&ndash;2021 or 2002&ndash;2025) and the steric route &mdash; is accounted for by neither ocean-mass nor steric change. This implies a Gulf-mean manometric trend of order 4&ndash;5 mm yr<sup>&minus;1</sup> that regional GRACE cannot independently confirm or refute; we weigh a dynamic, remotely forced origin against two alternatives in the Discussion. Gulf sea level rose in the year following each of the four strong positive Indian Ocean Dipole events of the record, consistent with remote forcing through the Strait of Hormuz.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5546</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5546/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145976</identifier>
    <datestamp>2026-09-24</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[Intensification of a European Storm Cluster in a Warmer Climate: Evidence from Regional Storylines]]></dc:title>
      <dc:creator>L. L. de Amorim, Felipe</dc:creator>
      <dc:creator>Feser, Frauke</dc:creator>
      <dc:creator>Weisse, Ralf</dc:creator>
      <dc:description><![CDATA[In February 2022 a series of three extreme winter storms hit the coast of Northern Germany and Northwestern Europe. In this study, cyclones Ylenia, Zeynep and Antonia &nbsp;were attributed to anthropogenic climate change, assessed through event-based storylines across five climate states: pre-industrial, present-time, +2K, +3K and +4K. The storylines vary only in sea surface temperatures and greenhouse gas concentrations, isolating the thermodynamic components of anthropogenic climate change. Global storylines were dynamically downscaled for Europe, focusing on Northwestern Germany and the German Bight. Spectral nudging was used to keep the large-scale weather patterns close to observations. Spectral nudging was turned off in a second step, which allows an assessment of dynamical effects beyond the thermodynamic ones. Anthropogenic warming amplified both wind speeds and precipitation during the February 2022 extra-tropical cyclone cluster, strengthening gradually from present-time to +4K warming and remaining robust across dynamical configurations, indicating systematically intensifying impacts on the analysed domain under continued warming. Changes in precipitation are more evident in northern regions of the analysed domain, with a notable precipitation increase in the Norwegian west coast. The changes in wind speed and precipitation are shown to possibly be related to changes in the storm tracks position, indicating a strong relationship with the large-scale circulation, even though only slightly changes were observed in jet stream position. Without spectral nudging, future storylines exhibit greater ensemble spread and a northward‑tilted storm track. Overall, the study found a gradual increase in areas with robust positive changes of wind speed and precipitation during the storm cluster in warmer climate states, with dynamical changes further amplifying the magnitude of already notable thermodynamic response, but evidencing the role of internal variability between storyline members in decreasing the spatial robustness.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5306</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5306/]]></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:egusphere146459</identifier>
    <datestamp>2026-09-24</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[GHLC: global harmonized land cover datasets for 2020&ndash;2024 at 10 m and 30 m resolution based on a rule-based ensemble approach]]></dc:title>
      <dc:creator>Moreno, Mateo</dc:creator>
      <dc:creator>Parente, Leandro</dc:creator>
      <dc:creator>Hein, Lars</dc:creator>
      <dc:creator>Bonannella, Carmelo</dc:creator>
      <dc:creator>Xu, Qin</dc:creator>
      <dc:creator>Isik, Mustafa Serkan</dc:creator>
      <dc:creator>Wibisana, Maulana Ikram</dc:creator>
      <dc:creator>Piccoli, Michelle</dc:creator>
      <dc:creator>Hengl, Tomislav</dc:creator>
      <dc:description><![CDATA[The paper describes the production and assessment of GHLC: a global harmonized land cover product at 10 meter spatial resolution for 2020 and at 30 meter resolution for 2020-2024. GHLC is generated using a rule-based ensemble approach that integrates 24 individual land cover and auxiliary layers from different projects. Because each class label is assigned based on an explicit, documented rule rather than a trained model, every classification decision in GHLC can be traced to a specific input dataset and threshold, making the product transparent, reproducible, and straightforward to update as improved input datasets become available. These 24 layers are combined around a primary spatial backbone provided by ESA WorldCover and GLAD GLCLUC (Global Land Cover and Land Use Change). The documented sequence of conditional rules describes how other thematic datasets (e.g., Global Mangrove Watch for mangroves, WorldCereal for maize, South American maps for soybeans, and GLC_FCS30D for detailed forest subtypes) are fused with ESA WorldCover and GLAD GLCLUC. The target legend is structured hierarchically to balance thematic detail with global mapping feasibility (Level 1 consists of 10 broad classes; Level 2 consists of 40+ distinct classes, including specific crop types, varying grassland management types, and forest types). The map was validated against a large pool of independent reference samples from the Global Ensemble Land Cover (GELC) database, matched to each product's mapped years. At the broadest level, the GHLC product achieved an overall accuracy of 0.92 for the 10 m and 0.86 for the 30 m maps, respectively. Forests, forest plantations, and woodland (<em>F</em>1 &ge; 0.94) and water bodies (<em>F</em>1 &ge; 0.85) performed best across both resolutions due to their high spectral distinctiveness and spatial coherence. Cropland classification was more accurate in the 30 m product (<em>F</em>1 = 0.81) than in the 10 m product (<em>F</em>1 = 0.72), as the 30~m GLAD GLCLUC backbone provides a stronger cropland signal. Macro-averaged F1 across all classes was effectively identical between 10 m (0.63) and 30 m (0.62), demonstrating that spatial resolution alone does not govern overall accuracy. The poorest performance was registered for sparsely vegetated ecosystems and inland wetlands. Urban ecosystems appear to be overestimated in the 30 m map. The datasets can be used for reporting on ecosystem extent and ecosystem services in ecosystem accounting. The biggest limitations of the GHLC are (1) that it is based on manual rules that may be subject to errors, and (2) that it relies on 24 independently derived external layers, each produced and maintained by separate research groups or agencies. If those external groups cease updating or maintaining their specific datasets, the corresponding GHLC rules cannot be applied, causing the classification system to degrade.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5540</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5540/]]></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:egusphere146409</identifier>
    <datestamp>2026-09-24</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[White Christmas in Germany? A High-Resolution Snow Climatology since 1950 (SNOWRAS v1.0)]]></dc:title>
      <dc:creator>Drüke, Markus</dc:creator>
      <dc:creator>Künzel, Alice</dc:creator>
      <dc:creator>Böhm, Uwe</dc:creator>
      <dc:creator>Castino, Fabiana</dc:creator>
      <dc:creator>Deutschländer, Thomas</dc:creator>
      <dc:creator>Fiedler, Anett</dc:creator>
      <dc:creator>Höschel, Ines</dc:creator>
      <dc:creator>Machui-Schwanitz, Grit</dc:creator>
      <dc:creator>Rauthe, Monika</dc:creator>
      <dc:creator>Schneider, Gerold</dc:creator>
      <dc:creator>Wichura, Bodo</dc:creator>
