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    <identifier>oai:publications.copernicus.org:tc133738</identifier>
    <datestamp>2026-08-13</datestamp>
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      <dc:title><![CDATA[Experimental investigation of the direct shear strength parameters of compacted snow]]></dc:title>
      <dc:creator>Huo, Haifeng</dc:creator>
      <dc:creator>Xu, Hui</dc:creator>
      <dc:creator>Wu, Jixiu</dc:creator>
      <dc:creator>Li, Tao</dc:creator>
      <dc:creator>Liu, Jingjin</dc:creator>
      <dc:creator>Xiao, Enzhao</dc:creator>
      <dc:creator>Tang, Xueyuan</dc:creator>
      <dc:description><![CDATA[<p>Compacted snow is utilized as a building material in various construction and engineering applications across global high-latitude regions. For the safety assessment of snow and ice structures in cold regions, cohesion and internal friction angle are key shear strength parameters for compacted snow. Direct shear tests were carried out on low-density natural snow and high-density artificial snow in a <span class="inline-formula">−</span>10 °C cold laboratory. In total, 112 test conditions were designed to quantify the effects of initial density, sintering time and sintering temperature on shear strength parameters at normal stresses below 100 kPa. Results show that under high sintering degree conditions and low normal pressures, the shear stress–displacement curve tends to exhibit strain softening. As initial density increases from 300 to 650 kg m<span class="inline-formula"><sup>−3</sup></span>, both cohesion and internal friction angle increase linearly. With sintering time increasing from 0 to 60 d, cohesion first rises and then falls, while the internal friction angle steadily decreases. As sintering temperature decreases from <span class="inline-formula">−</span>5 to <span class="inline-formula">−</span>25 °C, cohesion decreases, whereas the internal friction angle increases slightly. A Genetic Algorithm-Back Propagation (GA-BP) neural network was utilized to construct a shear strength prediction model, taking density, sintering time, sintering temperature, and normal stress as inputs, and offering benchmark values for cohesion and internal friction angle under various conditions. These benchmarks can be adaptively adjusted when additional influencing factors require consideration. This study provides essential strength parameters for the design and construction of compacted snow structures and offers a framework for accounting for the influence of other factors on these parameters.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/tc-20-4401-2026</dc:identifier>
      <dc:identifier><![CDATA[https://tc.copernicus.org/articles/20/4401/2026/]]></dc:identifier>
      <dc:source>eISSN: 1994-0424</dc:source>
      <dc:language>eng</dc:language>
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    <identifier>oai:publications.copernicus.org:sand140080</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>sand</setSpec>
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      <dc:title><![CDATA[The long history of promises by accelerator-driven systems]]></dc:title>
      <dc:creator>Frieß, Friederike</dc:creator>
      <dc:creator>Steigerwald, Björn</dc:creator>
      <dc:creator>Vogt, Yannick</dc:creator>
      <dc:description><![CDATA[<p>The use of accelerator-driven systems (ADSs) for transmuting high-level radioactive waste has attracted renewed attention, spurred in part by startups. In such systems, selected radionuclides are converted into other (radio)nuclides through nuclear reactions, particularly fission. ADSs couple an external neutron source to a subcritical reactor, offering greater flexibility in fuel composition compared to critical reactors. Although the idea dates back several decades, no systems have yet been implemented.</p>        <p>We argue that the core technological concept remains largely unchanged from earlier proposals and therefore inherits many of the same challenges – notably high costs and engineering complexity. We examine the potential role of radioisotope production as an additional revenue stream beyond electricity generation and waste incineration in more detail. We find that the projected contribution of radioisotope production to the overall economics of ADS facilities is highly sensitive to assumptions about market size, price stability, and deployment scale.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/sand-5-11-2026</dc:identifier>
      <dc:identifier><![CDATA[https://sand.copernicus.org/articles/5/11/2026/]]></dc:identifier>
      <dc:source>eISSN: 2749-4802</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:spd145141</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>spd</setSpec>
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      <dc:title><![CDATA[The pause of a decade-long warm water state of central Scotian Shelf in 2024&ndash;2025]]></dc:title>
      <dc:creator>Lu, Youyu</dc:creator>
      <dc:creator>Zhai, Li</dc:creator>
      <dc:creator>Hu, Xianmin</dc:creator>
      <dc:creator>Layton, Chantelle</dc:creator>
      <dc:creator>Brickman, David</dc:creator>
      <dc:creator>Greenan, Blair</dc:creator>
      <dc:creator>Garric, Gilles</dc:creator>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
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      <dc:identifier>https://doi.org/10.5194/sp-2026-26</dc:identifier>
      <dc:identifier><![CDATA[https://sp.copernicus.org/preprints/sp-2026-26/]]></dc:identifier>
      <dc:source>eISSN: 2752-0706</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:jbji138506</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>jbji</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[In vitro analysis of antiseptic solution effects  on Staphylococcus aureus biofilms  on orthopedic implant materials]]></dc:title>
      <dc:creator>Balagtas, Madison</dc:creator>
      <dc:creator>Chrulski, Kenneth</dc:creator>
      <dc:creator>Feffer, Marina</dc:creator>
      <dc:creator>Baldridge, Matthew</dc:creator>
      <dc:creator>Levack, Ashley E.</dc:creator>
      <dc:description><![CDATA[<p>Implant-related biofilm infections remain a major challenge in orthopedic surgery. Prior in vitro comparisons have focused on arthroplasty surfaces using static models; fracture fixation implants remain unstudied. We compared six antiseptic solutions against mature <i>S. aureus</i> biofilms on stainless steel, the most common fracture fixation metal, using a continuous-flow CDC biofilm reactor, more closely approximating hydrodynamic surgical conditions than static systems. Mature biofilms were created on stainless steel coupons using a continuous-flow reactor for 72 h, then washed for 3 min with one of six irrigation solutions: normal saline, 10 % PI (povidone-iodine), 0.35 % PI, a 10 % PI <span class="inline-formula">+</span> 3 % hydrogen peroxide mixture, hypochlorous acid, or 0.05 % chlorhexidine gluconate. Colony-forming units (CFUs) were quantified following standardized sonication and plating, and mixed-effects negative binomial regression was used to estimate treatment effects. All antiseptic solutions produced statistically significant reductions in biofilm-associated CFUs relative to untreated controls. Ten percent PI demonstrated the greatest reduction (3.46-<span class="inline-formula">log <sub>10</sub></span>), with 0.35 % PI producing a similar 3.42-<span class="inline-formula">log <sub>10</sub></span> reduction. The PI–hydrogen peroxide mixture achieved a 3.24-<span class="inline-formula">log <sub>10</sub></span> reduction without evidence of synergistic activity. Hypochlorous acid and chlorhexidine produced 2.95-<span class="inline-formula">log <sub>10</sub></span> and 2.46-<span class="inline-formula">log <sub>10</sub></span> reductions, respectively, while saline demonstrated minimal effect. These findings indicate that PI solutions, even at dilute concentrations, are highly effective at disrupting established biofilms on stainless steel. As an in vitro single-organism model, these findings establish a comparative efficacy baseline on a fracture-fixation-relevant surface but require validation in multispecies, multi-material, and mechanically realistic irrigation systems before clinical translation.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/jbji-11-493-2026</dc:identifier>
      <dc:identifier><![CDATA[https://jbji.copernicus.org/articles/11/493/2026/]]></dc:identifier>
      <dc:source>eISSN: 2206-3552</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:hgssd145316</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>hgssd</setSpec>
   </header>
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     <oai_dc:dc
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      <dc:title><![CDATA[The Remarkable Scientist and Writer Ukichiro Nakaya and his "Black Moon" and "White Moon" Worlds]]></dc:title>
      <dc:creator>Hamilton, Kevin</dc:creator>
      <dc:creator>Ohfuchi, Wataru</dc:creator>
      <dc:description><![CDATA[The physicist Ukichiro Nakaya (1900&ndash;1962) is renowned in Japan for his contributions to snow and ice science and for his outstanding achievements as a writer and film maker. His meticulous field observations and his laboratory investigations led to seminal discoveries about snow crystals. Notably in 1936 Nakaya produced the world&rsquo;s first artificial snow crystal created in a cloud chamber. This allowed him to determine the systematic dependence of snow crystal shapes on the conditions at formation, a result now summarized in the widely known &ldquo;Nakaya diagram&rdquo;. In the 1950&rsquo;s Nakaya began collaborations with the US Snow, Ice and Permafrost Research Establishment investigating the properties of glacial ice, notably including fieldwork in Greenland during the pioneering years of the deep ice coring project there. Nakaya was a very prolific writer of essays published in Japanese magazines, and his essays were often republished in book collections, many still in print today. His writing for the general public about science has led to his reputation as &ldquo;The Carl Sagan of Japan&rdquo;, but his writing extended more broadly to many areas of culture. Nakaya was also a pioneer in making educational documentary films and he was instrumental in the formation of a major film studio in Japan.</p> <p>This article was initiated to mark Nakaya&rsquo;s 125th anniversary year and aims to introduce his life and achievements to a broad international audience. We review Nakaya&rsquo;s biography and highlights of his scientific career, and include some brief discussion of the Japanese cultural context for his scientific work. We recount some particularly dramatic aspects of Nakaya&rsquo;s life which was shadowed by the great historical developments of his era, notably the Second World War. We also review his contributions to Japanese literature of his time. We sample a handful of Nakaya&rsquo;s articles written for the general public in order to convey the scope and flavour of his literary <em>oeuvre</em>. We describe in detail two of Nakaya&rsquo;s most ambitious magazine essays: &ldquo;World of the Black Moon&rdquo; and &ldquo;World of the White Moon&rdquo;, which are of particular interest as vivid first person accounts of middle 20<sup>th</sup> century research field trips (to Hawaii and Greenland, respectively). &ldquo;World of the White Moon&rdquo; is also notable for including a very early description for the general public of the issue of anthropogenic climate change.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hgss-2026-12</dc:identifier>
      <dc:identifier><![CDATA[https://hgss.copernicus.org/preprints/hgss-2026-12/]]></dc:identifier>
      <dc:source>eISSN: 2190-5029</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:os140449</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>os</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
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      <dc:title><![CDATA[Thermohaline gradients and frontal regimes in the  northwestern Tropical Atlantic]]></dc:title>
      <dc:creator>Napolitano, Dante C.</dc:creator>
      <dc:creator>Gula, Jonathan</dc:creator>
      <dc:creator>Coadou-Chaventon, Solange</dc:creator>
      <dc:creator>Speich, Sabrina</dc:creator>
      <dc:creator>Rocha, Cesar B.</dc:creator>
      <dc:creator>McWilliams, James C.</dc:creator>
      <dc:creator>Zhang, Dongxiao</dc:creator>
      <dc:creator>Carton, Xavier</dc:creator>
      <dc:description><![CDATA[<p>At the edge of the Amazon River plume, stirring by the North Brazil Current (NBC) and its eddies creates sharp surface thermohaline gradients on horizontal scales of <span class="inline-formula">?</span> (1–100) <span class="inline-formula">km</span>. This study provides a comprehensive picture of these gradients and fronts associated with the region's distinctive dynamics. Saildrone observations show that the plume amplifies density gradient variability at all scales from 1–100 <span class="inline-formula">km</span>, with frontal sharpness up to <span class="inline-formula">75×</span> stronger inside the plume than outside, with differences reaching <span class="inline-formula">100×</span> at scales below 3 <span class="inline-formula">km</span>. Density gradients are partially reinforced or compensated by temperature-salinity variations, with net frontogenesis observed in both regions. To expand in-situ observations, we use a 1 <span class="inline-formula">km</span> resolution CROCO (Coastal and Regional Ocean COmmunity model) simulation to assess the spatial distribution of surface fronts and their spatio-temporal variability. We characterize three distinct frontal regimes: (i) broken-up fronts parallel to shore occupy the plume core over the continental shelf, (ii) thin elongated fronts associated with NBC-plume interactions connect nearshore and offshore regions, and (iii) pools of anisotropic fronts driven by the seasonal mixed-layer cycle are present offshore. Salinity dominates density gradients throughout the year north of 15° N, whereas near-shore fronts exhibit seasonal shifts in temperature-salinity dominance linked to the Amazon discharge seasonality and NBC strength. Within the plume, freshwater filaments stirred by NBC rings systematically generate density-compensated fronts on their inner edge and reinforced fronts on their outer rim, a pattern with implications for energy cascades and tracer export.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/os-22-2425-2026</dc:identifier>
      <dc:identifier><![CDATA[https://os.copernicus.org/articles/22/2425/2026/]]></dc:identifier>
      <dc:source>eISSN: 1812-0792</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:nhess139188</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>nhess</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[Attribution of the record breaking 2025 European fire season to climate change]]></dc:title>
      <dc:creator>Keeping, Theodore R.</dc:creator>
      <dc:creator>Zachariah, Mariam</dc:creator>
      <dc:creator>Haas, Olivia</dc:creator>
      <dc:creator>Grillakis, Manolis</dc:creator>
      <dc:creator>Barnes, Clair</dc:creator>
      <dc:creator>Clay, Gareth D.</dc:creator>
      <dc:creator>Ekberzade, Bikem</dc:creator>
      <dc:creator>Jaupaj, Orjeta</dc:creator>
      <dc:creator>Ribeiro, Andreia</dc:creator>
      <dc:creator>Trigo, Ricardo</dc:creator>
      <dc:creator>Voulgarakis, Apostolos</dc:creator>
      <dc:creator>Otto, Friederike E. L.</dc:creator>
      <dc:description><![CDATA[<p>The 2025 European fire season was historically extreme, with record-breaking burned area exceeding 1 400 000 ha, and multiple regionally unprecedented wildfires. Emerging fire regimes and extreme wildfire behaviour in Europe pose increasing adaptation challenges. Extreme event attribution of a recent fire season, combined with analysis of changes in vegetation and land use, provides insight into the effect of climate and environmental change on high impact events. We analyse five regions that experienced particularly extreme wildfire activity in 2025 (northwestern Iberia, western and northern Britain, Occitania, the eastern Adriatic/Ionian, and northern and western Türkiye) capturing a diverse range of driving weather conditions and fire regimes. Strong trends towards drier summers and extreme weekly vapour pressure deficit (VPD) were found, with summer drought emergent from natural variability in most southern European regions, and VPD extreme emergent in reanalysis data for all regions. Changes in VPD are the main reason why combined hot, dry, and windy conditions have become more frequent than expected from natural variability. This emergence is seen in both reanalysis data and climate models for the Iberian, Adriatic/Ionian and Turkish regions. In contrast, in the British and Occitanian regions, models do not show observed trends.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/nhess-26-3761-2026</dc:identifier>
      <dc:identifier><![CDATA[https://nhess.copernicus.org/articles/26/3761/2026/]]></dc:identifier>
      <dc:source>eISSN: 1684-9981</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:hess125096</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>hess</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[Systematic overestimation of evapotranspiration over irrigated areas by an offline land surface model]]></dc:title>
      <dc:creator>Lunel, Tanguy</dc:creator>
      <dc:creator>Martí, Belén</dc:creator>
      <dc:creator>Boone, Aaron</dc:creator>
      <dc:creator>Moigne, Patrick</dc:creator>
      <dc:description><![CDATA[<p>Offline Land Surface Models (LSMs) are essential for a wide range of applications, including water resource management and agricultural planning. A critical variable in these models is evapotranspiration, but its value is easily biased in irrigated areas. In fact, irrigation fundamentally alters local atmospheric conditions – cooling and humidifying the air and reducing wind speeds – factors that contribute to reducing evapotranspiration rates. This phenomenon is called “atmospheric feedback”, but is often missing or poorly represented in offline LSMs because most of the atmospheric forcings used, such as reanalyses and climate model outputs, overlook the atmospheric effect of irrigation. This leads to a tendency for offline LSMs to overestimate evapotranspiration rates over irrigated areas. In this study, the atmospheric effects of irrigation are quantified using data from the Land surface Interactions with the Atmosphere over the Iberian Semi-arid Environment (LIAISE) project field campaign. The various surface processes that influence the dynamics of evapotranspiration in response to the atmospheric feedback are then systematically investigated. The results confirm the importance of considering the atmospheric feedback in the Interactions Soil Biosphere Atmosphere (ISBA) LSM over irrigated areas in many configurations. For well irrigated crops, the average overestimation of evapotranspiration is about 25 %. Conversely, for water-stressed crops, this overestimation is negligible because of the delay in stomatal closure caused by the atmospheric feedback mechanisms, providing a compensatory effect which mitigates the overestimation. These findings highlight the need for improved representation of irrigation-related atmospheric feedback in the atmospheric forcings used as upper boundary conditions in LSMs to improve the accuracy of evapotranspiration estimates in agricultural or hydrological contexts.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/hess-30-5117-2026</dc:identifier>
      <dc:identifier><![CDATA[https://hess.copernicus.org/articles/30/5117/2026/]]></dc:identifier>
      <dc:source>eISSN: 1607-7938</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd140326</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
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       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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      <dc:title><![CDATA[BinMod1D v1.0.10: a Python package for explicitly simulating 1D collisional coalescence/breakup processes with corresponding polarimetric radar signatures]]></dc:title>
      <dc:creator>Dunnavan, Edwin Lee</dc:creator>
      <dc:description><![CDATA[<p>This paper details a computationally efficient and versatile Python package (BinMod1D v1.0.10) that explicitly evolves spectral bin distributions and corresponding polarimetric radar variables for rain or snow according to atmospheric collisional coalescence and breakup processes. BinMod1D can be executed as a box model, a 1D steady-state model in height, or a full (time and height) 1D column model utilizing multiple particle categories, each of which can have their own densities, aspect ratios, and fall speeds. Forward simulations of polarimetric radar variables are implemented using standard Rayleigh analytic scattering equations. Two-moment (mass and number) or one-moment (mass only) particle interaction calculations follow a source-based spectral bin method. Bin interaction computations are parallelized using just-in-time (JIT) compilation for high performance. BinMod1D box model solutions are validated using analytic solutions of collision-coalescence using a variety of kernels as well as for breakup and the steady-state balance of coalescence with breakup. BinMod1D capabilities are demonstrated through steady-state simulations of rainfall and snow signatures, as well as vertical profiles of diverse meteorological scenarios. Convergence and timing tests are provided for the meteorological scenario of a cloud to rain transition using a realistic collision kernel and fragment distribution. BinMod1D is intended to enable cloud microphysics and weather radar researchers to efficiently simulate vertical profiles of complex weather events. Such a tool can be used to provide reference solutions for training machine learning models and validating various retrieval methodologies.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-7503-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/7503/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd133759</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[Enhancing air–sea CO2 exchange and modulating seawater carbonate–pH dynamics: the role of wave effect mechanisms in the POP2–waves coupled model]]></dc:title>
      <dc:creator>Lan, Yung-Yao</dc:creator>
      <dc:creator>Hsu, Huang-Hsiung</dc:creator>
      <dc:creator>Lee, Wei-Liang</dc:creator>
      <dc:creator>Chou, Simon</dc:creator>
      <dc:description><![CDATA[<p>In this study, a wave module is online-coupled into the Parallel Ocean Program version 2 (POP2) within the CESM1.2.2 framework (hereafter POP2–waves). Unlike empirical data analyses of observation-based products and offline-forced ocean models that treat wave-induced gas transfer velocity and the air–sea difference in partial pressure of CO<span class="inline-formula"><sub>2</sub></span> (<span class="inline-formula">Δ<i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span>) as decoupled variables, the online-coupled POP2–waves model captures their interactive, <span class="inline-formula">Δ<i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span>-mediated negative feedbacks. This setup enables wave properties to dynamically modulate gas transfer velocity and physical mixing through sequential processes. POP2–waves is evaluated alongside a control simulation (B–CTL) against the National Oceanic and Atmospheric Administration (NOAA) CarbonTracker (CT2022) inversion product. The spatial air–sea CO<span class="inline-formula"><sub>2</sub></span> flux in POP2–waves simulation shows generally closer structural agreement with NOAA CT2022 than the control B–CTL, thereby improving performance in most selected regions. Specifically, bubble-mediated transfer accounts for up to 41.3 % of the total flux, consistent with the <span class="inline-formula">∼40</span> % contribution reported in recent research. Although the inclusion of waves (POP2–waves) enhances regional oceanic CO<span class="inline-formula"><sub>2</sub></span> uptake by 11.8 % and outgassing by 41.6 %, these two processes largely offset each other. Consequently, this dual enhancement results in only a slight 1.8 % increase in the global net ocean CO<span class="inline-formula"><sub>2</sub></span> sink compared to the B–CTL simulation. Globally, air–sea <span class="inline-formula">Δ<i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span> and pH exhibit the strongest positive and negative regression coefficients with the air–sea CO<span class="inline-formula"><sub>2</sub></span> flux, respectively. Regionally, the gas transfer velocity shows a positive (negative) regression coefficient within oceanic CO<span class="inline-formula"><sub>2</sub></span> outgassing (uptake) regions, whereas SST displays the opposite trend.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-7479-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/7479/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd136933</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[SDMBCv2 (v1.0): correcting systematic biases  in RCM inputs for future projection]]></dc:title>
