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        <title>ACP - recent papers</title>


    <link rel="self" href="https://acp.copernicus.org/articles/"/>
    <id>https://acp.copernicus.org/articles/</id>
    <updated>2026-06-05T09:51:32+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7895-2026</id>
            <title type="html">Comparing secondary organic aerosols schemes implemented in current chemical transport models and the policy implications of uncertainties
            </title>
            <link href="https://doi.org/10.5194/acp-26-7895-2026"/>
            <summary type="html">
                &lt;b&gt;Comparing secondary organic aerosols schemes implemented in current chemical transport models and the policy implications of uncertainties&lt;/b&gt;&lt;br&gt;
                Ling Huang, Benjie Chen, Zi'ang Wu, Katie Tuite, Pradeepa Vennam, Greg Yarwood, and Li Li&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7895&#8211;7915, https://doi.org/10.5194/acp-26-7895-2026, 2026&lt;br&gt;
                Secondary organic aerosol (SOA) constitutes a major component of atmospheric aerosol that models must account for to assess how human activities influence air quality, climate, and public health. We find substantial differences in how current air quality models represent SOA highlighting a lack of consensus within the modelling community. Our findings emphasize the need to recognize the limitations of current SOA schemes in the context of air quality management and policy development.
            </summary>
            <content type="html">
                &lt;b&gt;Comparing secondary organic aerosols schemes implemented in current chemical transport models and the policy implications of uncertainties&lt;/b&gt;&lt;br&gt;
                Ling Huang, Benjie Chen, Zi'ang Wu, Katie Tuite, Pradeepa Vennam, Greg Yarwood, and Li Li&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7895&#8211;7915, https://doi.org/10.5194/acp-26-7895-2026, 2026&lt;br&gt;
                <p>Secondary organic aerosol (SOA) constitutes a major component of fine particulate matter (PM<span class="inline-formula"><sub>2.5</sub></span>) that models must account for to assess how human activities influence air quality, climate, and public health. We characterize the current state of SOA modeling by analyzing eight SOA schemes implemented in five widely used air quality models: CAMx, CMAQ, GEOS-Chem, WRF-Chem and CHIMERE. We performed offline calculations to compare non-aged SOA yields, the effects of SOA aging processes, and the influence of NO<span class="inline-formula"><sub><i>x</i></sub></span&gt; conditions on yields. Our objective is to understand variation rather than to identify a superior scheme. We find significant discrepancies in SOA yields with the ratio of maximum to minimum non-aged yield spans from 1.8 to over 1000, depending upon precursor. The impact of nitrogen oxide (NO<span class="inline-formula"><sub><i>x</i></sub></span>) conditions on SOA yields is also highly variable among schemes. While some schemes include SOA aging, their treatments differ substantially, with some schemes showing large increases in SOA mass, while others exhibit minimal changes. Box model simulations confirmed the substantial discrepancies in predicted SOA concentrations and their responses to precursor emission changes. The substantial differences among current SOA schemes highlight a lack of consensus within the air quality modelling community. Evaluating model simulation results using ambient measurements is unlikely to resolve these discrepancies because uncertainties in SOA formation and precursor emissions are deeply intertwined. The limitations of current SOA schemes should be recognized and acknowledged because model choice can greatly influence predicted SOA concentrations and their evolution, ultimately impacting air quality forecasts, assessments, and regulatory decisions.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-05T09:51:32+02:00</published>
            <updated>2026-06-05T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7867-2026</id>
            <title type="html">Impacts of lake on diurnal evolution of surface PM<sub>2.5</sub> concentrations around a typical megacity of China
            </title>
            <link href="https://doi.org/10.5194/acp-26-7867-2026"/>
            <summary type="html">
                &lt;b&gt;Impacts of lake on diurnal evolution of surface PM2.5 concentrations around a typical megacity of China&lt;/b&gt;&lt;br&gt;
                Zining Yang, Qike Yang, Chun Zhao, Zihan Xia, Qiuyan Du, Gudongze Li, Mingyue Xu, Zhiyuan Hu, Renmin Yuan, Jiawang Feng, Jun Gu, and Yubin Li&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7867&#8211;7894, https://doi.org/10.5194/acp-26-7867-2026, 2026&lt;br&gt;
                This study uses 1 km resolution Weather Research and Forecasting model coupled with&amp;#160;<br />Chemistry (WRF-Chem) simulations to investigate how Lake Chaohu affects fine&amp;#160;<br />particulate matter (PM<sub>2.5</sub>) in Hefei. The lake shows a diurnal reversal, increasing&amp;#160;<br />daytime pollution by secondary aerosol formation and storage zones with suppressed&amp;#160;<br />mixing and low deposition, while purifying urban air at night through enhanced vertical&amp;#160;<br />mixing. Lake emission treatment affects lake-urban air quality assessments.
            </summary>
            <content type="html">
                &lt;b&gt;Impacts of lake on diurnal evolution of surface PM2.5 concentrations around a typical megacity of China&lt;/b&gt;&lt;br&gt;
                Zining Yang, Qike Yang, Chun Zhao, Zihan Xia, Qiuyan Du, Gudongze Li, Mingyue Xu, Zhiyuan Hu, Renmin Yuan, Jiawang Feng, Jun Gu, and Yubin Li&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7867&#8211;7894, https://doi.org/10.5194/acp-26-7867-2026, 2026&lt;br&gt;
                <p>Lake-land thermal contrasts significantly modulate regional air quality, yet the coupling mechanisms by which inland lakes regulate the diurnal evolution of PM<span class="inline-formula"><sub>2.5</sub></span&gt; and its components remain poorly understood. This study conducts high-resolution (1&amp;#8201;km) WRF-Chem simulations over Lake Chaohu and the adjacent megacity of Hefei, China, during spring to elucidate these interactions. Results reveal a distinct diurnal reversal effect. During daytime, the lake presence facilitates PM<span class="inline-formula"><sub>2.5</sub></span&gt; increases of predominantly 0&amp;#8211;10&amp;#8201;<span class="inline-formula">&amp;#181;g</span>&amp;#8201;m<span class="inline-formula"><sup>&amp;#8722;3</sup></span&gt; both over the lake and in surrounding urban areas by suppressed planetary boundary layer height, weakened vertical mixing, and reduced dry deposition velocities, which collectively transform the lake into &amp;#8220;storage zone&amp;#8221; that prolongs PM<span class="inline-formula"><sub>2.5</sub></span&gt; lifetimes. This accumulation is dominated by secondary PM<span class="inline-formula"><sub>2.5</sub></span>, as the cooler and more humid lake air thermodynamically favors the ammonium nitrate formation. Furthermore, convergence zones where lake breezes meet background winds create localized stagnation traps that intensify shoreline pollution. At night, while the lake surface maintains higher PM<span class="inline-formula"><sub>2.5</sub></span&gt; concentrations than surrounding land, its impact on the city reverses, exerting a purification effect with urban PM<span class="inline-formula"><sub>2.5</sub></span&gt; decreasing by predominantly 0&amp;#8211;10&amp;#8201;<span class="inline-formula">&amp;#181;g</span>&amp;#8201;m<span class="inline-formula"><sup>&amp;#8722;3</sup></span&gt; as land-breeze circulation enhances vertical mixing and facilitates primary pollutant dispersion. Sensitivity experiments reveal that failing to distinguish lake surfaces in emission inventories can significantly amplify daytime pollution. These findings emphasize that lakes act as complex dual regulators of urban air quality, with identified mechanisms likely applicable to other urban-lake systems globally. This study highlights the necessity of high-resolution meteorological modeling and precise surface characterization for improved air quality forecasting in lake-adjacent megacities regions.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-05T09:51:32+02:00</published>
            <updated>2026-06-05T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7827-2026</id>
            <title type="html">Synchronization of source and sink by boundary  layer evolution: a key to new particle formation  under varying ozone pollution
            </title>
            <link href="https://doi.org/10.5194/acp-26-7827-2026"/>
            <summary type="html">
                &lt;b&gt;Synchronization of source and sink by boundary  layer evolution: a key to new particle formation  under varying ozone pollution&lt;/b&gt;&lt;br&gt;
                Yulin Wang, Deyu Liu, Honglei Wang, Shuangshuang Shi, Qun Hu, Zihan Wang, Zirui Liu, Tianliang Zhao, and Lijuan Shen&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7827&#8211;7842, https://doi.org/10.5194/acp-26-7827-2026, 2026&lt;br&gt;
                Atmospheric new particles formation plays an important role in air quality and climate change, but it does not always appear even in the similar situation. Using ground measurements and vertical observations, we found this process occurs only when the source increases while the sink weakens at the same time, which is mainly controlled by the development of the boundary layer. The finding helps us better understand particle formation in complex atmospheric environments.