      <dc:description><![CDATA[Snow cover is highly sensitive to changes in temperature and precipitation, making it an important indicator of climate variability and climate change. It also strongly influences hydrological processes, for example, groundwater recharge, runoff formation, and flood risk during snowmelt. Long-term, spatially detailed information on snow depth and snow cover duration is therefore needed for climate monitoring, hydrological applications, and impact assessments.<br />Here, we present SNOWRAS, a new gridded snow depth dataset for Germany covering extended winter seasons from 1950/51 to 2025/26. The dataset is based on daily snow depth observations from the extensive monitoring network of the Deutscher Wetterdienst (DWD), complemented by measurements from partner networks in Germany and neighboring countries. After quality control and data cleaning, the station observations were interpolated to a regular 1 &times; 1 km grid using an optimal interpolation scheme.<br />Based on this dataset, we derived and analyzed several snow-climatological indicators, including seasonal mean and maximum snow depth, the number of snow days, and the timing of the first and last days with seasonal snow cover. Across Germany, most indicators show a statistically significant decline over the past 75 years. The magnitude of these changes varies considerably with elevation: the largest decreases in snow depth and snow cover duration are found in lowland and mid-elevation regions, while these trends are generally weaker at higher elevations and are partly not statistically significant. SNOWRAS provides a spatially consistent, high-resolution dataset for monitoring snow conditions and investigating long-term changes in Germany&rsquo;s snow climate. Together with complementary information, such as snow water equivalent, the dataset can also support hydrological modeling, assessments of water availability, and analyses of hydrological risks.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5507</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5507/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146289</identifier>
    <datestamp>2026-09-24</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[Recovering nineteenth-century temperature and pressure measurements for Eurasian climate analysis]]></dc:title>
      <dc:creator>Shapiro, Anna V.</dc:creator>
      <dc:creator>Foelsche, Ulrich</dc:creator>
      <dc:description><![CDATA[Historical instrumental observations are a valuable source of quantitative information on past climate variability, especially when printed records can be transformed into machine-readable datasets. This study uses meteorological observations published in the '<em>Annalen des Physikalischen Centralobservatoriums</em>' in Saint Petersburg to assess their potential for Eurasian climate analysis. We digitized monthly temperature and pressure data from printed tables and converted them into a machine-readable dataset, addressing challenges related to station metadata, spatial coverage, multilingual headings, historical station names, decimal notation, missing entries, and optical character recognition errors. Using selected stations, we construct monthly surface air temperature and pressure anomaly maps for 1877 and 1879 relative to station-specific monthly reference means based on the other available years within 1874-1894. The year 1877 falls within the major 1877-1878 global climate anomaly, while 1879 provides a contrasting case. The station-based anomaly maps show coherent spatial structures across large parts of Eurasia. In 1877, late-year positive pressure anomalies over central and eastern Eurasia are accompanied in December by widespread cold anomalies. In 1879, the maps show stronger regional contrasts and a markedly different December pressure pattern. Our results demonstrate that the <em>Annalen</em> observations are valuable not only as historical records, but also as quantitative data for studying nineteenth-century atmospheric variability.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5428</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5428/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146347</identifier>
    <datestamp>2026-09-24</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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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Brief communication: NISAR pixel offsets measure but do not statistically resolve pre-failure motion at the 26 August 2026 Bhote Koshi ice&ndash;rock avalanche, Nepal]]></dc:title>
      <dc:creator>Meena, Sansar Raj</dc:creator>
      <dc:description><![CDATA[We analyse five NASA&ndash;ISRO Synthetic Aperture Radar (NISAR) pixel-offset pairs spanning the 26 August 2026 Bhote Koshi ice&ndash;rock avalanche, Nepal. The last pre-event pair estimates 0.96 m median displacement over 24 days, with its mean vector 18&deg; from the topographic fall line. No pre-event interval exceeds the 95th percentile of spatial comparison distributions for displacement or directional coherence. We report rankings rather than detections. The co-event field lacks directional organisation in both processing chains. Available interval averages do not establish precursory acceleration and cannot isolate motion during the final week before failure.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5462</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5462/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145655</identifier>
    <datestamp>2026-09-24</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[Hydrological Memory Regulates River Basin Recovery from Climate Extremes: Evidence from China&rsquo;s Major River Basins]]></dc:title>
      <dc:creator>Touseef, Muhammad</dc:creator>
      <dc:creator>Chen, Lihua</dc:creator>
      <dc:description><![CDATA[Hydrological memory from climate extremes depends not only on disturbance magnitude but also on the persistence of antecedent basin storage. This study developed a Hydrological Memory Framework (HMF) to quantify basin-scale hydrological memory and assess its influence on resilience across eight major river basins in China during 1981&ndash;2025. Hydrological memory was estimated using the Catchment Forgetting Curve (CFC), while drought and flood recovery were evaluated from standardized hydrological anomalies. Principal Component Analysis, Random Forest regression, generalized additive models, and mixed-effects modelling were used to identify environmental controls and quantify the memory&ndash;resilience relationship. Hydrological memory varied markedly among basins, from less than 3 years in the humid Yangtze and Pearl basins to approximately 5&ndash;6 years in the arid Heihe and Tarim basins. Recovery time increased strongly with memory duration (R&sup2; = 0.81, p &lt; 0.001), and drought recovery was generally two to three times longer than flood recovery. Mixed-effects modelling confirmed hydrological memory as the dominant predictor of recovery time (&beta; = 0.68, p &lt; 0.001), with the full model explaining 84% of the observed variability. Random Forest analysis identified groundwater storage (28.4%), climatic aridity (22.7%), soil moisture persistence (17.9%), and basin elevation (12.6%) as the principal controls on memory. The results show that antecedent storage exerts a measurable control on post-extreme recovery and basin resilience. The HMF provides a process-based basis for identifying vulnerable basins and improving climate-adaptive water resources management.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5097</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5097/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145684</identifier>
    <datestamp>2026-09-24</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[Simultaneous, in situ detection of gas-phase carbon disulfide (CS2) and carbonyl sulfide (OCS) via O2+ chemical ionization mass spectrometry]]></dc:title>
      <dc:creator>Kray, Elisabeth N.</dc:creator>
      <dc:creator>Kilgour, Delaney B.</dc:creator>
      <dc:creator>Rogers, Martina N.</dc:creator>
      <dc:creator>Jernigan, Christopher M.</dc:creator>
      <dc:creator>Vermeuel, Michael P.</dc:creator>
      <dc:creator>Bertram, Timothy H.</dc:creator>