      <dc:creator>Kim, Youngil</dc:creator>
      <dc:creator>Evans, Jason P.</dc:creator>
      <dc:description><![CDATA[<p>Regional Climate Models (RCMs) offer enhanced spatial resolution and a more realistic depiction of local climate processes. However, they often inherit systematic biases from their driving Global Climate Models (GCMs), which can compromise the accuracy of downscaled climate projections. To address this, bias correction techniques have been widely employed to adjust GCM and RCM outputs, particularly for climate impact and adaptation studies. Traditional methods, however, typically correct surface variables independently and lack physical and dynamical consistency. Bias correcting GCM boundary conditions prior to RCM simulation ensures a more coherent, physically and dynamically consistent, regional climate simulation with reduced errors. This study evaluates the effectiveness of such an approach using a calibration/validation framework, demonstrating significant error reduction during the validation (out-of-sample) period compared to uncorrected GCM data. We present an updated version of the open-source Python package, <i>Sub-Daily Multivariate Bias Correction (SDMBC) v2</i>, designed to correct RCM input variables using both reanalysis and raw GCM datasets. Enhancements include support for future climate projections, flexible horizontal and vertical interpolation for compatibility with diverse datasets, and a fully Python-based architecture optimized for parallel processing and high-performance computing. This paper illustrates the software's capabilities and provides a practical application example.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-7457-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/7457/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:gmd130130</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>gmd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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      <dc:title><![CDATA[Rapid Evaluation Framework for the CMIP7 Assessment Fast Track]]></dc:title>
      <dc:creator>Hoffman, Forrest M.</dc:creator>
      <dc:creator>Hassler, Birgit</dc:creator>
      <dc:creator>Swaminathan, Ranjini</dc:creator>
      <dc:creator>Lewis, Jared</dc:creator>
      <dc:creator>Andela, Bouwe</dc:creator>
      <dc:creator>Collier, Nathan</dc:creator>
      <dc:creator>Hegedűs, Dóra</dc:creator>
      <dc:creator>Lee, Jiwoo</dc:creator>
      <dc:creator>Pascoe, Charlotte</dc:creator>
      <dc:creator>Pflüger, Mika</dc:creator>
      <dc:creator>Stockhause, Martina</dc:creator>
      <dc:creator>Ullrich, Paul</dc:creator>
      <dc:creator>Xu, Min</dc:creator>
      <dc:creator>Bock, Lisa</dc:creator>
      <dc:creator>Chun, Felicity</dc:creator>
      <dc:creator>Gier, Bettina K.</dc:creator>
      <dc:creator>Kelley, Douglas I.</dc:creator>
      <dc:creator>Lauer, Axel</dc:creator>
      <dc:creator>Lenhardt, Julien</dc:creator>
      <dc:creator>Schlund, Manuel</dc:creator>
      <dc:creator>Sreeush, Mohanan G.</dc:creator>
      <dc:creator>Weigel, Katja</dc:creator>
      <dc:creator>Blockley, Ed</dc:creator>
      <dc:creator>Beadling, Rebecca</dc:creator>
      <dc:creator>Beucher, Romain</dc:creator>
      <dc:creator>Dugassa, Demiso D.</dc:creator>
      <dc:creator>Lembo, Valerio</dc:creator>
      <dc:creator>Lu, Jianhua</dc:creator>
      <dc:creator>Brands, Swen</dc:creator>
      <dc:creator>Tjiputra, Jerry</dc:creator>
      <dc:creator>Malinina, Elizaveta</dc:creator>
      <dc:creator>Medeiros, Brian</dc:creator>
      <dc:creator>Scoccimarro, Enrico</dc:creator>
      <dc:creator>Walton, Jeremy</dc:creator>
      <dc:creator>Kershaw, Phil</dc:creator>
      <dc:creator>Lanfer Marquez, André</dc:creator>
      <dc:creator>Roberts, Malcolm J.</dc:creator>
      <dc:creator>O'Rourke, Eleanor</dc:creator>
      <dc:creator>Dingley, Beth</dc:creator>
      <dc:creator>Turner, Briony</dc:creator>
      <dc:creator>Hewitt, Helene</dc:creator>
      <dc:creator>Dunne, John P.</dc:creator>
      <dc:description><![CDATA[<p>As Earth system models (ESMs) grow in complexity and in volume of output data, there is an increasing need for rapid, comprehensive evaluation of their scientific performance. The upcoming Assessment Fast Track for the Seventh Phase of the Coupled Model Intercomparison Project (CMIP7) will require expeditious response for model analyses designed to inform and drive integrated Earth system assessments. To meet this challenge, the Rapid Evaluation Framework (REF), a community-driven platform for benchmarking and performance assessment of ESMs, was designed and developed. The initial implementation of the REF, constructed to meet the near-term needs of the CMIP7 Assessment Fast Track, builds upon four disparate community evaluation and benchmarking tools that are coupled together using the Coordinated Model Evaluation Capabilities (CMEC) framework. The REF runs within a containerized workflow for portability and reproducibility and is aimed at generating and organizing diagnostics covering a variety of model variables. The REF leverages well documented observational datasets to provide assessments of model fidelity across a collection of diagnostics. All diagnostics were identified and selected with community involvement and consultation. Operational integration with the Earth System Grid Federation (ESGF) will permit automated execution of the REF for selected diagnostics as soon as model output data are published on ESGF by the originating modeling centers. The REF is designed to be portable across a range of current computational platforms to facilitate use by modeling centers for assessing the evolution of model versions or gauging the relative performance of CMIP simulations before being published on ESGF. When integrated into production simulation workflows, results from the REF provide immediate quantitative feedback that allows model developers and scientists to quickly identify model biases and performance issues. After the REF is released to the community, its subsequent development and support will be prioritized by an international consortium of scientists and engineers, enabling a broader impact across Earth science disciplines. For instance, the REF will facilitate improvements to models and will enhance confidence in model projections through process-based selection of models based on their performance with respect to observations. Production of reproducible diagnostics and community-based assessments are key features of the REF. Furthermore, providing interoperability with existing evaluation packages assures that contributions from previous community efforts will be available for use in future model intercomparison projects.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/gmd-19-7415-2026</dc:identifier>
      <dc:identifier><![CDATA[https://gmd.copernicus.org/articles/19/7415/2026/]]></dc:identifier>
      <dc:source>eISSN: 1991-9603</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd139460</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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      <dc:title><![CDATA[An airborne in-situ dataset of cloud microphysical properties in supercooled large droplet icing conditions]]></dc:title>
      <dc:creator>Menekay, Deniz</dc:creator>
      <dc:creator>Lucke, Johannes</dc:creator>
      <dc:creator>Jurkat-Witschas, Tina</dc:creator>
      <dc:creator>Voigt, Christiane</dc:creator>
      <dc:creator>Kirschler, Simon</dc:creator>
      <dc:creator>Bourdon, Aurélien</dc:creator>
      <dc:description><![CDATA[<p>Detailed and comprehensive data sets on microphysical cloud properties in icing conditions are rare. In April 2023, fifteen research flights were performed with the SAFIRE ATR 42 research aircraft during the SENS4ICE-EU airborne measurement campaign over France and adjacent marine regions to measure clouds containing supercooled large droplets (SLD) at altitudes between 2 and 6 km and temperatures of 0 to <span class="inline-formula">−</span>18 °C. Ten cloud probes were deployed on the aircraft, comprising four imaging probes, two light-scattering probes, and three hotwire probes, in order to characterise natural SLD conditions and serve as reference instruments for novel aircraft icing detection sensors. This work presents a comprehensive cloud dataset derived from the in-situ instruments used during the campaign, which is accessible on the HALO (High Altitude and Long Range Research Aircraft) database  (<a href="https://doi.org/10.17616/R39Q0T">https://doi.org/10.17616/R39Q0T</a>, <span class="cit" id="xref_altparen.1"><a href="#bib1.bibx41">Menekay et al.</a>, <a href="#bib1.bibx41">2026</a></span>). The dataset includes measurements of liquid and ice water content, combined particle size distributions, cloud microphysical properties, and meteorological parameters relevant to icing environments. In addition to documenting the dataset structure and processing methods, the paper provides an overview of flight strategies, instrument configurations, and statistical characteristics of the observed cloud properties, including their dependence on temperature and altitude. The dataset is suitable for studies of atmospheric icing conditions, mid-level clouds, sensor development, and model evaluation. It represents a rare collection of in-situ observations of SLD characteristics in icing environments and supports the evaluation of numerical weather prediction models under icing conditions to improve weather forecasts in hazardous conditions.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-5837-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/5837/2026/]]></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:essd140293</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>essd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[A global high-resolution temperature and salinity reconstruction by spatiotemporal multiscale correlations and dynamic height constraints]]></dc:title>
      <dc:creator>Wu, Haowen</dc:creator>
      <dc:creator>Li, Wei</dc:creator>
      <dc:creator>Li, Hong</dc:creator>
      <dc:creator>Han, Guijun</dc:creator>
      <dc:creator>Zhou, Gongfu</dc:creator>
      <dc:creator>Liu, Hanyu</dc:creator>
      <dc:creator>Cao, Lige</dc:creator>
      <dc:creator>Zheng, Qingyu</dc:creator>
      <dc:description><![CDATA[<p>High-resolution temperature and salinity (<span class="inline-formula"><i>T</i></span> &amp; <span class="inline-formula"><i>S</i></span>) gridded datasets are essential for exploring large and mesoscale ocean phenomena. In this study, a global, weekly <span class="inline-formula"><i>T</i></span> &amp; <span class="inline-formula"><i>S</i></span> gridded dataset with a horizontal resolution of <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">4</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="2b7a7aaa63926af08c46524e17d8d715"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="essd-18-5855-2026-ie00001.svg" width="20pt" height="14pt" src="essd-18-5855-2026-ie00001.png"/></svg:svg></span></span>° and a depth range of 0–1500 m from 2005 to 2023 is reconstructed using a four-dimensional multigrid analysis (4D-MGA) framework, based on the <span class="inline-formula"><i>T</i></span> &amp; <span class="inline-formula"><i>S</i></span> profiles in WOD23. With minimal prior statistical assumptions, the 4D-MGA efficiently extracts information from in-situ <span class="inline-formula"><i>T</i></span> &amp; <span class="inline-formula"><i>S</i></span> profiles and satellite-observed sea level anomalies by integrating multiscale spatiotemporal correlation and physical constraints. The results show that the 4D-MGA product successfully delivers a credible, high-resolution analysis that combines robustness with reliable mesoscale information. Specifically, our product exhibits a lower root mean square error and excellent unbiased performance on a global scale when compared with the ARMOR3D product and the GLORYS reanalysis. Furthermore, the clear recirculation in the western boundary currents (WBCs) can be well captured by the 4D-MGA product. The product is then applied to investigate the linear trends of geostrophic transport within five key sections in WBCs. The Kuroshio and Agulhas Current transports exhibit significant decreasing trends, with rates of 0.34 <span class="inline-formula">±</span> 0.07/0.26 <span class="inline-formula">±</span> 0.06, 0.23 <span class="inline-formula">±</span> 0.05/0.10 <span class="inline-formula">±</span> 0.06, and 0.30 <span class="inline-formula">±</span> 0.06/0.12 <span class="inline-formula">±</span> 0.05 Sv yr<span class="inline-formula"><sup>−1</sup></span> in 4D-MGA, ARMOR3D, and GLORYS, respectively. The weekly reconstructed dataset (4D-MGA) is freely available at <a href="https://doi.org/10.5281/zenodo.19378150">https://doi.org/10.5281/zenodo.19378150</a> (Wu et al., 2026a).</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-5855-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/5855/2026/]]></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:ejm140163</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>ejm</setSpec>
   </header>
   <metadata>
     <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[Fengruiite, [Ag6Sb2S7][Ag9CuS2Te2], a new Ag–Sb–Te sulfosalt mineral from the Haopinggou Ag–Pb–Zn–Au deposit, eastern Qinling, China]]></dc:title>
      <dc:creator>Tian, Yongfei</dc:creator>
      <dc:creator>Li, Guowu</dc:creator>
      <dc:creator>Sun, Ningyue</dc:creator>
      <dc:creator>Liu, Min</dc:creator>
      <dc:creator>Mao, Jingwen</dc:creator>
      <dc:creator>Dong, Yunpeng</dc:creator>
      <dc:creator>Liu, Peng</dc:creator>
      <dc:creator>Jian, Wei</dc:creator>
      <dc:creator>Yao, Wei</dc:creator>
      <dc:creator>Wang, Xiuquan</dc:creator>
      <dc:creator>Ye, Huishou</dc:creator>
      <dc:description><![CDATA[<p>Fengruiite, ideally [Ag<span class="inline-formula"><sub>6</sub></span>Sb<span class="inline-formula"><sub>2</sub></span>S<span class="inline-formula"><sub>7</sub></span>][Ag<span class="inline-formula"><sub>9</sub></span>CuS<span class="inline-formula"><sub>2</sub></span>Te<span class="inline-formula"><sub>2</sub></span>], is a new mineral species of the pearceite–polybasite group discovered in the Haopinggou Ag–Pb–Zn–Au deposit, eastern Qinling, China, and approved by the IMA Commission on New Minerals, Nomenclature and Classification as IMA 2024-045. The mineral occurs as irregular grains (<span class="inline-formula">&lt;</span> 20 <span class="inline-formula">×</span> 80 <span class="inline-formula">µ</span>m) intergrown with galena, cervelleite, and chalcopyrite in intermediate-sulfidation epithermal veins. Fengruiite is opaque, gray with a metallic luster, and brittle and has an estimated Mohs hardness of 3–4. EPMA analyses yield Ag (65.9 wt %–68.6 wt %), S (12.6 wt %–13.1 wt %), Sb (9.1 wt %–10.1 wt %), Te (6.3 wt %–7.6 wt %), and Cu (3.3 wt %–3.8 wt %), corresponding to the empirical formula [(Ag<span class="inline-formula"><sub>5.87</sub></span>Cu<span class="inline-formula"><sub>0.29</sub></span>)<span class="inline-formula"><sub>Σ6.16</sub></span>(Sb<span class="inline-formula"><sub>1.89</sub></span>As<span class="inline-formula"><sub>0.03</sub></span>)<span class="inline-formula"><sub>Σ1.92<i>S</i>7</sub></span>] [Ag<span class="inline-formula"><sub>9</sub></span>CuS<span class="inline-formula"><sub>2</sub></span>(Te<span class="inline-formula"><sub>1.28</sub></span>S<span class="inline-formula"><sub>0.63</sub></span>)S<span class="inline-formula"><sub>1.91</sub></span>]. Fengruiite is trigonal, space group <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M27" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>P</mi><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">‾</mo></mover><mi>m</mi><mn mathvariant="normal">1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="32pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="1bbc046b02fc4937363ceadaa1512235"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-519-2026-ie00001.svg" width="32pt" height="13pt" src="ejm-38-519-2026-ie00001.png"/></svg:svg></span></span> (#164), with <span class="inline-formula"><i>a</i>=7.6087</span>(9) Å, <span class="inline-formula"><i>c</i>=11.970</span>(2) Å, and <span class="inline-formula"><i>V</i>=600.13</span>(17) Å<span class="inline-formula"><sup>3</sup></span> (<span class="inline-formula"><i>Z</i>=1</span>). Its structure consists of alternating negatively charged [Ag<span class="inline-formula"><sub>6</sub></span>Sb<span class="inline-formula"><sub>2</sub></span>S<span class="inline-formula"><sub>7</sub></span>] (<span class="inline-formula"><i>A</i></span>) and positively charged [Ag<span class="inline-formula"><sub>9</sub></span>CuS<span class="inline-formula"><sub>2</sub></span>Te<span class="inline-formula"><sub>2</sub></span>] (<span class="inline-formula"><i>B</i></span>) layers, characteristic of the polybasite-Tac polytype. The combination of a Te-dominant <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M41" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Te</mi><mn mathvariant="normal">1</mn><mo>/</mo><mi mathvariant="normal">S</mi><mn mathvariant="normal">1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="39pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="c6fb1d2e9865b77b41ba71cdcd9a84a8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-519-2026-ie00002.svg" width="39pt" height="14pt" src="ejm-38-519-2026-ie00002.png"/></svg:svg></span></span> site in the <span class="inline-formula"><i>B</i></span>-layer module and S-dominant anion sites throughout the <span class="inline-formula"><i>A</i></span>-layer module distinguishes fengruiite from Te-rich polybasite-Tac and benleonardite. As the first structurally characterized Te-rich member of the pearceite–polybasite group reported from the East Qinling metallogenic belt, fengruiite expands the known structural and chemical diversity of Ag sulfosalts and documents Te incorporation into an Ag-rich sulfosalt structure in an epithermal system.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/ejm-38-519-2026</dc:identifier>
      <dc:identifier><![CDATA[https://ejm.copernicus.org/articles/38/519/2026/]]></dc:identifier>
      <dc:source>eISSN: 1617-4011</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:esd129117</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>esd</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Catalogue of strong nonlinear surprises in ocean, sea-ice, and atmospheric variables in CMIP6]]></dc:title>
      <dc:creator>Angevaare, Joran R.</dc:creator>
      <dc:creator>Drijfhout, Sybren S.</dc:creator>
      <dc:description><![CDATA[<p>The Coupled Model Intercomparison Project Phase 6 (CMIP6) archive was analysed for the occurrence of Strong Nonlinear Surprises (SNS) in future climate-change projections. To this end, we built an automated detection algorithm to identify SNS in a reproducible manner. Two different types of SNS were addressed: abrupt changes measured over decadal timescales and state transitions developing over multiple decades, too large to be explained by the forcing without invoking strong internal feedbacks in the climate system. We also discuss when one SNS case features a cascade from one variable to another (where sea-ice, deep convection, and temperature and salinity changes interact) and when two SNS interact to form a cascade, which occurs for the subpolar mixed-layer collapse triggering an Atlantic Meridional Overturning Circulation (AMOC) shutdown. Data from 54 models were analysed for five shared socio-economic pathways for ocean, sea ice, and atmospheric variables that are involved in the coupling to ocean and sea ice. The algorithm isolates regions of at least <span class="inline-formula">10<sup>6</sup></span> km<span class="inline-formula"><sup>2</sup></span> and utilizes stringent criteria to select SNS. In total 73 SNS were found, divided in 11 categories of which 4 apply to abrupt change and 7 to state transitions. Of the identified SNS <span class="inline-formula">45</span> % relate to sea-ice cover, <span class="inline-formula">19</span> % to ocean currents, <span class="inline-formula">29</span> % to mixed-layer depth, and <span class="inline-formula">7</span> % to atmospheric systems like the Intertropical Convergence Zone. For each category, probability density functions for time-windows of maximal change indicate SNS occurring earlier and at lower global temperature rise than assessed in previous reviews, in particular the ones associated with winter Arctic Sea ice disappearance, northern North Atlantic winter mixed-layer collapse and subsequent transition of the AMOC to a weak state in which the cell associated with North Atlantic Deep Water formation has vanished.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/esd-17-1081-2026</dc:identifier>
      <dc:identifier><![CDATA[https://esd.copernicus.org/articles/17/1081/2026/]]></dc:identifier>
      <dc:source>eISSN: 2190-4987</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:amt140145</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>amt</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Polarization calibration of spaceborne lidar using dense cirrus–scattered solar background with molecular scattering correction]]></dc:title>
      <dc:creator>Liu, Zhaoyan</dc:creator>
      <dc:creator>Vaughan, Mark A.</dc:creator>
      <dc:creator>Zhai, Pengwang</dc:creator>
      <dc:creator>Garnier, Anne Emilie</dc:creator>
      <dc:creator>Zeng, Shan</dc:creator>
      <dc:creator>Rodier, Sharon D.</dc:creator>
      <dc:creator>Hu, Yongxiang</dc:creator>
      <dc:creator>Omar, Ali H.</dc:creator>
      <dc:creator>Trepte, Charles R.</dc:creator>
      <dc:description><![CDATA[<p>Accurate calibration is essential for spaceborne polarization-sensitive lidars, as biases in depolarization ratio measurements can significantly affect the retrieval of cloud and aerosol properties. A polarization calibration technique based on solar background signals scattered by optically thick ice clouds (OTIC) provides a semi-continuous daytime calibration capability that complements onboard pseudo-depolarizer (PD) methods. This method was successfully applied to data from the Cloud-Aerosol Transport System (CATS) lidar at 1064 <span class="inline-formula">nm</span>, where molecular scattering effects are negligible. However, at shorter wavelengths, molecular scattering of sunlight between the lidar and the OTIC layer polarizes the background signal and introduces systematic biases. We present a molecular scattering correction (MSC) scheme based on vector radiative transfer modeling (VRTM) to account for this effect and demonstrate its performance using observations from the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP). The results show that molecular scattering introduces a daytime bias of approximately 1 % at 532 <span class="inline-formula">nm</span>, which is effectively removed by the VRTM-based MSC, yielding close agreement with onboard PD calibrations. For the Earth Cloud, Aerosol and Radiation Explorer (EarthCARE) Atmospheric Lidar (ATLID) operating at 355 <span class="inline-formula">nm</span>, model calculations indicate that molecular scattering contributions can be more than five times larger than at 532 <span class="inline-formula">nm</span>, underscoring the necessity of applying an MSC when the OTIC calibration technique is employed. Together, these results establish the OTIC calibration technique, combined with MSC, as a robust approach for achieving accurate polarization calibration across current and future spaceborne lidar missions.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-5325-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/5325/2026/]]></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:amt137217</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>amt</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Exploring the feasibility of an air sensor array for real-time detection and characterization of VOCs]]></dc:title>
      <dc:creator>Gao, Amanda</dc:creator>
      <dc:creator>Goss, Matthew B.</dc:creator>
      <dc:creator>Helstrom, Erik</dc:creator>
      <dc:creator>Hagan, David H.</dc:creator>
      <dc:creator>Kroll, Jesse H.</dc:creator>