            </summary>
            <content type="html">
                &lt;b&gt;Synchronization of source and sink by boundary  layer evolution: a key to new particle formation  under varying ozone pollution&lt;/b&gt;&lt;br&gt;
                Yulin Wang, Deyu Liu, Honglei Wang, Shuangshuang Shi, Qun Hu, Zihan Wang, Zirui Liu, Tianliang Zhao, and Lijuan Shen&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7827&#8211;7842, https://doi.org/10.5194/acp-26-7827-2026, 2026&lt;br&gt;
                <p>Atmospheric new particle formation (NPF) is a vital source of aerosol and cloud condensation nuclei, regulated by complex meteorological and chemical factors. Utilizing ground aerosol particle size distributions and vertical observations, this study employs a generalized additive model (GAM) and SHapley Additive exPlanations (SHAP) to quantitatively assess the marginal contributions of factors driving NPF under the NPF scenario and three non-NPF scenarios. We found that NPF depends on the synchronization of enhanced source strength and weakened sink intensity, a process controlled by planetary boundary layer evolution. Under the NPF scenario, the breakup of the inversion layer and entrainment of cleaner air aloft promote vertical mixing. This rapidly reduces the condensation sink (CS) while transporting ozone (<span class="inline-formula">O<sub>3</sub></span>) to the surface, allowing precursor formation to coincide with a clean background, thus creating a favorable nucleation window. In contrast, nucleation is inhibited in non-NPF scenarios through distinct mechanisms: insufficient oxidation capacity (Non-<span class="inline-formula">O<sub>3</sub></span&gt; scenario), source&amp;#8211;sink desynchronization caused by stable stratification suppressing vertical exchange (Low-<span class="inline-formula">O<sub>3</sub></span&gt; scenario), or rapid scavenging by high background particles (High-<span class="inline-formula">O<sub>3</sub></span&gt; scenario). Correlation analysis and SHAP method corroborate the source&amp;#8211;sink competition mechanism. Under the NPF scenario, nucleation (Nuc) mode significantly correlates with <span class="inline-formula">SO<sub>2</sub></span>, with high temperature and sufficient precursors contributing positively to its predicted value. However, predicted Nuc values are dominated by background particles under the Low-<span class="inline-formula">O<sub>3</sub></span&gt; scenario and negatively influenced by <span class="inline-formula"><i>T</i></span&gt; and <span class="inline-formula">SO<sub>2</sub></span&gt; under the Non-<span class="inline-formula">O<sub>3</sub></span&gt; scenario, while under the High-<span class="inline-formula">O<sub>3</sub></span&gt; scenario, pre-existing aerosols effectively offset precursor contributions.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-04T09:51:32+02:00</published>
            <updated>2026-06-04T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7843-2026</id>
            <title type="html">Long-term study of gravity wave potential energy and OH airglow emissions from 22 years of TIMED/SABER observations
            </title>
            <link href="https://doi.org/10.5194/acp-26-7843-2026"/>
            <summary type="html">
                &lt;b&gt;Long-term study of gravity wave potential energy and OH airglow emissions from 22 years of TIMED/SABER observations&lt;/b&gt;&lt;br&gt;
                Toyese Tunde Ayorinde, Cristiano Max Wrasse, Luiz Fillip Rodrigues Vital, Anderson Vestena Bilibio, Gabriel Augusto Giongo, Hisao Takahashi, Cosme Alexandre Oliveira Barros Figueiredo, Maryam Akinsola, and Peter Taiwo Muka&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7843&#8211;7866, https://doi.org/10.5194/acp-26-7843-2026, 2026&lt;br&gt;
                We analyzed 22 years of satellite observations to see how small-scale atmospheric waves and the OH emissions change across seasons and regions. Both show clear repeating patterns and are closely linked, revealing how energy moves through the upper atmosphere. These results provide a long-term baseline that can improve computer models used to study weather, climate, and atmospheric change.
            </summary>
            <content type="html">
                &lt;b&gt;Long-term study of gravity wave potential energy and OH airglow emissions from 22 years of TIMED/SABER observations&lt;/b&gt;&lt;br&gt;
                Toyese Tunde Ayorinde, Cristiano Max Wrasse, Luiz Fillip Rodrigues Vital, Anderson Vestena Bilibio, Gabriel Augusto Giongo, Hisao Takahashi, Cosme Alexandre Oliveira Barros Figueiredo, Maryam Akinsola, and Peter Taiwo Muka&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7843&#8211;7866, https://doi.org/10.5194/acp-26-7843-2026, 2026&lt;br&gt;
                <p>Using 22 years (2002&amp;#8211;2023) of TIMED/SABER satellite observations, we investigate the long-term coupling between mesospheric hydroxyl (OH) airglow and gravity wave potential energy (<span class="inline-formula"><i>E</i><sub>p</sub></span>). Continuous wavelet transform analysis extracts gravity wave signatures from temperature perturbations, and multiple linear regression decomposes the observed variability into contributions from solar activity, geomagnetic activity, the Quasi-Biennial Oscillation (QBO), and El Ni&amp;#241;o&amp;#8211;Southern Oscillation (ENSO). Three major findings emerge. First, OH emissions and gravity wave <span class="inline-formula"><i>E</i><sub>p</sub></span&gt; are positively coupled, with statistically significant (<span class="inline-formula"><i>p</i><0.05</span>) correlation coefficients of 0.3&amp;#8211;0.7 that peak during winter at mid-latitudes. Second, long-term trends reveal contrasting latitudinal patterns: OH trends are negative at mid-latitudes in both hemispheres (<span class="inline-formula">&amp;#8722;1</span&gt; to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">5</mn><mo>&amp;#215;</mo><msup><mn mathvariant="normal">10</mn><mrow><mo>-</mo><mn mathvariant="normal">10</mn></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="54pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="748b0574ce8219979e520161be590499"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7843-2026-ie00001.svg" width="54pt" height="14pt" src="acp-26-7843-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;W&amp;#8201;m<span class="inline-formula"><sup>&amp;#8722;3</sup></span>&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span>), consistent with mesospheric cooling, whereas <span class="inline-formula"><i>E</i><sub>p</sub></span&gt; trends are positive at mid-latitudes (up to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">5.3</mn><mo>&amp;#215;</mo><msup><mn mathvariant="normal">10</mn><mrow><mo>-</mo><mn mathvariant="normal">2</mn></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="51pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="08bca641a19c3508f7c13b9e9bd4a5f2"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7843-2026-ie00002.svg" width="51pt" height="14pt" src="acp-26-7843-2026-ie00002.png"/></svg:svg></span></span>&amp;#8201;J&amp;#8201;kg<span class="inline-formula"><sup>&amp;#8722;1</sup></span>&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span>), exceeding current model predictions. Both quantities show weaker trends near the equator. Third, a novel decomposition methodology separates temperature-driven chemical responses from non-thermal dynamical effects, revealing that solar forcing operates primarily through thermal mechanisms and accounts for 10&amp;#8201;%&amp;#8211;15&amp;#8201;% of OH variance, while QBO and ENSO influence mesospheric chemistry through dynamical pathways. ENSO drives negative OH responses yet enhances <span class="inline-formula"><i>E</i><sub>p</sub></span>, and QBO responses exhibit opposite patterns between the equator and mid-latitudes. Semi-annual oscillations dominate equatorial variability, while annual oscillations prevail at Southern Hemisphere mid-latitudes.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-04T09:51:32+02:00</published>
            <updated>2026-06-04T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7803-2026</id>
            <title type="html">Geostationary observations of atmospheric ammonia over East Asia: spatio-temporal variations revealed  by three years of FY-4B/GIIRS measurements
            </title>
            <link href="https://doi.org/10.5194/acp-26-7803-2026"/>
            <summary type="html">
                &lt;b&gt;Geostationary observations of atmospheric ammonia over East Asia: spatio-temporal variations revealed  by three years of FY-4B/GIIRS measurements&lt;/b&gt;&lt;br&gt;
                Mengya Sheng, Runyi Zhou, Jiancong Hua, Shan Han, Shangyi Liu, Lin Zhang, Wei Wang, Ruijun Dang, Hansen Cao, Zichong Chen, Yixuan Gu, Mingxu Liu, Lu Lee, Chengli Qi, Feng Lu, Changpei Han, Mark W. Shephard, Nadir Guendouz, Camille Viatte, Lieven Clarisse, Martin Van Damme, Cathy Clerbaux, and Zhao-Cheng Zeng&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7803&#8211;7826, https://doi.org/10.5194/acp-26-7803-2026, 2026&lt;br&gt;
                Geostationary observations of NH<sub>3</sub&gt; provide an unprecedented opportunity to monitor spatial and temporal variations in emissions and their evolution throughout the day. Using 3 years of observations from FY-4B/GIIRS over East Asia, we demonstrated the enhanced capability of geostationary observations to identify emission sources and capture daytime variations associated with agricultural activities. This shows the potential of future geostationary satellites for monitoring air quality globally.
            </summary>
            <content type="html">
                &lt;b&gt;Geostationary observations of atmospheric ammonia over East Asia: spatio-temporal variations revealed  by three years of FY-4B/GIIRS measurements&lt;/b&gt;&lt;br&gt;
                Mengya Sheng, Runyi Zhou, Jiancong Hua, Shan Han, Shangyi Liu, Lin Zhang, Wei Wang, Ruijun Dang, Hansen Cao, Zichong Chen, Yixuan Gu, Mingxu Liu, Lu Lee, Chengli Qi, Feng Lu, Changpei Han, Mark W. Shephard, Nadir Guendouz, Camille Viatte, Lieven Clarisse, Martin Van Damme, Cathy Clerbaux, and Zhao-Cheng Zeng&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7803&#8211;7826, https://doi.org/10.5194/acp-26-7803-2026, 2026&lt;br&gt;
                <p>Satellite observations play a crucial role in quantifying ammonia sources by capturing large-scale variations of atmospheric <span class="inline-formula">NH<sub>3</sub></span&gt; concentrations. As the world's first geostationary hyperspectral infrared sounder, the Geostationary Interferometric Infrared Sounder (GIIRS) on board China's FengYun-4 satellite series provides a unique opportunity to monitor the diurnal cycle of <span class="inline-formula">NH<sub>3</sub></span>. Using <span class="inline-formula">NH<sub>3</sub></span&gt; retrievals from July 2022 to June 2025, this study investigates the spatio-temporal variability of <span class="inline-formula">NH<sub>3</sub></span&gt; columns over East Asia, with a focus on daytime variations (07:00&amp;#8211;19:00&amp;#8201;LT &amp;#8211; local time) in major agricultural regions. Inter-comparison with polar-orbiting IASI and CrIS data shows that GIIRS <span class="inline-formula">NH<sub>3</sub></span&gt; retrievals are consistent in capturing spatial patterns and temporal dynamics. The <span class="inline-formula">NH<sub>3</sub></span&gt; peaks occur between March and July, with peak timing earlier in the south and later in the north, reflecting regional differences primarily driven by agricultural activities. Validation with ground-based FTIR measurements at Hefei in eastern China demonstrates the accuracy of GIIRS <span class="inline-formula">NH<sub>3</sub></span>, with a correlation coefficient of 0.77 and an RMSE of <span class="inline-formula">9.67&amp;#215;10<sup>15</sup></span>&amp;#8201;<span class="inline-formula">molec&amp;#8201;cm<sup>&amp;#8722;2</sup></span>, while reproducing daytime variations observed by FTIR. For major agricultural areas, the <span class="inline-formula">NH<sub>3</sub></span&gt; columns generally increase from early morning to late afternoon,<span id="page7804"/&gt; reaching 1.10&amp;#8211;1.56 times morning levels in summer and spring. Compared with GEOS-CF model simulations, the results reveal pronounced discrepancies in spatial distributions over the Sichuan Basin in southwestern China and daytime variations over northern India. These findings highlight the valuable capability of FY-4B/GIIRS in identifying and tracking daytime dynamics of <span class="inline-formula">NH<sub>3</sub></span&gt; sources over East Asia, offering new insights beyond current low-Earth orbit (LEO) instruments.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-03T09:51:32+02:00</published>
            <updated>2026-06-03T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7789-2026</id>
            <title type="html">Quantifying meteorological impacts on local landfill methane emissions by using field measurements  and machine learning
            </title>
            <link href="https://doi.org/10.5194/acp-26-7789-2026"/>
            <summary type="html">
                &lt;b&gt;Quantifying meteorological impacts on local landfill methane emissions by using field measurements  and machine learning&lt;/b&gt;&lt;br&gt;
                Donghee Kim, Sujong Jeong, Dong Yeong Chang, and Jaewon Joo&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7789&#8211;7802, https://doi.org/10.5194/acp-26-7789-2026, 2026&lt;br&gt;
                This study uses data and machine learning to better estimate methane emissions from a major landfill in South Korea. By considering local weather conditions like temperature and rain, the research improves how landfill methane is tracked over time. The results help us understand how climate affects emissions and provide tools that can be used worldwide to improve greenhouse gas monitoring and climate action planning.
