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      <source-app name="Horizon">Horizon</source-app>
      <rec-number>1</rec-number>
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        <key app="Horizon" db-id="fdi:010094820">1</key>
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      <ref-type name="Journal Article">17</ref-type>
      <work-type>ACL : Articles dans des revues avec comité de lecture répertoriées par l'AERES</work-type>
      <contributors>
        <authors>
          <author>
            <style face="bold" font="default" size="100%">Danielli, Vincent</style>
          </author>
          <author>
            <style face="bold" font="default" size="100%">Lengaigne, Matthieu</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Sadhvi, K.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Gopika, S.</style>
          </author>
          <author>
            <style face="bold" font="default" size="100%">Vialard, Jérôme</style>
          </author>
        </authors>
      </contributors>
      <titles>
        <title>Drivers of CMIP Tropical Pacific warming pattern diversity</title>
        <secondary-title>Earths Future</secondary-title>
      </titles>
      <pages>e2025EF005938 [20 p.]</pages>
      <keywords>
        <keyword>climate change</keyword>
        <keyword>tropical Pacific warming pattern</keyword>
        <keyword>CMIP models</keyword>
        <keyword>ocean dynamics</keyword>
        <keyword>evaporative feedback</keyword>
        <keyword>ocean-atmosphere coupling</keyword>
        <keyword>PACIFIQUE</keyword>
        <keyword>ATLANTIQUE</keyword>
        <keyword>ZONE TROPICALE</keyword>
      </keywords>
      <dates>
        <year>2025</year>
      </dates>
      <call-num>fdi:010094820</call-num>
      <language>ENG</language>
      <periodical>
        <full-title>Earths Future</full-title>
      </periodical>
      <accession-num>ISI:001542366900001</accession-num>
      <number>8</number>
      <electronic-resource-num>10.1029/2025ef005938</electronic-resource-num>
      <urls>
        <related-urls>
          <url>https://www.documentation.ird.fr/hor/fdi:010094820</url>
        </related-urls>
        <pdf-urls>
          <url>https://horizon.documentation.ird.fr/exl-doc/pleins_textes/2025-09/010094820.pdf</url>
        </pdf-urls>
      </urls>
      <volume>13</volume>
      <remote-database-provider>Horizon (IRD)</remote-database-provider>
      <abstract>Anthropogenic changes in sea surface temperature relative to the tropical mean (relative SST) play a pivotal role in influencing atmospheric stability and circulation. In the tropical Pacific, CMIP5/6 multi-model mean (MMM) projections by the end of the 21st century show a southeastern relative cooling and a reduced equatorial SST gradient, although individual models exhibit considerable diversity. Using a simplified heat budget framework, we analyze the processes driving these relative SST changes across 63 CMIP5/6 models under historical and most pessimistic future scenarios. In the southeastern tropical Pacific, MMM relative SST cooling is driven by intensified winds that enhance latent heat flux, with inter-model diversity explained by variations in clouds and winds. Conversely, the MMM equatorial SST gradient reduction arises from reduced evaporative cooling efficiency in the climatologically cold eastern Pacific. A heat budget covariance analysis reveals that inter-model diversity in equatorial Pacific warming is predominantly driven by ocean dynamical processes, challenging previous studies that emphasized cloud feedback mechanisms. Clouds instead mitigate inter-model spread. The inter-model spread in ocean dynamics is linked to two factors: trade wind relaxation and the cold tongue bias. Stronger trade wind relaxation amplifies western Pacific warming, while a weaker cold tongue indicates a less effective ocean thermostat, enhancing eastern Pacific warming. During the present-day period, only a subset of models captures the observed equatorial SST gradient strengthening, but the mechanisms vary across these models, complicating the identification of robust drivers of this observed trend.</abstract>
      <custom6>032 ; 021 ; 020</custom6>
      <custom1>UR248 / UR182</custom1>
      <custom7>Inde</custom7>
    </record>
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