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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</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/acp-26-5151-2026</article-id><title-group><article-title>Aerosol–cloud interactions in marine low-clouds in a warmer climate</article-title><alt-title>Aerosol–cloud interactions in marine low-clouds in a warmer climate</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Prabhakaran</surname><given-names>Prasanth</given-names></name>
          <email>prasantp@mtu.edu</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Myers</surname><given-names>Timothy A.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hoffmann</surname><given-names>Fabian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5136-0653</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Feingold</surname><given-names>Graham</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0774-2926</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Cooperative Institute for Research In Environmental Sciences (CIRES), University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Chemical Sciences Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Physical Sciences Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Freie Universität Berlin, Institut für Meteorologie, Berlin, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Prasanth Prabhakaran (prasantp@mtu.edu)</corresp></author-notes><pub-date><day>17</day><month>April</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>7</issue>
      <fpage>5151</fpage><lpage>5167</lpage>
      <history>
        <date date-type="received"><day>20</day><month>June</month><year>2025</year></date>
           <date date-type="rev-request"><day>27</day><month>June</month><year>2025</year></date>
           <date date-type="rev-recd"><day>14</day><month>December</month><year>2025</year></date>
           <date date-type="accepted"><day>5</day><month>January</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Prasanth Prabhakaran 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://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026.html">This article is available from https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e133">We explore the impact of aerosol perturbation on the stratocumulus-to-cumulus transition (SCT) in a warmer climate in the North-East Pacific region using a Lagrangian large-eddy simulation model coupled to a two-moment, bin-emulating bulk microphysics scheme. We explore two SCT cases with different free-tropospheric (FT) humidities – moist FT and dry FT. For each case, we consider two Shared Socioeconomic Pathways (SSPs), SSP3-7.0 and SSP1-2.6, from the most recent Coupled Model Intercomparison Project (CMIP6) to determine the extent of warming and changes in aerosol concentration at the end-of-the-century. We find that the cloud radiative effect (CRE) in non-precipitating stratocumulus clouds is more susceptible to climate change than to aerosol. However, after the breakup of the cloud deck, the impact of aerosol tends to dominate. Furthermore, in these low-clouds, aerosol-cloud interactions (Twomey effect and liquid water path adjustments) are to leading order immune to climate change, unless aerosol-induced cloud fraction adjustment is significant. We extend the analysis to marine cloud brightening and show that its efficacy decreases with warming because of the reduction in cloud fraction. We also explore the impact of climate change and aerosol perturbation on SCT. In the moist FT case, climate change advances the onset of cumulus activity and cloud breakup. However, in the dry FT case, climate change does not affect the onset of cumulus activity but delays cloud breakup. In both cases, aerosol injection delays cloud breakup via precipitation suppression but does not affect cumulus onset unless it is coupled to rain formation.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Climate Program Office</funding-source>
<award-id>03-01-07-001</award-id>
</award-group>
<award-group id="gs2">
<funding-source>U.S. Department of Commerce</funding-source>
<award-id>03-01-07-001</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Deutsche Forschungsgemeinschaft</funding-source>
<award-id>HO 6588/1-1</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="d2e145">Marine low-clouds strongly regulate global mean temperature by reflecting a substantial fraction of incoming short-wave (SW) radiation to outer space <xref ref-type="bibr" rid="bib1.bibx43" id="paren.1"/>. The climate feedback associated with these clouds is one of the largest uncertainties in Earth's climate projections <xref ref-type="bibr" rid="bib1.bibx46" id="paren.2"/>. The picture becomes more complex once the uncertainties associated with aerosol-cloud interactions are included <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx3" id="paren.3"/>. The key reason for this is the poor representation of turbulent cloud processes in climate models. In this paper, we explore the impact of climate change on aerosol-cloud interactions in marine low-clouds using Lagrangian (domain moving with mean wind) large-eddy simulations (LESs).</p>
      <p id="d2e157">With the advent of high-resolution numerical simulations (LES and cloud-resolving simulations), our understanding of the response of marine low-clouds to climate perturbations has improved substantially <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx8" id="paren.4"/>. These studies explored the response of marine stratocumulus, cumulus-under-stratocumulus, and shallow cumulus clouds to a warmer climate. They showed that weakening of the subsidence velocity and/or strengthening of the inversion aid in thickening of the stratocumulus deck, a negative feedback with respect to cloud radiative effect (CRE) <xref ref-type="bibr" rid="bib1.bibx7" id="paren.5"/>. However, weakened radiative cooling and warming result in a strong positive feedback. The net cloud feedback is positive in the stratocumulus and cumulus-under-stratocumulus cases, and weakly positive in the cumulus regime. Their analysis also explored the thermodynamic mechanism behind the thinning and reduction in cloud cover (<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in marine stratocumulus clouds in a warmer world that results in a positive cloud feedback (entrainment-liquid flux feedback). A similar framework was also used to explore cloud feedback in precipitating and spatially organized marine cumulus clouds <xref ref-type="bibr" rid="bib1.bibx40" id="paren.6"/>. Furthermore, several studies have attempted to observationally constrain marine low-cloud feedback. To do so, they quantify the sensitivity of marine low clouds to meteorological perturbations via satellite observations, and then use climate models to estimate meteorological changes with planetary warming.  The observation-based findings from these studies are in qualitative agreement with high-resolution models <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx14 bib1.bibx28 bib1.bibx25" id="paren.7"><named-content content-type="post">and references therein</named-content></xref>.</p>
      <p id="d2e185">Over the last two decades, several studies have focused on understanding the physical processes associated with aerosol-cloud interactions (ACI) in marine low-clouds. The Twomey effect, an increase in cloud albedo in response to an increase in cloud droplet concentration (<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) while assuming the LWP is constant, and the life-time effect, where the cloud albedo is increased by suppressing precipitation, have been well explored <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx2" id="paren.8"/>. LES studies have highlighted that decrease in sedimentation velocity (sedimentation-entrainment feedback) and the increase in evaporation rate (evaporation-entrainment feedback) at the cloud-top in response to increases in <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> result in an increase in the intensity of turbulence at the cloud-top <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx1 bib1.bibx10" id="paren.9"/>. This increases the entrainment rate at cloud-top that eventually results in a reduction in LWP. However, these studies do not account for the effects of the diurnal cycle. Using an ensemble of LES simulations, <xref ref-type="bibr" rid="bib1.bibx47" id="text.10"/> argue that the effects of SW absorption may buffer some of the aforementioned cloud adjustments in response to aerosol perturbations. Moreover, <xref ref-type="bibr" rid="bib1.bibx33" id="text.11"/> showed that weak precipitation suppression causes cloud darkening due to enhanced SW absorption. However, not many studies have focused on how ACI would change in a warmer climate, which is the central question addressed here. Changes in boundary layer turbulence as well as changes in baseline cloud properties due to climate change may alter the cloud response to aerosol. The aerosol perturbation we use in this study is a proxy for intermittent emissions from volcanoes, ship emissions, or a deliberate injection of aerosol to enhance the reflectivity of marine low-clouds (marine cloud brightening, MCB). MCB is a climate intervention approach aimed at mitigating some of the worst effects of anthropogenic radiative forcing <xref ref-type="bibr" rid="bib1.bibx22" id="paren.12"/>. The insights from this study should also be useful in assessing the efficacy of MCB in a warmer world.</p>
      <p id="d2e226">We use the stratocumulus-to-cumulus transition (SCT) as a framework for exploring ACI in a warmer climate. Consequently, we also explore the impact of climate change on SCT as few studies have explored this topic. The stratocumulus-topped boundary layer transitions into a cumulus-topped boundary layer as the air mass advects towards the equator over a continuously increasing ocean temperature. The associated increase in surface latent heat flux (LHF) and the weakening of subsidence promotes the deepening and decoupling of the cloud-topped boundary layer <xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx26 bib1.bibx44" id="paren.13"/>. Eventually, the formation of overshooting cumulus clouds erode the decoupled stratus layer at the top of the boundary layer. We refer to this transition as an entrainment-driven transition. Recent studies have shown that precipitation also likely plays a key role in the breakup of the stratocumulus cloud layer <xref ref-type="bibr" rid="bib1.bibx45 bib1.bibx48 bib1.bibx36" id="paren.14"/>. We refer to these transitions as the precipitation-mediated transition. In this study, we explore the impact of climate change and aerosol perturbation on both precipitation-mediated and entrainment-driven SCTs.</p>
