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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article">
  <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-26-14111-2026</article-id><title-group><article-title>Estimating Twomey forcing sensitivity  to aerosol plume spreading rates</article-title><alt-title>Estimating Twomey forcing sensitivity to aerosol plume spreading rates</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>McMichael</surname><given-names>Lucas A.</given-names></name>
          <email>mcmic@uw.edu</email>
        <ext-link>https://orcid.org/0000-0003-0980-370X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Erfani</surname><given-names>Ehsan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7364-1912</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wood</surname><given-names>Robert</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1401-3828</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>von Salzen</surname><given-names>Knut</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>University of Washington, Seattle, WA, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Desert Research Institute, Reno, NV, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Lucas A. McMichael (mcmic@uw.edu)</corresp></author-notes><pub-date><day>9</day><month>October</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>19</issue>
      <fpage>14111</fpage><lpage>14132</lpage>
      <history>
        <date date-type="received"><day>13</day><month>May</month><year>2026</year></date>
           <date date-type="rev-request"><day>27</day><month>May</month><year>2026</year></date>
           <date date-type="rev-recd"><day>4</day><month>September</month><year>2026</year></date>
           <date date-type="accepted"><day>22</day><month>September</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Lucas A. McMichael 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/26/14111/2026/acp-26-14111-2026.html">This article is available from https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e116">The amount of sunlight that reaches Earth's surface can be reduced by increasing cloud droplet number and decreasing droplet size (i.e., Twomey forcing), a central idea underpinning the Marine Cloud Brightening strategy. Cloud albedo depends nonlinearly on cloud droplet concentration, meaning the spatial extent of aerosol plumes could be an important constraint on the brightening potential. In this study, horizontal aerosol spreading is simulated using a Langevin particle model driven by a library of realistic, 2 d Large Eddy Simulations (LES) spanning the meteorological and aerosol phase space of northeast Pacific stratocumulus. The 2D reflectance fields from the LES are superimposed onto the 2D perturbed aerosol concentrations to calculate the 2D Twomey forcing response.</p>

      <p id="d2e119">The Day 1 and Day 2 LES regimes have distinct meteorological, aerosol, and turbulence characteristics associated with equatorward movement of the LES domain. Our results indicate that the Day 2 regime has substantially faster plume spreading than Day 1, with ensemble median differences exceeding 2 km h<sup>−1</sup>. Despite these differences, Twomey forcing is insensitive to the natural variability in spreading rate. This study suggests that Twomey forcing is resilient to variations in meteorology, aerosols, and turbulence, with its efficacy governed primarily by aerosol lifetime and assumptions surrounding cloud adjustments. Although the natural variation in spreading rate does not materially affect Twomey forcing, idealized plume spreading simulations suggest that current GCM assumptions of an infinitely fast spreading rate could lead to a 10 %–200 % overestimation of cooling.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Cooperative Institute for Climate, Ocean, and Ecosystem Studies, University of Washington</funding-source>
<award-id>NA22OAR4310474</award-id>
<award-id>NA20OAR4320271</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Simons Foundation</funding-source>
<award-id>SFI-MPS-SRM-00005157</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="d2e143">In perturbed aerosol conditions, such as freshly emitted ship tracks or theoretical Marine Cloud Brightening (MCB) deployments, the Twomey effect can reduce the amount of sunlight that reaches Earth's surface by producing more, smaller droplets for a fixed liquid water path, acting as a cooling agent in the climate system <xref ref-type="bibr" rid="bib1.bibx57 bib1.bibx58 bib1.bibx36" id="paren.1"/>. In both ship tracks and MCB scenarios, the aerosols are emitted from point sources that spread laterally and vertically over time, with the spatial distribution of the aerosol concentration being an important control on the brightening potential <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx62" id="paren.2"/>. The horizontal spreading of marine boundary layer aerosol plumes has received little attention in the literature <xref ref-type="bibr" rid="bib1.bibx29" id="paren.3"/>, with only a few studies in recent decades exploring horizontal spreading rate variability and behavior <xref ref-type="bibr" rid="bib1.bibx19 bib1.bibx59 bib1.bibx6 bib1.bibx40 bib1.bibx46 bib1.bibx41" id="paren.4"/>. In previous explorations of MCB feasibility and regional impact studies <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx48 bib1.bibx30 bib1.bibx31" id="paren.5"/>, global climate models (GCMs) used uniform subgrid aerosol concentrations, making the implicit assumption of an infinitely fast spreading rate. Provided the non-linear Twomey forcing behavior as a function of concentration, the potential consequences of infinite spreading rates in GCMs could be non-trivial. Recently, kilometer-scale regional simulations of ship tracks have enabled explicit representation of some aspects of plume spreading <xref ref-type="bibr" rid="bib1.bibx56" id="paren.6"/>. Although these models currently overestimate cooling <xref ref-type="bibr" rid="bib1.bibx56" id="paren.7"/>, they remain a promising tool for constraining Twomey forcing.</p>
      <p id="d2e168">The in-plume cloud droplet concentrations, which can impact cloud properties such as liquid water path (LWP) and cloud fraction, are not solely a function of horizontal and vertical plume spreading. Cloud droplet activation processes are highly dependent on the aerosol size, number, vertical velocity, and supersaturation <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx62" id="paren.8"/>. The relationship between cloud droplet concentrations and cloud evolution (aerosol-cloud-radiation interactions) has been a topic of extensive research over the past several decades and remains one of the leading sources of uncertainty in estimates of climate sensitivity <xref ref-type="bibr" rid="bib1.bibx4" id="paren.9"/>. LES explorations of individual ship tracks have suggested that precipitating, clean background aerosol cases augment cooling efficiency through increases in LWP and cloud fraction, with more polluted conditions having smaller, or even negative cloud adjustments <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx46" id="paren.10"/>.</p>
      <p id="d2e180">When trying to constrain cloud adjustments from observations, separating the confounding influence of meteorological variability from the cloud responses to aerosols represents a major challenge <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx28 bib1.bibx51" id="paren.11"/>. After attempting to control for meteorological variability, several studies find that radiative forcing changes driven by cloud adjustments are relatively weak compared to the Twomey forcing <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx17 bib1.bibx13" id="paren.12"/>. In contrast, <xref ref-type="bibr" rid="bib1.bibx27" id="text.13"/> found that after accounting for cloud morphology, Twomey forcing and cloud adjustments can offset one another, highlighting the potential importance of targeting MCB to focus on the most susceptible cloud regimes. Cloud adjustment sensitivity often diverges between precipitating and non-precipitating environments <xref ref-type="bibr" rid="bib1.bibx25" id="paren.14"/>. However, cloud buffering mechanisms such as the cloud-radiation-turbulence-entrainment feedback have the theoretical potential to limit such sensitivity <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx70 bib1.bibx61" id="paren.15"/>. This study does not explore cloud adjustments and makes the assumption that the Twomey forcing is the dominant radiative component; nevertheless, cloud adjustments remain a critical knowledge gap in the estimation of MCB forcing from both simple and sophisticated modeling frameworks.</p>
      <p id="d2e198">Beyond the aerosol concentration variability driven by plume spreading, the population of particles available for both transport and activation is governed by the aerosol lifetime, which is modulated by processes such as wet/dry scavenging, entrainment sources/sinks, sedimentation, and coagulation. In precipitating clouds, coalescence scavenging has been shown to be the dominant mechanism determining aerosol lifetime <xref ref-type="bibr" rid="bib1.bibx60" id="paren.16"/>, but GCMs show a wide spread in the relative importance of various dry and wet deposition mechanisms <xref ref-type="bibr" rid="bib1.bibx54" id="paren.17"/>. There have been relatively few attempts to estimate aerosol lifetimes with prognostic aerosol-enabled LES, but <xref ref-type="bibr" rid="bib1.bibx14" id="text.18"/> found that the e-folding timescale of 205 nm dry diameter ammonium sulfate aerosols in non-precipitating cases may be 2–3 d, which is substantially longer than the few hours estimated from observations of ship tracks <xref ref-type="bibr" rid="bib1.bibx25" id="paren.19"/>. In this work, we probe the sensitivity of Twomey forcing to a range of aerosol lifetimes.</p>
      <p id="d2e214">The horizontal spreading of aerosols injected from a point source into the marine boundary layer can be reasonably modeled by Langevin particle models (LPMs) <xref ref-type="bibr" rid="bib1.bibx52 bib1.bibx40" id="paren.20"/>, which depend on turbulence characteristics (i.e., variances and dissipation rates) and precipitation rates, since precipitating boundary layers have been shown to initiate spread-accelerating two-cell mesoscale circulations in large-eddy simulations (LESs) <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx40 bib1.bibx41" id="paren.21"/>. Since LES explicitly resolves much of the energy-containing motion within the boundary layer, velocity variances and dissipation rates are directly accessible from the resolved flow field. These turbulence fields can be used to simulate point source injections in a turbulence environment that originally did not contain aerosol perturbations. In cases where the interaction between the plume and turbulence is strong, such as precipitating boundary layers, the particle model is able to capture the impacts of spread-accelerating mesoscale features using only domain-averaged input parameters through a change in the precipitation-dependent free parameter (<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). The turbulence information that drives the Langevin particle model, along with background aerosol concentrations, boundary layer depth, precipitation rates, and cloud reflectance fields are derived from a library of realistic, 2 d LES cases based on Lagrangian trajectories, designed to span the meteorological and aerosol phase space of northeast Pacific stratocumulus.</p>
      <p id="d2e234">The following analysis is restricted to a subset of the full LES library (54 simulations), focusing on the cloudy LES cases (17 simulations with median cloud fraction <inline-formula><mml:math id="M3" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 50 %) that most closely match satellite observations of reflected shortwave energy and represent likely candidate environments for MCB. Additionally, the LPM has not been thoroughly tested in low cloud fraction or cumulus boundary layers. The purpose of this research is to characterize the spreading rate behavior in these cloudy boundary layers across a range of environments and determine how differences in spreading rate, macrophysics, and microphysics may impact the Twomey forcing. In order to do this, the 2D reflectance fields from the LES are superimposed on the 2D aerosol concentrations simulated by the Langevin particle model to calculate the Twomey forcing in each LPM grid column. Given the non-linear dependence of cloud albedo on cloud droplet concentration, variations of spreading rates, cloud morphologies, boundary layer depths, and background aerosol concentrations may lead to complex responses of the Twomey forcing.</p>
      <p id="d2e244">To date, plume spreading explorations have been limited to a few idealized LES cases, non-overlapping plumes, and 1–3 d simulation times. The computational effectiveness of the Langevin particle model allows for an exploration of a range of ship track densities, motion, and organization that would be difficult to replicate with LES. This work represents a natural extension of <xref ref-type="bibr" rid="bib1.bibx62" id="text.22"/>, where cloud morphologies and environmentally dependent spreading rates are now taken into account. Additionally, this study examines the sensitivity of Twomey forcing to aerosol lifetime (Sect. 3.3), injection timing, and duration (Sect. 3.4). The Twomey forcing is decomposed into contributions from particles of different age groups, as well as different aerosol concentration bins (Sect. 3.5). We discuss potential impacts of plume spreading assumptions in GCMs and develop a plume spreading parameterization that could be of use for global modelers (Sect. 3.6 and 3.7).</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methodology</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Large-eddy simulation library</title>
      <p id="d2e266"><xref ref-type="bibr" rid="bib1.bibx22" id="text.23"/> developed a methodology to explore the meteorological and aerosol phase space of northeast Pacific (NEP) clouds by analyzing eight primary cloud-controlling factors from the European Center for Medium-Range Weather Forecasts (ECMWF) reanalysis version 5 (ERA5) along 2 d Lagrangian trajectories during summer 2018–2021 from six source locations (source locations shown in Fig. <xref ref-type="fig" rid="F1"/>d). The factors were the trajectory mean 700 hPa water vapor mixing ratio, 700 hPa vertical velocity in pressure coordinates, estimated inversion strength (EIS), and 10 m wind speed, along with the corresponding changes (end minus beginning) in each variable over the trajectory. After performing principal component analysis on 1663 Lagrangian trajectories, <xref ref-type="bibr" rid="bib1.bibx22" id="text.24"/> showed that the first two principal components (PC1 and PC2) explain 43 % of the variance in the cloud controlling factors. At each of the six source locations, 9 trajectories spanning the PC1–PC2 phase space were also shown to reasonably capture the observed variability in surface pressure, liquid water path (LWP), droplet concentrations (<inline-formula><mml:math id="M4" 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>), background aerosol concentration (<inline-formula><mml:math id="M5" 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>), boundary layer depth, and precipitation <xref ref-type="bibr" rid="bib1.bibx22" id="paren.25"/>.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e303">Large eddy simulation library comparison with CERES observations of shortwave cloud radiative effects (SWCRE). <bold>(a)</bold> The normalized SWCRE bias between CERES and the LES simulation, calculated as SWCRE bias <inline-formula><mml:math id="M6" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> (LES SWCRE <inline-formula><mml:math id="M7" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> CERES SWCRE) <inline-formula><mml:math id="M8" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> CERES SWCRE) with a negative normalized bias indicating that the LES scenes are less reflective than the observations. The blue shaded region is the IQR and the black line is the median for cases with median cloud fraction above 50 % for the duration of the simulation, <bold>(b)</bold> the normalized SWCRE bias for cases with median cloud fraction below 50 %, <bold>(c)</bold> raw values of SWCRE from each of the 17 cloudy LES cases (circles) and from CERES (squares) averaged over the 2 daytime periods, with the circle color corresponding the 48 h averaged low cloud cover percentage and the dashed line showing the SWCRE bias (axis on the right, with positive values indicating an underestimation of SWCRE), <bold>(d)</bold> the cloudy LES domain trajectories for Day 1 in blue and Day 2 in red.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f01.png"/>

