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        <title>CP - recent papers</title>


    <link rel="self" href="https://cp.copernicus.org/articles/"/>
    <id>https://cp.copernicus.org/articles/</id>
    <updated>2026-10-16T21:24:52+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1881-2026</id>
            <title type="html">Antarctic sea ice over the past 130&#8201;000 years &#8211; Part 2: A review of its role in the Earth system
            </title>
            <link href="https://doi.org/10.5194/cp-22-1881-2026"/>
            <summary type="html">
                &lt;b&gt;Antarctic sea ice over the past 130 000 years – Part 2: A review of its role in the Earth system&lt;/b&gt;&lt;br&gt;
                Zanna Chase, Karen E. Kohfeld, Amy Leventer, David Lund, Xavier Crosta, Laurie Menviel, Helen C. Bostock, Matthew Chadwick, Samuel L. Jaccard, Jacob Jones, Alice Marzocchi, Katrin J. Meissner, Elisabeth Sikes, Louise C. Sime, and Luke Skinner&lt;br&gt;
                    Clim. Past, 22, 1881&#8211;1911, https://doi.org/10.5194/cp-22-1881-2026, 2026&lt;br&gt;
                The impacts of recent dramatic declines in Antarctic sea ice on the Earth system are uncertain. We reviewed how sea ice affects ocean circulation, ice sheets, winds, and the carbon cycle by considering theory and modern observations alongside paleo-proxy reconstructions. We found evidence of connections between sea ice and these systems, but also conflicting results, pointing to missing knowledge. Our work highlights the complex role of sea ice in the Earth system.
            </summary>
            <content type="html">
                &lt;b&gt;Antarctic sea ice over the past 130 000 years – Part 2: A review of its role in the Earth system&lt;/b&gt;&lt;br&gt;
                Zanna Chase, Karen E. Kohfeld, Amy Leventer, David Lund, Xavier Crosta, Laurie Menviel, Helen C. Bostock, Matthew Chadwick, Samuel L. Jaccard, Jacob Jones, Alice Marzocchi, Katrin J. Meissner, Elisabeth Sikes, Louise C. Sime, and Luke Skinner&lt;br&gt;
                    Clim. Past, 22, 1881&#8211;1911, https://doi.org/10.5194/cp-22-1881-2026, 2026&lt;br&gt;
                <p>Antarctic sea-ice cover reached historically low levels in 2023, consistent with the simulated decline in sea-ice extent in response to anthropogenic warming. As Antarctic sea ice is closely linked to multiple components of the Earth system, its demise could precipitate widespread, cascading changes across the cryosphere, atmosphere, and ocean. However, the nature and strength of these interconnections remain poorly understood and are often inadequately represented in models. In this review, we combine modern observations, models, and paleoclimate archives spanning the last glacial cycle to examine how reductions in sea ice may affect other components of the Earth system. We review how Antarctic sea ice interacts with ocean and atmosphere circulation, ice sheets and ice shelves, marine productivity, and the carbon cycle. We find evidence from theory and models that Antarctic sea ice exerts important influences on the Earth system. Paleo-proxy reconstructions provide examples in which changes in sea ice co-occur with changes in the carbon cycle, marine productivity, and ocean circulation. However, isolating the specific impact of sea ice remains challenging in such a highly interconnected system.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-10-08T21:24:52+02:00</published>
            <updated>2026-10-08T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1833-2026</id>
            <title type="html">From manual classification to transformer-based language models: assessing the quality and consistency of historical convective event records
            </title>
            <link href="https://doi.org/10.5194/cp-22-1833-2026"/>
            <summary type="html">
                &lt;b&gt;From manual classification to transformer-based language models: assessing the quality and consistency of historical convective event records&lt;/b&gt;&lt;br&gt;
                Franck Schätz and Rüdiger Glaser&lt;br&gt;
                    Clim. Past, 22, 1833&#8211;1861, https://doi.org/10.5194/cp-22-1833-2026, 2026&lt;br&gt;
                Before measuring instruments, thunderstorms and hail were recorded only in written reports. We analysed around 7000 reports from 1000 to 1817 and, using a rule-based workflow, linguistically decoded the intensity of the thunderstorm and hail events described. The annual cycle derived from this corresponds well with modern observations. With these data, language models can be trained to reliably classify such events and make large collections of text accessible for climate research.
            </summary>
            <content type="html">
                &lt;b&gt;From manual classification to transformer-based language models: assessing the quality and consistency of historical convective event records&lt;/b&gt;&lt;br&gt;
                Franck Schätz and Rüdiger Glaser&lt;br&gt;
                    Clim. Past, 22, 1833&#8211;1861, https://doi.org/10.5194/cp-22-1833-2026, 2026&lt;br&gt;
                <p>This article investigates whether Transformer-based language models could replace the labour-intensive, manual classification of convective weather phenomena found in written texts from the pre-instrumental measurement era. The training set is based on a corpus of 6999 written observations from 494 Central European sources, spanning the period from 1000 to 1817. This corpus has been linguistically normalised, ranging from Middle High German to Contemporary German.</p&gt;        <p>For the training set, the text sources containing observations of thunderstorm and hail events are first classified manually using a formalised procedure. Quality assurance is initially carried out at the level of the existing textual information. To this end, evidence classes are introduced. These are based on linguistic evidence regarding the associated phenomena of thunderstorm and hail events. In the next step, the plausibility of the classified thunderstorm and hail events is assessed by checking their consistency with the DWD normal periods (1961&amp;#8211;1990, 1991&amp;#8211;2020).</p&gt;        <p>The seasonal signal is preserved across four language stages and nine source types, from the early 15th to the early 19th century. The classified thunderstorm and hail events exhibit a plausible physical signal and show strong correlations with current observations. The trained models &amp;#8220;ThunderstormBERT&amp;#8221; and &amp;#8220;HailBERT&amp;#8221; achieve macro-F1 scores of 0.83 and 0.93 respectively. Misclassifications primarily impact the middle thunderstorm class (moderate thunderstorm), where the classification scheme is least clear-cut.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-10-07T21:24:52+02:00</published>
            <updated>2026-10-07T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1863-2026</id>
            <title type="html">Historical climate extremes in Europe and the connection between spring precipitation and summer heat
            </title>
            <link href="https://doi.org/10.5194/cp-22-1863-2026"/>
            <summary type="html">
                &lt;b&gt;Historical climate extremes in Europe and the connection between spring precipitation and summer heat&lt;/b&gt;&lt;br&gt;
                Laura Lipfert, Ralf Hand, Angela-Maria Burgdorf, Christian Pfister, Heinz Wanner, and Stefan Brönnimann&lt;br&gt;
                    Clim. Past, 22, 1863&#8211;1879, https://doi.org/10.5194/cp-22-1863-2026, 2026&lt;br&gt;
                We analyse the link between dry springs and hot summers in Europe over the past 600 years. Starting with a study of the heat summer of 1473, which followed dry spring conditions in Southeastern Europe, we use the ModE-RA data set family to statistically analyse the link. We find that the link is strongest in regions where evaporation is moisture-limited. Hot summers are preceded by increased blocking over north-central Europe and a positive East Atlantic pattern in spring.
            </summary>
            <content type="html">
                &lt;b&gt;Historical climate extremes in Europe and the connection between spring precipitation and summer heat&lt;/b&gt;&lt;br&gt;
                Laura Lipfert, Ralf Hand, Angela-Maria Burgdorf, Christian Pfister, Heinz Wanner, and Stefan Brönnimann&lt;br&gt;
                    Clim. Past, 22, 1863&#8211;1879, https://doi.org/10.5194/cp-22-1863-2026, 2026&lt;br&gt;
                <p>Hot European summers are often preceded by dry springs such as in 2022, but also in 1473 or 1540, two well-known summers of catastrophic heat. Spring precipitation deficits deplete soil moisture levels, which can amplify extreme summer temperature anomalies in Europe through land-atmosphere feedback mechanisms and altered atmospheric circulation. However, the link is not particularly strong, and hence long time series might help to better elucidate the mechanisms. Starting from documentary data and an atlas of temperature, precipitation, and atmospheric circulation over Europe for climate extremes in the last 600 years, we explore this relationship in more detail. We analyse the extreme heat summer of 1473, which followed dry spring conditions in Southeastern Europe related to a positive East Atlantic pattern. We then use the ModE-RA paleo-reanalysis and combine it with an analysis of 11&amp;#8201;760 years of atmospheric model simulations as well as other reanalyses and reconstructions. Using a moving climatology approach with LOESS regressions to calculate anomalies, we identify significant negative correlations between winter-spring precipitation and summer temperatures in all data sets in the latitude band 36&amp;#8211;48<span class="inline-formula"><i>&amp;#176;</i></span>&amp;#8201;N (strongest over southeastern Europe), corresponding to known moisture-limited regions. Moreover, apart from precipitation anomalies, hot summers are preceded by increased blocking over north-central Europe and a positive East Atlantic pattern. Conversely, dry winter-springs are followed by more frequent blocking over northern Europe and, in model simulations, an increase in frequency and intensity of summer heatwaves. A linear regression approach for temperature in the northern Mediterranean region shows that precipitation in April and May has a strong, direct influence that does not vanish when taking the detailed atmospheric circulation in winter, spring, and summer into account, and hence cannot be explained by the effect of circulation on both, spring precipitation and summer temperature.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-10-07T21:24:52+02:00</published>
            <updated>2026-10-07T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1803-2026</id>
            <title type="html">Using ocean surface paleo-density to evaluate PMIP3 and PMIP4 Last Glacial Maximum climate simulations
            </title>
            <link href="https://doi.org/10.5194/cp-22-1803-2026"/>
            <summary type="html">
                &lt;b&gt;Using ocean surface paleo-density to evaluate PMIP3 and PMIP4 Last Glacial Maximum climate simulations&lt;/b&gt;&lt;br&gt;
                Héloïse Barathieu, Thibaut Caley, Masa Kageyama, Didier Swingedouw, and Pascale Braconnot&lt;br&gt;
                    Clim. Past, 22, 1803&#8211;1832, https://doi.org/10.5194/cp-22-1803-2026, 2026&lt;br&gt;
                This study evaluates climate model simulations of the Last Glacial Maximum using ocean surface density reconstructions from foraminiferal shells &amp;#948;&amp;#185;&amp;#8312;O. Models capture global patterns but regional climate changes are less well simulated, especially in the North Indian Ocean. Tropical differences between reconstructions and model simulations are mainly driven by changes in ocean salinity linked to precipitation.
