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    <datestamp>2026-10-12</datestamp>
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      <dc:title><![CDATA[Design of a scaled wind turbine model for matching multiple structural load transients under blade-detachment conditions]]></dc:title>
      <dc:creator>Liu, Hongwen</dc:creator>
      <dc:creator>Song, Qingfu</dc:creator>
      <dc:creator>Guo, Feng</dc:creator>
      <dc:creator>Yang, Lin</dc:creator>
      <dc:creator>Xu, Wenhao</dc:creator>
      <dc:creator>Zhang, Lijun</dc:creator>
      <dc:creator>Gao, Zhen</dc:creator>
      <dc:description><![CDATA[Complete blade detachment simultaneously changes a wind turbine's aerodynamic, centrifugal, and gravitational loading, requiring these load changes to be matched consistently in model-scale experiments. This study develops a scaled wind turbine design method that establishes common force and moment scales to define coupled targets for rotor speed, blade mass, spanwise mass distribution, and axial aerodynamic loading. The method is demonstrated using a 1:100 model of a 10 MW prototype onshore turbine. The blade geometry is redesigned for low-Reynolds-number operation, and a modular construction combining a CNC-machined carbon-fibre spar with segmented PMI foam permits separate adjustment of the aerodynamic profile and material distribution. Centrifugal- and aerodynamic-load experiments show overall agreement between numerical predictions and measurements under the tested conditions. The resulting model provides an experimental basis for controlled blade-detachment testing and subsequent validation of numerical models of post-failure load redistribution.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
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      <dc:identifier>https://doi.org/10.5194/wes-2026-167</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/preprints/wes-2026-167/]]></dc:identifier>
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   <header>
    <identifier>oai:publications.copernicus.org:wesd147307</identifier>
    <datestamp>2026-10-12</datestamp>
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       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[Machine learning-based prediction of critical load events in airborne wind energy systems]]></dc:title>
      <dc:creator>Pasquali, Monika</dc:creator>
      <dc:creator>Cayon, Oriol</dc:creator>
      <dc:creator>Theodoulis, Spilios</dc:creator>
      <dc:creator>Farges, Christophe</dc:creator>
      <dc:creator>Airimitoaie, Tudor-Bogdan</dc:creator>
      <dc:creator>Lanusse, Patrick</dc:creator>
      <dc:creator>Schmehl, Roland</dc:creator>
      <dc:description><![CDATA[Predicting and avoiding critical load events is crucial for the reliable autonomous operation of airborne wind energy (AWE) systems. Such events can lead to actuator saturation, loss of steering authority, and increased structural stresses, eventually resulting in long-term degradation of the kite, tether, and ground-station components. The present study explores a data-driven approach to predicting tether force peaks, defined as instances in which the force exceeds a threshold set by the winch controller. The method is developed using a large-scale SCADA dataset from Kitepower's leading-edge inflatable V9 kite, including more than 1000 pumping cycles spanning 26 h of kite operation and covering a wide range of wind and operating conditions. Tether force peaks are detected and used to extract pre-peak time windows that capture the system behavior before each threshold exceedance. From these windows, statistical, temporal, and spectral features are computed from multiple kite, tether, and ground-station measurements. A supervised classification model is trained to distinguish normal operation from pre-peak dynamics. The proposed approach predicts critical load events 1 s in advance and shows strong generalization capability on flight data that was not used for training the model, correctly identifying 85.4 % of the critical load events (recall) and achieving a 90.9 % F1-score, a metric that indicates a strong balance between correctly detected events and false alarms. Moreover, the extracted features provide valuable insight into the system dynamics preceding these events. The obtained results enable preventive control actions, thereby improving the reliability of AWE systems.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
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      <dc:identifier>https://doi.org/10.5194/wes-2026-180</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/preprints/wes-2026-180/]]></dc:identifier>
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      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:wes142617</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>wes</setSpec>
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     <oai_dc:dc
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      <dc:title><![CDATA[Sub-minute fatigue monitoring for enhanced lifetime assessment of wind turbines]]></dc:title>
      <dc:creator>Oliveira, Catarina Miranda</dc:creator>
      <dc:creator>Biscaya, André</dc:creator>
      <dc:creator>Santos, João Pedro</dc:creator>
      <dc:creator>Caetano, Elsa</dc:creator>
      <dc:creator>Xu, Min</dc:creator>
      <dc:description><![CDATA[<p>Accurate fatigue-damage estimation is a critical step for managing and extending the life of wind turbine fleets and the basis on which operators decide whether an ageing asset can be kept in service beyond the end of design life. The most accurate estimation relies on continuous high-frequency strain measurements processed with rainflow cycle counting. However, only a small subset of turbines within a fleet are typically instrumented with strain sensors, and even for these, the data volumes, computational complexity, and cost of continuously processing high-frequency strain data via rainflow counting over long-term operation make this approach impractical to sustain at scale. For this reason, industry practice has long relied on stress data aggregated over 10 min windows already used by supervisory control and data acquisition (SCADA) systems, which are available across the full fleet. This choice is convenient but, when combined with conventional window-based rainflow counting, tends to underestimate fatigue damage generated by cycles whose period exceeds the window length, driven by factors such as slow variations in wind speed and direction, operational transitions, control actions, and seasonal or daily temperature variation, as well as, for offshore turbines, changes in wave parameters. Residual-preserving approaches, most notably low-frequency fatigue dynamics (LFFD), address this limitation by reconstructing cycles that span window boundaries but have so far been applied almost exclusively within the conventional 10 min framework.</p>        <p>Technology has recently enabled operators to deploy second-resolution SCADA metrics at scale and at reasonable cost, offering finer-grained statistical descriptors for applications such as load and bending-moment estimation and operational-state classification. This is also an opportunity to revisit fatigue monitoring at a SCADA-aligned timescale that is short enough to limit the truncation of boundary-spanning cycles inherent to conventional window-based counting yet aggregated enough to remain deployable across large fleets. This paper benchmarks the families of methods that make this opportunity actionable against continuous rainflow as a baseline: conventional window-based counting, a modified low-frequency fatigue dynamics (LFFD) formulation that explicitly resolves intra-window and inter-window damage contributions, and two reduced-information extrema-sequence representations – start–peaks–valleys–end (SPVE) and maximum and minimum (max–min). The evaluation uses 6 months of 15 s windows of SCADA and strain measurements acquired at 50 Hz from two instrumented tower sections of an onshore wind turbine and examines the influence of window length, sampling rate, and fatigue-curve formulation on damage computation (Eurocode 3 vs. DNV).</p>        <p>Reducing the aggregation window from 10 min to 15 s alone does not improve fatigue estimation, as shorter windows increasingly truncate the low-frequency cycles that dominate accumulated damage. The proposed modified LFFD framework overcomes this limitation by preserving cycle continuity across window boundaries,<span id="page3842"/> recovering 99.5 % of the baseline damage while requiring only a fraction of the original data volume. Reduced-information representations further demonstrate that fatigue can be estimated with high accuracy using strongly compressed stress sequences, with start–peaks–valleys–end (SPVE) and maximum and minimum (max–min) retaining 98.8 % and 96.2 % of the baseline damage, respectively. These findings establish a practical pathway towards SCADA-aligned, data-efficient fatigue monitoring, enabling scalable lifetime assessment across large wind turbine fleets while preserving the fidelity of high-resolution structural measurements.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/wes-11-3841-2026</dc:identifier>
      <dc:identifier><![CDATA[https://wes.copernicus.org/articles/11/3841/2026/]]></dc:identifier>
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    <identifier>oai:publications.copernicus.org:tc141191</identifier>
    <datestamp>2026-10-12</datestamp>
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      <dc:title><![CDATA[Temperature sensitivity of snow viscoplasticity: Evidence from controlled creep experiments]]></dc:title>
      <dc:creator>Védrine, Louis</dc:creator>
      <dc:creator>Brun, Marius</dc:creator>
      <dc:creator>Bozon, Mathis</dc:creator>
      <dc:creator>Laurent, Benoit</dc:creator>
      <dc:creator>Hagenmuller, Pascal</dc:creator>
      <dc:description><![CDATA[<p>Snow is a warm, porous material whose densification under its own weight is highly temperature-dependent. Despite decades of research, reported activation energies for snow viscoplasticity remain highly scattered, ranging from 40–600 <span class="inline-formula">kJ mol<sup>−1</sup></span>. We quantified the temperature dependence of snow viscoplasticity using in-tomograph creep experiments with a newly developed thermo-mechanical cell. This design allows accurate load and temperature control, micrometric displacement measurement, and microstructural evolution monitoring via X-ray tomography. To disentangle microstructural evolution and temperature effects on the compression rate, we used a state-of-the-art viscoplastic model. We conducted five experiments on centimetre-scale samples of decomposing and fragmented precipitation particles with initial densities ranging from 278–320 <span class="inline-formula">kg m<sup>−3</sup></span> under an applied stress of 1.25 <span class="inline-formula">kPa</span>. Each experiment comprised five temperature steps from <span class="inline-formula">−6</span> to <span class="inline-formula">−18 °C</span>, each lasting one day, and resulted in a mean final vertical strain of 4 %. We show that the viscoplastic response is consistent with a two-regime Arrhenius law, with apparent activation energies <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>Q</mi><mi mathvariant="normal">h</mi></msub><mo>=</mo><mn mathvariant="normal">126</mn><mo>±</mo><mn mathvariant="normal">6</mn><mspace linebreak="nobreak" width="0.125em"/><mrow class="unit"><mi mathvariant="normal">kJ</mi><mspace width="0.125em" linebreak="nobreak"/><msup><mi mathvariant="normal">mol</mi><mrow><mo>-</mo><mn mathvariant="normal">1</mn></mrow></msup></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="105pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="9347851094efa5f860619beb6048635a"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="tc-20-5813-2026-ie00001.svg" width="105pt" height="16pt" src="tc-20-5813-2026-ie00001.png"/></svg:svg></span></span> for temperatures above <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">13</mn><mo>±</mo><mn mathvariant="normal">1</mn><mspace linebreak="nobreak" width="0.125em"/><mrow class="unit"><mi mathvariant="normal">°</mi><mi mathvariant="normal">C</mi></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="53pt" height="11pt" class="svg-formula" dspmath="mathimg" md5hash="7d644a564e61f416f8916e70c56675ae"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="tc-20-5813-2026-ie00002.svg" width="53pt" height="11pt" src="tc-20-5813-2026-ie00002.png"/></svg:svg></span></span> and <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>Q</mi><mi mathvariant="normal">l</mi></msub><mo>=</mo><mn mathvariant="normal">51</mn><mo>±</mo><mn mathvariant="normal">18</mn><mspace linebreak="nobreak" width="0.125em"/><mrow class="unit"><mi mathvariant="normal">kJ</mi><mspace linebreak="nobreak" width="0.125em"/><msup><mi mathvariant="normal">mol</mi><mrow><mo>-</mo><mn mathvariant="normal">1</mn></mrow></msup></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="102pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="5c0864c10a472b9ea2f90eda2d7a4b40"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="tc-20-5813-2026-ie00003.svg" width="102pt" height="16pt" src="tc-20-5813-2026-ie00003.png"/></svg:svg></span></span> below. This temperature sensitivity matches that reported for polycrystalline ice but is greater than that used in detailed snowpack models.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
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      <dc:identifier>https://doi.org/10.5194/tc-20-5813-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/5813/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:tc135206</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>tc</setSpec>
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      <dc:title><![CDATA[Interannual and seasonal evolution of supraglacial drainage systems on Nivlisen Ice Shelf, East Antarctica]]></dc:title>
      <dc:creator>Chen, Jiao</dc:creator>
      <dc:creator>Hodge, Rebecca A.</dc:creator>
      <dc:creator>Jamieson, Stewart S. R.</dc:creator>
      <dc:creator>Stokes, Chris R.</dc:creator>
      <dc:description><![CDATA[<p>Supraglacial drainage systems represent critical components of the surface hydrology on Antarctic ice shelves, facilitating the redistribution of meltwater, including into and out of supraglacial lakes, potentially influencing ice-shelf stability. However, the seasonal and interannual variability in their spatial extent, structural evolution, and climatic sensitivity remain poorly quantified, particularly compared to observations of supraglacial lakes. In this study, we investigate the interannual evolution of supraglacial drainage systems on Nivlisen Ice Shelf in East Antarctica between 2017 and 2024 using Sentinel-2 and Landsat-8 satellite imagery, with a detailed seasonal analysis during the 2018–2019 melt season. Key metrics including surface water area, total channel length, number of supraglacial drainage components, and the number of individual channels were derived to quantify the drainage evolution, system connectivity and complexity. We find significant interannual variability in the number of drainage components (from 34–186) and total channel length (from 345–1275 km), with peak length of channels observed in 2018. During the 2018–2019 melt season, channels progressively integrated and connected to form a very well-connected drainage system, which then fragmented towards the end of the melt season. We find that drainage systems are strongly influenced by ice shelf surface structures and undulations at a range of scales, with larger channels reforming in the same location. Correlation analysis shows that the evolution of drainage systems is tightly coupled to regional air temperature, with surface water extent and drainage connectivity strongly linked to reanalysis-based temperature outputs (<span class="inline-formula"><i>r</i>&gt;0.9</span>, <span class="inline-formula"><i>p</i>&lt;0.05</span>). Snow had variable effects, depending on its timing and how readily it could be melted. Our findings underscore the important dynamic nature of supraglacial channels in redistributing meltwater on Antarctic ice shelves.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
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      <dc:identifier>https://doi.org/10.5194/tc-20-5785-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/5785/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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    <identifier>oai:publications.copernicus.org:nhess137821</identifier>
    <datestamp>2026-10-12</datestamp>
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      <dc:title><![CDATA[Human-centred design approaches to tsunami mitigation under sea level rise in Kesennuma, Japan]]></dc:title>
      <dc:creator>Leggett, Hayley</dc:creator>
      <dc:creator>Farizi, Muhammad Daffa</dc:creator>
      <dc:creator>Purnama, Muhammad Rizki</dc:creator>
      <dc:creator>Suppasri, Anawat</dc:creator>
      <dc:creator>Imamura, Fumihiko</dc:creator>
      <dc:description><![CDATA[<p>Human-centred design (HCD) is increasingly prioritised as studies show human experience is critical in infrastructure use, and recent policies call for more socially responsive design. Tsunami impacts intensify as sea level rise (SLR) raises baseline water levels and reduces existing defence effectiveness. This study aims to develop and evaluate HCD-integrated multi-layered tsunami defences, assessing whether socially integrated designs can deliver effective protection under projected SLR conditions. Based on identified infrastructure preferences in Kesennuma City, Japan, we develop three multi-layered defence configurations: an environmentally integrated eco-hybrid system (Defence 1), a discreet open-feeling barrier system (Defence 2), and a reinforced high-performance system (Defence 3). Using TUNAMI-N2 numerical modelling, 150 simulations combine three tsunami sources, five SLR conditions, and five defence states. Results for inundation extent, fatality rates, and economic loss show a consistent hierarchy: Defence 3 achieves the strongest containment, while Defence 2, which more closely aligns with residents' preferences for openness and access, delivers near equivalent reductions typically within 10 %–15 %. Defence 1 provides only limited hazard reduction and is unsuitable as a standalone mitigation system. We show that HCD-integrated configurations can deliver strong technical performance and support a shift toward socially integrated, multi-layered tsunami protection under rising sea levels.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-4911-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/4911/2026/]]></dc:identifier>
      <dc:source>eISSN: 1684-9981</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147444</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</setSpec>
   </header>
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      <dc:title><![CDATA[Comparing Sentinel-2 Spectral Indices for Mapping Forest Fire Damage in Pollino National Park, Italy]]></dc:title>
      <dc:creator>Costanzo, Giuseppina</dc:creator>
      <dc:creator>Ferrara, Gianluigi</dc:creator>
      <dc:creator>Parente, Claudio</dc:creator>
      <dc:creator>Verde, Vincenzo</dc:creator>
      <dc:description><![CDATA[In recent years, climate change has significantly increased the severity and frequency of wildfires across Europe, with the 2025 season marking an unprecedented peak of one million hectares burned. Rapid and cost-effective mapping of these damaged areas is crucial for environmental recovery, making satellite remote sensing an indispensable tool. This study evaluates and compares the performance of four Sentinel-2 spectral burn indices for mapping forest fire damage within the Pollino National Park (Italy) occurred in September 2025, an area severely affected by the devastating summer fires of 2025. The analyzed indices include the Normalized Burn Ratio (NBR), Normalized Burn Ratio Plus (NBR+), Normalized Burn Ratio Short Wave Infrared (NBR-SWIR), and Normalized Difference Short Wave Infrared (ND-SWIR). An image differencing technique was applied to pre-fire (June 7, 2025) and post-fire (November 14, 2025) datasets, followed by a supervised Maximum Likelihood classification to map burned and unburned classes. Accuracy assessment via confusion matrices showed that NBR and NBR+ delivered the highest performance, achieving an Overall Accuracy (OA) of 0.976 and 0.974, respectively. ND-SWIR performed closely at 0.966, whereas NBR-SWIR yielded a lower OA of 0.873 due to the misclassification of bare soil transitions as burned areas. These findings highlight the critical role of specific SWIR-band combinations in optimizing automated wildfire monitoring systems.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-1-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/1/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147449</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</setSpec>
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      <dc:title><![CDATA[Mapping Fuel Categories in Mediterranean Regions with Sentinel-2 and PlanetScope Satellite Acquisitions]]></dc:title>
      <dc:creator>Filipponi, Federico</dc:creator>
      <dc:creator>Stroppiana, Daniela</dc:creator>
      <dc:creator>Rajabi, Forough</dc:creator>
      <dc:creator>Voltolina, Debora</dc:creator>
      <dc:creator>Arca, Bachisio</dc:creator>
      <dc:creator>Salis, Michele</dc:creator>
      <dc:creator>Zucca, Francesco</dc:creator>