            </summary>
            <content type="html">
                &lt;b&gt;Quantifying meteorological impacts on local landfill methane emissions by using field measurements  and machine learning&lt;/b&gt;&lt;br&gt;
                Donghee Kim, Sujong Jeong, Dong Yeong Chang, and Jaewon Joo&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7789&#8211;7802, https://doi.org/10.5194/acp-26-7789-2026, 2026&lt;br&gt;
                <p>Landfills are a major anthropogenic source of methane (CH<span class="inline-formula"><sub>4</sub></span>), contributing up to 20&amp;#8201;% of global CH<span class="inline-formula"><sub>4</sub></span&gt; emissions. Although CH<span class="inline-formula"><sub>4</sub></span&gt; emissions from landfills are highly sensitive to meteorological conditions, their response to climate variations remains not fully understood, leading to substantial uncertainty in emission projections under climate change. This study evaluated the impact of meteorological factors on landfill CH<span class="inline-formula"><sub>4</sub></span&gt; generation, using a site-specific machine-learning-based model optimized for temperature and precipitation. The model optimized for meteorological conditions performed better than conventional models such as LandGEM and the IPCC model, with a root mean squared error (RMSE) of 6.57&amp;#8201;million&amp;#8201;m<span class="inline-formula"><sup>3</sup></span&gt; CH<span class="inline-formula"><sub>4</sub></span>, a mean absolute error (MAE) of 4.91&amp;#8201;million&amp;#8201;m<span class="inline-formula"><sup>3</sup></span&gt; CH<span class="inline-formula"><sub>4</sub></span>, and Pearson correlation coefficients of 0.89, when compared with field measurements. Sensitivity analysis and OLS regression showed that simulated CH<span class="inline-formula"><sub>4</sub></span&gt; generation had strong positive association with temperature (0.8&amp;#8211;1.0&amp;#8201;% per 1&amp;#8201;&amp;#176;C, <span class="inline-formula"><i>p</i><0.001</span>), while precipitation exhibited inverted-U response, peaking at intermediate levels (9&amp;#8211;10&amp;#8201;mm&amp;#8201;d<span class="inline-formula"><sup>&amp;#8722;1</sup></span>, <span class="inline-formula"><i>p</i><0.01</span>). Quantification of the contributions of the meteorological variables, revealed that temperature accounted for 5.96&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;3.06&amp;#8201;%, and precipitation for 7.38&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.58&amp;#8201;% of the total modeled CH<span class="inline-formula"><sub>4</sub></span&gt; generation. These results highlight the high importance of incorporating meteorological variability into landfill CH<span class="inline-formula"><sub>4</sub></span&gt; estimation to improve predictive accuracy, and emphasize the need for stronger and faster CH<span class="inline-formula"><sub>4</sub></span&gt; mitigation efforts under climate change.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-02T09:51:32+02:00</published>
            <updated>2026-06-02T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7765-2026</id>
            <title type="html">Distinct dual-isotopic signatures of major methane sources in South Asia
            </title>
            <link href="https://doi.org/10.5194/acp-26-7765-2026"/>
            <summary type="html">
                &lt;b&gt;Distinct dual-isotopic signatures of major methane sources in South Asia&lt;/b&gt;&lt;br&gt;
                Peng Yao, Katja Belec, Henry Holmstrand, Josh Balacky, Abdus Salam, Krishnakant Budhavant, Mohanan Remani Manoj, Khaled Shaifullah Joy, Md. Alamin Hossain, Atinderpal Singh, Anil Patel, Neeraj Rastogi, Chinmay Mallik, Kirpa Ram, Gyanesh Kumar Singh, and Örjan Gustafsson&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7765&#8211;7787, https://doi.org/10.5194/acp-26-7765-2026, 2026&lt;br&gt;
                Methane is a powerful greenhouse gas, but its sources remain uncertain in many regions. The isotope fingerprints of methane are diagnostic of its sources, yet their source end-members are poorly constrained for South Asia. Here we determined the methane isotope signal for major sources in South Asia and found these to differ from global averages. Improved regional-specific isotope source fingerprints will help to improve top-down assessments of methane budgets and climate mitigation strategies.
            </summary>
            <content type="html">
                &lt;b&gt;Distinct dual-isotopic signatures of major methane sources in South Asia&lt;/b&gt;&lt;br&gt;
                Peng Yao, Katja Belec, Henry Holmstrand, Josh Balacky, Abdus Salam, Krishnakant Budhavant, Mohanan Remani Manoj, Khaled Shaifullah Joy, Md. Alamin Hossain, Atinderpal Singh, Anil Patel, Neeraj Rastogi, Chinmay Mallik, Kirpa Ram, Gyanesh Kumar Singh, and Örjan Gustafsson&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7765&#8211;7787, https://doi.org/10.5194/acp-26-7765-2026, 2026&lt;br&gt;
                <p>Methane is a powerful greenhouse gas contributing significantly to global warming. South Asia is a major methane emission region, yet source-diagnostic isotopic signatures remain poorly constrained, limiting top-down source attribution. To address this gap, we conducted extensive sampling and isotopic analyses of major methane sources in South Asia. Our results reveal substantial deviations of South Asian methane source fingerprints from global means. Methane from C3 biomass burning is more depleted in <span class="inline-formula"><i>&amp;#948;</i><sup>13</sup>C</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">30.9</mn><mo>&amp;#177;</mo><mn mathvariant="normal">2.2</mn><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="9975e63315cf8c29337152691bfdb948"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00001.svg" width="70pt" height="10pt" src="acp-26-7765-2026-ie00001.png"/></svg:svg></span></span>) but more enriched in <span class="inline-formula"><i>&amp;#948;</i><sup>2</sup>H</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">201</mn><mo>&amp;#177;</mo><mn mathvariant="normal">18</mn><mspace linebreak="nobreak" width="0.125em"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="64pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="f18fb8c54e3cfeadc1633f8f8ac5bc49"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00002.svg" width="64pt" height="10pt" src="acp-26-7765-2026-ie00002.png"/></svg:svg></span></span>) relative to global means, while ruminant methane (C3) is strongly depleted in both <span class="inline-formula"><i>&amp;#948;</i><sup>13</sup>C</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">68.7</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.5</mn><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="299581d8b5f74b48dd4ed2aaa0acaa25"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00003.svg" width="70pt" height="10pt" src="acp-26-7765-2026-ie00003.png"/></svg:svg></span></span>) and <span class="inline-formula"><i>&amp;#948;</i><sup>2</sup>H</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">343</mn><mo>&amp;#177;</mo><mn mathvariant="normal">6</mn><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="58pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="44edd5e02f047587d08138aed4d032bf"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00004.svg" width="58pt" height="10pt" src="acp-26-7765-2026-ie00004.png"/></svg:svg></span></span>). In contrast, rice paddy methane is more enriched in <span class="inline-formula"><i>&amp;#948;</i><sup>13</sup>C</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M10" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">53.8</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.8</mn><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="fdeb5ea07a14fac5f8f33375338a8439"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00005.svg" width="70pt" height="10pt" src="acp-26-7765-2026-ie00005.png"/></svg:svg></span></span>) and <span class="inline-formula"><i>&amp;#948;</i><sup>2</sup>H</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M12" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">311</mn><mo>&amp;#177;</mo><mn mathvariant="normal">6</mn><mspace linebreak="nobreak" width="0.125em"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="58pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="e30a619173832ae1af82c96c808360b4"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00006.svg" width="58pt" height="10pt" src="acp-26-7765-2026-ie00006.png"/></svg:svg></span></span>) than global means, with their ratios signaling pre-emission oxidation. Wastewater methane shows enriched <span class="inline-formula"><i>&amp;#948;</i><sup>13</sup>C</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M14" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">45.0</mn><mo>&amp;#177;</mo><mn mathvariant="normal">2.4</mn><mspace linebreak="nobreak" width="0.125em"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="db4778865879109e6afe9718f0a23125"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00007.svg" width="70pt" height="10pt" src="acp-26-7765-2026-ie00007.png"/></svg:svg></span></span>) and depleted <span class="inline-formula"><i>&amp;#948;</i><sup>2</sup>H</span&gt; (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M16" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">350</mn><mo>&amp;#177;</mo><mn mathvariant="normal">10</mn><mspace linebreak="nobreak" width="0.125em"/><mi mathvariant="normal">&amp;#8240;</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="64pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="c264721f295cb8a08bc464a880d6b9d9"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00008.svg" width="64pt" height="10pt" src="acp-26-7765-2026-ie00008.png"/></svg:svg></span></span>) relative to global means, with minimal oxidation or spatial variation. These pronounced regional differences highlight the importance of using regionally constrained source fingerprints in isotope-based source apportionment. A global synthesis further shows that <span class="inline-formula"><i>&amp;#948;</i><sup>13</sup>C</span&gt; signatures of biomass burning and ruminant methane are primarily controlled by C3&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M18" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="62d2c8208bbdf49afb8db19c9f7b6b50"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7765-2026-ie00009.svg" width="8pt" height="14pt" src="acp-26-7765-2026-ie00009.png"/></svg:svg></span></span>&amp;#8201;C4 feedstocks, whereas <span class="inline-formula"><i>&amp;#948;</i><sup>2</sup>H</span&gt; is relatively insensitive to substrate type. Methane from rice paddies and wetlands exhibits strong latitudinal gradients worldwide.  Combining emission inventories with source-specific isotope fingerprints reveals a mismatch with atmospheric methane in South Asia, suggesting an overestimation of rice paddy emissions and/or an underestimation of other microbial sources. These findings demonstrate the utility of top-down dual-isotope constraints to refine regional methane budgets and mitigation strategies.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-02T09:51:32+02:00</published>
            <updated>2026-06-02T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7677-2026</id>
            <title type="html">Multi-model analysis of the impact of water vapor on the radiative forcing of volcanic aerosols after the 2022 Hunga Eruption
            </title>
            <link href="https://doi.org/10.5194/acp-26-7677-2026"/>
            <summary type="html">
                &lt;b&gt;Multi-model analysis of the impact of water vapor on the radiative forcing of volcanic aerosols after the 2022 Hunga Eruption&lt;/b&gt;&lt;br&gt;
                Ilaria Quaglia, Daniele Visioni, Ewa M. Bednarz, Yunqian Zhu, Georgiy Stenchikov, Valentina Aquila, Cheng-Cheng Liu, Graham W. Mann, Yifeng Peng, Takashi Sekiya, Simone Tilmes, Xinyue Wang, Shingo Watanabe, Pengfei Yu, Jun Zhang, Wandi Yu, and Zhihong Zhuo&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7677&#8211;7704, https://doi.org/10.5194/acp-26-7677-2026, 2026&lt;br&gt;
                On January 15, 2022, the Hunga volcano eruption released unprecedented amounts of water vapor into the atmosphere alongside a modest amount of SO<sub>2</sub>. In this work we analyse results from multiple Earth system models. The models agree that the eruption led to small negative radiative forcing from sulfate aerosols and that the contribution from water vapor was minimal. Therefore, the Hunga eruption cannot explain the exceptional surface warming observed in 2023.
