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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"><?xmltex \bartext{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-24-1919-2024</article-id><title-group><article-title>Effects of intermittent aerosol forcing on the stratocumulus-to-cumulus transition</article-title><alt-title>Effects of intermittent aerosol forcing on the stratocumulus-to-cumulus transition</alt-title>
      </title-group><?xmltex \runningtitle{Effects of intermittent aerosol forcing on the stratocumulus-to-cumulus transition}?><?xmltex \runningauthor{P. Prabhakaran et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Prabhakaran</surname><given-names>Prasanth</given-names></name>
          <email>prasanth.prabhakaran@noaa.gov</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Hoffmann</surname><given-names>Fabian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5136-0653</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Feingold</surname><given-names>Graham</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0774-2926</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Cooperative Institute for Research In Environmental Sciences (CIRES),<?xmltex \hack{\break}?> University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Chemical Sciences Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Meteorologisches Institut, Ludwig-Maximilians-Universität München, Munich, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Prasanth Prabhakaran (prasanth.prabhakaran@noaa.gov)</corresp></author-notes><pub-date><day>13</day><month>February</month><year>2024</year></pub-date>
      
      <volume>24</volume>
      <issue>3</issue>
      <fpage>1919</fpage><lpage>1937</lpage>
      <history>
        <date date-type="received"><day>26</day><month>July</month><year>2023</year></date>
           <date date-type="rev-request"><day>17</day><month>August</month><year>2023</year></date>
           <date date-type="rev-recd"><day>12</day><month>November</month><year>2023</year></date>
           <date date-type="accepted"><day>17</day><month>November</month><year>2023</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2024 </copyright-statement>
        <copyright-year>2024</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/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e114">We explore the role of intermittent aerosol forcing (e.g., injections associated with marine cloud brightening) in the stratocumulus-to-cumulus transition (SCT). We simulate a 3 d Lagrangian trajectory in the northeast Pacific using a large-eddy simulation model coupled to a bin-emulating, two-moment, bulk microphysics scheme that captures the evolution of aerosol and cloud droplet concentrations. By varying the background aerosol concentration, we consider two baseline systems – pristine and polluted. We perturb the baseline cases with a range of aerosol injection strategies by varying the injection rate, number of injectors, and the timing of the aerosol injection. Our results show that aerosol dispersal is more efficient under pristine conditions due to a transverse circulation created by the gradients in precipitation rates across the plume track. Furthermore, we see that a substantial enhancement in the cloud radiative effect (CRE) is evident in both systems. In the polluted system, the albedo effect (smaller but more numerous droplets causing brighter clouds at constant liquid water) is the dominant contributor in the initial 2 d. The contributions from liquid water path (LWP) and cloud fraction adjustments are important on the third and fourth day, respectively. In the pristine system, cloud fraction adjustments are the dominant contributor to the CRE on all 3 d, followed by the albedo effect. In both these systems, we see that the SCT is delayed due to the injection of aerosol, and the extent of the delay is proportional to the number of particles injected into the marine boundary layer.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Climate Program Office</funding-source>
<award-id>03-01-07-001</award-id>
<award-id>NA17OAR4320101</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Deutsche Forschungsgemeinschaft</funding-source>
<award-id>HO 6588/1-1</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e126">Clouds play an important role in the Earth's energy balance. In particular, marine stratocumulus clouds have a net cooling effect on the planet as they reflect a substantial fraction of the incoming solar radiation <xref ref-type="bibr" rid="bib1.bibx25" id="paren.1"/>. These overcast cloud decks are typically found in the sub-tropics over the eastern flanks of the ocean where sea surface temperatures are colder <xref ref-type="bibr" rid="bib1.bibx59" id="paren.2"/>. As these clouds advect towards the Equator, they undergo a transition from overcast stratocumulus to a shallow-cumulus-topped boundary layer with a much lower cloud fraction <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx61" id="paren.3"/>. Recent studies have shown that aerosol–precipitation interactions play an important role in regulating the stratocumulus-to-cumulus (SCT) transition <xref ref-type="bibr" rid="bib1.bibx63 bib1.bibx64" id="paren.4"/>. In this study, we explore the impact of aerosol perturbations (ship emissions, deliberate aerosol injection, etc.) on the SCT in the northeast Pacific region.</p>
      <p id="d1e141">To elucidate the mechanisms behind the SCT, several studies including field observations <xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx10" id="paren.5"/> and modeling  <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx36 bib1.bibx61 bib1.bibx45 bib1.bibx44 bib1.bibx63 bib1.bibx18" id="paren.6"/> have been undertaken. Until recently, the accepted theory of SCT was attributed to the advection of the cloud layer over a continuously warming sea surface. The increasing sea surface temperature (SST) enhances the surface latent heat flux (LHF). This increases the liquid water path<?pagebreak page1920?> (LWP), which results in enhanced cloud-top entrainment and shortwave (SW) absorption. This promotes the decoupling of the cloud layer from the surface <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx9 bib1.bibx61" id="paren.7"/>. Over time the decoupling gets stronger, which enables the formation of overshooting cumulus clouds that locally couple the cloud layer with the surface layer. The enhanced entrainment from cumulus clouds and a lack of steady supply of water vapor from the surface gradually thins and dissipates the stratocumulus layer. <xref ref-type="bibr" rid="bib1.bibx46" id="text.8"/> explored the SCT in four different ocean basins using multiple reanalysis trajectories and concluded that the transition is similar in all cases. These transitions were typically considered to be a multi-day process, based on numerical simulations using microphysical schemes with a fixed cloud droplet concentration (<inline-formula><mml:math id="M1" 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>). This lack of interaction between aerosol and cloud droplets significantly reduced the degree to which precipitation can influence the SCT. Using the same modeling framework, <xref ref-type="bibr" rid="bib1.bibx44" id="text.9"/> explored the factors influencing SCT. Their analysis showed that the SCT is primarily affected by the increasing SST, and the timescale of the transition is governed by the lower tropospheric stability.</p>