      <p id="d2e236">In the next section, we present our methodology for setting up cases in a warmer world. This is followed by the results from the simulations exploring the impact of climate change and aerosol perturbation on SCT in both precipitation-mediated and entrainment-driven scenarios. We end with a discussion of our results focusing on the impact of climate change on cloud properties, SCT, ACI, and MCB, followed by a summary.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methodology</title>
      <p id="d2e247">The setup of the LES follows the framework presented in <xref ref-type="bibr" rid="bib1.bibx45" id="text.15"/> and <xref ref-type="bibr" rid="bib1.bibx33" id="text.16"/>, and thus will only be briefly discussed.</p>
      <p id="d2e256">We use the System for Atmospheric Model (SAM) version 6.10.10 to simulate the dynamics <xref ref-type="bibr" rid="bib1.bibx24" id="paren.17"/> and the effects of radiation are computed using the Rapid Radiative Transfer Model for Global Climate Models (RRTMG) using the two-stream approximation with extended vertical profiles <xref ref-type="bibr" rid="bib1.bibx27" id="paren.18"/>. In addition, we use a two-moment, bin-emulating bulk scheme to represent the microphysical properties of the cloud system <xref ref-type="bibr" rid="bib1.bibx21" id="paren.19"/>. Our microphysics model allows local scavenging of aerosol that increases the chance of precipitation and associated feedback, which may play a prominent role in the breakup of stratocumulus clouds <xref ref-type="bibr" rid="bib1.bibx45" id="paren.20"/>.</p>
      <p id="d2e271">The focus of this study is to assess the impact of aerosol perturbations on the SCT in the North-East Pacific (NEP) region in a warmer climate. We use the well-explored composite reference case from <xref ref-type="bibr" rid="bib1.bibx35" id="text.21"/> to represent the present-day (PD) scenario (JJA from 2005–2006). In this case, precipitation plays a prominent role in the onset of cumulus activity and subsequent breakup <xref ref-type="bibr" rid="bib1.bibx45 bib1.bibx48 bib1.bibx33" id="paren.22"/>. However, not all SCTs exhibit a key role for precipitation (e.g., <xref ref-type="bibr" rid="bib1.bibx12" id="altparen.23"/>). To suppress the precipitation-mediated transition, we created an additional case with reduced humidity in the free troposphere (FT). This results in a case where the transition is driven by entrainment-deepening, which is more representative of the NEP region <xref ref-type="bibr" rid="bib1.bibx12" id="paren.24"/>. The humidity in the FT is lowered to 27 % of the reference value and is referred to as the dry FT case. Note that the dry FT case does not represent a climate perturbation; instead, it represents a different realization of the PD scenario.</p>
      <p id="d2e286">In exploring the dynamics associated with stratocumulus-to-cumulus transition (SCT), the choice of the simulation domain size becomes important. <xref ref-type="bibr" rid="bib1.bibx45" id="text.25"/> carried out sensitivity tests for the composite case in <xref ref-type="bibr" rid="bib1.bibx35" id="text.26"/> and showed that a horizontal domain size of at least 24 km is required to capture the role of precipitation and associated feedback in SCT. Here, all simulations have a domain size of 48 km in the horizontal directions with a uniform grid size of 100 m. The domain top is 4.25 km with a grid size of 10 m until a height of 2.775 km and then gradually stretched to the top of the domain.</p>
      <p id="d2e296">To represent the warmer climate at the end of the century (EoC), we consider two shared socioeconomic pathways (SSPs) with forcings from the Representative Concentration Pathways (RCPs) from the recent coupled model intercomparison project (CMIP6): (i) SSP1-2.6 represents sustainability and is one of the most optimistic warming scenarios, and (ii) SSP3-7.0 represents higher emissions associated with regional rivalry that maintains aerosol forcing <xref ref-type="bibr" rid="bib1.bibx34" id="paren.27"/>. The SSP1-2.6, henceforth referred to as SSP1, represents a scenario with cleanup and warming (with respect to preindustrial) restricted to less than 2 °C in global mean temperature. The SSP3-7.0, henceforth referred to as SSP3, is considered the middle-of-the-road scenario. Note that the worst-case-scenario in CMIP6 is SSP5-8.5, however, this scenario is considered highly unlikely <xref ref-type="bibr" rid="bib1.bibx37" id="paren.28"/>. Therefore, we use SSP1 and SSP3 as bounding scenarios to explore the efficacy of MCB in a warmer climate. We use the forcings from these scenarios to develop the equivalent EoC conditions for <xref ref-type="bibr" rid="bib1.bibx35" id="text.29"/> using the methodology described in <xref ref-type="bibr" rid="bib1.bibx8" id="text.30"/>. A brief overview of the methodology is given below. We also included an additional 12 h spin-up time for the cloud deck to adjust to its surroundings. During this time, the SST and the subsidence velocity remain constant. Aerosol perturbation (uniform surface flux <inline-formula><mml:math id="M4" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 2170 particles cm<sup>−2</sup> s<sup>−1</sup>) begins at the end of the spin-up period and is sustained for about 2.67 h (approximate time for a ship to traverse the domain at a speed of 5 m s<sup>−1</sup>).</p>
      <p id="d2e355">To set up simulations under EoC conditions, the variables required from CMIP6 models are changes in SST (<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">SST</mml:mi></mml:mrow></mml:math></inline-formula>), CO<sub>2</sub> concentration, and changes in subsidence velocity. Note that we are not considering regional variations in temperature due to climate change. We assume that <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>SST is spatially uniform. The <inline-formula><mml:math id="M11" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>SST and CO<sub>2</sub> concentrations are obtained from the global average values of the CMIP6 ensemble <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx30" id="paren.31"/>. The challenging part is to determine the sounding profiles for the scalars and the subsidence. The vertical temperature profile in the FT is close to that of a moist pseudoadiabat and is regulated by tropical-deep convective systems <xref ref-type="bibr" rid="bib1.bibx13" id="paren.32"/>. Under warmer conditions, the temperature in the FT is obtained by following another moist pseudoadiabat with a temperature at sea level that is warmer than the present day value by <inline-formula><mml:math id="M13" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>SST. Similar to earlier studies, we assume that RH in PD and EoC to be identical throughout the domain <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx8" id="paren.33"/>. The vertical profile of the subsidence velocity (defined as the pressure velocity <inline-formula><mml:math id="M14" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>) is determined by ensuring that the average FT temperature drift is minimal. To ensure this, subsidence-induced warming (<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mi mathvariant="italic">ω</mml:mi><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="italic">θ</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></inline-formula>) is balanced by clear-sky radiative cooling in the FT. For more details on determining subsidence profiles, see the appendix in <xref ref-type="bibr" rid="bib1.bibx8" id="text.34"/>.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Precipitation-mediated transition</title>
      <p id="d2e463">Figure <xref ref-type="fig" rid="F1"/> shows the time evolution of the key cloud-topped boundary layer properties for the original reference case in <xref ref-type="bibr" rid="bib1.bibx35" id="text.35"/> (red lines), henceforth referred to as the PD case, and its warmer-world counterpart at the EoC (black (SSP3) and green (SSP1) lines). We start by presenting the impact of warming on the SCT (solid lines) and then discuss the effect of aerosol perturbation (dashed lines). Note that SSP1 has fewer cloud droplets (120 mg<sup>−1</sup>) compared to the other two cases (150 mg<sup>−1</sup>) and thus will be discussed separately. Additionally, we use a new metric for determining the onset of cumulus activity. Earlier studies have used various metrics to define the magnitude of this transition. <xref ref-type="bibr" rid="bib1.bibx35" id="text.36"/> defined SCT based on reduction in scene albedo (<inline-formula><mml:math id="M18" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula>). In <xref ref-type="bibr" rid="bib1.bibx33" id="text.37"/> and <xref ref-type="bibr" rid="bib1.bibx4" id="text.38"/>, the transition is defined on the basis of a sustained reduction (6 to 24 h) in the cloud fraction <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The latter definition is applicable for the cases in which precipitation plays a prominent role in the transition. Here, we use the spatial variance in the cloud base (<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) as a metric for the onset of cumulus clouds in the boundary layer. For nearly horizontally homogeneous stratocumulus clouds, the variance in <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> will be near zero. However, with the onset of cumulus activity, i.e., for cumulus-under-stratocumulus, the variance will increase as the number of cumulus columns increases.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e547">Time series of <bold>(a)</bold> short wave upward (SWUP) flux, <bold>(b)</bold> liquid water path (LWP), <bold>(c)</bold> cloud droplet concentration (<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(d)</bold> cloud fraction (<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(e)</bold> variance of cloud base (<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(f)</bold> domain-averaged precipitation flux (rain rate) at <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and domain-averaged height of the inversion layer (<inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in the high humidity FT cases. <inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the cloud optical thickness used to identify the cloudy regions. The legend is shown in panel <bold>(e)</bold>, and “_aP” in the legend identifies the cases with aerosol perturbation. The time period between sunset and sunrise is shaded in gray.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f01.png"/>