      <dc:description><![CDATA[<p>Volatile organic compounds (VOCs) are an important class of atmospheric chemical species that can be directly harmful to human health and contribute to the formation of hazardous secondary products. Measurements of ambient VOCs are traditionally made using “offline” techniques, which are well-suited for distributed measurements but have low time resolution. They can also be made with real-time measurements using state-of-the-art in situ instruments, which have high precision and time resolution, but tend to be expensive and so cannot be deployed in a widespread manner. An alternative VOC measurement approach that is both real-time and lower in cost would open the possibility of widespread, spatially distributed measurements of VOCs in air quality and atmospheric chemistry contexts. While there are several commercially available air sensors that are sensitive to environmental VOCs, these sensors are “broadband,” meaning that each can only output a single scalar value that reflects the sensitivity of the sensor toward a wide and poorly defined range of VOCs. As a result, VOC air sensors have, to date, seen limited use in research. Here, we investigate the feasibility of a novel method for measuring speciated VOCs that uses an array of such broadband sensors. This array includes VOC air sensors representing three fundamentally different sensor types, and takes advantage of operational parameters that achieve a diversity of responses amongst sensors with the same type. Within a controlled laboratory setting, we obtained calibration curves for ten typical atmospheric VOCs between 5 and 100 <span class="inline-formula">ppb</span> and explored the effects of varying RH and introducing binary mixtures on sensor responses. Overall, we found that all observed sensor responses can be parameterized with linear or power-law models, consistent with results of prior studies and expectations based on physical sensing principles. Our results show that each of the 12 sensors in our array appear to have their own unique sensitivities to various VOCs, resulting in distinctive “fingerprints” of array responses for each compound tested. However, we also show that interferences by water vapour and other gases pose substantial challenges that likely cannot be fully addressed in the laboratory. Thus, co-location with a reference instrument in the field may first be required if this measurement approach is to yield quantitative, chemically specific information about ambient VOCs in indoor or outdoor environments.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/amt-19-5337-2026</dc:identifier>
      <dc:identifier><![CDATA[https://amt.copernicus.org/articles/19/5337/2026/]]></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:acp140876</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>acp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Sodium Lidar observed multiple sodium layer structures and their dynamical coupling mechanism]]></dc:title>
      <dc:creator>Jia, Yuxia</dc:creator>
      <dc:creator>Ban, Chao</dc:creator>
      <dc:creator>Li, Tao</dc:creator>
      <dc:creator>Fang, Xin</dc:creator>
      <dc:creator>Wu, Zhaopeng</dc:creator>
      <dc:creator>Wu, Jianfei</dc:creator>
      <dc:creator>Pan, Weilin</dc:creator>
      <dc:creator>Yang, Chengyun</dc:creator>
      <dc:description><![CDATA[<p>On the night of 13 June 2013, the University of Science and Technology of China (USTC) sodium lidar observed multiple sporadic sodium layers (SSLs) and enhanced sodium patterns (ESPs) over Hefei, China (31.8° N, 117.3° E). These structures appeared at different times, collectively spanning nearly the entire night, and exhibited distinct vertical motions and horizontal propagation behaviors. Their propagation was closely linked to the background horizontal wind, indicating the role of horizontal transport. Combined observations from the nearby meteor radar and ionosonde in Wuhan (<span class="inline-formula">∼200</span> <span class="inline-formula">mi</span> west of Hefei) revealed that SSLs occurring before 19:30 UT are closely associated with the sporadic E (Es) layer. The evolution of the Es layer shows an overall downward propagation consistent with tidal wind variations, suggesting that tidal waves may play a role in modulating ion distribution and associated sodium production. Notably, two ESP events exhibit quasi-periodic structures with periods of <span class="inline-formula">∼50</span>–60 <span class="inline-formula">min</span>, accompanied by similar oscillations in the Es layer and associated ion convergence regions. This behavior indicates that the atmospheric gravity waves may also modulate the horizontal wind, thereby influencing ion convergence, the Es layer, and sodium density. These observations provide new insights into the roles of wave-modulated horizontal winds in driving sodium-layer variability and underscore the importance of coupled neutral–ion processes in the MLT region.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-11409-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/11409/2026/]]></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:acp138518</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>acp</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Using high frequency observations of δ13C-CH4 and δ2H-CH4 and uncertain regional isotopic signatures to estimate sources of UK methane emissions]]></dc:title>
      <dc:creator>Ramsden, Alice E.</dc:creator>
      <dc:creator>Ganesan, Anita L.</dc:creator>
      <dc:creator>Rigby, Matthew</dc:creator>
      <dc:creator>Rennick, Chris</dc:creator>
      <dc:creator>Arnold, Tim</dc:creator>
      <dc:creator>Safi, Emmal</dc:creator>
      <dc:creator>Chung, Edward</dc:creator>
      <dc:creator>Kikaj, Dafina</dc:creator>
      <dc:creator>Yeo, Cameron</dc:creator>
      <dc:creator>Lowry, Dave</dc:creator>
      <dc:creator>Levy, Pete</dc:creator>
      <dc:creator>O'Doherty, Simon</dc:creator>
      <dc:creator>Stanley, Kieran M.</dc:creator>
      <dc:creator>Young, Dickon</dc:creator>
      <dc:creator>Pitt, Joe</dc:creator>
      <dc:creator>Martin, Damien</dc:creator>
      <dc:creator>Lopez, Morgan</dc:creator>
      <dc:creator>Ramonet, Michel</dc:creator>
      <dc:creator>Forster, Grant L.</dc:creator>
      <dc:creator>Frumau, Arnoud</dc:creator>
      <dc:creator>Manning, Alistair J.</dc:creator>
      <dc:description><![CDATA[<p>Methane is emitted from a range of anthropogenic and natural sources, and identifying these sources is important for emissions monitoring and mitigation. Different sources emit methane with different isotopic signatures. However, these signatures can vary spatially and temporally and are often not well understood. Top-down inverse methods can be used with measurements of methane mole fractions to estimate total emissions of methane from all sources. Here, we present an inverse system for concurrently estimating regional fossil-fuel (FF) and non-fossil-fuel (non-FF) emissions, using isotope ratio observations and considering uncertainty in the isotopic signatures. This method is highly adaptable and could be used to estimate emissions from any number of sources. Synthetic data tests with this method show that this inverse system can accurately estimate FF and non-FF methane emissions across the UK, when isotopic source signatures are fixed at known values. However, emissions estimation becomes less accurate when source signature uncertainties are increased to over approximately 50 % of their likely ranges. In a real-world test of this method, we estimated south-east UK FF and non-FF emissions using high-frequency <span class="inline-formula"><i>δ</i><sup>13</sup></span>C-CH<span class="inline-formula"><sub>4</sub></span> and <span class="inline-formula"><i>δ</i><sup>2</sup></span>H-CH<span class="inline-formula"><sub>4</sub></span> observations from one UK site, with source signature uncertainties reflecting our current understanding of these values. Results show only a limited impact on emissions uncertainty and magnitude, when compared with a methane-only inversion. This suggests that both an expansion of the UK network of isotope ratio observations and an improved understanding of isotopic<span id="page11422"/> signatures is required for this method to be effective in estimating UK FF and non-FF methane emissions with reduced uncertainty compared to traditional inverse methods.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/acp-26-11421-2026</dc:identifier>
      <dc:identifier><![CDATA[https://acp.copernicus.org/articles/26/11421/2026/]]></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:egusphere144438</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Highly oxygenated organic molecule formation from 2,5-dimethylfuran oxidation by O3 and OH: an experimental and computational study]]></dc:title>
      <dc:creator>Asgher, Rabbia</dc:creator>
      <dc:creator>Jha, Sakshi</dc:creator>
      <dc:creator>Kumar, Avinash</dc:creator>
      <dc:creator>Barua, Shawon</dc:creator>
      <dc:creator>Seal, Prasenjit</dc:creator>
      <dc:creator>Farhoudian, Sana</dc:creator>
      <dc:creator>Iyer, Siddharth</dc:creator>
      <dc:creator>Rissanen, Matti</dc:creator>
      <dc:description><![CDATA[The gas-phase oxidation of 2,5-dimethylfuran (2,5-DMF) by ozone (O<sub>3</sub>) and hydroxyl radicals (OH) was investigated in flow reactors at atmospheric pressure and room temperature using nitrate chemical ionization orbitrap mass spectrometry. At a residence time of 0.8 s, highly oxygenated organic molecules (HOM) with up to nine oxygen atoms were detected in the ozonolysis channel, and eight oxygen atoms in the OH channel. These observations demonstrate that sequential intramolecular hydrogen-shift autoxidation is sufficiently rapid to form products with up to nine oxygen atoms on sub-second timescales. At 7 s, C<sub>10</sub>&ndash;C<sub>12</sub> accretion products form through different combinations of C<sub>5</sub> and C<sub>6</sub> alkyl peroxy (RO<sub>2</sub>) radicals. Quantum chemical calculations using density functional theory and coupled-cluster methods identified a distinct Criegee intermediate geometry (Anti-CI-2A) that provides a plausible route to HOM species containing up to nine oxygen atoms. Its different methyl/hydrogen orientation relative to the conventional Syn and Anti conformers enables a rapid 1,6-H shift, facilitating autoxidation toward O<sub>9</sub> formation and suggesting that primary ozonide decomposition in structurally complex ozonolysis systems may access reactive Criegee intermediate geometries beyond the conventional Syn and Anti forms. For OH-initiated oxidation, the proposed mechanism accounts for HOM monomer formation up to O<sub>6</sub>, with rapid termination and radical recycling limiting further autoxidation. Overall, 2,5-DMF produces low-volatility oxidation products from both ozonolysis and OH-initiated pathways with implications for secondary organic aerosol formation.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4450</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4450/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144551</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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      <dc:title><![CDATA[The MESSy chamber DWARF: a box model for simulating chamber experiments (based on MESSy v2.55.2)]]></dc:title>
      <dc:creator>Do, Duong H.</dc:creator>
      <dc:creator>Kerkweg, Astrid</dc:creator>
      <dc:creator>Baker, Yarê</dc:creator>
      <dc:creator>Bohn, Birger</dc:creator>
      <dc:creator>Fuchs, Hendrik</dc:creator>
      <dc:creator>He, Quanfu</dc:creator>
      <dc:creator>Hohaus, Thorsten</dc:creator>
      <dc:creator>Kang, Sungah</dc:creator>
      <dc:creator>Kirfel, Timo</dc:creator>
      <dc:creator>Löher, Finja</dc:creator>
      <dc:creator>Diepenthal, Niklas</dc:creator>
      <dc:creator>Nölscher, Anke C.</dc:creator>
      <dc:creator>Novelli, Anna</dc:creator>
      <dc:creator>Pschera, Alexander</dc:creator>
      <dc:creator>Wieser, Felix</dc:creator>
      <dc:creator>Zorn, Sören R.</dc:creator>
      <dc:creator>Wahner, Andreas</dc:creator>
      <dc:creator>Taraborrelli, Domenico</dc:creator>
      <dc:description><![CDATA[Numerical simulation of environmental chamber experiments is essential for improving models of atmospheric composition. This task often relies on box models, which are not integral to three-dimensional atmospheric chemical transport models. Here, we present an application of the Modular Earth Submodel System (MESSy) DWARF model for chamber simulation experiments. It was developed as a zero-dimensional chemical box model of atmospheric oxidation. Chamber-specific features&mdash;including the injection of trace gases, variable radiation conditions, gas- and aqueous-phase chemistry, wall emissions, and dilution&mdash;are represented using existing and adapted MESSy submodels. We describe the multi-phase kinetic framework, the estimation of aerosol liquid water content and a simplified treatment of wall losses. We tested the MESSy chamber DWARF setup with experiments from three environmental chambers: The SAPHIR and SAPHIR-STAR chambers at Forschungszentrum J&uuml;lich, and the BATCH chamber at the University of Bayreuth. These chambers cover diverse designs and experimental conditions. The model reproduces observed time series of radicals, nitrogen oxides and ozone during an experiment in SAPHIR in which 2-methyl-3-butene-2-ol was oxidised. In another test the model was used to check the consistency of the experimental boundary conditions in the BATCH chamber. Further chamber DWARF tests also show that the framework can predict organic aerosol mass concentration via kinetic partitioning between the gas phase and deliquescent particles in SAPHIR-STAR. Modeled organic mass concentration during this experiment where &alpha;-pinene was oxidised agrees well with observations, supporting the framework&rsquo;s ability to simulate the chemical evolution in both the gaseous and aqueous phase. The MESSy chamber DWARF provides a useful tool for developing and evaluating kinetic models. Within this framework, we can test new laboratory findings directly for their atmospheric relevance. Thanks to the MESSy framework, we can use the same kinetic model for global simulations.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4522</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4522/]]></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:egusphere144491</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
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      <dc:title><![CDATA[Rapid simulation of 2-D contrail cross sections through Contrail Layer Approximation using Multi-crystal Particles (CLAMP) v1.0]]></dc:title>
      <dc:creator>Eastham, Sebastian David</dc:creator>
      <dc:creator>Abbasi, Hamid Reza</dc:creator>
      <dc:creator>Stettler, Marc E. J.</dc:creator>
      <dc:creator>Abbott, Tristan</dc:creator>
      <dc:creator>Engberg, Zebediah</dc:creator>
      <dc:description><![CDATA[Aircraft condensation trails (contrails) are increasingly studied with the aim of understanding and mitigating their climate impacts. Forming at the scale of a single aircraft, an individual contrail can take several hours to become large enough to be resolved by global-scale climate models, if they are resolved at all. High-fidelity simulations of individual contrails are too computationally intensive for use in global applications, but comparisons with existing reduced-order parameterizations have shown the need for approaches which can capture the development of size-resolved structures in the contrail as well as the dynamic interaction of contrail ice with the ambient humidity field. We introduce a new model of contrail physics, the Contrail Layer Approximation using Multi-crystal Particles (CLAMP) v1.0. CLAMP resolves challenges observed in other reduced-order models including lack of thermodynamic consistency and the inability to represent heterogeneity between the primary and secondary wakes due to gravitational sorting, providing an intermediate-fidelity simulation of a contrail with typical run times of about 60 seconds on one computational core for a 12-hour case. We use CLAMP to simulate the physics and radiative forcing of contrails across a broad parameter space, evaluating the effect of synoptic-scale downdrafts, mixing, settling, and gravity waves on contrail lifetime and climate impacts. We find that gravity wave forcing in particular may shorten contrail lifetimes, but that the stochastic nature of these effects is unlikely to be well captured by simple parameterizations. We also compare CLAMP to published results from other, more computationally expensive models, finding that it reproduces key trends in contrail properties with respect to common meteorological and aircraft parameters at a fraction of the computational cost. Furthermore, we show that carefully enforcing closed mass and energy budgets &ndash; not currently the case for most Lagrangian contrail models - can drive large differences in contrail properties, implying a potential shortcoming of current-generation contrail simulations. Although more work is needed to evaluate models against observations of real-world contrail behavior, including determining the importance of such inconsistencies, CLAMP is proposed as an alternative to existing single-contrail models for standalone contrail studies with sufficient speed and flexibility to inform emulations for use in global climate modeling applications.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4489</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4489/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145160</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Composite Detection of Continental Shelf Fronts from Sea Surface Temperature and Altimetry: Assessing the Added Value of SWOT KaRIn]]></dc:title>
      <dc:creator>Juhl, Marie-Christin</dc:creator>
      <dc:creator>Passaro, Marcello</dc:creator>
      <dc:creator>Dettermering, Denise</dc:creator>
      <dc:creator>Hart-Davis, Michael G.</dc:creator>
      <dc:creator>Saraceno, Martin</dc:creator>
      <dc:description><![CDATA[We present a composite front detection approach that uses horizontal gradients in Absolute Dynamic Topography (ADT) and Sea Surface Temperature (SST) to identify oceanic frontal structures on the Southwestern Continental Atlantic Shelf, a region characterized by strong mesoscale variability and multiple front types. SST fields are derived from the OSTIA satellite product, while four ADT datasets are compared: SWOT MIOST, CMEMS, OK-STv2, and GLORYS12v1. A joint front probability metric is introduced to quantify the co-occurrence of SST- and ADT-derived frontal signatures and to evaluate consistency and differences across products. The method is applied to assess the spatial and seasonal variability of major regional fronts, including the Shelf-Break Front, the San Mat&iacute;as Front, and the Magellan Plume Front. The ADT datasets showed significant differences in their ability to co-detect continental shelf fronts. The Shelf-Break Front was consistently represented across all datasets, with maximum joint front probabilities occurring in austral summer (DJF) and exceeding 96 % between 35 and 45&deg; S. In contrast, the seasonal and coastal San Mat&iacute;as Front exhibited stronger dataset dependence, with the highest joint probabilities obtained using SWOT MIOST ADT (73.63 %), followed by CMEMS (54.95 %), OK-STv2 (41.86 %), and GLORYS12v1 (35.16 %). In the mid-shelf region (38&ndash;41&deg; S), elevated joint frontal probabilities indicate that ADT and SST products, particularly altimetry-based datasets, capture a persistent Mid-Shelf Front. The Magellan Plume Front showed strong joint signatures, most pronounced in SWOT MIOST (97.85 %), followed by CMEMS (80.65 %), OK-STv2 (72.83 %), and GLORYS12v1 (51.09 %), with a distinct coastal plume structure during austral winter (JJA). The approach could be further evaluated using ADT from SWOT KaRIn L3 data during SWOT's Cal/val phase, potentially enabling improved detectability through the sharper ADT gradients provided. Overall, the results show that combining SST- and ADT-based gradient detection enhances the characterization of frontal dynamics. The intercomparison further demonstrates that SWOT KaRIn&ndash;enhanced gridded altimetry (SWOT MIOST) substantially improves the detection of coastal and seasonal fronts compared with conventional ADT products.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4751</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4751/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145168</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Contrasting sensitivities of Mediterranean cyclone forecasts to model resolution and physics across cyclone types]]></dc:title>
      <dc:creator>Andrade Cardoso, Andressa</dc:creator>
      <dc:creator>Gray, Suzanne L.</dc:creator>
      <dc:creator>Volonté, Ambrogio</dc:creator>
      <dc:creator>Harvey, Ben J.</dc:creator>
      <dc:creator>Sánchez, Claudio</dc:creator>
      <dc:description><![CDATA[Hazardous Mediterranean cyclones, including tropical-like medicanes, produce some of the most damaging wind and rainfall events in southern Europe, yet their prediction remains challenging because they are often small in scale and their evolution can be strongly controlled by diabatic processes. While previous research has assessed the role of diabatic processes in individual case studies and/or using resolutions that require parametrization of convection, it remains unclear whether the sensitivity of modelled Mediterranean cyclones to explicit representation of convection is robust across cyclone types. Using a consistent multi-case framework, we identify systematic rather than case-dependent sensitivities. Simulations of seven hazardous MedCys, with a range of characteristics, are performed using four limited-area configurations of the Met Office weather forecast model downscaled from ECMWF IFS analyses. The currently operational physics packages for the global (GAL9) and limited area (RAL3) versions of the model are used with 12-km and convection-permitting, 2.2-km grid spacing, respectively; an experimental package with the scale-aware convection scheme, CoMorph, is also used at both resolutions to cleanly identify resolution dependence.</p> <p>Sensitivity of dynamical variables and hazards to model configuration depends strongly on cyclone type, with medicanes exhibiting substantially greater and more robust dependence than more extratropical systems. The 2.2 km CoMorph configuration consistently over-intensifies medicanes, producing much lower minimum mean-sea-level pressures, and stronger winds and gusts than other simulations, especially for medicanes Ianos and Apollo. In contrast, the 12-km GAL9 configuration generally produces the weakest medicanes and tracks that is displaced eastward or southward; these biases are reduced using the 12-km CoMorph configuration. An in-depth analysis of medicane Ianos, which deepens by at least 20 hPa more in the 2.2-km CoMorph simulation than in the other simulations is presented. This CoMorph simulation yields a Ianos with a stronger potential vorticity tower, ascent and latent heat fluxes, and an eyewall structure resembling a tropical cyclone. These results demonstrate that the forecast skill of hazardous Mediterranean cyclones depends critically on the interaction between model resolution and physical parameterisations, implying that improvements in kilometre-scale forecasting require advances in model physics as well as increased resolution.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4757</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4757/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145181</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Impact of Increased ROMEX GNSS Radio Occultation Data on Forecast Performance in the Korean Integrated Model]]></dc:title>
      <dc:creator>Kim, Eun-Hee</dc:creator>
      <dc:creator>Chun, Hyoung-Wook</dc:creator>
      <dc:creator>Lee, Yong Hee</dc:creator>
