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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESD</journal-id><journal-title-group>
    <journal-title>Earth System Dynamics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Dynam.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2190-4987</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/esd-17-1365-2026</article-id><title-group><article-title>Everyday weather in a warmer world</article-title><alt-title>Everyday weather in a warmer world</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Thomas</surname><given-names>Rhidian</given-names></name>
          <email>r.h.thomas@reading.ac.uk</email>
        <ext-link>https://orcid.org/0000-0003-2309-9843</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Compo</surname><given-names>Gilbert P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>George</surname><given-names>Steve</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0396-0299</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hegerl</surname><given-names>Gabriele C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Schurer</surname><given-names>Andrew</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9176-3622</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Shepherd</surname><given-names>Theodore G.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Slivinski</surname><given-names>Laura C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Thompson</surname><given-names>Vikki</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hawkins</surname><given-names>Ed</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9477-3677</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>National Centre for Atmospheric Science, Department of Meteorology, University of Reading, Reading, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Cooperative Institute for Research in Environmental Sciences, University of Colorado at Boulder, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>NOAA Physical Sciences Laboratory, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>School of GeoSciences, University of Edinburgh, Edinburgh, UK</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Meteorology, University of Reading, Reading, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Rhidian Thomas (r.h.thomas@reading.ac.uk)</corresp></author-notes><pub-date><day>25</day><month>September</month><year>2026</year></pub-date>
      
      <volume>17</volume>
      <issue>5</issue>
      <fpage>1365</fpage><lpage>1380</lpage>
      <history>
        <date date-type="received"><day>3</day><month>May</month><year>2026</year></date>
           <date date-type="rev-request"><day>13</day><month>May</month><year>2026</year></date>
           <date date-type="rev-recd"><day>20</day><month>July</month><year>2026</year></date>
           <date date-type="accepted"><day>31</day><month>August</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Rhidian Thomas et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026.html">This article is available from https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026.html</self-uri><self-uri xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026.pdf">The full text article is available as a PDF file from https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e184">How would the weather of a year from history be experienced in a warmer world? We reconstruct the weather of 1903 using a reanalysis system that assimilates only surface pressure observations (20CRv3) with observed SSTs, and then reconstruct it again with increased SSTs and atmospheric <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels. By assimilating the same pressure observations, the reanalysis experiments produce the same weather patterns, and so we translate the weather of 1903 into a warmer context. We focus on changes in the everyday weather of four regions with a high density of historical pressure observations, where the circulation is constrained and differences between the experiments are due to the thermodynamic component of climate change. In these regions, nearly all days are warmer in the warmer world experiments, but the largest increases occur on cold days (below freezing) and hot days (above 20 °C). Daily rainfall becomes more variable, even in regions where total rainfall is reduced. Fewer days experience light rain while more days experience heavy rain, and rainfall only increases on less than 1 d in 10. This single year pair of reanalysis experiments also recovers common patterns of observed and projected long-term changes. For example, Western Mediterranean precipitation declines outside winter, but shows a small increase in winter in the absence of storm track shifts. By anchoring our analysis in weather patterns that have actually occurred, the reanalysis experiments point to how our day-to-day experience of the same weather patterns may change in a warmer world, even if the weather patterns themselves do not.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Natural Environment Research Council</funding-source>
<award-id>NE/Z000203/1</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Research Ireland</funding-source>
<award-id>22/CC/11103</award-id>
</award-group>
<award-group id="gs3">
<funding-source>National Oceanic and Atmospheric Administration</funding-source>
<award-id>NA22OAR4320151</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e207">Climate change is affecting the frequency and intensity of extreme weather, with implications for infrastructure adaptation and human health <xref ref-type="bibr" rid="bib1.bibx60" id="paren.1"/>. Over the 21st century, progress has been made in attributing the influence of climate change on individual extreme weather events <xref ref-type="bibr" rid="bib1.bibx65 bib1.bibx42 bib1.bibx12" id="paren.2"/>. However, while much attention has focused on extreme weather, less focus has been given to how climate change will affect the experience of everyday, non extreme weather. Though extreme weather is impactful, and can contribute disproportionately to the mean <xref ref-type="bibr" rid="bib1.bibx44" id="paren.3"/>, by definition it represents weather on only a small number of days. Previous work has considered how climate change has and will affect the occurrence of mild weather <xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx34 bib1.bibx79" id="paren.4"/> and the closely related concept of “outdoor days” <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx11" id="paren.5"/>, defined variously as days with comfortable near-surface temperature and/or clear skies and minimal precipitation. Model projections broadly show an increase in mild conditions in the mid-high latitudes and a decrease in the tropics <xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx11" id="paren.6"/>, albeit with substantial regional variation. However, regional projections of temperature and precipitation depend on uncertain future changes in large-scale weather patterns <xref ref-type="bibr" rid="bib1.bibx62" id="paren.7"/>.</p>
      <p id="d2e232">A different approach is to consider how the thermodynamic aspects of climate change – those related to rising temperature and humidity – will affect day-to-day weather, given no change in weather patterns. Those effects represent the most robust aspects of regional climate change. We adopt a storyline approach <xref ref-type="bibr" rid="bib1.bibx63" id="paren.8"/> to explore changes in the weather of a year from history. <xref ref-type="bibr" rid="bib1.bibx22" id="text.9"/> reconstructed an extreme event from 1903, Storm Ulysses, in an atmospheric reanalysis system, and translated its impacts into a warmer world. Using the same experiments, as well as an additional novel reanalysis experiment described below, we present a broader survey of changes across the 12 months of 1903. The weather from all 12 months of 1903 is first reconstructed using an atmospheric reanalysis system that assimilates observations of atmospheric pressure (including rescued pressure observations not available in the production version of the reanalysis) and uses observed SSTs and sea ice concentrations as lower boundary conditions <xref ref-type="bibr" rid="bib1.bibx64" id="paren.10"/>. Then, the model and data assimilation system are completely re-run while assimilating the same pressure observations, but altering the SST boundary conditions and atmospheric <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in order to translate the historical weather into a warmer world. As the same pressure observations are assimilated in each experiment, the experiments experience the same weather patterns, minimising uncertainty due to projected changes in atmospheric circulation. We then explore how the thermodynamic impacts of day-to-day weather differ in a warmer and moister atmosphere. For example, in the absence of circulation changes, how does a given ocean warming affect the distribution of daily temperature? Do cold days and hot days warm by the same amount? Does rainfall become more or less frequent, and more or less variable from day to day?</p>
      <p id="d2e255">Our approach is similar to other storyline attribution methods, such as nudging experiments where the large-scale winds are relaxed towards specified values <xref ref-type="bibr" rid="bib1.bibx76 bib1.bibx72 bib1.bibx54 bib1.bibx17" id="paren.11"/>, and  the pseudo global warming (PGW) method, where the boundary conditions for regional climate models (RCMs) are adjusted to reflect the effects of climate change <xref ref-type="bibr" rid="bib1.bibx57 bib1.bibx6 bib1.bibx33" id="paren.12"/>. These adjustments, often referred to as PGW “deltas”, are chosen such that the imposed dynamical driving at the RCM boundaries is unchanged in the warmer world simulation. Similarly to the reanalysis experiments, there is no change in intraannual variability between the control and “counterfactual” (nudged or PGW) simulations, which allows robust signals to be extracted from shorter simulations than are typically required with free-running climate models <xref ref-type="bibr" rid="bib1.bibx56" id="paren.13"/>. The main differences between these two methods are in how the circulation is constrained: in PGW, typically the 3D dynamics are imposed only at the edge of the RCM domain, while large-scale nudging can be performed globally or across a smaller regional domain in the free troposphere <xref ref-type="bibr" rid="bib1.bibx76 bib1.bibx72" id="paren.14"/>; in the reanalysis experiments, the synoptic circulation at the surface is constrained through the assimilation of surface pressure observations. Long historical records of surface pressure and SST observations allow the reanalysis approach to study periods that occurred before the advent of widespread upper-air observations in the mid-20th century. As in some nudged simulations, the reanalysis experiments are also global, allowing multiple locations to be studied in a single run. The reanalysis experiments in this paper thus offer an additional and computationally efficient line of evidence regarding the thermodynamic effects of warming on regional weather and climate.</p>
      <p id="d2e270">We begin by describing the reanalysis system and assimilated pressure data before presenting a global overview of changes in the warmer world experiments. The available pressure observations from 1903 are not distributed evenly in space, which restricts the regions we can study in detail using this approach for this particular year. We therefore focus on four regions with a high density of pressure observations in 1903. Our results are summarised in the final section.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Reanalysis experiments</title>
      <p id="d2e281">We reconstruct the weather of 1903 using the NOAA-CIRES-DOE 20th Century Reanalysis version 3 data assimilation system (20CRv3, <xref ref-type="bibr" rid="bib1.bibx64" id="altparen.15"/>). Using an Ensemble Kalman Filter, 20CRv3 assimilates observed pressure values with a NOAA atmospheric model to provide a best estimate of the atmospheric state at each point in time. The atmospheric model used is the NOAA GFS v14.0.1. The atmospheric model is coupled to the Noah land surface model, which incorporates a 4-layer soil model and dynamic fractional snow cover <xref ref-type="bibr" rid="bib1.bibx16" id="paren.16"/>. An 80-member ensemble of 3-hourly atmospheric fields is produced on a 0.7° Gaussian grid. SSTs and sea ice concentrations are prescribed from observed values. The system assimilates pressure observations taken over land and ocean as well as tropical cyclone central pressures from best-track datasets (see <xref ref-type="bibr" rid="bib1.bibx64" id="altparen.17"/>, for details of the boundary conditions and pressure observations).</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e295">Available pressure observations for the 1903 reanalysis experiments. Red circles denote land stations, blue dots denote pressure observations from ships, and orange crosses denote tropical cyclone best-track pressures. Blue boxes show well-observed regions used for analysis in later sections. 97.1 % of all pressure observations in 1903 were successfully assimilated in the 20CRv3<sup>+</sup> experiment. Note that some land stations have multiple observations per day and some have fewer.</p></caption>
        <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f01.png"/>