      <dc:description><![CDATA[Accurate and spatially explicit mapping of forest fuel types is essential for developing integrated wildfire risk management strategies, estimating fire danger, and modeling fire propagation in fire-prone Mediterranean ecosystems. While time series of Copernicus Sentinel-2 multispectral imagery at 10 m spatial resolution have proven effective for regional fuel mapping, severe spectral and spatial ambiguities persist in distinguishing complex canopy structures, heterogeneous shrublands, and pastures. This study explores the synergistic integration of Sentinel-2 time series and high-resolution PlanetScope satellite acquisitions (3 m spatial resolution) to produce a 10 m fuel type map (9 classes) over a pilot area in Sardinia, Italy. A total of 114 features were synthesized, combining dynamic Sentinel-2 metrics (kNDVI, FAPAR, NDMI, ReNDVI harmonics), PlanetScope seasonal kNDVI zonal statistics and Gray-Level Co-occurrence Matrix (GLCM) textural features, and static terrain/canopy parameters. Using an XGBoost machine learning classifier trained on 245 photo-interpreted Regions of Interest (80/20 spatial split), three sets of features were compared. The combined model achieved a test overall accuracy of 74.46%, compared to 74.05% for Sentinel-2 alone and 74.66% for PlanetScope alone. Notably, incorporating PlanetScope textural features significantly improved classification metrics for dense canopy classes, increasing the F1-score of broadleaf evergreen trees and needleleaf evergreen trees. The PlanetScope GLCM kNDVI autumn entropy emerged as the most important feature overall. Conversely, PlanetScope performed poorly on the grass class. These findings highlight the critical trade-offs and high complementarity between fine spatial texture and broad spectral coverage for operational wildfire management.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-9-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/9/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147451</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</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[Development of an Explainable GeoAI Wildfire Risk Analysis Model Using Multi-Source Geospatial Data]]></dc:title>
      <dc:creator>Günaydın, Esra</dc:creator>
      <dc:creator>Mete, Muhammed Oğuzhan</dc:creator>
      <dc:creator>Küçük, Furkan Ali</dc:creator>
      <dc:creator>Hafızoğlu, Ayça</dc:creator>
      <dc:creator>Selbesoğlu, Mahmut Oğuz</dc:creator>
      <dc:description><![CDATA[Accounting for approximately 31% of the global land surface, forests play a critical and indispensable role in sustaining ecological balance. Among the various pressures affecting forests, forest fires constitute a major environmental problem, posing significant threats to natural ecosystems while disrupting forestry activities and leading to substantial economic losses. In T&uuml;rkiye, forest fires are predominantly observed in the Aegean, Mediterranean, and Marmara regions. This study presents a proactive, explainable GeoAI framework for wildfire risk analysis by integrating multi-source geospatial data. The methodology calculates a physical hazard index by evaluating advanced ensemble machine learning algorithm, specifically extreme gradient boosting (XGBoost) with the latter demonstrating superior predictive performance. The model is driven by topographic, meteorological, biotic and anthropogenic parameters. In parallel, a comprehensive vulnerability matrix encompassing physical, social, economic and environmental dimensions is constructed utilizing the Best-Worst Method (BWM). These two main components are spatially synthesized in a Geographic Information Systems (GIS) environment. The model's interpretability is enhanced focusing on feature importance to identify the primary drivers of fire ignition and spread. Results demonstrate that anthropogenic pressures and Wildland-Urban Interface (WUI) dynamics are the most significant risk determinants. The resulting high-resolution maps provide a robust Spatial Decision Support System (SDSS) for local authorities, enabling targeted mitigation strategies and contributing to the development of sustainable, smart and resilient cities.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-17-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/17/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147457</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</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[Meteosat Third Generation active fire detection multi-temporal algorithm]]></dc:title>
      <dc:creator>Kamoun, Ines</dc:creator>
      <dc:creator>Hessel, Charles</dc:creator>
      <dc:creator>Nenes, Athanasios</dc:creator>
      <dc:description><![CDATA[Fire detection and monitoring are essential for mitigating the environmental and societal impacts of wildfire events. Earth Observation (EO) satellites have long played a central role in this domain, with polar-orbiting sensors such as MODIS and VIIRS providing global fire detections twice daily. However, their limited revisit frequency constrains the timeliness of fire alerts. Geostationary satellites, by contrast, offer high temporal resolution through multiple scans per hour, enabling near-real-time fire detection and rapid alerting. Despite this advantage, fire detection algorithms applied to geostationary imagery have predominantly relied on single-timestamp processing, limiting their ability to exploit the full temporal frequency of these observations. In this paper, we propose a multi-temporal approach for active fire detection using data from the Meteosat Third Generation (MTG) Flexible Combined Imager (FCI). The method first applies multi-temporal cloud masking based on the 10.5 &mu;m thermal infrared band, before implementing a multi-temporal fire detection algorithm inspired by the Robust Satellite Techniques (RST) methodology of (Filizzola et al., 2017). To improve detection reliability, a pixel is confirmed as an active fire only after repeated detection across successive timestamps. Compared to the operational single-timestamp MTG FRP-pixel product, the multi-temporal algorithm achieves higher recall with a slight reduction in precision. Additionally, the method demonstrates sensitivity to regional land-use characteristics, excluding persistent industrial heat sources and continuous gas flaring from fire detections. Finally, the algorithm retrieves Fire Radiative Power (FRP) estimates with associated uncertainty bounds, yielding an average uncertainty window of approximately 4.5 MW.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-25-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/25/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147458</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</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[A Modular, Cloud-Based GIS Platform for Automated Wildfire Risk Index Mapping]]></dc:title>
      <dc:creator>Ortega-Hita, Raquel</dc:creator>
      <dc:creator>Khan, Asim</dc:creator>
      <dc:creator>Gallego-Llopis, Mateo</dc:creator>
      <dc:creator>Valdes, Javier</dc:creator>
      <dc:creator>Weber, Andreas</dc:creator>
      <dc:creator>Miranda, Ricardo</dc:creator>
      <dc:creator>Papanikolaou, Ioannis</dc:creator>
      <dc:creator>Veiga-López, Fernando</dc:creator>
      <dc:description><![CDATA[Wildfires are a growing environmental and socio-economic threat driven by climate change and land abandonment. As fire frequency and intensity increase, suppression alone is no longer sufficient, making prevention and preparedness essential. Earth Observation and Geographic Information Systems (GIS) enable the integration of environmental and socio-economic factors into decision-support tools for wildfire risk assessment. This work presents a modular, web-based platform that computes a Wildfire Risk Index (WRI) through multi-criteria analysis and the Analytic Hierarchy Process (AHP). Two complementary risk formulations are developed for Galicia, northwestern Spain: a Static WRI, aimed at characterising baseline wildfire predisposition and supporting long-term prevention planning, and a Dynamic WRI, which incorporates short-term changes in vegetation and meteorological conditions to support operational preparedness. The Static WRI prioritises socio-economic factors (43.6%), while the Dynamic WRI gives greater weight to vegetation (45.6%) and meteorology (30.3%). The resulting maps show distinct spatial risk distributions, reflecting their different purposes. Validation of the dynamic model against MODIS active-fire detections yielded AUC-ROC values between 0.4935 and 0.8333, with six of eight validation periods exceeding 0.5. Both indices are integrated into a cloud-based Wildfire App, enabling automated risk calculation, visualisation, and updating through an interactive GIS dashboard. The results demonstrate the potential of combining static and dynamic WRI approaches to support complementary wildfire prevention and preparedness decisions.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-33-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/33/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147460</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</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[Biomass Prediction Combining Radar, Multispectral and Field Inventory Data]]></dc:title>
      <dc:creator>Pereira-Pires, João E.</dc:creator>
      <dc:creator>Guerra-Hernández, Juan</dc:creator>
      <dc:creator>Anil-Lathika, Amal</dc:creator>
      <dc:creator>Saarela, Svetlana</dc:creator>
      <dc:creator>Silva, João M. N.</dc:creator>
      <dc:creator>Fonseca, José M.</dc:creator>
      <dc:creator>Mora, André</dc:creator>
      <dc:description><![CDATA[Information on forest biomass is crucial for a better management and understanding of wildfires effects (pre- and post-fire analyses), as well as for a more accurate monitoring of carbon cycle dynamics. The current literature adopts two main approaches for the retrieving of biomass values: 1) predicting the biomass through allometric equations based on field measurements or Airborne Laser Scanning (ALS) metrics; and 2) using machine learning models based on spaceborne data sources (radar, optical, and laser), trained with field or ALS data. While approach 1) is usually spatially limited and has high costs; approach 2) mostly focuses on the Aboveground Biomass Density (AGBD) (i.e.: leaves, branches, trunk), disregarding the other components of the forest ecosystems as root biomass (BGBD), litter biomass (LBD) and shrubs biomass (SBD)) which leads to biomass underestimation.</p> <p>This article proposes a novel methodology capable of producing accurate predictions of the four previously mentioned biomass components, that integrates multi-source remote sensing observations acquired by synthetic aperture radars (ALOS-2 and Sentinel- 1), multispectral sensors (Sentinel-2), and ancillary data (on topography and land cover). The methodology resorts to an extreme gradient boosting regressor trained with field inventory data for the AGBD and BGBD, and ALS data for the LBD and SBD. It was demonstrated the importance of including all the proposed datasets and that reliable predictions were achieved. Namely, %RMSEs of 63.29%, 62.90%, 41.07%, 28.34% were achieved for the AGBD, BGBD, LBD, and SBD, respectively.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-41-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/41/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147462</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</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[Improving on the spatial location of geostationary satellite-derived FRP by accounting for parallax effect]]></dc:title>
      <dc:creator>Ponte Lira, Cristina</dc:creator>
      <dc:creator>Dutra, Emanuel</dc:creator>
      <dc:creator>Xu, Weidong</dc:creator>
      <dc:creator>Wooster, Martin</dc:creator>
      <dc:creator>Trigo, Isabel</dc:creator>
      <dc:description><![CDATA[When a satellite observes the Earth at an angle, the apparent position of elevated features, such as mountains, clouds or fires in high terrain, can be shifted from their true ground location. This effect, which may be particularly pronounced in the case of geostationary platforms providing observations under systematically high viewing angles in many places, is known as parallax displacement and becomes larger as terrain elevation and satellite viewing angle increase.<br />Meteosat satellites operated by EUMETSAT provide frequent near-real-time observations that are essential for wildfire detection and monitoring. The new Meteosat Third Generation (MTG) satellites, equipped with the Flexible Combined Imager (FCI), offer improved spatial, temporal and spectral capabilities compared with previous systems. These improvements support better detection and tracking of active fires.<br />The LSA SAF Fire Radiative Power product (FRP-PIXEL) provides information on the location, timing and radiative energy of active fires, which can be used as an indicator of fire intensity and biomass consumption. However, standard geostationary processing assumes that observed features are located at sea level. As a result, fires occurring in elevated terrain may be incorrectly geolocated due to parallax displacement.<br />This work presents an updated MTG FRP-PIXEL product that includes both the original fire and terrain-corrected coordinates. The correction aims to improve the spatial accuracy of active-fire locations, especially in mountainous regions. Preliminary comparisons with active-fire information derived from high-resolution Sentinel-2 imagery show that the correction can improve the location of FRP detections over high-elevation terrain.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-49-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/49/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:isprs-archives147465</identifier>
    <datestamp>2026-10-08</datestamp>
    <setSpec>isprs-archives</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[Wildfire Dynamics on the Kinburn Peninsula, Ukraine, Using Sentinel-1 SAR and Optical Data (2022–2025)]]></dc:title>
      <dc:creator>Shevchuk, Yuliia</dc:creator>
      <dc:creator>Davydov, Oleksiy</dc:creator>
      <dc:creator>Bevainis, Linas</dc:creator>
      <dc:creator>Kasianov, Yevhenii</dc:creator>
      <dc:description><![CDATA[Since 2022, the Kinburn Peninsula, Ukraine, has been located within an active war zone, where frequent and recurrent wildfires have affected heterogeneous coastal sandy ecosystems. Burned-area mapping in this landscape is complicated by wetlands, salt flats, exposed sands, reedbeds, artificial pine plantations, cloud cover, smoke and restricted field access. This study applies an integrated multi-sensor approach to map wildfire damage and recurrence during 2022&ndash;2025 using Sentinel-1 SAR, Sentinel-2 and Landsat 8/9 optical imagery, NASA FIRMS thermal anomalies and official fire-monitoring materials. Optical burn indicators were used to identify spectral evidence of burning, while Sentinel-1 VV/VH backscatter changes and Radar Forest Degradation Index (RFDI) were used to detect structural vegetation degradation. Optical burn candidate masks and SAR-derived structural damage masks were spatially overlaid to delineate confirmed fire-damage areas. The results show that wildfire impact was spatially recurrent rather than isolated. SAR-derived candidate areas increased from 637.06 ha in 2022 to 4297.97 ha in 2025, while mean &Delta;VH remained consistently negative, indicating reduced vegetation volume scattering. The largest confirmed optical&ndash;SAR fire-damage area was detected in 2025, reaching 598.26 ha. Fire recurrence mapping revealed zones of accumulated pyrogenic stress, particularly within artificial forest plantations, psammophytic steppe complexes and protected coastal ecosystems. The proposed optical&ndash;SAR framework improves wildfire damage mapping under wartime and data-limited conditions.]]></dc:description>
      <dc:date>2026-10-08</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/isprs-archives-XLVIII-M-13-2026-57-2026</dc:identifier>
      <dc:identifier><![CDATA[https://isprs-archives.copernicus.org/articles/XLVIII-M-13-2026/57/2026/]]></dc:identifier>
      <dc:source>eISSN: 2194-9034</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:msd146795</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>msd</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[Structural Characterization of Excavator Working Device Based on Measured Digging Trajectories and Different Working Loads]]></dc:title>
      <dc:creator>Zhang, Yijian</dc:creator>
      <dc:creator>Ren, Zhigui</dc:creator>
      <dc:creator>Cao, Shusheng</dc:creator>
      <dc:creator>Lv, Liang</dc:creator>
      <dc:creator>Pang, Xiaoping</dc:creator>
      <dc:creator>Ren, Kaitao</dc:creator>
      <dc:creator>Zhang, Heng</dc:creator>
      <dc:description><![CDATA[This study investigates the effects of different load characterization methods on the structural response of a 20-ton backhoe excavator working device under compound digging conditions. Based on field measured data, four typical compound digging trajectories were adopted, and the critical postures with peak cutting-loading resistance were selected for high-load analysis. A dynamic model of the working device was established via D&rsquo;Alembert&rsquo;s principle. Under identical postures and boundary conditions, three load schemes, namely measured excavation resistance, conventional compound digging force, and limit compound digging force, were applied to calculate structural loads on the boom and stick. Corresponding parametric finite element models were developed to compare structural equivalent stress and deformation. The results demonstrate that different load representations yield similar high-stress distributions and overall deformation modes for both components. The limit compound digging force produces higher maximum equivalent stress than the other two load schemes, providing a conservative evaluation for structural strength. Under the limiting load condition, the boom exhibits significantly increased deformation, while stick deformation presents non-monotonic variation due to the combined effects of load direction and working posture. This work can support design load selection and structural optimization for excavator working devices under compound digging operations.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/ms-2026-174</dc:identifier>
      <dc:identifier><![CDATA[https://ms.copernicus.org/preprints/ms-2026-174/]]></dc:identifier>
      <dc:source>eISSN: 2191-916X</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:lsd146499</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>lsd</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[Land-use change impacts on multidimensional well-being: insights from tropical forest frontiers in Madagascar, Myanmar and Laos]]></dc:title>
      <dc:creator>Zaehringer, Julie G.</dc:creator>
      <dc:creator>Diebold, Clara L.</dc:creator>
      <dc:creator>Michelotti, Madlaina</dc:creator>
      <dc:creator>Llopis, Jorge C.</dc:creator>
      <dc:creator>Nydegger, Katharina</dc:creator>
      <dc:creator>Aung Myin Htun</dc:creator>
      <dc:creator>Stenger, Nicolas</dc:creator>
      <dc:creator>Kommadam, Souliyaphon</dc:creator>
      <dc:creator>Harimalala, Paul-Clément</dc:creator>
      <dc:creator>Feurer, Mélanie</dc:creator>
      <dc:creator>Latthachack, Phokham</dc:creator>
      <dc:creator>Lundsgaard-Hansen, Lara</dc:creator>
      <dc:creator>Andriatsitohaina, Ntsiva</dc:creator>
      <dc:creator>Messerli, Peter</dc:creator>
      <dc:creator>Schneider, Flurina</dc:creator>
      <dc:description><![CDATA[Tropical forest frontiers are undergoing rapid land use change due to expanding global demands for agricultural commodities and conservation efforts. These changes profoundly affect the well-being of local populations, yet the pathways linking land use, ecosystem services, and well-being remain underexplored. This study examines these links across three forest frontier landscapes in Madagascar, Laos, and Myanmar. Using Nussbaum&rsquo;s capabilities framework, we conducted 14 workshops and 154 household interviews to assess how land use change influences diverse well-being components via ecosystem services.</p> <p>We identify three key findings. First, land use change impacts well-being both directly and indirectly via shifts in ecosystem service supply. Forests provide the broadest range of services that support essential components of well-being, including nutrition, income, housing, and spiritual values. Second, we find three generic mechanisms through which well-being is affected, often involving trade-offs within or between well-being components. For example, gains in income can coincide with losses in cultural identity or environmental quality. Third, we identify three substitution processes that can mitigate ecosystem service loss&rsquo; impact on well-being. However, these processes often fail to maintain relational and collective components of well-being and it might be that ecosystem services are often not substituted to the same level.</p> <p>Our findings highlight the need for a multidimensional, context-sensitive understanding of well-being in land system science. Development and conservation interventions should move beyond narrow economic framings and support multifunctional landscapes that sustain both ecosystem services and the full spectrum of human well-being in tropical forest frontiers.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/ls-2026-8</dc:identifier>
      <dc:identifier><![CDATA[https://ls.copernicus.org/preprints/ls-2026-8/]]></dc:identifier>
      <dc:source>eISSN: 3056-3666</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:lsd146563</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>lsd</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[Conditions for an effective EU regulation on deforestation-free products: Where will it likely reduce deforestation?]]></dc:title>
      <dc:creator>Coenen, Johanna</dc:creator>
      <dc:creator>Persson, U. Martin</dc:creator>
      <dc:creator>Angelsen, Arild</dc:creator>
      <dc:creator>Bastos Lima, Mairon</dc:creator>
      <dc:creator>Berning, Laila</dc:creator>
      <dc:creator>Kastner, Thomas</dc:creator>
      <dc:creator>Schulz, Dario</dc:creator>
      <dc:creator>Sotirov, Metodi</dc:creator>
      <dc:creator>Wunder, Sven</dc:creator>