        </fig>

      <p id="d2e641">The evolution of PD (solid red line) is similar to the results in <xref ref-type="bibr" rid="bib1.bibx33" id="text.39"/>. The diurnal cycle is clearly evident in the LWP and cloud fraction (<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) time series (Fig. <xref ref-type="fig" rid="F1"/>b, d). Note that cloud breakup in PD occurs earlier (by approximately 10–12 h) than in <xref ref-type="bibr" rid="bib1.bibx33" id="text.40"/>. We attribute this to the additional 12 h spin-up in the current simulations, which causes the boundary layer to deepen by an additional 200 m during this time period. The rapid reduction in <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (around 52 h in Fig. <xref ref-type="fig" rid="F1"/>d) is triggered by the onset of strong precipitation at the cloud base (Fig. <xref ref-type="fig" rid="F1"/>f), and is correlated with a rapid reduction in cloud droplet concentration <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F1"/>c). In the strongly warmer-world (SSP3), the LWP is substantially lower than its PD counterpart (Fig. <xref ref-type="fig" rid="F1"/>b). Note that the entrainment velocity is also lower in SSP3, which is evident from the inversion layer height <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> time series (Fig. <xref ref-type="fig" rid="F1"/>f). This is due to weakening of the boundary layer turbulence due to climate change <xref ref-type="bibr" rid="bib1.bibx11" id="paren.41"/>. <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the warmer world is lower than in the PD scenario until the onset of precipitation below <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M34" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 55 h). The reduction in LWP, despite the reduction in entrainment velocity, is an outcome of the entrainment-liquid flux (ELF) feedback associated with the increase in humidity jump across the inversion layer due to warming <xref ref-type="bibr" rid="bib1.bibx8" id="paren.42"/>. This increase in the humidity jump across the inversion layer enhances the evaporative cooling rate at the cloud-top, which translates to enhanced buoyancy production at cloud-top, thus increasing the entrainment flux despite a lower entrainment velocity (see <xref ref-type="bibr" rid="bib1.bibx8" id="text.43"/> for a detailed discussion of the ELF feedback mechanism). Additionally, <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> undergoes a stronger diurnal cycle in a warmer climate due to the strong reduction in cloud-top radiative cooling as well as the ELF feedback <xref ref-type="bibr" rid="bib1.bibx8" id="paren.44"/>. Interestingly, the onset of cloud breakup in the warmer world (SSP3) around 50 h (Fig. <xref ref-type="fig" rid="F1"/>d) is also driven by precipitation, and the timing of the onset of precipitation is a bit earlier than in PD. Post cloud breakup (after 64 h), the cloud properties and consequently the short wave upward (SWUP) flux for these two cases converge. The LWP and <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> converge within a few hours while the inversion heights take longer. Another variable of interest is the variance of the cloud base height <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F1"/>e). We see that cumulus activity is initiated earlier in SSP3 (enhanced value of the variance around 43 h), which is consistent with the earlier onset of precipitation. Note that the boundary layer coupling strengthens after sunset on day 2 and then weakens again after the onset of precipitation. Subsequently, in the remaining days, the magnitude of the <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> variance continues to increase. Thus, apart from the onset of precipitation and the reduction in <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the variance in <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is also a good indicator of cumulus activity in this system.</p>

<table-wrap id="T1"><label>Table 1</label><caption><p id="d2e825">Large-scale conditions for all the simulations. The changes for each scenario are with respect to the values for the composite reference trajectory in <xref ref-type="bibr" rid="bib1.bibx35" id="text.45"/>. We report the increase in SST, and the factor by which CO<sub>2</sub> concentration ([CO<sub>2</sub>]) and pressure velocity (<inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>) changes. The values in the brackets for <inline-formula><mml:math id="M44" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula> represent the conditions for the equivalent dry FT scenarios. <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> shows the aerosol concentration in each scenario.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Case</oasis:entry>
         <oasis:entry colname="col2">[CO<sub>2</sub>]</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M47" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>SST</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M48" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (mg<sup>−1</sup>)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">PD</oasis:entry>
         <oasis:entry colname="col2">1<inline-formula><mml:math id="M51" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M52" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0 K</oasis:entry>
         <oasis:entry colname="col4">1<inline-formula><mml:math id="M53" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> (1.4<inline-formula><mml:math id="M54" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col5">150</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SSP3</oasis:entry>
         <oasis:entry colname="col2">2.3<inline-formula><mml:math id="M55" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M56" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.1 K</oasis:entry>
         <oasis:entry colname="col4">0.90<inline-formula><mml:math id="M57" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> (1.29<inline-formula><mml:math id="M58" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col5">150</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SSP1</oasis:entry>
         <oasis:entry colname="col2">1.2<inline-formula><mml:math id="M59" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M60" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.9 K</oasis:entry>
         <oasis:entry colname="col4">0.96<inline-formula><mml:math id="M61" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> (1.37<inline-formula><mml:math id="M62" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col5">120</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d2e1089">In the muted warming scenario (SSP1), the effect of warming on cloud properties (solid green line in Fig. <xref ref-type="fig" rid="F1"/>) is a lot weaker compared to SSP3. This is an obvious outcome of weaker forcing associated with climate change (see Table <xref ref-type="table" rid="T1"/>). However, there are additional contributions from the lower aerosol concentration. The LWP and <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are similar to the PD case on days 1 and 2. A possible explanation is that the effects of the ELF feedback associated with warming are offset by the lower aerosol concentration within the marine boundary layer, i.e., the reduction in LWP associated with the effects of climate change (warming and weakened radiative cooling) and the increase in LWP due to the reduction in <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (weakened sedimentation-entrainment and evaporative-entrainment feedbacks), offset each other. Here too, the lower aerosol concentration results in a slightly earlier onset of precipitation compared to PD. The evolution of cloud properties post-transition is similar to SSP3 but does not show any signs of convergence towards the PD values. <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and SWUP flux are consistently higher in SSP1 after the transition (after <inline-formula><mml:math id="M66" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 65 h).</p>
      <p id="d2e1137">Post aerosol injection (<inline-formula><mml:math id="M67" display="inline"><mml:mo lspace="0mm">≥</mml:mo></mml:math></inline-formula> 12 h) and prior to cloud breakup (<inline-formula><mml:math id="M68" display="inline"><mml:mo lspace="0mm">≲</mml:mo></mml:math></inline-formula> 50 h), the in-cloud (<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>≥</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M70" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is cloud optical thickness) LWP is reduced relative to the unperturbed case (dashed lines in Fig. <xref ref-type="fig" rid="F1"/>). The reduction in LWP is more substantial in PD and SSP1. In SSP3, a combination of weaker boundary layer turbulence <xref ref-type="bibr" rid="bib1.bibx11" id="paren.46"/> and lower LWP <xref ref-type="bibr" rid="bib1.bibx16" id="paren.47"/> reduce the magnitude of sedimentation-entrainment feedback. In PD and SSP3, <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is weakly affected by aerosol perturbation prior to cloud breakup (<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/></mml:mrow></mml:math></inline-formula>50 h). However, in SSP1, suppression of weak precipitation around sunrise on day 2 causes a substantial reduction in <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (between 40–45 h, Fig. <xref ref-type="fig" rid="F1"/>d, f). This results in a reduction in the scene albedo as is evident from the SWUP flux time series (green dashed line in Fig. <xref ref-type="fig" rid="F1"/>a). A similar observation was reported in <xref ref-type="bibr" rid="bib1.bibx33" id="text.48"/>. This precipitation-suppression induced darkening (albedo reduction) was attributed to the effects of enhanced SW absorption.</p>
      <p id="d2e1223">Injection of aerosol into the boundary layer delays the onset of cloud breakup through precipitation suppression in all scenarios. Despite the reduction in LWP, the suppression of precipitation maintains overcast conditions for an additional day, leading to substantial cloud brightening on day 3. However, the reduction of <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the warmer world means that a reduced amount of cloud is available for brightening. This leads to a weaker enhancement of the SWUP flux in SSP3 on day 3 (Fig. <xref ref-type="fig" rid="F1"/>a).</p>
      <p id="d2e1239">To quantify the impact of aerosol perturbation on cloud properties, we explore aerosol-induced changes to the SW cloud radiative effect (dCRE <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">CRE</mml:mi><mml:mi mathvariant="normal">unperturbed</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">CRE</mml:mi><mml:mrow><mml:mi mathvariant="normal">aerosol</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">perturbed</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), where positive values indicate cloud brightening. Following <xref ref-type="bibr" rid="bib1.bibx20" id="text.49"/> and <xref ref-type="bibr" rid="bib1.bibx17" id="text.50"/>, we decompose dCRE into contributions from <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and LWP:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M78" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left right"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub><mml:mo mathvariant="italic">{</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mo>-</mml:mo><mml:mi>N</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:munder></mml:mrow></mml:mtd><mml:mtd/></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi></mml:mrow></mml:munder></mml:mrow></mml:mtd><mml:mtd/></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">clr</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mo>-</mml:mo><mml:mi>f</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:munder><mml:mo mathvariant="italic">}</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the incoming solar radiation at top-of-the-atmosphere (TOA), <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">clr</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the clear-sky albedo, <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the cloud albedo contribution from changes in <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> or LWP, <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is cloud fraction, and aP in the subscript indicates aerosol perturbation, respectively. dCRE <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> or dCRE <inline-formula><mml:math id="M85" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP represent the change in CRE while LWP or <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is unperturbed (with respect to aerosol), respectively. Both terms are directly proportional to the unperturbed <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. dCRE <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a product of cloud abedo changes and <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> changes in response to aerosol perturbation.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1633">Time series of changes in CRE (dCRE <inline-formula><mml:math id="M90" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CRE<inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">unperturbed</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">CRE</mml:mi><mml:mrow><mml:mi mathvariant="normal">aerosol</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">perturbed</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) due to aerosol perturbation in the high FT humidity cases and its contributions from changes to <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWP, and <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. A positive value indicates cloud brightening. <bold>(a)</bold> dCRE, <bold>(b)</bold> <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE, <bold>(c)</bold> LWP contribution to dCRE, <bold>(d)</bold> <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE. <inline-formula><mml:math id="M96" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the cloud optical thickness. The legend is shown in panel <bold>(d)</bold>. Note that <inline-formula><mml:math id="M97" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis range is different for each panel. </p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f02.png"/>