            </summary>
            <content type="html">
                &lt;b&gt;Using ocean surface paleo-density to evaluate PMIP3 and PMIP4 Last Glacial Maximum climate simulations&lt;/b&gt;&lt;br&gt;
                Héloïse Barathieu, Thibaut Caley, Masa Kageyama, Didier Swingedouw, and Pascale Braconnot&lt;br&gt;
                    Clim. Past, 22, 1803&#8211;1832, https://doi.org/10.5194/cp-22-1803-2026, 2026&lt;br&gt;
                <p>Quantitative reconstruction of ocean surface density during the Last Glacial Maximum (LGM) offers valuable insights into the ability of climate models to simulate past climate conditions, when global temperatures were about 4.5 to 6&amp;#176;C colder than today. We assess the performance of the LGM climate simulations, as part of the 3rd and 4th phase of the Paleoclimate Modeling Intercomparisons Project, using a recent ocean surface density reconstruction based on the <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O of foraminiferal calcite (<span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O<span class="inline-formula"><sub>c</sub></span>). We consider the differences between the LGM and the preindustrial climates and each period separately, at both global and regional scales. Because surface density reflects the combined effects of temperature and salinity, we also examined sea surface temperature (SST) to better identify the processes underlying model&amp;#8211;data differences.</p&gt;        <p>On a global scale, surface density reconstructions generally exhibit greater spatial variability than simulated surface density anomalies (LGM&amp;#8201;<span class="inline-formula">&amp;#8722;</span>&amp;#8201;PI), although part of this difference is reduced when reconstruction uncertainties are taken into account. Model simulations tend to underestimate the magnitude of reconstructed density anomalies and substantial differences between cumulative distribution persist. Part of the mismatch may arise from the uneven spatial distribution of reconstructions, which are mostly located near coastal areas.</p&gt;        <p>Density anomaly (LGM&amp;#8201;<span class="inline-formula">&amp;#8722;</span>&amp;#8201;PI) differences between data and models are largely controlled by sea surface salinity (SSS), with SST contributing to a lesser extent. This influence of SSS is directly linked to the reduction in tropical precipitation during the LGM: model simulations that best match the large-scale density anomalies also simulate the strongest reductions in reconstructed low-latitude precipitation during the LGM, highlighting the key role of hydrological cycle changes in shaping surface density.</p&gt;        <p>All simulations capture key features of the reconstructed surface densities when the LGM and PI periods are analysed separately at the global scale, with Taylor diagrams and complementary performance metrics indicating moderate to good overall agreement despite differences among simulations.</p&gt;        <p>Regional analyses show that most simulations reproduce reconstructed Indian Ocean surface density reasonably well, although model simulations performance is systematically lower in the North Indian Ocean than in the South Indian Ocean. Focusing on the Indo-Pacific Warm Pool, proxy reconstructions indicate a weakened West-East tropical Indian surface density gradient during the LGM, but only 7 out of 14 model simulations (50&amp;#8201;%) reproduce this feature.</p&gt;        <p>These results highlight the need to improve and better constrain regional hydrological cycle changes in models, as improving their representation is crucial to reduce uncertainties in both paleoclimate simulations and future climate projections.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-10-06T21:24:52+02:00</published>
            <updated>2026-10-06T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1781-2026</id>
            <title type="html">Ocean warming caused by Late Ordovician glacial onset in a coupled climate-ice sheet simulation
            </title>
            <link href="https://doi.org/10.5194/cp-22-1781-2026"/>
            <summary type="html">
                &lt;b&gt;Ocean warming caused by Late Ordovician glacial onset in a coupled climate-ice sheet simulation&lt;/b&gt;&lt;br&gt;
                Yudong Sun, Yonggang Liu, Jiacheng Wu, Kai Man, Haonan Yu, Shuai Yuan, Yizhang Liu, Yue Liu, Qi Cui, Qiang Wei, and Yongyun Hu&lt;br&gt;
                    Clim. Past, 22, 1781&#8211;1802, https://doi.org/10.5194/cp-22-1781-2026, 2026&lt;br&gt;
                This study investigates the dramatic global cooling during the Late Ordovician, 440 million years ago. Our simulations reveal a powerful feedback loop: as the ice sheet grew, it generated strong, cold winds flowing down its slopes. These winds further cooled the continents, causing the ice sheet to expand even more. The super ice sheet led to a substantial global temperature drop of about 1.5 &amp;#176;C. Interestingly, while continents froze, the oceans warmed.
            </summary>
            <content type="html">
                &lt;b&gt;Ocean warming caused by Late Ordovician glacial onset in a coupled climate-ice sheet simulation&lt;/b&gt;&lt;br&gt;
                Yudong Sun, Yonggang Liu, Jiacheng Wu, Kai Man, Haonan Yu, Shuai Yuan, Yizhang Liu, Yue Liu, Qi Cui, Qiang Wei, and Yongyun Hu&lt;br&gt;
                    Clim. Past, 22, 1781&#8211;1802, https://doi.org/10.5194/cp-22-1781-2026, 2026&lt;br&gt;
                <p>The Late Ordovician marks the first major continental ice sheet event in the Phanerozoic Eon, despite high CO<span class="inline-formula"><sub>2</sub></span&gt; levels, coinciding with a dramatic global temperature drop and one of the largest mass extinctions. However, the critical role of ice sheet-climate feedbacks in driving the Late Ordovician glaciation remains poorly understood. Using an asynchronous coupling approach, we capture the critical feedback of the ice sheet on large-scale processes such as atmospheric circulation and accurately reproduce regional cooling processes driven by the strong ice albedo positive feedback. We then reveal a key positive feedback loop: ice sheet growth triggers katabatic winds, which in turn promote further ice sheet expansion. Results show a 1.4&amp;#8201;&amp;#176;C decrease in global mean surface temperature caused by ice sheet onset, with significant cooling over mid- to high-latitude continents while warming over the ocean. In contrast, the impact on tropical ocean temperatures remained limited. The high-latitude ocean warming is driven by the atmospheric stationary wave triggered by the massive ice sheet on the Gondwana continent. Our findings highlight the complex interactions between ice sheet dynamics, atmospheric and ocean circulation, emphasizing the importance of incorporating coupled ice sheet-climate feedbacks in palaeoclimate simulations.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-10-01T21:24:52+02:00</published>
            <updated>2026-10-01T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1741-2026</id>
            <title type="html">Trends in south pole particle concentrations imply holocene westerly wind strengthening
            </title>
            <link href="https://doi.org/10.5194/cp-22-1741-2026"/>
            <summary type="html">
                &lt;b&gt;Trends in south pole particle concentrations imply holocene westerly wind strengthening&lt;/b&gt;&lt;br&gt;
                Aaron Chesler, Dominic Winski, Karl Kreutz, Bess Koffman, Erich Osterberg, David Ferris, Zayta Thundercloud, Jihong Cole-Dai, Mark Wells, Aaron Putnam, and Katherine Anderson&lt;br&gt;
                    Clim. Past, 22, 1741&#8211;1756, https://doi.org/10.5194/cp-22-1741-2026, 2026&lt;br&gt;
                The Southern Hemisphere Westerly Winds impact global climate and Antarctic ice sheet stability; however, there are few complete records over the past 12&amp;#8201;000 years. We use a new mineral dust record from a South Pole ice core and identify a decrease in particle concentration and an increase in coarse particle percentage over the past ~&amp;#8201;11&amp;#8201;000 years. Together with other records, our data suggests a southward shift in the winds starting ~&amp;#8201;6500 years ago related to warming in the Southern Hemisphere.