      <dc:description><![CDATA[In 2023, the European Union (EU) adopted the Regulation on Deforestation-free Products (EUDR) to curb deforestation and forest degradation linked to its agricultural and wood trade. While existing research has outlined how the regulation is expected to work when implemented from 2027, we still have a weak understanding of how these mechanisms are likely to play out across different country and commodity contexts. This study focuses on the conditions under which different outcomes emerge, encompassing both intended impacts and potential spillover effects. We highlight that the regulation is likely to produce heterogeneous, context-dependent outcomes in reducing future deforestation across commodities and countries, with EU market shares and associated deforestation embodied in EU trade being key conditions. Evaluated in absolute terms, the EUDR may not substantially reduce global deforestation or emissions, but it could be effective in certain contexts. Our results suggest that high EU market shares (e.g., cocoa, coffee) offer leverage, while low market shares (e.g., soy, palm oil) increase risks of market segregation and negative spillovers. The EUDR&rsquo;s most significant source of leverage likely stems from its broader influence on forest and supply-chain governance among multinational companies and non-EU countries. Achieving this wider impact requires coordinated collaboration with both producer and other consumer countries.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/ls-2026-10</dc:identifier>
      <dc:identifier><![CDATA[https://ls.copernicus.org/preprints/ls-2026-10/]]></dc:identifier>
      <dc:source>eISSN: 3056-3666</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:jecatsd147210</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>jecatsd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Influence of aircraft-induced dilution dynamics on near-field ice crystal formation]]></dc:title>
      <dc:creator>Vals, Margaux</dc:creator>
      <dc:creator>Annunziata, Rémy</dc:creator>
      <dc:creator>Bonne, Nicolas</dc:creator>
      <dc:description><![CDATA[The influence of aircraft-geometry-induced dynamics on ice crystal formation in contrails is investigated using a detailed 1D microphysics code combined with results from several 3D CFD simulations. Two configurations are considered: one including a complete aircraft geometry and another with an engine alone. For each configuration, two ambient temperatures and two combustion modes are considered, corresponding to soot-poor and soot-rich regimes. These simulations are used to determine the temperature and dilution profiles within the plume, which are then applied to the 1D microphysics code MoMiE. This code represents the various processes of ice crystal formation, notably ice nucleation from volatile particles and from hydrated soot particles. The results show that aircraft-geometry-induced dilution and temperature changes directly impact ice crystal formation, in particular ice particle concentration, number, and size. The difference observed between the engine-only configuration and the complete aircraft geometry is less than 10% for the number of ice crystals per meter of flight in the soot-poor regime, whereas it ranges from less than 1% to 21% in the soot-rich regime. Comparison with results obtained using Schumann&rsquo;s analytical dilution law, commonly used to represent dilution in 1D box models, also shows significant differences. In the soot-poor regime, the CFD-based dilution leads to a 35% underestimation of the ice crystal number relative to Schumann&rsquo;s law at high ambient temperatures, whereas it leads to a 118% overestimation at colder ones. Given that ice crystal number, concentration, and size are key parameters for determining the radiative impact of contrails, these results highlight the importance of the aircraft dynamics in ice crystal formation, but also the need for further study into the role of the dilution process in estimating contrail properties.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/jecats-2026-19</dc:identifier>
      <dc:identifier><![CDATA[https://jecats.copernicus.org/preprints/jecats-2026-19/]]></dc:identifier>
      <dc:source>eISSN: 3053-9277</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd142437</identifier>
    <datestamp>2026-10-12</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[Evaluating the EPICC-Model for regional air quality simulation: a comparative study with CAMx and CMAQ]]></dc:title>
      <dc:creator>Lou, Mengjie</dc:creator>
      <dc:creator>Wu, Qizhong</dc:creator>
      <dc:creator>Wang, Wending</dc:creator>
      <dc:creator>Chen, Huansheng</dc:creator>
      <dc:creator>Cao, Kai</dc:creator>
      <dc:creator>Fan, Xiaohan</dc:creator>
      <dc:creator>Liang, Dingyue</dc:creator>
      <dc:creator>Yu, Fenfen</dc:creator>
      <dc:creator>Zhang, Jiating</dc:creator>
      <dc:creator>Wang, Wei</dc:creator>
      <dc:creator>Wang, Zifa</dc:creator>
      <dc:description><![CDATA[<p>This study presents a systematic evaluation of the EPICC-Model developed in China for regional <span class="inline-formula">PM<sub>2.5</sub></span> and MDA8 <span class="inline-formula">O<sub>3</sub></span> simulations against established international models, using WRF meteorological fields and a multi-source integrated emission inventory. Results highlight the strengths of the EPICC-Model in several aspects: it achieves relatively high spatial consistency with measurements for <span class="inline-formula">PM<sub>2.5</sub></span>, with an annual index of agreement (IOA) of 0.80, and accurately captures pollution patterns in heavily polluted North China. It also demonstrates improved performance in simulating summer <span class="inline-formula">O<sub>3</sub></span> peaks, reducing maximum bias by more than 20 <span class="inline-formula">µg m<sup>−3</sup></span>; this performance may be partly associated with its inclusion of heterogeneous HONO formation and particulate nitrate photolysis. The model exhibits the highest hit rate (45.6 <span class="inline-formula">%</span>) for MDA8 <span class="inline-formula">O<sub>3</sub></span> pollution events exceeding 160 <span class="inline-formula">µg m<sup>−3</sup></span> and successfully reproduces persistent pollution episodes. However, all models share common limitations, including insufficient capability in reproducing heavy pollution episodes, systematic underestimation of <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">SO</mi><mn mathvariant="normal">4</mn><mrow><mn mathvariant="normal">2</mn><mo>-</mo></mrow></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="29pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="06a1e144313624090049b6627390d3e8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gmd-19-9651-2026-ie00001.svg" width="29pt" height="17pt" src="gmd-19-9651-2026-ie00001.png"/></svg:svg></span></span>, and uncertainties in SOA-related OC simulations. Future improvements should focus on refining secondary aerosol chemistry and emission inventories and further evaluating the representation of vertical turbulent mixing under stable boundary-layer conditions. This study benchmarks the performance of the EPICC-Model against established chemical transport models (CTMs) and identifies priorities for its further development and regional application.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9651-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9651/2026/]]></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:gmd139742</identifier>
    <datestamp>2026-10-12</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[Towards high-fidelity simulations of coastal submesoscale  baroclinic instabilities with MPAS–O (vE3SM3.0.0)  – Part 2: Realistic experiments]]></dc:title>
      <dc:creator>Schlichting, Dylan R.</dc:creator>
      <dc:creator>Smith, Katherine M.</dc:creator>
      <dc:creator>Petersen, Mark R.</dc:creator>
      <dc:creator>Hetland, Robert D.</dc:creator>
      <dc:creator>Hinson, Kyle E.</dc:creator>
      <dc:creator>Engwirda, Darren</dc:creator>
      <dc:description><![CDATA[<p>River plumes can strongly influence coastal dynamics but are poorly represented in global ocean models due to stringent resolution requirements. Following the idealized simulations presented in a companion paper (Hinson et al., 2026), this study presents submesoscale-permitting realistic simulations using unprecedented regional refinement with MPAS–O. We assess MPAS–O's ability to represent river plume dynamics by comparing with a validated ROMS configuration focused on the Mississippi–Atchafalaya (M–A) plume in the northern Gulf of Mexico (GoM). The variable-resolution mesh spans 1.4 km in the GoM to 100 km in the Pacific and Indian Oceans. We incorporate several improvements to the representation of river forcing in MPAS–O: the pseudo point source treatment of runoff, river temperature prescribed from air temperature, and passive tracers to track freshwater transport. MPAS–O generates vigorous submesoscales in the open GoM, as quantified by probability density functions of surface relative vorticity and divergence. While the model qualitatively captures the M–A plume's seasonal evolution, it does not realistically reproduce the summer submesoscale eddy field on the Texas–Louisiana shelf. A persistent brackish lens associated with reduced vertical mixing forms and is present throughout the M–A plume. We hypothesize that this arises from interacting parameterization and structural design choices within MPAS–O that affect plume stratification and instability growth under realistic forcing, rather than from deficiencies in numerics. Our results demonstrate MPAS–O's potential for simulating submesoscale processes in the open ocean while highlighting challenges in using regional refinement to model coastal dynamics.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9627-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9627/2026/]]></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:gmd138889</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Process-based evaluation of green roof models for assessment of heat mitigation efficacy in WRF (v4.3.1) and EnergyPlus (v8.6.0)]]></dc:title>
      <dc:creator>Martinez Mendoza, Maria</dc:creator>
      <dc:creator>Saeedi, Alireza</dc:creator>
      <dc:creator>Voogt, James A.</dc:creator>
      <dc:creator>Krayenhoff, E. Scott</dc:creator>
      <dc:description><![CDATA[<p>Green roofs mitigate urban heat, but to fully assess their impact, green roof models must be integrated into urban climate models, where they provide critical surface boundary conditions. Ensuring their reliability requires evaluation, yet such efforts remain limited in the literature. This study addresses that gap by evaluating two configurations of EcoRoof, the green roof module from EnergyPlus (ER<span class="inline-formula"><sub>o</sub></span> for the original version of the model, and ER<span class="inline-formula"><sub>m</sub></span> for a modified version), and a multilayer green roof parametrization for WRF (WRF-MLGR) (Heusinger et al., 2018; Sailor, 2008; Zonato et al., 2021). These models were tested against field observations from a monitored green roof in London, Ontario, focusing on latent heat flux (<span class="inline-formula"><i>Q</i><sub>e</sub></span>), surface temperature (<span class="inline-formula"><i>T</i><sub>surf</sub></span>), soil heat flux (<span class="inline-formula"><i>Q</i><sub>g</sub></span>) and substrate water content (SWC). Model performance varied by variable. The two EcoRoof versions showed similar performance, with mean RMSE across study periods of approximately 56–60 W m<span class="inline-formula"><sup>−2</sup></span> for <span class="inline-formula"><i>Q</i><sub>e</sub></span>, 3–4 °C for <span class="inline-formula"><i>T</i><sub>surf</sub></span>, 22 W m<span class="inline-formula"><sup>−2</sup></span> for <span class="inline-formula"><i>Q</i><sub>g</sub></span>, and 0.03 m<span class="inline-formula"><sup>3</sup></span> m<span class="inline-formula"><sup>−3</sup></span> for SWC. Performance for <span class="inline-formula"><i>Q</i><sub>e</sub></span> was comparable across models; however, WRF-MLGR exhibited much larger errors for <span class="inline-formula"><i>Q</i><sub>g</sub></span> (with mean RMSE exceeding 100 W m<span class="inline-formula"><sup>−2</sup></span>) and SWC (0.06 m<span class="inline-formula"><sup>3</sup></span> m<span class="inline-formula"><sup>−3</sup></span>), along with higher <span class="inline-formula"><i>T</i><sub>surf</sub></span> deviations (<span class="inline-formula">∼5</span> °C). Overall, EcoRoof provided a more consistent representation of the daytime energy balance, whereas WRF-MLGR showed structural biases in surface heating. These findings highlight the importance of process-level evaluation for urban climate applications and underscore the need for continued model development to address the structural limitations in green roof parametrizations.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9729-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9729/2026/]]></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:gmd138036</identifier>
    <datestamp>2026-10-12</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[Improving the CLASSIC (v1.8) snow model  to better simulate Arctic snowpacks]]></dc:title>
      <dc:creator>Lalande, Mickaël</dc:creator>
      <dc:creator>Roy, Alexandre</dc:creator>
      <dc:creator>Wang, Libo</dc:creator>
      <dc:creator>Verseghy, Diana</dc:creator>
      <dc:creator>Vionnet, Vincent</dc:creator>
      <dc:creator>Dominé, Florent</dc:creator>
      <dc:creator>Kinnard, Christophe</dc:creator>
      <dc:description><![CDATA[<p>This study enhances the snow model of the Canadian Land Surface Scheme including Biogeochemical Cycles (CLASSIC), with a particular focus on Arctic environments. Key snow model physics improvements include adjustments to the thermal conductivity at the top of the first soil layer, a revised computation of the temperature at the snow–soil interface (hereafter, bottom snow temperature), and the addition of a windless exchange coefficient in sensible heat flux calculations. Arctic-specific adaptations include blowing-snow sublimation losses, a new snow compaction scheme, and snow thermal conductivity parameterization. Evaluations at seven mid-latitude and alpine sites (SnowMIP sites) and three Arctic sites (Bylot Island, Umiujaq, and Trail Valley Creek) show that these enhancements improve the overall simulated snowpack characteristics and soil temperatures across both SnowMIP and Arctic sites. The revised bottom snow temperature yields better agreement between simulated and observed snow and bottom snow temperatures. The new windless exchange coefficient reduced the surface temperature RMSE from 3.50 to 1.93 °C on average across all sites. The improved snow compaction scheme reduces the snow depth biases from 12.0 to 0.1 cm on average across the Arctic sites and improves the simulated snow densities while not degrading the overall model performance at the SnowMIP sites. Blowing-snow sublimation had a negligible effect at most sites, except at the wind-exposed sites of Umiujaq, Trail Valley Creek, and Senator Beck, decreasing snow depth on average by 2–4 cm. Adding a new snow thermal conductivity parameterization – combined with all previous developments – reduces the RMSE of the simulated soil temperatures from 5.3 to 3.0 °C on average at all Arctic sites. Our new developments demonstrate the ability of a single-layer snow model to reasonably reproduce Arctic bulk snowpack characteristics, while maintaining good performance at the SnowMIP sites. Inherent uncertainties remain in the forcing datasets, especially due to the harsh Arctic environment characterized by strong winds, snow redistribution, frost, and polar night. Future model developments will focus on spatial-scale simulations across the whole Arctic, with particular attention to snow cover fraction parameterizations to better capture sub-grid-scale spatial heterogeneity in Arctic environments.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9581-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9581/2026/]]></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:gmd136820</identifier>
    <datestamp>2026-10-12</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[EnviFlux (v1.0): a simplified surface flux inversion tool based on four-dimensional variational data assimilation (4D-Var)]]></dc:title>
      <dc:creator>Bannister, Ross N.</dc:creator>
      <dc:description><![CDATA[<p>This paper introduces EnviFlux, which is a software tool (written in C++) to study the inverse problem of estimating the distribution of fluxes of a trace gas globally at the Earth's surface. This is done using a four-dimensional variational technique, which combines information from (i) synthetic observations of the trace gas spanning a defined time window, (ii) a transport model linking the initial concentration and surface fluxes to predictions of the observations, and (iii) a priori information. The novelty of this system – compared to those that attempt to solve for real data – is in its relative simplicity and low cost, allowing new ideas to be assessed and understood quickly and cheaply. This is in line with many other developments in data assimilation that are often first explored using so-called “toy” systems. Part of this paper is to document this system, which is sufficiently complex to allow assimilation of in situ and total column amount (TCA) observation in arbitrary configurations, and has a flexible background error covariance model, but is simple enough to be run relatively quickly.</p>        <p>Another part of this paper uses EnviFlux to explore the effect of model error and observation bias on inferred surface fluxes in two example scenarios and with two observation types, namely surface in situ (SIS) and TCA. The first is a highly idealised case with a flux pair (a localised source and a localised sink), where no a priori information concerning their positions is provided. It is found that model errors in the assimilation can severely affect the inferred flux positions and amounts, but observation biases do not affect the positions, but do affect the amounts. The second scenario is closer to a real-world example of methane flux estimates where an a priori is refined with observations. The effect of model error is less than for the first scenario, but is still evident, and the observation biases affect the flux amounts. In both cases, the SIS observations allow a more accurate estimate of surface flux characteristics than the TCA observations, even though the experiments are setup to allow a fair comparison of the two. The last part of the paper raises some research questions that EnviFlux could help address.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9751-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9751/2026/]]></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:gmd129338</identifier>
    <datestamp>2026-10-12</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[MONKI: a three-dimensional Monte Carlo simulator for transfer of polarised light in planetary atmospheres]]></dc:title>
      <dc:creator>Trees, Victor J. H.</dc:creator>
      <dc:creator>Wang, Ping</dc:creator>
      <dc:creator>Wiltink, Job I.</dc:creator>
      <dc:creator>Stammes, Piet</dc:creator>
      <dc:creator>Stam, Daphne M.</dc:creator>
      <dc:creator>Donovan, David P.</dc:creator>
      <dc:creator>Siebesma, A. Pier</dc:creator>
      <dc:description><![CDATA[<p>Spectropolarimetry is a powerful tool for characterising planetary atmospheres and surfaces. For the design and operation of spectro(polari)metric instrumentation, numerically simulated signals of the measured radiation are essential. We present MONKI (Monte Carlo KNMI), an efficient and accurate Monte Carlo radiative transfer code written in Fortran. MONKI computes total, linearly polarised, and circularly polarised radiances reflected by and transmitted through planetary atmospheres, fully accounting for the polarisation of light in all orders of scattering. Unlike classical Monte Carlo approaches that rely on post-sampling weight corrections and can therefore produce rare but disproportionately large photon weights, MONKI samples scattering directions from the full polarisation-dependent distribution, consistently in both forward and backward Monte Carlo modes. We provide the corresponding theoretical framework in the appendices. Because of this exact polarised sampling approach, the code converges robustly for optically thick and/or strongly polarising atmospheres. MONKI can handle horizontally homogeneous atmospheres as well as atmospheres with horizontal inhomogeneities, such as three-dimensional (3D) patchy clouds. We validate MONKI through comparisons with other radiative transfer codes. Finally, we present sample simulations of sunlight reflected by the Earth and Venus, and explain the total and polarised radiance features by analysing the altitudes at which photons are scattered. We conclude that MONKI is a versatile and accurate tool for simulations and detailed analyses of total and polarised light emerging from the atmospheres of the Earth, Venus, and, in principle, any other planet.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-9677-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/9677/2026/]]></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:gi138561</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>gi</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[THEMIS: spin axis magnetic field reconstruction]]></dc:title>
      <dc:creator>Pöppelwerth, Adrian</dc:creator>
      <dc:creator>Auster, Hans-Ulrich</dc:creator>
      <dc:creator>Angelopoulos, Vassilis</dc:creator>
      <dc:creator>McTiernan, James M.</dc:creator>
      <dc:creator>Lewis, James W.</dc:creator>
      <dc:creator>Plaschke, Ferdinand</dc:creator>