        </fig>

      <p id="d2e1745">Figure <xref ref-type="fig" rid="F2"/> shows the evolution of dCRE and its components in all scenarios, and Table <xref ref-type="table" rid="T2"/> shows the daytime average for the same quantities. Similar to <xref ref-type="bibr" rid="bib1.bibx33" id="text.51"/>, dCRE increases from day 1 to day 3 in all scenarios (Fig. <xref ref-type="fig" rid="F2"/>a). On day 1, dCRE is highest for SSP1 and PD and lowest for SSP3 (Fig. <xref ref-type="fig" rid="F2"/>a and Table <xref ref-type="table" rid="T2"/>). By day 2, the dCRE is highest for the SSP1 case and lowest for the PD case. On day 3, the highest dCRE is for SSP1 followed by PD and then SSP3. These trends suggest a combined influence of warming and the background aerosol concentrations in determining aerosol-induced CRE changes.</p>
      <p id="d2e1762">To gain a deeper understanding of these trends on each day, we examine the decomposition of dCRE (Fig. <xref ref-type="fig" rid="F2"/>b, c, and d). In the first two days, the positive contribution to dCRE is dominated by dCRE <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> with SSP1 having the highest value. On day 3, dCRE <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the dominant contributor to dCRE in all scenarios. This is associated with the suppression of precipitation-induced cloud breakup. As in dCRE <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, SSP1 has the highest magnitude, and SSP3 the lowest. The dCRE <inline-formula><mml:math id="M101" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP component is predominantly negative on all days as a result of the reduction in LWP from increased entrainment flux and SW absorption. This substantially offsets the brightening from the Twomey and lifetime effects. On most days, the highest magnitude is for PD followed by SSP1 and SSP3 (Table <xref ref-type="table" rid="T2"/>).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Entrainment-driven transition</title>
      <p id="d2e1824">Figure <xref ref-type="fig" rid="F3"/>, similar to Fig. <xref ref-type="fig" rid="F1"/>, shows the time series of key boundary layer properties in all scenarios with dry FT humidity (entrainment-driven transition). In this case, precipitation does not play a dominant role in the transition to a cumulus-topped boundary layer. This is evident from Fig. <xref ref-type="fig" rid="F3"/>f, which shows that the precipitation flux at <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is negligible prior to the onset of cumulus activity (around 66 h) in all unperturbed scenarios. As noted previously, we use the variance in <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as a metric to assess the onset of cumulus activity.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e1857">Same as Fig. <xref ref-type="fig" rid="F1"/>, but for the dry FT cases.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f03.png"/>

        </fig>

      <p id="d2e1868">The reduction in FT humidity substantially lowers the cloud LWP (Fig. <xref ref-type="fig" rid="F3"/>b) compared to the corresponding cases in Fig. <xref ref-type="fig" rid="F1"/>. Over time, the increase in SST enhances the LWP in the cloud layer in all the unperturbed cases. The LWP is lowest in SSP3 until the onset of precipitation, and similar in the PD and SSP1 cases on day 1 and most of day 2. The relatively low LWP in SSP3 results in weak precipitation below the cloud base until the end of the simulation (Fig. <xref ref-type="fig" rid="F3"/>f). The <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> time series is substantially altered by the degree of climate change (Fig. <xref ref-type="fig" rid="F3"/>d). The increase in SST due to climate change and the weakening of radiative cooling at cloud-top, enhances the magnitude of changes in <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> over the course of a diurnal cycle. Consequently, SSP3 has the lowest <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, followed by SSP1 and the reference case. It is interesting to note that the minimum value in <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is similar on all three days in SSP3, while, in the SSP1 and PD scenarios, the minima in <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> decrease from day 1 to day 3. On day 3, the value of the minimum in <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is similar in all three cases around 66 h, marking the onset of cumulus activity. This is evident from the sharp increase in the cloud base variance time series (<inline-formula><mml:math id="M110" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 66 h in Fig. <xref ref-type="fig" rid="F3"/>e). The onset of precipitation in the final 12 h of the simulation results in the breakup of the stratocumulus layer, lowers <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and further increases the variance in <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F3"/>d, e, and f). Note that despite the similarity in the onset times of cumulus clouds across scenarios, the cloud breakup timings are quite different. Substantial precipitation occurs first in SSP1 due to a lower <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, followed by PD, and then SSP3 (Fig. <xref ref-type="fig" rid="F3"/>f). Substantially lower LWP in SSP3 results in a delayed and weaker precipitation flux (20 %–50 % lower compared to PD). Consequently, cloud breakup is slower in SSP1 (Fig. <xref ref-type="fig" rid="F3"/>d) and the SWUP flux is highest for SSP1 on day 4 (Fig. <xref ref-type="fig" rid="F3"/>a). Note that precipitation only plays a secondary role in this entrainment-driven transition case. However, we will see later that the aerosol-induced changes in CRE are dominated by processes associated with precipitation.</p>
      <p id="d2e2010">The injection of aerosol lowers the LWP in all three scenarios until the onset of precipitation (dashed lines in Fig. <xref ref-type="fig" rid="F3"/>b). The magnitude of the change in LWP increases with time until the onset of precipitation (Fig. <xref ref-type="fig" rid="F3"/>b). Additionally, during the daytime, <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> also decreases weakly due to the increase in aerosol concentration prior to the onset of precipitation (Fig. <xref ref-type="fig" rid="F3"/>d). Furthermore, aerosol injection does not influence the onset of cumulus activity (see the variance of <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> time series in Fig. <xref ref-type="fig" rid="F3"/>e). Notable effects related to aerosol perturbation are evident only post precipitation suppression. This enhances <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in PD and SSP1 scenarios. Note that in SSP3, the increase in <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> post aerosol injection is weaker compared to SSP1 and PD due to the weaker precipitation flux at <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e2077">Figure <xref ref-type="fig" rid="F4"/> and Table <xref ref-type="table" rid="T2"/> show the dCRE and its components for the entrainment-driven transition cases. Until the onset of precipitation (day 3/day 4), the enhancement in CRE is weaker compared to the high-humidity cases (Fig. <xref ref-type="fig" rid="F4"/>a). This is an outcome of lower LWP and <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. However, post precipitation onset on the final day, the enhancement in CRE is comparable to the moist FT case. dCRE is comparable in PD and SSP1 on days 1 and 2. On day 3, the dCRE in SSP1 is substantially higher than in PD. For SSP3, the dCRE values are substantially lower than the other two cases on all days. The decomposition of dCRE offers further insights into the evolution of dCRE across scenarios. In SSP3, dCRE <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the lowest on all three days, and the values are similar in SSP1 and PD on each day with slightly higher values for SSP1 due to its lower baseline <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F4"/>b). dCRE <inline-formula><mml:math id="M123" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP and dCRE <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are largely negative with similar magnitude in both SSP1 and PD in the first two days (Fig. <xref ref-type="fig" rid="F4"/>c and d). Additionally, the lowest magnitude for dCRE <inline-formula><mml:math id="M125" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP on each day is for SSP3. On day 3, there are strong fluctuations in dCRE <inline-formula><mml:math id="M126" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP and dCRE <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> due to strong cumulus activity (Fig. <xref ref-type="fig" rid="F4"/>c, d). The substantially higher dCRE on day 3 for SSP1 is the outcome of strong positive LWP and <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution due to cumulus activity which is stochastic in nature and thus cannot be directly attributed as a response to aerosol perturbation. A more detailed discussion on ACI after separating the effects of climate change will be presented in Sect. <xref ref-type="sec" rid="Ch1.S4"/>.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e2191">Time series of changes in CRE due to aerosol perturbation in the dry FT cases and its contributions from changes to <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWP, and <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(a)</bold> dCRE, <bold>(b)</bold> <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE, <bold>(c)</bold> LWP contribution to dCRE, <bold>(d)</bold> <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE. <inline-formula><mml:math id="M133" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the cloud optical thickness. The legend is shown in panel <bold>(d)</bold>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f04.png"/>