      </fig>

      <p id="d2e313">We present results from three reanalysis experiments. The first experiment, denoted 20CRv3<sup>+</sup>, is identical to the improved reanalysis in <xref ref-type="bibr" rid="bib1.bibx22" id="text.18"/>. It consists of a reconstruction of 1903 using the same SST and radiative forcings as in the production version of 20CRv3, with two further changes: a refinement of the data assimilation scheme, and the inclusion of many additional rescued pressure observations over Europe. These changes sharpen features of the weather fields and improve the utility of the reconstructions; see the appendices of <xref ref-type="bibr" rid="bib1.bibx22" id="text.19"/> for details. Figure 1 shows the pressure observations used in the 20CRv3<sup>+</sup> experiment. Some regions are much richer in historical pressure observations than others. We expect the atmospheric circulation to be better constrained in these regions than in regions with fewer pressure observations, and so we focus most of our analysis on four regions with a high density of observations in 1903, shown by the blue boxes in Fig. 1. These regions cover northwestern Europe (NW_Europe), the western Mediterranean (Western_Med), the East Coast of the US (US_East_Coast), and Southeastern Australia (SE_Aus).</p>
      <p id="d2e341">In addition to 20CRv3<sup>+</sup>, two further experiments are performed to translate the weather of 1903 into a warmer world. The first, denoted <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K, is as in <xref ref-type="bibr" rid="bib1.bibx23" id="text.20"/>: a uniform <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K perturbation is added to the SSTs, with radiative forcings kept at 1903 values. In the second, denoted <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M10" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, in addition to the <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K SST perturbation, global atmospheric <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration is increased to 530 ppm. Differences between the two warmer world experiments therefore indicate the direct role of the <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radiative forcing. Sea ice boundary conditions are unchanged in the warmer world experiments compared to 20CRv3<sup>+</sup>. Sensitivity tests suggest that this can cause spurious signals near the ice edge, but these effects do not extend far from the ice edge due to the strong constraint of prescribed SSTs and the assimilation of pressure observations (not shown). The SST, <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and sea ice conditions are idealised and do not reflect observed or projected patterns of change – they are chosen to illustrate the role of ocean warming and atmospheric composition on the weather of 1903 in a simple way. In both experiments, the same pressure observations are assimilated as in 20CRv3<sup>+</sup>, so that the atmospheric flow is similarly constrained in all three experiments; we thus isolate the thermodynamic impacts of the perturbations on the reconstructed weather of 1903. We analyse 12 months of data (from January to December 1903) in each experiment. Each warmer world experiment is spun up for 6 months prior to January 1903 to allow the atmosphere to adjust to the perturbed boundary conditions. The 20CRv3<sup>+</sup> and <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiments are as in <xref ref-type="bibr" rid="bib1.bibx22" id="text.21"/> and <xref ref-type="bibr" rid="bib1.bibx23" id="text.22"/>, while the <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M21" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment is novel.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e523">Time series of 3-hourly 2 m-temperature (dotted line) and precipitation rate (solid line) averaged over central England (3–0° W, 51.5–54.0° N, see boxed region in Fig. 8). The 20CRv3<sup>+</sup> experiment is in black and the <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M25" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment is in red (see Fig. S1 in the Supplement for the <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment). Lines show the ensemble-means and shading denotes the 10 %–90 % range across the ensemble. Blue markers show daily-mean temperatures from the Central England Temperature (CET) series <xref ref-type="bibr" rid="bib1.bibx31" id="paren.23"/>, plotted at 09:00 UTC each day. Vertical bars on each marker indicate the CET daily maximum and minimum temperatures. The grey dashed line in the top panel indicates the air frost threshold (0 °C).</p></caption>
        <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f02.png"/>