      <dc:description><![CDATA[<p>The Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission investigates the coupling between the solar wind and Earth's magnetosphere using five identical spinning spacecraft. Each spacecraft rotates at a predefined rate to stabilize it and carries a suite of instruments, including a fluxgate magnetometer (FGM) that measures the three-dimensional magnetic field. Since 24 May 2024, the FGM on board THEMIS E has no longer recorded the magnetic field component along the spin axis, while the two components approximately within the spin plane remain fully available.</p>        <p>We present a method to reconstruct the missing magnetic field component using data from these two remaining components together with the spacecraft spin, yielding full three-component magnetic field vectors at spin period cadence and with an effective bandwidth of <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">60</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="27pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="7302c95ca190da66fd7d9a88fe97d775"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gi-15-273-2026-ie00001.svg" width="27pt" height="14pt" src="gi-15-273-2026-ie00001.png"/></svg:svg></span></span> <span class="inline-formula">Hz</span>. The approach was validated using original THEMIS E data from 2017 to 2020, when all three sensor components were available. We further estimated the reconstruction noise floor, indicating that the method is unlikely to be limited by sensor noise. These results demonstrate that on a spinning spacecraft, two components whose sensor axes lie close to, but not exactly in, the spin plane are sufficient to reconstruct three-dimensional magnetic field vectors, allowing continued magnetospheric observations despite the loss of one sensor component.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gi-15-273-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gi.copernicus.org/articles/15/273/2026/]]></dc:identifier>
      <dc:source>eISSN: 2193-0864</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gh133015</identifier>
    <datestamp>2026-10-12</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/"
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      <dc:title><![CDATA[Verkehrs- und Mobilitätsgerechtigkeit als theoretisch-konzeptionelle Grundlage  für die Analyse von Erreichbarkeiten]]></dc:title>
      <dc:creator>Ahlmeyer, Florian</dc:creator>
      <dc:creator>Groth, Sören</dc:creator>
      <dc:description><![CDATA[<p>„Accessibility“ is often reduced within classical transport research to its indicator function for measuring spatial relations and patterns. This creates the impression that the focus lies on measurements of socially and spatially differentiated access to specific opportunities within a given geographic context. In particular, German-speaking transport research could benefit from a theoretically and conceptually grounded understanding of justice. This article aims to establish a theoretical-conceptual foundation from the perspective of justice-oriented transport research. Accessibility planning can benefit from the considerations developed here, which draw on international research and concepts such as Transport Justice and Mobility Justice. These concepts also support the planning principle of public services, which is critical for rural areas. This results in the legitimization of transport and mobility strategies aimed to improve accessibility beyond private car use and beyond the debates on economic feasibility.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gh-81-567-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gh.copernicus.org/articles/81/567/2026/]]></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:esd140468</identifier>
    <datestamp>2026-10-05</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[From paper to proof: revealing Congo Basin warming through rescued climate archives]]></dc:title>
      <dc:creator>Muheki, Derrick</dc:creator>
      <dc:creator>Hufkens, Koen</dc:creator>
      <dc:creator>Jacobsen, Kim</dc:creator>
      <dc:creator>Verbeeck, Hans</dc:creator>
      <dc:creator>Boeckx, Pascal</dc:creator>
      <dc:creator>Kankonde Ntumba, Dominique</dc:creator>
      <dc:creator>Kapalay Moulasa, Olivier</dc:creator>
      <dc:creator>Vercruysse, Bas</dc:creator>
      <dc:creator>Birkholz, Julie M.</dc:creator>
      <dc:creator>Verbruggen, Christophe</dc:creator>
      <dc:creator>Hawkins, Ed</dc:creator>
      <dc:creator>Lampe, Seppe</dc:creator>
      <dc:creator>Yakusu, Emmanuel Kasongo</dc:creator>
      <dc:creator>Imwangana, Fils Makanzu</dc:creator>
      <dc:creator>Mbifo, José</dc:creator>
      <dc:creator>Likwela, Théophile Besango</dc:creator>
      <dc:creator>Meunier, Félicien</dc:creator>
      <dc:creator>Dewitte, Olivier</dc:creator>
      <dc:creator>Thorne, Peter</dc:creator>
      <dc:creator>Thiery, Wim</dc:creator>
      <dc:description><![CDATA[<p>The Congo Basin in Central Africa remains one of the few regions globally where the Intergovernmental Panel on Climate Change has neither assessed changes in hot extremes and extreme precipitation since the 1950s nor attributed such changes to anthropogenic influences, primarily due to the sparsity of in situ observational data. Although extensive daily weather records exist, spanning from the 1900s to the early 2000s and covering numerous stations across the basin, the majority of these remain archived on paper, limiting their accessibility for climate analysis. Here we present and analyse over 1 million temperature and precipitation observations from 37 weather stations in the Democratic Republic of the Congo, which have until now been unavailable to the research community. To produce this dataset, we first digitized (imaged) 9885 paper sheets stored in local archives during two dedicated field campaigns. We subsequently apply an improved version of the MeteoSaver software (version 1.1) to transcribe the imaged sheets, yielding daily time series of maximum, minimum, and average temperatures, precipitation, as well as dry bulb and wet bulb temperatures measured at three<span id="page1456"/> times per day (06:00, 15:00, and 18:00 local time). After quality control, analysis of multi-decadal temperature data across the basin reveals a consistent and accelerating warming signal since the 1960s, characterized by a warming shift in the distribution of daily maximum, minimum, and average temperatures with each successive decade. Median trends across 21 of the 37 stations with sufficient data availability are 0.22, 0.10, and 0.15 °C per decade for daily maximum, minimum, and average temperatures, respectively, corresponding to approximately 0.7, 0.3, and 0.5 °C of warming during the 1961–1990 period. We further find an increasing frequency of hot extremes and a decreasing frequency of cold extremes with each successive decade, with the most recent decade exhibiting nearly twice as many hot days per year and fewer cold days compared to the earliest decade. Analysis of precipitation at three stations with sufficient data indicates an increased frequency of heavy precipitation events at two stations and no substantial change at the third; however, limited spatial coverage due to data availability restricts broader conclusions for the DRC. Overall, this analysis of rescued weather data from Central Africa highlights the urgent need to close the knowledge gap on climate trends in the Congo Basin, one of the world's most data-sparse yet climatically significant regions.</p>]]></dc:description>
      <dc:date>2026-10-05</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-1455-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/1455/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd146810</identifier>
    <datestamp>2026-10-12</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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      <dc:title><![CDATA[A High-Resolution Gridded Dataset of Vertically Resolved Fine Root Biomass Across China]]></dc:title>
      <dc:creator>Zheng, Wenlu</dc:creator>
      <dc:creator>Zhao, Min</dc:creator>
      <dc:creator>Li, Woheng</dc:creator>
      <dc:creator>Zhang, Deshuai</dc:creator>
      <dc:creator>Tang, Weihua</dc:creator>
      <dc:creator>Luo, Junshen</dc:creator>
      <dc:creator>Jiao, Shuning</dc:creator>
      <dc:creator>Li, Fengtai</dc:creator>
      <dc:creator>Zhang, Haicheng</dc:creator>
      <dc:description><![CDATA[Fine root plays a critical role in ecosystem biogeochemical cycles, serving as the primary organs for water and nutrient uptake and exhibiting rapid turnover. However, a spatially explicit dataset of fine root biomass (FRB) across soil profiles and vegetation types remains lacking. To address this knowledge gap, we compiled 2,311 in-situ measurements of woody FRB and 3,580 measurements of herbaceous FRB from peer-reviewed studies across China. Using these observations, we developed random forest models to estimate surface-layer (0&ndash;20 cm) FRB and the vertical attenuation coefficient (<em>k</em>) of FRB for woody and herbaceous ecosystems, respectively. By integrating the predicted surface-layer FRB and vertical distribution functions, we finally generated a gridded dataset of FRB across 0&ndash;2 m soil depth (at 20 cm intervals) at 1 km spatial resolution for all woody and herbaceous ecosystems in China for 2005&ndash;2025. Model evaluation showed that our models explain approximately 86 % and 81 % of the observed variations in surface FRB across woody and herbaceous ecosystems, respectively, and reasonablely capture the interannual dynamics of observed FRB. Model predictions reveal substantial spatial and vertical variations in both woody and herbaceous FRB across China. Woody FRB density was generally higher in southern China than in central and northern China, whereas herbaceous FRB density was highest on the Qinghai&ndash;Tibet Plateau. Woody plants exhibit deeper root distributions in arid regions, whereas herbaceous species show consistently surface-concentrated rooting patterns across climate zones. The environmental controls of FRB also differed between vegetation types, with woody FRB being more strongly influenced by root traits and nutrient availability, whereas herbaceous FRB was more closely associated with climatic conditions. This dataset provides an observation-constrained, spatially explicit benchmark for quantifying belowground carbon stocks and dynamics, and it is archived and publicly available at <a href="https://doi.org/10.6084/m9.figshare.32353257" target="_blank" rel="noopener">https://doi.org/10.6084/m9.figshare.32353257</a> (Zheng et al., 2026).]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-777</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-777/]]></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:essdd146697</identifier>
    <datestamp>2026-10-12</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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      <dc:title><![CDATA[marinedb: An open-source, flexible and scalable Python workflow for curating, standardizing, and integrating marine biodiversity data]]></dc:title>
      <dc:creator>Berhocoïrigoin, Elena</dc:creator>
      <dc:creator>Noac'h, Philippe</dc:creator>
      <dc:creator>Laviale, Martin</dc:creator>
      <dc:creator>Ayata, Sakina-Dorothée</dc:creator>
      <dc:creator>Fix, Jérémy</dc:creator>
      <dc:creator>Pradalier, Cédric</dc:creator>
      <dc:description><![CDATA[The digital era and the emergence of data-aggregation initiatives have greatly expanded access to biodiversity occurrence records, but accessibility alone does not ensure usability for ecological modeling. Marine occurrence data must be cleaned and reconciled across spatial, temporal, and taxonomic dimensions before they can be reliably linked to environmental predictors and used to model species distributions. Here, we introduce <em>marinedb</em>, an open-source, modular, and scalable Python package for curating marine occurrence data. The package provides a suite of tools that can be freely combined into user-defined workflows tailored to study objectives and data characteristics. We applied <em>marinedb</em> to three major biodiversity resources: the Global Biodiversity Information Facility (GBIF), the Ocean Biogeographic Information System (OBIS), and the Jellyfish Database Initiative (JeDI). Together, these resources span hundreds of millions of occurrence records located at sea and more than one hundred thousand species. First, we used the framework to assess data quality non-destructively across the three sources. The analysis revealed substantial and source-dependent issues, including records located on land, missing depth information, heterogeneous, incomplete, or low-precision temporal information, records lacking species-level information or referring to non-marine taxa, weak or unspecified evidential support, absence records, and strong taxonomic imbalance. Second, we applied a tailored dataset-production workflow to produce a ready-to-use global marine occurrence dataset for large-scale modeling of present-day species distributions, which comprises 158,910,536 records representing 139,844 species. Together, the reusable Python tools and the curated dataset derived from GBIF, OBIS, and JeDI lower the technical barrier for multi-species and deep-learning approaches, both of which require extensive and diverse occurrence records, while preserving flexibility for future use-case-specific curation.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-771</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-771/]]></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:essdd143789</identifier>
    <datestamp>2026-10-12</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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      <dc:title><![CDATA[Atlas of geochemical, petrophysical and mechanical rock properties of the crystalline basement in Germany &ndash; first release]]></dc:title>
      <dc:creator>Weydt, Leandra Maren</dc:creator>
      <dc:creator>Ramírez-Guzmán, Ángel Andrés</dc:creator>
      <dc:creator>Muhl, Lena</dc:creator>
      <dc:creator>Deon, Fiorenza</dc:creator>
      <dc:creator>Schleicher, Anja Maria</dc:creator>
      <dc:creator>Sass, Ingo</dc:creator>
      <dc:description><![CDATA[A comprehensive and statistically robust understanding of rock characteristics is essential for reservoir characterization of the deep subsurface to accurately plan exploration campaigns, parameterize predictive 3D geological models, interpret geophysical data, and execute numerical thermo-hydraulic-mechanical-chemical simulations, thereby reducing economic risks and project uncertainties. Despite growing interest in the crystalline basement in Germany for e.g., geothermal energy applications and the safe storage of high-radioactive nuclear waste, systematic datasets covering the major crystalline and metamorphic basement units and their physiomechanical characteristics remain scarce, fragmented, or lack the metadata required for robust evaluation. To address this data gap, the AMPEDEK project established a unified, multi-scale national reference database for geochemical, petrophysical, and mechanical rock properties of crystalline rocks in Germany. The framework integrated extensive literature reviews, data from geological surveys, and newly conducted sampling and measurement campaigns, linking metadata, geochemistry, petrography, and physiomechanical rock properties through unique sample IDs.</p> <p>Existing data from more than 40 studies were compiled, evaluated, and integrated into the database. In addition, approximately 650 cylindrical plugs retrieved from drill cores and outcrop samples were systematically analyzed with respect to their mineralogical, geochemical, petrophysical, and rock mechanical properties to close remaining data gaps. Particular emphasis was placed on sampling a broad spectrum of lithologies to ensure coverage of the major crystalline units in Germany.</p> <p>The resulting open-access repository (Weydt et al., 2026; <a href="https://doi.org/10.48328/tudatalib-2167" target="_blank" rel="noopener">https://doi.org/10.48328/tudatalib-2167</a>) currently contains approximately 25,700 data points covering up to 34 parameters measured on 8,200 samples from more than 3,400 sampling locations across eight federal states in Germany. It represents the first standardized national-scale compilation of geochemical, petrophysical, and mechanical rock property data for the crystalline basement in Germany. The database provides a robust empirical foundation for early-stage exploration, reservoir characterization, and the validation of analytical measurement methods. Future efforts will focus on expanding the database towards regions with low data density and on high-temperature and high-pressure experiments to improve the understanding of parameter variations under in situ conditions.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-555</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-555/]]></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:essd132849</identifier>
    <datestamp>2026-10-12</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[The OpenSat4Weather dataset: Ku-band satellite link data for precipitation monitoring]]></dc:title>
      <dc:creator>Nebuloni, Roberto</dc:creator>
      <dc:creator>Graf, Maximilian</dc:creator>
      <dc:creator>Cazzaniga, Greta</dc:creator>
      <dc:creator>Mercier, François</dc:creator>
      <dc:creator>Turko, Maxime</dc:creator>
      <dc:description><![CDATA[<p>The TV-SAT signals received by the ground antennas of Satellite Microwave Links (SMLs) can be opportunistically used for detecting and quantifying precipitation. Consequently, SMLs have the potential to serve as low-cost rainfall sensors complementing conventional instruments. However,  a major challenge for opportunistic sensors, including both SMLs and their terrestrial counterpart – Commercial Microwave Links (CMLs) – is related to data ownership and accessibility  constraints, possibly hindering progress in the development of processing tools and validation studies. This limitation highlights the importance  of openly accessible datasets. While CML open datasets are already available, there are no large-scale SML datasets in public repositories. To address  this gap, we introduce  the OpenSat4Weather dataset, a comprehensive and openly accessible collection of measurements  from 215 SML sensors deployed in Southern France, over a five-month period from August to December 2022. The dataset is accessible at <a href="https://doi.org/10.5281/zenodo.16530166">https://doi.org/10.5281/zenodo.16530166</a> <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx34">Nebuloni et al.</a>, <a href="#bib1.bibx34">2025</a><a href="#bib1.bibx34">b</a>)</span>. OpenSat4Weather also includes concurrent conventional measurements, namely, 6 <span class="inline-formula">min</span> rainfall depths from 113 operational rain gauges, and radar-based estimates of rainfall intensity along each SML path. The radar data were derived from the gauge-adjusted weather radar product PANTHERE provided by Météo-France. Additionally, the dataset stores ERA5 reanalysis data of the 0 <span class="inline-formula">°C</span> isotherm height for rain height estimation, which are essential for accurately converting the  received signal level into rainfall intensity.</p>        <p>In this paper, we detail the OpenSat4Weather data preparation process and draw statistics of data availability. We then  provide a descriptive analysis of the dataset, including  rainfall characteristics, derived from rain gauges,  statistical properties of the SML received signal levels, and a comparison between SML and radar data. In addition, we illustrate  examples of disturbances and anomalous patterns observed in raw SML signals. Finally, we provide some practical guidelines for processing and analyzing SML data. Our ultimate goal is to promote open research initiatives aimed at accelerating the development of SML-based applications. Enhancing rainfall monitoring  by opportunistic sensors has the potential to provide  substantial benefits, particularly   in regions where conventional networks are  sparse or unavailable.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-7455-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/7455/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:angeo141022</identifier>
    <datestamp>2026-10-12</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/
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      <dc:title><![CDATA[Statistical properties of internal modulation in pulsating aurora]]></dc:title>
      <dc:creator>Nanjo, Sota</dc:creator>
      <dc:creator>Taki, Tomoe</dc:creator>
      <dc:creator>Hosokawa, Keisuke</dc:creator>
      <dc:creator>Brändström, Urban</dc:creator>
      <dc:creator>Miyoshi, Yoshizumi</dc:creator>
      <dc:creator>Johnsen, Magnar G.</dc:creator>
      <dc:description><![CDATA[<p>We statistically investigated the occurrence characteristics of internal modulation (IM), a rapid intensity modulation of a few hertz embedded in pulsating aurora (PsA), using high-speed ground-based optical data obtained with qCMOS cameras. For datasets acquired at Kiruna, Sweden, and Skibotn, Norway, we applied a two-step hierarchical machine-learning classification, first identifying the presence of PsA and then determining whether IM was present within the PsA. This enabled IM, which has previously been examined mainly through case studies, to be quantified for the first time in a systematic and statistically comparable manner. The results show that the fraction of PsA accompanied by IM increases toward the morning-sector magnetic local time (MLT) sector and tends to be higher at the lower-latitude site, Kiruna, than at the higher-latitude site, Skibotn. Representative examples from the classification results show that, on the midnight sector, IM commonly appears as a hierarchical structure superposed on clear main pulsations, whereas on the morning sector, the main pulsation tends to be relatively weak and the IM component often becomes dominant, suggesting that the morphology of IM itself also depends on MLT. These results suggest that IM is not merely an apparent subtype accompanying PsA, but rather a diagnostic feature that may provide insight into the wave–particle interaction underlying PsA.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/angeo-44-1023-2026</dc:identifier>
      <dc:identifier><![CDATA[https://angeo.copernicus.org/articles/44/1023/2026/]]></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:amt138805</identifier>
    <datestamp>2026-10-12</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[The enhanced capabilities of mid-infrared limb emission sounding to observe stratospheric aerosol injection geoengineering]]></dc:title>