            </summary>
            <content type="html">
                &lt;b&gt;Multi-model analysis of the impact of water vapor on the radiative forcing of volcanic aerosols after the 2022 Hunga Eruption&lt;/b&gt;&lt;br&gt;
                Ilaria Quaglia, Daniele Visioni, Ewa M. Bednarz, Yunqian Zhu, Georgiy Stenchikov, Valentina Aquila, Cheng-Cheng Liu, Graham W. Mann, Yifeng Peng, Takashi Sekiya, Simone Tilmes, Xinyue Wang, Shingo Watanabe, Pengfei Yu, Jun Zhang, Wandi Yu, and Zhihong Zhuo&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7677&#8211;7704, https://doi.org/10.5194/acp-26-7677-2026, 2026&lt;br&gt;
                <p>On 15&amp;#160;January 2022, the Hunga volcano eruption released unprecedented amounts of water vapor into the atmosphere alongside a modest amount of <span class="inline-formula">SO<sub>2</sub></span>. In this work we analyse results from multiple Earth system models as part of the Hunga Tonga-Hunga Ha'apai Volcano Impact Model Observation Comparison Project. Our results show a good model agreement over the climatic outcomes of the eruption, overall indicating a significant negative radiative forcing from the Hunga eruption. The multi-model mean of global instantaneous radiative forcing averaged over 2022&amp;#8211;2023 is estimated at <span class="inline-formula">&amp;#8722;</span>0.19&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.06&amp;#8201;<span class="inline-formula">W&amp;#8201;m<sup>&amp;#8722;2</sup></span&gt; at the top-of-atmosphere (TOA), and <span class="inline-formula">&amp;#8722;</span>0.16&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.06&amp;#8201;<span class="inline-formula">W&amp;#8201;m<sup>&amp;#8722;2</sup></span&gt; at the surface. Simulations with free-running meteorology and climatological sea surface temperatures and sea ice yield a global mean TOA forcing of <span class="inline-formula">&amp;#8722;</span>0.14&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.10&amp;#8201;<span class="inline-formula">W&amp;#8201;m<sup>&amp;#8722;2</sup></span&gt; across two models for the first 2&amp;#160;years, decreasing to <span class="inline-formula">&amp;#8722;</span>0.09&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.10&amp;#8201;<span class="inline-formula">W&amp;#8201;m<sup>&amp;#8722;2</sup></span&gt; on average between 2022 and 2027. However, these global values may be underestimated by about 50&amp;#8201;%, considering that recent <span class="inline-formula">SO<sub>2</sub></span&gt; injection retrievals suggest nearly twice the amount than the 0.5&amp;#8201;<span class="inline-formula">Tg</span>-<span class="inline-formula">SO<sub>2</sub></span&gt; used in the protocol. We also find that the contribution from added stratospheric water vapor is minimal and that the injected <span class="inline-formula">SO<sub>2</sub></span&gt; and the resulting formation of stratospheric sulfate dominate the radiative forcing. However, water vapor played a key role in the initial aerosol growth, leading to a stronger negative radiative forcing during the first 6&amp;#160;months after the eruption compared to simulations without water vapor co-injection.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-01T09:51:32+02:00</published>
            <updated>2026-06-01T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7721-2026</id>
            <title type="html">Elevated anthropogenic contributions to trace elements in marine aerosols compared to coastal Qingdao in eastern China
            </title>
            <link href="https://doi.org/10.5194/acp-26-7721-2026"/>
            <summary type="html">
                &lt;b&gt;Elevated anthropogenic contributions to trace elements in marine aerosols compared to coastal Qingdao in eastern China&lt;/b&gt;&lt;br&gt;
                Yuxuan Qi, Wenshuai Li, Wen Qu, Haizhou Zhang, Wenqing Zhu, Jinhui Shi, Daizhou Zhang, Yanjing Zhang, Lifang Sheng, Wencai Wang, Yunhui Zhao, Yuanyuan Ma, Danyang Ren, Guanru Wu, Xinfeng Wang, Xiaohong Yao, and Yang Zhou&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7721&#8211;7740, https://doi.org/10.5194/acp-26-7721-2026, 2026&lt;br&gt;
                To better constrain poorly resolved trace-element sources across the land-sea gradient, we applied a refined source apportionment to PM<sub>2.5</sub&gt; collected in Qingdao and adjacent seas in 2018. It showed that spring Fe, Mn and Cr were mainly dust-derived, although some dust aged and mixed into marine aerosol offshore. In summer, coal combustion enriched marine Zn, Pb, As and Cd, while residual oil combustion increased Fe and Mn, highlighting strong anthropogenic control on marine aerosols.
            </summary>
            <content type="html">
                &lt;b&gt;Elevated anthropogenic contributions to trace elements in marine aerosols compared to coastal Qingdao in eastern China&lt;/b&gt;&lt;br&gt;
                Yuxuan Qi, Wenshuai Li, Wen Qu, Haizhou Zhang, Wenqing Zhu, Jinhui Shi, Daizhou Zhang, Yanjing Zhang, Lifang Sheng, Wencai Wang, Yunhui Zhao, Yuanyuan Ma, Danyang Ren, Guanru Wu, Xinfeng Wang, Xiaohong Yao, and Yang Zhou&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7721&#8211;7740, https://doi.org/10.5194/acp-26-7721-2026, 2026&lt;br&gt;
                <p>Long-range transport of trace elements (TEs) by aerosols plays a critical role in modulating marine biogeochemistry; however, their source contributions and spatial variability across land-sea gradients remain poorly constrained. Here, we conducted a refined source apportionment of TEs (e.g., Fe, Mn, Cr, V, Ni, Cu, Zn, As, Pb and Cd) in PM<span class="inline-formula"><sub>2.5</sub></span&gt; collected in the coastal city of Qingdao (eastern China) and adjacent marine regions (the Bohai Sea and Yellow Sea) during spring and summer 2018, to quantitatively resolve terrestrial vs.&amp;#160;marine source contributions and identify the key processes controlling their spatial patterns. In spring, all TEs exhibited higher concentrations in Qingdao than in marine atmosphere. In contrast, in summer, Zn, Pb, As, and Cd became more enriched over the marine areas than in Qingdao, with coal combustion accounting for 52.5&amp;#8201;%&amp;#8211;78.8&amp;#8201;% of their concentrations, indicating enhanced anthropogenic impact on the marine atmosphere. For traditional crustal TEs (Fe, Mn and Cr), terrestrial dust dominated in spring Qingdao (e.g., Fe: 81.6&amp;#8201;%, 2832.0&amp;#8201;<span class="inline-formula">ng&amp;#8201;m<sup>&amp;#8722;3</sup></span>), where the pure dust contributions declined sharply in spring marine areas (Fe: 25.4&amp;#8201;%, 145.2&amp;#8201;<span class="inline-formula">ng&amp;#8201;m<sup>&amp;#8722;3</sup></span>). However, part of the dust likely underwent aging during transport and was incorporated into the aged marine aerosol factor, which contributed 33.6&amp;#8201;% of Fe, indicating that dust-related influence remained important offshore and that spring marine aerosols experienced substantial mixing among transported dust, marine processing and anthropogenic emissions. In contrast, coal combustion became the dominant source in summer marine aerosols (Fe: 43.2&amp;#8201;%, 82.8&amp;#8201;ng&amp;#8201;m<span class="inline-formula"><sup>&amp;#8722;3</sup></span>), exceeding its contribution in Qingdao (Fe: 14.1&amp;#8201;%, 45.5&amp;#8201;<span class="inline-formula">ng&amp;#8201;m<sup>&amp;#8722;3</sup></span>). Residual oil combustion was identified as the primary source of marine Ni and V (V: 65.7&amp;#8201;% in spring and 79.8&amp;#8201;% in summer) and also made substantial contributions to Fe, Mn, and Cr, particularly in summer marine aerosols (e.g., Fe: 26.1&amp;#8201;%, 50.0&amp;#8201;<span class="inline-formula">ng&amp;#8201;m<sup>&amp;#8722;3</sup></span>). Overall, the refined source apportionment demonstrates that anthropogenic emissions, especially<span id="page7722"/&gt; coal combustion and shipping-related residual oil combustion, play a dominant role in shaping the TE composition of marine aerosols over the Bohai and Yellow Seas, while transported dust and its atmospheric aging remain important for crustal elements.</p&gt;        <p>These results advance our understanding of land-sea interactions in atmospheric TE cycling and provide new constraints for regional air quality and climate models.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-01T09:51:32+02:00</published>
            <updated>2026-06-01T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7741-2026</id>
            <title type="html">Technical note: DACNO<sub>2</sub> &#8211; a multi-constraint deep learning framework for high-resolution 3D NO<sub>2</sub> field estimation
            </title>
            <link href="https://doi.org/10.5194/acp-26-7741-2026"/>
            <summary type="html">
                &lt;b&gt;Technical note: DACNO2 – a multi-constraint deep learning framework for high-resolution 3D NO2 field estimation&lt;/b&gt;&lt;br&gt;
                Wenfu Sun, Frederik Tack, Lieven Clarisse, and Michel Van Roozendael&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7741&#8211;7764, https://doi.org/10.5194/acp-26-7741-2026, 2026&lt;br&gt;
                Accurate maps of nitrogen dioxide pollution at fine scales are essential for assessing air quality and protecting public health. We developed a machine learning model that produces daily high-resolution 3D nitrogen dioxide fields across Western Europe by combining large-scale atmospheric simulations with ground-based measurements. This approach outperforms traditional methods, especially over cities and complex terrain, and can enhance satellite-based air quality monitoring.