        </fig>

<table-wrap id="T2" specific-use="star"><label>Table 2</label><caption><p id="d2e2270">Cloud radiative effect enhancement (dCRE <inline-formula><mml:math id="M134" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CRE<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">baseline</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">CRE</mml:mi><mml:mrow><mml:mi mathvariant="normal">aerosol</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">perturbation</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) and its decomposition at the TOA for all cases. The budgeting is done using cloud properties for a threshold of <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>&gt;</mml:mo></mml:mrow></mml:math></inline-formula> 1. The quantity for each day is averaged between sunrise and sunset. Column RES is the residual of the dCRE budget. RES <inline-formula><mml:math id="M137" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> dCRE <inline-formula><mml:math id="M138" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> sum of dCRE components. A smaller value for RES suggests a uniform cloud field. Note that a positive value for dCRE indicates cloud brightening.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="17">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right" colsep="1"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right"/>
     <oasis:colspec colnum="12" colname="col12" align="right" colsep="1"/>
     <oasis:colspec colnum="13" colname="col13" align="right"/>
     <oasis:colspec colnum="14" colname="col14" align="right"/>
     <oasis:colspec colnum="15" colname="col15" align="right"/>
     <oasis:colspec colnum="16" colname="col16" align="right"/>
     <oasis:colspec colnum="17" colname="col17" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">case</oasis:entry>
         <oasis:entry colname="col2">ID</oasis:entry>
         <oasis:entry rowsep="1" namest="col3" nameend="col7" align="center" colsep="1">day 1 (W m<sup>−2</sup>) </oasis:entry>
         <oasis:entry rowsep="1" namest="col8" nameend="col12" align="center" colsep="1">day 2 (W m<sup>−2</sup>) </oasis:entry>
         <oasis:entry rowsep="1" namest="col13" nameend="col17" align="center">day 3 (W m<sup>−2</sup>) </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">dCRE</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">LWP</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">RES</oasis:entry>
         <oasis:entry colname="col8">dCRE</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col10">LWP</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col12">RES</oasis:entry>
         <oasis:entry colname="col13">dCRE</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col15">LWP</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col17">RES</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Moist</oasis:entry>
         <oasis:entry colname="col2">PD</oasis:entry>
         <oasis:entry colname="col3">3.7</oasis:entry>
         <oasis:entry colname="col4">4.9</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M148" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.6</oasis:entry>
         <oasis:entry colname="col6">0.2</oasis:entry>
         <oasis:entry colname="col7">1.2</oasis:entry>
         <oasis:entry colname="col8">3.8</oasis:entry>
         <oasis:entry colname="col9">22.4</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M149" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>24.9</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M150" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1</oasis:entry>
         <oasis:entry colname="col12">6.4</oasis:entry>
         <oasis:entry colname="col13">177.0</oasis:entry>
         <oasis:entry colname="col14">39.0</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>36.6</oasis:entry>
         <oasis:entry colname="col16">148.4</oasis:entry>
         <oasis:entry colname="col17">26.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">SSP1</oasis:entry>
         <oasis:entry colname="col3">4.3</oasis:entry>
         <oasis:entry colname="col4">6.0</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M152" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.8</oasis:entry>
         <oasis:entry colname="col6">0.2</oasis:entry>
         <oasis:entry colname="col7">1.0</oasis:entry>
         <oasis:entry colname="col8">16.9</oasis:entry>
         <oasis:entry colname="col9">32.6</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M153" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>14.6</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M154" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6</oasis:entry>
         <oasis:entry colname="col12">0.6</oasis:entry>
         <oasis:entry colname="col13">188.3</oasis:entry>
         <oasis:entry colname="col14">31.8</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M155" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30.6</oasis:entry>
         <oasis:entry colname="col16">173.5</oasis:entry>
         <oasis:entry colname="col17">13.6</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">SSP3</oasis:entry>
         <oasis:entry colname="col3">2.6</oasis:entry>
         <oasis:entry colname="col4">3.9</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M156" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.4</oasis:entry>
         <oasis:entry colname="col6">0.6</oasis:entry>
         <oasis:entry colname="col7">1.5</oasis:entry>
         <oasis:entry colname="col8">9.0</oasis:entry>
         <oasis:entry colname="col9">18.3</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M157" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.2</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M158" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.0</oasis:entry>
         <oasis:entry colname="col12"><inline-formula><mml:math id="M159" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.1</oasis:entry>
         <oasis:entry colname="col13">137.2</oasis:entry>
         <oasis:entry colname="col14">33.6</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M160" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>32.0</oasis:entry>
         <oasis:entry colname="col16">120.1</oasis:entry>
         <oasis:entry colname="col17">15.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Dry</oasis:entry>
         <oasis:entry colname="col2">PD</oasis:entry>
         <oasis:entry colname="col3">5.7</oasis:entry>
         <oasis:entry colname="col4">10.4</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M161" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.9</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M162" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5</oasis:entry>
         <oasis:entry colname="col7">0.7</oasis:entry>
         <oasis:entry colname="col8">6.8</oasis:entry>
         <oasis:entry colname="col9">15.7</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M163" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.3</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M164" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.9</oasis:entry>
         <oasis:entry colname="col12">0.3</oasis:entry>
         <oasis:entry colname="col13">5.6</oasis:entry>
         <oasis:entry colname="col14">10.3</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M165" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.3</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M166" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5</oasis:entry>
         <oasis:entry colname="col17">1.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">SSP1</oasis:entry>
         <oasis:entry colname="col3">4.1</oasis:entry>
         <oasis:entry colname="col4">10.9</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M167" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.8</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M168" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.7</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M169" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.2</oasis:entry>
         <oasis:entry colname="col8">7.2</oasis:entry>
         <oasis:entry colname="col9">17.0</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M170" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.3</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M171" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.5</oasis:entry>
         <oasis:entry colname="col12"><inline-formula><mml:math id="M172" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1</oasis:entry>
         <oasis:entry colname="col13">13.3</oasis:entry>
         <oasis:entry colname="col14">11.1</oasis:entry>
         <oasis:entry colname="col15">5.0</oasis:entry>
         <oasis:entry colname="col16">3.2</oasis:entry>
         <oasis:entry colname="col17"><inline-formula><mml:math id="M173" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">SSP3</oasis:entry>
         <oasis:entry colname="col3">0.3</oasis:entry>
         <oasis:entry colname="col4">5.1</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M174" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.9</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M175" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.7</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M176" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1</oasis:entry>
         <oasis:entry colname="col8">1.9</oasis:entry>
         <oasis:entry colname="col9">11.5</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M177" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.1</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M178" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.9</oasis:entry>
         <oasis:entry colname="col12"><inline-formula><mml:math id="M179" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.3</oasis:entry>
         <oasis:entry colname="col13">2.0</oasis:entry>
         <oasis:entry colname="col14">8.1</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M180" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.9</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M181" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5</oasis:entry>
         <oasis:entry colname="col17">1.2</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>CRE: Role of climate change</title>
      <p id="d2e3081">It is tempting to interpret the differences between scenarios in dCRE (Figs. <xref ref-type="fig" rid="F2"/> and <xref ref-type="fig" rid="F4"/>) as an outcome of changes in ACI due to climate change. Instead, these trends are a combination of warming-induced changes and aerosol-induced changes. To better understand this, we quantify the effects of climate change on the unperturbed (with respect to aerosol) state of the cloud. This will aid us in separating the effect of aerosol perturbation from that of climate change.</p>
      <p id="d2e3088">The impact of climate change on CRE in cases with moist and dry humidities is shown in Fig. <xref ref-type="fig" rid="F5"/>, which depicts the difference in CRE between PD conditions and EoC conditions (dCRE<sub>clm</sub>). We only consider the cases without aerosol perturbation for calculating dCRE<sub>clm</sub>. A positive value indicates cloud brightening. Note that dCRE<sub>clm</sub> is different from dCRE in Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>). The latter represents the change in CRE due to aerosol perturbation.</p>

      <fig id="F5"><label>Figure 5</label><caption><p id="d2e3124">Changes in CRE due to climate change. The color code is same as in Figs. <xref ref-type="fig" rid="F1"/> and <xref ref-type="fig" rid="F3"/>. The panel at the top (bottom) represents the moist (dry) FT case. Note that the changes are relative to the PD scenario without aerosol perturbation. A negative value indicates cloud darkening due to climate change.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f05.png"/>