      <dc:description><![CDATA[Global Navigation Satellite System Radio Occultation (GNSS RO) data can be assimilated to improve global numerical weather prediction (NWP). While simulation studies and observing system experiments have indicated benefits from increasing RO data volume, the extent to which large-volume RO assimilation improves forecasts in an operational NWP configuration has been less thoroughly quantified. As part of the international Radio Occultation Modeling Experiment (ROMEX), which assesses the forecast impact of GNSS RO observations, this study evaluates the effect of increased GNSS RO data volume on the forecast performance of the Korean Integrated Model (KIM), the operational global NWP model of the Korea Meteorological Administration (KMA). Four baseline experiments were conducted: NoRO (without GNSS RO observations), CTL (operational-level GNSS RO volume), EXP_20k (&asymp;20 000 profiles d⁻&sup1;), and EXP_35k (&asymp;35 000 profiles d⁻&sup1;). To investigate the sensitivity of the EXP_35k results to the assimilation configuration, additional experiments were conducted by adjusting the observation-error inflation factor and the refractivity coefficient <em>k</em><sub>1</sub> (the dry-term coefficient in the refractivity equation). A comparison of NoRO and CTL results showed that the assimilation of GNSS RO observations in KIM generally improved temperature and geopotential height forecasts in the lower stratosphere and upper troposphere. With larger GNSS RO datasets, EXP_20k showed relatively consistent improvements across most regions and levels, whereas EXP_35k maintained the global-mean improvement in 100 hPa temperature forecasts but showed weaker improvement in the tropics at that level. It also produced a pronounced increase in tropical 500 hPa geopotential height root-mean-square error, clearest through the first three forecast days and weakening only gradually through day 5. These results indicate that increasing the RO data volume does not translate linearly into forecast improvement and that the response of the current KIM assimilation configuration depends on the region, pressure level, and forecast variable. Increasing the observation-error inflation factor mitigated part of the mid-level geopotential height degradation but also indicated that this change weakens the upper-level temperature improvement attributable to RO data. In the <em>k</em><sub>1</sub> adjustment experiments, increasing <em>k</em><sub>1</sub> in KIM produced more favorable results than did decreasing it for certain variables and levels but did not directly resolve the main degradation observed in EXP_35k. The analysis-increment diagnostics showed similar tropical mid-level increment statistics across the three experiments, suggesting that the degradation is more likely related to accumulated differences in the analysis field or the forecast error growth than to excessive per-cycle analysis adjustment. These results show that the forecast impact of large-volume GNSS RO data is sensitive to the observation-error configuration and observation-operator coefficient. They further highlight that maximizing the value of future high-density GNSS RO observing systems depends not only on increased observation availability but also on continued improvements in observation-error modeling, observation handling, and observation operators within data assimilation systems.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4767</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4767/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145205</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Tight physics and chemistry coupling improves air quality forecasts: a case study of the 2020 North American wildfires with the Rapid Refresh model coupled to Chemistry (RAP-Chem v1.0)]]></dc:title>
      <dc:creator>Schnell, Jordan</dc:creator>
      <dc:creator>Ahmadov, Ravan</dc:creator>
      <dc:creator>Grell, Georg A.</dc:creator>
      <dc:creator>Olson, Joseph B.</dc:creator>
      <dc:creator>James, Eric</dc:creator>
      <dc:creator>Hu, Ming</dc:creator>
      <dc:creator>Wong, Ka Yee</dc:creator>
      <dc:creator>McDonald, Brian</dc:creator>
      <dc:creator>Schwantes, Rebecca H.</dc:creator>
      <dc:creator>He, Jian</dc:creator>
      <dc:creator>Harkins, Colin</dc:creator>
      <dc:creator>Angevine, Wayne M.</dc:creator>
      <dc:creator>Jamison, Brian</dc:creator>
      <dc:creator>Pierce, R. Bradley</dc:creator>
      <dc:creator>Coggon, Matthew</dc:creator>
      <dc:creator>Baker, Barry</dc:creator>
      <dc:creator>Freitas, Saulo</dc:creator>
      <dc:creator>Pereira, Gabriel</dc:creator>
      <dc:creator>Tsidulko, Marina</dc:creator>
      <dc:description><![CDATA[The Rapid Refresh model coupled to Chemistry (RAP-Chem) is an experimental forecast model built and operated by the NOAA Global Systems Laboratory (GSL). The RAP-Chem is a full chemistry extension to the operational smoke forecasting model, RAP-Smoke. RAP-Chem&rsquo;s chemistry includes a reduced complexity, carbon-bond, gas-phase mechanism and an aerosol scheme that are coupled together to produce secondary aerosols and perform heterogeneous chemistry. The model includes chemical lateral boundary conditions, hourly anthropogenic emissions and online emissions from biomass burning, dust, sea salt, and biogenic sources. RAP-Chem also includes the direct aerosol effect on radiation and photolysis and a simplified indirect aerosol effect that couples prognostic aerosols to representative aerosols in the aerosol-aware microphysics scheme. The default &lsquo;offline&rsquo; vertical mixing implemented in WRF-Chem is updated to instead mix chemical species alongside other scalars in the model&rsquo;s planetary boundary layer (PBL) scheme, which tends to improve predictions across species &ndash; increasing surface ozone (O<sub>3</sub>) and decreasing less reactive tracers (e.g., CO). Sub-grid boundary layer clouds in the PBL scheme are also coupled to a WRF-Chem photolysis scheme for the first time, overall reducing O<sub>3</sub> biases in the eastern US. Here we present the ability of the RAP-Chem model to simulate the extreme North American wildfires in 2020. We demonstrate that the relatively simple gas-phase chemical mechanism alongside our model physics developments and coupling with chemistry can predict maximum daily 8-h average O<sub>3</sub> with exceptional skill (Normalized Mean Bias (NMB) = 6.6 %) averaged over CONUS, improving on simulations that neglect the direct aerosol effect (NMB = 9.5 %). Ozone biases are large in regions with extreme aerosol loading, but the NMB improves more significantly. The model produces the observed extreme aerosol loading with less skill; tending to underpredict extreme wildfire induced concentrations while overpredicting urban particle pollution. As with O<sub>3</sub>, daily average PM2.5 is predicted with better skill when the direct aerosol feedback is included (-15.8 % vs. -16.8 %). Overall we find that improving the coupling between chemistry and physics processes in the air quality model improves its predictions of both weather and atmospheric composition.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4786</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4786/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145207</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Impact of the chemical regime on highly oxygenated molecule and secondary organic aerosol formation: Effects of varying the importance of NO, HO2&middot;, RO2&middot; reactions on &alpha;-pinene photooxidation products]]></dc:title>
      <dc:creator>Baker, Yarê</dc:creator>
      <dc:creator>Geretti, Veronica</dc:creator>
      <dc:creator>Kang, Sungah</dc:creator>
      <dc:creator>Wu, Rongrong</dc:creator>
      <dc:creator>Wang, Hui</dc:creator>
      <dc:creator>He, Quanfu</dc:creator>
      <dc:creator>Hohaus, Thorsten</dc:creator>
      <dc:creator>Zanders, Annika</dc:creator>
      <dc:creator>Bachner, Mathias</dc:creator>
      <dc:creator>Wu, Cheng</dc:creator>
      <dc:creator>Bannan, Thomas J.</dc:creator>
      <dc:creator>O'Meara, Simon P.</dc:creator>
      <dc:creator>Voliotis, Aristeides</dc:creator>
      <dc:creator>Hallquist, Mattias</dc:creator>
      <dc:creator>McFiggans, Gordon</dc:creator>
      <dc:creator>Zorn, Sören R.</dc:creator>
      <dc:creator>Mentel, Thomas F.</dc:creator>
      <dc:description><![CDATA[An important source of secondary organic aerosol (SOA) are highly oxygenated molecules (HOMs) formed by atmospheric oxidation of volatile organic compounds. HOM formation is governed by the fate of HOM peroxy radicals (RO₂&middot;) which depends on the availability of reaction partners (RO₂&middot;, HO₂&middot;, NO) and on their overall lifetime &ndash; factors often insufficiently explored in laboratory studies.</p> <p>We performed &alpha;-pinene photooxidation experiments systematically exploring these parameters and present the impacts on HOM and SOA formation within a generic framework explaining the changes in HOM production. Steady-state experiments were performed in the SAPHIR-STAR atmospheric simulation chamber. The reaction regime was shifted by increasing HO₂&middot; and NO, separately and simultaneously, while keeping the &alpha;-pinene primary oxidation conditions constant. (NH₄)₂SO₄ particles were added to observe gas-phase HOM condensation and investigate product volatilities.</p> <p>We find decreasing SOA formation potential when moving away from RO₂&middot;-dominated regimes. One reason is the suppression of HOM accretion product formation from HOM-RO₂&middot;+RO₂&middot;. Alkoxy radicals (RO&middot;) from RO₂&middot;+RO₂&middot; or RO₂&middot;+NO play another important role. RO&middot; are crucial intermediates in certain HOM formation pathways but also produce lower-mass, more fragmented HOM with higher volatility, decreasing SOA formation potential. Additionally, RO₂&middot;+NO forms organic nitrates, which we show have higher volatility than other termination products. Our mechanistic considerations illustrate which factors impact the HOM product distribution and explain the reduced SOA formation through changes in HOM composition and volatility.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4788</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4788/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143781</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Linking cloud hydrometeor growth and surface precipitation to synoptic forcing at Dumont d&rsquo;Urville, East Antarctica]]></dc:title>
      <dc:creator>Sreenath, A. V.</dc:creator>
      <dc:creator>May, Peter T.</dc:creator>
      <dc:creator>Siems, Steven</dc:creator>
      <dc:creator>Corden, Heather</dc:creator>
      <dc:creator>Berne, Alexis</dc:creator>
      <dc:description><![CDATA[We investigate how weather regimes influence surface precipitation and associated cloud microphysical processes at Dumont d&rsquo;Urville (DDU; 66.7&deg; S, 140.0&deg; E) using data from the Antarctic Precipitation: Remote Sensing from Surface and Space (APRES3) project. Two precipitation-producing regimes, Summer Warm Air Advection (S-WAA) and Low-Pressure (Low-P), account for 94.2 % of total precipitation at DDU. Hydrometeor growth processes were analysed through comprehensive case studies of Low-P and S-WAA events. The polarimetric signatures during the Low-P event indicate riming and secondary ice production (SIP) within the &minus;10 to &minus;14 &deg;C layer (2&ndash;3.5 km), which falls within the dendritic growth zone (DGZ; approximately &minus;10 to &minus;20 &deg;C). Riming intensifies between 1 and 2 km (&minus;7 to &minus;10 &deg;C), whereas below 1 km, downslope flow leads to pronounced hydrometeor sublimation and sublimation-induced SIP. Thus, the surface precipitation associated with this event displays an intermittent pattern, with a predominance of graupel. In contrast, the S-WAA regime is associated with a moist boundary layer, favouring persistent surface precipitation. The polarimetric signatures in the upper half of the DGZ (&minus;14 to &minus;20 &deg;C, 2.5&ndash;3.5 km) suggest hydrometeor growth through vapour deposition, while signatures below down to 1 km (&minus;8 to &minus;14 &deg;C) align with aggregation processes. Enhanced riming and SIP driven by the Hallett&ndash;Mossop process are observed below 1 km. Our findings emphasise that synoptic weather regimes primarily impact precipitation growth, while boundary-layer flow and moisture play a significant role in snowfall efficiency at DDU in East Antarctica.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4159</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4159/]]></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:egusphere143599</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Assessing evaporative cooling from seawater spraying in the marine boundary layer]]></dc:title>
      <dc:creator>Broerze, Annelot</dc:creator>
      <dc:creator>Roode, Stephan R.</dc:creator>
      <dc:creator>Russchenberg, Herman</dc:creator>
      <dc:description><![CDATA[Increasing frequency and intensity of extreme heat events motivate improved understanding of processes that may modify near-surface thermal conditions. This study investigates seawater spraying as a method for direct atmospheric cooling. Using large-eddy simulations (LES), we quantify plume dynamics, cooling response, and impacts on heat stress across a range of atmospheric conditions. Simulated spray rates of 50 L s<sup>-1</sup> produce near-surface temperature reductions of approximately 0.5&ndash;1 &deg;C within the first few kilometers. Although theoretical analysis suggests that evaporative cooling potential can exceed -20 &deg;C under hot and dry conditions, atmospheric mixing and advection substantially reduce this potential under realistic conditions. Cooling is strongest near the source due to evaporatively driven downdrafts, but decays rapidly downstream. We compare deployment from wind turbines with ship-based platforms. A key finding is that injection height governs plume structure and cooling response. Ship-based spraying produces strong, localized near-surface cooling, whereas wind turbine deployment redistributes cooling more effectively within the lower boundary layer. The turbine wake modifies local mixing, but vertical redistribution is mainly governed by evaporatively driven buoyancy perturbations. Extending the analysis to human thermal comfort reveals that temperature reductions alone do not determine effectiveness. Changes in Heat Index are non-linear and depend on background humidity, with benefits near the source that may diminish or even reverse downstream. Overall, seawater spraying can provide measurable cooling, but its performance is highly sensitive to background atmospheric conditions.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4092</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4092/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142899</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Contrasting Arctic Cirrus Clouds: Properties and Processes from Observations and Simulations]]></dc:title>
      <dc:creator>Dekoutsidis, Georgios</dc:creator>
      <dc:creator>Groß, Silke</dc:creator>
      <dc:creator>Ewald, Florian</dc:creator>
      <dc:creator>Krämer, Martina</dc:creator>
      <dc:creator>Rolf, Christian</dc:creator>
      <dc:creator>Schäfler, Andreas</dc:creator>
      <dc:creator>Wirth, Martin</dc:creator>
      <dc:description><![CDATA[Cirrus clouds in the Arctic play a central role in the regional radiation budget, yet their formation pathways and properties remain poorly constrained, especially during Warm Air Intrusions (WAI). In this study, we analyse and contrast cirrus observed during WAI events (WAI cirrus) with those formed under undisturbed Arctic Conditions (AC cirrus) using remote sensing measurements from the HALO&ndash;(AC)&sup3; campaign, combined with backward trajectory modelling with CLaMS-Ice and LAGRANTO. This allows us to connect the optical, macro- and microphysical properties measured via lidar and radar to the cloud origin and dynamics during their evolution. We find that WAI cirrus encountered stronger vertical transport along their trajectories compared to AC cirrus. At the time of detection, WAI cirrus were geometrically and optically thicker, exhibited higher depolarization ratios and ice supersaturation, and contained more numerous but smaller ice crystals, consistent with homogeneous ice nucleation at colder temperatures. AC cirrus, in contrast, showed larger ice crystals and a comparably greater contribution from heterogeneous ice nucleation. As WAI events are projected to become more frequent and long-lasting, a resulting increase in the formation of WAI cirrus may enhance their influence on the Arctic radiation budget leading to cooling. Our results provide observational constraints on cirrus variability in the Arctic and emphasize the need for their improved representation in weather and climate models.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3788</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3788/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144147</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Initial generation and validation of the JAXA four-sensor synergy radiation budget product (ALL_RAD) for the EarthCARE mission]]></dc:title>
      <dc:creator>Nagao, Takashi M.</dc:creator>
      <dc:creator>Suzuki, Kentaroh</dc:creator>
      <dc:creator>Yamauchi, Akira</dc:creator>
      <dc:creator>Oikawa, Eiji</dc:creator>
      <dc:creator>Sekiguchi, Miho</dc:creator>
      <dc:creator>Ishida, Haruma</dc:creator>
      <dc:creator>Muto, Masataka</dc:creator>
      <dc:description><![CDATA[The Earth Cloud, Aerosol and Radiation Explorer (EarthCARE) mission provides an unprecedented opportunity to investigate the Earth&rsquo;s radiation budget using synergistic observations from active and passive sensors. In this study, we present the development and validation of the JAXA four-sensor synergy radiation budget product (ALL_RAD), version Ba, which was publicly released on 1 December 2025. The ALL_RAD algorithm generates composite cloud and aerosol profiles by integrating Level-2 retrieval products from the Cloud Profiling Radar (CPR), the Atmospheric Lidar (ATLID), and the Multi-Spectral Imager (MSI), and then estimates broadband shortwave and longwave radiative fluxes and heating rate profiles using a one-dimensional radiative transfer model. The performance of ALL_RAD is evaluated against the ESA radiative flux product (BMA-FLX) derived from broadband radiometer (BBR) observations. The comparison shows substantial improvements in radiative flux estimates relative to earlier pre-launch evaluations, with instantaneous shortwave bias and root-mean-square error (RMSE) reduced to &minus;0.6 and 33.7 W m⁻&sup2;, respectively, and the longwave bias and RMSE reduced to +2.2 and 8.1 W m⁻&sup2;, respectively. In addition, comparisons with ground-based observations from the Baseline Surface Radiation Network (BSRN) demonstrate good agreement for both shortwave and longwave surface fluxes. The physical consistency of the product is further assessed using cloud radiative effects and associated heating rate profiles as well as aerosol radiative effects, which are found to be broadly consistent with previous studies using A-Train observations. Future work will extend the validation to longer periods and broader cloud regimes, and will further assess uncertainty sources related to aerosol representation, spatial representativeness, and three-dimensional radiative effects. Overall, ALL_RAD provides a reliable basis for estimating EarthCARE radiative fluxes and derived quantities, thus establishing a foundation for radiative closure studies using EarthCARE observations.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4324</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4324/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143948</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Integrating Geodetic Constraints into Earthquake Source Characterization for Probabilistic Seismic Hazard Analysis: A Dual Statistical&ndash;Physical Framework]]></dc:title>
      <dc:creator>Yuliastuti, Yuliastuti</dc:creator>
      <dc:creator>Meilano, Irwan</dc:creator>
      <dc:creator>Puspito, Nanang T.</dc:creator>
      <dc:creator>Rahmadani, Suchi</dc:creator>
      <dc:description><![CDATA[Reliable earthquake source characterization is essential for probabilistic seismic hazard analysis (PSHA), yet remains particularly challenging in low-seismicity regions where sparse earthquake catalogs introduce substantial epistemic uncertainty. Although geodetic observations provide independent constraints on contemporary crustal deformation, existing hybrid earthquake source models have generally been selected solely on the basis of statistical forecasting performance without explicitly considering their physical consistency with regional deformation. This study presents a statistical&ndash;physical hybrid framework that integrates independently validated catalog-based and GNSS-derived geodetic earthquake source models for PSHA. The proposed framework combines retrospective earthquake forecast evaluation using the Collaboratory for the Study of Earthquake Predictability (CSEP) with independent physical screening based on the regional geodetic moment budget. A total of 126 candidate hybrid models were evaluated for Kalimantan, Indonesia, representing alternative catalog models, geodetic scenarios, and hybrid formulations. Although several candidates improved retrospective forecasting skill, only three satisfied both the statistical and physical selection criteria, with the preferred adaptive-smoothing hybrid model achieving the highest average retrospective pass rate (67.5 %). Physical screening rejected six of the seven evaluated geodetic scenarios because their implied seismic moment release exceeded the available geodetic moment budget. Incorporating the selected hybrid models into PSHA increased median peak ground acceleration by approximately 2&ndash;29 % for the 475-year return period and 2&ndash;23 % for the 2475-year return period. In contrast, equal-weight and performance-based logic-tree ensembles produced nearly identical hazard estimates, differing by less than 1.5 %. These results demonstrate that integrating statistical forecasting skill with independent geodetic constraints provides a physically consistent framework for earthquake source characterization and a transferable methodology for improving earthquake hazard assessment in low-seismicity regions.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4242</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4242/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142401</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Mamba-Stormer v1.0: A Bidirectional Vision Mamba Backbone for Accurate and Scalable Global Weather Forecasting]]></dc:title>
      <dc:creator>Chao, Jiayou</dc:creator>
      <dc:creator>Tong, Guanchao</dc:creator>
      <dc:creator>Liu, Zhenhua</dc:creator>
      <dc:creator>Lin, Wuyin</dc:creator>
      <dc:creator>Zhang, Minghua</dc:creator>
      <dc:creator>Ma, Merry</dc:creator>
      <dc:creator>Zhu, Wei</dc:creator>
      <dc:description><![CDATA[Accurate global weather forecasting at increasing spatial resolution is a central challenge in atmospheric science. Machine learning models have recently matched or exceeded numerical weather prediction systems on standard medium-range benchmarks, with transformer-based architectures at their core. However, the self-attention mechanism underlying these models scales quadratically in memory and compute with sequence length &mdash; a critical bottleneck as training and inference resolutions approach operational standards. We describe Mamba-Stormer, which replaces the transformer backbone in the Stormer architecture with a bidirectional Vision Mamba (BiMamba) backbone. Our key design contributions are: (1) bidirectional Mamba scanning applied in an alternating horizontal&ndash;vertical pattern across 14 layers to capture 2D atmospheric structure, and (2) the integration of bidirectional SSMs into Stormer&rsquo;s adaLN-Zero residual block by replacing the self-attention sub-block while retaining the feed-forward sub-block and zero-initialized lead-time conditioning. In a controlled local comparison on ERA5 WeatherBench 2 (240x121 grid, 69 atmospheric variables, multi-step finetuned), Mamba-Stormer outperforms the 24-layer Transformer baseline: +2.73 % mean per-variable RMSE improvement at 6h, +2.34 % at 72 h, and +1.07 % at 120 h (all <em>p</em> &lt; 0.01), with BiMamba winning on 67/69, 69/69, and 66/69 variables respectively. Simultaneously, its <em>O</em>(<em>L</em>) backbone delivers a 1.10x computational throughput speedup at the WeatherBench 2 1.5&deg; training resolution (121x240), growing to 2.59x at 512x512 as the <em>O</em>(<em>L</em>&sup2;) attention cost increasingly dominates. These results suggest that bidirectional Vision Mamba is a strong backbone for neural weather prediction &mdash; achieving better accuracy and growing computational efficiency, consistent with a more suitable spatial inductive bias for atmospheric modeling.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3398</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3398/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142499</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>egusphere</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Towards a risk governance framework for reducing the seismic vulnerability of existing buildings: a comparative analysis of national strategies with implications for Algeria]]></dc:title>