            </summary>
            <content type="html">
                &lt;b&gt;Technical note: DACNO2 – a multi-constraint deep learning framework for high-resolution 3D NO2 field estimation&lt;/b&gt;&lt;br&gt;
                Wenfu Sun, Frederik Tack, Lieven Clarisse, and Michel Van Roozendael&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7741&#8211;7764, https://doi.org/10.5194/acp-26-7741-2026, 2026&lt;br&gt;
                <p>High-resolution 3D fields of nitrogen dioxide (NO<span class="inline-formula"><sub>2</sub></span>) are critical for air quality management and satellite retrievals, yet traditional chemistry-transport models (CTMs) face challenges in fine-scale modeling. Machine learning (ML) alternatives often struggle with generalization and transferability, inheriting biases from CTMs or being limited by sparse surface measurements. We present the Deep Atmospheric Chemistry NO<span class="inline-formula"><sub>2</sub></span&gt; model (DACNO<span class="inline-formula"><sub>2</sub></span>), a deep learning model that generates daily 2&amp;#8201;km&amp;#8201;<span class="inline-formula">&amp;#215;</span>&amp;#8201;2&amp;#8201;km 3D NO<span class="inline-formula"><sub>2</sub></span&gt; fields over Western Europe. The model's three-phase multi-constraint training strategy begins by pre-training on European Copernicus Atmosphere Monitoring Service (CAMS) reanalysis data to learn large-scale atmospheric patterns, then fine-tunes with CAMS and in-situ European Environmental Agency (EEA) surface data to correct biases and refine local detail, and completes with an adaptive fine-tuning to capture evolving trends. An evaluation for 2023 shows that DACNO<span class="inline-formula"><sub>2</sub></span&gt; reproduces broad-scale 3D CAMS fields (<span class="inline-formula"><i>R</i><sup>2</sup>=0.90</span>) and improves agreement with independent EEA stations over the CAMS reanalysis (<span class="inline-formula"><i>R</i><sup>2</sup></span&gt; enhanced from 0.61 to 0.66; bias reduced from <span class="inline-formula">&amp;#8722;</span>1.15 to <span class="inline-formula">&amp;#8722;</span>0.38&amp;#8201;<span class="inline-formula">&amp;#181;g</span>&amp;#8201;m<span class="inline-formula"><sup>&amp;#8722;3</sup></span>). The model resolves spatial details and exhibits physically plausible behavior. This hybrid training approach fuses the physical consistency of a process-based model with the real-world surface measurements, overcoming the limitations of using either constraint alone. Applying DACNO<span class="inline-formula"><sub>2</sub></span&gt; a-priori profiles to TROPOMI retrievals increases tropospheric NO<span class="inline-formula"><sub>2</sub></span&gt; columns by 3&amp;#8201;% on average over those using European CAMS profiles, with enhanced contrast between low- and high-NO<span class="inline-formula"><sub>2</sub></span&gt; regions, primarily attributable to improved resolution. These results demonstrate the framework's potential to advance air quality monitoring and satellite remote sensing.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-01T09:51:32+02:00</published>
            <updated>2026-06-01T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7705-2026</id>
            <title type="html">Advancing the quantification of aerosol-cloud interactions with the CALIPSO-CloudSat-Aqua/MODIS record
            </title>
            <link href="https://doi.org/10.5194/acp-26-7705-2026"/>
            <summary type="html">
                &lt;b&gt;Advancing the quantification of aerosol-cloud interactions with the CALIPSO-CloudSat-Aqua/MODIS record&lt;/b&gt;&lt;br&gt;
                Zhujun Li, David Painemal, Yan Feng, and Xiaojian Zheng&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7705&#8211;7720, https://doi.org/10.5194/acp-26-7705-2026, 2026&lt;br&gt;
                This study is the first global assessment of aerosol-cloud interactions (ACI) and cloud adjustments that relies on vertically resolved aerosol retrievals that are vertically matched with the location of the cloud layer. We computed ACI metrics and cloud adjustments over the global ocean by combining retrievals from active and passive satellite sensors and found high sensitivity of clouds to changes in their cloud droplet number concentration due to aerosols.
            </summary>
            <content type="html">
                &lt;b&gt;Advancing the quantification of aerosol-cloud interactions with the CALIPSO-CloudSat-Aqua/MODIS record&lt;/b&gt;&lt;br&gt;
                Zhujun Li, David Painemal, Yan Feng, and Xiaojian Zheng&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7705&#8211;7720, https://doi.org/10.5194/acp-26-7705-2026, 2026&lt;br&gt;
                <p>Aerosol-cloud-precipitation interactions are assessed over the non-polar ocean using more than 11&amp;#160;years of combined Aqua-MODIS, CALIPSO-CALIOP, and CloudSat products. The analysis first shows the benefit of incorporating vertically resolved aerosol extinction coefficient (<span class="inline-formula"><i>&amp;#963;</i><sub>ext</sub></span>) in aerosol-cloud interactions (ACI) assessments, demonstrating that: <span class="inline-formula"><i>&amp;#963;</i><sub>ext</sub></span&gt; vertically collocated with the cloud layer (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi mathvariant="italic">&amp;#963;</mi><mtext>ext</mtext><mtext>CL</mtext></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="134f148df379b0ab0113b3e771b3aefd"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7705-2026-ie00001.svg" width="20pt" height="17pt" src="acp-26-7705-2026-ie00001.png"/></svg:svg></span></span>) correlates best with cloud droplet number concentration (<span class="inline-formula"><i>N</i><sub>d</sub></span>), column-integrated aerosol optical depth (AOD) cannot explain the <span class="inline-formula"><i>N</i><sub>d</sub></span&gt; variability in the extratropics, and the S-shape of the AOD-<span class="inline-formula"><i>N</i><sub>d</sub></span&gt; relationship reported in previous studies is not replicated when using <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi mathvariant="italic">&amp;#963;</mi><mtext>ext</mtext><mtext>CL</mtext></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="9b3f8bac2ed1f645edf5b84d78dbecd1"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7705-2026-ie00002.svg" width="20pt" height="17pt" src="acp-26-7705-2026-ie00002.png"/></svg:svg></span></span&gt; instead of AOD, with a <span class="inline-formula"><i>N</i><sub>d</sub></span>-<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi mathvariant="italic">&amp;#963;</mi><mtext>ext</mtext><mtext>CL</mtext></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="44fc494748f64407c68a2e16c7d8e787"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7705-2026-ie00003.svg" width="20pt" height="17pt" src="acp-26-7705-2026-ie00003.png"/></svg:svg></span></span&gt; linearity more consistent with in-situ studies over the ocean.</p&gt;        <p>ACI metric, estimated as the log-scale regression between CALIOP <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M10" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi mathvariant="italic">&amp;#963;</mi><mtext>ext</mtext><mtext>CL</mtext></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="4a3d120642efcb476cf137985ae12721"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7705-2026-ie00004.svg" width="20pt" height="17pt" src="acp-26-7705-2026-ie00004.png"/></svg:svg></span></span&gt; and MODIS <span class="inline-formula"><i>N</i><sub>d</sub></span&gt; reveals that the eastern Pacific is the region with the strongest ACI, followed by the Southern Ocean. The susceptibility of clouds to changes in their liquid water path (LWP) and frequency of precipitation followed a 2-step calculation by combining the <span class="inline-formula"><i>N</i><sub>d</sub></span>-<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M13" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi mathvariant="italic">&amp;#963;</mi><mtext>ext</mtext><mtext>CL</mtext></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="db8dfbef6fea424438618e000ed78960"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-26-7705-2026-ie00005.svg" width="20pt" height="17pt" src="acp-26-7705-2026-ie00005.png"/></svg:svg></span></span&gt; regression (ACI) with the regression between these macrophysical variables and <span class="inline-formula"><i>N</i><sub>d</sub></span>. LWP susceptibility is negative (LWP decreases with aerosol loading) and statistically significant over the eastern Pacific, eastern Atlantic, and extratropics. In contrast, vast areas of the tropical and subtropical ocean feature negligible changes in LWP with aerosol. Precipitation frequency susceptibility is negative, but the values are only significant over the coastal eastern Pacific and Atlantic. The findings suggest that previous modeling assessments relying on AOD may need to be revisited by taking advantage of the synergy between passive and active sensors.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-01T09:51:32+02:00</published>
            <updated>2026-06-01T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7647-2026</id>
            <title type="html">European HFC emissions evaluated with multiple atmospheric inverse models and UNFCCC national inventories
            </title>
            <link href="https://doi.org/10.5194/acp-26-7647-2026"/>
            <summary type="html">
                &lt;b&gt;European HFC emissions evaluated with multiple atmospheric inverse models and UNFCCC national inventories&lt;/b&gt;&lt;br&gt;
                Hélène De Longueville, Daniela B. Melo, Alison L. Redington, Alice Ramsden, Alexandre Danjou, Peter Andrews, Joseph Pitt, Brendan Murphy, Lionel Constantin, Kieran M. Stanley, Simon O'Doherty, Angelina Wenger, Dickon Young, Andreas Engel, Tanja Schuck, Katharina Meixner, Thomas Wagenhaeuser, Fides Gad, Martin K. Vollmer, Stefan Reimann, Michela Maoine, Jgor Arduini, Chris Lunder, Norbert Schmidtbauer, László Haszpra, Mihály Molnár, Arnoud Frumau, Cedric Couret, Matthew Rigby, Stephan Henne, Alistair Manning, and Anita L. Ganesan&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7647&#8211;7675, https://doi.org/10.5194/acp-26-7647-2026, 2026&lt;br&gt;
                This study estimates emissions of hydrofluorocarbons, potent greenhouse gases, in north-western Europe using atmospheric observations and atmospheric modelling. The estimates are compared with nationally reported emissions submitted to the United Nations. Overall, our results are consistent with reported values, although differences are found for some gases and countries. The findings indicate that emissions in north-western Europe are declining, reflecting the effects of climate regulations.