        </fig>

      <p id="d2e3138">In the moist FT case, the magnitude of the CRE decreases (cloud darkening) before the onset of strong precipitation in both warming scenarios. This is associated with the reduction in LWP and <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> through the effects of warming SST (due to climate change) and the weakening of radiative cooling at cloud-top <xref ref-type="bibr" rid="bib1.bibx8" id="paren.52"/>. The resulting positive low-cloud feedback is consistent with other LES <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx8" id="paren.53"/> and observational studies <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx14 bib1.bibx15 bib1.bibx25" id="paren.54"/>. As expected, to leading order, the darkening is stronger for SSP3, though SSP1 shows similar reductions on day 2 due to precipitation losses (Fig. <xref ref-type="fig" rid="F1"/>f) in LWP and <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F1"/>b and c). On day 3, after the cloud breakup, the magnitude of dCRE<sub>clm</sub> decreases substantially. Note that SSP1 has a slightly higher magnitude on day 3 as precipitation starts earlier. Furthermore, we also see that dCRE<sub>clm</sub> is positive on day 4 in SSP1 due to the higher residual <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e3206">In the dry FT case, precipitation does not play a prominent role until after sunset on day 3. Until then, SSP3 exhibits the largest darkening. After the onset of cumulus activity (<inline-formula><mml:math id="M190" display="inline"><mml:mo lspace="0mm">≥</mml:mo></mml:math></inline-formula> 65 h on day 3), the magnitude of dCRE<sub>clm</sub> reduces to near zero. However, slow cloud breakup in SSP3 due to low LWP results in a positive value for dCRE<sub>clm</sub> (brightening). Overall, the dry FT case exhibits larger (negative) dCRE<sub>clm</sub> compared to the moist FT case and therefore warrants further scrutiny. In particular, we need to understand the impact of climate change on <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP.</p>
      <p id="d2e3254">Figure <xref ref-type="fig" rid="F6"/> depicts the fractional changes in LWP and <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> due to climate change. While we show the results for both SSP1 and SSP3, for ease of discussion we focus on SSP3. In moist FT case, the fractional reduction in <inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP is substantial. On day 1, the reduction in <inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ranges between 5 % and 10 % and increases to 20 %–25 % on day 2. The reduction in LWP is around 20 % on day 1 and less than 5% on day 2. (Note that we are only considering the time period before the onset of precipitation, i.e., before sunset on day 2.) In the dry FT case, the reduction in <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is higher than its moist counterpart (around 30 % to 35 % on days 1 and 2). However, the reduction in LWP is lower compared to the moist case (less than 10 % on day 1). These results indicate that the extent of reduction in <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> due to climate change is a function of LWP.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3317">Fractional changes in LWP (top) and <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (bottom) due to climate change. The color code is shown in panel <bold>(a)</bold> and is same as in Figs. <xref ref-type="fig" rid="F1"/> and <xref ref-type="fig" rid="F3"/>. The panels to the left represent the moist FT case and the panels to the right represent the dry FT case. Note that the changes are relative to the equivalent present day scenario. These are average values for each day. Two values per day represent the two averaging periods, between sunrise and sunset (first data point), and sunset to sunrise (second data point).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Marine cloud brightening</title>
      <p id="d2e3352">One of the main themes of this study is to evaluate the effect of climate change on the efficacy of marine cloud brightening. To address this, we look at changes to the TOA radiative fluxes. Figure <xref ref-type="fig" rid="F7"/> shows time-averaged SWUP flux (panels to the left) and the long-wave upward flux (LWUP) (panels to the right) at the TOA for all cases simulated in this study. There are two data points for each day, each representing the average values between sunrise and sunset and between sunset and sunrise. The top panels represent the moist FT case and the bottom panels represent the dry FT case. In the SSP1 and SSP3 scenarios, the enhancement in SWUP flux due to aerosol perturbation (difference between hatched bars and solid bars) is smaller than the reduction associated with climate change. The effects of positive cloud feedback reduce the brightening prospects of marine low-clouds in the absence of precipitation (see Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/>).</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e3361">Bar plots representing average SWUP (panels to the left) and LWUP (panels to the right) flux at the TOA for each scenario in the moist (top panels) and dry (bottom panels) FT cases. For each day, two average values are reported per scenario. The averaging period for each data point is between sunrise and sunset and between sunset and sunrise. The color code is shown in the top-right panel. The plain and hatched bar plots represent the cases without and with aerosol perturbation, respectively. Note that the vertical axis is different for <inline-formula><mml:math id="M201" display="inline"><mml:mover accent="true"><mml:mi mathvariant="normal">SWUP</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> and <inline-formula><mml:math id="M202" display="inline"><mml:mover accent="true"><mml:mi mathvariant="normal">LWUP</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>. </p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f07.png"/>

        </fig>

      <p id="d2e3390">Suppression of precipitation leads to substantial enhancement in SWUP flux. Some of this enhancement is offset by the reduction in the outgoing LW radiation due to a rise in cloud top height (see the panels to the right in Figs. <xref ref-type="fig" rid="F7"/> and <xref ref-type="fig" rid="F1"/>f). Despite this, in all climate scenarios, suppression of precipitation leads to an enhancement in SWUP flux that is substantially greater than the unperturbed PD scenario, as the effects of cloud feedback are weaker after the cloud breaks up to open-cellular clouds. However, the net enhancement in SWUP flux due to precipitation suppression is not immune to climate change. For instance, in the moist FT case, the highest enhancement in <inline-formula><mml:math id="M203" display="inline"><mml:mover accent="true"><mml:mi mathvariant="normal">SWUP</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is for the PD and SSP1 scenarios due to the greater <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> during daytime on day 3 (Fig. <xref ref-type="fig" rid="F7"/>a).</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Aerosol–cloud interactions in a warmer climate</title>
      <p id="d2e3429">In this section, we explore a framework to separate the effects of climate change on the cloud properties from those of aerosol perturbation. Changes in SW CRE due to aerosol injection (dCRE) are shown in Figs. <xref ref-type="fig" rid="F2"/> and <xref ref-type="fig" rid="F4"/>, and the daytime average values are shown in Table <xref ref-type="table" rid="T2"/>. The decomposition of dCRE into individual contributions from <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWP, and <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is given by Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>). The Twomey contribution dCRE <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the LWP contribution dCRE <inline-formula><mml:math id="M208" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP to dCRE are both proportional to unpertured (with respect to aerosol) <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Furthermore, these components of dCRE are proportional to changes in the cloud albedo due to <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (or LWP) while LWP (or <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is held constant (unperturbed state). The <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution, dCRE <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, is a more complex component of dCRE as it is a function of changes in both <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and total cloud albedo post aerosol perturbation. Under moist FT conditions, the magnitude of dCRE <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is negligible until the onset of precipitation (see first two days in Fig. <xref ref-type="fig" rid="F2"/>). Then, to leading order, in the absence of substantial <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> changes, dCRE can be expressed as the sum of dCRE <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and dCRE <inline-formula><mml:math id="M218" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> LWP

          <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M219" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub><mml:mo mathvariant="italic">{</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:msub><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mi>N</mml:mi></mml:msub><mml:msub><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:munder></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:msub><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:mrow></mml:munder><mml:mo mathvariant="italic">}</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

        If we factor out <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from the above expression, we obtain

          <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M222" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mo>+</mml:mo><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">c</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">aP</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        The first term on the right side of Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) is the change in cloud albedo due to the changes in <inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> while LWP is kept unchanged and the second term is the change in cloud albedo due to the changes in LWP while <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is kept unchanged.</p>
      <p id="d2e3866">The components of albedo changes based on Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) are shown in Fig. <xref ref-type="fig" rid="F8"/> for moist and dry FT cases. There is a remarkable collapse for the <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contributions across different scenarios in both cases (Fig. <xref ref-type="fig" rid="F8"/>a and b). We see minor differences between SSP1 and the other two scenarios, which we attribute to the lower aerosol concentration in SSP1 and associated entrainment feedbacks. In the moist FT case, we see a strong deviation in the SSP1 scenario on day 2 due to suppression of weak precipitation. Apart from these minor differences, the collapse in the <inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> albedo component extends to clouds with strong precipitation as well (days 3 and 4). In the dry FT case, we see a substantial spread in the <inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> albedo component between the scenarios only on day 4. This is related to differences in the timing of the onset and intensity of precipitation across scenarios (Fig. <xref ref-type="fig" rid="F3"/>f).</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e3913">Components of cloud albedo changes due to aerosol perturbation in the moist (left column) and dry (right column) cases. The panels at the top (bottom) show the <inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (LWP) component in Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>). The color code is shown in panel <bold>(a)</bold>.</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f08.png"/>