      </fig>

      <p id="d2e583">An example of everyday weather in a well-observed region is shown in Fig. 2, which shows 3-hourly time series of 2 m-temperature and precipitation in 20CRv3<sup>+</sup> and the <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M30" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M31" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment averaged over Central England (the boxed area in Fig. 8b–d) for January and July 1903. The equivalent plots for the <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment are shown in Fig. S1 in the Supplement. Temperatures in 20CRv3<sup>+</sup> are in good agreement with observed daily values from the Central England Temperature series (CET) <xref ref-type="bibr" rid="bib1.bibx31" id="paren.24"/>, which represents observed average temperatures over a similar region. As no temperature observations are assimilated, this comparison provides an independent verification of the reanalysis skill in reproducing observed weather in this region. The warmer world simulations show day-to-day fluctuations in temperature and precipitation in phase with those of 20CRv3<sup>+</sup>, which indicates that the synoptic circulation is well constrained by the assimilated observations (the experiments experience the “same” weather). Temperatures in the warmer world experiments are consistently warmer than in 20CRv3<sup>+</sup>, with little overlap between the 20CRv3<sup>+</sup> and warmer world ensemble shading, especially in January. The grey dashed line in the top panel indicates the air frost threshold (0 °C). Eight nights in the 20CRv3<sup>+</sup> ensemble-mean dip below this threshold, while only five do in the <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M39" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M40" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment – a reduction of 60 % in this small sample. For comparison, the annual number of air frost days in the UK has declined by around a quarter since the 1980s <xref ref-type="bibr" rid="bib1.bibx27" id="paren.25"/>.  Precipitation peaks in the warmer world experiments generally line up with those in 20CRv3<sup>+</sup>, though rainfall is less well constrained by the assimilated pressure observations than is near-surface temperature.</p>
      <p id="d2e723">In addition to Central England, we also show a version of Fig. 2 for a region over northern Patagonia with far fewer nearby land-based pressure stations (Fig. S2, the green boxed region in Fig. 1). Day-to-day variations in temperature and precipitation are surprisingly similar in both experiments, despite the much weaker observational constraint than over Central England (Fig. 1). Although we restrict most of the later analysis to well-observed regions, Fig. S2 suggests that even a small number of nearby observations (from ships in this case) can constrain the circulation relatively well in the reanalysis system. This is particularly noteworthy given that the markers in Fig. 1 represent observations across all of 1903; within a single assimilation window, the density of ship-based observations will be much lower than that shown in Fig. 1.</p>
      <p id="d2e726">Focusing on the year 1903 allows us to exploit the existing reanalysis experiments of <xref ref-type="bibr" rid="bib1.bibx23" id="text.26"/>. Globally, 1903 was a cold year: it is the 3rd coldest in the 175-year HadCRUT5.1 dataset <xref ref-type="bibr" rid="bib1.bibx39" id="paren.27"><named-content content-type="post">Fig. S3a</named-content></xref>, and it is in at least the coldest third of years in each of the four well-observed regions we analyse in later sections (the lowest rank is 57th/175 in NW_Europe, i.e. 32nd percentile; Fig. S3b–e). The eruption of the Santa Maria volcano in October 1902 – one of the largest tropical volcanic eruptions of the century <xref ref-type="bibr" rid="bib1.bibx53" id="paren.28"/> – presumably contributed to the generally cool conditions <xref ref-type="bibr" rid="bib1.bibx58" id="paren.29"/>. Note that the volcanic aerosol forcing is identical in all of our experiments. The cold baseline conditions in 1903 mean that the perturbed climates in the warmer world experiments are not much warmer than some of the later years in the original 20CRv3 dataset, for which the system's performance has been validated. This builds confidence in the ability of the reanalysis system to plausibly represent the warmer world climates in our experiments.</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e746">Globally and annually averaged 2 m-temperature <bold>(a)</bold>, total-column precipitable water (PWAT) <bold>(b)</bold>, and precipitation rate <bold>(c)</bold> in the reanalysis experiments. Curves show the density of values across the 80 ensemble members in each experiment.</p></caption>
        <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f03.png"/>

      </fig>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e766">Annual-mean changes in 2 m-temperature <bold>(a–c)</bold> and precipitation <bold>(d–f)</bold> between the reanalysis experiments. Changes are shown as differences between experiments for temperature, and as percentage changes between experiments for precipitation. The value at the top right of each plot is the global (area-weighted) average of the changes at each gridpoint (note that this is different to the changes in the global-mean shown in Fig. 3). Hatching obscures non-significant changes at the 5 % level using a two-tailed Student's <inline-formula><mml:math id="M42" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test. The colour bar in panels <bold>(a)</bold>–<bold>(b)</bold> is centred on a change of <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K as this is the perturbation applied to the SSTs.</p></caption>
        <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f04.png"/>