      <p id="d1e171">The interaction of precipitation and stratiform clouds was investigated in <xref ref-type="bibr" rid="bib1.bibx50" id="text.10"/> and <xref ref-type="bibr" rid="bib1.bibx39" id="text.11"/>. They argued that the evaporation of sub-cloud precipitation decouples the cloud layer from the surface. This enhances cumulus activity in deeper boundary layers and accelerates the transition from stratocumulus- to cumulus-topped boundary layers <xref ref-type="bibr" rid="bib1.bibx44" id="paren.12"/>. Recent simulations with a prognostic aerosol scheme have shown that the interactions among aerosol concentration (<inline-formula><mml:math id="M2" 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>), <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and drizzle play an important role in determining the SCT timescale <xref ref-type="bibr" rid="bib1.bibx62 bib1.bibx63" id="paren.13"/>. The onset of collision–coalescence triggers weak precipitation, which results in lower <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> and <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>. This promotes the growth of cloud droplets to larger sizes, which makes the cloud colloidally unstable. This increases precipitation, resulting in further reduction in <inline-formula><mml:math id="M6" 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>, which further strengthens precipitation. This positive feedback (referred to as runaway precipitation) significantly reduces <inline-formula><mml:math id="M7" 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> in the boundary layer. Similar conclusions were drawn from recent simulations of Lagrangian trajectories drawn from the CSET campaign <xref ref-type="bibr" rid="bib1.bibx18" id="paren.14"/>. However, conclusions from observational studies are ambiguous in assessing the role of precipitation. Using satellite data, <xref ref-type="bibr" rid="bib1.bibx16" id="text.15"/> concluded that rain has little role in determining the timescale of SCT once the marine boundary layer (MBL) height and inversion strength are factored in. A more refined study suggests that precipitation plays an important role in the transition from closed-to-open cellular transition but not so much in the closed-to-disorganized cumulus transition <xref ref-type="bibr" rid="bib1.bibx17" id="paren.16"/>. Furthermore, the analysis of three trajectories from the CSET campaign shows that under pristine conditions precipitation may play an important role in the transition <xref ref-type="bibr" rid="bib1.bibx47" id="paren.17"/>. All of these studies suggest that the importance of precipitation in SCT is conditional on the meteorology. In the present study, we investigate the well-studied SCT system from <xref ref-type="bibr" rid="bib1.bibx44" id="text.18"/>, where precipitation plays an important role in the transition to cumulus clouds <xref ref-type="bibr" rid="bib1.bibx63" id="paren.19"/>.</p>
      <p id="d1e272">The aerosol perturbations applied in this study should be considered a proxy for the emissions from ships and deliberate aerosol injection for marine cloud brightening (MCB). MCB is a proposed climate intervention approach where sub-tropical marine stratocumulus clouds are seeded with sea-spray aerosol particles to enhance their reflectivity <xref ref-type="bibr" rid="bib1.bibx37" id="paren.20"/>. Recent studies based on general circulation models have suggested that MCB has the potential to mitigate the warming effects of anthropogenic greenhouse gas emissions <xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx2 bib1.bibx49" id="paren.21"/>. However, these models do not represent marine stratocumulus with sufficient fidelity, nor do they account for aerosol-induced cloud adjustments correctly, leaving questions about their ability to assess the net enhancement in cloud reflectivity.</p>
      <p id="d1e282">The susceptibility of the cloud radiative effect (CRE) to an aerosol perturbation has three major contributions: <inline-formula><mml:math id="M8" 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>, liquid water path (LWP), and cloud fraction (<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). The enhancement in cloud reflectivity in response to an increase in <inline-formula><mml:math id="M10" 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>, stratified by LWP and <inline-formula><mml:math id="M11" 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 known as the Twomey or albedo effect <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx52" id="paren.22"/>. In reality, LWP and <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are affected by aerosol perturbations. The addition of aerosol enhances the colloidal stability of the cloud layer and suppresses precipitation, which increases LWP and <inline-formula><mml:math id="M13" 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> <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx22" id="paren.23"/>. However, it also increases the cloud-top entrainment rate through the evaporation–entrainment feedback <xref ref-type="bibr" rid="bib1.bibx56" id="paren.24"/> and  sedimentation–entrainment feedback <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx6" id="paren.25"/> potentially causing a decrease in LWP and <inline-formula><mml:math id="M14" 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>. Additionally, LWP and <inline-formula><mml:math id="M15" 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> adjustments are affected by aerosol-enhanced SW absorption <xref ref-type="bibr" rid="bib1.bibx42" id="paren.26"/> and surface flux changes <xref ref-type="bibr" rid="bib1.bibx12" id="paren.27"/>.</p>
      <p id="d1e393">In this study, we use large-eddy simulations (LESs) to assess the impact of aerosol perturbations on SCT by varying the injection rates and the frequency of perturbations. We consider two SCT baseline systems: polluted (150 particles mg<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and pristine (50 particles mg<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). The simulations can be considered of interest to both possible future MCB activities as well as to the broader problem of aerosol–cloud–climate forcing. In the next section, we will present the details of the simulation setup, including the aerosol forcing function. This is followed by a presentation of simulation results. We end the article with a discussion of the results in the context of MCB, followed by a summary and outlook.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methodology</title>
      <p id="d1e428">Traditional LES is capable of representing aerosol–cloud interactions faithfully over a wide range of meteorological<?pagebreak page1921?> conditions. However, these studies are limited to rather small domains (<inline-formula><mml:math id="M18" display="inline"><mml:mo lspace="0mm">≤</mml:mo></mml:math></inline-formula> 100 km). Consequently, large-scale meteorological feedbacks are not captured in such studies. To date, in the context of MCB, most LES studies have been based on fixed meteorological conditions and short durations (12–36 h) <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx29 bib1.bibx40 bib1.bibx12 bib1.bibx42" id="paren.28"/>. To understand the impact of MCB-like aerosol perturbations on the SCT, we require domains with horizontal extent spanning several hundred kilometers and time integration up to 3 or more days, which are computationally prohibitive at LES resolutions. A good compromise in this regard is Lagrangian LES, where a smaller domain with horizontally uniform properties is advected along the mean wind <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx46" id="paren.29"/>. Thus, the spatial variation in the large-scale forcings is represented as temporally varying boundary conditions. Further temporal changes are imposed on the model domain through nudging to a predefined value obtained from coarser models or reanalysis data sets. This methodology has been used to investigate SCT in several studies <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx62 bib1.bibx64 bib1.bibx23" id="paren.30"/>, and is used in the current study as well. We note that this methodology, despite its advantages compared to traditional LES, has its limitations in representing the large-scale effects and feedbacks. Additionally, the accuracy of the temporally evolving boundary conditions is dependent on the reanalysis data.</p>
      <p id="d1e447">The simulations reported here follow the setup in <xref ref-type="bibr" rid="bib1.bibx63" id="text.31"/>, and therefore only a brief overview is provided here. The Lagrangian LES model is coupled to a two-moment, bin-emulating bulk microphysical model <xref ref-type="bibr" rid="bib1.bibx19" id="paren.32"/>. The conditions and trajectories are based on the reference Lagrangian SCT case study developed by <xref ref-type="bibr" rid="bib1.bibx44" id="text.33"/>. The model domain is advected along the mean boundary layer wind in the northeast Pacific (NEP) region. (See Fig. <xref ref-type="fig" rid="Ch1.F1"/> for a schematic of the trajectory.) The subsidence rates along the trajectory are obtained from <xref ref-type="bibr" rid="bib1.bibx7" id="text.34"/>, and the time evolution of the SST is obtained from <xref ref-type="bibr" rid="bib1.bibx44" id="text.35"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e470">The white curve is the 6 d Lagrangian trajectory identified by <xref ref-type="bibr" rid="bib1.bibx46" id="text.36"/> in the NEP. The red curve is the 3 d Lagrangian trajectory simulated here (see <xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx63" id="altparen.37"/>). The contours represent the marine low-cloud fraction obtained from Aqua-MODIS between 2005 and 2014. The dashed white square box indicates the region studied by <xref ref-type="bibr" rid="bib1.bibx35" id="text.38"/>. The black stars indicate the air parcel position at 24 h intervals, and the cyan stars are the positions of each aerosol pulse. Each aerosol pulse may have one or two active sprayers. The panels to the right represent the one- and two-sprayer configurations. The red (blue) areas in these two panels represent the plume track (background) in the NA150 case identified using the methodology described in the Appendix.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f01.png"/>