      <dc:description><![CDATA[Carbonyl sulfide (OCS) is the largest gas-phase sulfur reservoir in the troposphere. OCS is both directly emitted to the atmosphere and formed chemically in the atmosphere following the oxidation of reduced sulfur species such as carbon disulfide (CS<sub>2</sub>) and dimethyl sulfide (C<sub>2</sub>H<sub>6</sub>S, DMS). OCS is the largest continuous contributor to stratospheric sulfate aerosol and a key diagnostic for the photosynthetic uptake of&nbsp;carbon dioxide&nbsp;(CO<sub>2</sub>).&nbsp;Despite its importance to the OCS budget, <em>in situ</em> measurements of CS<sub>2</sub> are extremely limited. Here, we describe a new technique for the simultaneous measurement of CS<sub>2</sub>, OCS, and DMS utilizing O<sub>2</sub><sup>+</sup> chemical ionization time-of-flight mass spectrometry (O<sub>2</sub><sup>+</sup> CI-ToFMS). We highlight the utility of the measurement through the reanalysis of three distinct data sets taken in remote marine, remote continental, and urban environments. We report mean CS<sub>2</sub> mixing ratios for the Eastern North Atlantic (2.2 ppt) and Downtown Chicago, IL (9.5 ppt), while CS<sub>2</sub> was not detected in Northern Wisconsin. In the Eastern North Atlantic, CS<sub>2</sub> showed limited temporal variability during the summer. In Chicago, CS<sub>2</sub> was highly variable, with episodic large enhancements (&gt;85 ppt) suggesting local, anthropogenic sources. Results of laboratory measurements and success in the quantification of field measurements suggest that primary and secondary O<sub>2</sub><sup>+</sup> CI-ToFMS is suitable for simultaneous, <em>in situ</em> detection of CS<sub>2</sub> and OCS.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5120</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5120/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145802</identifier>
    <datestamp>2026-09-24</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[Airborne Microplastics in the PM2.5 Fraction: Empirically Calibrated &micro;FTIR-ATR Imaging Detects Particles Down to 2 &micro;m]]></dc:title>
      <dc:creator>Niida, Yasuhiro</dc:creator>
      <dc:creator>Okochi, Hiroshi</dc:creator>
      <dc:creator>Yoshida, Norihisa</dc:creator>
      <dc:creator>Tani, Yuto</dc:creator>
      <dc:creator>Sasai, Shunki</dc:creator>
      <dc:creator>Fujii, Yusuke</dc:creator>
      <dc:creator>Takenaka, Norimichi</dc:creator>
      <dc:description><![CDATA[Reliable identification of airborne microplastics (AMPs) in the PM<sub>2.5 </sub>fraction remains challenging. Conventional &micro;FTIR imaging studies of atmospheric aerosol have generally targeted larger particles, and the reliability of library-matching scores at this smaller size range has not been systematically examined. We present a &micro;FTIR-ATR imaging workflow that separates spectral processing for chemical identification from image processing for physical characterisation. For chemical identification, particle-level spectra were smoothed and evaluated through library matching combined with diagnostic-band interpretation. For physical characterisation, PCA-based image processing and blank-derived intensity thresholds defined particle boundaries for Feret-dimension measurement and morphological classification. We defined the TopHit ratio as the proportion of top-ranked library assignments agreeing with diagnostic-band interpretation within each maximum-correlation-coefficient (<em>R</em><sub>max</sub>) interval. Among 674 particles, this ratio rose from 41.1% at <em>R</em><sub>max</sub> = 0.4&ndash;0.5 to 96.0% at <em>R</em><sub>max</sub> = 0.8&ndash;0.9 and 100.0% at <em>R</em><sub>max</sub> = 0.9&ndash;1.0; a Richards growth model best described this relationship across four tested library/bin-width combinations. The workflow also enabled identification and measurement of an airborne polyethylene terephthalate particle collected in the PM<sub>2.5</sub> fraction, with an apparent minimum Feret dimension of 2.3 &micro;m. To our knowledge, this is the first study to combine &micro;FTIR-based polymer identification of an airborne PM<sub>2.5</sub> particle approaching 2 &micro;m with explicit empirical calibration of spectral-matching confidence.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5191</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5191/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145776</identifier>
    <datestamp>2026-09-24</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[Evaluating a Virtual Tall Tower approach for estimating atmospheric CO2 mixing ratios from near-surface measurements]]></dc:title>
      <dc:creator>Marcon-Henge, Lediane</dc:creator>
      <dc:creator>Peichl, Matthias</dc:creator>
      <dc:creator>Larmanou, Eric</dc:creator>
      <dc:creator>Graf, Alexander</dc:creator>
      <dc:description><![CDATA[Atmospheric CO<sub>2</sub> measurements provide essential constraints for atmospheric modelling and carbon-budget estimates. Measurements made at tall towers, typically at heights of approximately 100m and above, are more representative of well-mixed atmospheric conditions than near-surface observations, however their spatial coverage is limited. Virtual Tall Tower (VTT) methods offer a potential approach to scale CO<sub>2</sub> mixing ratios from eddy-covariance stations, where measurements are made closer to the surface, typically 2&ndash;50m above ground, to tall-tower heights, thereby expanding the spatial coverage of the existing sparse atmospheric observation network. In this study, we evaluated the performance of an existing VTT approach<br />for estimating CO<sub>2</sub> mixing ratios from 35m to 150m at the combined ecosystem&ndash;atmosphere station at Svartberget, a forest-dominated site in northern Sweden. The dataset covered five years (2020&ndash;2024) of eddy-covariance fluxes, tall-tower CO<sub>2</sub> mixing-ratio measurements, and planetary boundary layer height from ERA5 reanalysis. The baseline VTT set-up estimated CO<sub>2</sub> mixing ratios with low bias (0.03 &mu;molmol<sup>&minus;1</sup>), low RMSE (0.75 &mu;molmol<sup>&minus;1</sup>), and a high squared Pearson correlation coefficient (r<sup>2</sup> = 0.99). The largest discrepancies between estimated and measured mixing ratios occurred under atmospheric conditions with weakened vertical mixing, particularly during winter months and in the early morning. Moreover, surface CO<sub>2</sub> flux, sensible heat flux, planetary boundary layer height, and displacement height were among the most influential variables in the approach, as perturbations in these variables led to changes in performance metrics. The underlying VTT assumption of well-mixed conditions is an important constraint that limits the applicability of the method under stable atmospheric conditions, such as during night-time and cold days. In addition, well-calibrated eddy- covariance CO<sub>2</sub> mixing-ratio measurements are crucial for good VTT performance. Therefore, although the VTT approach is a promising tool for expanding atmospheric CO<sub>2</sub> mixing-ratio information from near-surface measurements, further investigations across different sites and environmental conditions are needed to improve and generalize the approach.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5181</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5181/]]></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:essd139032</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Italian Fluvial Sediment Transport Database: a comprehensive hub for archiving and analyzing hydrological data]]></dc:title>
      <dc:creator>Luppichini, Marco</dc:creator>
      <dc:creator>Comiti, Francesco</dc:creator>
      <dc:creator>Andreoli, Andrea</dc:creator>
      <dc:creator>Aldighieri, Barbara</dc:creator>
      <dc:creator>Billi, Paolo</dc:creator>
      <dc:creator>Bollati, Irene Maria</dc:creator>
      <dc:creator>Brenna, Andrea</dc:creator>
      <dc:creator>Chirici, Diletta</dc:creator>
      <dc:creator>Ciavola, Paolo</dc:creator>
      <dc:creator>Cilli, Silvia</dc:creator>
      <dc:creator>Donnini, Marco</dc:creator>
      <dc:creator>Francalanci, Simona</dc:creator>
      <dc:creator>Innocenti, Lorenzo</dc:creator>
      <dc:creator>Longoni, Laura</dc:creator>
      <dc:creator>Mao, Luca</dc:creator>
      <dc:creator>Marchesini, Ivan</dc:creator>
      <dc:creator>Murgia, Ilenia</dc:creator>
      <dc:creator>Pellegrini, Giacomo</dc:creator>
      <dc:creator>Penna, Daniele</dc:creator>
      <dc:creator>Picco, Lorenzo</dc:creator>
      <dc:creator>Rainato, Riccardo</dc:creator>