        </fig>

      <p id="d2e346">All 54 simulations were carried out with the System for Atmospheric Modeling <xref ref-type="bibr" rid="bib1.bibx35" id="paren.26"/>, version 6.10.9, with the same model configuration outlined in <xref ref-type="bibr" rid="bib1.bibx22" id="text.27"/> that is enabled with a two-moment, prognostic aerosol scheme <xref ref-type="bibr" rid="bib1.bibx5" id="paren.28"/>. Initial ERA5 temperature and moisture profiles required an inversion sharpening procedure to better align with microwave LWP observations and compensate for the coarse representation of inversion structure in ERA5 <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx22" id="paren.29"/>. During a 12 h, nocturnal spin-up period, temperature and moisture nudging within the boundary layer was applied on a 1 h timescale. In <xref ref-type="bibr" rid="bib1.bibx22" id="text.30"/>, boundary layer <inline-formula><mml:math id="M9" 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> was initialized with the Modern Era Retrospective analysis for Research and Applications, version 2 (MERRA2) reanalysis product <xref ref-type="bibr" rid="bib1.bibx24" id="paren.31"/>, but MERRA2 boundary layer <inline-formula><mml:math id="M10" 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> is known to exhibit biases relative to aircraft measurements <xref ref-type="bibr" rid="bib1.bibx21" id="paren.32"/>. For all 54 of the LES library members, the initial MERRA2 boundary layer <inline-formula><mml:math id="M11" 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> values at each height level are corrected using the Clouds and the Earth's Radiant Energy System (CERES; <xref ref-type="bibr" rid="bib1.bibx18" id="altparen.33"/>) <inline-formula><mml:math id="M12" 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> estimates using

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M13" display="block"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi>a</mml:mi><mml:mi>c</mml:mi><mml:mi>o</mml:mi><mml:mi>r</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:msub><mml:mi>F</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">acorr</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the CERES-corrected MERRA2 <inline-formula><mml:math id="M15" 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> value and <inline-formula><mml:math id="M16" 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 the correction factor defined as

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M17" display="block"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          with <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being the assumed activation fraction, that is set to 80 % in accordance with previous studies <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx53" id="paren.34"/>, <inline-formula><mml:math id="M19" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is the average of CERES-<inline-formula><mml:math id="M20" 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> during the first day of the trajectory, and <inline-formula><mml:math id="M21" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is the average of MERRA2-<inline-formula><mml:math id="M22" 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> during the first day of the trajectory and over the entire boundary layer depth. Details on how CERES <inline-formula><mml:math id="M23" 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 calculated based on measurements of cloud optical depth and effective radius are given in <xref ref-type="bibr" rid="bib1.bibx43" id="text.35"/>. MERRA2 <inline-formula><mml:math id="M24" 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> is calculated from the mass mixing ratios of aerosol species, following the methodology described in Appendix A of <xref ref-type="bibr" rid="bib1.bibx21" id="text.36"/>.</p>
      <p id="d2e626">After the 12 h initialization stage, the simulations are allowed to evolve freely within the boundary layer for 48 h, forced with time-varying ERA5 large-scale vertical velocity, large-scale temperature/moisture advective tendencies, geostrophic winds, and sea surface temperatures along each trajectory. Free tropospheric aerosols, temperature, moisture are nudged on an hourly timescale and winds are nudged on a 12 h timescale. The horizontal domain is 51.2 km <inline-formula><mml:math id="M25" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 51.2 km with a uniform horizontal grid spacing of 100 m. The vertical grid uses 7 m between 450 and 1200 m, and then gradually coarsens above and below this range, so that it is <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> m near the model top at 4.8 km and 20 m near the ocean surface.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>LES library case selection</title>
      <p id="d2e654">When examining the shortwave cloud radiative effect (SWCRE), the bias between the LES library simulations and CERES-derived SWCRE indicates a clear dependence on cloud fraction (Fig. <xref ref-type="fig" rid="F1"/>a and b). Since SWCRE is negative, a negative CERES-normalized bias indicates that the LES is underestimating the magnitude of SWCRE relative to the CERES-derived value. Cases with median cloud fractions above 50 % along the 2 d trajectory have substantially weaker normalized SWCRE biases than cases with median cloud fraction below 50 % (Fig. <xref ref-type="fig" rid="F1"/>a and b), with biases generally smaller than 50 % for cloudy cases. Among the 54 LES simulations, 17 cases have median cloud fractions above 50 %, with 3 LES cases overestimating cloud reflectivity relative to CERES, 6 cases within 20 W m<sup>−2</sup>, and 8 cases underestimating cloud reflectivity by 20–65 W m<sup>−2</sup> when examining the average over the two daytime periods (Fig. <xref ref-type="fig" rid="F1"/>c).</p>
      <p id="d2e687">Potential sources of persistent LES–observation biases are numerous, including uncertainties in the initialization of boundary-layer and free-tropospheric aerosol, as well as unresolved large-scale adjustment processes, domain-size and grid-spacing limitations. The goal of the present study is not to diagnose the root causes of these discrepancies, but instead to focus on the best performing cases and the most plausible candidates for MCB. Using the 17 cloudy cases, we build a representative summertime climatology of the Day 1 and Day 2 portions of the Lagrangian LES trajectories (Fig. <xref ref-type="fig" rid="F1"/>d) spanning distinct aerosol, meteorological, and turbulence regimes, and use it to estimate the sensitivity of Twomey forcing to aerosol plume spreading rates. A manuscript describing the full ensemble's performance, behavior, and key characteristics is currently in preparation.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Langevin particle model</title>
      <p id="d2e700">Given our objective of evaluating many different ship sprayer densities, aerosol lifetime assumptions, injection timings/durations, and sprayer motions, performing large-domain LES for all of these variations across the LES library is cost prohibitive. For this reason, estimating the horizontal spreading of ship tracks requires a more computationally efficient approach. As an alternative to explicitly modeling fluid motion and aerosol transport in physical space using the filtered Navier-Stokes equations solved on a numerical grid, as done in the LES, fluid flow can be described statistically by building probability distributions of individual stochastic particle trajectories that are governed by the following simplified Langevin equation described in <xref ref-type="bibr" rid="bib1.bibx45" id="text.37"/> and <xref ref-type="bibr" rid="bib1.bibx40" id="text.38"/>: 