      <dc:creator>Sellitto, Pasquale</dc:creator>
      <dc:creator>Kosary, Mona</dc:creator>
      <dc:creator>Höpfner, Michael</dc:creator>
      <dc:creator>Funke, Bernd</dc:creator>
      <dc:creator>Hoffmann, Alex</dc:creator>
      <dc:creator>Ungermann, Jörn</dc:creator>
      <dc:creator>Errera, Quentin</dc:creator>
      <dc:creator>Tilmes, Simone</dc:creator>
      <dc:creator>Sinnhuber, Björn-Martin</dc:creator>
      <dc:description><![CDATA[<p>Using a model-based pseudo-reality (PR) future scenario and realistic pseudo-observations (POs) representative for a proposed satellite mission concept (CAIRT – the Changing-Atmosphere Infra-Red Tomography explorer), we analyse the capabilities of a high-spectral-resolution limb-emission sounding technique to detect and quantitatively monitor very weak stratospheric aerosol injections (SAI) geoengineering deployments, in terms of the injected sulphur dioxide (SO<span class="inline-formula"><sub>2</sub></span>) and its evolution into sulphate aerosols (SA). Our results suggest that this technique would detect SO<span class="inline-formula"><sub>2</sub></span> injections, at the horizontal and vertical scale, within hours to a few days since the SAI deployment. This concept would quantify the SO<span class="inline-formula"><sub>2</sub></span> injected mass, even for injections of the order of magnitude of a few hundreds of tonnes of SO<span class="inline-formula"><sub>2</sub></span> per day, characteristic of “near-term” to “mid-term” experiments feasible even unilaterally, or in the context of small-scale outdoor experiments, with presently existing technology and at relatively low cost. In addition, our results suggest that this concept would be able to track the temporal evolution of the subsequently formed SA, as it spreads zonally and then toward higher latitudes through meridional dispersion, and to monitor changes in its vertical distribution over time through processes like self-lofting of the resulting SA plume. Existing satellite instruments, e.g. based on limb scattering, solar occultation, nadir observations and space LiDARs, do not have the capability to carry out such strategical observations of SAI. Our results stress the importance of increasing our global observational capabilities with high-spectral-resolution limb-emission satellite instruments, a capability not available at present and not foreseen in the near future.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-6379-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/6379/2026/]]></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:acp143629</identifier>
    <datestamp>2026-10-12</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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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Warm-sector heavy rainfall over the eastern China plains: identification, characteristics, and precursor dynamic signals]]></dc:title>
      <dc:creator>Deng, Weilong</dc:creator>
      <dc:creator>Guo, Jianping</dc:creator>
      <dc:creator>Li, Ning</dc:creator>
      <dc:creator>Zhang, Zhen</dc:creator>
      <dc:creator>Wang, Yifei</dc:creator>
      <dc:creator>Yang, Yi</dc:creator>
      <dc:description><![CDATA[<p>Warm-sector heavy rainfall (WSHR) poses forecasting challenges, while its contribution to regional heavy rainfall and short-term precursors remain poorly quantified. Drawing on 2021–2025 warm-season (June–September) observations from 493 surface rain gauges, ERA5 reanalysis, and a radar wind profiler (RWP) mesonet across the eastern China plains, we build an objective identification framework integrating automated front detection, warm-sector mask, and station-specific 99th-percentile hourly rainfall thresholds to separate WSHR from other heavy rain events. We detect 477 station-based WSHR events alongside 6002 other heavy rainfall events. WSHR is spatially scattered, peaks in July–August, and preferentially begins at 20:00–03:00 Beijing Time (BJT). Accounting for merely 5 %–10 % of annual heavy rainfall occurrences, WSHR has shorter durations yet comparable median rainfall accumulations and heavier extreme rainfall tails. Among the 297 stations recording at least one WSHR event, the mean station-level contribution of WSHR to heavy-rainfall accumulation is 13.8 %, with a maximum of 48.1 %. Composite ERA5 fields show that WSHR initiates within an 850 hPa moist tongue of high pseudo-equivalent potential temperature south of the front, superimposed on strengthening low-level moisture flux convergence. RWP composites of 62 WSHR events show increasing low-level jet (LLJ) occurrence and enhanced low-level ascent shortly before rainfall onset. Comparison with 271 warm-sector non-heavy rainfall events indicates a more pronounced late increase in LLJ occurrence and a stronger upper tail of ascent speeds at 1–2 km in WSHR, although the distributions overlap substantially. These observations identify candidate kinematic indicators whose event-level predictive skill remains to be evaluated.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14259-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14259/2026/]]></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:acp142682</identifier>
    <datestamp>2026-10-12</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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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Simultaneous measurements of gas- and aerosol-phase water-soluble organic nitrogen in the winter  urban atmosphere of Chengdu, China]]></dc:title>
      <dc:creator>Chen, Kaitao</dc:creator>
      <dc:creator>Li, Zheng</dc:creator>
      <dc:creator>Li, Rui</dc:creator>
      <dc:creator>Chen, Luyao</dc:creator>
      <dc:creator>Li, Rongjie</dc:creator>
      <dc:creator>Xiao, Binyu</dc:creator>
      <dc:creator>Lv, Shaojun</dc:creator>
      <dc:creator>Wu, Can</dc:creator>
      <dc:creator>Li, Rui</dc:creator>
      <dc:creator>Zhang, Junke</dc:creator>
      <dc:creator>Wang, Gehui</dc:creator>
      <dc:description><![CDATA[<p>Partitioning gaseous water-soluble organic nitrogen (WSON) to the aerosol phase is a major formation pathway of atmospheric secondary organic aerosols (SOA). However, the factors influencing this WSON partitioning process remain unclear. We conducted simultaneous wintertime measurements of WSON in both gas and aerosol phases at an urban site in Chengdu (CD), located in the Sichuan Basin (SCB), China, to investigate the concentration, gas-particle partitioning processes, and driven factors of WSON. The average concentration of particulate WSON (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">2.3</mn><mo>±</mo><mn mathvariant="normal">1.4</mn><mspace linebreak="nobreak" width="0.125em"/><mrow class="unit"><mi mathvariant="normal">µ</mi><mi mathvariant="normal">g</mi><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">N</mi><mspace width="0.125em" linebreak="nobreak"/><msup><mi mathvariant="normal">m</mi><mrow><mo>-</mo><mn mathvariant="normal">3</mn></mrow></msup></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="87pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="9e64c81eadfc41352c7b971674372505"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-14329-2026-ie00001.svg" width="87pt" height="15pt" src="acp-26-14329-2026-ie00001.png"/></svg:svg></span></span>) was about twice that of gaseous WSON (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1.2</mn><mo>±</mo><mn mathvariant="normal">0.9</mn><mspace linebreak="nobreak" width="0.125em"/><mrow class="unit"><mi mathvariant="normal">µ</mi><mi mathvariant="normal">g</mi><mspace linebreak="nobreak" width="0.125em"/><mi mathvariant="normal">N</mi><mspace width="0.125em" linebreak="nobreak"/><msup><mi mathvariant="normal">m</mi><mrow><mo>-</mo><mn mathvariant="normal">3</mn></mrow></msup></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="87pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="92807039df6b23c960678c42788b2f88"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-14329-2026-ie00002.svg" width="87pt" height="15pt" src="acp-26-14329-2026-ie00002.png"/></svg:svg></span></span>) and increased significantly as <span class="inline-formula">PM<sub>2.5</sub></span> increased. In winter, WSON readily partitions into the particle phase (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>F</mi><mtext>WSON</mtext></msub><mo>=</mo><mn mathvariant="normal">0.70</mn><mo>±</mo><mn mathvariant="normal">0.14</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="100pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="b349a7c3f7671df74b32694f6ba847cc"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-14329-2026-ie00003.svg" width="100pt" height="12pt" src="acp-26-14329-2026-ie00003.png"/></svg:svg></span></span>), partitioning into the organic phase under warm, dry conditions and into aerosol liquid water under cold, humid conditions, with higher <span class="inline-formula"><i>F</i><sub>WSON</sub></span> in the latter. Amines (methylamine, MA; dimethylamine, DMA) were predominantly present in the gas phase but exhibited enhanced partitioning into the particle phase during the <span class="inline-formula">PM<sub>2.5</sub></span> polluted periods. Amines preferentially partitioned into aerosol liquid water throughout the entire campaign, stably existing as amine-sulfate or amine-nitrate salts in <span class="inline-formula">PM<sub>2.5</sub></span>. The influence of aerosol liquid water content (ALWC) on the partitioning behavior of both WSON and amines was substantially greater than that of temperature (<span class="inline-formula"><i>T</i></span>), relative humidity (RH), and aerosol acidity (pH), as further confirmed by thermodynamic modeling with S-curve analysis. Furthermore, <span class="inline-formula">NH<sub>4</sub>NO<sub>3</sub></span> was identified as the primary contributor to ALWC, suggesting that controlling <span class="inline-formula">NO<sub><i>x</i></sub></span> and <span class="inline-formula">NH<sub>3</sub></span> emissions is crucial for reducing ALWC and subsequent WSON formation.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14329-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14329/2026/]]></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:acp142253</identifier>
    <datestamp>2026-10-12</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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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Characterizing lightning NOx production in the Ebro Valley with meteosat 12 LI and LMA observations]]></dc:title>
      <dc:creator>Pérez-Invernón, Francisco J.</dc:creator>
      <dc:creator>Gordillo-Vázquez, Francisco J.</dc:creator>
      <dc:creator>Velde, Oscar</dc:creator>
      <dc:creator>Montanyà, Joan</dc:creator>
      <dc:creator>López Trujillo, Jesús Alberto</dc:creator>
      <dc:creator>Pineda, Nicolau</dc:creator>
      <dc:creator>Loyola, Diego</dc:creator>
      <dc:creator>Seo, Sora</dc:creator>
      <dc:creator>Knote, Christoph</dc:creator>
      <dc:creator>Fierro, Alexandre O.</dc:creator>
      <dc:creator>Huntrieser, Heidi</dc:creator>
      <dc:description><![CDATA[<p>Lightning is one of the main sources of NO<span class="inline-formula"><sub><i>x</i></sub></span> in the Earth's atmosphere, yet there is considerable variability in NO<span class="inline-formula"><sub><i>x</i></sub></span> production during thunderstorms. In this study, we combined optical lightning data from the Meteosat Third Generation (MTG) Lightning Imaging (LI) instrument, which provides information on the occurrence rate and physical characteristics of lightning flashes, measurements from an extended Lightning Mapping Array (LMA) consisting of 24 sensors, lightning measurements from the Lightning Location System (LLS) of the Meteorological Service of Catalonia (MSC), and TROPOspheric Monitoring Instrument (TROPOMI) cloud and NO<span class="inline-formula"><sub>2</sub></span> research products to investigate lightning NO<span class="inline-formula"><sub><i>x</i></sub></span> emissions in the Ebro Valley (Spain). WRF-Chem simulations were used to calculate the necessary air mass factors and to subtract the NO<span class="inline-formula"><sub><i>x</i></sub></span> not produced by lightning from the TROPOMI measurements, allowing a more accurate estimation of lightning-induced NO<span class="inline-formula"><sub><i>x</i></sub></span>. We found positive relationships between lightning-produced NO<span class="inline-formula"><sub><i>x</i></sub></span> per flash and several lightning properties, including flash channel length, radiance, footprint, duration and the length of the optical continuous signal detected from space. These results highlight the importance of combining detailed lightning observations with atmospheric modeling to quantify NO<span class="inline-formula"><sub><i>x</i></sub></span> emissions from thunderstorms.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14277-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14277/2026/]]></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:acp139028</identifier>
    <datestamp>2026-10-12</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[Cloud vertical structure across China from a national Ka-band cloud radar network: thermodynamic, dynamical, and land-surface controls]]></dc:title>
      <dc:creator>Xu, Hui</dc:creator>
      <dc:creator>Guo, Jianping</dc:creator>
      <dc:creator>Deng, Jianbo</dc:creator>
      <dc:creator>Yang, Rongfang</dc:creator>
      <dc:creator>Meng, Deli</dc:creator>
      <dc:creator>Zhang, Zhen</dc:creator>
      <dc:creator>Li, Ning</dc:creator>
      <dc:creator>Sun, Yuping</dc:creator>
      <dc:creator>Jiang, Shuairu</dc:creator>
      <dc:creator>Chen, Tianmeng</dc:creator>
      <dc:creator>Chen, Juan</dc:creator>
      <dc:creator>Zeng, Liping</dc:creator>
      <dc:creator>Zhou, Yongshui</dc:creator>
      <dc:creator>Tong, Bing</dc:creator>
      <dc:description><![CDATA[<p>Cloud vertical structure (CVS) plays a fundamental role in regulating the Earth's radiation budget and hydrological cycle, yet its representation in numerical weather prediction and climate models remains highly uncertain, largely due to limited high-resolution regional observations. Using a newly established national network of 80 Ka-band millimeter-wave cloud radars (MMCRs), here we present a high-spatiotemporal-resolution (vertical resolution of 30 m, temporal resolution of 1 min) characterization of CVS across China based on one year (2024) of observations, and quantify its thermodynamic, dynamical, and land-surface controls. Cloud boundaries are retrieved using an improved algorithm that integrates height-dependent radar sensitivity with variance-based clutter suppression. Results show that the national annual mean cloud occurrence frequency is 56.7 <span class="inline-formula">±</span> 7.2 %, dominated by single-layer clouds (34.7 <span class="inline-formula">±</span> 4.0 %), followed by two-layer (14.7 <span class="inline-formula">±</span> 3.2 %) and multi-layer clouds (7.1 <span class="inline-formula">±</span> 2.4 %). Spatially, single-layer clouds prevail over arid northwestern China, whereas multi-layer clouds are more frequent in humid southeastern region. Cloud base height (CBH) exhibits strong seasonality (summer <span class="inline-formula">&gt;</span> spring <span class="inline-formula">&gt;</span> autumn <span class="inline-formula">&gt;</span> winter), with notably low CBH over the Tibetan Plateau. Diurnally, summer clouds show a pronounced afternoon peak between 3 and 9 km, while winter clouds remain largely below 3 km and peak near sunrise. Thermodynamic conditions exert the primary control on CVS. Higher 2 m specific humidity promotes deeper cloud development and raises cloud top height (CTH), whereas enhanced lower-tropospheric stability suppresses vertical cloud growth and lowers both CBH and CTH. Dynamical forcing further modulates cloud structure: stronger vertical wind shear (VWS) generally inhibits vertical cloud development, reducing CBH, CTH and cloud thickness, while moderate VWS can enhance organization under unstable conditions. Joint dependence analyses reveal that moisture, stability, and shear act in a coupled manner, with moisture being the dominant driver and stability and shear serving as strong regulators. In addition, land-surface characteristics<span id="page14304"/> significantly influence CBH, especially for afternoon single-layer low clouds, which exhibit a mean CBH is 21.7 % higher than the all-hour low clouds, with the strongest enhancement over evergreen broadleaf forests (<span class="inline-formula">+41.7 <i>%</i></span>). These findings provide the first observationally constrained, national-scale assessment of CVS based on this radar network, offering quantitative benchmarks for evaluating and improving cloud parameterizations in weather and climate models.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14303-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14303/2026/]]></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:acp135612</identifier>
    <datestamp>2026-10-12</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[Synoptic and regional-scale meteorological controls of stratus altitude in the Namib Desert]]></dc:title>
      <dc:creator>Hipler, Viola</dc:creator>
      <dc:creator>Andersen, Hendrik</dc:creator>
      <dc:creator>Spirig, Robert</dc:creator>
      <dc:creator>Vogt, Roland</dc:creator>
      <dc:creator>Piketh, Stuart</dc:creator>
      <dc:creator>Adler, Bianca</dc:creator>
      <dc:creator>Cermak, Jan</dc:creator>
      <dc:description><![CDATA[<p>In the Namib Desert, fog is an essential water source and occurs when and where advected marine stratus clouds intersect with the land surface. However, the meteorological controls of the cloud base height are still insufficiently understood. This study aims to develop a basic understanding of the processes that influence the stratus altitude and, by extension, the spatial occurrence of fog. We combine satellite and in situ observations with large-scale meteorological data from reanalysis data (ERA5) to compare fog events to lifted stratus at the coast (low-cloud events). In fog situations, the marine boundary layer is shallower by up to <span class="inline-formula">130 m</span> along the entire coastline than in low-cloud situations. This is found to be related to the large-scale high-pressure systems. Fog situations exhibit a weaker Atlantic High but elevated continental pressure. The weaker Atlantic High is connected to less pronounced near-surface winds along the coastline, less cold advection, and heat fluxes upstream of the study region, leading to the shallower marine boundary layer. In parallel, higher continental pressures on fog days facilitate the formation of stronger nocturnal katabatic winds which can mix with, undercut or block the advected cloudy marine air. An alternative mechanism is highlighted in a case study of an off-season fog event, where a ridging high produces hot and dry subsiding easterly air masses which lower and intensify the inversion from above. To assess the predictive power of the continental and Atlantic high-pressure systems and the regional pressure pattern, a logistic regression is trained with three corresponding features. The classification outperformed a climatological baseline by <span class="inline-formula">≈10</span> %, suggesting that the features contain relevant process information. The results improve our understanding of the processes that determine the seasonal and day-to-day variability of fog versus elevated low-cloud occurrence in the Namib.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14367-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14367/2026/]]></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:acp138590</identifier>
    <datestamp>2026-10-12</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[Vertical distribution of pollution trapped by wintertime surface inversions in Fairbanks, Alaska, during the ALPACA experiment]]></dc:title>
      <dc:creator>Stutz, Jochen</dc:creator>
      <dc:creator>Kuhn, Jonas</dc:creator>
      <dc:creator>Cooperdock, Sol</dc:creator>
      <dc:creator>Johnson, Sarah</dc:creator>
      <dc:creator>Guo, Fangzhou</dc:creator>
      <dc:creator>Flynn, James H.</dc:creator>
      <dc:creator>Cesler-Maloney, Meeta</dc:creator>
      <dc:creator>Simpson, William R.</dc:creator>
      <dc:description><![CDATA[<p>Air pollution in cold wintertime urban areas is a ubiquitous problem. Surface temperature inversions under low wind conditions and surface emissions lead to the formation of a shallow polluted surface layer (PSL). The presence of this PSL is well documented, but its height, the rates of exchange with the background atmosphere, and the interplay between vertical mixing and chemistry remain poorly quantified. Here we provide quantitative insights into this coupled chemistry-transport system using observations and modeling of vertical pollutant profiles.</p>        <p>Long-path Differential Optical Absorption Spectroscopy of vertical trace gas profiles during the 2022 Alaskan Layered Pollution and Chemical Analysis (ALPACA) experiment in Fairbanks, Alaska, quantitatively track the frequent establishment of PSLs with heights of 20–40 m, which sometimes persist for several days. PSL trace gas mixing ratios often plateau at levels of up to 35 ppb <span class="inline-formula">SO<sub>2</sub></span>, 60 ppb <span class="inline-formula">NO<sub>2</sub></span>, 2.5 ppb HONO, 7 ppb HCHO, and low ozone as a result of surface emissions, gas-phase chemistry, and ineffective mixing with the background atmosphere. Parameterizing vertical mixing with observed surface temperature gradients and wind speed in the PACT-1D chemistry and transport model leads to excellent agreement of modeled and measured trace gas profiles. The PACT-1D transport scheme determines the residence time of pollutants within the PSL to be 1–4 h, confirming the strong influence of atmospheric mixing on the composition of sustained PSL events. Altitude-dependent ozone and <span class="inline-formula">NO<sub><i>x</i></sub></span> chemistry highlight the strong coupling between mixing and chemistry, which must be considered to quantify pollutant concentrations accurately in shallow PSLs.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14345-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14345/2026/]]></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:acp137639</identifier>