      </fig>

      <p id="d2e3939">The LWP albedo contribution time series is quite noisy and the collapse across different scenarios is less remarkable compared to the <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> component (Fig. <xref ref-type="fig" rid="F8"/>c and d). Note that unlike <inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the LWP adjustment to aerosol perturbation is not instantaneous and could range from a few to several hours <xref ref-type="bibr" rid="bib1.bibx16" id="paren.55"/>. The critical role of meteorology in determining these time scales is poorly understood. These differences in the LWP adjustment timescale could explain the improved (lower scatter) collapse in the LWP component of the albedo changes in the scenarios with dry FT compared to the equivalent moist FT scenarios in the first two days. Nevertheless, to leading order, there is reasonable collapse across scenarios in both cases on the first two days, and the collapse extends to the third and fourth day in the moist FT scenarios. In the dry FT case, we see a substantial spread across scenarios on days 3 and 4 due to the onset of cumulus activity and precipitation, respectively (Fig. <xref ref-type="fig" rid="F8"/>d).</p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
      <p id="d2e3980">In the previous two sections, we explored the effects of climate change on SCT and ACI in the North-East Pacific region. We analyzed two cases of SCT (i) a precipitation-mediated transition, and (ii) an entrainment-driven transition. These cases were created by altering the humidity in the FT, with the high humidity case [the reference case in <xref ref-type="bibr" rid="bib1.bibx35" id="altparen.56"/>] resulting in strong precipitation and the low humidity case resulting in low or negligible precipitation. These cases were subjected to different climate  and aerosol perturbations. The results show that until the onset of precipitation the effect of aerosol perturbation is much weaker than the effects of climate change. However, in precipitating cloud systems, the effects of aerosol-induced precipitation suppression dominate over the effects of climate change. In addition, we explore the impact of climate change on the onset of cumulus activity and cloud breakup. The results show that the onset of cumulus activity is not affected by climate change under dry FT conditions and occurs around noon on day 3 (around 66 h). However, the cloud breakup times are different, with the earliest in SSP1, followed by PD and then SSP3. In the moist FT case, SSP3 results in an early onset of cumulus activity (around 42 h) and cloud breakup (around 45 h).</p>
      <p id="d2e3986">The insights gained from this study would help address the efficacy of MCB as a potential climate intervention strategy to reduce global mean temperature. Our results show that there is a substantial decrease in <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the warmer world (SSP1 and SSP3 scenarios). This is also supported by the long-term observation trend <xref ref-type="bibr" rid="bib1.bibx29" id="paren.57"/>. In particular, in our simulations we find that the cases with a drier FT appear to be more susceptible to warming-induced <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> reduction. All of this points to a significant reduction in the potential efficacy of MCB as climate change progresses. Thus, from an operational perspective, it would be more effective if MCB were to be deployed sooner rather than later, thus buying additional time for decarbonization technologies to become viable.</p>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Impact of climate change</title>
      <p id="d2e4021">Our results in Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/> show that in the stratocumulus regime, the dry FT case exhibits a stronger effect of climate change on CRE. We attribute this to the shielding effect of higher LWP in the moist FT case. In all scenarios in Figs. <xref ref-type="fig" rid="F1"/> and <xref ref-type="fig" rid="F3"/>, a substantial reduction in <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> does not start until the LWP reaches a sufficiently low value <xref ref-type="bibr" rid="bib1.bibx32" id="paren.58"/>. In simpler terms, cloud thinning precedes reduction in <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Consequently, the higher LWP in the moist FT case shields <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from the effects of weakened radiative cooling and climate-change-induced warming. The lower LWP in the dry FT case results in a stronger reduction in <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Since CRE, to leading order, is controlled by <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, until the onset of precipitation, dCRE<sub>clm</sub> is higher in the dry FT case.</p>
      <p id="d2e4098">In the moist FT case, after cloud breakup, the fractional changes in <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP are low, resulting in low dCRE<sub>clm</sub> (Fig. <xref ref-type="fig" rid="F5"/>). After precipitation-induced breakup, the cloud layer transitions into an open-cellular structure and has the characteristics of a surface driven cloud system (e.g. cumulus clouds) <xref ref-type="bibr" rid="bib1.bibx41" id="paren.59"/>. Thus, the low value for dCRE<sub>clm</sub> post cloud breakup is consistent with the locally weak low-cloud feedback seen in marine cumulus clouds <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx40 bib1.bibx19 bib1.bibx28" id="paren.60"/>.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Aerosol–cloud interactions</title>
      <p id="d2e4148">The similarity in the values for <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP components of albedo change across climate scenarios in both dry and moist FT cases is, at first sight, puzzling as the impact of climate change on LWP and, by extension, the cloud albedo is clearly evident from the time series plots in Figs. <xref ref-type="fig" rid="F1"/>b and <xref ref-type="fig" rid="F3"/>b. It is important to note that the bulk of the reduction in cloud LWP due to climate change is visible post-sunset and before sunrise. Interestingly, after sunrise, the impact of climate change on cloud LWP decreases as clouds with higher LWP are more susceptible to SW absorption <xref ref-type="bibr" rid="bib1.bibx31" id="paren.61"/>. During this time, the dominant effect of climate change on CRE is evident from the changes in <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/>). Thus, by factoring out <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>) we are eliminating (to leading order) the effects of climate change on dCRE in non-precipitating marine low-clouds.</p>
      <p id="d2e4196">The similarity we see here appears to be case-specific as there is no universality among these albedo change time series between the moist and dry FT cases. This local similarity suggests that in stratocumulus clouds, changes in albedo contributions from <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP are immune to climate change, i.e., the magnitude of Twomey effect and LWP adjustments do not change within the cloudy region. The scenario-specific differences we see in the dCRE components in Table <xref ref-type="table" rid="T2"/> and Figs. <xref ref-type="fig" rid="F2"/> and <xref ref-type="fig" rid="F4"/> are an outcome of warming-induced changes to the unperturbed state (mainly <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of the cloud system and not an outcome of the impact of climate change on ACI.</p>
      <p id="d2e4227">We have established that the <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP components of <inline-formula><mml:math id="M248" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> are, to leading order, invariant under climate change. If we know the magnitude of the albedo adjustment in the non-precipitating stratocumulus clouds in the present day, then we can estimate the magnitude of CRE adjustment in a warmer climate provided we know <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> under warmer conditions. <xref ref-type="bibr" rid="bib1.bibx11" id="text.62"/> have established that changes in the CRE of stratocumulus clouds due to planetary warming can be approximated as a linear combination of changes in meteorological factors. This linear approximation has also been used in several recent observational studies <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx28 bib1.bibx14 bib1.bibx25" id="paren.63"/>. We extend this to account for <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and express changes in CRE in non-precipitating clouds under climate change as

            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M251" display="block"><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>=</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:munderover><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>M</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents <inline-formula><mml:math id="M253" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>th cloud-controlling meteorological factor and <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></inline-formula>. As discussed earlier, our results suggest that <inline-formula><mml:math id="M255" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> is invariant under climate change. We leave it to future studies to assess the validity of this hypothesis using a larger dataset (observational or simulation).</p>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Stratocumulus-to-cumulus transition</title>
      <p id="d2e4461">It is important to note that the low-cloud transitions investigated here are (i) precipitation-mediated (moist FT): from a closed marine startocumulus cloud deck to an open cellular low-cloud layer, and (ii) entrainment-driven (dry FT): the transition from a marine stratocumulus cloud deck to a cumulus-under-stratocumulus cloud deck. Technically, in both cases, the transition to a cumulus-topped boundary layer is not yet complete.</p>
      <p id="d2e4464">In the precipitation-mediated transition, climate change affects the onset of the transition. The transition is initiated earlier in SSP3 than in PD. Note that both cases have similar aerosol number concentration at the start, and so microphysics is unlikely to explain the difference in initiation time. The boundary layer decoupling is stronger in the SSP3 scenario compared to the PD scenario due to weakened radiative cooling at cloud-top and increased surface latent heat flux <xref ref-type="bibr" rid="bib1.bibx9" id="paren.64"/>. This is also supported by the buoyancy integral ratio (BIR) time series in Fig. <xref ref-type="fig" rid="F9"/>a. BIR is a ratio between the magnitudes of the negative buoyancy flux in the sub-cloud layer and the positive buoyancy flux in the boundary layer <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx9" id="paren.65"/>. A higher BIR value indicates a stronger decoupling. Note that the level of decoupling is higher in SSP3 especially during the night on day 1. The magnitude of decoupling increases in strength on day 2, which eventually leads to the earlier onset of cumulus activity on day 2. The stronger decoupling in SSP3 is also evident from the jump in the magnitude of the cloud base variance around 43 h (Fig. <xref ref-type="fig" rid="F1"/>e). The earlier onset of cumulus activity eventually leads to the early onset of precipitation-induced breakup. An earlier transition also occurs in the SSP1 case, but this is driven by both the lower aerosol concentration and the effects of climate change.</p>

      <fig id="F9"><label>Figure 9</label><caption><p id="d2e4479">Buoyancy integral ratio (BIR) for <bold>(a)</bold> moist FT scenarios, and <bold>(b)</bold> dry FT scenarios. The color code is shown in panel <bold>(a)</bold>. The vertical arrows at the top of each panel represent the cloud base precipitation onset time. The length of these arrows is a relative measure of the precipitation intensity.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/5151/2026/acp-26-5151-2026-f09.png"/>