      <dc:creator>Schippa, Leonardo</dc:creator>
      <dc:creator>Solari, Luca</dc:creator>
      <dc:creator>Tronti, Gianluca</dc:creator>
      <dc:creator>Testa, Bruno</dc:creator>
      <dc:creator>Verdone, Matteo</dc:creator>
      <dc:creator>Bini, Monica</dc:creator>
      <dc:description><![CDATA[<p>Fluvial sediment transport plays a key role in geomorphological and hydrological processes, influencing river morphology, watershed and coastal sediment balances, and the environmental response to climatic and anthropogenic changes. In Italy, the availability of homogeneous and long-term data is strongly limited due to the discontinuity of monitoring activities and the fragmentation of existing sources. This study presents the development of a relational database and web application specifically designed for the collection, storage, and consultation of sediment transport data, aimed at integrating and enhancing heterogeneous datasets from both<span id="page7022"/> historical and contemporary monitoring networks: the Italian Fluvial Sediment Transport Database (ITASED). The database architecture, developed in PostgreSQL with the PostGIS extension, enables a direct link between observational data and their associated geographical, instrumental, and methodological metadata, ensuring traceability, interoperability, and the possibility to perform multi-temporal analyses. The web interface, built using open-source technologies, allows controlled data entry and interactive data exploration through maps, tables, and export functions. Analysis of the archived datasets highlights strong instrumental, temporal, and spatial heterogeneity: some physical-chemical parameters (e.g., pH and electrical conductivity) show standardized measurement protocols, whereas sediment transport variables exhibit high methodological variability. Time series range from sub-daily to annual observations, with denser coverage in northern Italian basins (e.g., Po, Adige, Piave, Tagliamento) since 1924. Despite these inconsistencies, integration within a unified relational framework enhances the value of a largely underused data heritage. The experience gained through this project enabled the identification of both the limitations and the potential of Italy's sediment monitoring system, providing operational guidance for methodological standardization, metadata improvement, and data harmonization at the national scale. The ITASED represents a concrete step toward establishing a shared sedimentological archive that supports scientific research, environmental management, and sustainable river basin planning. The dataset is publicly available on Zenodo at <a href="https://doi.org/10.5281/zenodo.18799025">https://doi.org/10.5281/zenodo.18799025</a> (Luppichini et al., 2026).</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-7021-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/7021/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd143427</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A global dataset of soil microplastics (2005&ndash;2026)]]></dc:title>
      <dc:creator>Wu, Peiwen</dc:creator>
      <dc:creator>Su, Yang</dc:creator>
      <dc:creator>Wang, Mengru</dc:creator>
      <dc:creator>Yang, Xiaomei</dc:creator>
      <dc:creator>Rillig, Matthias C.</dc:creator>
      <dc:creator>Wang, Xiahui</dc:creator>
      <dc:creator>Liu, Ruiping</dc:creator>
      <dc:creator>Ye, Su</dc:creator>
      <dc:creator>Zhou, Lianqing</dc:creator>
      <dc:creator>Shi, Zhou</dc:creator>
      <dc:creator>Chen, Songchao</dc:creator>
      <dc:description><![CDATA[Microplastics (&lt;5 mm) pose persistent global ecological risks due to their ubiquitous environmental distribution and negligible biodegradability. Compared with marine and freshwater ecosystems, for which global-scale distribution datasets have been increasingly developed, soil microplastic research still lacks a unified dataset that can support cross-regional comparison and geospatial analysis. Existing syntheses are mostly limited to national or regional scales, and the few global compilations remain constrained by data volume, spatial coverage, or variable harmonization. To address this gap, we systematically compiled published records of soil microplastics worldwide from 2005 to 2026. The resulting database comprises 6,197 harmonized records from 4,901 sampling sites across 49 countries, nearly doubling the record-level evidence base compared with the largest soil-microplastic distribution or risk synthesis identified to date. To enable cross-study synthesis, we developed a standardized schema to harmonize microplastic abundance records, land-use classifications, polymer types, shape categories, and particle-size data. Notably, we implemented particle-size distribution models to correct and harmonize abundance data reported across heterogeneous size fractions. Analysis of the compiled data reveals a highly uneven geographic distribution of current records, with Asia accounting for 89% of records with abundance information and China contributing the largest share. Soil microplastic abundance showed strongly right-skewed distributions across land-use types, and abundance patterns differed markedly between quantification methods. Spectroscopy-based records showed significantly higher median abundance than visual-based records. Differences in particle size, shape, and polymer composition among land-use categories further indicate substantial heterogeneity in soil microplastic characteristics across terrestrial environments. This dataset is archived on the Zenodo platform at https://doi.org/10.5281/zenodo.20806151 (Wu et al., 2026). The standardized data foundation presented here is critical for initializing global monitoring networks and accurately modeling soil microplastic dynamics across the Earth system.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-536</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-536/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd145620</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A knowledge-guided daily multi-layer soil freeze-thaw dataset for the Northern Hemisphere during 1950-2025]]></dc:title>
      <dc:creator>Yu, Han</dc:creator>
      <dc:creator>Wu, Mousong</dc:creator>
      <dc:creator>Yin, Dongjie</dc:creator>
      <dc:creator>Ran, Youhua</dc:creator>
      <dc:creator>Yi, Yonghong</dc:creator>
      <dc:description><![CDATA[Soil freeze-thaw (FT) dynamics regulate key thermal, hydrological, and ecological processes in cold regions, yet long-term, spatially continuous, and vertically resolved daily FT records remain scarce, particularly before the satellite era. Here, we present a soil Freeze-Thaw dataset generated using Knowledge-Guided Machine Learning (FT-KGML), providing daily FT states at 0.1&deg; spatial resolution across Northern Hemisphere frozen-ground regions from 1950 to 2025 at depths of 10, 30, and 50&thinsp;cm. FT-KGML was generated using a knowledge-guided neural network model that learns process-based FT relationships from soil-temperature simulations and is subsequently constrained by in situ observations, enabling a continuous 76-year reconstruction of subsurface FT dynamics. Independent station evaluation yielded overall daily classification accuracies of 86.12&thinsp;%, 89.67&thinsp;%, and 90.39&thinsp;% at 10, 30, and 50&thinsp;cm, respectively. Seasonal FT phenology was also well reproduced, with generally stronger agreement for the onset of soil freezing than for the onset of soil thawing. Matched comparisons with passive-microwave FT products and ERA5-Land showed broadly consistent daily FT dynamics and seasonal transition timing across datasets, providing additional support for the reliability of FT-KGML despite differences in their spatial scales and FT representations. The long-term record reveals relatively weak and spatially heterogeneous FT phenology changes during 1950-1978, followed by widespread earlier spring thaw and later autumn freezing after 1979. During 1979-2025, spring thaw advanced by 2.93-3.12&thinsp;d&thinsp;decade<sup>-1</sup>, whereas autumn freezing was delayed by 2.22-3.24&thinsp;d&thinsp;decade<sup>-1</sup> across the three soil depths. By combining long temporal coverage, daily resolution, and multi-depth representation, FT-KGML provides a new resource for cryospheric, hydrological, ecological, and land-surface modelling communities investigating frozen-ground variability, subsurface seasonality, and long-term environmental change. The dataset is available at <a href="https://doi.org/10.5281/zenodo.22019944">https://doi.org/10.5281/zenodo.22019944</a> (Yu and Wu, 2026).]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-683</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-683/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd146314</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[SCS-TCWave: an event-based hindcast dataset of typhoon waves and reconstructed wind fields for the South China Sea (1979&ndash;2025)]]></dc:title>