            </summary>
            <content type="html">
                &lt;b&gt;European HFC emissions evaluated with multiple atmospheric inverse models and UNFCCC national inventories&lt;/b&gt;&lt;br&gt;
                Hélène De Longueville, Daniela B. Melo, Alison L. Redington, Alice Ramsden, Alexandre Danjou, Peter Andrews, Joseph Pitt, Brendan Murphy, Lionel Constantin, Kieran M. Stanley, Simon O'Doherty, Angelina Wenger, Dickon Young, Andreas Engel, Tanja Schuck, Katharina Meixner, Thomas Wagenhaeuser, Fides Gad, Martin K. Vollmer, Stefan Reimann, Michela Maoine, Jgor Arduini, Chris Lunder, Norbert Schmidtbauer, László Haszpra, Mihály Molnár, Arnoud Frumau, Cedric Couret, Matthew Rigby, Stephan Henne, Alistair Manning, and Anita L. Ganesan&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7647&#8211;7675, https://doi.org/10.5194/acp-26-7647-2026, 2026&lt;br&gt;
                <p>Hydrofluorocarbons (HFCs) are potent greenhouse gases widely used in refrigeration, air-conditioning, and heat pump systems. Accurate monitoring of HFC emissions is essential to evaluate compliance with climate regulations and inform mitigation strategies. This study presents trends of HFC emissions across north-western Europe between 2013 and 2024, derived from atmospheric inverse modelling combining atmospheric measurements at eleven monitoring stations with two transport models (NAME and FLEXPART) and three Bayesian inversion systems (InTEM, ELRIS, RHIME). Although global emissions continue to rise for most HFCs, in north-western Europe our results show an overall steady decline in total HFC emissions from 40&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;3&amp;#8201;&amp;#8201;Tg&amp;#8201;CO<span class="inline-formula"><sub>2</sub></span>-eq&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span&gt; in 2016 (prior to enhanced regulation) to 29&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;2&amp;#8201;&amp;#8201;Tg&amp;#8201;CO<span class="inline-formula"><sub>2</sub></span>-eq&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span&gt; in 2023, following EU F-gas Regulations. This reduction is driven primarily by decreasing emissions of HFC-134a, HFC-143a and HFC-125 despite increasing HFC-32 emissions due to its adoption as a lower-global-warming-potential alternative refrigerant. Comparisons with national inventories reported to the United Nations Framework Convention on Climate Change (UNFCCC) show generally good agreement over north-western Europe but reveal discrepancies for specific compounds and countries, particularly for HFC-134a and HFC-125 in France and Germany during the earlier years of the study period. The recent expansion of the European measurement network demonstrates potential to improve spatial coverage and resolution of inverse emission estimates, especially in southern and central Europe. This study highlights the value of multi-model inversions to provide robust emission estimates with realistic, hence actionable, uncertainty characterisation.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-01T09:51:32+02:00</published>
            <updated>2026-06-01T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7555-2026</id>
            <title type="html">Melt period methane emissions in northern high latitude wetlands are governed by the length of the period and presence of permafrost
            </title>
            <link href="https://doi.org/10.5194/acp-26-7555-2026"/>
            <summary type="html">
                &lt;b&gt;Melt period methane emissions in northern high latitude wetlands are governed by the length of the period and presence of permafrost&lt;/b&gt;&lt;br&gt;
                Sara Hyvärinen, Maria K. Tenkanen, Aki Tsuruta, Anttoni Erkkilä, Kimmo Rautiainen, Hermanni Aaltonen, Motoki Sasakawa, and Tuula Aalto&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7555&#8211;7587, https://doi.org/10.5194/acp-26-7555-2026, 2026&lt;br&gt;
                We analyzed melt period methane emissions from northern high-latitude wetlands using satellite thaw data and inverse modeling (2011&amp;#8211;2021). Comparing region-based and grid-based approaches, we found that emissions varied with the length of the melt period, which depended on air temperature. We found spring melt period emissions ranged from 0.45 to 1.83 Tg depending on the approach, with no clear trend over the period. Our methods allow for seasonal methane monitoring across different scales.
            </summary>
            <content type="html">
                &lt;b&gt;Melt period methane emissions in northern high latitude wetlands are governed by the length of the period and presence of permafrost&lt;/b&gt;&lt;br&gt;
                Sara Hyvärinen, Maria K. Tenkanen, Aki Tsuruta, Anttoni Erkkilä, Kimmo Rautiainen, Hermanni Aaltonen, Motoki Sasakawa, and Tuula Aalto&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7555&#8211;7587, https://doi.org/10.5194/acp-26-7555-2026, 2026&lt;br&gt;
                <p>Northern high latitude wetlands are significant sources of methane, with emissions driven by seasonal soil freezing and thawing. To better understand the seasonality of northern high latitude methane emissions, we defined the melt period occurring in spring time using the remote sensing Soil Moisture and Ocean Salinity Freeze/Thaw data from 2011&amp;#8211;2021. To estimate methane emissions in the northern high latitudes, we used the atmospheric inverse model CarbonTracker Europe-<span class="inline-formula">CH<sub>4</sub></span>. The melt period was defined for three permafrost zones and for a seasonally frozen non-permafrost region using two approaches: region-based, which considered climatological conditions of permafrost regions, and grid-based, which defines the melt period at a finer <span class="inline-formula">1<i>&amp;#176;</i>&amp;#215;1<i>&amp;#176;</i></span&gt; scale.</p&gt;        <p>The length and timing of the melt period varied significantly depending on the approach. The melt period generally occurred between March and June and was influenced by air temperature, with a negative correlation between the length and the mean temperature of the melt period. The longest melt period was in the non-permafrost zone and the shortest varied between the two methods. The melt period emissions were on average 1.83&amp;#8201;Tg with the region-based approach and 0.45&amp;#8201;Tg with the grid-based approach, the non-permafrost zone having the largest share of the emissions. They were largely dependent on the season&amp;#8217;s length. Year-to-year variation was modest, within 15&amp;#8201;% (region-based) and 23&amp;#8201;% (grid-based) of average emissions, and there was also no trend during the study period. Our dual-method approach allows for robust comparison with both large-scale regional studies and localized site-level research.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7523-2026</id>
            <title type="html">Atmospheric forcing of dust source activation across East Asia
            </title>
            <link href="https://doi.org/10.5194/acp-26-7523-2026"/>
            <summary type="html">
                &lt;b&gt;Atmospheric forcing of dust source activation across East Asia&lt;/b&gt;&lt;br&gt;
                Lingle Chen, Kerstin Schepanski, Kai Zhang, Anya J. Crocker, Chuang Xuan, and Paul A. Wilson&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7523&#8211;7538, https://doi.org/10.5194/acp-26-7523-2026, 2026&lt;br&gt;
                East Asia is among the most dust-active regions globally, yet the atmospheric processes behind these dust emissions remain poorly understood. Using an hourly dust source activation record across East Asia, we identify two primary regions with distinct diurnal cycles: a northern region driven by low-pressure systems, a southern one linked to low-level jet breakdown and deep convection, and a third minor region on the Tibetan Plateau presumably driven by wintertime mountain-valley winds.
            </summary>
            <content type="html">
                &lt;b&gt;Atmospheric forcing of dust source activation across East Asia&lt;/b&gt;&lt;br&gt;
                Lingle Chen, Kerstin Schepanski, Kai Zhang, Anya J. Crocker, Chuang Xuan, and Paul A. Wilson&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7523&#8211;7538, https://doi.org/10.5194/acp-26-7523-2026, 2026&lt;br&gt;
                <p>East Asian dust storms impact the health and livelihoods of millions but the atmospheric processes responsible are far from fully understood because suitable observations are lacking. Here we analyse dust source activation (DSA) frequency data for East Asia (80&amp;#8211;130&amp;#176;&amp;#8201;E, 27&amp;#8211;52&amp;#176;&amp;#8201;N, January 2016 through December 2023, Chen et al.,&amp;#160;2025, <a href="https://doi.org/10.1088/1748-9326/addee6">https://doi.org/10.1088/1748-9326/addee6</a>) to understand atmospheric controls on dust activation. We show that East Asia's two primary dust source regions (Chen et al.,&amp;#160;2025) display distinct diurnal and seasonal variations in DSA frequency. A southern region, sandwiched between the Mongolian Plateau and the Tibetan Plateau, chiefly consisting of the Taklimakan Desert and the Alashan Plateau, is active year-round, with 40&amp;#8201;%&amp;#8211;60&amp;#8201;% of events predominantly occurring during late morning (09:00&amp;#8211;12:00 local solar time, LST) under clear-sky conditions. We show that breakdown of the Low-level Jet (LLJ) is a major control on dust activation across this region (not only the Taklimakan Desert), driven by morning heating of the land surface, deepening the convective boundary layer and momentum transfer to the land surface. Here, convective activities also contribute to cloud-associated dust source activations during summer afternoon (i.e., haboobs). A northern region, centred on the Mongolian Plateau-Gobi Desert is dust-active from morning to afternoon (08:00&amp;#8211;19:00&amp;#8201;LST), primarily under cloudy conditions, driven by the passage of low-pressure systems. A third (less active) dust source region, the Tibetan Plateau, is typically active during winter afternoons presumably in response to strong mountain-valley winds. Meso- and local-scale winds are more extensive drivers of dust activation across East Asia than previously documented, adding uncertainty to model predictions of future dust emissions in East Asia under a warming climate.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7407-2026</id>
            <title type="html">A modified stratiform cloud microphysics parameterization: evaluation using the Community Atmosphere Model version 6 single-column model
            </title>
            <link href="https://doi.org/10.5194/acp-26-7407-2026"/>
            <summary type="html">
                &lt;b&gt;A modified stratiform cloud microphysics parameterization: evaluation using the Community Atmosphere Model version 6 single-column model&lt;/b&gt;&lt;br&gt;
                Chandra Shekhar Pant, Deepak Waman, Sachin Patade, Akash Deshmukh, Niharika Singh, Vaughan Phillips, and Aaron Bansemer&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7407&#8211;7433, https://doi.org/10.5194/acp-26-7407-2026, 2026&lt;br&gt;
                Large-scale stratiform clouds play a decisive role in the Earth's radiation budget and precipitation patterns, yet global models historically exhibit major biases in their simulations. Our study addresses these gaps by implementing physically-based representations of secondary ice production pathways and advanced aerosol activation schemes, including bin-bulk microphysics. These improvements enable the robust simulation of both cloud droplet and ice formation.