      </fig>

</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Overview of global changes</title>
      <p id="d2e813">Before focusing on regional aspects, we first present a global overview of changes in the warmer world experiments. Figure 3 shows globally and annually averaged 2 m-temperature, precipitable water (PWAT) and precipitation rate in each experiment. The distributions show the spread of values across the 80 ensemble members. The spatial patterns of the ensemble-mean temperature and precipitation changes are shown in Fig. 4. As seen in Fig. 3a, globally, the <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiments are 2.1 K warmer than 20CRv3<sup>+</sup> in the ensemble-mean, with the additional 0.1 K of warming arising due to enhanced warming over land (Fig. 4a). This highlights the prominent role of oceanic warming in driving continental temperatures, even in the absence of changes in <inline-formula><mml:math id="M46" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> forcing, such as through the moistening of continental air and hence enhanced downwelling longwave (LW) radiation over land <xref ref-type="bibr" rid="bib1.bibx13" id="paren.30"/>. Interestingly, however, we also find an important role for direct <inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-induced warming, with a further 0.2 K of global warming in the <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M49" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M50" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment due to additional enhanced warming over extratropical land (Fig. 4b). This corresponds to a larger global land/ocean warming ratio (1.35 in <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M52" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, compared to 1.21 in <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K). Both warming ratio values are notably smaller in the warmer world experiments than in climate models and observations <xref ref-type="bibr" rid="bib1.bibx67 bib1.bibx13 bib1.bibx7" id="paren.31"><named-content content-type="pre">e.g.</named-content></xref>; the warmer world experiments are idealised and differ from observed climate change in several ways, including the uniform SST increase and the lack of changes in other forcing agents such as tropospheric aerosols (which are constant at modern day levels in 20CRv3), so we would not expect the ratios to match the real world values precisely. Another idealised design choice is the unchanged sea ice fields in the warmer world experiments, which is likely the reason for the weak Arctic warming in Fig. 4a. Keeping sea ice fixed in the warmer world experiments will result in a smaller increase in global-mean temperatures than if more plausible reductions in sea ice concentration had been specified (Fig. 3a). Enhanced warming also occurs over regions of high elevation including the Andes and Himalayas (Fig. 4a–b), consistent with thermodynamic mechanisms such as a reduction in snow albedo and Planck feedbacks <xref ref-type="bibr" rid="bib1.bibx49" id="paren.32"/>. The direct <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-induced warming is small over tropical land (Fig. 4b–c), likely due to masking of its radiative forcing by high clouds and upper-tropospheric water vapour <xref ref-type="bibr" rid="bib1.bibx37" id="paren.33"/>. It has a larger warming effect in the extratropics, particularly over arid regions such as the Sahara and the Western US. In the latter region, additional warming of 0.6 K or more is seen due to the higher <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels, which is around a fifth of the total warming in the <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M58" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M59" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> runs. This is likely to be a purely radiative consequence of the <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> forcing, as the high density of pressure observations in the Western US will strongly constrain the circulation in each experiment (Fig. 1). Thus, even in the absence of circulation changes, the direct warming effect of atmospheric <inline-formula><mml:math id="M61" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> varies regionally and can be large in the extratropics.</p>
      <p id="d2e1012">Higher surface temperatures are associated with increased atmospheric moisture content in the warmer world experiments, as seen in globally averaged precipitable water (PWAT, Fig. 3b). The PWAT increases follow the same ordering as the temperature distributions. Accounting for the additional warming in the <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M63" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> runs, the relative increase in PWAT is similar in both experiments and is broadly in line with Clausius-Clapeyron scaling at 8.5 % K<sup>−1</sup> and 8.2 % K<sup>−1</sup> respectively <xref ref-type="bibr" rid="bib1.bibx70 bib1.bibx43 bib1.bibx74" id="paren.34"/>.</p>
      <p id="d2e1071">Global precipitation also increases in the warmer world simulations (Fig. 3c), but more slowly than atmospheric moisture. Latent heating from precipitation is balanced globally by LW cooling of the atmosphere, which increases as the surface and atmosphere warm. This explains why a smaller precipitation increase is seen in the <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M68" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment than in <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K, despite a larger increase in atmospheric moisture: additional <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reduces LW emission to space and thus a smaller increase in precipitation is required to balance it. Hence, in isolation, the higher <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration acts to blunt the precipitation increase that arises due to surface warming <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx46" id="paren.35"/>. The increase of 2.4 % K<sup>−1</sup> in the <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M75" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment is notably similar to values seen in climate model experiments <xref ref-type="bibr" rid="bib1.bibx2" id="paren.36"/>, despite the lack of strict energy conservation in the reanalysis system due to the inclusion of analysis increments.</p>
      <p id="d2e1182">The spatial pattern of precipitation change is shown in Fig. 4d–e. In many respects, the pattern of change in the warmer world simulations resembles the canonical projected response to greenhouse warming in comprehensive climate models <xref ref-type="bibr" rid="bib1.bibx59 bib1.bibx30" id="paren.37"/>, despite the specificity of the 1903 SST boundary conditions and atmospheric circulation. Precipitation increases over much of the extratropics, while drying is seen over the Mediterranean and subtropical ocean basins. Precipitation intensity over land increases everywhere, but land areas including Africa, the western US, and Mediterranean experience fewer wet days (Fig. S4). Much of the drying over subtropical oceans is due to the inclusion of <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 4f), which may reflect a shift of convection from ocean to land in association with the enhanced land warming driven by increased <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx24" id="paren.38"/>. The sparse observations over much of the tropics mean that the atmospheric circulation is less constrained in these regions; in the following sections, we therefore focus on changes in the four well-observed regions identified in Fig. 1.</p>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Regional changes in everyday weather</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Temperature changes</title>
      <p id="d2e1228">Annual-mean temperatures in the warmer world experiments are consistently higher than in 20CRv3<sup>+</sup>. But do cool and warm days change by the same amount? Figure 5 shows the pairwise change in near-surface temperature in the warmer world experiments compared to 20CRv3<sup>+</sup>, as a function of the 20CRv3<sup>+</sup> daily-mean temperature, for the four well-observed regions indicated in Fig. 1.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e1260">Change in ensemble-mean, daily-mean 2 m-temperature in the warmer world experiments versus 20CRv3<sup>+</sup>, as a function of temperature percentile in 20CRv3<sup>+</sup>. The pairwise difference between experiments is calculated for every (lat, lon, day) pair and is then binned according to the temperature value of that (lat, lon, day) in 20CRv3<sup>+</sup>. Solid lines show the mean difference in each bin. The blue dotted line shows the pairwise difference between the <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M86" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M87" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiments (again binned according to 20CRv3<sup>+</sup> temperature). Only land gridcells are used. The horizontal dashed line indicates a change of <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> °C and the vertical dotted lines show absolute temperatures in 20CRv3<sup>+</sup>.</p></caption>
          <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f05.png"/>