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M29" display="block"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msubsup><mml:mi>U</mml:mi><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:msubsup><mml:mi>U</mml:mi><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msubsup></mml:mrow><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>L</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:mi mathvariant="normal">deterministic</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">drift</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">term</mml:mi></mml:mrow></mml:munder><mml:mo>+</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>L</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:msqrt><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>W</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:mi mathvariant="normal">Brownian</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">motion</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">term</mml:mi></mml:mrow></mml:munder><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msubsup><mml:mi>U</mml:mi><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is the individual horizontal particle acceleration in m s<sup>−2</sup>, <inline-formula><mml:math id="M32" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is the boundary layer mean environmental velocity in m s<sup>−1</sup>, <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> is the boundary layer mean horizontal velocity variance in m<sup>2</sup> s<sup>−2</sup>, and <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>W</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the random walk increment in s<sup>1∕2</sup>. This study focuses on the horizontal spreading of ship tracks, meaning Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) is solved independently for the <inline-formula><mml:math id="M39" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M40" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> components. The relaxation timescale (<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is defined as

            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M42" display="block"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>L</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">3</mml:mn><mml:mn mathvariant="normal">4</mml:mn></mml:mfrac></mml:mstyle><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mi mathvariant="italic">ε</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> [m<sup>2</sup> s<sup>−3</sup>] is the boundary layer-averaged turbulence dissipation rate and <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is a free parameter <xref ref-type="bibr" rid="bib1.bibx40" id="paren.39"/>. <xref ref-type="bibr" rid="bib1.bibx40" id="text.40"/> found that <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> requires tuning to account for an anisotropic two-cell mesoscale circulation that develops within ship tracks in precipitating environments. The <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> parameter takes on one of two values depending on the surface precipitation rate (<inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">sfc</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in the LES (Eq. <xref ref-type="disp-formula" rid="Ch1.E5"/>), with lower values of <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increasing the relaxation timescale and spreading rates accordingly. Recent LES mechanism denial experiments suggest that precipitation suppression may not be the only mechanism that can initiate a spread-accelerating, two-cell mesoscale circulation, with cloud droplet sedimentation potentially being sufficient to drive the circulation in clean aerosol environments <xref ref-type="bibr" rid="bib1.bibx41" id="paren.41"/>. Nonetheless, we choose to maintain the precipitation threshold, considering the uncertainty of a potential background aerosol threshold and the lack of observational data on two-cell mesoscale circulation occurrence in ship tracks.

            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M51" display="block"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0.15</mml:mn></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="normal">if</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">sfc</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">mm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">d</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0.5</mml:mn></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="normal">if</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">sfc</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">mm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">d</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          In practice, higher order moments such as <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M53" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> are difficult to obtain or unavailable and are often parameterized in existing operational Langevin models such as FLEXPART <xref ref-type="bibr" rid="bib1.bibx52" id="paren.42"/>. However, these turbulence-related quantities are accessible in the LES and can be used to directly force the Langevin particle model. In previous work, the Langevin particle model driven by domain- and boundary layer-averaged <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M55" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> was found to reliably reproduce horizontal spreading rates in the LES under a range of turbulence and aerosol conditions <xref ref-type="bibr" rid="bib1.bibx40" id="paren.43"/>. As a result, the northeast Pacific library simulations, which do not include ship tracks, can be used in combination with the Langevin particle model to estimate the spreading rates that would occur if ship tracks were explicitly modeled in each LES simulation.</p>
      <p id="d2e1219">At each Langevin particle model time step (<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">600</mml:mn></mml:mrow></mml:math></inline-formula> s) a fixed number of particles are emitted, controlled by the number of sprayers (<inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) multiplied by the number of injected particles per sprayer (<inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>), with the total number of particles in each batch given by <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">batch</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Each modeled particle represents a multiplicity of particles (i.e., a superparticle). The number of real particles represented by each superparticle (<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">rep</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is given by

            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M61" display="block"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">rep</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">inj</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          with <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">inj</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being the injection rate, set to 10<sup>16</sup> particles per second. Superparticle positions are converted to perturbed aerosol concentrations (<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msubsup><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in # mg<sup>−1</sup>) with the following equation:

            <disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M66" display="block"><mml:mrow><mml:msubsup><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">rep</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">bin</mml:mi></mml:msub><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">bin</mml:mi></mml:msub><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">inv</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">mg</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          with <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> representing the number of binned superparticles with a bin size of <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<sup>2</sup> (<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">bin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">bin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">mg</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being the density in mg m<sup>−3</sup>. The vertical aerosol concentrations are assumed to be evenly distributed throughout the time-dependent boundary layer depth (<inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">inv</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) calculated from the LES library (Fig. <xref ref-type="fig" rid="F2"/>e), implying that each bin volume remains in a well-mixed state.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1538">Example snapshot of the particle model concentration-LES cloud field merging process with <bold>(a)</bold> being the particle model boundary layer-averaged perturbed aerosol concentration output at a given time, <bold>(b)</bold> the tiled unperturbed reflectance field (to match the domain size of the particle model) from the LES, and <bold>(c)</bold> the computed Twomey forcing using Eq. (<xref ref-type="disp-formula" rid="Ch1.E11"/>), with shortwave reflectance, LES background aerosol, and LPM perturbed aerosol concentrations used as the inputs.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f02.png"/>

        </fig>

      <p id="d2e1559">All particle model simulations were performed on a <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mn mathvariant="normal">200</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km<sup>2</sup> horizontal domain with doubly periodic boundary conditions. A <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mn mathvariant="normal">200</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km<sup>2</sup> domain was used to minimize artificial plume self-interaction under periodic boundary conditions on diurnal timescales and to capture changes in plume geometry, such as elongation and changes in plume-axis orientation, associated with ship motion and time-varying mean winds. The ship plumes are initialized with a Gaussian particle position distribution that has a standard deviation (<inline-formula><mml:math id="M79" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) of 1 km in both the <inline-formula><mml:math id="M80" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M81" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> dimensions and no initial velocity perturbations. Ship motions are determined randomly from a sample of 8 possible compass directions (N, NE, E, SE, S, SW, W, NW) with a default ship velocity of 10 m s<sup>−1</sup>. If a ship leaves the domain, its position and compass direction are randomly regenerated with the number of ships within the domain at any given time remaining fixed.</p>
      <p id="d2e1638">While the LES calculates wet scavenging within the aerosol microphysics, the impacts of scavenging processes (both wet and dry) are approximated in the particle model using a range of aerosol decay timescales (<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn></mml:mrow></mml:math></inline-formula>, 0.5, 1, 2 d), with the probability of a particle being removed (<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">removal</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) from the population given by the exponential decay function

            <disp-formula id="Ch1.E8" content-type="numbered"><label>8</label><mml:math id="M85" display="block"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">removal</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi mathvariant="normal">age</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where age<sup>*</sup> is the particle age calculated as the time elapsed since injection. Particles are removed randomly from each batch of released particles if <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">removal</mml:mi></mml:msub><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">batch</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>. This age-dependent removal represents the accumulated probability of removal processes over the history of a particle batch, rather than implying that particle age itself is the physical cause of removal.</p>
      <p id="d2e1731">The Day 1 and Day 2 portions of each trajectory are run separately and represent distinct meteorological regimes with differing boundary layer depths, precipitation, mean winds, background aerosol, and turbulence (see Sect. 3.1). To approximate equilibrium conditions representative of multi-day, repeated injections as expected in an MCB scenario, we repeat the 12 h daytime aerosol injection until the domain-mean peak aerosol concentration changes by less than 2 % between consecutive days. Under this criterion, the number of repeated diurnal cycles necessary for periodic equilibrium for <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn></mml:mrow></mml:math></inline-formula>, 0.5, 1, 2 d is 1, 2, 4, and 8 cycles (days), respectively. Interpolated LES fields are smoothed with a 3 h averaging window to avoid sharp discontinuities from morning to night. Unless stated otherwise, aerosol injections begin at sunrise each day and continue for 12 h each day. To derive plume widths and spreading rates from the LPM, a single batch of particles is released and the <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> width (single <inline-formula><mml:math id="M90" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> multiplied by 2) of the <inline-formula><mml:math id="M91" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M92" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> particle positions is calculated as done in <xref ref-type="bibr" rid="bib1.bibx40" id="text.44"/>, neglecting particle decay/removal.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>LES/LPM merging and Twomey forcing calculation</title>
      <p id="d2e1792">The Twomey forcing is diagnosed at 20 min intervals (the LES statistics output frequency) by merging the 2D LPM aerosol perturbation fields (<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msubsup><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>; Fig. <xref ref-type="fig" rid="F2"/>a), defined on the LPM grid (<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), with the radiative fields from each LES case, defined on the LES grid (<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">les</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">les</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). The LES output provides the net shortwave radiative flux at TOA (SW<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">net</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">les</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">les</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) and the total incoming shortwave insolation at TOA (<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">inc</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>), from which a scene reflectance (<inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">scene</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) can be computed using 