            </summary>
            <content type="html">
                &lt;b&gt;A modified stratiform cloud microphysics parameterization: evaluation using the Community Atmosphere Model version 6 single-column model&lt;/b&gt;&lt;br&gt;
                Chandra Shekhar Pant, Deepak Waman, Sachin Patade, Akash Deshmukh, Niharika Singh, Vaughan Phillips, and Aaron Bansemer&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7407&#8211;7433, https://doi.org/10.5194/acp-26-7407-2026, 2026&lt;br&gt;
                <p>Large-scale stratiform clouds are widespread and dominate the Earth's radiation budget. Their radiative and microphysical properties are inseparable, depending on ambient aerosol conditions and on properties of any convective outflow. In the Community Atmospheric Model, version 6 (CAM6), large-scale clouds were originally treated two decades ago with a two-moment bulk microphysics approach. Since then, the technological and empirical basis of global models has improved, for example by representing cloud microphysics to encompass extra processes of ice and droplet initiation, and by including dependencies on aerosol conditions of size, composition, and loading.</p&gt;        <p>To advance the microphysical realism of the large-scale cloud scheme of the global model CAM6, most of the known mechanisms of secondary ice production (SIP) and an empirical formulation for heterogeneous ice nucleation have been represented in the stratiform scheme of the Global model CAM6. We included a hybrid bin/bulk microphysics scheme that treats aerosol activation, growth processes of accretion, aggregation, and riming, and three SIP mechanisms in the stratiform cloud scheme. We simulated an observed case of a mesoscale convective system during the Mid-latitude Continental Convective Clouds Experiment (MC3E) in Oklahoma, USA, using the Single-Column Atmosphere Model (SCAM6). The results from the simulations are validated against the aircraft, satellite, and ground measurements.</p&gt;        <p>Results show that the modified stratiform scheme can predict the cloud properties of the observed stratiform clouds realistically. Together with our improved convective scheme in CAM6, this paves the way for more realism in the treatment of aerosol-cloud interactions in global climate change by conventional General Circulation Models.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7607-2026</id>
            <title type="html">Stratospheric gravity waves in three high-resolution models and AIRS satellite observations
            </title>
            <link href="https://doi.org/10.5194/acp-26-7607-2026"/>
            <summary type="html">
                &lt;b&gt;Stratospheric gravity waves in three high-resolution models and AIRS satellite observations&lt;/b&gt;&lt;br&gt;
                Phoebe Noble, Haruka Okui, Joan Alexander, Manfred Ern, Neil P. Hindley, Lars Hoffmann, Laura Holt, Annelize van Niekerk, Riwal Plougonven, Inna Polichtchouk, Claudia C. Stephan, Martina Bramberger, Milena Corcos, William Putnam, Christopher Kruse, and Corwin J. Wright&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7607&#8211;7630, https://doi.org/10.5194/acp-26-7607-2026, 2026&lt;br&gt;
                Gravity waves are small-scale processes that drive the circulation in the middle and upper atmosphere. In this work, we assess 3 new high-resolution (3-5km horizontal resolution) models against satellite data. Generally, models capture the spatial patterns and represent stratospheric northern hemisphere mountain generated waves well. However, they still underestimate amplitudes globally and struggle with the representation of southern hemispheric convective waves.
            </summary>
            <content type="html">
                &lt;b&gt;Stratospheric gravity waves in three high-resolution models and AIRS satellite observations&lt;/b&gt;&lt;br&gt;
                Phoebe Noble, Haruka Okui, Joan Alexander, Manfred Ern, Neil P. Hindley, Lars Hoffmann, Laura Holt, Annelize van Niekerk, Riwal Plougonven, Inna Polichtchouk, Claudia C. Stephan, Martina Bramberger, Milena Corcos, William Putnam, Christopher Kruse, and Corwin J. Wright&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7607&#8211;7630, https://doi.org/10.5194/acp-26-7607-2026, 2026&lt;br&gt;
                <p>Advances in computational power and model development have enabled the generation of global high-resolution models. These new models can resolve a large proportion of gravity waves (GWs) explicitly, reducing reliance on subgrid parametrizations. GWs are vital components of the middle and upper atmosphere, they transport energy and momentum both horizontally and vertically, driving the atmospheric circulation. Evaluating the realism of these resolved waves is a crucial step in advancing future model development.</p&gt;        <p>Here we provide the first global multi-model GW observational comparison that accounts for the observational filter. We assess the representation of stratospheric GWs in three high-resolution (3&amp;#8211;5&amp;#8201;<span class="inline-formula">km</span&gt; horizontal resolution) global free-running simulations (ICON, IFS and GEOS), for the period 20&amp;#160;January&amp;#8211;29&amp;#160;February 2020, against AIRS satellite observations.</p&gt;        <p>Time-mean wave amplitudes are systematically lower in the models than observations, consistent with previous studies. GW occurrence rates are higher in all models than the observations, dominated by low amplitude waves in the models. During the first 10&amp;#8201;<span class="inline-formula">d</span&gt; spatial patterns of GW occurrence rate, amplitudes and momentum flux agree across the models and observations but subsequently they diverge. Agreement is more consistent in the Northern Hemisphere (where orographic waves dominate) than in the Southern Hemisphere (where convective waves dominate).</p&gt;        <p>These results benchmark the current state of high-resolution modelling and demonstrate that whilst there are strengths in models' ability to capture the morphology of GWs (particularly orographically generated waves), there is room for improvement in modelling amplitudes, occurrence rates and zonal-mean flux magnitudes globally, with the largest discrepancies in the tropical convective regions.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7435-2026</id>
            <title type="html">Effects of model grid spacing for warm conveyor belt (WCB) moisture transport into the upper troposphere and lower stratosphere (UTLS) &#8211; Part 1: Lagrangian perspective
            </title>
            <link href="https://doi.org/10.5194/acp-26-7435-2026"/>
            <summary type="html">
                &lt;b&gt;Effects of model grid spacing for warm conveyor belt (WCB) moisture transport into the upper troposphere and lower stratosphere (UTLS) – Part 1: Lagrangian perspective&lt;/b&gt;&lt;br&gt;
                Cornelis Schwenk and Annette Miltenberger&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7435&#8211;7462, https://doi.org/10.5194/acp-26-7435-2026, 2026&lt;br&gt;
                We studied how model grid-spacing affects how moisture and ice are carried upward in large weather systems that move warm, moist air into the upper troposphere. By comparing high- and low-resolution simulations, we found that models which are able to represent convectively ascending air produce much drier air at high altitudes. This shows that model resolution strongly influences how water and clouds are transported and how they may affect climate.
            </summary>
            <content type="html">
                &lt;b&gt;Effects of model grid spacing for warm conveyor belt (WCB) moisture transport into the upper troposphere and lower stratosphere (UTLS) – Part 1: Lagrangian perspective&lt;/b&gt;&lt;br&gt;
                Cornelis Schwenk and Annette Miltenberger&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7435&#8211;7462, https://doi.org/10.5194/acp-26-7435-2026, 2026&lt;br&gt;
                <p>Warm conveyor belts (WCBs) in extratropical cyclones transport moisture and hydrometeors into the upper troposphere and lower stratosphere (UTLS), influencing the radiative balance. Earlier research has shown that the horizontal grid spacing of numerical weather prediction (NWP) models has an impact on the modelled WCB properties, such as ascent rates and diabatic heating. This first part of a two-part study examines the impact of model grid spacing on the transport of moisture from a Lagrangian perspective. We analyze two ICON model simulations of one North Atlantic WCB case study: a convection-parameterizing run at <span class="inline-formula">&amp;#8764;</span>&amp;#8201;13&amp;#8201;km and a convection-permitting run at <span class="inline-formula">&amp;#8764;</span>&amp;#8201;3.5&amp;#8201;km approximate grid spacing. We hypothesize that key differences in the modelled transport of moisture arise from higher vertical velocities in the high-resolution simulation. The convection-permitting simulation produces more rapid ascent and a drier WCB outflow with lower specific and relative humidity. We attribute this to higher ice number concentrations, which deplete supersaturation more efficiently. This high-resolution simulation also exhibits more pronounced frozen-phase microphysics, stronger frozen precipitation, notably different hydrometeor mass mixing ratios, number concentrations, and radii than the lower resolution simulation &amp;#8211; indicating that horizontal resolution substantially influences modelled WCB cloud composition. These results demonstrate that weather and climate models using convection-parameterizing resolutions may systematically misrepresent WCB cloud properties and UTLS humidity, with potential consequences for accurately simulating Earth's radiative budget and upper-level flow.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7463-2026</id>
            <title type="html">G6-1.5K-SAI and G6sulfur: changes in impacts and uncertainty depending on stratospheric aerosol  injection strategy in the Geoengineering  Model Intercomparison Project
            </title>
            <link href="https://doi.org/10.5194/acp-26-7463-2026"/>
            <summary type="html">
                &lt;b&gt;G6-1.5K-SAI and G6sulfur: changes in impacts and uncertainty depending on stratospheric aerosol  injection strategy in the Geoengineering  Model Intercomparison Project&lt;/b&gt;&lt;br&gt;
                Walker Raymond Lee, Daniele Visioni, Benjamin Moore Wagman, Christopher Robert Wentland, Ben Kravitz, Shingo Watanabe, Takashi Sekiya, Andy Jones, Jim Haywood, Matthew Henry, and Ewa Monika Bednarz&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7463&#8211;7483, https://doi.org/10.5194/acp-26-7463-2026, 2026&lt;br&gt;
                Stratospheric aerosol injection (SAI) is a proposed method of cooling the planet by introducing reflective particles called aerosols into the middle atmosphere to reflect sunlight back into space. We consider recent simulations of SAI from four different climate models. SAI cools the planet effectively in all four models; we examine the impacts on temperature and precipitation in each model and compare to previous experiments. Our simulations will help inform future research and policy.