        </fig>

      <p id="d2e1363">Fewer than 1 % of points in each bin become cooler in the <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K or <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M94" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiments compared to 20CRv3<sup>+</sup> (not shown). In the <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment, temperatures increase by 2–2.5 °C on what could be considered typical days in each region (between the 20th and 80th percentiles of daily temperature in 20CRv3<sup>+</sup>). Higher <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M101" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment leads to a roughly constant additional warming of 0.2–0.4 °C on these days. However, three of the four regions show much larger temperature increases on cold days (particularly days below freezing; Fig. 5a–c) in both the <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K and <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M105" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiments. Analysis of the surface heat budget reveals a reduction in the fraction of solar radiation that is reflected by the land surface on days below 5 °C in these regions (Fig. S5), likely due to reduced snow cover. Thus, in the warmer world simulations, proportionally less sunlight is reflected by snow and more is absorbed by the darker land surface, leading to amplified warming of cold days. The lack of cold-day amplification in SE_Aus (Fig. 5d) is consistent with the low occurrence of freezing temperatures.</p>
      <p id="d2e1512">Amplified warming is also seen for the hottest days in the Western_Med, US_East_Coast, and SE_Aus regions, with increases of 3 °C or more on days above 30 °C (Fig. 5b–d). In all regions, an increase in evaporative cooling is seen in the <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment for days below the 70th percentile (Fig. S5); however, for the hottest days, the evaporative cooling increase is smaller. In the US East Coast region, the sign reverses, with a sharp reduction in evaporative cooling seen in the <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment for days above the 97th percentile of temperature (Fig. S5c). Negative soil moisture anomalies can amplify heat waves, as the land surface is less able to lose heat through evaporation <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx18" id="paren.39"/>. This suggests that the hottest days in the US_East_Coast region are days with low soil moisture and thus reduced ability for the land surface to cool evaporatively, leading to larger increases in near-surface air temperature. In the Western_Med, evaporative cooling is also reduced on days above approximately the 70th percentile of temperature, but not on the very hottest days (matching the weaker amplification of warming in the <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment on these days). Changes in latent heat flux contribute less to amplified warming of hot extremes in NW_Europe – perhaps indicating that the hottest days are less limited by soil moisture – and in SE_Aus, where the amplification of hot extremes appears related to reduced cloud cover and increased warming from incident solar radiation <xref ref-type="bibr" rid="bib1.bibx13" id="paren.40"/>.</p>
      <p id="d2e1551">Heat waves and cold spells as experienced in nature often coincide with particular atmospheric circulation patterns, such as the well-known relationship between cold air outbreaks over Northern Europe and the negative phase of the North Atlantic Oscillation <xref ref-type="bibr" rid="bib1.bibx66" id="paren.41"/>. Long-lived anticyclones in the summer months can similarly lead to heat waves in the extratropics <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx75" id="paren.42"/>. Feedbacks between the atmospheric circulation and land surface can also precondition the land surface in ways that amplify hot extremes, such as by reducing soil moisture in the months prior to a heatwave <xref ref-type="bibr" rid="bib1.bibx18" id="paren.43"/>. Changes in the number of hot and cold days can, in general, be due to changes in the occurrence of such persistent weather patterns, in addition to the direct thermodynamic effects of increased radiative forcing. The reanalysis experiments suggest that, even if large-scale weather patterns remain unchanged, daily cold and hot extremes will experience amplified warming in a warmer world. This highlights the role of land surface feedbacks in addition to the atmospheric circulation in amplifying extreme heat events <xref ref-type="bibr" rid="bib1.bibx75" id="paren.44"/>.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Precipitation changes</title>
      <p id="d2e1574">Next we analyse how the global precipitation changes in Figs. 3 and 4 compare to changes in the well-observed regions. Additionally, are changes in mean precipitation accompanied by changes in variability? Figure 6a–d show the change in mean precipitation and daily precipitation variability in <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M111" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compared to 20CRv3<sup>+</sup> for our selected regions. The global increase in annual-mean precipitation is also seen in the NW_Europe, US_East_Coast, and SE_Aus regions. The distribution spread is notably wider in SE_Aus than in the other regions, which may reflect the lower observation density (Fig. 1) and hence more weakly constrained circulation.</p>

      <fig id="F6"><label>Figure 6</label><caption><p id="d2e1616"><bold>(a–d)</bold> percentage changes in mean and variability of daily precipitation in the <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M115" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M116" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment compared to 20CRv3<sup>+</sup> across the whole year. Variability is calculated as the standard deviation of daily precipitation. The dashed grey lines indicate the local Clausius-Clapeyron scaling at 7 % K<sup>−1</sup>. <bold>(e–h)</bold> Changes in mean Western_Med precipitation in each season compared to 20CRv3<sup>+</sup>. Each quantity is calculated at each grid cell before being averaged over the region, using all 12 months in each experiment. Only land grid cells are used. The violin bodies show the range of changes possible by resampling the 80 ensemble members in each experiment, and the horizontal violin bars indicate the median, 5th and 95th percentiles.</p></caption>
          <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f06.png"/>

        </fig>

      <p id="d2e1689">In contrast to the other regions, mean precipitation declines in Western_Med. This is consistent with climate model experiments which show a reduction in Mediterranean precipitation in response to anthropogenic forcing. Observations also show a decline in Mediterranean precipitation, although at present the forced signal may be difficult to distinguish from multidecadal variability <xref ref-type="bibr" rid="bib1.bibx73" id="paren.45"/>. In models, precipitation reduction is often associated with poleward expansion of the subtropical dry zones leading to fewer Mediterranean cyclones <xref ref-type="bibr" rid="bib1.bibx78 bib1.bibx77" id="paren.46"/>, which is not represented in our experiments. Changes in large-scale circulation are more important in winter <xref ref-type="bibr" rid="bib1.bibx5" id="paren.47"/>, whereas the summer precipitation response is due mainly to thermodynamic factors such as changes in humidity and the land/sea warming contrast <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx3" id="paren.48"/>. We find that the annual-mean change in Fig. 6b is due to reduced rainfall outside winter (Fig. 6f–h), with little change in DJF (Fig. 6e). The reanalysis experiments therefore suggest that local thermodynamic factors can drive a reduction in annual-mean precipitation over the Western Mediterranean, even in the absence of large-scale circulation changes. Figure 6e–h also show that, while the SST warming causes a small increase in winter rainfall but a decrease in the other seasons, the additional <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M122" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiments always reduces rainfall in our experiments regardless of season. As the SSTs are the same in both warmer world experiments, the main effect of the <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is to enhance land warming at the expense of the ocean, potentially leading to reduced relative humidity over land and reduced precipitation.</p>
      <p id="d2e1756">Despite a decline in total precipitation, daily precipitation variability increases in Western_Med as well as in all other regions, meaning the warmer world experiences larger swings in rainfall from day to day (Fig. 6a–d). An increase in precipitation variability is consistent with modelling and theory <xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx80" id="paren.49"/> and with trends emerging in observations <xref ref-type="bibr" rid="bib1.bibx81" id="paren.50"/>. Variability increases more than the mean in each region, but by less than the availability of moisture as defined by the local Clausius-Clapeyron scaling (grey dashed lines in Fig. 6a–d). Precipitation is proportional to the product of moisture and vertical motion <xref ref-type="bibr" rid="bib1.bibx55" id="paren.51"/> and so, for fixed vertical motion, precipitation variability scales with moisture availability <xref ref-type="bibr" rid="bib1.bibx48" id="paren.52"/>. Thus, the lower rate of increase in the warmer world experiment indicates a change in the distribution of vertical motion <xref ref-type="bibr" rid="bib1.bibx45" id="paren.53"/>. This suggests that, although the synoptic circulation in the reanalysis experiments is constrained by the pressure assimilation, there is some flexibility for the statistics of vertical velocity to change, which may explain why the precipitation amplification in Fig. 2 is less robust than the temperature response.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e1776">Precipitation characteristics of the NW_Europe <bold>(a–c)</bold> and Western_Med <bold>(d–f)</bold> regions. <bold>(a, d)</bold> Number of dry days, defined as days experiencing less than 1 mm of rain (here 1.04 mm due to numerical rounding). The median is shown by the horizontal line and the violin shows the distribution of ensemble members. <bold>(b, e)</bold> Daily precipitation occurrence in 20CRv3<sup>+</sup> and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M127" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M128" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The blue line shows the percentage change in each bin in <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M130" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Error bars show the 10 %–90 % range through sampling all combinations of ensemble members, and vertical dashed lines show percentiles of the precipitation distribution in 20CRv3<sup>+</sup>. <bold>(c, f)</bold> Ratio of large event cutoff <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi>s</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M135" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vs 20CRv3<sup>+</sup> (see text). Only land gridcells are used for all calculations. Bins in <bold>(b)</bold> and <bold>(e)</bold> are logarithmically distributed with the smallest nonzero bin centred at 1.11 mm d<sup>−1</sup> and successive bin widths increasing by 14.7 %.</p></caption>
          <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f07.png"/>