      </fig>

      <?pagebreak page1922?><p id="d1e489">We use the System for Atmospheric (SAM) model as the LES dynamical core <xref ref-type="bibr" rid="bib1.bibx34" id="paren.39"/>. The radiative effects are represented using the Rapid Radiative Transfer Model for Global Climate Models (RRTMG) with extended vertical profiles above the domain top <xref ref-type="bibr" rid="bib1.bibx38" id="paren.40"/>. The microphysical scheme consists of two modes representing cloud droplets and raindrops separately, allowing for more precise bin-by-bin mass transfer rates for modeling the collision–coalescence processes (bin-emulating). The size distributions are represented as log-normal distributions, each with a fixed geometric standard deviation of 1.2 <xref ref-type="bibr" rid="bib1.bibx19 bib1.bibx53" id="paren.41"/>. The two modes are separated by a threshold value of 25 <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m in radius <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx33" id="paren.42"/>. Additionally, a separate prognostic equation is solved for <inline-formula><mml:math id="M20" 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>, which includes a fixed surface flux of 70 cm<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx30" id="paren.43"/>, and losses or gains through cloud processing (activation, deactivation, collision–coalescence, and wet removal). The activation of aerosol particles is determined by the local supersaturation, which is calculated prognostically following the semi-analytical method of <xref ref-type="bibr" rid="bib1.bibx13" id="text.44"/>. The aerosol follows a log-normal size distribution with a geometric standard deviation of 1.5 and a geometric mean radius of 100 nm <xref ref-type="bibr" rid="bib1.bibx63" id="paren.45"/>. In the applied modeling framework, cloud processing of aerosol affects the number concentration of aerosol but not the shape of the distribution <xref ref-type="bibr" rid="bib1.bibx19 bib1.bibx63" id="paren.46"/>. Note that the recommended radius of aerosol particles for MCB is thought to be between 15 and 85 nm <xref ref-type="bibr" rid="bib1.bibx60 bib1.bibx26" id="paren.47"/>, which is slightly smaller than the size range considered. We assume the injected particle size distribution to be the same as the background size distribution to avoid treating two separate populations, which would in any case become indistinguishable once processed by the cloud. This differs from the more rigorous aerosol treatment using the superdroplet approach <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx42 bib1.bibx28" id="paren.48"/>, which is computationally unfeasible for the long simulations and large domains used here. In spite of this simpler aerosol and cloud microphysical treatment, the results are highly relevant in terms of the injection-related modification to <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> and the subsequent adjustments of LWP and <inline-formula><mml:math id="M24" 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>, which together determine the degree of cloud brightening.</p>
      <p id="d1e589">All the simulations have a domain size of 128 km in the horizontal directions and 4.25 km in the vertical direction. A uniform grid spacing of 100 m is used in the horizontal directions. In the vertical direction, a uniform grid spacing of 10 m is used below 2.775 km, and above this height, the grid is smoothly stretched to the domain top with the grid spacing increasing linearly with height. The total number of grid points in the vertical direction is 300. Such a large horizontal domain is chosen to capture the spread rates of the injected aerosol plume, as well as precipitation and associated cloud-field organization <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx63" id="paren.49"/>. The time step is set to 3 s with adaptive sub-stepping to satisfy the Courant–Friedrichs–Lewy stability condition. The radiative heating profiles are updated every minute. The simulation is integrated in time for 3 d, starting on the 196.75th day of the year (15 July 10:00 local time).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e598">Cloud radiative effect enhancement (dCRE <inline-formula><mml:math id="M25" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CRE<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo><mml:mtext>-</mml:mtext><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M27" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> CRE<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">case</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">ID</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>) and its decomposition at the TOA for all the seeded cases in NA150. The budgeting is done using cloud properties for a threshold of <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M30" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2. The quantity for each day is averaged between sunrise and sunset. On day 4, the averaging is done between sunrise and simulation end time. Column RES is the residual of the dCRE budget. RES <inline-formula><mml:math id="M31" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> dCRE <inline-formula><mml:math id="M32" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> sum of dCRE components.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="16">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right" colsep="1"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right" colsep="1"/>
     <oasis:colspec colnum="12" colname="col12" align="right"/>
     <oasis:colspec colnum="13" colname="col13" align="right"/>
     <oasis:colspec colnum="14" colname="col14" align="right"/>
     <oasis:colspec colnum="15" colname="col15" align="right"/>
     <oasis:colspec colnum="16" colname="col16" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Case ID</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col6" align="center" colsep="1">Day 2 (W m<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) </oasis:entry>
         <oasis:entry rowsep="1" namest="col7" nameend="col11" align="center" colsep="1">Day 3 (W m<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) </oasis:entry>
         <oasis:entry rowsep="1" namest="col12" nameend="col16" align="center">Day 4 (W m<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">dCRE</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">LWP</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">RES</oasis:entry>
         <oasis:entry colname="col7">dCRE</oasis:entry>
         <oasis:entry colname="col8"><inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9">LWP</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col11">RES</oasis:entry>
         <oasis:entry colname="col12">dCRE</oasis:entry>
         <oasis:entry colname="col13"><inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col14">LWP</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col16">RES</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1<inline-formula><mml:math id="M42" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100</oasis:entry>
         <oasis:entry colname="col2">3.1</oasis:entry>
         <oasis:entry colname="col3">4.5</oasis:entry>
         <oasis:entry colname="col4">1.4</oasis:entry>
         <oasis:entry colname="col5">0.8</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M43" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.7</oasis:entry>
         <oasis:entry colname="col7">9.8</oasis:entry>
         <oasis:entry colname="col8">7.0</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M44" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.8</oasis:entry>
         <oasis:entry colname="col10">2.1</oasis:entry>
         <oasis:entry colname="col11">2.4</oasis:entry>
         <oasis:entry colname="col12">5.8</oasis:entry>
         <oasis:entry colname="col13">1.7</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M45" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.9</oasis:entry>
         <oasis:entry colname="col15">4.9</oasis:entry>
         <oasis:entry colname="col16">4.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1<inline-formula><mml:math id="M46" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-101</oasis:entry>
         <oasis:entry colname="col2">3.1</oasis:entry>