      <dc:creator>Benfarhat, Bachir</dc:creator>
      <dc:creator>Benouar, Djillali</dc:creator>
      <dc:description><![CDATA[Every major earthquake is a reminder that buildings do not collapse because of geology alone: they collapse because the societies in which they stand have not invested in making them safer. This study examines national governance frameworks for reducing the seismic vulnerability of existing buildings through a comparative analysis of six high-seismicity countries (Japan, New Zealand, California in the United States, Turkey, Italy, and Greece). Using a five-pillar analytical framework spanning regulatory, technical, financial, institutional, and cultural dimensions, we identify the mechanisms that distinguish effective governance from ineffective intent. Our central finding is that successful seismic risk reduction is never the product of a single policy instrument but emerges from the coherent alignment of five interdependent conditions: enforceable legislation specifically targeting the existing building stock, performance-based financial incentives capable of mobilising private capital, comprehensive national building-risk inventories, coordinated multi-level governance, and a deeply embedded societal risk culture. These findings are translated into a phased and operationally specific governance framework for Algeria, a country whose location on one of the Mediterranean basin's most active seismic belts, combined with a critically vulnerable pre-code building stock and a currently reactive policy architecture, makes the transition to proactive seismic risk governance both urgent and achievable.]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3476</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3476/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg132171</identifier>
    <datestamp>2026-08-13</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
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       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Uncertainty in Land Carbon Fluxes Simulated by CMIP6 Models from Treatments of Crop Distributions and Photosynthetic Pathways]]></dc:title>
      <dc:creator>Ovwemuvwose, Joseph</dc:creator>
      <dc:creator>Prentice, Ian Colin</dc:creator>
      <dc:creator>Graven, Heather</dc:creator>
      <dc:description><![CDATA[<p>A reliable representation of the diversity of vegetation in terrestrial ecosystems is needed for the accurate simulation of present and future biogeochemical cycling and global climate, particularly as climate change affects different vegetation types differently. We compare the distributions of crops and of C<span class="inline-formula"><sub>3</sub></span> vs. C<span class="inline-formula"><sub>4</sub></span> photosynthetic pathways in both natural vegetation and crops across Earth System Models in the 6th Coupled Model Intercomparison Project (CMIP6). We find a large range in C<span class="inline-formula"><sub>3</sub></span> and C<span class="inline-formula"><sub>4</sub></span> crops, natural and total vegetation for area and gross primary production (GPP) across the models. Even though 10 of the 11 models used Land Use Harmonisation (LUH2) crop areas as input data, modelled total crop area ranges from <span class="inline-formula">−</span> 28 % to <span class="inline-formula">+</span> 10 % of a satellite-based estimate. The C<span class="inline-formula"><sub>3</sub></span> and C<span class="inline-formula"><sub>4</sub></span> crop areas were <span class="inline-formula">−</span> 56 % to <span class="inline-formula">+</span> 15 % and <span class="inline-formula">−</span> 100 % to <span class="inline-formula">+</span> 38 % of LUH2 for 2014, respectively. The C<span class="inline-formula"><sub>4</sub></span> fraction of total vegetation area in the models is 9 %–25 %, compared to 20 % <span class="inline-formula">±</span> 3 % in observation-based estimates for the year 2014. Total global GPP varies by a factor of two across the models, and the C<span class="inline-formula"><sub>4</sub></span> fraction of GPP ranges from 12 % to 27 %. Simulated trends in the fraction of GPP by C<span class="inline-formula"><sub>3</sub></span> vs. C<span class="inline-formula"><sub>4</sub></span> vegetation type (<span class="inline-formula">−</span> 20 % to <span class="inline-formula">+</span> 29 %) would have changed global stable carbon isotopic discrimination by <span class="inline-formula">−</span> 0.35 ‰ to <span class="inline-formula">+</span> 0.11 ‰ over 1975–2005, not including changes in discrimination over time within C<span class="inline-formula"><sub>3</sub></span> and C<span class="inline-formula"><sub>4</sub></span> vegetation, indicating that modeled changes in the fraction of GPP by C<span class="inline-formula"><sub>3</sub></span> and C<span class="inline-formula"><sub>4</sub></span> vegetation do not account for the <span class="inline-formula">+</span> 0.7 ‰ increase indicated by atmospheric data. Disparity in vegetation with these photosynthetic pathways in models contributes to uncertainty in land carbon flux simulations, and further constraints and improvements in models are needed.</p>]]></dc:description>
      <dc:date>2026-08-13</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-5593-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/5593/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg136788</identifier>
    <datestamp>2026-08-12</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
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       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 Ni cycle in the Southern Ocean: insights from Ni concentrations, isotopes and metagenomics]]></dc:title>
      <dc:creator>Lemaitre, Nolwenn</dc:creator>
      <dc:creator>Faure, Emile</dc:creator>
      <dc:creator>Zamora, Ricardo</dc:creator>
      <dc:creator>Archer, Corey</dc:creator>
      <dc:creator>Sieber, Matthias</dc:creator>
      <dc:creator>Ellwood, Michael</dc:creator>
      <dc:creator>Hassler, Christel</dc:creator>
      <dc:creator>Lin, Yajuan</dc:creator>
      <dc:creator>Cassar, Nicolas</dc:creator>
      <dc:creator>Maignien, Lois</dc:creator>
      <dc:creator>Vance, Derek</dc:creator>
      <dc:description><![CDATA[<p>Nickel (Ni) is an essential micronutrient for marine microorganisms, involved in enzymes controlling the nitrogen cycle and metabolic responses to oxidative stress. In this study, we examine the role of potential Ni utilisation by marine microorganisms in oceanic Ni and <span class="inline-formula"><i>δ</i><sup>60</sup></span>Ni distributions, and specifically the influence of Ni-containing enzyme abundances on Ni isotope fractionation. Dissolved Ni concentrations and isotope compositions were measured together with microbial gene composition in Southern Ocean samples from the Antarctic Circumnavigation Expedition. We show that lower Ni concentrations are associated with higher <span class="inline-formula"><i>δ</i><sup>60</sup></span>Ni values in surface waters north of the Sub-Antarctic Front compared to southerly locations. The high-latitude Mertz Glacier stands as an exception, as systematics between Ni and <span class="inline-formula"><i>δ</i><sup>60</sup></span>Ni resemble those of low-latitude stations. No single enzyme could be identified as the sole driver of <span class="inline-formula"><i>δ</i><sup>60</sup></span>Ni variations across all stations, as the strength and significance of correlations varied depending on the level of precision of functional annotations and the size fractions considered. Still, relative abundances of gene clusters annotated as  urease and Ni superoxide dismutase (Ni-SOD) enzymes in metagenomes correlated with <span class="inline-formula"><i>δ</i><sup>60</sup></span>Ni, suggesting the preferential removal of isotopically light Ni by microorganisms using these enzymes. Despite differences in enzymatic and taxonomic profiles, the three stations exhibiting heavy surface Ni isotope compositions share a specific nitrogen biogeochemistry, characterised by high particulate organic nitrogen pool and strong nitrate consumption. We thus hypothesise that Ni and <span class="inline-formula"><i>δ</i><sup>60</sup></span>Ni distributions reflect variations in Ni metabolic requirements driven by complex microbial and enzymatic activity linked to the relative availability of inorganic and organic nitrogen. We further propose that the use of urea as an alternative nitrogen source during the late productive season could explain the unexpected isotope fractionation observed<span id="page5572"/> at Mertz. This study represents an initial exploration of the influence of enzymes and microbial communities on the Ni biogeochemical divide.</p>]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-5571-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/5571/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:bg135616</identifier>
    <datestamp>2026-08-12</datestamp>
    <setSpec>bg</setSpec>
   </header>
   <metadata>
     <oai_dc:dc
       xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
       xmlns:dc="http://purl.org/dc/elements/1.1/"
       xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[Estimation of the degree of decomposition of peat and past net primary production from mid-infrared spectra]]></dc:title>
      <dc:creator>Teickner, Henning</dc:creator>
      <dc:creator>Arsenault, Julien</dc:creator>
      <dc:creator>Gałka, Mariusz</dc:creator>
      <dc:creator>Knorr, Klaus-Holger</dc:creator>
      <dc:description><![CDATA[<p>The degree of decomposition of peat (<span class="inline-formula"><i>γ</i></span>) is useful to understand peatland degradation and peat accumulation, to reconstruct past net primary production (NPP), and to improve peatland models. None of the available decomposition indicators allows to estimate <span class="inline-formula"><i>γ</i></span> with sufficient accuracy. We suggest prediction of <span class="inline-formula"><i>γ</i></span> measured in litterbag experiments from mid-infrared spectra (MIRS) as a novel decomposition indicator, <span class="inline-formula"><i>γ</i><sub>MIRS</sub></span>, and compute prediction models for <span class="inline-formula"><i>γ</i><sub>MIRS</sub></span> with available litterbag experiments and litter data from diverse species from the Peatland Mid-Infrared Database. For individual litter samples, the prediction models fit the data well, have reasonable prediction errors (average RMSE between 0.09–0.12 <span class="inline-formula">g g<sup>−1</sup></span>), and neither confound differences in litter chemistry nor differences in silicate contents with decomposition losses. We show that an underestimation of <span class="inline-formula"><i>γ</i></span> by <span class="inline-formula"><i>γ</i><sub>MIRS</sub></span> matches theoretical expectations; it can therefore be compensated, using plant macrofossil analysis data as a first approximation to mass fractions of peat components and a simple mixing model, or it can be avoided with component-specific measurements instead of bulk measurements. This allows to estimate <span class="inline-formula"><i>γ</i></span> of peat samples and of dominant litter types and therefore also to reconstruct past NPP. To illustrate the approach, we analyze three cores from European mountain bogs and discuss how it can be used to improve process models and support restoration of peatlands. In particular, we test previously suggested relations between the saturated hydraulic conductivity and <span class="inline-formula"><i>γ</i></span>, illustrate how <span class="inline-formula"><i>γ</i></span> measured on individual litter types may allow to use peat cores as natural litterbag experiments, and define reference states for <span class="inline-formula"><i>γ</i></span> and NPP for the three analyzed peat cores. The method requires further validation by future studies. Improvements to reduce prediction errors of the approach require more diverse litterbag data, especially woody species and more decomposed litter. Further improvements can be achieved with measurements of MIRS on individual macrofossil types instead of bulk measurements, and an improved estimation of mass fractions of macrofossil types in peat samples instead of assuming that macrofossil abundances equal macrofossil masses.</p>]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/bg-23-5549-2026</dc:identifier>
      <dc:identifier><![CDATA[https://bg.copernicus.org/articles/23/5549/2026/]]></dc:identifier>
      <dc:source>eISSN: 1726-4189</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142087</identifier>
    <datestamp>2026-08-12</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[Spatiotemporal Distribution of Tropopause Folds over the Arctic during Spring Season: A 24-Year Analysis (2000&ndash;2023)]]></dc:title>
      <dc:creator>Chen, Yiqi</dc:creator>
      <dc:creator>Cao, Le</dc:creator>
      <dc:creator>Zhu, Xiaochun</dc:creator>
      <dc:creator>Xia, Yan</dc:creator>
      <dc:creator>Zhang, Tianqi</dc:creator>
      <dc:creator>Lei, Xiuli</dc:creator>
      <dc:creator>Wang, Mengke</dc:creator>
      <dc:creator>Xu, Liqiang</dc:creator>
      <dc:creator>Zhao, Tianliang</dc:creator>
      <dc:description><![CDATA[Springtime tropopause folds facilitate stratosphere&ndash;troposphere exchange and may influence Arctic tropospheric composition, yet their long-term variability and dynamical background over the Arctic remain insufficiently characterized. Here, we use ERA5 reanalysis data and a three-dimensional labeling algorithm to identify tropopause folds over the Arctic during March&ndash;May from 2000 to 2023, with particular focus on four monitoring sites: Alert, Barrow, Villum, and Zeppelin. The results show spatial heterogeneity and depth dependence. Total and shallow folds occur over relatively broad Arctic regions, with high-frequency centers around Greenland, the Greenland&ndash;Barents Sea region, and the North Pacific side of the Arctic. Medium and deep folds are less frequent and are more strongly confined to the lower-latitude Arctic periphery. This spatial structure is dynamically consistent with the 700&ndash;250 hPa layer-mean maximum Eady growth rate, which is larger along the Arctic margins than over the central Arctic. Station-based composites further indicate that deeper folds are associated with stronger 250 hPa geopotential height contrasts, larger horizontal GPH gradient magnitude (<em>G</em><sub><em>Z</em></sub>), and stronger wind speed characteristics. Temporally, total fold frequency shows interannual positive trends at all four stations during 2000&ndash;2023, with the strongest increases at Alert and Villum, mainly contributed by shallow folds. A monthly decline is also found from March to May, with May frequencies only about 20 %&ndash;30 % of March values, whereas diurnal variations are weak. These results provide a climatological framework for understanding Arctic springtime tropopause folds and their potential implications for Arctic tropospheric composition.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3196</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3196/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142113</identifier>
    <datestamp>2026-08-12</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[Assessment of humidity ground checks for GRUAN-compliant automatic radiosonde operations]]></dc:title>
      <dc:creator>Romanens, Gonzague</dc:creator>
      <dc:creator>Martucci, Giovanni</dc:creator>
      <dc:creator>Rosoldi, Marco</dc:creator>
      <dc:creator>Poltera, Yann</dc:creator>
      <dc:creator>Cardós, Cristina</dc:creator>
      <dc:creator>Prats, Natalia</dc:creator>
      <dc:creator>Ambe, Sunji</dc:creator>
      <dc:creator>Cosimato, Gessica</dc:creator>
      <dc:creator>Farah, Antoine</dc:creator>
      <dc:creator>Félix, Christian</dc:creator>
      <dc:creator>Gandolfi, Ilaria</dc:creator>
      <dc:creator>Haefele, Alexander</dc:creator>
      <dc:creator>Hernández, Miguel</dc:creator>
      <dc:creator>Iwabuchi, Masami</dc:creator>
      <dc:creator>Jann, Patrick</dc:creator>
      <dc:creator>Lam, Jason Ming Chun</dc:creator>
      <dc:creator>Marra, Fabrizio</dc:creator>
      <dc:creator>Rodríguez, José María</dc:creator>
      <dc:creator>Roulet, Yves-Alain</dc:creator>
      <dc:creator>Tanaka, Yuta</dc:creator>
      <dc:creator>Dirksen, Ruud</dc:creator>
      <dc:creator>Madonna, Fabio</dc:creator>
      <dc:description><![CDATA[Automated Radiosonde Launchers (ARLs) are increasingly adopted for upper-air observations as they offer major operational advantages compared to manual launches, but they introduce new challenges for maintaining reference-quality humidity measurements within the GCOS Reference Upper-Air Network (GRUAN). In particular, the applicability of the pre-launch Standard Humidity Chamber (SHC) test, routinely used for manual radiosonde launches, has not been systematically assessed for radiosondes stored inside ARLs prior to launch.</p> <p>This study investigates how residence time inside ARLs affects radiosonde humidity sensor performance and the adequacy of SHC tests for automated GRUAN operations. A coordinated experiment was conducted at six sites using three radiosonde models (Vaisala RS41, Meisei IMS-100, and MeteoModem M10) and three ARL systems (Vaisala AS15, Meisei ARS, and MeteoModem Robotsonde). Radiosondes were tested in an SHC prior to storage and again after residence times of 7 and 14 days. Relative humidity biases at saturation (RH = 100 %) were analyzed using aggregated statistics, including a paired RH bias difference&mdash;i.e., the change in bias between pre-storage and post-storage measurements, to quantify temporal drift. A non-parametric bootstrap resampling analysis was first applied to assess the robustness and confidence intervals of the paired RH bias difference estimates. Statistical significance of the paired RH bias difference distributions was subsequently evaluated using the Wilcoxon signed-rank test. A normalized storage-effect metric, combining the systematic drift and variability of the paired RH bias differences, was compared with the GRUAN humidity uncertainty contribution associated with ground preparation.</p> <p>Results indicate that radiosonde humidity performance remains stable for residence times up to 14 days under the tested storage conditions, particularly for the RS41&ndash;AS15 configuration, where only small negative drifts were observed (approximately ~ &minus;0.1 % RH week<sup>-1</sup>). In contrast, the IMS-100&ndash;ARS configuration exhibited a pronounced increase in drift with storage time (approximately ~ &minus;0.8 % RH week<sup>-1</sup>), which was amplified under high-humidity and temperature seasonal conditions, while the M10&ndash;Robotsonde configuration showed a reversed drift with partial bias reduction during storage (~ +0.12 % RH week<sup>-1</sup>). These findings demonstrate that radiosonde behavior during storage strongly depends on the combined radiosonde&ndash;ARL system.</p> <p>Based on the experimental and statistical evidence, an operational upper limit of 14 days for radiosonde storage inside ARLs is recommended for GRUAN-compliant operations, with residence times up to 7 days providing optimal reliability. The study confirms the feasibility of implementing SHC tests for ARL operations while highlighting the need for manufacturer- and site-specific procedures to ensure long-term traceability and consistency of reference humidity measurements. The results demonstrate that residence time inside ARLs constitutes a system-dependent source of uncertainty, warranting explicit inclusion as an additional component in the GRUAN Data Product (GDP) humidity uncertainty budget.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3215</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3215/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere141124</identifier>
    <datestamp>2026-08-12</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[WaggleDop: Autonomous event characterization and adaptive scanning using Doppler LiDAR systems]]></dc:title>
      <dc:creator>Jackson, Robert</dc:creator>
      <dc:creator>Muradyan, Paytsar</dc:creator>
      <dc:creator>Krishnamurthy, Raghavendra</dc:creator>
      <dc:creator>Newsom, Rob</dc:creator>
      <dc:creator>Wharton, Sonia</dc:creator>
      <dc:creator>Puccioni, Matteo</dc:creator>
      <dc:creator>Raut, Bhupendra</dc:creator>
      <dc:creator>Park, Seongha</dc:creator>
      <dc:creator>Sankaran, Rajesh</dc:creator>
      <dc:creator>Collis, Scott</dc:creator>
      <dc:creator>O'Brien, Joseph</dc:creator>
      <dc:creator>Kotamarthi, V. Rao</dc:creator>
      <dc:description><![CDATA[Adaptive scanning plays a key role in balancing observational strategies to address diverse scientific objectives while maximizing data collection for weather phenomena of interest. Current adaptive scanning capabilities for pulsed Doppler LiDARs (model Streamline XR), aimed at probing the streamwise velocity of atmospheric boundary layer flows, are limited to predefined scans based on wind directions derived from short-term wind profiles measured by the same instrument. As a result, high data rejection rates characterize the post-campaign phase due to excessive wind direction misalignment. To expand the Streamline LiDAR&rsquo;s adaptive scanning capabilities, we designed a novel WaggleDop instrument. WaggleDop is an edge computing-enabled system for adaptive scan that supports external inputs and multi-LiDAR configurations via cloud-native infrastructure. In this paper, we test the WaggleDop-LiDAR setup by studying 20 low level jet events and 19 wind reversal events resolved during two U.S. Department of Energy (DOE)-funded field campaigns. We demonstrate that WaggleDop successfully captured these events through adaptive scanning strategies that could not be implemented via classic standalone LiDAR setup, resulting in a substantial enhancement in data availability of up to 90 %. The results shown here demonstrate the importance of more sophisticated scan adaptations to probe complex atmospheric boundary layer flows.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2568</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2568/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144424</identifier>
    <datestamp>2026-08-12</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[Warming-induced agricultural nitrous oxide emissions can offset mitigation benefits of fertiliser management]]></dc:title>
      <dc:creator>Jiang, Jize</dc:creator>
      <dc:creator>Winkel, Lenny H. E.</dc:creator>
      <dc:creator>Stenke, Andrea</dc:creator>
      <dc:creator>Necpalova, Magdalena</dc:creator>
      <dc:creator>Laub, Moritz</dc:creator>
      <dc:creator>Feigenwinter, Iris</dc:creator>
      <dc:creator>Buchmann, Nina</dc:creator>
      <dc:creator>Six, Johan</dc:creator>
      <dc:description><![CDATA[Agriculture is the dominant source of anthropogenic nitrous oxide (N<sub>2</sub>O), a potent greenhouse gas with a high global warming potential. In Switzerland, substantial changes in fertiliser use alongside climatic conditions have occurred over the past four decades, yet the relative contributions of management practices versus environmental change to long-term N<sub>2</sub>O emission trends remain incompletely understood. Here, we applied the biogeochemical model DayCent at 1 km resolution across Switzerland, integrating spatially explicit datasets on climate, soil properties and agricultural management, to quantify N<sub>2</sub>O emissions for the period 1981&ndash;2020 from croplands and grasslands and attribute emission changes to management versus climate drivers. Simulated national N<sub>2</sub>O emissions from agricultural soils declined by roughly 5 % from 4.0 to 3.8 kt N yr⁻&sup1; between the 1980s and 2010s, primarily due to a 25 % reduction in N fertiliser use. Our attribution simulations suggested that under real climate conditions, such a decrease in fertiliser N inputs (&ndash;25 %) over the period studied lowered emissions by 15.2 % in croplands and by 12.0 % in grasslands (including permanent meadows and pastures, and high alpine summer pastures). However, compared to a control scenario (in the absence of climate change), rising temperatures over the past 40 years offset these gains, increasing emissions by 5.7 % in croplands and 13.6 % in grasslands. These results show that warming-induced N<sub>2</sub>O emissions partially negate mitigation from improved fertiliser management, highlighting the need for integrated agricultural N<sub>2</sub>O mitigation strategies that are resilient to future warming.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4445</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4445/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144170</identifier>