      <dc:creator>Fang, Feifan</dc:creator>
      <dc:creator>Yang, Yifeng</dc:creator>
      <dc:creator>Jin, Peng</dc:creator>
      <dc:creator>Zhou, Binzhen</dc:creator>
      <dc:description><![CDATA[Extreme-wave estimates for the South China Sea (SCS) depend on the peak sea states of tropical cyclones, yet reanalysis winds smooth the storm core and no openly archived, event-resolved typhoon wave record exists for the basin. We present SCS-TCWave, an event-based hindcast of the 480 tropical cyclones that reached tropical storm intensity inside the SCS during 1979&ndash;2025. Each event is forced by 10-m winds reconstructed from best-track records (a Holland-type vortex with motion asymmetry and far-field gale-radius anchoring, blended into ERA5) and simulated with SWAN on one-way nested 0.25&deg;/0.05&deg; grids under a frozen, fully audited configuration. Each event ships three CF-1.8 NetCDF layers: hourly wave fields, the reconstructed wind forcing, and an extreme-value catalogue of per-cell event maxima. Validation against 64,529 calibrated altimeter super-observations from 187 events shows near-zero bias in background sea states and a single-signed core overestimation that grows with intensity (+1.15 to +2.99 m within 100 km of the centre). A distance-binned multiplicative correction annex with bootstrap confidence intervals centres the per-event peak distribution: the median relative error of per-event maxima moves from +9.5 % raw to &minus;1.4 % corrected, with 78 % of events within &plusmn;25 %. At the highest observed peak (9.4 m, Pearl River estuary, Typhoon Mangkhut) the product stays within &plusmn;25 % where an identically configured ERA5-forced run does not; beyond 400 km ERA5-based products remain preferable, and this distance-based usage rule ships with the data. Method tiers, quality flags, the frozen configuration, and the full calibration record accompany the archive (<a href="https://doi.org/10.57760/sciencedb.011ul">https://doi.org/10.57760/sciencedb.011ul</a>; Fang et al., 2026).]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-737</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-737/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd146400</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A harmonized radiocarbon chronology framework for subarctic North Pacific marine sediment cores]]></dc:title>
      <dc:creator>Wang, Rong</dc:creator>
      <dc:creator>Ren, Jian</dc:creator>
      <dc:creator>Diekmann, Bernhard</dc:creator>
      <dc:description><![CDATA[Published marine sediment chronologies from the subarctic North Pacific differ in calibration curves, reservoir corrections, input selection, and modelling conventions, complicating comparisons among palaeoceanographic records. We present a chronology framework for 17 cores from the Bering Sea, Gulf of Alaska, Sea of Okhotsk, and open subarctic North Pacific. The main inventory contains 19 core or segment records: 16 Marine20&ndash;rbacon reconstructions, two separately identified legacy calendar-age models, and one segment without a chronology. The 18 canonical age-model tables provide posterior median ages and pointwise 95 % intervals on a standardized 201-depth grid. Users can assign these ages to depth-registered proxy measurements from the same cores after verifying depth-scale correspondence; the framework cannot date a new core without its own chronological constraints.</p> <p>The archive preserves 555 chronology-control rows with their provenance, material roles, and admission decisions. The 18 verified formal model-input files contain 285 rows representing 282 dated-depth clusters or legacy calendar-age nodes. Twenty-eight constraints misassigned to surface chronology during an earlier stage of this compilation are retained with their material-role and exclusion records, allowing users to inspect or revise the admission decisions. The primary precision descriptor is the median width of the pointwise 95 % posterior age interval within each dated interval. Among 14 inventory rows assigned a derived convenience bin, this statistic ranges from 677 to 2765 yr, with a median of approximately 1100 yr. Sampling diagnostics are reported at all evaluation depths. Independent reruns of four preselected records changed this continuous statistic by at most 6.64 yr, although one boundary-adjacent record crossed a derived-bin boundary.</p> <p>Posterior precision is conditional on calibration, the reservoir correction and its adopted date-level uncertainty, input representation, and the modelling protocol; it does not establish absolute chronological accuracy. The adopted reservoir corrections are based on modern observations, whereas deglacial reservoir histories remain incompletely constrained. The release combines age tables, audited inputs, cluster definitions, diagnostics, per-record JSON/CSV packages, source references, and implementation records to support reuse and alternative chronological modelling. Executed model inputs are preserved, but recovery of the full source-to-prepared transformation chain is incomplete. The data are deposited at PANGAEA under <a href="https://doi.pangaea.de/10.1594/PANGAEA.996868">https://doi.pangaea.de/10.1594/PANGAEA.996868</a>.]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-742</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-742/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gh131001</identifier>
    <datestamp>2026-09-24</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[Mehr-als-irdische Geographien und die zweite Kopernikanische Wende des planetarischen  Denkens. Eine metaphorologische Kritik]]></dc:title>
      <dc:creator>Runkel, Simon</dc:creator>
      <dc:description><![CDATA[<p>The article examines the terms earth, globe and world as central ciphers of geographical thinking and places them in a genealogy of the history of ideas and science. The focus is on the current boom in planetary thinking, which is fanned out into two currents: on the one hand in (earth) system-theoretical totality, on the other hand in post-humanist perspectives on co-existence. In both discourses, a new Copernican turn is claimed, whose metaphorological content, however, points to a continuation of post-Copernican ambivalence. Based on Hans Blumenberg's metaphorology, it is shown how planetary semantics oscillates between epistemic upheaval and anthropocentric self-assertion (Selbstbehauptung). The article is intended as a plea for a stronger reception of humanities thinking styles in geography. Here, metaphorology proves to be an approach to the critical reflection of disciplinary world and self-relations under the sign of planetarism. The euphoric welcome of planetary thinking in geography and the pleas for a new Copernican turn are evidence of the unbroken discursive power of this metaphor.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gh-81-517-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gh.copernicus.org/articles/81/517/2026/]]></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:esd132460</identifier>
    <datestamp>2026-09-24</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/"
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      <dc:title><![CDATA[Ocean dynamics amplify remote warming effects of reforestation]]></dc:title>
      <dc:creator>Banville, Pierre Etienne</dc:creator>
      <dc:creator>MacIsaac, Alexander J.</dc:creator>
      <dc:creator>Zickfeld, Kirsten</dc:creator>