         <oasis:entry colname="col3">4.5</oasis:entry>
         <oasis:entry colname="col4">1.4</oasis:entry>
         <oasis:entry colname="col5">0.8</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M47" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.7</oasis:entry>
         <oasis:entry colname="col7">12.4</oasis:entry>
         <oasis:entry colname="col8">11.1</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M48" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.2</oasis:entry>
         <oasis:entry colname="col10">2.6</oasis:entry>
         <oasis:entry colname="col11">1.9</oasis:entry>
         <oasis:entry colname="col12">16.6</oasis:entry>
         <oasis:entry colname="col13">2.2</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M49" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.4</oasis:entry>
         <oasis:entry colname="col15">14.4</oasis:entry>
         <oasis:entry colname="col16">6.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1<inline-formula><mml:math id="M50" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-110</oasis:entry>
         <oasis:entry colname="col2">3.2</oasis:entry>
         <oasis:entry colname="col3">4.8</oasis:entry>
         <oasis:entry colname="col4">1.3</oasis:entry>
         <oasis:entry colname="col5">0.8</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M51" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.7</oasis:entry>
         <oasis:entry colname="col7">10.5</oasis:entry>
         <oasis:entry colname="col8">12.7</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M52" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.6</oasis:entry>
         <oasis:entry colname="col10">0.9</oasis:entry>
         <oasis:entry colname="col11">5.5</oasis:entry>
         <oasis:entry colname="col12">9.9</oasis:entry>
         <oasis:entry colname="col13">1.9</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M53" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.3</oasis:entry>
         <oasis:entry colname="col15">6.9</oasis:entry>
         <oasis:entry colname="col16">2.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5<inline-formula><mml:math id="M54" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100</oasis:entry>
         <oasis:entry colname="col2">11.2</oasis:entry>
         <oasis:entry colname="col3">16.6</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M55" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.6</oasis:entry>
         <oasis:entry colname="col5">1.6</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M56" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.3</oasis:entry>
         <oasis:entry colname="col7">31.6</oasis:entry>
         <oasis:entry colname="col8">24.9</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M57" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.4</oasis:entry>
         <oasis:entry colname="col10">6.7</oasis:entry>
         <oasis:entry colname="col11">0.4</oasis:entry>
         <oasis:entry colname="col12">33.9</oasis:entry>
         <oasis:entry colname="col13">5.2</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M58" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11.4</oasis:entry>
         <oasis:entry colname="col15">29.3</oasis:entry>
         <oasis:entry colname="col16">10.9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5<inline-formula><mml:math id="M59" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200</oasis:entry>
         <oasis:entry colname="col2">21.8</oasis:entry>
         <oasis:entry colname="col3">32.0</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M60" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.6</oasis:entry>
         <oasis:entry colname="col5">2.4</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M61" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.0</oasis:entry>
         <oasis:entry colname="col7">38.4</oasis:entry>
         <oasis:entry colname="col8">36.1</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M62" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.6</oasis:entry>
         <oasis:entry colname="col10">7.0</oasis:entry>
         <oasis:entry colname="col11">1.0</oasis:entry>
         <oasis:entry colname="col12">94.4</oasis:entry>
         <oasis:entry colname="col13">14.3</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M63" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.5</oasis:entry>
         <oasis:entry colname="col15">81.8</oasis:entry>
         <oasis:entry colname="col16">19.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5<inline-formula><mml:math id="M64" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-220</oasis:entry>
         <oasis:entry colname="col2">23.1</oasis:entry>
         <oasis:entry colname="col3">33.9</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M65" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.7</oasis:entry>
         <oasis:entry colname="col5">2.6</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M66" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.8</oasis:entry>
         <oasis:entry colname="col7">53.5</oasis:entry>
         <oasis:entry colname="col8">51.7</oasis:entry>
         <oasis:entry colname="col9">0.7</oasis:entry>
         <oasis:entry colname="col10">9.6</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M67" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.1</oasis:entry>
         <oasis:entry colname="col12">173.8</oasis:entry>
         <oasis:entry colname="col13">27.9</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M68" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>27.6</oasis:entry>
         <oasis:entry colname="col15">149.6</oasis:entry>
         <oasis:entry colname="col16">24.0</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{1}?></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1366">As in Table <xref ref-type="table" rid="Ch1.T1"/> but for case NA50.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.97}[.97]?><oasis:tgroup cols="16">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right" colsep="1"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right" colsep="1"/>
     <oasis:colspec colnum="12" colname="col12" align="right"/>
     <oasis:colspec colnum="13" colname="col13" align="right"/>
     <oasis:colspec colnum="14" colname="col14" align="right"/>
     <oasis:colspec colnum="15" colname="col15" align="right"/>
     <oasis:colspec colnum="16" colname="col16" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Case ID</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col6" align="center" colsep="1">Day 2 (W m<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) </oasis:entry>
         <oasis:entry rowsep="1" namest="col7" nameend="col11" align="center" colsep="1">Day 3 (W m<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) </oasis:entry>
         <oasis:entry rowsep="1" namest="col12" nameend="col16" align="center">Day 4 (W m<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">dCRE</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">LWP</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">RES</oasis:entry>
         <oasis:entry colname="col7">dCRE</oasis:entry>
         <oasis:entry colname="col8"><inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9">LWP</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col11">RES</oasis:entry>
         <oasis:entry colname="col12">dCRE</oasis:entry>
         <oasis:entry colname="col13"><inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col14">LWP</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col16">RES</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1<inline-formula><mml:math id="M78" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100</oasis:entry>
         <oasis:entry colname="col2">15.7</oasis:entry>
         <oasis:entry colname="col3">10.2</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M79" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.8</oasis:entry>
         <oasis:entry colname="col5">11.6</oasis:entry>
         <oasis:entry colname="col6">2.8</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M80" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.4</oasis:entry>
         <oasis:entry colname="col8">8.7</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M81" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.2</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M82" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.5</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M83" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.4</oasis:entry>
         <oasis:entry colname="col12">2.4</oasis:entry>