    <datestamp>2026-08-12</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[From Earth Observation Access to Spatial Evidence Literacy: Evidentiary Alignment in General-Education Geoscience Communication]]></dc:title>
      <dc:creator>Zhang, Min</dc:creator>
      <dc:description><![CDATA[As environmental challenges become increasingly complex, general education in higher education faces the challenge of preparing students to interpret and communicate environmental information across disciplinary boundaries. Earth Observation (EO) data and geospatial technologies are increasingly available through open archives, cloud platforms, and web maps. However, the expansion of access to spatial data does not automatically enable learners to understand how such data are interpreted, evaluated, and transformed into evidence. This study examines how EO-integrated general education curricula function as sites of curriculum-based geoscience communication, where expert EO and geospatial knowledge is transformed into accessible, communicable, and assessable forms of spatial evidence for non-specialist undergraduates. Using qualitative document analysis, we examine publicly available curriculum materials from 20 undergraduate EO-integrated general education courses in selected APEC higher-education contexts. We analyze the transformation of EO and geospatial knowledge across six curricular dimensions, namely course positioning, learning outcomes, project tasks, scaffolding, assessment, and evidentiary expectations, as well as the role of evidentiary alignment in shaping this transformation. The analysis identifies four patterns of evidentiary alignment, ranging from courses that primarily introduce satellite imagery and geospatial applications to those that require evidence-based reasoning with spatial data. Most sampled courses demonstrate intermediate levels of evidentiary alignment, asking students to interpret spatial patterns or produce maps and Story Maps. These tasks connect EO and geospatial data to climate, sustainability, hazards, urban change, Digital Earth, or geospatial literacy, but evidentiary expectations remain rarely explicit in publicly available documents, especially regarding data quality, uncertainty, scale, validation, and limitations. By extending the understanding of geoscience communication beyond the transmission of scientific information, this study highlights evidentiary alignment as a curriculum-level perspective for examining how curricula transform EO and geospatial knowledge into spatial evidence and create opportunities for developing spatial evidence literacy among non-specialist learners.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4340</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4340/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144201</identifier>
    <datestamp>2026-08-12</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[Analytical improvements and a machine-learning assessment of age dispersion in laser-ablation (U-Th)/He zircon dating]]></dc:title>
      <dc:creator>Ehrenfels, Maximilian K.</dc:creator>
      <dc:creator>Stockli, Daniel F.</dc:creator>
      <dc:creator>Ketcham, Richard A.</dc:creator>
      <dc:creator>Patterson, Desmond B.</dc:creator>
      <dc:creator>Prior, Michael G.</dc:creator>
      <dc:description><![CDATA[Laser-ablation (U-Th)/He dating offers major advantages over conventional whole-grain dissolution analysis, including spatially resolved sampling, minimal sample preparation, and much faster data acquisition. Despite these advantages, the method&rsquo;s full potential is held back by issues including the lack of standardized, fully documented analytical protocols, and age dispersion that commonly exceeds the propagated analytical uncertainty. In this study, we document a complete LA-(U-Th)/He workflow for zircon, combining ultra-high-vacuum laser extraction, white-light-interferometric pit-volume measurement, and time-resolved LA-ICP-MS parent-nuclide quantification, and introducing two methodological refinements: a dynamic multi-phase oxide normalization for the parent concentration calculation, and parent-source depth weighting to account for alpha redistribution. Applied to 811 spots in Fish Canyon Tuff (FCT) zircon, the workflow yields a median age of 28.32 Ma (&sigma;<sub>MAD</sub> = 3.85 Ma; 13.6 %), in agreement with the published reference age, and reduces dispersion by a factor of ~1.7 relative to conventional <sup>29</sup>Si- or <sup>91</sup>Zr-based reductions. To identify the drivers of the remaining dispersion, we train a gradient-boosted regression model on 33 simultaneously measured per-spot parameters. He pit volumes emerge as the strongest predictor of age residuals, highlighting volume-correlated analytical and geometric effects as the largest identifiable and potentially correctable source, while elevated <sup>208</sup>Pb concentrations flag inclusion-related disturbance and provide a practical spot-screening criterion. The measured degree of zonation within the ICP-MS profile on the other hand carries no independent predictive information. Instead, a simple two-layer zonation model shows that U-Th zonation in the grain volume removed during polishing can alone generate age offsets exceeding the entire residual dispersion, a mechanism confirmed by the contrast in dispersion between zoned FCT zircon (13.6 %) and the compositionally homogeneous LGC megacryst (1.5 %). The residual dispersion is therefore not an instrumental limitation, and further gains in precision will require a new generation of methods that characterize or circumvent the polished-away parent-source volume.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4367</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4367/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144207</identifier>
    <datestamp>2026-08-12</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[Wine, victuals and volcanoes &ndash; potential impacts of the 1640/1641 double volcanic eruption on climate and society in early modern Switzerland]]></dc:title>
      <dc:creator>Bartlome, Niklaus Emanuel</dc:creator>
      <dc:description><![CDATA[This study examines how three municipal hospitals on the Swiss Plateau &ndash; in Fribourg, Bern and St. Gallen &ndash; coped with climate anomalies in the early 1640s that coincided with the Komagatake/Parker double volcanic eruption. The eruption led to catastrophic consequences in regions such as China, Japan and northern Europe. Unlike these regions, Switzerland did not experience a comparable famine. Rather than focusing on a narrative of disaster, the study analyses how local authorities coped with climate anomalies. The focus is on the cities of Fribourg, Bern and St. Gallen and their respective municipal hospitals (care institutions), whose economies and agrarian sectors (viticulture, husbandry, dairy production and crop cultivation) are analysed. Between 1639 and 1643, the study region experienced cold springs and summers, likely resulting from a combination of internal stochastic variability and volcanic forcing from the double eruption. All sectors of the hospitals&rsquo; agricultural production were affected simultaneously, due to their interconnectedness. The hospitals&rsquo; greatest vulnerability was the extent of their involvement in direct cultivation. Staple food shortages and high prices caused by multi-annual climate anomalies and the impacts of the neighbouring war between France and the Franche-Comt&eacute; led to a subsistence crisis across the Swiss Plateau. Coping strategies were implemented on two levels. Hospitals adopted internal measures, such as switching from exporting to importing foodstuffs or reducing unnecessary expenditure, to increase the availability of staple food products. They also benefited from external measures ordered by the city authorities, who issued mandates to ensure food security for their populations. Although the available hospital records do not show an obvious increase in recorded deaths among residents and the authorities&rsquo; economic policy coincided with a peasant revolt in Bern in 1641, the subsistence crisis nonetheless placed the hospitals under considerable pressure. While the study primarily focuses on urban populations, further research on rural populations would be useful to examine how they coped with the subsistence crisis.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4370</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4370/]]></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:egusphere144290</identifier>
    <datestamp>2026-08-12</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[Increasing model parsimony without loss of process fidelity: a simplified LASCAM rainfall-runoff model]]></dc:title>
      <dc:creator>Zhang, Ziqi</dc:creator>
      <dc:creator>Fowler, Keirnan</dc:creator>
      <dc:creator>Turner, Margot</dc:creator>
      <dc:creator>Hall, Joel</dc:creator>
      <dc:description><![CDATA[Rainfall-runoff models are widely used to support water resource planning, yet many struggle under prolonged drought. During these periods, cumulative water deficits can strongly affect streamflow response by altering vegetation water use and contributing to multi-annual storage dynamics. The Large Scale Catchment Model (LASCAM) is well suited to representing these processes through its deep groundwater store and flux structure, but its large number of calibrated parameters increases computational cost and limits practical application. This study developed a simplified version of LASCAM by reducing the number of free parameters while retaining the structural features of the original model. Using the latest version of LASCAM (LASCAM22) as the starting point, we applied a staged simplification procedure that combined sensitivity analysis, parameter default-value testing, and stepwise parameter-fixing calibration. The reduced configuration was then compared with GR4J, Sacramento, and LASCAM22 in split-sample testing. Several low-sensitivity parameters were fixed with limited loss of performance, while the stepwise parameter-fixing calibration supported the 15-parameter configuration (LASCAM15) as the best compromise between dimensionality reduction and performance retention. In the split-sample test, LASCAM15 achieved stronger validation performance than LASCAM22 and outperformed GR4J and Sacramento during both calibration and validation. The resulting model is more parsimonious (i.e., fewer calibrated parameters), is more computationally efficient to calibrate, and provides more robust simulations for catchment modelling applications.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4407</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4407/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143685</identifier>
    <datestamp>2026-08-12</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[Sea level rise in Los Santos and Los Angeles: a comparative flood analysis using Grand Theft Auto V]]></dc:title>
      <dc:creator>Nörenberg, Paul</dc:creator>
      <dc:creator>Lantuit, Hugues</dc:creator>
      <dc:description><![CDATA[We present the first quantitative GIS-based flood inundation analysis using terrain data extracted from a commercial video game, applied to the fictional city of Los Santos from Grand Theft Auto V (GTA V) under two contrasting IPCC Fifth Assessment Report (AR5) Representative Concentration Pathway (RCP) scenarios (RCP 2.6, strong mitigation, and RCP 8.5, high-emission baseline) combined with historical storm surge records from the Los Angeles tide gauge, across three time horizons (2100, 2300, and 2500). Los Santos serves as an ideal case study because it faithfully replicates Los Angeles (LA), enabling direct comparison of simulated flood outcomes in the game world with published scientific vulnerability analyses for LA. Results indicate that Los Santos is modelled with sufficient geomorphological detail for projected flooding patterns to closely resemble those identified for Los Angeles, including the spatial sequence of inundation across the marina district, the Pacific Palisades coastline, and the port. Under RCP 8.5 conditions with storm surges, combined sea levels of up to 5.18 m by 2300 would inundate 5.1 % of the mapped land area; in a longer-term illustrative projection to 2500, extreme sea levels of 8.22 m would inundate 6.5 %, rendering the port, wastewater infrastructure, and coastal energy facilities permanently non-functional. The mitigation scenario RCP 2.6 limits inundation to 2.2 % of land area at 2300 with no major infrastructure at risk. We evaluate the potential of this approach for geoscience communication and education, arguing that the intrinsic familiarity of the Los Santos environment provides an affective engagement with climate change impacts that is difficult to achieve through conventional visualisation alone.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4130</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4130/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143509</identifier>
    <datestamp>2026-08-12</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[Brief communication: Repeated supraglacial lake drainage from the Purepu Glacier system, central Himalaya]]></dc:title>
      <dc:creator>Xu, Qiangqiang</dc:creator>
      <dc:creator>Kang, Shichang</dc:creator>
      <dc:creator>Du, Wentao</dc:creator>
      <dc:creator>Wu, Wei</dc:creator>
      <dc:creator>Hu, Zhaofu</dc:creator>
      <dc:creator>He, Xiaobo</dc:creator>
      <dc:creator>Cao, Bo</dc:creator>
      <dc:creator>Xie, Biwen</dc:creator>
      <dc:description><![CDATA[We report repeated drainage from the Purepu supraglacial lake system in the central Himalaya using high-resolution satellite imagery. A satellite-inferred 2023 drainage event is constrained to 12&ndash;15 July, whereas a reported GLOF occurred early on 8 July 2025. Both followed lake expansion to ~0.70&ndash;0.72 km&sup2;, but DEM-constrained lake-volume loss increased from 0.87 &times; 10⁶ m&sup3; in 2023 to 3.55 &times; 10⁶ m&sup3; in 2025. The 2025 event remained incomplete, and flood-volume reconstruction suggests additional englacial or subglacial contributions cannot be excluded. Residual water persisted into 2026, supporting high-frequency monitoring in early July 2026.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4065</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4065/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere145123</identifier>
    <datestamp>2026-08-12</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[Accelerating greenhouse gas retrievals with neural network-based forward models]]></dc:title>
      <dc:creator>Lippert, Fiona</dc:creator>
      <dc:creator>Barr, Andrew Gerald</dc:creator>
      <dc:creator>Herreras-Giralda, Marcos</dc:creator>
      <dc:creator>Momoi, Masahiro</dc:creator>
      <dc:creator>Rejano, Fernando</dc:creator>
      <dc:creator>Lu, Sha</dc:creator>
      <dc:creator>Hasekamp, Otto</dc:creator>
      <dc:creator>Dubovik, Oleg</dc:creator>
      <dc:creator>Malina, Edward</dc:creator>
      <dc:creator>Landgraf, Jochen</dc:creator>
      <dc:description><![CDATA[Greenhouse gas (GHG) retrievals rely on repeated evaluations of computationally expensive physics-based forward models, which limit the feasibility of near-real-time retrievals and timely detection of emission hotspots. A promising alternative is to replace these forward models with fast machine learning emulators trained to approximate their input-output mapping, while retaining the overall retrieval algorithm.</p> <p>Here, we assess the feasibility of this approach in the context of the Sentinel-5 mission, systematically comparing two different emulation strategies: an end-to-end approach, which directly approximates the full forward model with neural networks, and a hybrid approach, which combines fast non-scattering simulations with a neural network-based correction for atmospheric scattering effects. We comprehensively validate each emulator in the full retrieval chain, evaluating their impact on the accuracy of retrieved XCO<sub>2</sub> and XCH<sub>4</sub>.</p> <p>Our results show that a hybrid approach is needed to meet the stringent accuracy requirements on XCH<sub>4</sub> and XCO<sub>2</sub>. While the end-to-end emulator achieves large speed-ups exceeding a factor of 300, it introduces considerable errors of 7.22 ppb for XCH<sub>4</sub> and 4.25 ppm for XCO<sub>2</sub> compared to full-physics retrievals, and fails to generalize to high-emission scenarios beyond the training range. In contrast, the hybrid approach can effectively leverage the information provided by the non-scattering approximation, reducing emulator-induced retrieval errors to less than 1.5 ppb for XCH<sub>4</sub> and 0.5 ppm for XCO<sub>2</sub>, while still being an order of magnitude faster than full-physics retrievals and maintaining robust performance for high-emission scenarios.</p> <p>Together, these results pave the way for operational deployment of neural network-based forward models in GHG retrievals from Sentinel-5, and more broadly demonstrate the potential of hybrid machine learning emulators to facilitate timely and accurate processing of the rapidly growing data volumes from modern satellite missions.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4724</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4724/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144896</identifier>
    <datestamp>2026-08-12</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[An Open-Source Python Framework for the Flexible Deployment and Advanced Applications of the Variable Infiltration Capacity (VIC) Model]]></dc:title>
      <dc:creator>Zheng, Xudong</dc:creator>
      <dc:creator>Liu, Dengfeng</dc:creator>
      <dc:creator>Tang, Qiuhong</dc:creator>
      <dc:creator>Li, Qiang</dc:creator>
      <dc:creator>Liao, Haoyu</dc:creator>
      <dc:creator>Wang, Hao</dc:creator>
      <dc:description><![CDATA[The development of the Variable Infiltration Capacity (VIC) model to version 5 has endowed it with enhanced land-surface-modelling features, establishing it as a modern and cutting-edge tool for hydrological research. However, its adoption is limited by challenges in complex data processing and parameter preparation. To address this issue, this study proposes the Easy VIC Build (EVB) framework, an open-source Python package with an object-oriented, modular design, developed for efficient and flexible VIC deployment. Two real-world basin setups were selected for model application to validate the effectiveness of the EVB framework. The results indicate that, based on the EVB framework, reliable spatial parameters with robust transferability can be derived, while VIC models can be conveniently deployed and achieve satisfactory simulation performance. The EVB framework provides a well-suited workbench for advanced applications of the VIC model, promising to further leverage the value of VIC-5 in hydrology and related fields.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4655</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4655/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144885</identifier>
    <datestamp>2026-08-12</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[Quantifying trends and transitions in a Miocene benthic &delta;18O stack]]></dc:title>
      <dc:creator>Hobart, Bethany</dc:creator>
      <dc:creator>Zhou, Yuxin</dc:creator>
      <dc:creator>Lee, Taehee</dc:creator>
      <dc:creator>Lawrence, Charles E.</dc:creator>
      <dc:creator>Lisiecki, Lorraine E.</dc:creator>
      <dc:description><![CDATA[Marine isotopic records from benthic foraminifera are central to understanding Miocene climate, but developing reliable Miocene age models that are consistent across sites has been challenging due ambiguities in biostratigraphy and magnetostratigraphy. Detailed chemostratigraphic alignment of globally distributed marine records can assist in comparing paleoclimate proxy records and their proposed forcing mechanisms. We present a continuous benthic &delta;<sup>18</sup>O stack (average) across the Miocene based on alignment of published records from 24 sites. Stack estimates of global mean benthic &delta;<sup>18</sup>O changes may improve reconstructions of Miocene ice volume change and deep-sea cooling and help distinguish between causal mechanisms. We estimate the rate of change in the global stack&rsquo;s benthic &delta;<sup>18</sup>O throughout the Miocene as well as the amplitude of abrupt transitions associated with the onset of the Miocene Climatic Optimum (MCO) and the Middle Miocene Climatic Transition (MMCT). We find that the global stack&rsquo;s change in benthic &delta;<sup>18</sup>O across the abrupt onset of the MCO at ~16.9 Ma is 0.27 &permil;, which is about half the amplitude recorded in the deep Eastern Equatorial Pacific (EEP) and in the CENOGRID splice (Westerhold et al., 2020). We additionally find the total change in stack benthic &delta;<sup>18</sup>O across the Miocene is 0.82 &permil;, which is 15 % less than in the CENOGRID splice.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4648</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4648/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144812</identifier>
    <datestamp>2026-08-12</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[Bank Pull or Bar Push: Who Leads the Dance of Meander Migration?]]></dc:title>
      <dc:creator>Nagel, Gustavo W.</dc:creator>
      <dc:creator>Darby, Stephen</dc:creator>
      <dc:creator>Leyland, Julian</dc:creator>
      <dc:creator>Lazarus, Eli D.</dc:creator>
      <dc:description><![CDATA[Despite significant advances in the study of meandering rivers, the precise mechanisms by which erosion and sedimentation interact to drive meander migration remain poorly understood. Two long-standing competing theories attempt to explain this interaction: one suggests that inner-bank sediment deposition precedes outer-bank erosion (bar push), while the other posits that outer-bank erosion initiates inner-bank sedimentation (bank pull). To date, empirical research addressing which of these mechanisms dominates in real-world environments has predominantly focused on a small number of bends and at limited temporal scales. In this paper, we identify analyse the occurrence of bank pull versus bar push across 4,923 river bends worldwide. We estimated outer-bank erosion and inner-bank sedimentation rates using a 38-year time series of Landsat data, from which classifications of bank pull and bar push were derived through Dynamic Cross-Correlation analysis. Of the 4,923 bends analyzed, 20 % were classified as bank pull dominated, 16 % as bar push dominated, whilst the remaining 63 % showed no clear migration signal. We also identified river characteristics that control the relative frequency of push versus pull migrating bends. Our findings indicate that vegetated bends, with higher soil compactness surrounded by sandy substrates and situated in rivers with slower flow velocities, are more likely to exhibit bend migration via bar push, where sediment deposition along the inner bank plays a dominant role. In contrast, less densely vegetated rivers with higher flow velocities and lower soil compactness show a higher occurrence of bends migrating via bank pull. This means that most bar-push migrating bends are located in densely vegetated tropical environments, with bar pull tending to dominate in other regions. This study represents the first quasi-global empirical framework capable of distinguishing the temporal sequencing of erosion and sedimentation across thousands of river bends using long-term satellite observations, providing valuable insights that could be used to improve river dynamics modelling and inform more effective river management strategies.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4621</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4621/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144795</identifier>
    <datestamp>2026-08-12</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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       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
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      <dc:title><![CDATA[An assessment of the North Atlantic Oscillation in the Late Pliocene and its impact on European climate]]></dc:title>
      <dc:creator>Buchan, Abigail E. C.</dc:creator>
      <dc:creator>Haywood, Alan M.</dc:creator>
      <dc:creator>Dolan, Aisling M.</dc:creator>