      <dc:description><![CDATA[<p>Forestation, including reforestation, afforestation, and forest restoration, is prevalent in net-zero climate strategies due to the large carbon sequestration potential of forests. In addition to capturing carbon, forestation has biogeophysical effects that can influence surface temperatures locally (local effects), and at distant locations (non-local effects). Biogeophysical effects may offset the cooling benefits of carbon sequestration, hence requiring a robust understanding of their mechanisms to adequately integrate forestation into climate mitigation strategies. Yet, the role of ocean dynamics, such as ocean circulation, ocean-atmosphere interactions, and ocean-sea ice interactions in mediating the non-local effects of forestation remains underexplored. In this study, we investigate the impact of ocean dynamics on the magnitude and geographic patterns of the non-local biogeophysical effects of large-scale reforestation, with the exclusion of cloud feedbacks, over a multi-century timescale using the University of Victoria Earth System Climate Model. We conduct multi-century paired global reforestation simulations, with the first set of simulations using a dynamic ocean and the second set using prescribed sea surface temperatures. We separate local from non-local effects using the checkerboard approach. Our results show that non-local warming effects are of much greater magnitude and encompass a greater geographic area, particularly at high latitudes, when ocean dynamics are considered. Moreover, this study shows that ocean dynamics introduce a lag in the non-local effects, leading to a continued increase in non-local warming even after the local effects have stabilized. This committed non-local warming is driven by the thermal inertia of the ocean, which sustains a gradual long-term increase in sea surface temperatures, combined with amplifying climate feedbacks. Decision-making frameworks must therefore consider the complete Earth system response to forestation over a sufficiently long timeframe to account for the committed non-local warming.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-1315-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/1315/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:hess135606</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>hess</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Calibration using downscaled and bias-corrected satellite soil-moisture data can improve watershed model representation of soil-moisture variability]]></dc:title>
      <dc:creator>Asfaw, Binyam Workeye</dc:creator>
      <dc:creator>Maksud, Siam</dc:creator>
      <dc:creator>Fuka, Daniel R.</dc:creator>
      <dc:creator>Collick, Amy S.</dc:creator>
      <dc:creator>White, Robin R.</dc:creator>
      <dc:creator>Easton, Zachary M.</dc:creator>
      <dc:description><![CDATA[<p>Watershed streamflow is often the focus of hydrological model calibration and evaluation, despite other potential objectives, including water quality management, flood protection, or agricultural management. When hydrological models are calibrated on streamflow, intermediate processes such as those affecting soil-moisture are not necessarily well represented. This research evaluated whether calibration using downscaled and bias-corrected satellite soil-moisture improves prediction of field-scale soil-moisture relative to conventional streamflow-based calibration. In this work, downscaled satellite soil-moisture and streamflow data are used to calibrate a soil and water assessment tool – variable source area model initialized using a terrain informed process to create hydrologic response units. In-situ soil-moisture measurements at 25 locations across a 4.2-ha mixed-grass pasture located in southwestern Virginia were used to estimate field-scale average soil-moisture variability for model evaluation. Leveraging downscaled satellite soil-moisture data substantially improved estimation of temporal soil-moisture variability without affecting the model streamflow performance. The multi-objective calibration using streamflow and satellite soil-moisture improved soil-moisture performance while maintaining streamflow performance comparable to streamflow-only calibration. These results demonstrate the potential for satellite soil-moisture–informed calibration to improve internal hydrologic state estimation in small, saturation excess watersheds. Furthermore, these results highlight the importance of coupling statistical performance gains with evaluation of hydrologic realism when extending such approaches to broader modeling applications.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-5999-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/5999/2026/]]></dc:identifier>
      <dc:source>eISSN: 1607-7938</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:hess138230</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>hess</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The Canadian Surface Reanalysis (CaSR) v3.2 precipitation dataset: a 45-year high-resolution analysis for North America (1980–2024)]]></dc:title>
      <dc:creator>Khedhaouiria, Dikraa</dc:creator>
      <dc:creator>Gasset, Nicolas</dc:creator>
      <dc:creator>Fortin, Vincent</dc:creator>
      <dc:creator>Dimitrijevic, Milena</dc:creator>
      <dc:creator>Bulat, Maxim</dc:creator>
      <dc:creator>Wang, Xihong</dc:creator>
      <dc:description><![CDATA[<p>The Canadian Surface Reanalysis (CaSR) includes an offline, high-resolution gridded total precipitation reanalysis designed to provide accurate estimates across North America. This product, referred to as CaPA-24h, builds on the Canadian Precipitation Analysis (CaPA) system of Environment and Climate Change Canada (ECCC). It combines a dense network of daily surface observations with a background field from the CaSR dynamical component, using updated quality-control and assimilation procedures to filter spurious observations. This study evaluates the CaPA-24h fields produced in CaSR v3.2, together with their background field, and compares them with the previous version (v2.1) as well as with two independent datasets, ERA5-Land and PRISM. Results show substantial improvements in v3.2, particularly in data-sparse regions, with an enhanced representation of precipitation events of different intensities. Compared to ERA5-Land, CaPA-24h v3.2 provides more accurate seasonal and regional precipitation patterns, while evaluations against PRISM confirm this improved performance. However, biases persist in southern and western mountainous areas, especially for orographic precipitation. A first-time assessment of the hourly disaggregated product reveals limitations in the diurnal cycle representation, indicating the need for refined disaggregation methods and background field generation. Overall, CaPA-24h v3.2 delivers a reliable and well-established gridded precipitation dataset, offering a valuable resource for hydrological, climatological, and impact studies across North America.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-5971-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/5971/2026/]]></dc:identifier>
      <dc:source>eISSN: 1607-7938</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd134208</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Three-stream modelling of radiative transfer for the simulation of Black Sea biogeochemistry in a NEMO framework]]></dc:title>
      <dc:creator>Macé, Loïc</dc:creator>
      <dc:creator>Vandenbulcke, Luc</dc:creator>
      <dc:creator>Brankart, Jean-Michel</dc:creator>
      <dc:creator>Grailet, Jean-François</dc:creator>
      <dc:creator>Brasseur, Pierre</dc:creator>
      <dc:creator>Grégoire, Marilaure</dc:creator>