         <oasis:entry colname="col13">2.3</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M84" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.8</oasis:entry>
         <oasis:entry colname="col15">1.1</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M85" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1<inline-formula><mml:math id="M86" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-110</oasis:entry>
         <oasis:entry colname="col2">14.0</oasis:entry>
         <oasis:entry colname="col3">12.8</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M87" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.9</oasis:entry>
         <oasis:entry colname="col5">11.6</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M88" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6</oasis:entry>
         <oasis:entry colname="col7">0.8</oasis:entry>
         <oasis:entry colname="col8">17.5</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M89" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10.4</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M90" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.7</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M91" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.6</oasis:entry>
         <oasis:entry colname="col12">5.9</oasis:entry>
         <oasis:entry colname="col13">4.1</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M92" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6</oasis:entry>
         <oasis:entry colname="col15">3.9</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M93" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1<inline-formula><mml:math id="M94" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200</oasis:entry>
         <oasis:entry colname="col2">19.6</oasis:entry>
         <oasis:entry colname="col3">10.8</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M95" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.0</oasis:entry>
         <oasis:entry colname="col5">17.3</oasis:entry>
         <oasis:entry colname="col6">0.4</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M96" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.6</oasis:entry>
         <oasis:entry colname="col8">4.5</oasis:entry>
         <oasis:entry colname="col9">0.0</oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M97" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.0</oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M98" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.1</oasis:entry>
         <oasis:entry colname="col12"><inline-formula><mml:math id="M99" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.4</oasis:entry>
         <oasis:entry colname="col13">2.7</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M100" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.6</oasis:entry>
         <oasis:entry colname="col15"><inline-formula><mml:math id="M101" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.1</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M102" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5<inline-formula><mml:math id="M103" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100</oasis:entry>
         <oasis:entry colname="col2">53.7</oasis:entry>
         <oasis:entry colname="col3">30.3</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M104" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.4</oasis:entry>
         <oasis:entry colname="col5">42.2</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">78.6</oasis:entry>
         <oasis:entry colname="col8">21.0</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18.9</oasis:entry>
         <oasis:entry colname="col10">73.2</oasis:entry>
         <oasis:entry colname="col11">3.5</oasis:entry>
         <oasis:entry colname="col12">12.7</oasis:entry>
         <oasis:entry colname="col13">1.6</oasis:entry>
         <oasis:entry colname="col14">6.4</oasis:entry>
         <oasis:entry colname="col15">8.8</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M106" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">8.6<inline-formula><mml:math id="M107" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100</oasis:entry>
         <oasis:entry colname="col2">73.9</oasis:entry>
         <oasis:entry colname="col3">36.0</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M108" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23.8</oasis:entry>
         <oasis:entry colname="col5">60.0</oasis:entry>
         <oasis:entry colname="col6">1.7</oasis:entry>
         <oasis:entry colname="col7">120.6</oasis:entry>
         <oasis:entry colname="col8">27.9</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M109" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.6</oasis:entry>
         <oasis:entry colname="col10">112.2</oasis:entry>
         <oasis:entry colname="col11">3.0</oasis:entry>
         <oasis:entry colname="col12">48.0</oasis:entry>
         <oasis:entry colname="col13">6.0</oasis:entry>
         <oasis:entry colname="col14"><inline-formula><mml:math id="M110" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.3</oasis:entry>
         <oasis:entry colname="col15">36.0</oasis:entry>
         <oasis:entry colname="col16">8.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5<inline-formula><mml:math id="M111" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200</oasis:entry>
         <oasis:entry colname="col2">144.1</oasis:entry>
         <oasis:entry colname="col3">34.9</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M112" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>24.2</oasis:entry>
         <oasis:entry colname="col5">133.3</oasis:entry>
         <oasis:entry colname="col6">0.1</oasis:entry>
         <oasis:entry colname="col7">133.4</oasis:entry>
         <oasis:entry colname="col8">26.4</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M113" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.5</oasis:entry>
         <oasis:entry colname="col10">125.0</oasis:entry>
         <oasis:entry colname="col11">2.5</oasis:entry>
         <oasis:entry colname="col12">23.6</oasis:entry>
         <oasis:entry colname="col13">4.1</oasis:entry>
         <oasis:entry colname="col14">6.6</oasis:entry>
         <oasis:entry colname="col15">16.3</oasis:entry>
         <oasis:entry colname="col16"><inline-formula><mml:math id="M114" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.4</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table><?xmltex \gdef\@currentlabel{2}?></table-wrap>

      <p id="d1e2121">Two sets of simulations are conducted for different baseline <inline-formula><mml:math id="M115" 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>: 150 mg<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (NA150) and 50 mg<inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (NA50). In the baseline case in NA150, the transition from overcast stratocumulus to low-cloud-fraction (<inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) clouds occurs due to the increasing SST. The timescale of the transition is determined by precipitation. On the other hand, in the NA50 baseline case, the transition is solely driven by precipitation resulting in an open-cellular cloud structure. Note that the precipitation-driven transitions are reversible (i.e., overcast stratocumulus layer can be re-established) if a sufficient amount of aerosol particles is injected into the boundary layer <xref ref-type="bibr" rid="bib1.bibx20" id="paren.50"/>. In our study, the transition is said to be complete when <inline-formula><mml:math id="M119" 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> decreases to a value below 40 % and stays below this value for at least 6 h. Both NA150 and NA50 systems are subjected to various aerosol seeding strategies summarized in Tables <xref ref-type="table" rid="Ch1.T1"/> and <xref ref-type="table" rid="Ch1.T2"/>. We vary aerosol injection rates: low (<inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> particles s<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> referred to as 1<inline-formula><mml:math id="M122" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>) and high (<inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> s<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> referred to as 5<inline-formula><mml:math id="M126" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> and 8.6<inline-formula><mml:math id="M127" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>, respectively), which are the recommended ranges per sprayer for MCB <xref ref-type="bibr" rid="bib1.bibx60" id="paren.51"/>. Note that the 8.6<inline-formula><mml:math id="M128" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> injection is explored only for the NA50 system. We also vary the number of