            </summary>
            <content type="html">
                &lt;b&gt;Trends in south pole particle concentrations imply holocene westerly wind strengthening&lt;/b&gt;&lt;br&gt;
                Aaron Chesler, Dominic Winski, Karl Kreutz, Bess Koffman, Erich Osterberg, David Ferris, Zayta Thundercloud, Jihong Cole-Dai, Mark Wells, Aaron Putnam, and Katherine Anderson&lt;br&gt;
                    Clim. Past, 22, 1741&#8211;1756, https://doi.org/10.5194/cp-22-1741-2026, 2026&lt;br&gt;
                <p>The Southern Hemisphere Westerly Winds (SHWW) play an important role in global climate and Antarctic ice sheet dynamics; however, high-resolution proxy reconstructions are sparse. Conflicting evidence suggests SHWW latitudinal change, weakening and/or strengthening, throughout the Holocene. Dust microparticle characteristics preserved in Antarctic ice cores (i.e., changes in concentration and size) provide a useful physical proxy reflecting wind dynamics. We present South Pole Ice Core (SPC14) dust records spanning the Holocene. Dust concentrations (1.1&amp;#8211;5.1&amp;#8201;<span class="inline-formula">&amp;#181;</span>m) decrease through the Holocene, while the coarse particle percentage (CPP) increase due to a relatively larger decrease in finer (1.1&amp;#8211;3.2&amp;#8201;<span class="inline-formula">&amp;#181;</span>m) dust, highlighting an opposing trend. The South Pole dust trends, consistent with CMIP6-PMIP4 model trends, southern mid-latitude insolation, and mid- to high latitude Southern Hemisphere proxy records, reflect SHWW southward migration and strengthening of wind speed south of 51&amp;#176;&amp;#8201;S during the mid-Holocene (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;7000&amp;#8211;3000 years ago). Our findings suggest orbitally-driven warming throughout the Holocene led to strengthening and southward migration of the SHWW beginning <span class="inline-formula">&amp;#8764;</span>&amp;#8201;7000&amp;#160;years&amp;#160;BP.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-28T21:24:52+02:00</published>
            <updated>2026-09-28T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1757-2026</id>
            <title type="html">Holocene-like summer climate during Marine Isotope Stage 11 in northwestern Greenland
            </title>
            <link href="https://doi.org/10.5194/cp-22-1757-2026"/>
            <summary type="html">
                &lt;b&gt;Holocene-like summer climate during Marine Isotope Stage 11 in northwestern Greenland&lt;/b&gt;&lt;br&gt;
                John Michael N. Aguilar, Elizabeth K. Thomas, Diana S. Aga, Paul R. Bierman, Jason P. Briner, Isla S. Castañeda, and Andrew J. Christ&lt;br&gt;
                    Clim. Past, 22, 1757&#8211;1779, https://doi.org/10.5194/cp-22-1757-2026, 2026&lt;br&gt;
                As the Arctic warms, the Greenland Ice Sheet is losing mass, with implications for global sea levels. We analyzed biomarkers from sediments beneath 1387 m of ice at Camp Century, Greenland, deposited when the ice sheet was smaller. Reconstructed summer temperature and precipitation isotopes from ~ 400 000 years ago show summers ~ 4.7 &amp;#176;C warmer than today, with more local moisture from reduced ice. This result highlights that both how warm and how long warming lasts matter to reduce ice loss.
            </summary>
            <content type="html">
                &lt;b&gt;Holocene-like summer climate during Marine Isotope Stage 11 in northwestern Greenland&lt;/b&gt;&lt;br&gt;
                John Michael N. Aguilar, Elizabeth K. Thomas, Diana S. Aga, Paul R. Bierman, Jason P. Briner, Isla S. Castañeda, and Andrew J. Christ&lt;br&gt;
                    Clim. Past, 22, 1757&#8211;1779, https://doi.org/10.5194/cp-22-1757-2026, 2026&lt;br&gt;
                <p>Determining the climatic conditions under which the Greenland Ice Sheet (GrIS) was smaller than present is important to quantify GrIS sensitivity to climate change. We use biomarkers in sediment collected beneath the GrIS at Camp Century, northwestern Greenland, to reconstruct summer temperature and atmospheric circulation 416&amp;#8201;000&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;38&amp;#8201;000 years ago, at some point during Marine Isotope Stage 11 (MIS 11). We find that northwestern Greenland summer climate during MIS 11 was similar to the middle Holocene but different than the 20th century. Air temperature was 4.7&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;3.2&amp;#8201;&amp;#176;C warmer, and atmospheric water vapor isotope values were 22&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;18&amp;#8201;&amp;#8240; <span class="inline-formula"><sup>2</sup></span>H-enriched, indicating a greater contribution of locally evapotranspired moisture. These conditions are similar to or slightly warmer than during peak Holocene warmth on Greenland, when the Camp Century site remained ice-covered, and cooler than the Last Interglacial (LIG). Biomarkers from lower in the section likely represent an earlier ice-free interval, potentially during the Pliocene or early Pleistocene, and record climatic conditions similar to MIS 11. These data add to the sparse available climate data for the early and middle Pleistocene on Greenland, and suggest interglacial periods had similar temperature throughout the Pleistocene. We interpret the reduced GrIS extent in northwestern Greenland during MIS11 compared to the Holocene, despite similar temperature, to indicate ice-sheet response to prolonged warmth, as reconstructed in southern Greenland. Therefore, efforts to reduce both the magnitude and duration of summer warmth in the coming centuries will be important to curbing ice-sheet retreat.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-28T21:24:52+02:00</published>
            <updated>2026-09-28T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1729-2026</id>
            <title type="html">Middle to late Holocene cooling and increased zonal asymmetry in the mid-latitude North Atlantic
            </title>
            <link href="https://doi.org/10.5194/cp-22-1729-2026"/>
            <summary type="html">
                &lt;b&gt;Middle to late Holocene cooling and increased zonal asymmetry in the mid-latitude North Atlantic&lt;/b&gt;&lt;br&gt;
                Weimin Si, Timothy Herbert, and John R. Toggweiler&lt;br&gt;
                    Clim. Past, 22, 1729&#8211;1740, https://doi.org/10.5194/cp-22-1729-2026, 2026&lt;br&gt;
                Transient climate models simulate warming over the past 5000 years due to a 20 ppm CO<sub>2</sub&gt; rise, yet paleo-proxies indicate cooling. In this study, we examine the mid-latitude North Atlantic, where model-data mismatch is largest. Our analysis links Late Holocene cooling to increased zonal SST (Sea Surface Temperature) asymmetry, likely from basin-scale reorganization of inter-gyre circulation. Transient models, however, do not to capture this spatial pattern and associated circulation changes.
            </summary>
            <content type="html">
                &lt;b&gt;Middle to late Holocene cooling and increased zonal asymmetry in the mid-latitude North Atlantic&lt;/b&gt;&lt;br&gt;
                Weimin Si, Timothy Herbert, and John R. Toggweiler&lt;br&gt;
                    Clim. Past, 22, 1729&#8211;1740, https://doi.org/10.5194/cp-22-1729-2026, 2026&lt;br&gt;
                <p>Sea Surface Temperature reconstructions derived from alkenone biomarker (SST-alk) reveal a cooling trend in the North Atlantic during the late Holocene (the last 5000 years), contrary to the warming simulated by transient climate models driven by 20&amp;#8201;ppm increase in greenhouse gas concentrations. In this study, we present new SST-alk time series from the inter-gyre region of the North Atlantic. Our results, together with existing data, indicate that late Holocene cooling is marked by an increasing zonal SST gradient across the mid-latitude North Atlantic, with more pronounced cooling in the west than in the east. Complementary planktonic foraminifera assemblage data, interpreted alongside other circulation proxies, suggest that a late Holocene reorganization of inter-gyre ocean circulation as a likely driver of this zonal asymmetry. Finally, we compare these proxy-based reconstructions with transient climate model simulations (TraCE-21k), and find that models do not reproduce the observed zonally asymmetric cooling and the inferred circulation changes. This misrepresentation of spatial and temporal variability likely explains the data-model discrepancy in the mid-latitude North Atlantic.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-25T21:24:52+02:00</published>
            <updated>2026-09-25T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1711-2026</id>
            <title type="html">Muted orbital-scale monsoon variability over the Korean Peninsula
            </title>
            <link href="https://doi.org/10.5194/cp-22-1711-2026"/>
            <summary type="html">
                &lt;b&gt;Muted orbital-scale monsoon variability over the Korean Peninsula&lt;/b&gt;&lt;br&gt;
                Nitesh Sinha, Axel Timmermann, Sun-Seon Lee, Kyoung-Nam Jo, Jasper A. Wassenburg, Daniel M. Cleary, and Kyung-Sook Yun&lt;br&gt;
                    Clim. Past, 22, 1711&#8211;1727, https://doi.org/10.5194/cp-22-1711-2026, 2026&lt;br&gt;
                A longstanding conundrum regarding the stable oxygen isotope (&amp;#948;<sup>18</sup>O) proxy for hydroclimate in speleothems from the Korean Peninsula, which, unlike records from East Asia (e.g., China), do not exhibit isotopic shifts in response to precession forcing. Using Korean speleothem records spanning several orbital-scale segments of the last ~550,000 years and paleoclimate simulations, the present study proposes a plausible role of the oceanic and continental moisture mixing in suppressing &amp;#948;<sup>18</sup>O signals.