        </fig>

      <p id="d2e1943">Daily precipitation densities in the 20CRv3<sup>+</sup> and <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M141" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiments are shown by the grey and red points, respectively, in Fig. 7b and e. The curves follow a similar shape in both NW_Europe and Western_Med (the other regions are shown in Fig. S6), which approximately follow a gamma distribution <xref ref-type="bibr" rid="bib1.bibx36" id="paren.54"/>:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M143" display="block"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>∝</mml:mo><mml:msup><mml:mi>s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:msup><mml:mi>exp⁡</mml:mi><mml:mo mathsize="1.1em">[</mml:mo><mml:mi>s</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>s</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo mathsize="1.1em">]</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M144" display="inline"><mml:mi>s</mml:mi></mml:math></inline-formula> is daily precipitation size, <inline-formula><mml:math id="M145" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is a power law exponent, and <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msub><mml:mi>s</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a cutoff scale beyond which occurrence falls exponentially. Warming leads to an increase in <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi>s</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and therefore larger relative increases in the occurrence of heavier precipitation <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx36" id="paren.55"/>. We find <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi>s</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> increases approximately in line with Clausius-Clapeyron scaling in our regions (Figs. 7c and f, and S3c and f). However, this does not mean that the number of days with heavy precipitation also increases by 7 % K<sup>−1</sup>: instead, the increase is exponential with precipitation rate, as can be seen from the blue curves in Fig. 7b and e which show the percentage change for each precipitation bin. The number of days with moderate to heavy rainfall – above the 90–95th percentile of all days in 20CRv3<sup>+</sup> – increases exponentially with precipitation rate in the warmer world.</p>
      <p id="d2e2102">On the other hand, the number of days with light to moderate rainfall (below the 90–95th percentile in 20CRv3<sup>+</sup>) decreases slightly in the <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M153" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M154" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment. The magnitude of these changes is smaller than at heavy rain rates and the sign of change is more uncertain, however the ensemble-mean values show similar characteristics in all four regions (see also Fig. S6b and e). This highlights the counterintuitive point, made previously by <xref ref-type="bibr" rid="bib1.bibx2" id="text.56"/>, that the time-mean precipitation increases seen in previous figures (Figs. 3, 4, 6) occur only on less than 1 d in 10, with most wet days actually becoming drier in the warmer world experiments.</p>
      <p id="d2e2145">The number of dry days in each experiment is shown in Figs. 7a, d, S4a and d, defined as days experiencing less than 1 mm of rain as in previous studies <xref ref-type="bibr" rid="bib1.bibx52 bib1.bibx15" id="paren.57"><named-content content-type="pre">here 1.04 mm due to numerical rounding;</named-content></xref>. The number of dry days also increases in three of the four regions in <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M156" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M157" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, with the exception of SE_Australia. The additional <inline-formula><mml:math id="M158" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> appears to be an important factor for dry days over NW_Europe and Western_Med, but not over US_East_Coast and SE_Australia. Previous studies have also found an increase in the number of dry days in warmer world experiments <xref ref-type="bibr" rid="bib1.bibx52" id="paren.58"/>, as is also seen on the global scale in the reanalysis experiments (Fig. S4a–c). One possible mechanism for this is a reduction in relative humidity over land leading to increased convective inhibition (CIN) and hence longer intervals between convective events <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx8" id="paren.59"/>, although convective precipitation is likely to be less well constrained by the assimilated pressure observations than rain associated with frontal systems.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>October 1903: an extreme month</title>
      <p id="d2e2209">An advantage of the counterfactual reanalysis experiments is the ability to look at changes in climate impacts over a variety of timescales, as the assimilation process means weather patterns in the warmer world counterfactuals remain close to the original (factual) reanalysis. While short, intense weather events can lead to acute damages, extreme months or seasons, or even sequences of seasons, can also be significant for sectors such as agriculture <xref ref-type="bibr" rid="bib1.bibx41" id="paren.60"/>. Here we present an example of an event falling between the annual timescales discussed in previous sections and the synoptic timescales that are typically the subject of storyline attribution studies.</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e2217">October rainfall in <bold>(a)</bold> observations (HadUKGrid at 60km resolution <xref ref-type="bibr" rid="bib1.bibx26" id="paren.61"/>) and <bold>(b–d)</bold> the reanalysis experiments. The value in the top right of panel <bold>(b)</bold> is the average rainfall over the UK and Ireland in 20CRv3<sup>+</sup>. The corresponding increase compared to 20CRv3<sup>+</sup> is shown in the top right of panels <bold>(c)</bold> and <bold>(d)</bold>. Panel <bold>(e)</bold> shows daily rainfall over Central England (the red boxed region, also used in Fig. 2; using reanalysis data from 09:00–09:00 UTC to match the observational definition). Shading shows the 10 %–90 % range across the ensemble and grey dashed lines indicate all-year daily rainfall percentiles in 20CRv3<sup>+</sup> for 1903. Note that the boxes used to define the Central England region differ by a small amount in the observations compared to the reanalyses due to differences in the grids used (cf. the boxes in panels <bold>a</bold> and <bold>b</bold>).</p></caption>
        <graphic xlink:href="https://esd.copernicus.org/articles/17/1365/2026/esd-17-1365-2026-f08.png"/>