aerosol sprayers and the number of aerosol pulses along the trajectory. A schematic of the trajectory, the position of the aerosol pulses, and the configuration of the sprayers is provided in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. Each seeding strategy has a five-character code (e.g., 1<inline-formula><mml:math id="M129" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-120). The two characters before the hyphen represent the strength of the aerosol injection rate (0<inline-formula><mml:math id="M130" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>/1<inline-formula><mml:math id="M131" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>/5<inline-formula><mml:math id="M132" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>/8.6<inline-formula><mml:math id="M133" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>), and the last three digits represent the number of sprayers (0/1/2) active during each of the three aerosol pulses. A value of 0 indicates that no aerosol is injected during the time period of that pulse. The first aerosol pulse is introduced 4 h after the start of the simulation. The next pulse is introduced approximately 20 h after the first pulse, and the final pulse is introduced 19 h later. An approximately 20 h separation between pulses is maintained to ensure sufficient time for the aerosol plume to spread across the domain. During this time the cloud layer advects approximately 350 to 400 km. The total aerosol injected into the marine boundary layer can be calculated as the aerosol injection strength times the sum of the last three digits in the code. Each aerosol pulse represents the passage of sprayer(s) upstream from one end of the domain to the other at a speed of 5 m s<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; i.e., the relative speed between the sprayer and the domain is 5 m s<inline-formula><mml:math id="M135" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Each sprayer has the dimension of one grid cell (100 <inline-formula><mml:math id="M136" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 100 m<inline-formula><mml:math id="M137" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>), and all the particles are injected from the surface.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>NA150: polluted system</title>
      <p id="d1e2384">Figure <xref ref-type="fig" rid="Ch1.F2"/>a shows the time evolution of the injected aerosol plume areal coverage. The injected plume is distinguished from the background by setting a threshold on the vertically integrated  boundary layer aerosol concentration (<inline-formula><mml:math id="M138" 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>). A plume is identified when <inline-formula><mml:math id="M139" 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> exceeds the background variability in <inline-formula><mml:math id="M140" 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> (see Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/> for more details). Ideally, for MCB applications one should consider cloud optical thickness (<inline-formula><mml:math id="M141" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>) or cloud albedo (<inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) for identifying the plume. However, the signal from these quantities is not very strong for the polluted system, especially in the 1<inline-formula><mml:math id="M143" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases. To leading order, the plume coverage increases linearly with time in all cases (Fig. <xref ref-type="fig" rid="Ch1.F2"/>a). The spread rate is approximately 2 times faster for the two-sprayer configuration compared to the single-sprayer configuration, which is expected. The spread rates are qualitatively similar for the 1<inline-formula><mml:math id="M144" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> and 5<inline-formula><mml:math id="M145" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, although the 5<inline-formula><mml:math id="M146" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases appear to be spreading at a faster rate. Note that the turbulent kinetic energy (Fig. <xref ref-type="fig" rid="Ch1.F3"/>), which is a measure of mixing within the MBL, is similar in all the cases, until the onset of precipitation, which occurs in the morning of day 3 (<inline-formula><mml:math id="M147" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 35 h after the start of injection). Thus, for a given number of sprayers, the plume spread rates are for the most part not affected by the number of aerosol particles injected. Therefore, the slower spread rate in the 1<inline-formula><mml:math id="M148" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases is an artifact of the plume detection methodology. In the 1<inline-formula><mml:math id="M149" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, along the plume edges, the absolute value of <inline-formula><mml:math id="M150" 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> becomes comparable to the background value (low signal-to-noise ratio) after some time due to dilution. This reduces the detected plume area, as is evident from the decrease in plume area coverage in the 1<inline-formula><mml:math id="M151" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases after sunset on day 2.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e2524">Time series of <bold>(a)</bold> plume area coverage, <bold>(b)</bold> liquid water path (LWP), <bold>(c)</bold> cloud droplet concentration (<inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(d)</bold> cloud fraction (<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(e)</bold> domain-averaged precipitation flux (rain rate) at cloud base <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <bold>(f)</bold> domain-averaged height of the inversion layer (<inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in NA150. <inline-formula><mml:math id="M156" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the cloud optical thickness. The legend is shown in panel <bold>(e)</bold>. The dotted lines in panels <bold>(b)</bold>–<bold>(f)</bold> are the cloud properties in case 5<inline-formula><mml:math id="M157" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 with a delayed aerosol perturbation. The perturbation is delayed by 5 h (relative to 5<inline-formula><mml:math id="M158" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100). The downward-pointing arrows at the top of each panel represent the time at which the three aerosol pulses start spraying, if active. Note that all the time series plots in this article start at 10:00 LT on day 1 and end at 10:00 LT on day 4.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f02.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2629">Time series of the  resolved turbulent kinetic energy (TKE) (solid lines) and resolved vertical velocity variance (<inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>) (dashed lines) at 700 m in NA150. See Fig. <xref ref-type="fig" rid="Ch1.F2"/>e for the color code.</p></caption>
          <?xmltex \igopts{width=190.633465pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f03.png"/>

        </fig>

      <p id="d1e2652">Regarding the plume area fraction, a value of unity is an outcome of the limited horizontal domain. This restricts the scope of this study in the context of ship tracks because “real” tracks evolve in an “infinite” domain and never reach an area fraction of 1. Consequently, the cloud properties would be continuously affected by spreading and dilution of the track. However, in the context of MCB, the primary focus here, several sprayers are operating in tandem. An area fraction of unity indicates that multiple plume tracks have merged, and no more dilution due to spreading is occurring.</p>