    <datestamp>2026-10-12</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[Non-monotonic response of net dust deposition  kinetics to low wind speeds]]></dc:title>
      <dc:creator>Jia, Ruochen</dc:creator>
      <dc:creator>Ba, Chaoqun</dc:creator>
      <dc:creator>Zhang, Chao</dc:creator>
      <dc:creator>Kuang, Wennong</dc:creator>
      <dc:creator>Liu, Yuan</dc:creator>
      <dc:creator>Wang, Zhigang</dc:creator>
      <dc:creator>Liu, Fang</dc:creator>
      <dc:creator>Xin, Zhiming</dc:creator>
      <dc:creator>Liu, Yuting</dc:creator>
      <dc:creator>Ma, Qun</dc:creator>
      <dc:creator>Zong, Lu</dc:creator>
      <dc:creator>Liang, Wei</dc:creator>
      <dc:creator>Qian, Jianqiang</dc:creator>
      <dc:creator>Liu, Zhimin</dc:creator>
      <dc:description><![CDATA[<p>Dry deposition is a major sink for mineral dust, yet its behavior under weak winds remains poorly constrained and is often parameterized monotonically with wind speed. Here we quantify size-resolved dust net accumulation kinetics in a closed-circuit recirculating wind tunnel using a two-stage protocol (brief high-wind loading followed by low-wind deposition at 0, 2, 4, and 6 <span class="inline-formula">m s<sup>−1</sup></span>). Cumulative retained-mass time series were measured with an array of collection trays, with the initial suspended dust loading recorded by an online concentration monitor. Particle sizes were characterized by laser diffraction and grouped into six diameter-threshold classes (<span class="inline-formula">PM<sub>2.5</sub></span>–<span class="inline-formula">PM<sub>63</sub></span>). A first-order kinetic model described the temporal accumulation dynamics and yielded a fitted asymptotic retained mass (<span class="inline-formula"><i>a</i></span>), effective net-accumulation rate coefficient (<span class="inline-formula"><i>k</i></span>), characteristic time scale (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi mathvariant="italic">τ</mi><mo>=</mo><mn mathvariant="normal">1</mn><mo>/</mo><mi>k</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="39pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="317af451a8391105b2386cc63dec3bd2"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-14245-2026-ie00001.svg" width="39pt" height="14pt" src="acp-26-14245-2026-ie00001.png"/></svg:svg></span></span>), and initial net accumulation flux (<span class="inline-formula"><i>J</i><sub>0</sub>=<i>a</i><i>k</i></span>). The observed <span class="inline-formula"><i>J</i><sub>0</sub></span> was highest at 2 <span class="inline-formula">m s<sup>−1</sup></span> for <span class="inline-formula">PM<sub>2.5</sub></span>–<span class="inline-formula">PM<sub>30</sub></span>, and 4 <span class="inline-formula">m s<sup>−1</sup></span> for <span class="inline-formula">PM<sub>40</sub></span> and <span class="inline-formula">PM<sub>63</sub></span>, while <span class="inline-formula"><i>J</i><sub>0</sub></span> declined markedly at 6 <span class="inline-formula">m s<sup>−1</sup></span> for the lower diameter thresholds. Quadratic fits across the four wind-speed levels suggest a potential maximum near 2–3 <span class="inline-formula">m s<sup>−1</sup></span> for <span class="inline-formula">PM<sub>2.5</sub></span>–<span class="inline-formula">PM<sub>40</sub></span>. These measurements quantify the size-dependent response of effective surface retention to low wind speeds and provide benchmark behavior for coupled deposition, retention, and re-entrainment parameterizations.</p>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-14245-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/14245/2026/]]></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:egusphere146656</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The regional Earth system model ENEA-REG (version 3.0): development and validation for the Med-CORDEX region]]></dc:title>
      <dc:creator>Anav, Alessandro</dc:creator>
      <dc:creator>Hamitouche, Mohamed</dc:creator>
      <dc:creator>Fois, Matteo</dc:creator>
      <dc:creator>Catalano, Franco</dc:creator>
      <dc:creator>Napolitano, Ernesto</dc:creator>
      <dc:creator>Sannino, Gianmaria</dc:creator>
      <dc:creator>Struglia, Maria Vittoria</dc:creator>
      <dc:description><![CDATA[Regional Earth system models are essential tools for representing climate processes and interactions among Earth system components at spatial scales relevant to impact studies, thereby providing the scientific basis for reliable impact assessments and effective adaptation strategies.</p> <p>This paper presents the third version of the ENEA-REG regional Earth system model, specifically designed to simulate past and present climate variability and to produce centennial-scale climate projections over the Euro-Mediterranean region. Compared with the previous model version (i.e. ENEA-REG2), ENEA-REG3 introduces an enhanced representation of river discharge and floodplain processes and a substantially revised coupler implementing a time-averaged explicit atmosphere&ndash;ocean coupling strategy that improves the temporal consistency of the exchanged fluxes.</p> <p>Model performances are assessed using a hindcast simulation driven by the ERA5 and ORAS5 reanalyses, together with two historical downscaling simulations driven by the CMIP6 models EC-Earth3 and MPI-ESM1-2-HR. Compared to ENEA-REG2, the results indicate a substantial improvement in simulated river discharge and reduced biases in the ocean component, particularly in regions strongly influenced by freshwater inputs, such as the Adriatic Sea and several coastal areas of the eastern Mediterranean, where the excessive salinization simulated by ENEA-REG2 is markedly reduced. The results also show close agreement among the hindcast and historical simulations, suggesting that model performance is largely governed by the regional coupled system and its parameterizations rather than by the driving global climate models. This consistency strengthens confidence in the robustness of future climate projections.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5695</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5695/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146595</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Online single-particle characterization of ice-nucleating particles (INPs) at the High Altitude Research Station Jungfraujoch (3580 m a.s.l.), Switzerland]]></dc:title>
      <dc:creator>Zhang, Cuiqi</dc:creator>
      <dc:creator>Shen, Xiaoli</dc:creator>
      <dc:creator>Jacquot, Justin</dc:creator>
      <dc:creator>Lacher, Larissa</dc:creator>
      <dc:creator>Vishnupriya, Selvakumar</dc:creator>
      <dc:creator>Brem, Benjamin T.</dc:creator>
      <dc:creator>Modini, Robin L.</dc:creator>
      <dc:creator>Nowak, Nora</dc:creator>
      <dc:creator>Sprenger, Michael</dc:creator>
      <dc:creator>Steinbacher, Martin</dc:creator>
      <dc:creator>Henne, Stephan</dc:creator>
      <dc:creator>Collaud Coen, Martine</dc:creator>
      <dc:creator>Conen, Franz</dc:creator>
      <dc:creator>Höhler, Kristina</dc:creator>
      <dc:creator>Möhler, Ottmar</dc:creator>
      <dc:creator>Gysel-Beer, Martin</dc:creator>
      <dc:creator>Cziczo, Daniel J.</dc:creator>
      <dc:creator>Kanji, Zamin A.</dc:creator>
      <dc:description><![CDATA[Ice-nucleating particles (INPs) modulate the phase, radiative properties, and lifetime of clouds, yet direct observational evidence linking single aerosol particles to atmospheric ice nucleation (IN) remains challenging because of the low abundance of INPs. We sampled ambient aerosols by coupling an INP counter to a single-particle mass spectrometry (SPMS) via a pumped counter-flow virtual impactor at Jungfraujoch during wintertime. Ice crystal residuals (ICRs) sampled under conditions representative of mixed-phase and cirrus cloud formation and total aerosol sampled directly by the SPMS were chemically characterized. Mineral dust (MD) dominated the ICR population under both cloud regimes despite its minor contribution to ambient aerosol particles by number. Two distinct MD subclasses associated with local construction activities (MD-K/Al/Fe) and transported sources (MD-Ca) were identified. MD-K/Al/Fe contributed substantially to the INP population in the cirrus cloud regime, demonstrating that local anthropogenic activity can influence atmospheric INPs populations. In contrast, sulfate, organics, nitrate, and biomass burning aerosol (BBA) particles contributed only a minor fraction of ICRs despite dominating the ambient aerosol population, indicating low IN activity under the investigated conditions. However, Pb signatures were enriched in BBA ICRs, suggesting enhanced IN activity of Pb-containing BBA particles, whereas no corresponding enrichment was observed for Pb-containing MD-K/Al/Fe particles. Sporadic meteoric particles detected during stratospheric-intrusion events indicate a potential contribution of stratospheric aerosols to tropospheric primary IN. Limited in-cloud observations suggest that natural cloud processing may modify the IN activity of MD-K/Al/Fe and BBA particles.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5645</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5645/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146836</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Summertime Turbulence Characteristics across China&rsquo; Planetary Boundary Layer: Roles of Wind Shear, Static Stability, Cloud and Topography-Land-Cover Conditions]]></dc:title>
      <dc:creator>Xian, Tian</dc:creator>
      <dc:creator>Sun, Yuping</dc:creator>
      <dc:creator>Chen, Tianmeng</dc:creator>
      <dc:creator>Xu, Hui</dc:creator>
      <dc:creator>Guo, Xiaoran</dc:creator>
      <dc:creator>Zhang, Zhen</dc:creator>
      <dc:creator>Wu, Zhongwang</dc:creator>
      <dc:creator>Hu, Huaquan</dc:creator>
      <dc:creator>Chen, Juan</dc:creator>
      <dc:creator>Zeng, Liping</dc:creator>
      <dc:creator>Wang, Yifei</dc:creator>
      <dc:creator>Jiang, Shuairu</dc:creator>
      <dc:creator>Yao, Pengzhan</dc:creator>
      <dc:creator>Li, Ning</dc:creator>
      <dc:creator>Yang, Honglong</dc:creator>
      <dc:creator>Guo, Jianping</dc:creator>
      <dc:description><![CDATA[The spatio-temporal pattern of turbulence dissipation rate (&epsilon;) and its evolution remain elusive inside and above the planetary boundary layer (PBL). Using summertime 2022 data from a nationwide network of 132 radar wind profilers (RWPs), we contrast &epsilon; within the inner PBL (0.3 zᵢ &le; z &le; zᵢ) and above it (z ᵢ&lt; z &le; 3 zᵢ). Results reveal pronounced spatial heterogeneity: &epsilon; is strongest over Northwest and North China within the 30&ndash;40&deg;N belt and weakest over the Tibetan Plateau and Southwest China, and it is systematically weaker aloft than within the PBL; &epsilon; also peaks near 1300 local time in both layers and persists day-to-day for roughly 9 days. We examine four modulating factors&mdash;topography and land cover, cloud conditions, static stability, and vertical wind shear (VWS). Of these, terrain complexity and land-cover type partly shape the observed heterogeneity, with stronger near-PBL turbulence over rough arid regions and weaker over water-dominated basins. Cloud cover enhances &epsilon; throughout the vertical column, with a stronger amplification above the PBL (△<span>log₁₀&epsilon; = 0.16 m&sup2; s⁻&sup3;) than within it (0.1 m&sup2; s⁻&sup3;), mainly through intensified VWS. The dominant controls also differ with height: within the PBL, static stability and VWS jointly govern turbulence, whereas above the PBL turbulence is driven overwhelmingly by shear-generated disturbances. Spectral analysis further reveals distinct vertical stratification of turbulent energy density that strengthens under stronger VWS. These findings demonstrate the value of national RWP networks for resolving turbulent dynamics across China and provide observational constraints for PBL turbulence parameterization.</span>]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5822</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5822/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146777</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Evaluating the benefits of SWOT data assimilation and implications for future operational oceanography]]></dc:title>
      <dc:creator>Fouchet, Ergane</dc:creator>
      <dc:creator>Benkiran, Mounir</dc:creator>
      <dc:creator>Escudier, Romain</dc:creator>
      <dc:creator>Traon, Pierre-Yves</dc:creator>
      <dc:description><![CDATA[We present the first evaluation of SWOT data assimilation in a high-resolution ocean forecasting system at the global scale under operational conditions. Observing System Experiments performed with the Mercator Ocean operational data assimilation system are used to assess the gain in model performance associated with the assimilation of SWOT observations into Copernicus Marine Service products. We find that SWOT assimilation improves the global representation of sea level anomaly (SLA), particularly at spatial scales below 100 km. The global gain is of the order of 4 %, which is lower than those reported in previous studies, likely reflecting the strong constraint provided by the numerous nadir altimeters already assimilated in the system. Independent validation using drifters deployed during the SWOT Cal/Val phase shows improvements in both the zonal and meridional current components, highlighting the ability of wide-swath observations to provide a more balanced constraint on surface circulation than conventional nadir altimetry. Assimilation experiments with data from both the high-frequency Cal/Val and spatially extensive Science phases show that broader spatial coverage provides a larger global benefit than higher revisit frequency. Experiments with two model configurations further show that the higher-resolution model, which resolves more physical processes, derives greater benefits from SWOT data assimilation. These results provide guidance for the future development of operational oceanography based on wide-swath altimetry, highlighting the need for broader and more frequent satellite sampling, higher-resolution models with improved physical representation, and data assimilation methods adapted to dense, high-resolution, two-dimensional observations.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5789</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5789/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147245</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Drivers of multi-year &delta;13C-CO2 source signature variability in the Amazon rainforest]]></dc:title>
      <dc:creator>Vardag, Sanam N.</dc:creator>
      <dc:creator>Ticks, Kilian</dc:creator>
      <dc:creator>Botía, Santiago</dc:creator>
      <dc:creator>Eisele, Gerrit</dc:creator>
      <dc:creator>Papastefanou, Philip</dc:creator>
      <dc:creator>Quaresma, Cleo</dc:creator>
      <dc:creator>Asperen, Hella</dc:creator>
      <dc:creator>Souza, Carla</dc:creator>
      <dc:creator>D'Oliveira, Flavio A. F.</dc:creator>
      <dc:creator>Trumbore, Susan</dc:creator>
      <dc:creator>Zaehle, Sönke</dc:creator>
      <dc:creator>Jones, Sam P.</dc:creator>
      <dc:description><![CDATA[The carbon isotopic composition of ecosystem CO<sub>2</sub> exchange provides information on the physiological and environmental controls of land&ndash;atmosphere carbon fluxes. Here, we use continuous CO<sub>2</sub> and &delta;<sup>13</sup>C&ndash;CO<sub>2</sub> measurements from five inlet heights at the Amazon Tall Tower Observatory (ATTO) in central Amazonia to derive apparent &delta;<sup>13</sup>Cs source signatures from vertical-profile Keeling-plot relationships without prescribing an external background. The resulting continuous 2.5-year record from 2022 to 2024 substantially extends previous campaign-based and irregular measurements and provides a unique observational basis for resolving source signature variability in the Amazonia rainforest over time. The observations show pronounced variability on diurnal and seasonal time scales. The diurnal cycle is characterized by more enriched source signatures during the day (-28.5 to -27.5 &permil;) and more depleted values during the night (-29.5 to -28.5 &permil;). In contrast, the seasonal cycle showed less variability, with an amplitude of approximately 1.5&permil;. We compare the observed temporal variability of the inferred source signatures with source signatures simulated by the process-based model QUINCY. The observed diurnal cycle is broadly consistent with the sign and timing of the QUINCY response. Although QUINCY is systematically more depleted than the observations, the comparable diurnal amplitude suggests that the model captures the short-term functional response. On seasonal time scales, however, QUINCY simulates substantially stronger variability and much tighter relationships with environmental drivers than observed. These results indicate that the current model representation of isotope discrimination and environmental responses cannot fully explain the observed seasonal behaviour. The weaker observed seasonal response to environmental drivers suggests that Amazonian carbon&ndash;water&ndash;isotope coupling may be more buffered than represented in QUINCY, for example through canopy microclimate or deep-water access. Overall, the continuous multi-year ATTO record provides a valuable data set for evaluating Amazonian vegetation dynamics and identifies key areas in which process-model representations of isotope discrimination and water-stress responses require improvement.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6034</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6034/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147344</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Projected changes to cold-season extratropical cyclones over northeastern North America in an ensemble of regional climate model simulations]]></dc:title>
      <dc:creator>Labonté, Marie-Pier</dc:creator>
      <dc:creator>Asselin, Olivier</dc:creator>
      <dc:creator>Paquin, Dominique</dc:creator>
      <dc:creator>Leduc, Martin</dc:creator>
      <dc:creator>McCray, Christopher</dc:creator>
      <dc:description><![CDATA[Extratropical cyclones (ETCs) are the main drivers of cold-season weather in northeastern North America (NENA), yet their response to climate change remains uncertain. Here, we assess cold-season (November&ndash;March) ETCs in a high-resolution (0.11&deg;) regional climate model ensemble driven by four CMIP6 global climate models under multiple emissions scenarios, including five initial-condition members for one model&ndash;scenario combination. Historical simulations reproduce the main ERA5 track and genesis patterns, although they generally simulate more cyclones, lower minimum sea-level pressures, and stronger winds. With warming, cyclone track density decreases across much of North America, including over NENA, where cyclogenesis also tends to decline. The five-member subset exhibits substantial spread in projected track-density and cyclogenesis changes, highlighting the influence of internal variability on these regional patterns. Yet the total number of cyclones affecting NENA declines robustly across all driving models. Changes in cyclone characteristics are generally weak and driving-model dependent, although some statistically significant changes indicate stronger winds or slower-moving cyclones. Most apparent deepening in minimum sea-level pressure disappears when pressure is expressed as an anomaly from the local climatology, weakening the evidence for pressure-based intensification. Nevertheless, the number of cyclones falling below a fixed historical pressure-anomaly threshold remains broadly unchanged as total cyclone frequency declines, so the proportion classified as intense tends to increase. Despite fewer cyclones, total cold-season ETC-associated precipitation tends to increase over NENA land areas, including at every major city examined. These results point to fewer but wetter cold-season cyclones, with increasing ETC-associated precipitation despite limited dynamical intensification.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6110</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6110/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147346</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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      <dc:title><![CDATA[The NASA Aerosol Wind Profiler Doppler Wind Lidar, Part II: Airborne Flight Demonstration]]></dc:title>
      <dc:creator>Bedka, Kristopher</dc:creator>
      <dc:creator>Khlopenkov, Konstantin</dc:creator>
      <dc:creator>Cooney, John</dc:creator>
      <dc:creator>Marketon, John</dc:creator>
      <dc:creator>Applin, Samantha</dc:creator>
      <dc:creator>Begay, Seth</dc:creator>
      <dc:creator>Cross, Maurice</dc:creator>
      <dc:creator>Henderson, Sammy</dc:creator>
      <dc:creator>Traore, Aboubakar</dc:creator>
      <dc:creator>Wilson, Frederick G.</dc:creator>