            <disp-formula id="Ch1.E9" content-type="numbered"><label>9</label><mml:math id="M101" display="block"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">scene</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="normal">SW</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">inc</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">inc</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">scene</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contains the detailed cloud morphology information available from the LES (Fig. <xref ref-type="fig" rid="F2"/>b).</p>
      <p id="d2e1990">The doubly periodic LES grid is tiled and clipped to match the size of the <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mn mathvariant="normal">200</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km<sup>2</sup> LPM domain. The <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">scene</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> field is then coarse-grained to map from 100 m grid spacing in the LES to the 1 km bin size in the LPM by averaging the <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mn mathvariant="normal">10</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> chunk of grid boxes from the LES. We denote the tiled, clipped, and coarse-grained LES field as <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">scene</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values below 0.07 are set to zero to limit the inclusion of clear-sky/ocean-like reflectances. An example snapshot of the 2D <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">scene</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> field is shown in Fig. <xref ref-type="fig" rid="F2"/>b.</p>
      <p id="d2e2093">Droplet concentration perturbations can be converted to changes in <inline-formula><mml:math id="M110" display="inline"><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> using Twomey's albedo susceptibility equation <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx62" id="paren.45"/>:

            <disp-formula id="Ch1.E10" content-type="numbered"><label>10</label><mml:math id="M111" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>)</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">n</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msubsup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">n</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msubsup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced close=")" open="("><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:msubsup><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">les</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">les</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:math></inline-formula>, with <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">les</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> being the time-dependent, boundary layer-averaged background accumulation mode aerosol concentration from the LES. Twomey forcing depends on <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>, but we make the assumption that all aerosol is activated so that <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. As mentioned in <xref ref-type="bibr" rid="bib1.bibx62" id="text.46"/>, the primary sensitivity in Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>) is the perturbation ratio term (<inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and not changes in <inline-formula><mml:math id="M117" display="inline"><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>. The reflectance changes (<inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi mathvariant="normal">lpm</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) are converted to the indirect shortwave radiative forcing (Twomey forcing) with

            <disp-formula id="Ch1.E11" content-type="numbered"><label>11</label><mml:math id="M119" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">grid</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">inc</mml:mi></mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          and an example snapshot of <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is shown in Fig. <xref ref-type="fig" rid="F2"/>c. The particle model <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is converted to global mean Twomey forcing (<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula>) by averaging <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> over all LPM grid boxes and times during the final 24 h period of the equilibrium LPM simulations and multiplying that value by the fraction of global surface area that is assumed to be actively sprayed (taken to be 3.147 %) with a given sprayer density. This assumes that the sprayed ocean area is <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mn mathvariant="normal">4000</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula> km<sup>2</sup> (4.4 % of the ocean area), consistent with recent global modeling studies targeting the most susceptible cloud regions, primarily the northeast and southeast Pacific during the summer months <xref ref-type="bibr" rid="bib1.bibx12" id="paren.47"/>. The primary ship densities explored in this paper represent low-end (<inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula>) and mid-range (<inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">16</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:math></inline-formula>) MCB deployments <xref ref-type="bibr" rid="bib1.bibx62" id="paren.48"/>, where we expect spreading rate impacts to potentially be most relevant. For <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mo>(</mml:mo><mml:mn mathvariant="normal">16</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">000</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> , there are 10 (40) sprayers active in the particle model domain during the injection period, corresponding to a ship density of <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup> (10<sup>−3</sup> ships per km<sup>2</sup>) with a characteristic sprayer spacing of <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">63</mml:mn></mml:mrow></mml:math></inline-formula> km (32 km). For comparison with <xref ref-type="bibr" rid="bib1.bibx62" id="text.49"/> and global modeling studies, it is helpful to define the injected salt mass rate (<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; Tg yr<sup>−1</sup>), assuming a geometric mean dry diameter (<inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of 100 nm, a geometric standard deviation (<inline-formula><mml:math id="M137" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>) of 1.6, the density of sodium chloride (<inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2160</mml:mn></mml:mrow></mml:math></inline-formula> kg m<sup>3</sup>), and <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">inj</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the following equation from <xref ref-type="bibr" rid="bib1.bibx62" id="text.50"/> can be solved

            <disp-formula id="Ch1.E12" content-type="numbered"><label>12</label><mml:math id="M141" display="block"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">inj</mml:mi></mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:msubsup><mml:mi>D</mml:mi><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup></mml:mrow><mml:mn mathvariant="normal">6</mml:mn></mml:mfrac></mml:mstyle><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">4.5</mml:mn><mml:mi>ln⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>S</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          with <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> Tg yr<sup>−1</sup> for <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> Tg yr<sup>−1</sup> for <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">16</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e2796">There are two critical assumptions underlying the offline coupling of the LPM aerosol field with LES reflectances. First, we assume that cloud adjustments are negligible, meaning that the primary control on the radiative flux is the Twomey forcing and not LWP and/or cloud fraction changes. Since the aerosol concentrations from the LPM are not fully coupled to the LES, processes like precipitation suppression <xref ref-type="bibr" rid="bib1.bibx3" id="paren.51"/>, entrainment enhancement related to smaller droplets and shifts in the radiative cooling profile <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx32" id="paren.52"/>, and potential cloud morphology changes associated with ship track/aerosol plume circulations <xref ref-type="bibr" rid="bib1.bibx59 bib1.bibx14 bib1.bibx46 bib1.bibx40 bib1.bibx41" id="paren.53"/> are not captured. As outlined in the introduction, there is considerable uncertainty regarding cloud adjustments in high aerosol/MCB environments, but a growing body of observational studies suggests that radiative impacts of cloud adjustments may be minor compared to the Twomey forcing on both regional <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx17" id="paren.54"/> and global scales <xref ref-type="bibr" rid="bib1.bibx13" id="paren.55"/>. In <xref ref-type="bibr" rid="bib1.bibx62" id="text.56"/>, the heuristic model used to estimate global Twomey forcing also assumed negligible cloud adjustments and was in broad agreement with existing LES of ship tracks.</p>
      <p id="d2e2819">Second, we assume that all injected aerosols are activated in cloudy regions (100 % activation fraction). This choice represents an upper-bound estimate of the Twomey forcing to highlight potential dependencies on plume spreading rates. In reality, activation will be sensitive to aerosol size, number, updraft velocity, and supersaturation, all of which vary in both space and time <xref ref-type="bibr" rid="bib1.bibx62" id="paren.57"/>. As a result of these assumptions, the forcing should be interpreted as the cloud-state-prescribed sensitivity of reflectance to droplet number, rather than a fully coupled response of the cloud field to the aerosol.</p>
      <p id="d2e2825">Despite the simplifying assumptions of negligible cloud adjustments and 100 % activation, the LES-LPM merging process represents complex, non-linear interactions by capturing the spatial overlap between aerosol perturbations and cloud reflectance fields. Given the stochastic nature of both the Langevin particle model and ship motion, some degree of run-to-run variability is expected; however, even at low sprayer densities (<inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2000</mml:mn></mml:mrow></mml:math></inline-formula>) the run-to-run variability in Twomey forcing is less than 3.5 %, suggesting LPM ensembles of each LES case are not necessary. The Twomey forcing is marginally sensitive to <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, with <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> producing 0.7 %–1.8 % less forcing than simulations using <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2000</mml:mn></mml:mrow></mml:math></inline-formula>.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Macrophysical, microphysical, and turbulence properties of cloudy LES cases</title>
      <p id="d2e2900">The cloudy LES cases evolve consistently with theoretical, modeling, and observational understanding of climatological changes along equatorward-moving trajectories, which typically involve decreasing cloud fraction, LWP, and accumulation mode aerosol (NA<sub>c</sub>), along with increasing surface precipitation occurrence, deepening boundary layers, and larger mesoscale cellular structures  <xref ref-type="bibr" rid="bib1.bibx66 bib1.bibx50 bib1.bibx49 bib1.bibx61 bib1.bibx20 bib1.bibx15 bib1.bibx67 bib1.bibx42 bib1.bibx8 bib1.bibx21" id="paren.58"/> (Fig. <xref ref-type="fig" rid="F3"/>).</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e2919">Time series of <bold>(a)</bold> cloud fraction, <bold>(b)</bold> liquid water path (LWP), <bold>(c)</bold> boundary layer-averaged accumulation mode aerosol (NA<sub><italic>c</italic></sub>), <bold>(d)</bold> surface rain rate, <bold>(e)</bold> inversion height, and <bold>(f)</bold> mesoscale cell size for the cloudy LES ensemble. The top panels show each individual LES simulation, while the bottom panels show the ensemble median (black line) and IQR (green shaded region). Bold black numbers correspond to Day 1 and Day 2 ensemble averages.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f03.png"/>