      <?pagebreak page1923?><p id="d1e2655"><?xmltex \hack{\newpage}?>Figure <xref ref-type="fig" rid="Ch1.F2"/>b, c, and d depict the evolution of the cloud-averaged properties conditional on <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>: liquid water path (LWP <inline-formula><mml:math id="M161" display="inline"><mml:mo>∣</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>), cloud droplet concentration (<inline-formula><mml:math id="M163" 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> <inline-formula><mml:math id="M164" display="inline"><mml:mo>∣</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>), and cloud fraction (<inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M167" display="inline"><mml:mo>∣</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>), respectively. Note that we have not separated the plume and background regions when calculating these properties. In the baseline case (0<inline-formula><mml:math id="M169" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-000), barring the variability associated with the diurnal cycle, the LWP increases with time in response to the increasing SST and associated MBL deepening (Fig. <xref ref-type="fig" rid="Ch1.F2"/>f). This trend continues until day 3 in the afternoon. <inline-formula><mml:math id="M170" 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 nearly constant for the first 2 d. The reduction in <inline-formula><mml:math id="M171" 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> due to weak collision–coalescence is offset by the steady flux of aerosol from the ocean surface. In the morning hours of day 3, the LWP is high enough to cause precipitation at cloud base (<inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) on the order of 0.5 mm d<inline-formula><mml:math id="M173" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F2"/>e). On day 3, <inline-formula><mml:math id="M174" 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> decreases by about 40 % by midday due to (i) collision–coalescence and precipitation losses and (ii) a likely reduced aerosol activation rate due to the weakening of the updrafts (Fig. <xref ref-type="fig" rid="Ch1.F3"/>) from precipitation evaporation and SW absorption. The subsequent recovery in LWP late in the afternoon triggers runaway precipitation that removes aerosol from the MBL and breaks up the stratocumulus layer. This is evident from the time series of <inline-formula><mml:math id="M175" 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>, which follows the familiar diurnal cycle up to day 3 in the morning. The weak (<inline-formula><mml:math id="M176" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 1 mm d<inline-formula><mml:math id="M177" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) precipitation in the morning and the afternoon enhances the daytime reduction in <inline-formula><mml:math id="M179" 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> slightly. However, post-sunset, the cloud system recovers and generates sustained stronger precipitation (on the order of 3 mm d<inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), eventually reducing <inline-formula><mml:math id="M182" 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> to below 30 % by the end of the simulation.</p>
      <?pagebreak page1924?><p id="d1e2911"><inline-formula><mml:math id="M183" 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> increases in all the perturbed cases. After the initial linear increase, while the sprayer is active, in the weakly perturbed cases (1<inline-formula><mml:math id="M184" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>), <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is nearly constant in time until the morning of day 3. This is similar to the baseline case. In the strongly perturbed cases (5<inline-formula><mml:math id="M186" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>), there is a steady decrease in <inline-formula><mml:math id="M187" 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> with time consistent with the deepening of the MBL (Fig. <xref ref-type="fig" rid="Ch1.F2"/>f). The 1<inline-formula><mml:math id="M188" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> and baseline cases are not affected by this deepening because the difference in <inline-formula><mml:math id="M189" 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> between the free troposphere (150 mg<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and the MBL (150–200 mg<inline-formula><mml:math id="M191" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) is not significant, unlike in the 5<inline-formula><mml:math id="M192" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases. Note that in realistic conditions, a strong gradient in <inline-formula><mml:math id="M193" 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> can exist between the free troposphere and the MBL. Under those conditions, MBL deepening should be considered an added factor influencing the evolution of <inline-formula><mml:math id="M194" 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> <xref ref-type="bibr" rid="bib1.bibx62" id="paren.52"/>. In the LWP time series (Fig. <xref ref-type="fig" rid="Ch1.F2"/>b), no significant changes are evident on day 1 in the perturbed cases as the plume coverage is quite small (Fig. <xref ref-type="fig" rid="Ch1.F2"/>a). A weak negative LWP adjustment is visible around midnight on day 2, where the baseline case has the highest LWP, and the value in the perturbed cases is lower depending on the total aerosol particles injected into the MBL. The negative LWP adjustment here is an outcome of the entrainment feedback associated with the reduction in the sedimentation flux of droplets <xref ref-type="bibr" rid="bib1.bibx6" id="paren.53"/> and enhanced evaporation rate near the cloud top <xref ref-type="bibr" rid="bib1.bibx56" id="paren.54"/>. During this time, <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in all the cases is identical. Note that the entrainment velocity (<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is inferred from changes in the inversion height (<inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mi>D</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M198" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is the large-scale divergence of the horizontal velocity field).</p>
      <p id="d1e3114">At sunrise on day 3, in the seeded cases, injection of aerosol suppresses precipitation and increases LWP relative to the baseline case (Fig. <xref ref-type="fig" rid="Ch1.F2"/>b, e). The degree of precipitation suppression is proportional to the amount of injected aerosol to that point in time. However, the gain in LWP is not directly proportional to the degree of precipitation suppression but is partly offset by entrainment effects (Fig. <xref ref-type="fig" rid="Ch1.F2"/>f). Furthermore, the increased <inline-formula><mml:math id="M199" 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> sustains slightly higher LWP relative to the baseline case until midday, after which the LWP in the seeded cases decreases below that of the baseline case. Similarly, higher <inline-formula><mml:math id="M200" 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> also sustains higher <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the morning and lower <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the afternoon. This reduction in LWP and <inline-formula><mml:math id="M203" 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 due to enhanced SW absorption associated with the higher LWP and <inline-formula><mml:math id="M204" 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 the morning (Fig. <xref ref-type="fig" rid="Ch1.F4"/>). The subsequent recovery in LWP and <inline-formula><mml:math id="M205" 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> late in the afternoon and early evening triggers strong precipitation in all the cases and significantly depletes <inline-formula><mml:math id="M206" 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> and <inline-formula><mml:math id="M207" 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> within the MBL. The precipitation (<inline-formula><mml:math id="M208" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> a few mm d<inline-formula><mml:math id="M209" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) breaks up the stratocumulus layer, as is evident from the decreasing values of <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The onset of the break-up (or transition) is controlled by the amount of aerosol injected into the MBL. The delay in the onset of the break-up is proportional to the number of injected particles into the MBL and is delayed the most in case 5<inline-formula><mml:math id="M211" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-220 (Fig. <xref ref-type="fig" rid="Ch1.F2"/>e). By the end of the simulation (morning of day 4), weak precipitation has started in case 5<inline-formula><mml:math id="M212" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-220. A longer simulation would be<?pagebreak page1925?> required to determine whether this would lead to the break-up of the stratocumulus layer. Additionally, suppression of precipitation deepens the boundary layer, as is evident from the inversion height (<inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) on days 3 and 4 (Fig. <xref ref-type="fig" rid="Ch1.F2"/>f).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e3286">Time series of the SW absorption by the cloud layer in NA150. See Fig. <xref ref-type="fig" rid="Ch1.F2"/>e for the color code.</p></caption>