        </fig>

      <p id="d2e4498">In the entrainment-driven case, the effects of climate change do not influence the onset of the cumulus clouds. However, the onset of breakup, which is influenced by precipitation, is affected by the effects of warming through changes in LWP. The substantial reduction in LWP in the SSP3 scenario delays the onset and weakens the intensity of precipitation. This results in brighter clouds in the SSP3 case post-transition. This is in contrast to the behavior prior to the transition. It is puzzling that unlike in the scenarios with moist FT, climate change does not affect the onset of cumulus activity in the dry scenarios despite changes in the cloud properties. A possible explanation for this could be that the lower humidity in the FT ensures that radiative cooling at the cloud top is large enough to preserve the structure of the marine boundary layer (MBL) despite the effects of climate change. The BIR time series in Fig. <xref ref-type="fig" rid="F9"/>b for the dry FT case shows that there is a certain degree of decoupling during the day on the first two days and the extent of decoupling increases from day 1 to day 2. However, after sunset, the boundary layer is recoupled in all scenarios during this time period. On day 3, the decoupling gets a lot stronger in all scenarios, which eventually results in cumulus activity. Note that in the scenarios with moist FT a certain level of decoupling is maintained in the boundary layer even after sunset on all days until the onset of precipitation. Comparison of BIR time series in both cases supports the hypothesis that substantially lower radiative cooling of the boundary layer in the moist FT case (83 W m<sup>−2</sup> in moist FT and 113 W m<sup>−2</sup> in dry FT) makes the onset of cumulus activity more susceptible to climate change. However, more case studies are required to assess the robustness of this conclusion.</p>
      <p id="d2e4527">The injection of aerosol delays the breakup of the stratocumulus deck in both moist and dry FT cases by delaying the onset of precipitation in cumulus-cloumns. This leads to substantial brightening of the cloud deck in all climate scenarios. However, the onset of cumulus activity in both cases is largely unaffected by aerosol perturbation (all scenarios in dry FT and SSP3 in moist FT) unless influenced by precipitation formation (PD and SSP1 in moist FT).</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Summary and Outlook</title>
      <p id="d2e4539">In this study, we explored aerosol-cloud interactions (ACI) in a warmer climate in marine low-clouds using Lagrangian (domain advecting with mean wind) large-eddy simulations (LES) coupled to two-moment, bin-emulating bulk microphysics models. We used the well-explored composite reference case from <xref ref-type="bibr" rid="bib1.bibx35" id="text.66"/> to set up the stratocumulus-to-cumulus transition (SCT) simulations. In this case, precipitation plays a prominent role in the transition (precipitation-mediated transition) <xref ref-type="bibr" rid="bib1.bibx45" id="paren.67"/>. Since not all SCTs are driven by precipitation, we created another case with reduced FT humidity. The humidity was reduced to 27 % of the value in the composite reference case in <xref ref-type="bibr" rid="bib1.bibx35" id="text.68"/>. This resulted in a case where the onset of cumulus activity was driven by the classical entrainment-deepening of the marine boundary layer (entrainment-driven transition). The equivalent cases for warmer conditions at the end-of-the-century were created following the methodology laid out in <xref ref-type="bibr" rid="bib1.bibx8" id="text.69"/>. The large-scale forcings for this setup were obtained from the latest coupled model intercomparison project (CMIP6) data. We considered two shared socioeconomic pathways (SSP) from CMIP6: (i) SSP1-2.6: this is the best-case scenario with a sustainable future with clean up, and (ii) SSP3-7.0: fossil-fueled growth due to regional rivalry.</p>
      <p id="d2e4554">Our results showed that the effect of climate change on the cloud radiative effect (CRE) dominates over the effect of aerosol perturbation prior to the onset of precipitation in both precipitation-mediated and entrainment-driven cases. In particular, the impact of climate change is much stronger in the entrainment-driven case compared to the precipitation-mediated case. This is because of the higher LWP in the precipitation-mediated case, which shields the cloud fraction (<inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) from erosion against the weakened radiative cooling and warming effects associated with climate change. Interestingly, the impact of climate change is muted once the cloud deck is broken up into open-cellular cumulus clouds.</p>
      <p id="d2e4568">We also explored the impact of climate change on the onset of cumulus activity, as quantified using the variance in cloud base height. In the moist FT case (precipitation-mediated), the effects of climate change resulted in an earlier onset of cumulus activity, which advanced the onset of precipitation-induced cloud breakup in a strongly warmer climate (SSP3). In the dry FT case (entrainment-driven), the onset of cumulus activity appeared immune to the effects of climate change. Our analysis indicated that the weaker radiative cooling associated with higher humidity in the FT makes the boundary layer less coupled in the precipitation-mediated case. Further weakening of radiative cooling associated with climate change enhances the decoupling of the boundary layer, resulting in an earlier onset of cumulus activity. A substantially higher cooling rate at cloud-top in the entrainment-driven case (due to the lower humidity in the FT) maintained a well-mixed boundary layer in all cases until the onset of cumulus activity on day 3. In this case, a similarity in the onset time of cumulus clouds does not translate into a similarity in the onset time of cloud breakup. In a strongly warmer climate (SSP3), the onset of cloud breakup is substantially delayed due to its lower LWP and weaker precipitation intensity. In both moist and dry FT cases, aerosol injection delayed the breakup of the stratocumulus layer through precipitation-suppression, thus substantially enhancing the magnitude of CRE in all scenarios.</p>
      <p id="d2e4571">The central focus of our study was to assess the impact of climate change on ACI in marine low-clouds. Our analysis showed that the <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP components of the cloud albedo changes due to aerosol perturbation are similar under the influence of climate change. Thus, in non-precipitating clouds, to leading order, changes in CRE due to aerosol perturbation (dCRE) normalized by <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are constant under the influence of climate change. However, the albedo contributions associated with precipitation-suppression are coupled to changes in both <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and cloud albedo, and are not immune to climate change. Despite this similarity in the ACI in a warmer climate in non-precipitating clouds, the efficacy of marine cloud brightening (MCB) reduces substantially towards the end-of-the-century due to the reduction in cloud fraction associated with the effects of climate change. Moreover, the dCRE in precipitating clouds also decreases due to the effects of climate change. Thus, if considered, a practical implementation of MCB would be more efficient sooner rather than later.</p>
      <p id="d2e4608">The simulations carried out here are based on an idealized SCT case study built from a 2-year (summer-time) composite trajectory that does not account for all the real-world complexity and variations (e.g., changes in wind speed), and an active coupling between the tropics and the sub-tropics. <xref ref-type="bibr" rid="bib1.bibx18" id="text.70"/>, employing a weak-temperature gradient framework, report that such coupling could affect the results presented here. However, there is still much uncertainty in how to realistically represent such coupling in a warmer climate in Lagrangian LES of the kind used here. Additionally, the insights from the current study and similar LES studies are only relevant in assessing ACI in the initial phase of MCB. Sustained MCB will result in significant changes in large-scale climatology and background aerosol concentration. Furthermore, evaporation of the sprayed seawater can alter the dynamics of the boundary layer, affecting the efficacy of MCB <xref ref-type="bibr" rid="bib1.bibx23" id="paren.71"/>. To overcome these challenges, future studies should focus on an ensemble of trajectories based on realistic conditions in the present and warmer world to assess the impact of climate change on the efficacy of MCB, changes in ACI, and SCT. These studies would aid in assessing the generality of the key hypotheses from the current study – (i) in non-precipitating clouds, changes in CRE due to aerosol perturbation when normalized by <inline-formula><mml:math id="M262" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, are invariant under climate change, and (ii) the efficacy of MCB decreases in a warmer climate due to the reduction in cloud fraction.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d2e4632">The simulations were carried out using SAM (<uri>https://wiki.harvard.edu/confluence/display/climatemodeling/SAM</uri>, last access: 30 July 2021). The data from the simulations are available from the NOAA Chemical Sciences Laboratory's Clouds, Aerosol, &amp; Climate program webpage at <uri>https://csl.noaa.gov/groups/csl9/datasets/data/2026-Prabhakaran-etal/</uri> (last access: 4 February 2026).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e4644">PP and GF designed the research with inputs from TM. PP carried out the simulations and analysis. PP, TM, FH, and GF discussed the results. PP wrote the manuscript with input from TM, FH and GF.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e4650">At least one of the (co-)authors is a member of the editorial board of <italic>Atmospheric Chemistry and Physics</italic>. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e4659">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="d2e4665">Prof. Marat Khairoutdinov graciously provided the SAM model. PP thanks Dr. Jan Kazil and Dr. Isabel McCoy for their inputs in setting up the warmer world simulations.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e4670">This research was supported by the U.S. Department of Commerce, Earth's Radiation Budget grant, NOAA CPO Climate and CI no. 03-01-07-001. FH appreciates support from the Emmy Noether program of the German Research Foundation (DFG) under grant HO 6588/1-1.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e4676">This paper was edited by Anna Possner and reviewed by two anonymous referees.</p>
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