      <dc:description><![CDATA[The NASA Aerosol Wind Profiler (AWP) instrument, described in Part I of this paper, was flown aboard a NASA Gulfstream-3 aircraft during its first two airborne science campaigns based in Hampton, Virginia and central California in September&ndash;November 2024. These campaigns were focused on demonstrating how a coherent-detection Doppler wind lidar could address NOAA wind observation requirements, and to observe planetary boundary layer processes to address NASA and U.S. Naval Research Laboratory science objectives in conjunction with High Altitude Lidar Observatory (HALO) differential absorption lidar (DIAL) water vapor and high spectral resolution lidar (HSRL) aerosol profiling. AWP observed a wide variety of weather regimes and phenomena with high detail (66&ndash;133 m vertical and 0.6&ndash;4 km spatial resolution, scan pattern dependent) and precision (.1 m/s bias, 0.89 m/s uncertainty) over nearly 100 hours of data collection. This is Part II of the AWP instrument description and airborne demonstration paper series that highlights wind profile measurements from Fall 2024 campaign flights and quantifies measurement performance with co-located Airborne Vertical Atmospheric Profiling System (AVAPS) dropsonde and NOAA Global Forecast System (GFS) wind profiles.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6111</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6111/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146573</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Atmospheric bromine deposition as a source of seasonal snowpack bromide reservoirs for Arctic bromine explosion events: evidence from linking chemistry-climate simulations with snow observations using a layered snow model]]></dc:title>
      <dc:creator>Falk, Stefanie</dc:creator>
      <dc:creator>Jacobi, Hans-Werner</dc:creator>
      <dc:creator>El-Mansi, Hugo</dc:creator>
      <dc:creator>Ginot, Patrick</dc:creator>
      <dc:creator>Sinnhuber, Björn-Martin</dc:creator>
      <dc:description><![CDATA[Bromine explosion events (BEs) are an important source of reactive bromine in the Arctic boundary layer and contribute to episodic ozone depletion in spring. While bromide-rich sea ice and snow are generally regarded as the primary source, the extent to which atmospheric deposition of bromine can establish and replenish a snowpack bromide reservoir remains poorly constrained. We combine simulations with the ECHAM/MESSy Atmospheric Chemistry model (EMAC), field observations, and laboratory analyses of snow samples collected around Ny-&Aring;lesund (Svalbard) in April 2024 to investigate the role of atmospheric bromine deposition for BEs. To connect atmospheric deposition fluxes with observed snow chemistry, we developed the Snow Model with Evolving Layers (SMELs), a simple offline snow model that tracks bromide accumulation within a dynamically evolving snowpack.</p> <p>EMAC simulations indicate that bromine dry deposition from very short-lived substances (VSLS) and sea-salt aerosol (SSA) dehalogenation can establish snow bromide reservoirs sufficient to sustain typical Arctic springtime BrO abundances. Bromine species partitioning upon deposition suggests that a lack of HBr deposition may suppress heterogeneous Br<sub>2</sub> production during fall. SMELs reproduces the observed vertical bromide enhancement and depletion patterns and demonstrates that finite snowpit sampling can introduce substantial biases. The strong agreement between modeled and observed normalized bromide profiles suggests that bromine deposition and post-depositional processing operate on regional scales around Ny-&Aring;lesund. Our results identify atmospheric bromine deposition as an important seasonal bromide reservoir and highlight the role of bromine speciation and snowpack processes in controlling Arctic bromine activation.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5627</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5627/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146572</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[The Structural Topology Model: A Topology&ndash;Ontology Framework for Assigning Geological Legends in 3D and 2D Geomodelling]]></dc:title>
      <dc:creator>Monti, Riccardo</dc:creator>
      <dc:creator>Hussain, Waqas</dc:creator>
      <dc:creator>Monopoli, Bruno</dc:creator>
      <dc:creator>Herwegh, Marco</dc:creator>
      <dc:creator>Drvoderić, Sebastian</dc:creator>
      <dc:creator>Furlan, Matteo</dc:creator>
      <dc:creator>Musso Piantelli, Ferdinando</dc:creator>
      <dc:creator>Piaz, Giovanni</dc:creator>
      <dc:creator>Bistacchi, Andrea</dc:creator>
      <dc:description><![CDATA[Three-dimensional geological modelling of orogenic belts and other highly deformed complexes remains challenging, especially in metamorphic complexes, where the obliteration of stratigraphy complicates the definition of units, boundaries, and their relations. In such contexts, approaches inherited from modelling in sedimentary basins often lead to ambiguous definition of the legend (and the units represented therein) and topologically inconsistent 3D models. Here, we present the Structural Topology Model (STM), a conceptual framework designed to formalise the construction of consistent geological legends by making explicit the relations between units, bounding surfaces, and their structural roles, according to the concept of oriented topology (based on the properties of continuity and conformability). Central to STM is the concept of the Structural Level, which integrates absolute ages, relative ages, and structural relations into a scalar field used to define an ordered sequence of geological units and events, even where chronological constraints are incomplete or ambiguous. STM was conceived for 3D modelling, but it could be applied also in 2D to geological maps and cross-section providing useful constraints and tools to validate topological relationships and conceptual models. The method is illustrated with two case studies in the Helvetic units of the Aar Massif (Helvetics, Central Swiss Alps) and in Penninic units of the Gressoney Valley (Western Italian Alps). In both examples, STM enables the construction of topologically consistent volumetric models that preserve internal structures, foliation patterns, and cross-cutting relationships, while providing an unambiguous framework for labelling units and boundaries. STM, already implemented in the open-source PZero 3D modelling platform, is independent of specific software implementations or interpolation techniques and could be potentially applied in a wide range of geological settings and software. In this way, limitations of implicit 3D modelling in complex polydeformed areas are reduced substantially.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5626</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5626/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147239</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Increased future ice loss due to nested ice-climate feedbacks if Antarctic heatwaves intensify]]></dc:title>
      <dc:creator>Nicola, Lena</dc:creator>
      <dc:creator>Beckmann, Johanna</dc:creator>
      <dc:creator>McCormack, Felicity S.</dc:creator>
      <dc:creator>Winkelmann, Ricarda</dc:creator>
      <dc:description><![CDATA[Record-breaking extreme events, including heatwaves leading to surface melt and extreme snowfall, have been observed in Antarctica in recent years. Such extreme events are generally expected to become more frequent and intense with anthropogenic climate change. However, they are not typically considered in the climatic forcing used as the surface boundary condition for ice-sheet models projecting Antarctic mass changes into the future. With a suite of numerical ice-sheet simulations, we explore the additional Antarctic contribution to future sea-level rise when including atmospheric temperature extremes of varying frequency and intensity in projections. Our results suggest that by 2100, increasingly severe and frequent heatwaves have a limited effect on sea-level rise. However, by 2300, atmospheric extreme events could amplify sea-level rise by more than 2 m as atmosphere impacts on Antarctica contribute, rather than mitigate, ice loss. This study also highlights substantial uncertainties in ice-atmosphere interactions (e.g. the role of surface albedo) that amplify the sea-level rise response in an interlinked manner and play a key role in determining future sea-level rise.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6030</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6030/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147355</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Persistent increases in bioaccessible iron deposition from anthropogenic processing activities to the North Pacific and Indian Oceans despite rapid decreases from fuel combustion sources]]></dc:title>
      <dc:creator>Ito, Akinori</dc:creator>
      <dc:creator>Kurisu, Minako</dc:creator>
      <dc:description><![CDATA[The trend of atmospheric deposition of bioaccessible iron (BFe) from anthropogenic sources is driven by changes in aerosol column loading of total Fe (TFe) and Fe bioaccessibility, primarily due to the evolution of human activities. Black carbon (BC) is often used as a temporal and spatial proxy for BFe emissions from anthropogenic aerosols. However, derived changes in BFe concentrations from anthropogenic processing activities (e.g., smelting and abrasion) and fuel combustion have not been explored separately because of a lack of evaluation of BFe aerosols for separate anthropogenic sources. The Fe stable isotope ratio (&delta;<sup>56</sup>Fe) of size-segregated aerosols is a useful tracer to disentangle anthropogenic Fe sources. Here, we evaluate the source contributions predicted by an atmospheric chemical transport model using size-segregated aerosol observations over the North Pacific. Using the improved model, we investigate the relative changes in BFe aerosols from anthropogenic processing activities and fuel combustion sources in the major continental outflow regions during 2002&ndash;2022. The model reveals a persistent increase in BFe supply to the North Pacific and Indian Oceans from anthropogenic processing activity sources from 2002 (18 Gg Fe yr<sup>&minus;1</sup>) to 2022 (20 Gg Fe yr<sup>&minus;1</sup>) despite a decrease from fuel combustion from 2012 (20 Gg Fe yr<sup>&minus;1</sup>) to 2022 (15 Gg Fe yr<sup>&minus;1</sup>). These findings may have important implications for projections of future micronutrient supply to the oceans, which regulates the magnitude and dynamics of marine primary productivity.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6118</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6118/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147179</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[An overview of FRIDA v3.1: An update to a feedback-based, fully coupled, global integrated assessment model of climate and humans]]></dc:title>
      <dc:creator>Schoenberg, William</dc:creator>
      <dc:creator>Blanz, Benjamin</dc:creator>
      <dc:creator>Rajah, Jefferson K.</dc:creator>
      <dc:creator>Callegari, Beniamino</dc:creator>
      <dc:creator>Wells, Christopher</dc:creator>
      <dc:creator>Putranti, Theresia B.</dc:creator>
      <dc:creator>Mahu, Francisco</dc:creator>
      <dc:creator>Molina, Maria</dc:creator>
      <dc:creator>Köberle, Alexandre C.</dc:creator>
      <dc:creator>Li, Catherine</dc:creator>
      <dc:creator>Costa, Wanderson</dc:creator>
      <dc:creator>Collste, David</dc:creator>
      <dc:creator>Zwetsloot, Karel</dc:creator>
      <dc:creator>Breier, Jannes</dc:creator>
      <dc:creator>Ramme, Lennart</dc:creator>
      <dc:creator>Smith, Chris</dc:creator>
      <dc:creator>Mauritzen, Cecilie</dc:creator>
      <dc:description><![CDATA[The Feedback-based knowledge Repository for IntegrateD Assessments (FRIDA) v3.1 is a fully coupled climate-human systems model designed to explore the global long-term co-evolution of environmental, technological, economic, financial, and social processes under deep uncertainty. While many integrated assessment models represent climate damages primarily through aggregate economic impacts, important feedbacks among human behaviour, energy systems, land use, climate impacts, technological change, and financial stability remain weakly represented or exogenous. FRIDA v3.1 addresses this limitation through a system dynamics framework that embeds these processes within a unified feedback-rich structure, enabling emergent dynamics to arise from interactions across sectors rather than from externally prescribed assumptions. Building on earlier model versions, FRIDA v3.1 introduces representations of climate-driven wildfire dynamics, endogenous fertilizer use, sectorally disaggregated and behaviourally-informed energy demand, climate impacts on wind energy productivity, endogenous life expectancy, carbon capture and storage technologies, and macro-financial policy mechanisms designed to reduce climate-related financial risks. The model integrates these additions with existing representations of the climate system, carbon cycle, hydrology, population, economy, agriculture, land use, and energy supply. Calibration and evaluation against a large historical dataset and extensive uncertainty ensembles show that the updated model reproduces history while generating novel feedbacks that influence future development pathways. FRIDA v3.1 advances the capacity of integrated assessment modelling to investigate how behavioural, biophysical, technological, and financial processes jointly shape climate outcomes, providing a transparent and computationally efficient platform for uncertainty analysis, scenario exploration, and policy assessment in a rapidly changing world.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5980</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5980/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147065</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[From Surface Warming to Vertical Phytoplankton Reorganization in the North Pacific Subtropical Gyre]]></dc:title>
      <dc:creator>Adroli, Nurmalia</dc:creator>
      <dc:creator>Letelier, Ricardo</dc:creator>
      <dc:creator>Berlianty, Dessy</dc:creator>
      <dc:creator>Harte, Michael</dc:creator>
      <dc:creator>Strutton, Peter</dc:creator>
      <dc:creator>Ellwood, Michael J.</dc:creator>
      <dc:description><![CDATA[The North Pacific Subtropical Gyre (NPSG) has experienced sustained warming and biological change in recent decades, yet how these changes through the water column are less well resolved. Here, we combined satellite observations from 1998&ndash;2024 with physical and biogeochemical Argo data and a long-term record from Station ALOHA to examine changes across the upper 300 m. Surface chlorophyll declined as sea-surface temperature increased. A marked physical transition around 2013&ndash;2014 involved changes in mixed-layer depth, ocean heat content, density structure, and the separation between the mixed layer and euphotic-zone depth. Subsequent biological changes were strongly depth-dependent, with chlorophyll declining most in the 75&ndash;105 m range, and the deep chlorophyll maximum deepened despite a comparatively stable euphotic-zone depth. These chlorophyll changes did not translate directly into changes in phytoplankton carbon biomass. In the upper water column, recent carbon biomass increased even as chlorophyll declined, while increases in chlorophyll relative to carbon at depth suggested that the deepening chlorophyll maximum did not simply represent a deeper biomass maximum. Station ALOHA observations also revealed depth-dependent changes in phytoplankton community composition that may have added to these patterns. Together, these results show that long-term warming in the NPSG has occurred alongside a reorganization of upper-ocean physical structure and phytoplankton vertical distribution, rather than a uniform decline in phytoplankton biomass through the water column.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5927</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5927/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147468</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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      <dc:title><![CDATA[Subtropical gyres dominate global calcium carbonate production by coccolithophores]]></dc:title>
      <dc:creator>Wiseman, Nicola A.</dc:creator>
      <dc:creator>Vries, Joost</dc:creator>
      <dc:creator>Poulton, Alex J.</dc:creator>
      <dc:creator>Marsh, Nichole J.</dc:creator>
      <dc:creator>Wolf, Levi J.</dc:creator>
      <dc:creator>Monteiro, Fanny M.</dc:creator>
      <dc:description><![CDATA[Marine calcifying phytoplankton known as coccolithophores are a key part of the ocean carbon cycling, contributing to both the export of organic matter via the biological pump and the establishment of the vertical seawater alkalinity gradient known as a the carbonate counter pump. As dominate producers of calcium carbonate production, the rate at which coccolithophores produce calcium carbonate, determines the magnitude of the carbonate counter pump, and is sensitive to future changes in temperature, pH, and nutrient and light availability. Our understanding of spatiotemporal distributions of calcium carbonate production is limited, as measuring calcium carbonate production at sea is labour-intensive, and currently biased both seasonally and spatially. Here we leverage novel machine learning techniques to predict calcium carbonate production on a global scale to a depth of 200m, providing resolution with depth that has not been possible for previous remote sensing based approaches. We find a global integrated annual production of 1.23 PgC/yr [0.78&ndash;1.71], with the majority (59%) occurring in the subtropical gyres, challenging the dominance of more-often studied high latitude bloom regions. Our model also shows 18% of global annual CP occurring below the euphotic zone. Our results highlight the need for additional sampling and process studies in the subtropical gyres and at low lights levels/deep in the water column in particular to further constrain our understanding of the ocean carbonate cycle.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6172</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6172/]]></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:egusphere147471</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Technical note: MixSIAPy &ndash; Bayesian stable isotope mixing models in Python with multi-backend inference and formula-based compositional regression]]></dc:title>
      <dc:creator>Yang, Jing</dc:creator>
      <dc:creator>Dai, Heng</dc:creator>
      <dc:creator>Ye, Ming</dc:creator>
      <dc:creator>Cheng, Su</dc:creator>
      <dc:creator>Zhao, Yonghua</dc:creator>
      <dc:creator>Qian, Hui</dc:creator>
      <dc:description><![CDATA[Bayesian stable isotope mixing models quantify source contributions, but environmental studies increasingly require testing how multiple interacting drivers alter entire source compositions. The widely used R package MixSIAR restricts covariate structures, while post <em>hoc</em> regression of estimated proportions neither propagates posterior uncertainty nor preserves compositional dependence. Its reliance on a separately installed JAGS engine also constrains direct evaluation of gradient based samplers and accelerator-aware computation. We here introduce MixSIAPy, an open-source Python framework addressing these statistical and computational limitations while retaining established MixSIAR model structures. Its principal methodological contribution is formula-based compositional regression embedded directly in the mixing-model likelihood. Multiple categorical and numerical predictors and their interactions act jointly on source compositions in isometric log-ratio coordinates, with regression, grouping, source, and error parameters estimated in one posterior. A single PyMC model can be fitted through four interchangeable No-U-Turn Sampler backends, enabling CPU sampling and optional GPU execution. A shared engine supports scripted, local graphical, and hosted web workflows with reproducible outputs. Across 20 paired benchmarks, 19 converged in both implementations and showed close posterior correspondence; MixSIAPy reached an acceptable posterior faster in 13 cases. Backend performance was model dependent, and GPUs became advantageous only for some models at high chain parallelism. In an additional crop-water-uptake case study, the model identified a biomass associated shift from shallow to middle soil water in linseed, whereas broader effects remained uncertain. MixSIAPy thus enables interacting environmental controls to be tested within source-partitioning models instead of through separate analyses of uncertain estimated proportions.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6173</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6173/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere147484</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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      <dc:title><![CDATA[Circulation, tides, and mixing at a seamount off the Antarctic Peninsula]]></dc:title>
      <dc:creator>Yamazaki, Kaihe</dc:creator>
      <dc:creator>Heywood, Karen J.</dc:creator>
      <dc:creator>Damerell, Gillian M.</dc:creator>
      <dc:creator>Azaneu, Marina</dc:creator>
      <dc:creator>Jakes, Maya I.</dc:creator>
      <dc:description><![CDATA[Seamounts are hotspots of ocean mixing and current&ndash;topography interactions. This study investigates the circulation, tidal influence, and potential for instabilities and mixing over a seamount on the South Scotia Ridge near the tip of the Antarctic Peninsula. The seamount is 20&ndash;50 km across and rises from 1200 m to within 300 m of the surface. It is known to host a stationary anticyclonic eddy associated with the bifurcation of the Antarctic Slope Front, yet the underlying dynamics remain unclear. We analyse in situ hydrographic and velocity data from two Seaglider surveys, complemented by a barotropic tide model and satellite measurements. Horizontal velocities derived from glider drift reveal a complex interplay between topography and energetic tides of up to 0.8 m s⁻&sup1;. De-tided residuals reveal an anticyclonic circulation of 0.1&ndash;0.3 m s⁻&sup1; around the seamount, with a transport of about 1.5 Sv. The observations support the presence of a stratified Taylor column and topographic steering. Diagnostics suggest that tidal rectification accounts for up to 66 % of the residual current. An upscale energy transfer from small-scale turbulence over the slope may supply the additional energy required to maintain the eddy. Strong tides over the steep topography favour internal tide generation and hydraulic control, while weak stratification and strong horizontal shear leave the flow susceptible to submesoscale instability. Stratification is reduced over the summit, where vigorous turbulent mixing counteracts frictional downwelling and supports net upwelling, creating a diapycnal chimney over the seamount. Overall, the seamount emerges as a dynamic site for localised energy dissipation and upwelling, with implications for sea ice retreat, iceberg drift, and nutrient supply to the euphotic zone. Similar conditions are expected at other tidally energetic seamounts in high latitudes, where the dominant diurnal tidal constituents are subinertial.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-6184</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6184/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145880</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Evaluating metre-scale methane plume simulations with MicroHH against AVIRIS-4 remote sensing observations]]></dc:title>