      <dc:description><![CDATA[<p>In this paper, we propose a three-stream ocean radiative transfer module as an extension of the Nucleus for European Modelling of the Ocean (NEMO). This module solves in-water irradiance fields in 1D water columns, discriminating between two downward streams, direct and scattered, and a backscattered upward stream. The module solves 33 wavebands between 250 and 4000 nm, with a resolution of 25 nm in the visible range. The sea surface reflectance is also calculated as a model output, based on the ratio between the upward and downward irradiances at the air-sea interface. We also use a feedback loop towards the computation of temperature in the NEMO model, made optional with this module. It also includes a stochastic version in which the inherent optical properties of the major optically active components of seawater can be perturbed. This mode is meant to account for uncertainty in the modelling of marine optics. This module can be plugged into any NEMO configuration, with the computation of optical properties driven either by a coupled biogeochemical model or directly forced into the radiative transfer module.</p>        <p>We apply this module in a test case for the Black Sea, within the NEMO framework and coupled to the Biogeochemical Model for Hypoxic and Benthic Influenced areas (BAMHBI). We find that substituting the existing radiative transfer scheme with our model unlocks the ability to simulate radiometric variables that can be compared more directly to observations, both in situ and from remote-sensing. We also find that using irradiances to compute the temperature and scalar irradiance that is available to phytoplankton in the coupled model maintains consistency in the calculation of physical and biogeochemical variables. The simulation of variables such as temperature or chlorophyll concentration is maintained, while enabling additional capabilities in the model with the simulation of radiometric quantities.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9077-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9077/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd132287</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Natural methane emissions feedbacks in MAGICC v. 7.6]]></dc:title>
      <dc:creator>Sloughter, Trevor</dc:creator>
      <dc:creator>Nicholls, Zebedee</dc:creator>
      <dc:creator>Tang, Gang</dc:creator>
      <dc:creator>Kleinen, Thomas</dc:creator>
      <dc:creator>Zhang, Zhen</dc:creator>
      <dc:creator>Rogelj, Joeri</dc:creator>
      <dc:description><![CDATA[<p>Literature estimates of natural methane emissions, particularly from wetlands, have a wide range of uncertainty. Meanwhile, few Earth System Models (ESMs) explicitly model wetlands as a potential source of methane. As a result, Simple Climate Models that aim to emulate the behaviour of ESMs have little to constrain their present and future contributions. MAGICC, as of version 7.5.3, fixed natural methane concentrations as constant after the historical period. Two studies that model wetland methane emissions over the 21st century both find a relationship between those emissions and global temperature, though disagree on the extent of this temperature sensitivity. An updated version of MAGICC has been created that uses this evidence to include a linearised representation of the relationship between wetland methane emissions and global temperature. The temperature-sensitivity parameter in this relationship has been parametrised in a way such that its distribution encompasses the uncertainty in both modelling literature and carbon budget studies, reflecting the currently high degree of uncertainty in wetland emissions. Our results show how incorporating a temperature feedback in methane emissions leads to both higher temperature projections for all scenarios used here, and a widening of the uncertainty in global temperature response.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9063-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9063/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd131805</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A hybrid method for winter road surface temperature prediction using improved LSTMs and stacking-based ensemble learning]]></dc:title>
      <dc:creator>Li, Wanting</dc:creator>
      <dc:creator>Zhou, Linyi</dc:creator>
      <dc:creator>Wu, Xianghua</dc:creator>
      <dc:creator>Guan, Yuanhong</dc:creator>
      <dc:creator>Guo, Yuanhao</dc:creator>
      <dc:creator>Chen, Kun</dc:creator>
      <dc:creator>Huang, Weiqi</dc:creator>
      <dc:creator>Zhao, Wenqian</dc:creator>
      <dc:description><![CDATA[<p>Accurate prediction of road surface temperature (RST) is essential for proactive winter road maintenance and traffic safety management. However, existing approaches – ranging from physics-based models to data-driven methods – either require detailed pavement thermal parameters that are rarely available at operational road meteorological stations, or lack the capacity to simultaneously exploit local meteorological analogues and long-range temporal dependencies in an interpretable ensemble framework. This study proposes the Improved LSTMs Ensemble with Stacking (ILES) framework, which integrates two base learners with partially complementary predictive characteristics within a stacking ensemble employing out-of-fold cross-validation. The first base learner, KNN-LSTM, augments sequential modelling with similarity-based retrieval of historically analogous meteorological states to capture locally recurrent patterns. The second, BiLSTM-MHA, combines bidirectional recurrent processing with multi-head self-attention to extract long-range temporal dependencies across a 24 h input window. Moreover, a Bayesian Ridge Regression meta-learner fuses the base-learner outputs through Evidence Maximization, yielding probabilistic forecasts with closed-form posterior predictive uncertainty at the ensemble combination layer. The framework is trained and evaluated on four consecutive winter seasons (December 2020 to February 2024) of road meteorological observations from station M9393 in the northwest inland plain of Jiangsu Province, China. Results indicate that ILES achieves lower prediction errors in general than ten other models spanning persistence forecasting, traditional machine learning, and deep learning approaches, with <span class="inline-formula"><i>R</i><sup>2</sup></span> reaching 0.993, 0.923, and 0.826 at 1, 3, and 6 h forecasting horizons, respectively. Among three input configurations evaluated, physics-motivated feature engineering incorporating the air–surface temperature gradient and multi-scale RST temporal tendencies outperforms both the station-only baseline and ERA5-Land reanalysis augmentation, indicating that domain-knowledge-guided feature construction provides a more effective and operationally practical input strategy at instrumented sites. SHAP-based interpretability analysis, stratified by temperature regime and diurnal cycle, confirms that the learned feature importance rankings are qualitatively consistent with the dominant drivers of RST evolution identified by surface energy balance theory. Multi-site generalization is further validated at two independent stations within the same temperate monsoon climate zone, confirming the transferability of the proposed framework across different road environments within this climate setting.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9035-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9035/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd140589</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Consideration of radiation absorption by stems in forests for microclimate modeling]]></dc:title>
      <dc:creator>Béland, Martin</dc:creator>
      <dc:creator>Bonan, Gordon</dc:creator>
      <dc:creator>Kobayashi, Hideki</dc:creator>
      <dc:creator>Baldocchi, Dennis</dc:creator>
      <dc:description><![CDATA[<p>Forest canopy models are used to simulate biosphere–atmosphere coupling in global climate models, as well as the microclimate influences of forests at the stand scale. It has recently been shown that wood structures store significant heat following radiation absorption and impact air temperature diurnal patterns inside canopies. Yet, radiation absorption by woody stems is not fully considered in current models. Here we modify the radiative transfer component of the CanVeg2 multilayer canopy model to include radiation absorption by woody stems. We evaluate the model modifications by comparing estimates against a 3D ray tracing radiative transfer model parametrized using ground lidar measurements, and against tower observations of albedo in four broadleaf forests. We found a very good agreement between the 1D and 3D models, and a good agreement between models and observations. Our approach provides a tractable and computationally efficient implementation of radiation absorption by woody stems to calculate biomass heat storage in canopy models.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9019-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9019/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:tc137977</identifier>