      <dc:creator>Hill, Daniel J.</dc:creator>
      <dc:creator>Tindall, Julia C.</dc:creator>
      <dc:description><![CDATA[The North Atlantic Oscillation (NAO) heavily influences European climate and weather and is projected to change with future warming. Despite it's strong links to climate, there has not yet been an analysis of the NAO using the most recent climate model simulations of the Late Pliocene. Using data from the Pliocene Model Intercomparison Project Phase 2 (PlioMIP2), the NAO and North Atlantic atmospheric circulation are analysed. In winter an increased meridional sea level pressure gradient contributes to an increase in the multi-model mean NAO index. However, this is model dependent with only a few models displaying changes in the NAO index. Using forcing factorisation simulations, the differences in sea level pressure are found to be driven by non‑CO<sub>2</sub> boundary conditions such as ice sheets and orography. These changes in the NAO also relate to shifts in the zonal winds, with North Atlantic Westerlies being more poleward in winter, and more equatorward in summer. When examining European climate, Northern Europe is on average wetter in the Late Pliocene compared to the pre‑industrial, but this is not linked to a difference in NAO behaviour. The simulations examined all show increased mean precipitation over Northern Europe in the Late Pliocene compared to the pre-industrial. Shifts in the distribution of wettest month rainfall are not linked to any change in the NAO index. This could imply changes in Northern European Late Pliocene precipitation extremes, but that these differences are may not be related to differences in the NAO. These shifts in rainfall distributions demonstrate the importance of considering multiple models when examining variability, especially in a palaeoclimate context.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4616</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4616/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144787</identifier>
    <datestamp>2026-08-12</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[Contrails cannot exist without flights: physics-informed contrail detection, tracking, and attribution in ground-based camera video]]></dc:title>
      <dc:creator>Dalmau, Ramon</dc:creator>
      <dc:creator>Jarry, Gabriel</dc:creator>
      <dc:creator>Very, Philippe</dc:creator>
      <dc:description><![CDATA[A contrail cannot exist without a flight. We exploit this constraint by inverting the usual detect-then-attribute pipeline: instead of finding contrails in an image and asking which flight made them, we start from each flight and ask whether its contrail is visible. Aircraft positions from surveillance data and reanalysis wind fields feed a contrail lifecycle model that predicts where each flight's contrail should appear in a ground-based camera image, not at the aircraft's position but where the wind has carried the plume. These predictions become spatial prompts that guide a video segmentation model to either outline the contrail or reject the prompt when nothing is visible. Because each prompt belongs to exactly one flight, the output mask carries the flight's identity by construction, and tracking across frames requires no re-identification. We compare prompt encodings of increasing physical richness: binary presence, age-weighted freshness, and suppression of competing flights. On the Ground Visible Camera Contrail Sequences dataset, the richest design improves mean average precision, averaged over intersection-over-union matching thresholds from 0.25 to 0.75, by 25 % over the binary baseline, reaches 96.2 % attribution precision, rejects empty prompts with an area under the receiver operating characteristic curve of 0.97, and maintains detection across roughly three-quarters of a contrail's visible lifetime. A video-level cluster bootstrap confirms the attribution and segmentation-quality gains, and is equally clear that the richer prompts do <em>not</em> find more contrails: detection coverage is statistically indistinguishable from the binary baseline. What richer prompts buy is delineation and identity, not discovery.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4608</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4608/]]></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:egusphere144706</identifier>
    <datestamp>2026-08-12</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[Post-depositional Geochemical Transformations of Aerosol Impurities in EPICA Dome C Ice Core: Dissolution, Mineral Neoformation, and Immobilization Revealed by CFA-sp-ICP-TOFMS]]></dc:title>
      <dc:creator>Lee, Geunwoo</dc:creator>
      <dc:creator>Erhardt, Tobias</dc:creator>
      <dc:creator>Larkman, Piers</dc:creator>
      <dc:creator>Zeppenfeld, Chantal</dc:creator>
      <dc:creator>Jackson, Sarah</dc:creator>
      <dc:creator>Schmitt, Jochen</dc:creator>
      <dc:creator>Delmonte, Barbara</dc:creator>
      <dc:creator>Baccolo, Giovanni</dc:creator>
      <dc:creator>Ritz, Catherine</dc:creator>
      <dc:creator>Wilhelms, Frank</dc:creator>
      <dc:creator>Dahl-Jensen, Dorthe</dc:creator>
      <dc:creator>Nikolaus, Kevin Michael</dc:creator>
      <dc:creator>Bohleber, Pascal</dc:creator>
      <dc:creator>Fischer, Hubertus</dc:creator>
      <dc:description><![CDATA[Aerosol-derived impurities in deep Antarctic ice cores provide high-resolution records of past climate and atmospheric variability. However, post-depositional englacial geochemical processes driven by impurity remobilization through ice metamorphism can perturb the originally deposited signals, challenging the interpretation of deep ice records. To address this, we investigate englacial mineral alterations by analyzing the elemental composition of 18 ice-core sections of the EPICA Dome C (EDC) ice core (ranging from 281.6&ndash;3137.1 m depth) using single-particle inductively coupled plasma time-of-flight mass spectrometry (sp-ICP-TOFMS) coupled to a continuous flow analysis (CFA) system. This reveals a deep-ice environment dominated by pervasive acid dissolution, leaving behind refractory mineral phases. We document the progressive neoformation of potassium-rich alunite-supergroup minerals (jarosite, alunite, and mixed phases) and the probable formation of Fe-(oxyhydr)oxide coatings. These secondary phases concurrently immobilize trace elements (iodine, arsenic, lead) via surface adsorption and structural substitution. These transformations occur within highly localized microenvironments and are accelerated by increasing in situ temperatures with depth. They are further enabled by the old age of deep ice, which provides hundreds of thousands of years for these reactions to occur. These findings underscore the importance of accounting for the effects of post-depositional geochemical transformation when interpreting impurity records from EDC and other old ice cores. The colder thermal regime of the Beyond EPICA Little Dome C is expected to lead to slower geochemical transformation, potentially providing a higher-fidelity impurity record for the epochs currently covered by EDC.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4574</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4574/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
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  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144563</identifier>
    <datestamp>2026-08-12</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[Humanitarian Needs in a Protracted Crisis: Systemic Impact of the June 2026 Venezuelan Earthquakes]]></dc:title>
      <dc:creator>García Guzmán, Lester Fidel</dc:creator>
      <dc:creator>Hasan, Mehedi</dc:creator>
      <dc:creator>Tekleberhan Weldesilasie, Esrom</dc:creator>
      <dc:creator>Durá Vicaria, Lucia</dc:creator>
      <dc:creator>Jiménez Ramírez, Yonathan Josué</dc:creator>
      <dc:creator>Eriksson, Anneli</dc:creator>
      <dc:description><![CDATA[The Venezuelan humanitarian crisis is a protracted emergency characterized by systemic stagnation. This study measures the trend of humanitarian needs from 2020 to 2026 using the 7eed framework. The severity score reached a plateau of 16.5 (High Severity); additionally, the 2026 Need Score (130.5) represents an official baseline projection formulated prior to the June 24 seismic events. The twin earthquakes caused an estimated $37 million in losses and added 1.3 million people to the 2026 population in need.</p> <p>This methodology identified a significant correlation between the collapsed health system and crisis stagnation at a high-severity level. The Syrian emergency serves as the most accurate comparative proxy for managing this health system collapse. Addressing a health system collapsed prior to seismic events requires holistic strategies; isolated, disaster-focused interventions risk becoming temporary solutions that deepen the crisis.</p> <p>Comparing pre- and post-disaster severity and need scores validates the utility of this model in recognizing acute disaster impacts within a protracted emergency. Medium- and long-term planning must adopt a Triple Nexus approach, integrating humanitarian aid, peacebuilding, and development. Ultimately, utilizing the Need Score to guide funding allocation presents a critical opportunity to reduce human suffering by overcoming inefficiencies inherent in delayed emergency decision-making.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4524</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4524/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144689</identifier>
    <datestamp>2026-08-12</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[Are we approaching water budget closure at basin scale for the right reasons?]]></dc:title>
      <dc:creator>Lefebve, Julien</dc:creator>
      <dc:creator>Biancamaria, Sylvain</dc:creator>
      <dc:creator>Blazquez, Alejandro</dc:creator>
      <dc:creator>Munier, Simon</dc:creator>
      <dc:creator>Gal, Laetitia</dc:creator>
      <dc:creator>Augusto Jucá Oliveira, Rômulo</dc:creator>
      <dc:creator>Etchanchu, Jordi</dc:creator>
      <dc:description><![CDATA[The water cycle represents the continuous circulation of water through the atmosphere, the continents and the oceans. At the basin scale, this cycle can be decomposed into incoming and outgoing fluxes as well as changes of water stored within the basin. The relationship between these fluxes and changes in storage is called the water budget. Closing the water‑budget at basin scale, using observations, model outputs or a combination of both, provides a deeper understanding of water fluxes, storage changes as well as the underlying hydrological processes.</p> <p>Satellite measurements, especially those from the Gravity Recovery And Climate Experiment (GRACE, 2002&ndash;2017) and GRACE Follow-On (GRACE-FO, 2018&ndash;present) missions, now allows to estimate the water budget closure level for large basins worldwide, including those poorly or not instrumented at all. One of the outgoing fluxes for exorheic basins, river discharge, is not available for many basins, particularly during the twenty‑first century due to the spatial and temporal heterogeneity of openly accessible in‑situ river discharge. To address this issue, several studies have attempted to close the basin‑scale water‑budget by estimating river discharge as the simple sum of runoff calculated from Land Surface Models. Despite well-documented significant errors in runoff estimation, uncertainties associated with these approaches are often neglected as river discharge is, in most cases, the flux with the smallest amplitude in the water budget. In this study, using an ensemble approach to assess the state‑of‑the‑art estimates of water cycle fluxes and stocks, we precisely evaluate the impact of river discharge errors on the conclusions drawn from the water budget analysis of 82 exorheic basins worldwide. When ensembles of products are used to estimate combination of precipitation, evapotranspiration and discharge that are the closest to the GRACE storage change variations, we demonstrate compensations between the components of the water budget can occur. Although river discharge is the flux with the smallest amplitude, its dispersion (36 %), when derived from aggregated runoff, is comparable to that of precipitation (44 %) and evapotranspiration (34 %) and a seemingly high level of water budget closure can be achieved with, for some basin, errors of more than 40 % in the annual volume assessment of precipitation and evaporation. Errors caused by these compensations are larger for continental, sub‑arctic and polar basins (around 15  %) than for tropical, arid and temperate basins (around 6  %). Moreover, applying a simple routing scheme to the runoff does not significantly reduce these errors. In this study, we mitigate and assess these compensations by using a combination of in situ and satellite-based discharge estimates. Future studies should explore methods that further limit the compensation effect when attempting to approach a water budget closure at basin scale.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4569</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4569/]]></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:egusphere144443</identifier>
    <datestamp>2026-08-12</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[Meso to sub-mesoscale origins of strong surface winds and influence of surface waves in an extra-tropical cyclone]]></dc:title>
      <dc:creator>Brumer, Sophia E.</dc:creator>
      <dc:creator>Pantillon, Florian</dc:creator>
      <dc:creator>Pianezze, Joris</dc:creator>
      <dc:creator>Maury, Nicolas</dc:creator>
      <dc:description><![CDATA[Extra-tropical cyclones can bring extreme surface winds. Several mesoscale jets can be associated with these winds originating from the upper, mid, and lower troposphere. Sub-mesoscale processes have been shown to play a major role in the downward transport of jets, but few modeling studies represent them explicitly. This study sheds light in the relative contribution and storm-relative location of jets present in the explosive cyclone Alex which made landfall in southern Brittany in October 2020 causing extensive wind damage in Belle-Ile and further inland. A series of stand-alone atmospheric simulations and coupled wave-atmosphere simulations using the Meso-NH and WAVEWATCH-III<sup>&reg;</sup> models were run. Their horizontal grid spacing was incrementally halved by two going from 1.6 km (numerical weather prediction mode) down to 100 m (large eddy simulation mode). The simulated storm is consistent across resolutions at the mesoscale with little differences in extreme wind values between the kilometric and hectometric resolutions. Waves coupling is shown to decrease surface wind extremes by 0.5 to 1.5 m s<sup>-1</sup>. Impacts on the surface drag coefficient and winds are not uniform spatially with winds decreasing ahead of the cold front and within the high wind core while decreasing elsewhere. Online trajectory calculations allow for a Lagrangian air mass tracking in Meso-NH. In the kilometric simulation, four distinct jets are shown to be responsible for the strongest winds. The evolution of state parameters along these trajectories helps match the jets to the classical conceptual model for extra-tropical cyclones. Evidence hints to the presence of a Sting Jet associated with Alex&rsquo;s extreme winds, along with the more common Cold Conveyor Belt, and Dry Intrusion. The fourth jet is labeled as Potential Sting Jet on account of its similarities with the Sting Jet prior to subsidence. The Cold Jet is shown to be responsible not only for the majority of the strong wind trajectories in the lower 500 m, but also for the strongest wind speeds. Spatial distributions of these jets is further investigated in the hectometric simulation. These reveal that the Sting Jet descends towards the surface at the rear of the high wind core in the frontal fracture region. This location differs from that reported for previously studied storms where the sting jets are typically found at the forefront of the high wind core. Two distinct Dry Jets are shown to coexist, one descending to the surface around the Sting Jet and another one remaining above the Cold Jet. The Potential Sting Jet is located above the cold conveyor belt and shown to be brought down towards the lower troposphere by coherent structures invigorated by moist processes and spanning several kilometers in width and height at the outer edge of the cloud head. Unlike in previous high-resolution numerical studies, boundary layer rolls are not found to play a key role at the studied instant. Different sting jet location and processes associated with potential sting jet subsidence compared to literature, encourage more systematic studies of extra-topical cyclones through common diagnostics adapted for both kilometric and hectometric resolutions.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4453</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4453/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144485</identifier>
    <datestamp>2026-08-12</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[Development and Evaluation of Online Gas-Phase Chemistry in the Global Variable-Resolution Atmospheric Model iAMAS (v2.5.1): Resolution-Dependent Surface Ozone over North China]]></dc:title>
      <dc:creator>Xia, Zihan</dc:creator>
      <dc:creator>Zhao, Chun</dc:creator>
      <dc:creator>Jin, Chen</dc:creator>
      <dc:creator>Qu, Xin</dc:creator>
      <dc:creator>Yang, Zining</dc:creator>
      <dc:creator>Zhang, Ziyu</dc:creator>
      <dc:creator>Yang, Qike</dc:creator>
      <dc:creator>Gu, Jun</dc:creator>
      <dc:creator>Li, Gudongze</dc:creator>
      <dc:creator>Feng, Jiawang</dc:creator>
      <dc:creator>Du, Shen</dc:creator>
      <dc:creator>Liu, Jane</dc:creator>
      <dc:description><![CDATA[Atmospheric composition is governed by multiscale processes spanning global transport to local chemistry. Simultaneously capturing these scales is essential, yet conventional modeling trades global coverage for regional detail restricted by artificial boundaries. Global variable-resolution (VR) modeling provides a unified alternative, yet online gas-phase chemistry within nonhydrostatic VR frameworks remains limited, and how mesh refinement alters coupled physical&ndash;chemical responses is not fully understood. Here, we develop and evaluate an online gas-phase chemistry framework in the VR model iAMAS (v2.5.1). Operating on a unified unstructured mesh without lateral boundaries, the modular framework couples KPP-generated SAPRC-99 tropospheric chemistry, Linoz stratospheric ozone, Fast-J photolysis, emissions, transport, and deposition. Global baseline simulations at ~60 km resolution (U60km) for July 2019 validate large-scale tracer distributions (O<sub>3</sub>​, NO<sub>2</sub>, HCHO, CO) and surface ozone diurnal cycles across China. Regionally refined simulations at ~4 km over North China (V4km) demonstrate how online VR chemistry resolves cross-scale physical&ndash;chemical coupling over complex terrain. V4km recovers the observed ridge-high/valley-low nighttime ozone pattern, reversing spatial correlation from R=&minus;0.40(U60km) to R=+0.46 by resolving slope circulations and heterogeneous NO<sub>x​</sub> emissions within a shallow nocturnal boundary layer. Refinement also reorganizes urban&ndash;rural and day&ndash;night ozone responses: higher urban NO<sub>x</sub> suppresses daytime ozone peak under VOC-limited conditions, whereas reduced coarse-grid NO<sub>x</sub> dilution weakens rural nighttime titration and sustains higher ozone. These results demonstrate that mesh refinement in a global VR model alters the coupled dynamical&ndash;chemical state rather than merely sharpening concentration gradients, establishing iAMAS as a modular platform for seamless global-to-regional atmospheric-composition studies.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4483</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4483/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere144490</identifier>
    <datestamp>2026-08-12</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[Towards Resolving Equifinality in Aerosol-Cloud Radiative Forcing Through Process-Level Constraints]]></dc:title>
      <dc:creator>Stanford, McKenna</dc:creator>
      <dc:creator>Mahfouz, Naser</dc:creator>
      <dc:creator>Muelmenstaedt, Johannes</dc:creator>
      <dc:creator>Mikkelsen, August</dc:creator>
      <dc:creator>Burrows, Susannah</dc:creator>
      <dc:description><![CDATA[Equifinality&mdash;where multiple parameter combinations produce indistinguishable climate states&mdash;is a fundamental obstacle to calibrating Earth system models (ESMs). Parameter sets that agree well with the observed mean state can produce dramatically different responses to external perturbations, reflecting a mathematical non-uniqueness that standard calibration approaches cannot resolve. This poses a critical challenge for constraining the effective radiative forcing due to aerosol-cloud interactions (ERF<sub>ACI</sub>), which depends sensitively on cloud responses to aerosol perturbations. We use a perturbed parameter ensemble that, as a minimal working example, varies only two parameters related to warm-rain formation (autoconversion and accretion) and constrain on synthetic observations in a perfect-model setup. Even under ideal conditions, radiation-only constraints produce a fundamentally degenerate, bimodal ERF<sub>ACI</sub> posterior. Incorporating the observable cloud state (liquid water path, ?) for warm marine stratocumulus clouds can resolve this bimodality, but its utility diminishes with large observational uncertainty. A far more robust constraint is achieved by directly targeting the underlying physical process rates that modulate ?. Process-rate constraints effectively eliminate bimodality and dramatically reduce posterior uncertainty even under large assumed observational uncertainties. As process rates are not directly observable, we test their observable proxies as a tractable alternative, finding they offer only limited additional value over cloud state due to their emergent behavior. These results establish a critical principle for ESM calibration: to achieve robust constraints on ERF<sub>ACI</sub> and beyond, it is necessary to constrain both the emergent climate state and the physical pathways that govern its formation.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-4488</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-4488/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142912</identifier>
    <datestamp>2026-08-12</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[Probabilistic modelling for avalanche hazard and risk assessment]]></dc:title>
      <dc:creator>Kleinn, Jan</dc:creator>
      <dc:creator>Aller, Dörte</dc:creator>
      <dc:creator>Bühler, Yves</dc:creator>
      <dc:creator>Glaus, Julia</dc:creator>
      <dc:creator>Peter, Adrian</dc:creator>
      <dc:creator>Hählen, Nils</dc:creator>
      <dc:description><![CDATA[The number of requirements for hazard and risk assessment of mass movements like avalanches has increased over time. We are presenting a feasibility study of applying the approach of probabilistic hazard and risk assessment, which was originally developed for seismic hazards and risks, to avalanches. This modelling approach is based on the idea of simulating a large range of possible events and associate probabilities or rates to these events. The aim of such a probabilistic modelling approach is to provide more nuanced modelling results as a basis for consistent hazard and risk management. It allows to derive continuous intensity frequency curves for any location in the affected area. Furthermore, continuous loss frequency curves can be derived by combining the simulated event intensities with affected objects and their vulnerabilities. The probabilistic modelling approach is enabling several products and applications, which are not possible with the current Swiss approach of hazard and risk assessment for avalanches. This first attempt of the probabilistic modelling approach to avalanches provides plausible results, which are in line with existing hazard assessments. Furthermore, it provides more differentiated results by enabling hazard maps for any given return period, and it enables the generation of maps depicting the probabilities of being affected by avalanches of a certain avalanche intensity. These types of products are not possible with the current Swiss hazard assessment approach.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3799</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3799/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere142775</identifier>