      <dc:creator>Meier, Sandro</dc:creator>
      <dc:creator>Brunner, Dominik</dc:creator>
      <dc:creator>Kuhlmann, Gerrit</dc:creator>
      <dc:description><![CDATA[High-resolution imaging spectrometers resolve anthropogenic plumes at metre to sub-metre scales, creating opportunities for emission quantification but requiring models that reproduce turbulent plume morphology at comparable resolution. We evaluate the large-eddy simulation model MicroHH against Airborne Visible/Infrared Imaging Spectrometer (AVIRIS-4) observations from 2024 controlled releases in France. Using site-specific wind, surface, and source parameters, we simulated the four releases with the longest plumes at 1 m horizontal resolution. Synthetic CH<sub>4</sub> column enhancements were evaluated using plume structure, turbulence spectra, Gaussian cross-section statistics, along-plume flux variability, and plume power spectral density. For one release with a pronounced double plume, we integrated the three-dimensional model field along the slant illumination and viewing paths to investigate parallax effects. MicroHH reproduced the expected inertial-subrange behaviour of turbulent kinetic energy spectra and observed plume width, intermittency, and spatial power spectra for most releases. However, modelled vertical columns were more Gaussian than the observations and did not reproduce the double plumes. The exploratory slant-path calculation generated a comparable double structure, indicating that observational geometry can explain part of this discrepancy. Other differences likely reflect rapid near-source dilution at finite grid resolution, the absence of online plume-rise and buoyancy treatments, and omitted obstacle effects on near-surface flow. Overall, MicroHH can generate realistic high-resolution synthetic plume imagery for retrieval evaluation and machine-learning applications when inputs are well constrained and observational geometry is considered. This first systematic multi-metric comparison of LES plume morphology with metre-scale imaging-spectrometer observations provides a validation framework for other high-resolution dispersion models.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5235</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5235/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146024</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Organic and inorganic proxy development for advective heat flux in a basal-melt-dominated glacial system: Petermann Fjord, North Greenland]]></dc:title>
      <dc:creator>Davies, Joanna</dc:creator>
      <dc:creator>Middleton, Jennifer</dc:creator>
      <dc:creator>Harning, David</dc:creator>
      <dc:creator>Washam, Peter</dc:creator>
      <dc:creator>D'Andrea, William</dc:creator>
      <dc:creator>Reilly, Brendan</dc:creator>
      <dc:description><![CDATA[Mass loss from the Greenland Ice Sheet directly impacts sea level rise and the freshwater balance of the ocean. Petermann Glacier, North Greenland, provides a unique setting to explore atmosphere-ocean-ice interactions in a basal melt&ndash;dominated system using proxy records. We analyse organic (sea ice-associated highly branched isoprenoids (HBIs) and open water phytoplankton sterols) and inorganic (<sup>10</sup>Be, <sup>230</sup>Th) proxies from five sediment cores spanning the inner to outer Petermann Fjord to investigate oceanic advection and glacial dynamics, during times when the ice shelf occupied extended (after 0.6 ka BP) and reduced (pre-0.6 ka BP) positions. Results show higher fluxes of <sup>10</sup>Be, HBIs, and sterols during the reduced ice shelf phase. However, <sup>10</sup>Be, HBIs, and sterols are also present in sediments deposited when the ice shelf was extended, suggesting lateral advection and glacial meltwater contribute to their deposition. Whilst <sup>10</sup>Be has previously been applied as a proxy for ice shelves and perennial sea ice, in Petermann Fjord our results indicate that lateral advection, enhanced by buoyant subglacial melt, is the dominant source of <sup>10</sup>Be, with glacial melt providing secondary input. Our study highlights the potential to use a multi-proxy approach to reconstruct circulation regimes and advective heat flux patterns in basal-melt-dominated environments.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5321</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5321/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145824</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[PyAges v1.0: an extensible Python toolkit for inferring groundwater transit-time distributions from environmental tracers]]></dc:title>
      <dc:creator>Dreuzy, Jean-Raynald</dc:creator>
      <dc:creator>Leray, Sarah</dc:creator>
      <dc:creator>Marçais, Jean</dc:creator>
      <dc:description><![CDATA[Lumped-parameter models infer groundwater transit-time distributions by combining environmental-tracer input histories with parameterized age distributions. Their practical use requires flexible tracer representation, reliable repeated numerical integration, and explicit treatment of uncertainty when different parameter combinations fit observations similarly. We present PyAges v1.0, an open-source Python toolkit that separates tracer definitions, lumped-parameter models, convolution, and calibration; supports Bayesian inference of parameter uncertainty; and uses an integration scheme based on the cumulative distribution function and partial first moment for repeated evaluation of narrow, shifted, mixed, and shape-free transit- time distributions. Independent reference calculations across 270 cases characterize numerical discrepancies of the PyAges convolution operator across four classical model families. A cross-software benchmark against TracerLPM shows that both tools estimate the prescribed parameters with broadly comparable accuracy. Mean transit time is estimated more robustly under added noise than the model- specific parameter controlling either exponential&ndash;piston mixing or dispersion. Two field sites, Holten and Ploemeur, illustrate the framework with real observations. At Holten, PyAges posterior medians reproduce all 28 published four-bin age fractions within 0.02. At Ploemeur, calibrations using the full record or only 2014&ndash;2015 observations show how repeated measurements can resolve age ambiguity or reveal incompatibility among the assumptions used to interpret the tracers. PyAges therefore provides a reproducible framework for testing tracer and transit-time hypotheses, determining what observations constrain, and integrating tracer inference into broader hydrogeological workflows.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5201</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5201/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146047</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Long-duration shipboard performance of a humidity-conditioned optical particulate matter monitor along inter-polar transit routes: Antarctic inter-unit agreement and Arctic redeployment]]></dc:title>
      <dc:creator>Son, Myunghee</dc:creator>
      <dc:creator>Baek, Sung Hoon</dc:creator>
      <dc:description><![CDATA[Optical particulate matter (PM) measurements aboard ships are vulnerable to relative-humidity (RH)-dependent particle growth, sampling disturbances, and platform exhaust. We evaluated the long-duration field performance of the Tiny Aerosol Monitor with Tiny Aerosol Conditioner (TAM/TAC) using two co-deployed instruments during an Antarctic voyage and the subsequent Arctic redeployment of the same physical instrument (unit 70). The Antarctic loggers recorded every scheduled 10 min time step from 25 October 2022 to 3 May 2023 (27,342 records per unit), and unit 70 recorded every scheduled time step during the Arctic deployment from 21 June to 11 October 2023 (16,124 records). A prespecified quality-control rule excluded 50 Antarctic unit-70 records with nonzero instrument status codes, leaving 27,292 valid Antarctic pairs; unit 71 and the Arctic unit-70 dataset contained no flagged records. Across PM₁.₀, PM₂.₅, PM₄.₀, and PM₁₀, Antarctic inter-unit correlations were 0.995&ndash;0.997, equal-variance Deming slopes were 0.992&ndash;1.033, and relative mean biases were &minus;1.1 % to +2.1 %. Paired relative precision was 9.0&ndash;9.8 % for PM₂.₅&ndash;PM₁₀ and 16.3 % for PM₁.₀, for which the route-wide mean was only about 1.53 &micro;g m⁻&sup3;. In the polar subsets, TAC reduced mean ambient RH from 54.0 % to 32.2 % in the Antarctic and from 73.7 % to 34.5 % in the Arctic; internal RH was at or below 40 % for 99.99 % and 100 % of valid records, respectively. These results provide evidence of timebase continuity, inter-unit comparability, and repeatable humidity control across two extreme marine deployments. They do not establish absolute accuracy, inlet efficiency, or freedom from ship-exhaust contamination, which require a collocated reference instrument and ship-relative wind or exhaust-tracer measurements.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5333</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5333/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145564</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Theory of Recession Based on Concepts from Percolation Theory]]></dc:title>
      <dc:creator>Hunt, Allen Gerhard</dc:creator>
      <dc:creator>Mohan, Sonali</dc:creator>
      <dc:creator>Zhang, Yongqiang</dc:creator>
      <dc:creator>Krajewski, Witold</dc:creator>
      <dc:creator>Duan, Qingyun</dc:creator>
      <dc:description><![CDATA[Using the definition of recession as the decline in streamflow following a rainfall event peak and before the next peak (provided evapotranspiration may be neglected), recession defines the relationship between catchment storage and outflow. The present analysis addresses the limiting processes absent in existing recession analysis, which are nonetheless treatable in the language of percolation theory. This includes: a) a universal decline in hydraulic conductivity as the percolation threshold is approached, and b) a universal decline in accessible moisture content beyond the simple decline in overall moisture content. The process of addressing these two time-dependent phenomena generates the basic structure of recession response: 1) linear response for an average of multiple events, 2) the corresponding time frame variation, 3) the specific characteristics of its non-linear response, specifically, its convexity.&nbsp; The present approach results in an absolute value of the non-linearity that is still underestimated as compared to results published in the literature.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5030</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5030/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145674</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Boundary Layer Characteristics of a Land-Terminating Ice Cliff &ndash; Turbulence Measurements from the Summit of Kilimanjaro, Tanzania]]></dc:title>
      <dc:creator>Schroeder, Marie</dc:creator>
      <dc:creator>Stiperski, Ivana</dc:creator>
      <dc:creator>Winkler, Michael</dc:creator>
      <dc:creator>Kaser, Georg</dc:creator>
      <dc:creator>Steiner, Jakob</dc:creator>
      <dc:creator>Abermann, Jakob</dc:creator>
      <dc:creator>Wohlfahrt, Georg</dc:creator>
      <dc:creator>Prinz, Rainer</dc:creator>
      <dc:description><![CDATA[Land-terminating ice cliffs (LTICs) are common features of glacier margins that can contribute disproportionately to glacier ablation, yet direct observations of their boundary-layer structure and turbulent exchange are almost entirely lacking. Here, we analyse a unique 42.5-hour eddy-covariance dataset collected at a 25 m tall near-vertical ice cliff on the summit glaciers of Kilimanjaro, Tanzania, to investigate the microclimate, turbulence structure, and surface&ndash;atmosphere exchange associated with an LTIC. The measurements reveal a geometry-induced secondary circulation superimposed on the prevailing along-cliff flow, with air moving towards and ascending the cliff during daytime and reversing at night. Strong thermal contrasts between the warm volcanic ash forefield and the cold ice surface produced pronounced spatial heterogeneity in turbulence. While the upper cliff exhibited a coherent, wall-bounded turbulence regime consistent with locally generated exchange, the cliff foot was characterized by disrupted turbulence, counter-gradient transport, and evidence of flow separation associated with the cliff geometry. Using these observations, we evaluate the applicability of a classical bulk aerodynamic parameterization to a near-vertical glacier surface. Despite the unconventional geometry, the bulk method reproduced the observed sensible and latent heat fluxes well at the upper cliff with an RMSE of 5.2 and 3.3 W m<sup>-2</sup>, respectively. At the cliff foot, the bulk method failed to capture the nighttime flux reversal, indicating that local turbulence structure, rather than surface slope alone, determines the validity of bulk parameterizations. Compared with previous measurements over Kilimanjaro's adjacent flat glacier surface, the LTIC exhibited substantially weaker latent heat fluxes, suggesting a shift from the sublimation-dominated regime characteristic of the plateau glaciers toward a comparatively more melt-dominated energy balance at the cliff. These observations provide the first field-based characterization of turbulence at a LTIC and point towards the idea that steep glacier margins can sustain coherent boundary-layer exchange despite their near-vertical geometry, with implications for understanding and modelling turbulent heat exchange over complex glacier terrain. Given the short duration and single-site nature of the observations, these findings should be regarded as a first case-study insight into LTIC boundary-layer processes rather than a general characterization of turbulent exchange at steep glacier margins.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5112</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5112/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:egusphere145490</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
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      <dc:title><![CDATA[A comparison of the accuracy and stability of numerical schemes used to solve the equations derived from the shallow-shelf approximation]]></dc:title>
      <dc:creator>Rhee, Deborah</dc:creator>
      <dc:creator>Sun, Sainan</dc:creator>
      <dc:creator>Gudmundsson, G. Hilmar</dc:creator>
      <dc:description><![CDATA[The shallow-shelf approximation (SSA) is widely used to model the evolution of fast-flowing ice that is either floating or sliding rapidly over the bed, resulting in plug flow. However, so far there has been no rigorous, comparative study of the different numerical approaches to solve the SSA equations. We calculate the conditions for different numerical schemes to remain stable and accurate when solving the linear 1D SSA equations for a simple geometry. The comparison spans central difference and upwind schemes, explicit and semi-implicit multistep schemes, and explicit or implicit monolithic schemes. Also considered are schemes time stepping using the &Theta;-method, where the value of &Theta; is used to form a weighted combination of the forward and backward Euler methods. We find that monolithic schemes remain stable at all tested time steps for &Theta; &ge; 0.5 whilst multistep schemes become unstable at large time steps. Of the tested schemes the monolithic finite element scheme with &Theta; = 0.5 remains accurate for the largest range of time steps.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4978</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4978/]]></dc:identifier>
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      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145487</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
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      <dc:title><![CDATA[A magnetite reference material for LA-ICP-MS U&ndash;Pb geochronology from the Troodos Ophiolite, Cyprus]]></dc:title>
      <dc:creator>Beranoaguirre, Aratz</dc:creator>
      <dc:creator>Peillod, Alexandre</dc:creator>
      <dc:creator>Dunkl, Istvan</dc:creator>
      <dc:creator>Patten, Clifford G. C.</dc:creator>
      <dc:creator>Hector, Simon</dc:creator>
      <dc:creator>Junge, Malte</dc:creator>
      <dc:creator>Kolb, Jochen</dc:creator>
      <dc:creator>Gerdes, Axel</dc:creator>
      <dc:description><![CDATA[Magnetite is an increasingly important target material for in situ geochemical analysis and has recently emerged as a promising U&ndash;Pb geochronometer. However, the wider application of the method is hindered by the lack of a widely available matrix-matched reference material. Here we propose TR41, a hydrothermal magnetite from the Troodos ophiolite (Cyprus), as a candidate reference material for LA-ICP-MS U&ndash;Pb magnetite geochronology. Petrographic, geochemical, and isotopic data demonstrate that TR41 is sufficiently homogeneous for laser ablation analyses and yields clearly defined regressions in Tera&ndash;Wasserburg diagram despite U concentrations below 1 &micro;g g<sup>-1</sup>. As independent ID-TIMS characterisation of magnetite is currently not feasible, the age of TR41 was constrained using complementary geochronological approaches. U&ndash;Pb dating of coexisting hydrothermal andradite yields a lower-intercept age of 92.04 &plusmn; 2.23 Ma. Assuming that the andradite and magnetite formed during the same hydrothermal event, four blind-test samples containing coexisting magnetite and garnet or apatite were analysed. In all cases, magnetite ages obtained using TR41 as the primary reference material agree, within uncertainty, with independently determined ages of the associated minerals. These results demonstrate that TR41 provides an appropriate matrix correction for LA-ICP-MS U&ndash;Pb analyses of magnetite and represents a practical reference material for expanding the magnetite U&ndash;Pb geochronology. TR41 is available for distribution to interested laboratories upon request from the corresponding author.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4975</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4975/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere146181</identifier>
    <datestamp>2026-10-12</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[FORTE 3.0 and its simulation of equatorial Pacific warming]]></dc:title>
      <dc:creator>Robbins, Connor</dc:creator>
      <dc:creator>Gollop, Amee</dc:creator>
      <dc:creator>Joshi, Manoj</dc:creator>
      <dc:creator>Stevens, David P.</dc:creator>
      <dc:creator>Webb, Mark J.</dc:creator>
      <dc:creator>Blaker, Adam T.</dc:creator>
      <dc:creator>Chadwick, Robin</dc:creator>
      <dc:description><![CDATA[FORTE 3 is an intermediate-resolution coupled atmosphere&ndash;ocean general circulation model (AOGCM) consisting of the Intermediate General Circulation Model 4 (IGCM4.1), a T42 spectral atmosphere with 35 <em>&sigma;</em>-layers, coupled to Modular Ocean Model &ndash; Array (MOMA), a 2&deg; &times; 2&deg; ocean with 15 z-layer depth levels. It is a significant upgrade from its predecessor, the fast flexible AOGCM FORTE2, in terms of its mean climate and climate response. The model has been compiled using the Intel ifx compiler. Here we describe the changes between FORTE2 and FORTE3 and demonstrate its use by simulating global and Pacific ocean change under both idealised CO<sub>2</sub> forcing and stratospheric O<sub>3</sub> depletion. In the atmosphere a new formulation for convective entrainment in IGCM4.1 alleviates a cold upper tropospheric bias in IGCM4. The formulation for precipitating convection has been changed to reduce an existing strong negative cloud forcing bias in the model, and a new formulation for stratocumulus cloud has been introduced. Effects of changes are especially evidenced in climate simulations: the transient climate response in FORTE3 is 1.8 K, and the equilibrium climate sensitivity in a slab version of IGCM4.1 is 4.2 K, compared to FORTE2/slab IGCM4 values of 1.0 K and 2.1 K respectively, and are more consistent with CMIP6 GCMs and observations. In the ocean, a new parameterisation of equatorial mixing based on the meridional sea surface temperature gradient alleviates the equatorial cold bias. The Atlantic Meridional Overturning Circulation at 30&deg; N is 17 Sv, while the transport of the Antarctic Circumpolar Current is 130 Sv, slightly stronger, and more in agreement in observations than FORTE2. We demonstrate the use of FORTE3 by conducting sensitivity experiments where CO<sub>2</sub> is increased by 1 % per year. We find that the introduction of a "high-volume" Andes mountain range does not change the pattern of global warming over the Pacific Ocean; conversely, the effect of stratospheric O<sub>3</sub> depletion does appear to change the equatorial Pacific gradient slightly.]]></dc:description>
      <dc:date>2026-10-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-5372</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5372/]]></dc:identifier>
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      <dc:language>eng</dc:language>
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