            </summary>
            <content type="html">
                &lt;b&gt;Muted orbital-scale monsoon variability over the Korean Peninsula&lt;/b&gt;&lt;br&gt;
                Nitesh Sinha, Axel Timmermann, Sun-Seon Lee, Kyoung-Nam Jo, Jasper A. Wassenburg, Daniel M. Cleary, and Kyung-Sook Yun&lt;br&gt;
                    Clim. Past, 22, 1711&#8211;1727, https://doi.org/10.5194/cp-22-1711-2026, 2026&lt;br&gt;
                <p>A recent study identified an east-west dipole pattern in Asian Summer Monsoon precipitation and in its oxygen-isotope composition variability in response to orbital forcing (Wen et al.,&amp;#160;2024). The Korean Peninsula (KP) is situated near the nodal line of this dipole and should therefore exhibit muted precessional variability in both. So far, this conjecture has not been tested using paleoclimatic data. Here, we present speleothem oxygen isotope (<span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O) records from the KP, which support the notion of suppressed orbital-scale hydroclimate variability. Conducting a transient model simulation with the isotope-enabled Community Earth System Model (iCESM1.2) covering the past 130&amp;#8201;000&amp;#160;years, along with tagging experiments for low and high insolation conditions, we show that, on precessional timescales, isotopic contributions from oceanic and continental moisture sources compensate each other over the KP, resulting in only a weak regional signal in precipitation <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O. Based on iCESM1.2 simulations, we further demonstrate that deuterium excess (d-excess) variability over the KP would still capture the moisture source region's zonal seesaw response to precessional forcing. We propose that, given the region's strong sensitivity to changes in moisture sources, paleo-water d-excess reconstructions from East Asia speleothems could provide valuable additional constraints on the drivers of regional monsoon systems. This study offers new insights into the spatiotemporal variability of Pan-Asian hydroclimates and its links to changes in moisture source.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-22T21:24:52+02:00</published>
            <updated>2026-09-22T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1691-2026</id>
            <title type="html">Complex interplay of forcings drives Indian vegetation and summer monsoon variability during MIS 11
            </title>
            <link href="https://doi.org/10.5194/cp-22-1691-2026"/>
            <summary type="html">
                &lt;b&gt;Complex interplay of forcings drives Indian vegetation and summer monsoon variability during MIS 11&lt;/b&gt;&lt;br&gt;
                Dulce Oliveira, Stéphanie Desprat, Qiuzhen Yin, Coralie Zorzi, Zhipeng Wu, Krishnamurthy Anupama, Srinivasan Prasad, Montserrat Alonso-García, and Philippe Martinez&lt;br&gt;
                    Clim. Past, 22, 1691&#8211;1709, https://doi.org/10.5194/cp-22-1691-2026, 2026&lt;br&gt;
                We present an unprecedented record of Indian summer monsoon (ISM)-induced vegetation changes for Marine Isotope Stage (MIS) 11, a key interglacial. Site U1446 pollen data and models show that ISM-vegetation shifts stem from an interplay of dominant forcings based on boundary conditions. Insolation is the main driver during MIS 11c interglacial conditions, akin to future scenarios, while ice volume and CO&amp;#8322; prevail in the glacial inception. Superimposed changes are marked by prominent forest contractions and expansions.
            </summary>
            <content type="html">
                &lt;b&gt;Complex interplay of forcings drives Indian vegetation and summer monsoon variability during MIS 11&lt;/b&gt;&lt;br&gt;
                Dulce Oliveira, Stéphanie Desprat, Qiuzhen Yin, Coralie Zorzi, Zhipeng Wu, Krishnamurthy Anupama, Srinivasan Prasad, Montserrat Alonso-García, and Philippe Martinez&lt;br&gt;
                    Clim. Past, 22, 1691&#8211;1709, https://doi.org/10.5194/cp-22-1691-2026, 2026&lt;br&gt;
                <p>Marine Isotope Stage (MIS) 11 has long been considered a unique Quaternary interglacial stage due to its orbital similarities with the Holocene, persistent high atmospheric CO<span class="inline-formula"><sub>2</sub></span&gt; concentrations and its extended duration, which triggered an unusual polar ice-sheet loss. Despite its importance, variability of the Asian summer monsoon, as well as its impacts on vulnerable tropical forests, during MIS 11 remain unexplored. Here, we document, for the first time, the vegetation and monsoon changes in eastern peninsular India and their underlying forcings using pollen analysis from IODP Site U1446, strategically retrieved from the Bay of Bengal to record changes in the summer monsoon rainfall in the core monsoon zone of India. Our results reveal the distinct roles of insolation, CO<span class="inline-formula"><sub>2</sub></span>, ice volume, and millennial-scale variability in driving vegetation and summer monsoon changes, depending on the changing boundary conditions throughout MIS 11. Site U1446 pollen data, supported by model simulations, indicate that the maximum tropical forest expansion and strongest monsoon activity during the interglacial period (MIS 11c) followed boreal summer insolation, revealing the dominant role of insolation under a warm climate state with high CO<span class="inline-formula"><sub>2</sub></span&gt; and reduced ice volume. Conversely, during the late MIS 11 (MIS 11b-a), the tropical forest decreased despite high insolation, indicating that expanding ice sheets and lower CO<span class="inline-formula"><sub>2</sub></span&gt; overshadowed the insolation influence on the summer monsoon. Millennial-scale variability during late MIS 11 likely played an additional role in counteracting the response of the summer monsoon to insolation. Abrupt forest contractions, tied to low monsoon rainfall and southward shifts of the intertropical convergence zone, are attributed to ice sheet dynamics and ocean circulation disturbances. These events were rapidly followed by pronounced forest expansions, linked to northward shifts of the intertropical convergence zone, reinvigoration of deep-ocean circulation, and CH<span class="inline-formula"><sub>4</sub></span&gt;  overshoots. Conspicuously, the first and most severe forest setback interrupted the full interglacial conditions of MIS 11, suggesting that extreme summer monsoon weakening could also occur under similarly warm future conditions. Our findings provide new insights into monsoon behavior during MIS 11, highlighting its high sensitivity to climate changes in the context of projected summer monsoon intensification and its effect on the tropical forest, which is a key component of both global carbon and methane cycles.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-15T21:24:52+02:00</published>
            <updated>2026-09-15T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1675-2026</id>
            <title type="html">Limited atmospheric iron availability increase during the Younger Dryas in the Northern Hemisphere
            </title>
            <link href="https://doi.org/10.5194/cp-22-1675-2026"/>
            <summary type="html">
                &lt;b&gt;Limited atmospheric iron availability increase during the Younger Dryas in the Northern Hemisphere&lt;/b&gt;&lt;br&gt;
                François Burgay, Haley Derrod, Tobias Erhardt, Federico Scoto, Delia Segato, Niccolò Maffezzoli, Federico Dallo, Daniele Zannoni, Azzurra Spagnesi, Helle-Astrid Kjær, Hubertus Fischer, Cristiano Varin, Carlo Barbante, and Andrea Spolaor&lt;br&gt;
                    Clim. Past, 22, 1675&#8211;1689, https://doi.org/10.5194/cp-22-1675-2026, 2026&lt;br&gt;
                <span data-olk-copy-source="MessageBody">Ice-core measurements from Greenland suggest that atmospheric iron deposition played a smaller role than previously thought in regulating marine productivity in the iron-limited North Pacific. Despite a strong increase in total iron deposition, the fraction of iron more likely to be available to phytoplankton rose only modestly, pointing to sea-ice extent and sedimentary iron remobilization as potentially more important factors during the last glacial transition.</span>
            </summary>
            <content type="html">
                &lt;b&gt;Limited atmospheric iron availability increase during the Younger Dryas in the Northern Hemisphere&lt;/b&gt;&lt;br&gt;
                François Burgay, Haley Derrod, Tobias Erhardt, Federico Scoto, Delia Segato, Niccolò Maffezzoli, Federico Dallo, Daniele Zannoni, Azzurra Spagnesi, Helle-Astrid Kjær, Hubertus Fischer, Cristiano Varin, Carlo Barbante, and Andrea Spolaor&lt;br&gt;
                    Clim. Past, 22, 1675&#8211;1689, https://doi.org/10.5194/cp-22-1675-2026, 2026&lt;br&gt;
                <p>Iron (Fe) availability modulates phytoplankton blooms in High-Nutrient Low-Chlorophyll (HNLC) regions, i.e., ocean areas characterized by an abundance of major nutrients but low marine productivity. Fe can be delivered to the oceans through atmospheric dust deposition, making ice cores unique archives for reconstructing past changes in aeolian Fe deposition. However, while it is known that during dustier periods atmospheric Fe depositions increased, uncertainties remain regarding the fraction of Fe actually available to phytoplankton. Here, we present evidence from the EGRIP ice core (Greenland) during the Pleistocene-Holocene transition (10.3&amp;#8211;13.0&amp;#8201;ka), which provides insights into atmospheric aerosol deposition over the Fe-limited North Pacific Ocean. Results show that, in contrast to the 17-fold enhancement in total Fe determined by Inductively Coupled Plasma Mass Spectrometry, the iron fraction more likely available for phytoplankton (i.e., labile iron) increased only modestly (<span class="inline-formula">+</span>29&amp;#8201;%) during the Younger Dryas compared to the Early Holocene, likely due to prevailing alkaline aerosol conditions reducing its solubility. This finding supports the hypothesis that factors other than atmospheric Fe deposition (e.g., stronger water stratification, sea-ice extent, volcanic eruptions, iron remobilization from sediments), played a more relevant role in regulating marine net primary productivity in the HNLC North Pacific Ocean over the last glacial transition.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-15T21:24:52+02:00</published>
            <updated>2026-09-15T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1655-2026</id>
            <title type="html">Quantifying Southern Hemisphere dust sources during the Last Glacial-Interglacial Transition using rare earth elements in the EPICA Dome C ice core
            </title>
            <link href="https://doi.org/10.5194/cp-22-1655-2026"/>
            <summary type="html">
                &lt;b&gt;Quantifying Southern Hemisphere dust sources during the Last Glacial-Interglacial Transition using rare earth elements in the EPICA Dome C ice core&lt;/b&gt;&lt;br&gt;
                Sibylle Boxho, Aubry Vanderstraeten, Nadine Mattielli, Goulven G. Laruelle, Aloys Bory, Paolo Gabrielli, and Steeve Bonneville&lt;br&gt;
                    Clim. Past, 22, 1655&#8211;1674, https://doi.org/10.5194/cp-22-1655-2026, 2026&lt;br&gt;
                We present a high-resolution, quantitative reconstruction of dust provenance in the EPICA Dome C ice core (33.7&amp;#8211;2.8 kyr BP) using Rare Earth Elements (REE). Dust was mainly sourced from Patagonia during glacial periods, shifting toward Australia, Southern Africa, and the Puna-Altiplano after 14.5 kyr BP due to sea-level rise and hydrological rearrangement in Patagonia. These changes also reflect major reorganizations of Southern Hemisphere atmospheric circulation.