        </fig>

      <p id="d2e2956">Cloud fraction varies considerably between individual LES cases (captured by <inline-formula><mml:math id="M154" display="inline"><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>), experiencing abrupt changes at times, with collapses near midday and recoveries in the evening, in agreement with satellite observations of NEP clouds <xref ref-type="bibr" rid="bib1.bibx10" id="paren.59"/> (Fig. <xref ref-type="fig" rid="F3"/>a). The median cloud fraction on Day 2 of the trajectories is <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> % lower than Day 1 during the midday hours (Fig. <xref ref-type="fig" rid="F3"/>a), representing a gently transitioning environment rather than the full stratocumulus-to-cumulus transition where cloud fractions would be expected to be much lower. The LWP evolution generally mirrors the cloud fraction behavior (Fig. <xref ref-type="fig" rid="F3"/>b) and agrees well with satellite and aircraft observations, with peak LWP near the morning hours and minimum LWP in the late evening <xref ref-type="bibr" rid="bib1.bibx65 bib1.bibx42" id="paren.60"/>. The median boundary layer-averaged NA<sub>c</sub> is on the order of 100 # mg<sup>−1</sup> on Day 1 as observed during the CSET campaign <xref ref-type="bibr" rid="bib1.bibx8" id="paren.61"/>, which declines by nearly half on Day 2 (Fig. <xref ref-type="fig" rid="F3"/>c). Surface precipitation is minimal on Day 1, but becomes much more common on Day 2, with several cases with surface rain rates greater than 1 mm d<sup>−1</sup> (Fig. <xref ref-type="fig" rid="F3"/>d). Initial median boundary layer depth is near 1 km, growing to nearly 1.5 km on Day 2, with a corresponding increase in the characteristic mesoscale cell size <xref ref-type="bibr" rid="bib1.bibx64" id="paren.62"/>, which is calculated by coarse-graining the horizontal velocity fields and counting the number of consecutive grid boxes of a given sign (Fig. <xref ref-type="fig" rid="F3"/>e and d). Mesoscale cell sizes are generally smaller than reported sizes in <xref ref-type="bibr" rid="bib1.bibx64" id="text.63"/>, which may be related to domain-size limitations in the LES. Figure S1 in the Supplement provides an example of the counting method used to calculate mesoscale cell size.</p>
      <p id="d2e3042">The particle model forcing from the LES also has distinct differences in boundary layer-averaged mean winds, velocity variances, and relaxation timescales (<inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) from Day 1 to Day 2 (Fig. <xref ref-type="fig" rid="F4"/>). Mean winds are consistent with regional climatological winds associated with persistent subtropical high pressure <xref ref-type="bibr" rid="bib1.bibx42" id="paren.64"/>, as initially stronger north/northeasterly winds slacken and become more easterly on Day 2 (Fig. <xref ref-type="fig" rid="F4"/>a and b).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e3065">Time series of <bold>(a)</bold> mean zonal velocity, <bold>(b)</bold> mean meridional velocity, <bold>(c)</bold> zonal variance, <bold>(d)</bold> meridional variance, <bold>(e)</bold> horizontal relaxation timescale, and <bold>(f)</bold> the decoupling parameter (<inline-formula><mml:math id="M160" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>) for the cloudy ensemble.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f04.png"/>

        </fig>

      <p id="d2e3100">Horizontal velocity variances show a clear diurnal cycle with maximum variances in the early morning hours and minimum variances in the late evening hours (Fig. <xref ref-type="fig" rid="F4"/>c and d) related to daytime solar absorption that suppresses TKE production and reduces entrainment <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx39" id="paren.65"/>. The IQR of horizontal variances narrows considerably during the evening hours on both Day 1 and Day 2, despite large differences in boundary-layer depth, precipitation, LWP, and cloud fraction among cases. This behavior supports the idea that the cloud-radiation-turbulence-entrainment feedback acts to limit intercase spread <xref ref-type="bibr" rid="bib1.bibx70" id="paren.66"/>. Larger LWP and deeper boundary layer cases have greater cloud-top negative buoyancy fluxes which drive stronger entrainment and may be more prone to drizzle, with both of these mechanisms promoting decoupling and limiting the ability of the cloud-top TKE production to be effectively mixed within the boundary layer. Thinner clouds have smaller cloud-top buoyancy fluxes, but can more easily mix TKE throughout the boundary layer depth. As a result, the IQR range of daytime LWP from 25–55 g m<sup>−2</sup> corresponds to a narrow range of boundary layer-mean horizontal variances <xref ref-type="bibr" rid="bib1.bibx39" id="paren.67"/>, with higher case-to-case variability in the early morning hours. On average, Day 2 has <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> % larger velocity variances than Day 1; however, Day 2 variances near sunrise are <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % larger than Day 1.</p>
      <p id="d2e3147">The relaxation timescale (<inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is almost a factor of 2 larger on Day 2 (Fig. <xref ref-type="fig" rid="F4"/>e), suggesting that all else equal, particles would revert back to the mean more slowly, resulting in faster Day 2 spreading. It is useful to define a decoupling parameter (<inline-formula><mml:math id="M165" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>) to quantify the extent of decoupling <xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx63" id="paren.68"/>,

            <disp-formula id="Ch1.E13" content-type="numbered"><label>13</label><mml:math id="M166" display="block"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">cl</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">sc</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">ft</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">sc</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          
          where <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">cl</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the total water mixing ratio in the cloud layer, subcloud layer (<inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">sc</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), and free troposphere (<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="normal">t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">ft</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>). As the boundary layer deepens on Day 2, <inline-formula><mml:math id="M170" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> increases by approximately 50 % across the ensemble (Fig. <xref ref-type="fig" rid="F4"/>f), consistent with observational estimates of decoupling in the northeast Pacific <xref ref-type="bibr" rid="bib1.bibx63" id="paren.69"/>. The <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> evolution is strongly correlated with the mesoscale cell size (<inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.59</mml:mn></mml:mrow></mml:math></inline-formula>) and the degree of decoupling (<inline-formula><mml:math id="M173" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>) (<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.32</mml:mn></mml:mrow></mml:math></inline-formula>), since the dissipation rate is sensitive to both flow geometry and stratification (Fig. S2).</p>
      <p id="d2e3346">In our merged LES-LPM modeling framework, cloud fraction, LWP, NA<sub>c</sub>, precipitation, boundary layer depth, mean winds, vertical velocity variances, and relaxation timescales may all influence Twomey forcing in nonlinear ways. As shown in Fig. <xref ref-type="fig" rid="F3"/>, the Day 1 and Day 2 states represent distinct meteorological, aerosol, and turbulence regimes along the trajectories and provide an opportunity to probe Twomey forcing sensitivity in each environment.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>LPM-derived plume spreading rates</title>
      <p id="d2e3368">Horizontal aerosol plume widths vary substantially with the turbulence forcing used in the LPM, with the slowest- and fastest-spreading cases in the cloudy LES library differing by as much as 80 km after 48 h (Fig. <xref ref-type="fig" rid="F5"/>a). Across the ensemble, plume width is well approximated by a linear growth rate of 1.5 km h<sup>−1</sup> (Fig. <xref ref-type="fig" rid="F5"/>b), consistent with existing LES estimates of lateral plume spreading <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx41" id="paren.70"/> and with the observational estimate of 1.85 km h<sup>−1</sup> reported by <xref ref-type="bibr" rid="bib1.bibx19" id="text.71"/>. Although the ensemble-median plume width is well described by a linear spreading rate, the instantaneous spreading rate exhibits a pronounced diurnal cycle (Fig. <xref ref-type="fig" rid="F5"/>c and d) associated with diurnal variations in the horizontal velocity variances and <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. There are several instances of plume spreading rates in excess of 3 km h<sup>−1</sup>, predominantly occurring in the early morning hours (Fig. <xref ref-type="fig" rid="F5"/>c). On average, Day 2 median spreading rates are 0.3 km h<sup>−1</sup> faster than Day 1 (<inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> % faster), but median spreading rates a few hours after sunrise vary by more than 1 km h<sup>−1</sup> (Fig. <xref ref-type="fig" rid="F5"/>d).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e3472">LPM-derived <bold>(a)</bold> LES case plume width, <bold>(b)</bold> LES library median and IQR plume width, <bold>(c)</bold> LES case plume spreading rate, and <bold>(d)</bold> LES library median and IQR plume spreading rate. Red dashed line on panel <bold>(b)</bold> corresponds to a 1.5 km h<sup>−1</sup> growth rate. Particle batch was released a time <inline-formula><mml:math id="M184" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0 h and tracked for 48 h.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f05.png"/>

        </fig>

      <p id="d2e3516">In the Twomey forcing sensitivity analyses that follow, the Day 1 and Day 2 LPM simulations are treated as distinct climatological regimes, with injections initiated at sunrise and active injections for 12 h each day until equilibrium concentrations are reached. To better quantify plume spreading differences between these regimes, spreading rates were calculated from particle batches released at sunrise each day. During most daylight hours, median Day 2 spreading rates exceed those on Day 1 by approximately 1–2 km h<sup>−1</sup> (Fig. <xref ref-type="fig" rid="F6"/>). At night, spreading rates are slightly higher on Day 1 than on Day 2 (Fig. <xref ref-type="fig" rid="F6"/>c). These results indicate that the two regimes differ not only in their background cloud and boundary layer properties, but also in the rate at which injected aerosol is dispersed, which has the potential to alter aerosol concentration probability distributions and the associated Twomey forcing. Day 2 has a higher incidence of surface precipitation, therefore, <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> values are adjusted accordingly. However, early morning spreading rates are controlled primarily by changes in variances and not <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. S3). After 5 or so hours after the start of the injection, precipitation-related changes in <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> result in a 0.5–1 km h<sup>−1</sup> acceleration of the plume spreading rate during the midday period (Fig. S3).</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3584">LPM-derived spreading rates for particle batches released at sunrise on Day 1 <bold>(a)</bold> and Day 2 <bold>(b)</bold>, <bold>(c)</bold> median spreading rates for Day 1 and Day 2 particle batches, and <bold>(d)</bold> the difference in median spreading rate (Day 2 <inline-formula><mml:math id="M190" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> Day 1).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Twomey forcing sensitivity to northeast Pacific climatology</title>
      <p id="d2e3620">Global mean forcing estimates (<inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula>) from the merged LPM-LES library are of the same order of magnitude as implied by the heuristic framework of <xref ref-type="bibr" rid="bib1.bibx62" id="text.72"/> for the same total injected mass, although larger. For example, at 8 Tg yr<sup>−1</sup>, <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d, and <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">16</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:math></inline-formula>, our model suggests <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.8</mml:mn></mml:mrow></mml:math></inline-formula> W m<sup>−2</sup> (Fig. <xref ref-type="fig" rid="F7"/>), compared with about 1 W m<sup>−2</sup> in <xref ref-type="bibr" rid="bib1.bibx62" id="text.73"/>. The difference likely arises because our sprayers are limited to 4.4 % of the ocean surface rather than distributed across the entire eligible ocean area (54 %) and the injections are occurring preferentially in cloudy regions. As an additional point of comparison, <xref ref-type="bibr" rid="bib1.bibx12" id="text.74"/> found that by selectively spraying eastern Pacific cloudy regions (<inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % of the ocean surface), nearly 1 °C of cooling was achieved. Assuming the mid-range injection scenario and <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d, <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.8</mml:mn></mml:mrow></mml:math></inline-formula> W m<sup>−2</sup> would impute a temperature sensitivity of 0.56 °C per W m<sup>−2</sup>, which is broadly consistent with GCM estimates of temperature sensitivity for spatially inhomogeneous forcing <xref ref-type="bibr" rid="bib1.bibx31" id="paren.75"/>. While the aim of this study is not to accurately determine <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula>, it is encouraging that the <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> magnitudes are within a plausible range.</p>