            </summary>
            <content type="html">
                &lt;b&gt;G6-1.5K-SAI and G6sulfur: changes in impacts and uncertainty depending on stratospheric aerosol  injection strategy in the Geoengineering  Model Intercomparison Project&lt;/b&gt;&lt;br&gt;
                Walker Raymond Lee, Daniele Visioni, Benjamin Moore Wagman, Christopher Robert Wentland, Ben Kravitz, Shingo Watanabe, Takashi Sekiya, Andy Jones, Jim Haywood, Matthew Henry, and Ewa Monika Bednarz&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7463&#8211;7483, https://doi.org/10.5194/acp-26-7463-2026, 2026&lt;br&gt;
                <p>We report initial results for G6-1.5K-SAI, a climate model experiment proposed by the Geoengineering Model Intercomparison Project (GeoMIP). G6-1.5K-SAI simulates a stratospheric aerosol injection (SAI) to limit global warming to <span class="inline-formula">&amp;#8764;</span>&amp;#8201;1.5&amp;#8201;&amp;#176;C above preindustrial in each model and features several design updates relative to previous GeoMIP experiment G6sulfur, such as hemispherically symmetric subtropical injection (30&amp;#176;&amp;#8201;N and 30&amp;#176;&amp;#8201;S) instead of equatorial injection. Due to differences in climate sensitivity, models disagree on the amount of warming to be offset, and therefore on the total injection required. While they agree strongly on the rate of cooling per unit rate of injection (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;0.1&amp;#8201;&amp;#176;C&amp;#8201;(Tg&amp;#8201;SO<span class="inline-formula"><sub>2</sub></span>&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span>)<span class="inline-formula"><sup>&amp;#8722;1</sup></span>, a similar value to G6sulfur models with interactive SO<span class="inline-formula"><sub>2</sub></span>), similarities in aerosol representation and disagreements in aerosol optical depth (AOD) per rate of unit injection and in rate of cooling per unit AOD mean this agreement may not imply accuracy. In all participating models, SAI cools the land surface more than the ocean and offsets mid- and high-latitude precipitation increases under global warming, but models disagree on the magnitude of residual Arctic amplification and changes to tropical precipitation. Relative to G6sulfur, G6-1.5K-SAI cools the Arctic more strongly, and also decreases precipitation less, especially in the tropics and over land. All in all, while the new G6-1.5K-SAI experiment constitutes an update over the older G6sulfur, due to the differences in scenario across these two experiments, any differences in SAI impacts must be evaluated carefully.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7503-2026</id>
            <title type="html">Evaluation of ozone trends in the mesosphere/lower thermosphere using a new merged dataset of  ozone profiles
            </title>
            <link href="https://doi.org/10.5194/acp-26-7503-2026"/>
            <summary type="html">
                &lt;b&gt;Evaluation of ozone trends in the mesosphere/lower thermosphere using a new merged dataset of  ozone profiles&lt;/b&gt;&lt;br&gt;
                Monika E. Szelag, Viktoria F. Sofieva, Edward Malina, Pekka T. Verronen, Michelle L. Santee, Manuel López-Puertas, Bernd Funke, Gabriele Stiller, Alexandra Laeng, Kaley A. Walker, Patrick E. Sheese, Mark E. Hervig, and Benjamin T. Marshall&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7503&#8211;7522, https://doi.org/10.5194/acp-26-7503-2026, 2026&lt;br&gt;
                We present a new global dataset of ozone profiles in the mesosphere and lower thermosphere, created by combining several satellite measurements covering more than three decades. Our results show that ozone is recovering in the stratosphere but decreasing in the mesosphere, with the strongest declines near the mesopause. This dataset provides a valuable resource for investigating long-term changes, improving model performance, and addressing an observational gap in the upper atmosphere.
            </summary>
            <content type="html">
                &lt;b&gt;Evaluation of ozone trends in the mesosphere/lower thermosphere using a new merged dataset of  ozone profiles&lt;/b&gt;&lt;br&gt;
                Monika E. Szelag, Viktoria F. Sofieva, Edward Malina, Pekka T. Verronen, Michelle L. Santee, Manuel López-Puertas, Bernd Funke, Gabriele Stiller, Alexandra Laeng, Kaley A. Walker, Patrick E. Sheese, Mark E. Hervig, and Benjamin T. Marshall&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7503&#8211;7522, https://doi.org/10.5194/acp-26-7503-2026, 2026&lt;br&gt;
                <p>In recent years, the need for high-quality long-term mesospheric ozone records has become increasingly evident, as they are essential for understanding chemical, dynamical, and radiative processes in the middle and upper atmosphere and their coupling with the lower layers. Here, we present a new merged dataset of ozone profiles in the middle atmosphere (METEOR-O3), created from several limb-viewing satellite instruments: HALOE, GOMOS, MIPAS, ACE-FTS, MLS, and SOFIE. The merged dataset covers the period from 1991 to 2023 and provides deseasonalized ozone anomalies in 10&amp;#176;&amp;#8201;latitude bins between 80&amp;#176;&amp;#8201;S and 80&amp;#176;&amp;#8201;N, from approximately 22  to 100&amp;#8201;km. The deseasonalized ozone anomalies are used for global and seasonal trend analysis. The results show positive upper stratospheric ozone trends in both hemispheres, with magnitudes of 1&amp;#8201;%&amp;#8211;2&amp;#8201;% per decade between 35 and 45&amp;#8201;km, indicating continued ozone recovery consistent with previous assessments. In contrast, mesospheric ozone (above <span class="inline-formula">&amp;#8764;</span>&amp;#8201;60&amp;#8201;km) exhibits negative trends of <span class="inline-formula">&amp;#8722;</span>1&amp;#8201;% to <span class="inline-formula">&amp;#8722;</span>3&amp;#8201;% per decade, with the strongest decreases of about <span class="inline-formula">&amp;#8722;</span>8&amp;#8201;% to <span class="inline-formula">&amp;#8722;</span>12&amp;#8201;% per decade between 80 and 90&amp;#8201;km. Seasonal analyses confirm positive trends in the upper stratosphere across all seasons and persistent negative trends in the upper mesosphere, strongest at high latitudes above 80&amp;#8201;km. The METEOR-O3 dataset provides the first global, long-term merged record suitable for detailed studies of mesospheric/lower thermospheric ozone variability and trend evaluation, providing valuable information for model validation and assessments of upper atmospheric changes.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/acp-26-7589-2026</id>
            <title type="html">Efficacy assessment of stratospheric aerosol scrubbing as a counter climate intervention strategy
            </title>
            <link href="https://doi.org/10.5194/acp-26-7589-2026"/>
            <summary type="html">
                &lt;b&gt;Efficacy assessment of stratospheric aerosol scrubbing as a counter climate intervention strategy&lt;/b&gt;&lt;br&gt;
                Anthony C. Jones, James M. Haywood, Matthew Henry, and Alistair Duffey&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7589&#8211;7605, https://doi.org/10.5194/acp-26-7589-2026, 2026&lt;br&gt;
                Injecting aerosol into the stratosphere has been suggested to rapidly cool the planet and counter climate change. Rival actors who oppose deployment may seek to counter stratospheric aerosol injection. Using a climate model, we investigate whether stratospheric aerosol removal could be hastened by injecting coarse aerosol which promote aerosol growth and gravitational settling. We find that this could be effective, reducing aerosol impacts by 30 % in simulations, and warrants further research.
            </summary>
            <content type="html">
                &lt;b&gt;Efficacy assessment of stratospheric aerosol scrubbing as a counter climate intervention strategy&lt;/b&gt;&lt;br&gt;
                Anthony C. Jones, James M. Haywood, Matthew Henry, and Alistair Duffey&lt;br&gt;
                    Atmos. Chem. Phys., 26, 7589&#8211;7605, https://doi.org/10.5194/acp-26-7589-2026, 2026&lt;br&gt;
                <p>Stratospheric Aerosol Injection (SAI) has been proposed to counteract global warming. Countering SAI may prove attractive to actors who oppose deployment and methods have been suggested but not tested for efficacy. Using a global climate model with double moment aerosol microphysics, we investigate the viability of &amp;#8220;Stratospheric Aerosol Scrubbing&amp;#8221; (SAS) scenarios where coarse calcite aerosol is deliberately injected to enhance aerosol growth, reduce particle radiative efficiency, and enhance sedimentation thereby reducing SAI impacts. We simulate two equatorial SAI and SAS scenarios: pulse interventions lasting 2 months, and sustained interventions lasting 20 years. We find that SAS reduces the global Stratospheric Aerosol Optical Depth by 30&amp;#8201;%&amp;#8211;40&amp;#8201;% when the calcite mass is equal to the sulphur dioxide (SO<span class="inline-formula"><sub>2</sub></span>) mass in the pulse intervention and half of the SO<span class="inline-formula"><sub>2</sub></span&gt; mass in the sustained intervention. The global radiative impact in the sustained simulations is reduced from <span class="inline-formula">&amp;#8722;</span>3.3  to <span class="inline-formula">&amp;#8722;</span>2.3&amp;#8201;Wm<span class="inline-formula"><sup>&amp;#8722;2</sup></span&gt; under SAS, a counterbalancing of approximately 30&amp;#8201;%. Our results suggest that SAS could be partially effective at offsetting SAI impacts.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-29T09:51:32+02:00</published>
            <updated>2026-05-29T09:51:32+02:00</updated>
        </entry>
</feed>