            </summary>
            <content type="html">
                &lt;b&gt;Quantifying Southern Hemisphere dust sources during the Last Glacial-Interglacial Transition using rare earth elements in the EPICA Dome C ice core&lt;/b&gt;&lt;br&gt;
                Sibylle Boxho, Aubry Vanderstraeten, Nadine Mattielli, Goulven G. Laruelle, Aloys Bory, Paolo Gabrielli, and Steeve Bonneville&lt;br&gt;
                    Clim. Past, 22, 1655&#8211;1674, https://doi.org/10.5194/cp-22-1655-2026, 2026&lt;br&gt;
                <p>Dust deposits in ice cores provide a valuable archive of past atmospheric circulation, offering insights into climate dynamics during key climate transitions such as the last glacial termination. Here, we present a novel high-resolution reconstruction of dust provenance in the EPICA Dome&amp;#160;C (EDC) ice core from 33.7 to 2.8&amp;#8201;kyr BP, based on Rare Earth Element (REE) patterns. Using a statistical unmixing algorithm on 279 samples, we quantify, for the first time, contributions from key Southern Hemisphere dust sources. During the late Marine Isotope Stage&amp;#160;3 (MIS3), the Last Glacial Maximum (LGM) and Heinrich Stadial&amp;#160;1 (HS1), dust at EDC was dominated by Patagonian sources, <span class="inline-formula">&amp;#8764;</span>&amp;#8201;65&amp;#8201;%&amp;#8211;75&amp;#8201;% of total deposition, with secondary inputs from Australia (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;9&amp;#8201;%&amp;#8211;11&amp;#8201;%), Southern Africa (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;5&amp;#8201;%&amp;#8211;9&amp;#8201;%), New Zealand (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;6&amp;#8201;%&amp;#8211;14&amp;#8201;%), and Puna-Altiplano (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;2&amp;#8201;%&amp;#8211;4&amp;#8201;%). After <span class="inline-formula">&amp;#8764;</span>&amp;#8201;14.5&amp;#8201;kyr BP, and especially during the Holocene, the dust assemblage shifted toward greater contributions from low-latitude sources including Australia (21&amp;#8201;%&amp;#8211;28&amp;#8201;%), Southern Africa (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;8&amp;#8201;%&amp;#8211;9&amp;#8201;%), and the Puna-Altiplano (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;8&amp;#8201;%&amp;#8211;9&amp;#8201;%) &amp;#8211; while the Patagonian contribution decreased to an average of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;43&amp;#8201;%&amp;#8211;53&amp;#8201;%, New Zealand (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;4&amp;#8201;%&amp;#8211;10&amp;#8201;%) &amp;#8211; and source compositions became more variable. This transition in dust provenance contribution is supported by our modeled Sr-Nd isotope composition of EDC dust, which also aligns with changes observed in other East Antarctic ice cores. Comparison with the EDML ice core provenance record reveals overall agreement in major sources and timing of the shifts but also highlights regional variations in the secondary contributions, with EDC showing more consistent inputs from Australia and EDML from Southern Africa. The coherence of the provenance shift recorded at EDC and EDML ice cores points to a common large-scale control, in line with the influence of eustatic sea-level rise and postglacial reorganization of fluvial sediment routing and availability in southern South America.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-08T21:24:52+02:00</published>
            <updated>2026-09-08T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1609-2026</id>
            <title type="html">Mixed layer depth in the PMIP4 <i>midHolocene</i> simulations: comparison to proxy data in North Atlantic deep convection regions
            </title>
            <link href="https://doi.org/10.5194/cp-22-1609-2026"/>
            <summary type="html">
                &lt;b&gt;Mixed layer depth in the PMIP4 midHolocene simulations: comparison to proxy data in North Atlantic deep convection regions&lt;/b&gt;&lt;br&gt;
                Xiner Wu, Anne de Vernal, and Paul G. Myers&lt;br&gt;
                    Clim. Past, 22, 1609&#8211;1629, https://doi.org/10.5194/cp-22-1609-2026, 2026&lt;br&gt;
                The ocean mixed layer needs to be correctly represented in climate models to provide reliable future projections. We evaluate the mixed layer depth in 15 climate models against reconstructions for the mid-Holocene North Atlantic. The lack of meltwater input to models causes the simulated mixed layer to be deeper than reconstructed in the Labrador Sea but does not affect the Nordic Seas. Deep ocean mixing in the Labrador Sea may be particularly sensitive to ice-sheet melting under global warming.
            </summary>
            <content type="html">
                &lt;b&gt;Mixed layer depth in the PMIP4 midHolocene simulations: comparison to proxy data in North Atlantic deep convection regions&lt;/b&gt;&lt;br&gt;
                Xiner Wu, Anne de Vernal, and Paul G. Myers&lt;br&gt;
                    Clim. Past, 22, 1609&#8211;1629, https://doi.org/10.5194/cp-22-1609-2026, 2026&lt;br&gt;
                <p>The ocean mixed layer plays an essential role in the climate system, regulating energy fluxes at the ocean-atmosphere interface. Its representation in climate models is thus critical. Here, we evaluate the mixed layer depth (MLD) in 15 models from the Paleoclimate Modelling Intercomparison Project 4 (PMIP4) against dinocyst-based MLD reconstructions from the subpolar North Atlantic for the mid-Holocene (MH, 6&amp;#8201;ka&amp;#8201;BP). We find a large spread in MLD responses to MH forcings across the models in the present-day deep-water formation areas, underscoring the importance of model uncertainty. Most models fail to capture the direction of MLD change, and the ensemble mean does not necessarily outperform individual models. While the ensemble mean aligns broadly with proxy data in the Nordic Seas, pronounced proxy-model discrepancy in the Labrador Sea suggests that meltwater forcing is a missing parameter, and that deep-water formation in the Labrador Sea may be particularly vulnerable under a future scenario of global warming and ice-sheet melting.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-02T21:24:52+02:00</published>
            <updated>2026-09-02T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1631-2026</id>
            <title type="html">Paleoenvironmental and paleoclimatic reconstruction in the Western Mediterranean during the Late Early Pleistocene
            </title>
            <link href="https://doi.org/10.5194/cp-22-1631-2026"/>
            <summary type="html">
                &lt;b&gt;Paleoenvironmental and paleoclimatic reconstruction in the Western Mediterranean during the Late Early Pleistocene&lt;/b&gt;&lt;br&gt;
                Maé Catrain, Séverine Fauquette, Odile Peyron, Nathalie Combourieu-Nebout, Vincent Lebreton, Morgane Fischer-Fries, Mary Robles, Viviane Bout-Roumazeilles, Patricia Richard, Marion Delattre, Lionel Dubost, Sébastien Joannin, Amandine Viala, Yul Altolaguirre, Jean-Pierre Suc, Jeanne Lepelletier, and Marie-Hélène Moncel&lt;br&gt;
                    Clim. Past, 22, 1631&#8211;1653, https://doi.org/10.5194/cp-22-1631-2026, 2026&lt;br&gt;
                This multiproxy study investigates changes in climate cyclicity at Early-Middle Pleistocene Transition. Clay mineralogy analysis highlights a sudden change in oceanic and atmospheric circulation in the Alboran Basin around 1140 ka. Pollen, foraminifera and faunal data suggest that the climate and vegetation of this region are more likely to be influenced by variations in precipitation, hinting at major differences between the Iberian Peninsula and southern Italy.