      <fig id="F7"><label>Figure 7</label><caption><p id="d2e3820">Global mean Twomey forcing (<inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula>) as a function of particle lifetime (<inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Green and orange markers correspond to the low-end MCB scenario with <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula> and blue and purple markers correspond to the mid-range MCB scenario with <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">16</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:math></inline-formula>. Each marker represents the ensemble average global mean Twomey forcing and the shading represents the interquartile range (IQR) of the ensemble.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f07.png"/>

        </fig>

      <p id="d2e3883">As shown in Fig. <xref ref-type="fig" rid="F7"/>, and consistent with <xref ref-type="bibr" rid="bib1.bibx62" id="text.76"/>, Twomey forcing increases in strength with longer <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, with the largest fractional increases in <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> associated with the shorter aerosol lifetimes. Quadrupling <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> only increases <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> by a factor of 2.1 at <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d (Fig. <xref ref-type="fig" rid="F7"/>), indicating a saturation in forcing efficiency as sprayer density increases. Day 1 and Day 2 <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> differ by less than 8 % for all values of <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and at both the low- and mid-range ship densities (<inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula>, 16 000) (Fig. <xref ref-type="fig" rid="F7"/>). This weak regime sensitivity suggests that for a fixed <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and negligible cloud adjustments, the deeper boundary layer and slightly more broken cloud conditions on Day 2 are approximately as susceptible to aerosol perturbations as the more overcast, shallower boundary layers on Day 1. The particle lifetime (set by <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is the leading-order control on global mean Twomey forcing given a fixed sprayer density.</p>
      <p id="d2e4017">It is not immediately clear which of the meteorological, aerosol, and turbulence variables are most responsible for the weak regime sensitivity. To assess their relative roles, we perform a sensitivity analysis in which Day 2 values of boundary-layer depth, cloud fraction/morphology, particle model turbulence forcing, mean winds, and background aerosol concentration are substituted individually into the corresponding Day 1 simulations for each case, while all other variables retain their Day 1 evolution. We then quantify the resulting change in <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> relative to the corresponding Day 1 control simulation.</p>
      <p id="d2e4030">Deeper boundary layers (which dilute the aerosol perturbation over a greater depth) and lower Day 2 cloud fractions both act to reduce Twomey forcing by 10 %–20 % relative to the Control, while the influence of mean winds is negligible (Fig. <xref ref-type="fig" rid="F8"/>a). The predominant factor counteracting these reductions is the cleaner background aerosol environment on Day 2, resulting in a nearly 50 % increase in Day 1 Twomey forcing (Fig. <xref ref-type="fig" rid="F8"/>a). Crucially, and of great relevance to this work, the Twomey forcing is insensitive to changes in the spreading rate between regimes (Fig. <xref ref-type="fig" rid="F8"/>a). However, while the domain-averaged forcing remains stable when particle forcing is swapped, the underlying aerosol concentration distributions are impacted, with faster spreading rates resulting in reduced frequency of the smallest concentrations and more frequent extreme concentrations (Fig. <xref ref-type="fig" rid="F8"/>b).</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e4043"><bold>(a)</bold> Twomey forcing sensitivity analysis for <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d and <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula>, where BLD is the boundary layer depth, CF is the cloud fraction/cloud reflectance, Turb is the particle model turbulence forcing that controls the spreading rate, which includes the <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> changes related to precipitation, MeanWind is the mean wind, and NA<sub>c</sub> is the background aerosol concentration. Positive percentages indicate that Day 2 values of a given variable act to increase Twomey forcing relative to Day 1 values. The circles represent each LPM simulation, the diamond is the ensemble mean, and the line is the ensemble median. <bold>(b)</bold> Average aerosol concentration probability distributions across all cases at local noon for the Control (Day 1 regime) and the Control run using Day 2 turbulence forcing in the particle model.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Twomey forcing sensitivity to sprayer motion, injection duration, and injection timing</title>
      <p id="d2e4115">To our knowledge, the sensitivity of MCB forcing to sprayer velocity has received little direct attention in the literature. Sprayer velocity is potentially important as it constrains platform design and dictates total energy demand, which could increase substantially if high operating velocities are required. Given a theoretical understanding of the diminishing returns of Twomey forcing at high concentrations, it seems logical to assume that higher ship velocities would spread aerosol over larger regions, thus increasing Twomey forcing efficiency. However, the LPM results indicate that the Twomey forcing is largely insensitive to the ship velocity, with velocities ranging from 0 to 10 m s<sup>−1</sup> changing <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> minimally (Fig. <xref ref-type="fig" rid="F9"/>a). While the area-averaged forcing of <inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>F</mml:mi></mml:mrow></mml:math></inline-formula> remains nearly constant, the spatial distribution of the perturbed aerosol concentration does change, most notably at ship velocities of 10 m s<sup>−1</sup>, with reduced occurrence of low concentrations and more frequent concentrations in the 20–80 # mg<sup>−1</sup> range (Fig. <xref ref-type="fig" rid="F9"/>b). By running the LPM simulations with no mean wind (<inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> in Eq. 3), the sensitivity to ship velocity emerges with ship velocities below 5 m s<sup>−1</sup> resulting in dramatically reduced cooling efficiency (Fig. <xref ref-type="fig" rid="F9"/>a). In the no mean wind scenario experiments, underlying probability distributions of aerosol concentrations begin to shift considerably, with the most susceptible Twomey forcing range experiencing reduced probabilities and a marked increase in concentrations above 200 # mg<sup>−1</sup> (Fig. <xref ref-type="fig" rid="F9"/>b). This finding suggests that in environments like the northeast Pacific, the energy and mechanical requirements of MCB could be meaningfully reduced by utilizing stationary or slow-moving platforms without compromising radiative efficacy. Of course, it remains possible that this result could be impacted by processes that control the vertical dispersion of aerosols in different environments (i.e., evaporation, local buoyancy perturbations) <xref ref-type="bibr" rid="bib1.bibx16" id="paren.77"/>. Simulations using uniformly-spaced sprayers moving in parallel, rather than randomly moving sprayers, indicate that Twomey forcing is also insensitive to ship organization (not shown).</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e4232"><bold>(a)</bold> Markers indicate the ensemble-averaged global mean Twomey forcing sensitivity to ship velocity for time-varying mean winds (Blue) and no mean wind (Red). Shading corresponds to the IQR of the ensemble. <bold>(b)</bold> Ensemble mean aerosol concentration probability distributions as a function of ship velocity and mean wind/no mean wind. Sensitivity tests using <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> d and <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f09.png"/>

        </fig>

      <p id="d2e4276">The global mean Twomey forcing scales roughly linearly with increasing injection duration, with the slope of the increase depending on the assumed value of <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F10"/>a). Longer <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is associated with higher sensitivity to the injection duration, with <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>a</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d resulting in 0.06 W m<sup>−2</sup> h<sup>−1</sup> of injection and <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> d resulting in 0.04 W m<sup>−2</sup> h<sup>−1</sup> of injection (Fig. <xref ref-type="fig" rid="F10"/>a). Given 50 % increases in Twomey forcing from 6 to 12 h injection duration, it is likely worthwhile to continue injecting well after the “peak” susceptibility window in the morning hours <xref ref-type="bibr" rid="bib1.bibx33" id="paren.78"/>. The sensitivity to injection timing is generally consistent with the modeling studies of <xref ref-type="bibr" rid="bib1.bibx33" id="text.79"/>, with 10 %–25 % enhancement in Twomey forcing achieved by injecting in the early mornings hours, versus a few hours after sunrise (Fig. <xref ref-type="fig" rid="F10"/>b).</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e4406">Ensemble-averaged global mean Twomey forcing as a function of <bold>(a)</bold> the daily injection duration for <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 1 and 2 d and <bold>(b)</bold> the injection timing relative to sunrise, for a 12 h daily injection. Shading corresponds to the IQR of the ensemble. Sensitivity tests use <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f10.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Twomey forcing as a function of particle age and concentration bin</title>
      <p id="d2e4456">The particle model allows for the explicit tracking of particle age and the associated Twomey forcing from each particle age group. With <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d, periodic equilibrium is reached after 8 d in the particle model, which means the maximum particle age is 8 d, despite the LES only having a run time of 2 d. Although not a strong function of <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> or case-to-case variability, the percentage of Twomey forcing from a given particle age group is strongly dependent on <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, as expected, with 3<inline-formula><mml:math id="M247" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> day old particles contributing to 2 % of the forcing when <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> d and 41 % of the forcing when <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> d (Fig. <xref ref-type="fig" rid="F11"/>a). Aerosols less than 1 d old are responsible for 25 %–65 % of the Twomey forcing, while aerosols 1–3 d old contribute close to 35 % across the <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> range (Fig. <xref ref-type="fig" rid="F11"/>a).</p>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e4551"><bold>(a)</bold> The percent of Twomey forcing as a function of particle age for <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 1, 2, and 4 d. <bold>(b)</bold> The percent of Twomey forcing from each particle concentration bin for <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d. Bold lines represent the LES ensemble mean percentage of total Twomey forcing (left <inline-formula><mml:math id="M254" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) and the dashed lines correspond to the cumulative percentage of Twomey forcing going from left to right in the bin space (right <inline-formula><mml:math id="M255" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis). Different colors are for different values of <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f11.png"/>