    <datestamp>2026-09-24</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[Impact of climate forcing time step in an ice-sheet firn model]]></dc:title>
      <dc:creator>Aker, Tesse E. A.</dc:creator>
      <dc:creator>Kuipers Munneke, Peter</dc:creator>
      <dc:creator>Berg, Willem Jan</dc:creator>
      <dc:creator>Immerzeel, Walter W.</dc:creator>
      <dc:creator>Broeke, Michiel R.</dc:creator>
      <dc:description><![CDATA[<p>The firn layer regulates how an ice sheet responds to atmospheric climate change by modifying how changes in surface temperature, snow accumulation and ablation affect the ice-sheet mass balance. Firn properties are often simulated with a firn densification model. Prior studies have used a variety of time steps in the climate forcings of such firn models, ranging from 3 h to 1 d, 1-month, or even annual. The climate forcing time step impacts the creation of pore space by snow accumulation and the depletion of pore space by snowmelt and firn densification. To investigate this effect, we force the firn densification model IMAU-FDM with surface mass balance components and meteorological variables at different time steps for the Antarctic Peninsula and southern Greenland Ice Sheet. We show that the final modelled firn layer contains more pore space for larger forcing time steps, and that the magnitude of this effect depends on the climate regime. Locations with limited firn pore space due to seasonal melt, and regions with emerging firn aquifers, are most sensitive. The key in causing the differences in firn pore space is the presence or absence of a diurnal cycle in the input data. A climate forcing time step equal to or greater than a day allows for a non-physical coexistence of snowmelt and sub-zero surface temperatures, leading to immediate shallow refreezing of meltwater. Subsequent melting removes refrozen higher density firn rather than porous firn, reducing the amount of firn air that is lost through melting. Therefore, for locations experiencing surface melt, the decoupled temperature and snowmelt in the upper layers results in more firn air with a climate forcing time step equal to or greater than a day. We also found that model parameterizations can become unsuitable when applied outside the physical conditions or climate forcing time step on which they are based, leading to unrealistic firn densification behavior in the model. We argue that (1) firn models forced with surface mass balance terms and meteorological variables require a timestep small enough to capture at least the diurnal cycle, (2) parameterizations should be used in a way that is consistent with the development data.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/tc-20-5475-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/5475/2026/]]></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:wes135358</identifier>
    <datestamp>2026-09-24</datestamp>
    <setSpec>wes</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[SANDWake3D: a 3D parabolic RANS solver for atmospheric surface layers and turbine wakes]]></dc:title>
      <dc:creator>Cheung, Lawrence</dc:creator>
      <dc:creator>Mohan, Prakash</dc:creator>
      <dc:creator>Henry de Frahan, Marc T.</dc:creator>
      <dc:creator>Yalla, Gopal R.</dc:creator>
      <dc:creator>Hsieh, Alan</dc:creator>
      <dc:creator>Brown, Kenneth</dc:creator>
      <dc:creator>deVelder, Nathaniel</dc:creator>
      <dc:creator>Kaufman-Martin, Sam</dc:creator>
      <dc:creator>Day, Marc</dc:creator>
      <dc:creator>Sprague, Michael</dc:creator>
      <dc:description><![CDATA[<p>Despite many recent advances, modeling wind turbine wakes using semi-empirical and analytical models still faces challenges when dealing with more complicated situations involving wind shear, veer, atmospheric stratification, and wake superposition. To address these limitations, this study introduces a three-dimensional, parabolic Reynolds-averaged Navier–Stokes (RANS) <span class="inline-formula"><i>k</i>−<i>ϵ</i></span> formulation which includes an atmospheric boundary layer model and an actuator disk model for turbine wakes. The full three-dimensional solution for the velocity, temperature, and turbulence variables is efficiently solved through an alternating-direction implicit scheme that requires orders of magnitude fewer computational resources than traditional high-fidelity approaches, such as fully elliptic RANS or large-eddy simulations (LESs). The results of the parabolic RANS model are compared to the equivalent LES and semi-empirical wake models at different wind speeds under stable atmospheric conditions with veer and shear at a single TI level, as well as a convectively unstable-inflow case. For the single-turbine wake the RANS model was able to capture the wake deficit behavior, including the wake stretching and skewing that was observed in the LES. The distribution of the wake turbulence in the RANS model also agreed with results from the higher-fidelity simulations. In simulations of a two-turbine, directly waked configuration, the new RANS model was able to handle the wake superposition behavior without difficulty and also correctly modeled the corresponding increase in wake turbulence when compared to LES. A demonstration of the RANS model on a nine-turbine, three-row wind farm is shown and compared to LES, and comparisons with a semi-empirical veered Gaussian model are also discussed. The work in this study can be generalized in future investigations to handle additional wind conditions and more complex wind farm configurations.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/wes-11-3719-2026</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/articles/11/3719/2026/]]></dc:identifier>
      <dc:source>eISSN: 2366-7451</dc:source>
      <dc:language>eng</dc:language>
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    <identifier>oai:publications.copernicus.org:wes133893</identifier>
    <datestamp>2026-09-24</datestamp>
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      <dc:title><![CDATA[Economic and design optimization of a 15&thinsp;MW floating offshore wind platform using time series forecasting]]></dc:title>
      <dc:creator>White, Craig</dc:creator>
      <dc:creator>Benifla, Victor</dc:creator>
      <dc:creator>Cândido, José</dc:creator>
      <dc:creator>Gato, Luís M. C.</dc:creator>
      <dc:description><![CDATA[<p>A structural and economic optimization framework applicable to floating semi-submersible platforms, demonstrated here for a 15 MW offshore wind design, is presented. A genetic algorithm was developed that can seek a multi-objective solution to minimize mass whilst respecting the constraints of loads acting upon the system. Statistical and machine learning methods are then employed to forecast short- and long-term costs of the platform under a range of exogenous data scenarios, selected to support and boost forecasting accuracy alongside a hybrid forecasting method. Steel mass was reduced from 3916 to 3273 t whilst respecting platform response constraints. The uncertainty in steel prices has the most significant impact on CAPEX, approximately EUR 150–200 million at the 1 GW level. Levelized cost of energy (LCoE) is calculated to gauge the technical and economic viability, with EUR 3–5 MW h<span class="inline-formula"><sup>−1</sup></span> variation across forecasts.</p>]]></dc:description>
      <dc:date>2026-09-24</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/wes-11-3703-2026</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/articles/11/3703/2026/]]></dc:identifier>
      <dc:source>eISSN: 2366-7451</dc:source>
      <dc:language>eng</dc:language>
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