            </summary>
            <content type="html">
                &lt;b&gt;Paleoenvironmental and paleoclimatic reconstruction in the Western Mediterranean during the Late Early Pleistocene&lt;/b&gt;&lt;br&gt;
                Maé Catrain, Séverine Fauquette, Odile Peyron, Nathalie Combourieu-Nebout, Vincent Lebreton, Morgane Fischer-Fries, Mary Robles, Viviane Bout-Roumazeilles, Patricia Richard, Marion Delattre, Lionel Dubost, Sébastien Joannin, Amandine Viala, Yul Altolaguirre, Jean-Pierre Suc, Jeanne Lepelletier, and Marie-Hélène Moncel&lt;br&gt;
                    Clim. Past, 22, 1631&#8211;1653, https://doi.org/10.5194/cp-22-1631-2026, 2026&lt;br&gt;
                <p>The major climate change recorded during the Early-Middle Pleistocene Transition (1.4&amp;#8211;0.4&amp;#8201;Ma) is characterized by an increase in the length of climatic cycles from 41  to 100&amp;#8201;ka. During this period, the Mediterranean climate underwent aridification associated with a drop in temperatures. This period also corresponds to the arrival of the first hominins in Western Europe. This study aims to establish the climatic framework at the end of the Early Pleistocene between MIS 37-31 (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;1.25 to 1.06&amp;#8201;Ma). To this end, a multiproxy approach was applied to assemblages of planktonic foraminifera, pollen and clay mineralogy, constituting a multi-method approach to climate reconstruction. Comparisons with other sequences from the Central and Western Mediterranean show major differences between the Iberian Peninsula and southern Italy. Indeed, the MIS 31 appears cooler and dryer in the south of the Iberian Peninsula than in central Mediterranean. Clay mineralogy analysis highlights a sudden change in oceanic and atmospheric circulation in the Alboran Basin around 1140&amp;#8201;ka. Climate reconstructions follow climatic cycles, with temperatures that appear to be underestimated compared to temperature reconstructions based on fauna from southern Spain. Precipitation reconstructions, on the other hand, are more consistent, suggesting that the climate and vegetation of this region are more likely to be influenced by variations in precipitation. These new data enhance our understanding of the climate of the South-western Mediterranean at the beginning of the Early-Middle Pleistocene Transition.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-02T21:24:52+02:00</published>
            <updated>2026-09-02T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1585-2026</id>
            <title type="html">Anatolia (T&#252;rkiye) during the late Eocene and the Eocene&#8211;Oligocene Transition: successive warming and cooling, aridification, and implications for the westward dispersal of Asian terrestrial mammals
            </title>
            <link href="https://doi.org/10.5194/cp-22-1585-2026"/>
            <summary type="html">
                &lt;b&gt;Anatolia (Türkiye) during the late Eocene and the Eocene–Oligocene Transition: successive warming and cooling, aridification, and implications for the westward dispersal of Asian terrestrial mammals&lt;/b&gt;&lt;br&gt;
                Paul Botté, Alexis Licht, Anne-Lise Jourdan, Leny Montheil, François Demory, Mustafa Kaya, Faruk Ocakoğlu, Mehmet Serkan Akkiraz, Deniz İbilioğlu, Pauline Coster, Grégoire Métais, Benjamin Raynaud, and K. Christopher Beard&lt;br&gt;
                    Clim. Past, 22, 1585&#8211;1608, https://doi.org/10.5194/cp-22-1585-2026, 2026&lt;br&gt;
                The Eocene&amp;#8211;Oligocene Transition (EOT; ~34 Ma) marks a major global cooling that transformed terrestrial ecosystems and influenced mammalian dispersals. A continental record from Anatolia reveals a Late Eocene warming followed by abrupt cooling at the EOT, documented by geochemistry and sedimentology. This interval is also characterized by increasing aridity, which likely contributed to the decline of endemic taxa and facilitated the westward expansion of Asian mammals into western Europe.
            </summary>
            <content type="html">
                &lt;b&gt;Anatolia (Türkiye) during the late Eocene and the Eocene–Oligocene Transition: successive warming and cooling, aridification, and implications for the westward dispersal of Asian terrestrial mammals&lt;/b&gt;&lt;br&gt;
                Paul Botté, Alexis Licht, Anne-Lise Jourdan, Leny Montheil, François Demory, Mustafa Kaya, Faruk Ocakoğlu, Mehmet Serkan Akkiraz, Deniz İbilioğlu, Pauline Coster, Grégoire Métais, Benjamin Raynaud, and K. Christopher Beard&lt;br&gt;
                    Clim. Past, 22, 1585&#8211;1608, https://doi.org/10.5194/cp-22-1585-2026, 2026&lt;br&gt;
                <p>The Eocene&amp;#8211;Oligocene Transition (EOT dated at <span class="inline-formula">&amp;#8764;</span>&amp;#8201;34&amp;#8201;Ma) represents one of the most significant climatic shifts of the Cenozoic, marking the transition from the last warmhouse state to a coolhouse state. This global cooling had major consequences for terrestrial ecosystems and was synchronous with the dispersal of numerous Asian mammalian clades towards western Europe. However, the terrestrial expression of the EOT exhibits strong regional heterogeneity questioning its role in establishing dispersal corridors associated with floral and faunal turnovers.</p&gt;        <p>Here, we describe, date, and document the paleoenvironments of a continental sedimentary section from Balkanatolia, a biogeographic province corresponding to the present-day Balkans (NE Mediterranean region) and Anatolia (T&amp;#252;rkiye). This region most likely functioned as a critical stepping stone for the dispersal of Asian mammals toward western Europe. Our sedimentary record represents a fluvio-lacustrine system exposed over a <span class="inline-formula">&amp;#8764;</span>&amp;#8201;200&amp;#8201;m section located in B&amp;#252;y&amp;#252;kteflek (&amp;#199;i&amp;#231;ekda&amp;#287;&amp;#305;/K&amp;#305;r&amp;#351;ehir area, T&amp;#252;rkiye), dated by magnetostratigraphy to the Priabonian and the lower Rupelian, including the Oi-1 glaciation (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;33.65&amp;#8201;Ma). Clumped isotope analyses on pedogenic carbonates across our record show evidence for a Late Eocene Warming starting during the middle Priabonian (ca. 37&amp;#8201;Ma), followed by a marked cooling event at the Eocene&amp;#8211;Oligocene Glacial Maximum (EOGM). Stable isotopic data and sedimentary facies further indicate that this complete interval is associated with a long-term aridification trend, starting during the Late Eocene warming and culminating at the EOT. Our results provide the first quantitative record of late Eocene warming on land, and our temperature estimates for the earliest Oligocene cooling are consistent with other Eurasian clumped-isotope records. These temperature shifts and associated aridification steps may have acted as contributing drivers of the late Eocene decline of Balkanatolian endemic taxa and likely facilitated the westward expansion of Asia-derived mammals ultimately resulting in the colonization of western Europe.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-31T21:24:52+02:00</published>
            <updated>2026-08-31T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1559-2026</id>
            <title type="html">Increased abyssal ocean density stratification across the Middle Pleistocene Transition
            </title>
            <link href="https://doi.org/10.5194/cp-22-1559-2026"/>
            <summary type="html">
                &lt;b&gt;Increased abyssal ocean density stratification across the Middle Pleistocene Transition&lt;/b&gt;&lt;br&gt;
                Nicola C. Thomas, Heather L. Ford, Mervyn Greaves, and David A. Hodell&lt;br&gt;
                    Clim. Past, 22, 1559&#8211;1584, https://doi.org/10.5194/cp-22-1559-2026, 2026&lt;br&gt;
                We reconstruct interbasinal temperature and salinity gradients using stacked Mg/Ca and benthic&amp;#160;&amp;#948;&amp;#185;&amp;#8312;O records for the past 1.5 Myr. Across the Middle Pleistocene Transition, the deep Atlantic cooled and the Pacific became more saline, increasing deep ocean density stratification. The glacial ocean became a more effective carbon trap, which lowered atmospheric <em>p</em>CO<sub>2</sub>, and led to the growth of larger ice sheets. Results support a physical role for abyssal ocean stratification in explaining the MPT.