        </fig>

      <p id="d2e4632">In addition to particle age, we quantified the contribution of each particle concentration bin to the Twomey forcing. For each bin, Twomey forcing was summed over all particle model grid cells falling within that concentration range. The contribution from each bin was then expressed as a percentage of the domain-total Twomey forcing (Fig. <xref ref-type="fig" rid="F11"/>b). Our results reveal that for <inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1600</mml:mn></mml:mrow></mml:math></inline-formula>, only 10 %–15 % of the total Twomey forcing originates from concentration bins <inline-formula><mml:math id="M258" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 120 # mg<sup>−1</sup> assuming <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>a</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> d (Fig. <xref ref-type="fig" rid="F11"/>b), emphasizing the difficulty of detecting the Twomey-forcing relevant aerosol perturbations <xref ref-type="bibr" rid="bib1.bibx68" id="paren.80"/>, even in regions of relatively dense ship traffic. In the low-end MCB scenario (<inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4000</mml:mn></mml:mrow></mml:math></inline-formula>), only 20 % of the forcing originates from bins below 120 # mg<sup>−1</sup> (Fig. <xref ref-type="fig" rid="F11"/>b), making such a perturbation easily detectable.</p>
</sec>
<sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Theoretical importance of spreading rate for GCMs</title>
      <p id="d2e4738">We explore the maximum theoretical importance of spreading rate and quantify potential errors associated with assumptions made in GCMs (i.e., infinite spreading rate and uniform aerosol concentrations) using a changing particle model domain size with a single, fixed point source at the center of the domain. With doubly periodic boundary conditions, the changing domain size is a proxy for ship density. Cloud fraction is assumed to be unity, background aerosol is fixed at 20 # mg<sup>−1</sup>, and boundary layer depth is constant at 1 km, to maximize the potential importance of spreading rate. First, we examine the fastest (FAST) and slowest (SLOW) spreading cases in the LES library, which have daily average spreading rates of 3.18 and 0.2 km h<sup>−1</sup>, respectively. The difference between these two cases represents the upper bound on expected spreading-related Twomey forcing errors for naturally varying turbulence conditions, and the Twomey forcing magnitude and percentage differences are shown in Fig. <xref ref-type="fig" rid="F12"/>a and b. For <inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5000</mml:mn></mml:mrow></mml:math></inline-formula> or a ship density <inline-formula><mml:math id="M266" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.125</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup>, spreading rate-related Twomey forcing errors could potentially be in the 5 %–30 % range (Fig. <xref ref-type="fig" rid="F12"/>b). Beyond <inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">20</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.25</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup>), errors related to spreading rates are likely to be small.</p>

      <fig id="F12" specific-use="star"><label>Figure 12</label><caption><p id="d2e4868">The theoretical maximum importance of spreading rate explored using a changing domain size with a single, fixed point source at the center of the domain. Cloud fraction is assumed to be unity, background aerosol is fixed at 20 # mg<sup>−1</sup>, and boundary layer depth is constant at 1 km, to maximize the potential importance of spreading rate. <bold>(a)</bold> FAST-SLOW difference in global mean Twomey forcing, <bold>(b)</bold> FAST-SLOW percentage increase in global mean Twomey forcing, <bold>(c)</bold> INF-SLOW difference in global mean Twomey forcing, and <bold>(d)</bold> INF-SLOW percentage increase in global mean Twomey forcing. The different colored lines correspond to the different aerosol lifetime assumptions (<inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f12.png"/>

        </fig>

      <p id="d2e4913">To estimate an upper bound on potential Twomey forcing errors in GCMs, we compare the SLOW case to the assumption made in current GCM simulations of MCB, which is that the aerosol is instantaneously spread evenly throughout the grid box. The working assumption in current GCM implementations is that the spreading rate is infinitely fast (INF), with Fig. <xref ref-type="fig" rid="F12"/>c and d showing the Twomey forcing magnitude and percentage differences between the INF and SLOW cases. Errors become much more substantial when making the INF assumption, with ship densities below <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup> resulting in 10 %–200 % errors in global mean Twomey forcing, depending on <inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F12"/>d). Even at sprayer densities representative of high-end MCB scenarios, spreading-related Twomey forcing errors could exceed 10 % in environments where <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is less than 1 d (Fig. <xref ref-type="fig" rid="F12"/>d).</p>
      <p id="d2e4973">Additional idealized experiments indicate that concentration variability driven by random overlaps of ship tracks does not strongly impact the spreading rate and Twomey forcing relationship (Fig. S4). Using the median library spreading rate, instead of the extreme SLOW case, the expected spreading-related GCM errors for a mid-range MCB scenario (<inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayer</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:math></inline-formula>) would generally be 10 % or less (Fig. S5). In the context of a mid- to high-end MCB scenario, Twomey forcing is unlikely to be impacted substantially by differences in naturally occurring horizontal spreading rates, but the instantaneous spreading rate assumption may still lead to overestimates of cooling in GCMs. These errors, especially in short aerosol lifetime environments, can be reduced by assuming a fixed, finite spreading rate (e.g., <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> km h<sup>−1</sup>).</p>
</sec>
<sec id="Ch1.S3.SS7">
  <label>3.7</label><title>Statistical predictions of spreading rate from LES properties</title>
      <p id="d2e5024">Assuming a finite spreading rate in GCMs could ameliorate some of the spreading-related radiative forcing errors, but in some global injection scenarios sprayer density might be on the lower end of Fig. <xref ref-type="fig" rid="F12"/>, necessitating a more sophisticated approach to estimating the spreading rate within a GCM. One potential promising predictor of the particle model-derived spreading rate is the boundary layer-averaged horizontal TKE (TKE<sub>hor</sub>) multiplied by <inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which has diffusivity units (m<sup>2</sup> s<sup>−1</sup>) and explains nearly 50 % of the variance in spreading rate (Fig. <xref ref-type="fig" rid="F13"/>). When all times along the trajectories are included there is a clear time dependence of the spreading rate, with earlier times corresponding to faster spreading rates (Fig. <xref ref-type="fig" rid="F13"/>a). Bearing in mind this time-dependence, the statistical spreading rate relationships may need to vary as a function of time since injection. When the first 10 h of spreading are neglected, the TKE<inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">hor</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> quantity explains <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> % of the variance. In future work, relationships such as these may be implemented within the GCM as an effective plume spreading parameterization. In models that employ CLUBB, such as E3SM <xref ref-type="bibr" rid="bib1.bibx69" id="paren.81"/>, <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and TKE<sub>hor</sub> are readily available quantities, but their agreement with LES requires further investigation.</p>