      </fig>

      <p id="d2e2282">October 1903 is the wettest recorded calendar month for the UK (220.0 mm, in a series back to 1836; <xref ref-type="bibr" rid="bib1.bibx26" id="altparen.62"/>) and in the longer England and Wales Precipitation series (218.1 mm, in a series back to 1766 <xref ref-type="bibr" rid="bib1.bibx1" id="paren.63"/>). Figure 8a shows the October 1903 rainfall total in a gridded observational product that interpolates between in-situ measurements <xref ref-type="bibr" rid="bib1.bibx26" id="paren.64"/>. Large parts of Wales, Southwest England, and western Scotland recorded rainfall totals exceeding 200 mm. These regions also receive the most rain in 20CRv3<sup>+</sup> (Fig. 8b), though the magnitude is smaller in the reanalysis than in the observations. We would not expect perfect quantitative agreement with the observations as the reanalysis grid is too coarse to fully resolve the orography in these regions; similar underestimates are seen over western regions of Great Britain in the case of Storm Ulysses earlier in 1903 <xref ref-type="bibr" rid="bib1.bibx22" id="paren.65"/>. Output from the reanalysis could be downscaled using regional atmospheric models to better represent rainfall over mountainous regions if desired. Historical daily gridded rainfall observations are rarer outside the UK, so we also validate 20CRv3<sup>+</sup> rainfall against station observations from each of the well-observed regions in the Supplement (see Sect. S2 in the Supplement).</p>
      <p id="d2e2317">Over flatter terrain, the reanalysis is in better agreement with the observations, such as over a less mountainous region in Central England (Fig. 8e). As no rainfall data is assimilated, this represents an additional independent verification of the reanalysis. Daily rainfall is shown in Fig. 8e for comparison with the observations, but the higher frequency rainfall data in the reanalysis reveals several intense, sub-daily rainfall events during October that are obscured in the daily-mean (e.g. the 3 h-rain rate centred at 6 October, 15:00 UTC is 44 mm d<sup>−1</sup> in 20CRv3<sup>+</sup>, Fig. S10).</p>
      <p id="d2e2341">Both warmer world experiments see increased rainfall over the UK and Ireland (Fig. 8c and d). The increase of 17 % in the <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K experiment is equivalent to 8.8 % per K of local warming, while the increase of 12 % in <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M168" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M169" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is somewhat smaller (equivalent to 6.0 % K<sup>−1</sup>). These values are substantially larger than the increase in annual-mean precipitation of 3.0 % K<sup>−1</sup> over the larger NW_Europe region in the <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M173" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M174" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment (not shown). The increase in October rainfall over the UK and Ireland is closer to, or even above, the Clausius-Clapeyron scaling seen in extreme daily rainfall events (Fig. 7c). This likely reflects the unusually high occurrence of heavy rainfall events in this month, with 5 distinct events above the all-year 95th percentile of daily precipitation in 20CRv3<sup>+</sup> (Fig. 8e). Rainfall totals in extreme months or seasons may therefore scale much more rapidly with warming than the annual-mean.</p>
      <p id="d2e2444">On sub-daily time scales, the largest changes in October rainfall occur on wet days, whereas rain rates on drier days are comparable in both experiments (Fig. S10). This supports the finding in the previous section that substantial increases in time-mean rainfall can result from increased rainfall in a small number of heavy events. Notably, the warmer world rainfall rate at 6 October, 15:00 UTC is 58 mm d<sup>−1</sup>, an increase of 31 % over the value in 20CRv3<sup>+</sup> or around 15 % K<sup>−1</sup> – much greater than Clausius-Clapeyron scaling, as has previously been found for sub-daily rainfall extremes <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx21" id="paren.66"/>.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Discussion and conclusions</title>
      <p id="d2e2491">How would the everyday weather of a year from history be experienced in a warmer world? The reanalysis experiments in this paper share the same weather patterns, but by perturbing the SSTs and atmospheric <inline-formula><mml:math id="M179" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> we can explore how the weather of 1903 would be experienced in a warmer world by residents of four well-observed regions (the boxed regions in Fig. 1). We focus on changes in two key meteorological variables which affect day-to-day perception of the weather: temperature and rainfall. Residents of these regions would experience warmer near-surface temperatures nearly every day, with 99 % of days becoming warmer than in the 20CRv3<sup>+</sup> reconstruction of 1903. On a typical day, land areas would be warmer by around 2–2.5 °C for a 2 K ocean surface warming. However, increases of 2.5–3 °C are seen on hot days (temperatures around 20 °C or above), and larger increases of 4–5 °C on days below freezing. The cold day response appears to be due to enhanced absorption of solar radiation by the land surface due to a reduction in snow cover; the warmer world version of 1903 would also be one with substantially less snow and ice. Mechanisms for the hot day response are mixed: in the US_East_Coast region it is linked to reduced evaporative cooling on the hottest days, while changes in cloud cover appear to be more important in the SE_Aus region.</p>
      <p id="d2e2514">The everyday experience of rainfall would also be different in the warmer world. Even without substantial changes in large-scale weather patterns, annual rainfall would increase in NW_Europe and SE_Australia, decrease in Western_Med, and show little change in US_East_Coast – but in each region, daily rainfall would become more variable, meaning larger rainfall swings from day to day, with implications for infrastructure and adaptation. Even in regions where the total annual rainfall increases, the increase would occur on roughly 1 d in every 10 (that is, on days above the 90th percentile of rainfall). Instead, there would be fewer drizzly days, and in three of the four regions an overall reduction in the number of rainy days when the additional <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is included. Conversely, the number of days in the heavier rainfall bins grows exponentially with increasing rain rate.</p>
      <p id="d2e2528">We find that the October 1903 rainfall total over the UK and Ireland, already the wettest month on record in England and Wales, would be 12 %–17 % higher in a <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K warmer world. The reanalysis experiments presented here are idealised experiments rather than best estimates of the current climate, however they can give an indication of how much more rain the weather conditions of October 1903 might produce today. If we assume that global temperatures have warmed by 1.5 °C since 1903 (as compared to 2.3 °C in the <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M184" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M185" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment, Fig. 3a) then we estimate that the weather conditions of October 1903 would produce an extreme UK average rainfall of around 240 mm in the current climate. The next wettest observed month is December 2015 at 216.3 mm <xref ref-type="bibr" rid="bib1.bibx26" id="paren.67"/>. Future planned work using patterned SST perturbations and consistent <inline-formula><mml:math id="M186" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations will provide better estimates of how the impacts of historical extreme weather events would be different in the current climate. We will also perform additional experiments to translate events into a warmer future climate to inform adaptation planning.</p>
      <p id="d2e2584">We also find evidence of a direct <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> effect on everyday weather. Higher atmospheric <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> leads to enhanced warming of extratropical land than from SST warming alone, contributing 19 % of the total warming over the Western US in the <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M190" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M191" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment. Higher <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels act to suppress global precipitation and reduce the number of rainy days over NW_Europe, Western_Med, and US_East_Coast.</p>