            </summary>
            <content type="html">
                &lt;b&gt;Increased abyssal ocean density stratification across the Middle Pleistocene Transition&lt;/b&gt;&lt;br&gt;
                Nicola C. Thomas, Heather L. Ford, Mervyn Greaves, and David A. Hodell&lt;br&gt;
                    Clim. Past, 22, 1559&#8211;1584, https://doi.org/10.5194/cp-22-1559-2026, 2026&lt;br&gt;
                <p>The cause of the fundamental reorganisation of the climate system during the Middle Pleistocene Transition (MPT; <span class="inline-formula">&amp;#8764;</span>&amp;#8201;1.25&amp;#8211;0.65&amp;#160;million years ago (Ma)), when glacial cycles intensified and lengthened from 41 thousand  year (kyr) to quasi-100&amp;#8201;kyr periodicity, remains one of the enduring unsolved questions in palaeoclimate science. Increasing attention has focused on the role of the marine carbon cycle, with enhanced carbon storage in the deep sea linked to changes in deep-water temperature and salinity that increase abyssal ocean density stratification. Here we report new high-resolution reconstructions of deep-water temperature and the isotopic composition of seawater (<span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O<span class="inline-formula"><sub>seawater</sub></span>), a proxy for ice volume and salinity, from North Atlantic Site U1385, using paired benthic foraminiferal <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Mg</mi><mo>/</mo><mi mathvariant="normal">Ca</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="37pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="bda123048c697326946a54d2f5b8ecc8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1559-2026-ie00001.svg" width="37pt" height="14pt" src="cp-22-1559-2026-ie00001.png"/></svg:svg></span></span&gt;  and oxygen isotope (<span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O) analyses. Together with published records, we present basin-scale and globally distributed compilations of deep-water temperature and <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O<span class="inline-formula"><sub>seawater</sub></span&gt; to assess changes in abyssal ocean stratification for the past 1.5&amp;#160;million years (Myr). Across the MPT, interbasinal gradients suggest North Atlantic deep-water became colder while Pacific deep-water became more saline during glacial periods after <span class="inline-formula">&amp;#8764;</span>&amp;#8201;930 thousand years ago (ka). Deep-ocean <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O<span class="inline-formula"><sub>seawater</sub></span&gt; increased in both the Atlantic and Pacific across the MPT indicating increased continental ice volume. But, the increase was greater in the Pacific than the Atlantic, which we suggest reflects increased salinity of Southern Component Water (SCW). We propose the following sequence of changes during the MPT as a working hypothesis: (1) freshwater input to the marginal seas around Antarctica was reduced beginning at 930&amp;#8201;ka by decreased melting of the Antarctic Ice Sheet and/or marine ice shelves and increased sea ice formation in the Southern Ocean; (2) the salinity and density of SCW increased, resulting in enhanced abyssal ocean density stratification and rendering the deep ocean a more effective carbon trap; (3) together with increased export production of organic matter and reduced deep-to-surface water exchange in the Southern Ocean, carbon storage in the deep ocean increased, lowering glacial atmospheric <span class="inline-formula"><i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span>; (4) lower <span class="inline-formula"><i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span&gt; permitted the growth of larger continental ice sheets, which reached a critical size and lengthened the glacial cycles. Our hypothesis supports an important role for abyssal ocean density stratification in the MPT, and requires further testing with additional benthic <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M15" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Mg</mi><mo>/</mo><mi mathvariant="normal">Ca</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="37pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="f61f2ebcf556ab7ba55441a9a818d8bd"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1559-2026-ie00002.svg" width="37pt" height="14pt" src="cp-22-1559-2026-ie00002.png"/></svg:svg></span></span>-<span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O records, numerical model simulations, and forthcoming atmospheric <span class="inline-formula"><i>p</i></span>CO<span class="inline-formula"><sub>2</sub></span&gt; and mean ocean temperature results from the Beyond EPICA&amp;#8211;Oldest Ice core from Antarctica.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-19T21:24:52+02:00</published>
            <updated>2026-08-19T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1537-2026</id>
            <title type="html">Holocene hydroclimatic variability and multi-frequency analyses at Lake Sidi Ali (Morocco)
            </title>
            <link href="https://doi.org/10.5194/cp-22-1537-2026"/>
            <summary type="html">
                &lt;b&gt;Holocene hydroclimatic variability and multi-frequency analyses at Lake Sidi Ali (Morocco)&lt;/b&gt;&lt;br&gt;
                Johannes Schmidt, Markus Reichert, Cathleen Kertscher, Birgit Schneider, Elisabeth Dietze, Laura Bergmann, Abdelfattah Benkaddour, Abdeslam Mikdad, Sylvain Pichat, William Fletcher, Steffen Mischke, and Christoph Zielhofer&lt;br&gt;
                    Clim. Past, 22, 1537&#8211;1557, https://doi.org/10.5194/cp-22-1537-2026, 2026&lt;br&gt;
                This study uses lake sediments from Lake Sidi Ali in Morocco to understand how climate and the surrounding landscape changed over the past 11,000 years. The results show repeating climate patterns that influenced lake water levels and erosion in the catchment at different timescales. These findings help explain how regional climate and local landscape processes interacted at the North African desert margin.
            </summary>
            <content type="html">
                &lt;b&gt;Holocene hydroclimatic variability and multi-frequency analyses at Lake Sidi Ali (Morocco)&lt;/b&gt;&lt;br&gt;
                Johannes Schmidt, Markus Reichert, Cathleen Kertscher, Birgit Schneider, Elisabeth Dietze, Laura Bergmann, Abdelfattah Benkaddour, Abdeslam Mikdad, Sylvain Pichat, William Fletcher, Steffen Mischke, and Christoph Zielhofer&lt;br&gt;
                    Clim. Past, 22, 1537&#8211;1557, https://doi.org/10.5194/cp-22-1537-2026, 2026&lt;br&gt;
                <p>The North African desert margin is considered one of the most sensitive areas to future climate changes, yet the periodicities, coupling mechanisms and external forcing of Holocene environmental variability remain poorly understood. To investigate millennial- to centennial-scale periodicities in Holocene climatic variability and geomorphological processes, we use a Holocene sediment record from Lake Sidi Ali in the semiarid to sub-humid Middle Atlas with a robust <span class="inline-formula"><sup>210</sup></span>Pb&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" 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="527256ea34e0af356380afd605ccefc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1537-2026-ie00001.svg" width="8pt" height="14pt" src="cp-22-1537-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;<span class="inline-formula"><sup>137</sup></span>Cs and pollen-concentrates-based <span class="inline-formula"><sup>14</sup></span>C chronology. We use a high-resolution core scanning-XRF record, in order to distinguish between lake-internal (e.g., chemical precipitation) and lake-external (e.g., detrital input) processes. Redfit and Wavelet time series analyses reveal distinct periodicities of millennial to centennial scale. By a correlation analysis of extracted, highly significant, frequency analysis spectra, three XRF-based &amp;#8220;Redfit Proxy Groups&amp;#8221; (RPGs) which potentially reflect different hydroclimatic forcing mechanisms were derived. Subsequently, we integrated environmental and climatic proxies from the same core (<i>Cedrus</i&gt; pollen abundance, magnetic susceptibility, <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup></span>O and <span class="inline-formula"><i>&amp;#948;</i><sup>13</sup></span>C values of ostracod shells, grain-size endmembers and total organic carbon) and used their wavelet domain to improve the interpretation. Finally, we identified two main periodicity regimes that affected, on the one hand, the hydrological regime and, on the other hand, the lake productivity and catchment erosion dynamics. For RPG 1 (Ca, Sr, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Ca</mi><mo>/</mo><mi mathvariant="normal">Ti</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="31pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="d3badf24d8a286f1058cd2a90bd6a522"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1537-2026-ie00002.svg" width="31pt" height="14pt" src="cp-22-1537-2026-ie00002.png"/></svg:svg></span></span>, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Sr</mi><mo>/</mo><mi mathvariant="normal">Ti</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="28pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="6dd11be51cdfcae6fafdf15a94c26dc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1537-2026-ie00003.svg" width="28pt" height="14pt" src="cp-22-1537-2026-ie00003.png"/></svg:svg></span></span>), we identified 2 and 1&amp;#8201;kyr periodicities, which we interpret as precipitation/evaporation related proxies in the context of North Atlantic and solar forcing. For RPG 2 (Fe, Ti, K, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Si</mi><mo>/</mo><mi mathvariant="normal">Ti</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="27pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="9f51eb8be35d03003e0cb6879d8eb8cc"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1537-2026-ie00004.svg" width="27pt" height="14pt" src="cp-22-1537-2026-ie00004.png"/></svg:svg></span></span>), we observe 3.5 and 1.5&amp;#8201;kyr periodicities, which we interpret as driven by lake productivity or detrital input. Overall, our results show that Holocene environmental variability at Lake Sidi Ali was structured by two partly decoupled regimes: hydroclimatic variability linked to precipitation/evaporation changes and catchment-related variability linked to erosion, productivity and terrestrial sediment supply.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-10T21:24:52+02:00</published>
            <updated>2026-08-10T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1507-2026</id>
            <title type="html">Advancing Last Glacial Maximum paleoclimate reconstructions in Europe using pollen data: a multi-method (mega)biomization approach
            </title>
            <link href="https://doi.org/10.5194/cp-22-1507-2026"/>
            <summary type="html">
                &lt;b&gt;Advancing Last Glacial Maximum paleoclimate reconstructions in Europe using pollen data: a multi-method (mega)biomization approach&lt;/b&gt;&lt;br&gt;
                Gabriel Fénisse, Manuel Chevalier, Odile Peyron, David Vincent Bekaert, and Pierre-Henri Blard&lt;br&gt;
                    Clim. Past, 22, 1507&#8211;1536, https://doi.org/10.5194/cp-22-1507-2026, 2026&lt;br&gt;
                Fossil pollen offers insights into past climates, yet results differ depending on reconstruction methods. By comparing multiple approaches across Europe during the Last Glacial Maximum, we highlight how method choice influences outcomes. Our work introduces a new methodological framework that reduces biases and improves the reliability of climate reconstructions.