      <fig id="F13" specific-use="star"><label>Figure 13</label><caption><p id="d2e5128">The statistical relationship between particle model-derived spreading rate and TKE<inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">hor</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for <bold>(a)</bold> all times and <bold>(b)</bold> all times excluding the first 10 h after injection. Colors change as a function of time since injection. Black lines indicate the power-law regression, with the equation and <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values provided in the upper right hand portion of the panels. All times from all cloudy LES ensemble members are shown.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14111/2026/acp-26-14111-2026-f13.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d2e5180">In this study, we employ a combination of 2 d, realistically time-varying Lagrangian large-eddy simulations (LES) and Langevin particle modeling (LPM) to investigate the importance of horizontal spreading rate, meteorological, and aerosol variability on Twomey forcing. The analysis focuses on the cloudy LES cases (17 cases with median cloud fraction <inline-formula><mml:math id="M291" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 50 %) in the 54-member LES library, as these cases show the strongest agreement with satellite observations and represent prime candidate environments for Marine Cloud Brightening (MCB) deployments. The LPM has previously been shown to reproduce horizontal spreading rates in LESs of single ship tracks in various turbulence and background aerosol environments when forced by boundary layer-averaged turbulence and dissipation rates <xref ref-type="bibr" rid="bib1.bibx40" id="paren.82"/>. Explicitly modeling many different sprayer and injection configurations for the LES library is computationally cost prohibitive; however, by leveraging the LPM framework, we can estimate the spatio-temporal evolution of injected aerosol by forcing the LPM with the background meteorology and turbulence data from the LES library.</p>
      <p id="d2e5193">The Twomey forcing calculation involves merging the 2D LPM aerosol fields with the 2D reflectance fields from the LES. This merging process allows for complicated interactions between aerosol distributions and the cloud morphologies modeled in the LES library; although, the direct mapping of the aerosol concentrations onto the LES cloud fields makes the assumptions that the aerosol is well-mixed in the vertical, 100 % of the aerosol is activated, and cloud adjustments are relatively small compared to the Twomey forcing. A decoupling parameter analysis indicates that many of the cases remain weakly decoupled with minor moisture stratification. Assuming 100 % aerosol activation simplifies the analysis and provides an upper bound on potential spreading rate-driven Twomey forcing differences. If cloud adjustments were taken into account, it is possible that Twomey forcing could be augmented or weakened in certain environments and cloud morphology could change in complex ways (e.g., cloud clearing near ship-track mesoscale circulation boundaries in precipitating environments), depending on background meteorological and aerosol conditions. This work represents a natural extension of the <xref ref-type="bibr" rid="bib1.bibx62" id="text.83"/> heuristic framework, where environmentally dependent spreading rates and their interactions with changing cloud morphologies are now estimated.</p>
      <p id="d2e5199">In the cloudy LES case library, meteorological, aerosol, and turbulence properties responsible for plume spreading differ appreciably between the Day 1 and Day 2 regimes, with Day 2 being characterized by deeper boundary layers, stronger turbulence, longer relaxation timescales, cleaner background aerosol conditions, and lower cloud fraction, all of which are consistent with our understanding of the equatorward evolution of low clouds. Despite these distinct meteorological, aerosol, and turbulence differences, there is weak regime sensitivity to Twomey forcing between Day 1 and Day 2, regardless of the assumed aerosol lifetime (<inline-formula><mml:math id="M292" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) or ship density implied by <inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">sprayers</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. A sensitivity analysis shows that the weak regime sensitivity arises because of cleaner Day 2 background aerosol conditions that offset Twomey forcing reductions from reduced cloud cover and deeper boundary layers. The consequence of this is that given a fixed <inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mrow><mml:mi>d</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>a</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and assuming negligible cloud adjustments, the Day 1 and Day 2 regimes are nearly equally susceptible to MCB. Previous LES of ship tracks suggest that the cleaner, precipitating boundary layers may be more prone to positive cloud adjustments that would enhance Twomey forcing, which may mean that the Day 2 regime would ultimately be more efficient <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx46" id="paren.84"/>; however, the leading-order control on Twomey forcing and the MCB efficiency of each regime is the aerosol lifetime assumption <inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which emphasizes the need for a greater understanding of injected aerosol lifetime-modulating processes such as collision-coalescence, interstitial scavenging, sedimentation, turbulent impaction, coagulation, and entrainment sources/sinks <xref ref-type="bibr" rid="bib1.bibx62" id="paren.85"/>.</p>
      <p id="d2e5262">Day 1 and Day 2 spreading rate regimes differ by over 2 km h<sup>−1</sup> at times, with Day 2 relaxation timescales (<inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) that are nearly a factor of 2 larger than those on Day 1. These longer relaxation timescales are associated with dissipation rate decreases related to larger mesoscale cells, more decoupled boundary layers, and modest increases in velocity variances. To isolate the effect of turbulence-driven spreading differences on Twomey forcing, we repeated the Day 1 LPM simulations using the Day 2 turbulence characteristics while maintaining the Day 1 cloud morphology, boundary-layer depth, mean wind, and background aerosol concentration conditions. Despite the substantially faster spreading associated with the Day 2 turbulence, the resulting Twomey forcing changes are smaller than 1 %. Therefore, in these simulations, the differences in turbulence-driven horizontal plume spreading alone do not produce appreciable changes in Twomey forcing, even though the underlying aerosol concentration distributions are impacted by the spreading rate differences.</p>
      <p id="d2e5289">The spreading rates exhibit a pronounced diurnal cycle, with the strongest spreading rates near sunrise (3<inline-formula><mml:math id="M298" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> km h<sup>−1</sup>) and a dramatic decrease in the spreading rate occurring in the late evening associated with the diurnal cycle of turbulence (<inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> km h<sup>−1</sup>). The instantaneous spreading rates experience a wide degree of variability, but the ensemble plume width is well-approximated by a linear growth rate of 1.5 km h<sup>−1</sup>, which is reasonably close to the <xref ref-type="bibr" rid="bib1.bibx19" id="text.86"/> estimate of 1.85 km h<sup>−1</sup> used in <xref ref-type="bibr" rid="bib1.bibx62" id="text.87"/>.</p>
      <p id="d2e5364">Additional LPM sensitivity tests suggest that Twomey forcing is largely unaffected by changing sprayer velocity (in the 0–10 m s<sup>−1</sup> range) and ship motion (random versus organized) in the northeast Pacific mean wind environment, implying that slow-moving or stationary spraying platforms may be viable, assuming efficient vertical transport and subsequent activation. Additionally, there is still forcing upside to injecting for much of the daylight hours (<inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> h versus 6 h), with injections beginning several hours before sunrise being most efficient, in agreement with <xref ref-type="bibr" rid="bib1.bibx33" id="text.88"/>. In an analysis of particle ages and concentration bins, a majority of the Twomey forcing originates from particles <inline-formula><mml:math id="M306" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1 d old and from concentrations below 100 # mg<sup>−1</sup>.</p>
      <p id="d2e5411">The relative role of horizontal spreading rate on Twomey forcing across a range of time-varying cloud fields, meteorological, and aerosol conditions is small, but idealized LPM experiments using 100 % cloud fraction and the most extreme spreading rate cases in the LES library indicate that if the range of naturally varying spreading is neglected, Twomey forcing could be overestimated by 5 %–30 % for sprayer densities below <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.125</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup>, with larger errors for shorter aerosol lifetimes. Above a sprayer density of <inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.25</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup>, errors from the naturally occurring range of spreading rates tend to zero. However, the spreading rate is much faster in GCMs than the fastest spreading rate in the LES library, as GCMs assume that the plume spreads infinitely fast within a climate model grid box. The infinite spreading rate assumption leads to potential Twomey forcing overestimations of 10 %–200 % at sprayer densities below <inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ships per km<sup>2</sup>. Even at high sprayer densities representative of a high-end MCB scenario, errors may exceed 10 % for aerosol lifetimes less than 1 d.</p>
      <p id="d2e5496">In light of the results from our merged LES-LPM framework, there are four primary emergent priorities for the future of plume spreading and Twomey forcing sensitivity research: <list list-type="bullet"><list-item>
      <p id="d2e5501">Narrow uncertainties regarding the aerosol lifetime (<inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">decay</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), addressing issues such as potential dry deposition enhancement driven by intense aerosol-induced mesoscale circulations. </p></list-item><list-item>
      <p id="d2e5517">Continue to constrain possible cloud adjustments, accounting for the potential of repeated aerosol injections. Substantial cloud adjustments, with fully coupled aerosols, have the potential to alter the relationship between Twomey forcing and spreading rate found in this paper.</p></list-item><list-item>
      <p id="d2e5521">Develop subgrid plume parameterizations, such as the one discussed in Sect. 3.7, to reduce the risk of overestimating MCB cooling potential in GCMs.</p></list-item><list-item>
      <p id="d2e5525">Further understanding of vertical aerosol spreading rates, realistic activation processes, and aerosol size distribution evolution to more accurately predict <inline-formula><mml:math id="M315" 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> in GCMs.</p></list-item></list></p>
      <p id="d2e5539">In summary, our results indicate that although horizontal plume spreading rates do not strongly affect global mean Twomey forcing across realistic northeast Pacific MBL regimes when assuming negligible cloud adjustments, the infinite spreading rate assumption inherent in current GCMs may lead to an overestimation of MCB efficiency that should be addressed through physically grounded subgrid plume spreading parameterizations. In addition, aerosol lifetimes differ strongly between precipitating and non-precipitating clouds. Therefore, the co-variability of aerosols and clouds affects the aerosol lifetime, which translates to potentially large changes in Twomey forcing, highlighting the importance of parameterizations of subgrid-scale aerosol and cloud processes in GCMs.</p>
</sec>

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

      <p id="d2e5547">The LES library statistics files used to force the particle model can be found on Zenodo at <ext-link xlink:href="https://doi.org/10.5281/zenodo.20097959" ext-link-type="DOI">10.5281/zenodo.20097959</ext-link> <xref ref-type="bibr" rid="bib1.bibx23" id="paren.89"/>. LES source code can be found at <ext-link xlink:href="https://doi.org/10.5281/zenodo.14895699" ext-link-type="DOI">10.5281/zenodo.14895699</ext-link> <xref ref-type="bibr" rid="bib1.bibx38" id="paren.90"/>. The Langevin particle model and Twomey calculation code can be accessed at <ext-link xlink:href="https://doi.org/10.5281/zenodo.20145149" ext-link-type="DOI">10.5281/zenodo.20145149</ext-link> <xref ref-type="bibr" rid="bib1.bibx37" id="paren.91"/>. The 2D LES library files needed for the calculation of reflectance and zonal and meridional wind fields for the mesoscale cell size calculation are available upon request.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e5569">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-26-14111-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-26-14111-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5578">LAM: particle model development, study conceptualization, data visualization, ran simulations for LES library, and manuscript writing. EE: developed LES library methodology, ran simulations for the LES library, performed observational analysis of LES library, manuscript review and editing. RW: Study conceptualization, manuscript review and editing. KvS: Study conceptualization, manuscript review and editing.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5585">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e5591">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="d2e5597">This work used Bridges-2 <xref ref-type="bibr" rid="bib1.bibx9" id="paren.92"/> at Pittsburgh Supercomputing Center through allocation EES210037 from the Advanced Cyberinfrastructure Coordination Ecosystem Services and Support (ACCESS) program <xref ref-type="bibr" rid="bib1.bibx7" id="paren.93"/>, which is supported by National Science Foundation grants 2138259, 2138286, 2138307, 2137603, and 2138296. This research utilized the Stampede3 supercomputer at the Texas Advanced Computing Center (TACC).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5608">This study was partially supported by the NOAA Climate Program Office Earth's Radiation Budget (ERB) program (grant no. NA22OAR4310474) and by the Cooperative Institute for Climate, Ocean, &amp; Ecosystem Studies (CICOES) under NOAA Cooperative Agreement NA20OAR4320271, contribution no. 2026-1590. The development of the particle model was partially supported by the Simons Foundation (SFIMPS-SRM-00005157). Support for Knut von Salzen was provided by the University of Washington's Marine Cloud Brightening Research Program, which is funded by the generous support of a growing consortium of individual and foundation donors.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5614">This paper was edited by Guy Dagan and reviewed by two anonymous referees.</p>
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