    <datestamp>2026-08-12</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[Mechanistic Insights into Nitric Sulfuric Acid Formation and Its Enhancement of Sulfuric Acid-Ammonia Nucleation under Severe Urban Pollution]]></dc:title>
      <dc:creator>Zhang, Chengyan</dc:creator>
      <dc:creator>Wang, Guanhua</dc:creator>
      <dc:creator>Guo, Xiaokai</dc:creator>
      <dc:creator>Li, Yaogeng</dc:creator>
      <dc:creator>Feng, Xueping</dc:creator>
      <dc:creator>Zuo, Yuan</dc:creator>
      <dc:creator>Wang, Rui</dc:creator>
      <dc:description><![CDATA[Organosulfates (OSs) constitute an important component of secondary organic aerosols (SOA). Although previous studies have investigated the aerosol nucleation of OSs such as glycolic acid sulfate and methyl hydrogen sulfate, exploring the aerosol nucleation behavior of additional OSs remains essential. Herein, the formation mechanism of nitric sulfuric acid (NSA) from the reaction of sulfur trioxide (SO<sub>3</sub>) with nitric acid (NA)and its role in sulfuric acid (SA)-ammonia (A) aerosol nucleation was investigated using quantum chemical calculations combined with kinetic simulations. Our results demonstrate that NSA can be formed rapidly and stably in the gas phase with a low barrier of 3.61 kcal&middot;mol<sup>-1</sup>. The SO<sub>3</sub> + HNO<sub>3</sub> reaction remains competitive with major atmospheric SO<sub>3</sub> loss pathways, including reactions of SO<sub>3</sub> + HCOOH, SO<sub>3</sub> + C<sub>6</sub>H<sub>5</sub>COOH and NH<sub>3</sub>-catalyzed reactions, and even H<sub>2</sub>O-catalyzed hydrolysis under dry conditions. Kinetic simulations further demonstrate that NSA significantly accelerates SA-A nucleation, with rates reaching ~ 10<sup>-3</sup> cm<sup>-3</sup> s<sup>-1</sup> under heavily polluted urban conditions (e.g., Beijing), corresponding to a five-order-of-magnitude enhancement over binary clusters and a 10<sup>1</sup>-10<sup>11</sup>-fold increase relative to nitric acid. These findings underscore the importance of incorporating NSA into atmospheric aerosol models.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3682</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3682/]]></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:egusphere142755</identifier>
    <datestamp>2026-08-12</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[An aircraft-based Bayesian inversion of Berlin CO2 emissions with explicit background treatment]]></dc:title>
      <dc:creator>Pilz, Lukas</dc:creator>
      <dc:creator>Lüken-Winkels, Christopher</dc:creator>
      <dc:creator>Fiehn, Alina</dc:creator>
      <dc:creator>Roiger, Anke</dc:creator>
      <dc:creator>Vardag, Sanam N.</dc:creator>
      <dc:description><![CDATA[Quantifying greenhouse gas (GHG) emissions from urban areas is critical for assessing progress toward climate goals. Aircraft-based measurements provide valuable information on urban emission fluxes; however, their interpretation is often limited by uncertainties in atmospheric background concentrations. Here, we present an emission estimate of Berlin city emissions that explicitly includes background concentrations from a Eulerian background run as state vector elements in a Bayesian inversion framework. Using data from the 20<sup>th</sup> of July flight of the 2018 3DO aircraft campaign of the [UC]<sup>2</sup> (&ldquo;Urban Climates Under Change&rdquo;) project over Berlin and high-resolution GHG and meteorological simulations using Weather Research and Forecasting (WRF) model, we derive a CO<sub>2</sub> emission estimate for the city of Berlin. We find an optimized Berlin emission rate of 13.4 &plusmn; 4.6 MtCO<sub>2</sub>a<sup>&minus;1</sup>. The emissions rate is about 48 % higher than the prior total annual emissions of the TNO anthropogenic bottom-up inventory (time-scaled emissions, 10.8 MtCO<sub>2</sub>a<sup>&minus;1</sup>) and VPRM biogenic (time-varying, -1.7 MtCO<sub>2</sub>a<sup>&minus;1</sup>) and about 30 % of the estimate from the traditional mass balance approach (44 &plusmn; 24 MtCO<sub>2</sub>a<sup>&minus;1</sup>), while reducing the uncertainty by over a factor of five. We verify our posterior background concentration with independent concentration measurements above the boundary layer. This study provides an improved independent estimate of urban emissions and demonstrates that explicit treatment of background concentrations in inversions improves aircraft-based urban flux estimates.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3665</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3665/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143213</identifier>
    <datestamp>2026-08-12</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[Impact of meteorological conditions on rockfalls: a case study of the Saint Eynard cliff]]></dc:title>
      <dc:creator>Bouaziz, Sabrine</dc:creator>
      <dc:creator>Amitrano, David</dc:creator>
      <dc:creator>Lin-Kwong-Chon, Christophe</dc:creator>
      <dc:creator>Méger, Nicolas</dc:creator>
      <dc:creator>Helmstetter, Agnès</dc:creator>
      <dc:description><![CDATA[Rockfall events are influenced by various climatic factors. Identifying these factors is crucial for anticipating rockfall events and managing the risks to infrastructure and populations. Previous studies have particularly highlighted rainfall and freezing conditions as key triggers, based on rockfall catalogs derived from visual observations or diachronic comparisons, with temporal precision ranging from a few to several days.</p> <p>The purpose of this study is to use a catalog derived from seismic detection, giving a much greater temporal accuracy, to explore and better understand the meteorological conditions that contribute to rockfall at Mont Saint-Eynard, a limestone cliff in the French Alps. This study introduces a probabilistic approach that combines different temporal horizons and cumulative models capturing delayed effects to analyze the influence of rainfall and freezing conditions on rockfall triggering. By integrating multiple statistical metrics relative to a specific condition including empirical probabilities, lift measures, confidence intervals and Chi-squared tests, we identified not only the likelihood but also the strength and reliability of triggering patterns. We identified the significant role of short term triggers like recent intense rainfall on high magnitude rockfall, and delayed effect of freezing depth in rockfall activity. This knowledge could be used to implement a risk management strategy.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3939</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3939/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere143090</identifier>
    <datestamp>2026-08-12</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[Balloon-borne measurements of quasi-static electric fields at stratospheric altitudes from low latitudes]]></dc:title>
      <dc:creator>Jawahar, Kaliappan</dc:creator>
      <dc:creator>Mahavarkar, Prasanna</dc:creator>
      <dc:creator>Selvaraj, Chellaiah</dc:creator>
      <dc:creator>Sripathi, Samireddipalle</dc:creator>
      <dc:creator>Gurubaran, Subramanian</dc:creator>
      <dc:creator>Rao, Tanneeru Venkateswara</dc:creator>
      <dc:creator>Dimri, Ashok Priyadarshan</dc:creator>
      <dc:description><![CDATA[This paper describes the design, deployment and performance of an improved balloon-borne payload, BEENS-2 (Balloon Experiment on the Electrodynamics of Near Space), developed to measure quasi-static horizontal and vertical electric fields in the low-latitude stratosphere. Measuring weak electric fields (few mV/m) at altitudes up to 32 km presents significant challenges due to ultra-high atmospheric impedance (10&sup1;&sup3;&ndash;10&sup1;⁴ &Omega;) and payload-induced interference. We present a differential electrometer design utilizing the INA116 instrumentation amplifier to achieve the necessary input impedance and common-mode rejection. To address limitations identified in previous flights, the BEENS-2 configuration employed non-conducting glass-reinforced plastic booms and a redundant, eight-probe setup. We used an inverted probe setup for the vertical field measurements to distinguish ambient vertical electric field from hardware-induced DC offsets. Experimental results from a flight conducted on January 17, 2025, from Hyderabad, India, reveal that electromagnetic noise from the orienter motor significantly masked ambient signals while the motor was in operation. However, by analyzing data during periods when the motor power was withdrawn and the payload slowed down (rotation with &lt; 2 RPM), we successfully recovered horizontal fields of 15&ndash;25 mV/m and a vertical field of ~200 mV/m. The high-resolution data confirms the effectiveness of the measurement approach for future studies on stratospheric electric fields at low latitudes.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-3904</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-3904/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:egusphere140469</identifier>
    <datestamp>2026-08-12</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[Rain gauge aerodynamic design to minimise wind-induced bias in precipitation measurement]]></dc:title>
      <dc:creator>Chinchella, Enrico</dc:creator>
      <dc:creator>Cauteruccio, Arianna</dc:creator>
      <dc:creator>Chan, Pak-Wai</dc:creator>
      <dc:creator>Lanza, Luca G.</dc:creator>
      <dc:description><![CDATA[The presence of wind introduces biases in precipitation measurements obtained from traditional rain gauges due to the interaction between the airflow and the outer shell of the instrument, which acts like a bluff body immersed in a wind stream. The airflow is diverted, creating an updraft and accelerating the flow velocity. This interacts with the fall trajectories of hydrometeors near the gauge rim, causing some to deviate out of the collector. The resulting wind-induced undercatch can be minimised by adopting a suitable design for the outer shell of the gauge. While the effectiveness of an inverted conical shape for the outer walls of the gauge has already been demonstrated in the literature, this work proves that the size and geometric profile of the collector's rim are crucial in reducing the effect of wind on precipitation measurements. Building on the construction requirements derived from operational constraints, various single and dual inclination rim profiles were tested using computational fluid dynamics simulation and Lagrangian particle tracking to identify the most effective design. The proposed rim profile is then thoroughly tested in numerical simulations performed over an extended range of wind speeds and precipitation intensities. The scalability of the rim profile to suit different sizes of the collector area is demonstrated, and adjustment curves are obtained to address residual bias. A comparison with existing high-performance gauges on the market revealed that the proposed design significantly outperforms existing solutions.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/egusphere-2026-2108</dc:identifier>
      <dc:identifier><![CDATA[https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2108/]]></dc:identifier>
      <dc:source>eISSN:</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essd128981</identifier>
    <datestamp>2026-08-12</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"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[OpenMesh: wireless signal dataset for opportunistic urban weather sensing in New York City]]></dc:title>
      <dc:creator>Jacoby, Dror</dc:creator>
      <dc:creator>Yu, Shuyue</dc:creator>
      <dc:creator>Hu, Qianfei</dc:creator>
      <dc:creator>Hine, Zachary</dc:creator>
      <dc:creator>Johnson, Rob</dc:creator>
      <dc:creator>Ostrometzky, Jonatan</dc:creator>
      <dc:creator>Kadota, Igor</dc:creator>
      <dc:creator>Zussman, Gil</dc:creator>
      <dc:creator>Messer, Hagit</dc:creator>
      <dc:description><![CDATA[<p>We introduce OpenMesh, a publicly available dataset of wireless signal measurements from the NYC Mesh, a community-run communication network in New York City (NYC). While originally designed for affordable internet access, these links can be used opportunistically for high-resolution weather monitoring in diverse settings, including dense urban areas, providing 1 min sampling of signal strength measurements with dense spatial coverage across the study region. Spanning eight months of measurements (November 2023 to June 2024), the dataset comprises 103 wireless links in Lower Manhattan and Brooklyn, operating in three primary frequency ranges: 5–6 GHz (C-band), 24 GHz (K-band), and 58–70 GHz (V-band), part of the millimeter-wave (mmWave) spectrum.</p>        <p>Our analysis incorporates meteorological records from two primary sources: (1) 37 Weather Underground (WUnderground) personal weather stations (PWS) across Manhattan and Brooklyn with 5 and 15 min sampling, and (2) three Automated Surface Observing System (ASOS) stations. The study period saw total rainfall of approximately 900 mm and included diverse weather events, from intense rain to snowstorms in winter 2023–2024. These events were captured by the NYC Mesh wireless network, with intense rainfall causing attenuation up to 30 dB and frequent outages, especially on high-frequency V-band links. This highlights the trade-off of using high-frequency bands in wireless networks: while precipitation might cause severe channel disruptions, this greater sensitivity simultaneously makes them effective opportunistic weather sensors. The OpenMesh dataset is available at <a href="https://doi.org/10.5281/zenodo.15287692">https://doi.org/10.5281/zenodo.15287692</a> <span class="cit" id="xref_paren.1">(<a href="#bib1.bibx36">Jacoby et al.</a>, <a href="#bib1.bibx36">2025</a><a href="#bib1.bibx36">b</a>)</span>. By publishing the dataset and demonstrating its usability, we aim to encourage further research that leverages wireless networks for real-time urban weather sensing.</p>]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-18-5817-2026</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/articles/18/5817/2026/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd142311</identifier>
    <datestamp>2026-08-12</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"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[A 1 km resolution dataset of Northern Hemisphere permafrost active layer thickness (2000&ndash;2024)]]></dc:title>
      <dc:creator>Wei, Yujiao</dc:creator>
      <dc:creator>Wu, Zhaoqi</dc:creator>
      <dc:creator>Wang, Jiaxue</dc:creator>
      <dc:creator>Shen, Huanfeng</dc:creator>
      <dc:creator>Chen, Yiyun</dc:creator>
      <dc:description><![CDATA[Active layer thickness (ALT) is a key indicator of permafrost change, with important implications for soil hydrothermal conditions, carbon feedbacks, ecosystem processes, and cold-region infrastructure. However, hemispheric-scale ALT mapping remains challenging because field observations are sparse and unevenly distributed, while thaw depth is controlled by complex and nonlinear environmental interactions. Here, we compiled 2,196 annual ALT observations and developed an ensemble spatiotemporal machine-learning framework to reconstruct a continuous annual ALT dataset at 1 km resolution for the Northern Hemisphere permafrost region from 2000 to 2024. Spatial leave-one-site-out cross-validation yielded an ensemble <em>R<sup>2</sup></em> of 0.76 and an RMSE of 60.48 cm. Independent temporal evaluation showed a significant correlation between observed and predicted Sen&rsquo;s slopes (<em>r</em> = 0.73, <em>p</em> &lt; 0.001), with 86.8 % agreement in trend direction. The dataset reproduced broad latitudinal and elevational patterns, biome-related differences, and interannual variability. Comparisons with two existing 1 km hemispheric products showed that our reconstruction occupied an intermediate position in hemispheric mean ALT while preserving relatively fine spatial variability. Substantial inter-product differences in both magnitude and spatial structure further highlighted persistent structural uncertainty in large-scale ALT mapping. Pixel-wise uncertainty maps further provide spatially explicit information on prediction confidence. This dataset provides a spatially detailed, temporally continuous, and uncertainty-explicit resource for regional- to hemispheric-scale studies of permafrost dynamics, carbon-cycle feedbacks, ecosystem and hydrological responses, and infrastructure exposure.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-447</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-447/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
     </oai_dc:dc>
   </metadata>
  </record>
  <record>
   <header>
    <identifier>oai:publications.copernicus.org:essdd143374</identifier>
    <datestamp>2026-08-12</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"
       xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/
       http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
      <dc:title><![CDATA[4-D Aviation Emission Inventory Data of China Estimated with QAR Data in 2023 (4D-AEID-2023)]]></dc:title>
      <dc:creator>Lu, Binbin</dc:creator>
      <dc:creator>Shi, Lingkun</dc:creator>
      <dc:creator>Wang, Chun</dc:creator>
      <dc:creator>Sun, Huabo</dc:creator>
      <dc:creator>Guo, Qinli</dc:creator>
      <dc:creator>Wang, Xinbo</dc:creator>
      <dc:creator>Wang, Xuhui</dc:creator>
      <dc:description><![CDATA[Accurate aviation emission inventories are essential for environmental impact assessment and mitigation, yet existing estimates predominantly rely on aircraft performance models and standardized assumptions, introducing significant uncertainties. Here, we present a high-resolution, four-dimensional aviation emission inventory for China's civil aviation sector in 2023, built directly from Quick Access Recorder (QAR) data covering 4.52 million flights (~96.8 % of national commercial movements). By coupling second-level fuel-flow measurements with observed flight-state and meteorological parameters via the Boeing Fuel Flow Method 2 and a dynamic thermodynamic correction, this dataset yields temporally and spatially explicit emission estimates for CO₂, NOₓ, SO₂, PM, CO, and HC across all flight phases. In 2023, China's civil aviation consumed 28.4 Mt of fuel, emitting 89.3 Mt CO₂, 634.6 kt NOₓ, 28.4 kt SO₂, 8.46 kt PM, 44.3 kt CO, and 6.35 kt HC. Monte Carlo analysis demonstrates that direct physical observations substantially constrain inventory uncertainty, reducing coefficients of variation (CV) for major pollutants to 2 %&ndash;10 % and shifting the dominant error source from activity-level assumptions to emission index parameterizations. High temporal resolution reveals pronounced phase-specific variations: taxiing accounts for 23.7 % of HC and 19.4 % of CO emissions due to low-thrust incomplete combustion, while the brief high-thrust acceleration segment preceding climb contributes 18.0 % of total PM. Spatially, emissions are highly concentrated, with the top 10 % of grid cells accounting for 74.2 % of national CO₂ emissions, exhibiting significant clustering (Global Moran's I = 0.3389, p &lt; 0.05) along major corridors. Providing second-level and high resolution, this dataset serves as an observation-based benchmark for refining existing inventories and assessing near-airport air quality. The dataset is publicly available at <a href="https://doi.org/10.5281/zenodo.20828076" target="_blank" rel="noopener">https://doi.org/10.5281/zenodo.20828076</a> (Lu et al., 2026).]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-530</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-530/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:essdd144806</identifier>
    <datestamp>2026-08-12</datestamp>
    <setSpec>essdd</setSpec>
   </header>
   <metadata>
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      <dc:title><![CDATA[CFDID: a China Flood Disaster Impact Database from 1994 to 2023]]></dc:title>
      <dc:creator>Cui, Shibo</dc:creator>
      <dc:creator>Li, Ni</dc:creator>
      <dc:creator>Hu, Shiruo</dc:creator>
      <dc:creator>Wan, Zhiqi</dc:creator>
      <dc:creator>Wang, Jiaru</dc:creator>
      <dc:creator>Tang, Jinchao</dc:creator>
      <dc:creator>Zhang, Ruixi</dc:creator>
      <dc:creator>Li, Yingjia</dc:creator>
      <dc:creator>Yu, Xinpeng</dc:creator>
      <dc:creator>Tan, Yiqian</dc:creator>
      <dc:creator>Shan, Wenbo</dc:creator>
      <dc:creator>Zhao, Jianshi</dc:creator>
      <dc:description><![CDATA[China is one of the countries most severely affected by flood disasters worldwide. Long-term and systematic flood impact data are essential for flood risk assessment, flood impact model calibration, disaster prevention and reduction. However, an open, long-term, China-focused event-scale database with detailed flood disaster impact indicators remains lacking. Here we present the China Flood Disaster Impact Database (CFDID), which contains 1716 flood disaster event records from 1994 to 2023, including 1391 top-level (L1) event records. CFDID is compiled from 66 official documents and covers five flood-related disaster categories: rainstorm flood, typhoon, snowmelt flood, ice-jam flood, and dam-break flood. Each record includes date, location, disaster category, eight impact indicators, and data source. The database was constructed using a workflow that combines optical character recognition (OCR), large language model (LLM)-based information extraction, and manual verification, thereby improving the efficiency of converting unstructured text information into structured event records while ensuring data quality. Based on these L1 records, CFDID achieves total coverage ratios of 67.22 % for deaths and missing persons, 72.25 % for affected population, 60.70 % for affected cropland area, 65.68 % for collapsed dwellings, and 74.86 % for direct economic losses relative to official annual flood disaster impact totals during 1994&ndash;2023. Compared with commonly used international flood impact databases, CFDID contains more flood disaster event records and has higher coverage for most impact indicators. CFDID also includes agricultural impact indicators, which are rarely available in international hazard impact databases. CFDID is available at https://doi.org/10.5281/zenodo.21699973 and will be continuously updated by year.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-607</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-607/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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   <header>
    <identifier>oai:publications.copernicus.org:essdd141622</identifier>
    <datestamp>2026-08-12</datestamp>
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   </header>
   <metadata>
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      <dc:title><![CDATA[A Global Dataset of Individual Fire Events (2012&ndash;2025) derived from VIIRS Active Fire Product]]></dc:title>
      <dc:creator>Su, Hongxuan</dc:creator>
      <dc:creator>Yu, Yan</dc:creator>
      <dc:description><![CDATA[Accurate characterization of individual fire events is critical for understanding global fire regimes and their interactions with climate. However, existing global inventories relying on coarse-resolution data and annual-aggregation algorithm may obscure small-scale thermal anomalies and artificially fragment prolonged fires. Here, we present a global dataset of individual fire events for 2012&ndash;2025 derived from Suomi-NPP VIIRS 375 m active fire detections. To address the spatiotemporal discontinuities in conventional clustering approaches, we develop a tracking framework based on a sliding-window method that merges spatially overlapped and temporally continuous fire patches. This approach maintains the continuity of long-duration events and reduces artificial segmentation, as demonstrated by validation against ground-based and higher-resolution satellite benchmarks. Our dataset provides a range of event-level metrics, including ignition location, fire duration, daily expansion rates, burned area, and fire radiative power. This fire event inventory offers an observational foundation for tracking extreme fire behaviour, calibrating fire spread models, and refining global emissions estimates.]]></dc:description>
      <dc:date>2026-08-12</dc:date>
      <dc:type>Text</dc:type>
      <dc:format>application/pdf</dc:format>
      <dc:identifier>https://doi.org/10.5194/essd-2026-387</dc:identifier>
      <dc:identifier><![CDATA[https://essd.copernicus.org/preprints/essd-2026-387/]]></dc:identifier>
      <dc:source>eISSN: 1866-3516</dc:source>
      <dc:language>eng</dc:language>
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