            </summary>
            <content type="html">
                &lt;b&gt;Advancing Last Glacial Maximum paleoclimate reconstructions in Europe using pollen data: a multi-method (mega)biomization approach&lt;/b&gt;&lt;br&gt;
                Gabriel Fénisse, Manuel Chevalier, Odile Peyron, David Vincent Bekaert, and Pierre-Henri Blard&lt;br&gt;
                    Clim. Past, 22, 1507&#8211;1536, https://doi.org/10.5194/cp-22-1507-2026, 2026&lt;br&gt;
                <p>Pollen records are among the highest-resolution spatial and temporal proxies for reconstructing past vegetation dynamics, environmental changes and climate variability. Over the past decade, a large variety of methods based on different ecological or mathematical concepts has been used to reconstruct paleoclimatic conditions from pollen assemblages. However, the accuracy of these climate reconstructions strongly depends on the choice of the modern calibration dataset, the taxonomic resolution, and/or the modelling assumptions. The lack of a univocal response still limits the application of pollen-based climate reconstructions to assess key climate changes over multiple time periods especially during the Last Glacial Maximum (LGM, <span class="inline-formula">&amp;#8764;</span>&amp;#8201;23&amp;#8211;19&amp;#8201;ka&amp;#8201;BP). Here, we present a multi-method approach, including the Modern Analogue Technique (MAT), the Weighted Averaging Partial Least Squares regression (WA-PLS) and the probability density function-based Climate REconstruction SofTware (CREST), to reconstruct European climates during the LGM. The quality and performance of our climate reconstructions show strong heterogeneity when based on large calibration datasets encompassing wide climatic and vegetation gradients, making local sampling for climate reconstructions difficult. Instead of sampling the global calibration dataset, we test the effect of the latest biomization and megabiomization methods (local calibrations based on megabiomization approaches) on climate reconstructions by introducing a new biome-based approach. Unlike previous studies, we use the weighted mean of climate variables from all megabiome scores rather than only considering the dominant (i.e., highest score) megabiome. This significantly reduces some of the statistical noise of climate reconstructions, drastically minimizing threshold and non-linear effects associated with megabiome classification changes. With these methodological advancements and our multi-method comparison, we evaluate the uncertainties (RMSEP) of the paleoclimate reconstructions for the LGM in Europe. Across climate reconstruction methods (MAT, WA-PLS and CREST methods), European LGM annual temperatures from the biomization method were on average <span class="inline-formula">6.4&amp;#177;2.0</span>&amp;#8201;&amp;#176;C (mean SD) colder than today, consistent with megabiomization results (<span class="inline-formula">6.8&amp;#177;2.2</span>&amp;#8201;&amp;#176;C colder). Winter temperature (mean temperature of the coldest month, MTCO) results exhibit substantial spatial variability across Europe. Local calibration techniques significantly reduce uncertainties in LGM MTCO reconstructions, but they&amp;#160;remain highly sensitive to the choice of calibration datasets.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-10T21:24:52+02:00</published>
            <updated>2026-08-10T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1499-2026</id>
            <title type="html">Amplified cooling of Snowball Earth from a salt-albedo feedback
            </title>
            <link href="https://doi.org/10.5194/cp-22-1499-2026"/>
            <summary type="html">
                &lt;b&gt;Amplified cooling of Snowball Earth from a salt-albedo feedback&lt;/b&gt;&lt;br&gt;
                Aksel Samuelsberg, Per Kristen Jakobsen, and Martin Rypdal&lt;br&gt;
                    Clim. Past, 22, 1499&#8211;1506, https://doi.org/10.5194/cp-22-1499-2026, 2026&lt;br&gt;
                In this work we implement a feedback mechanism with proposed relevance for Snowball Earth in a simple climate model, a salt-albedo feedback. Our results show that this mechanism could have amplified cooling during the initial phase of Snowball Earth, suggesting it may have played an overlooked role in the climate evolution of Snowball Earth.
            </summary>
            <content type="html">
                &lt;b&gt;Amplified cooling of Snowball Earth from a salt-albedo feedback&lt;/b&gt;&lt;br&gt;
                Aksel Samuelsberg, Per Kristen Jakobsen, and Martin Rypdal&lt;br&gt;
                    Clim. Past, 22, 1499&#8211;1506, https://doi.org/10.5194/cp-22-1499-2026, 2026&lt;br&gt;
                <p>It is believed that the atmospheric circulation on Snowball Earth produced a net ablation zone exposing bare sea ice. Under sufficiently low temperatures, salt begins to precipitate out of sea ice, forming a lag deposit of crystals with high albedo as the ice sublimates. This could have resulted in a salt-albedo feedback that has not previously been included in modeling studies of Snowball Earth. We implement a salt-albedo feedback in a simple climate model and show that, once initiated, this mechanism could have intensified global cooling in the initial phase of Snowball Earth. Our results suggest that salt precipitation may have played a role in shaping the early climate of Snowball Earth.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-06T21:24:52+02:00</published>
            <updated>2026-08-06T21:24:52+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/cp-22-1481-2026</id>
            <title type="html">Permian-Triassic redox shift and its ferruginous aftermath in epicontinental seas
            </title>
            <link href="https://doi.org/10.5194/cp-22-1481-2026"/>
            <summary type="html">
                &lt;b&gt;Permian-Triassic redox shift and its ferruginous aftermath in epicontinental seas&lt;/b&gt;&lt;br&gt;
                Fen Yang, Sen Li, Stephen E. Grasby, David P. G. Bond, Ming Pan, and Yadong Sun&lt;br&gt;
                    Clim. Past, 22, 1481&#8211;1497, https://doi.org/10.5194/cp-22-1481-2026, 2026&lt;br&gt;
                The end-Permian mass extinction was the most severe loss of life in Earth history, yet the role of ocean oxygen restriction remains debated. We examined rock records from South China and western Canada to track redox conditions before and after the crisis. Oxygen levels were already low prior to the extinction, and widespread seafloor anoxia developed at its peak. Afterwards, ferruginous conditions dominated, reducing nutrient availability, limiting productivity, and slowing life&amp;#8217;s recovery.
            </summary>
            <content type="html">
                &lt;b&gt;Permian-Triassic redox shift and its ferruginous aftermath in epicontinental seas&lt;/b&gt;&lt;br&gt;
                Fen Yang, Sen Li, Stephen E. Grasby, David P. G. Bond, Ming Pan, and Yadong Sun&lt;br&gt;
                    Clim. Past, 22, 1481&#8211;1497, https://doi.org/10.5194/cp-22-1481-2026, 2026&lt;br&gt;
                <p>Marine anoxia has been implicated as a key environmental driver of the end-Permian mass extinction (EPME) and the subsequent prolonged recovery. However, the spatial and temporal extent of oxygen limitation during the EPME interval remains contentious. Here, we present iron speciation, pyrite framboid and molybdenum&amp;#8211;uranium (Mo&amp;#8211;U) covariation data from two palaeogeographically distinct settings: the Tethyan Chibi section (South China) and the Panthalassian Ursula Creek section (Western Canada) to evaluate redox dynamics across the Permian-Triassic transition. Our data suggest that bottom waters were predominantly dysoxic during the late Changhsingian at both sites. Later, the prevalence of small pyrite framboids, elevated Mo and U enrichment factors (Mo<span class="inline-formula"><sub>EF</sub></span&gt; and U<span class="inline-formula"><sub>EF</sub></span>), and high Mo<span class="inline-formula"><sub>EF</sub></span>&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="57ee8123d9c9aefcf23d9c7f6463c158"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cp-22-1481-2026-ie00001.svg" width="8pt" height="14pt" src="cp-22-1481-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;U<span class="inline-formula"><sub>EF</sub></span&gt; ratios near the EPME horizon implicate seafloor anoxia as a key trigger for marine extinctions in the Ursula Creek section. In the post-extinction Early Triassic, iron speciation and Mo<span class="inline-formula"><sub>EF</sub></span>&amp;#8211;U<span class="inline-formula"><sub>EF</sub></span&gt; covariation data reveal a shift to persistently ferruginous conditions in both locations. A global compilation of iron speciation data indicates redox variation between ferruginous and euxinic conditions in epicontinental seas during the Permian-Triassic crisis, with ferruginous conditions expanding significantly in the earliest Triassic. The expansion of a ferruginous seafloor would have limited phosphorus bioavailability, suppressing primary productivity in the immediate aftermath of the EPME, thereby contributing to the slow recovery.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-06T21:24:52+02:00</published>
            <updated>2026-08-06T21:24:52+02:00</updated>
        </entry>
</feed>