      <p id="d2e2650">Our approach shares some of the limitations of other storyline attribution methods. The method in this paper makes two implicit assumptions: (1) that the weather patterns that occurred in 1903 could in principle occur in a world that is 2 K warmer; and (2) that assimilating the 1903 pressure observations with the 20CRv3 system does not lead to inconsistencies when the system's boundary conditions (SST, sea ice, and <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels) are perturbed. We can gain insight into both by comparing the reanalysis assimilation statistics from the 20CRv3<sup>+</sup> and <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M196" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiments. We find that the innovation (i.e. observed value minus first guess) and localisation length scales do not change substantially in the <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M199" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M200" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> experiment (Figs. S11a–d and S12a–b). However, the assimilation system does reject more pressure observations in <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K <inline-formula><mml:math id="M202" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M203" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> than in 20CRv3<sup>+</sup> (Figs. S11e–f and S12c). The relative increase is largest in NW_Europe, the region with proportionally the fewest rejections in 20CRv3<sup>+</sup>, and smallest in SE_Aus. An increase in the number of rejected observations may indicate that the model’s response to the warming causes some inconsistencies with the pressure observations, particularly where the density of observations is high and hence the observational constraint is strongest, as in NW_Europe. Note that tropical cyclone central pressures are assimilated without opportunity for rejection in both experiments.</p>
      <p id="d2e2777">However, the increased number of rejected observations does not in itself mean that the simulated weather events are necessarily implausible in a warmer world, even if they become slightly less compatible with the model’s own forced circulation response. The atmospheric circulation response to warming is both uncertain theoretically and variable among climate models <xref ref-type="bibr" rid="bib1.bibx62" id="paren.68"/>, which suggests caution regarding how much weight we assign to the dynamical response in 20CRv3. Even if the particular weather patterns of 1903 were to become less likely in a warmer world, it is difficult to argue that they would be impossible a priori, notwithstanding certain features of the 1903 climate (e.g. the eruption of the Santa Maria volcano in 1902, Fig. S3).</p>
      <p id="d2e2783">If changes in the atmospheric circulation do occur in future, they could lead to much larger changes in extreme temperature and precipitation, for example if persistent weather patterns were to occur more frequently <xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx35" id="paren.69"/>. The reanalysis experiments can thus be considered a strongly conditioned form of attribution, as we consider only the effects of warming that are not related to changes in the large-scale circulation <xref ref-type="bibr" rid="bib1.bibx69" id="paren.70"/>. This also means that feedbacks from the warming onto the large-scale circulation are neglected. For example, some studies have suggested that in heat waves arising due to a persistent atmospheric block, soil moisture anomalies can, in certain circumstances, feed back onto the atmospheric circulation pattern itself <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx38" id="paren.71"/>. Temperature increases on the hottest days may thus be higher than estimated in Fig. 5 if the circulation were allowed to respond. On the other hand, assimilating observed surface pressure does not constrain the atmospheric circulation entirely at all time and length scales – for example, the super-CC scaling of short-duration rainfall extremes in October 1903 (Fig. S10) indicate that sub-daily updraft velocities can show large changes, even in well-observed regions. Changes in vertical motion will also affect cloud behaviour, and may contribute to the cloud-mediated amplification of hot days in the SE_Aus region (Fig. S5d). Future work will compare where and how strongly the circulation is constrained in the reanalysis experiments versus other established methods such as spectral nudging <xref ref-type="bibr" rid="bib1.bibx17" id="paren.72"/>.</p>
      <p id="d2e2798">In reality, the dynamics and thermodynamics of the system cannot be cleanly separated, but in studies like ours it allows us to focus our investigation on processes that we think are better represented by the current generation of climate models (thermodynamic effects) than others (such as persistent weather regimes). This can offer insight into the robust physical processes behind regional climate signals. For example, Mediterranean precipitation declines in spring, summer, and autumn in the warmer world experiments, but increases in winter, presumably due to local changes in atmospheric stability and humidity. We also find that, in the absence of shifts in the Mediterranean storm track, seasonality in the Mediterranean precipitation response is driven entirely by SST warming, as the direct effect of increased atmospheric <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is to reduce Mediterranean rainfall regardless of season. Other Mediterranean climates are also projected to dry, with atmospheric circulation contributing to the recent Chilean “megadrought” <xref ref-type="bibr" rid="bib1.bibx19 bib1.bibx20" id="paren.73"/>. Forthcoming experiments will consider the modern period where there are more pressure observations over Chile and other Mediterranean-like climates outside Europe.</p>
      <p id="d2e2815">This study has presented an exploration of a single year's weather. Our conclusions are restricted to regions with a high density of historical pressure observations, and some may be sensitive to the reanalysis system used – for example, there are longstanding problems in the simulation of light rainfall in numerical models <xref ref-type="bibr" rid="bib1.bibx9" id="paren.74"/>, which limits confidence in the reduction of light rainfall and overall rainfall occurrence seen in the warmer world experiments. However, it is notable that even in a single year, the reanalysis experiments support changes in rainfall characteristics that have been seen in multiple generations of coupled models <xref ref-type="bibr" rid="bib1.bibx25 bib1.bibx28 bib1.bibx47" id="paren.75"/>.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e2828">Ensemble-means and ensemble-standard deviations for 2 m-temperature and precipitation rate are available for each of the three experiments at <ext-link xlink:href="https://doi.org/10.5281/zenodo.19949356" ext-link-type="DOI">10.5281/zenodo.19949356</ext-link> <xref ref-type="bibr" rid="bib1.bibx68" id="paren.76"/>. The repository also includes the pressure observation text files used to generate Fig. 1. Individual ensemble members can be provided upon request.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e2837">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/esd-17-1365-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/esd-17-1365-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e2846">GPC, SG, and LCS assisted with the design and running of the reanalysis experiments. EH and RT ran the reanalysis experiments. RT analysed the experiments and prepared the paper, with contributions from all co-authors. EH conceived and supervised the project.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e2852">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e2858">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e2864">The authors would like to thank Manoj Joshi for comments on an earlier draft of this work and two anonymous reviewers for their feedback. This work was supported by the UK National Centre for Atmospheric Science. Author GPC was supported in part by the NOAA Physical Sciences Laboratory. Author LS was supported by the NOAA Physical Sciences Laboratory. This work used JASMIN, the UK's collaborative data analysis environment (<uri>https://www.jasmin.ac.uk</uri>, last access: 16 September 2026; <xref ref-type="bibr" rid="bib1.bibx29" id="altparen.77"/>), and the ARCHER2 UK National Supercomputing Service (<uri>https://www.archer2.ac.uk</uri>, last access: 16 September 2026; <xref ref-type="bibr" rid="bib1.bibx4" id="altparen.78"/>).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e2881">This research has been funded by the Natural Environment Research Council (grant no. NE/Z000203/1), a Co-Centre award from Research Ireland, Northern Ireland's Department of Agriculture, Environment and Rural Affairs (DAERA) and UK Research and Innovation (UKRI) (grant no. 22/CC/11103), the National Oceanic and Atmospheric Administration (grant no. NA22OAR4320151), and the Cooperative Institute for Earth System Research and Data Science.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e2888">This paper was edited by Olivia Martius and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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