          <?xmltex \igopts{width=221.931496pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f04.png"/>

        </fig>

      <p id="d1e3298">Figure <xref ref-type="fig" rid="Ch1.F5"/>a shows the Lagrangian evolution of the vertical profiles of <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in case 5<inline-formula><mml:math id="M215" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100, with the cloud-top and cloud-base heights marked by black lines. Figure <xref ref-type="fig" rid="Ch1.F5"/>b shows snapshots of <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at intervals of 8 h. Figure <xref ref-type="fig" rid="Ch1.F5"/>c shows the vertical integral of sub-cloud negative buoyancy flux integral, BFI <inline-formula><mml:math id="M217" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:mo>∫</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">air</mml:mi></mml:msub><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi mathvariant="normal">d</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M219" display="inline"><mml:mo lspace="0mm">∀</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), a measure of the decoupling between the cloud layer and surface <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx42" id="paren.55"/>. The minimum criterion for decoupling is BFI <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>&lt;</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> because vertical turbulent kinetic energy (TKE) is destructed, thus limiting vertical mixing. Here, <inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:msup><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> are fluctuating components of virtual potential temperature and vertical velocity, respectively, and the overline represents the horizontal average. The vertical profiles indicate that the boundary layer is well-mixed until sunrise on day 2, which is supported by the near-zero BFI. Thus, the injected aerosol from the first aerosol pulse mixes throughout the layer. On day 2, the boundary layer is deeper, but the vertical mixing is weaker due to the enhanced SW absorption from the increase in LWP. This is reflected in the increase in the (negative) magnitude of BFI. The same is evident from the accumulation of aerosol emitted from the ocean surface in the lower levels of the MBL. Post-sunset on day 2, the cloud layer continues to deepen, which further strengthens the decoupling from the surface. This continued deepening triggers weak collision–coalescence  and precipitation on the morning of day 3, accompanied by diverging values of BFI (around 02:00 LT). Note that runaway precipitation only occurs after the recovery of LWP and <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> during the night on day 3.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e3500"><bold>(a)</bold> Lagrangian curtains of <inline-formula><mml:math id="M226" 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>+<inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in case 5<inline-formula><mml:math id="M228" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100, with the black lines representing cloud base and cloud top. <bold>(b)</bold> Vertical profiles of <inline-formula><mml:math id="M229" 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>+<inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at select times (“d” is the day and “h” is the hour of the day). <bold>(c)</bold> Sub-cloud negative buoyancy flux integral, a measure of the degree of MBL mixing for all the cases. At any instant, more negative values of BFI indicate poorer vertical mixing.</p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f05.png"/>

        </fig>

      <p id="d1e3569"><?xmltex \hack{\newpage}?>The onset of weak precipitation increases mixing within the sub-cloud layer, as indicated by the BFI approaching zero in the 1<inline-formula><mml:math id="M231" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases between 02:00 and 12:00 LT on day 3. The strong suppression of precipitation in the 5<inline-formula><mml:math id="M232" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases enhances the decoupling due to increased cloud-top entrainment and MBL deepening (see the values of BFI between 02:00 and 10:00 LT on day 3). For 5<inline-formula><mml:math id="M233" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100, this enhanced decoupling associated with precipitation suppression is also evident from the vertical profiles of <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in Fig. <xref ref-type="fig" rid="Ch1.F5"/>b (e.g., d 2, h 5). This decoupling is sustained until the onset of runaway precipitation (e.g., d 2, h 13 and d 2, h 21 in Fig. <xref ref-type="fig" rid="Ch1.F5"/>b).</p><?xmltex \hack{\newpage}?>
<?pagebreak page1926?><sec id="Ch1.S3.SS1.SSSx1" specific-use="unnumbered">
  <title>Cloud radiative effect</title>
      <p id="d1e3623">To assess the impact of the various seeding scenarios under polluted conditions, we explore the changes to the cloud radiative effect CRE <inline-formula><mml:math id="M235" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mo>[</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>]</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">clr</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the incoming solar radiation. Figure <xref ref-type="fig" rid="Ch1.F6"/>a shows the changes to the CRE (dCRE <inline-formula><mml:math id="M238" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CRE<inline-formula><mml:math id="M239" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo><mml:mtext>-</mml:mtext><mml:mn mathvariant="normal">000</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M240" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> CRE<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">case</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">ID</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>) at the top of the atmosphere (TOA) relative to the baseline in all the seeded cases. No significant changes to CRE are detected on day 1 as the injected aerosol plume track is quite narrow. By day 2, we see a substantial enhancement in the CRE in all the seeded cases. On day 3, the  dCRE continues to grow. In some cases, this is due to an increase in aerosol concentration, but even in cases like 1<inline-formula><mml:math id="M242" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 and 5<inline-formula><mml:math id="M243" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 where no additional aerosol is added compared to day 2, we see a greater enhancement in dCRE on day 3. Note that the bulk of the dCRE enhancement occurs in the morning with a dominant peak around 08:00 to 10:00 LT. A similar result is evident in the simulations of <xref ref-type="bibr" rid="bib1.bibx42" id="text.56"/>. In the absence of precipitation, the clouds are thicker in the morning with near 100 % cloud coverage. The absorption of incoming SW radiation reduces the LWP and <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the afternoon. Consequently, the enhancement in CRE is greatest in the morning. In the afternoon of day 3, there is a hint of cloud darkening. The reason for this is discussed below, along with the dCRE decomposition. On day 4, there is a strong spread in dCRE due to variation in the timing of the transition. In the 1<inline-formula><mml:math id="M245" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, the dCRE is negligible, whereas the 5<inline-formula><mml:math id="M246" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases with two sprayers show a substantial increase in dCRE. In particular, 5<inline-formula><mml:math id="M247" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-220 shows the highest enhancement, with a morning peak value of about 250 W m<inline-formula><mml:math id="M248" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, which is well above the peaks on days 2 and 3.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e3801">Time series of changes in CRE relative to the unseeded case and its contributions. <bold>(a)</bold> dCRE, <bold>(b)</bold> <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE, <bold>(c)</bold> LWP contribution to dCRE, and <bold>(d)</bold> <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE. <inline-formula><mml:math id="M251" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the cloud optical thickness. The legend is shown in panel <bold>(d)</bold>.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f06.png"/>

          </fig>

      <p id="d1e3855">In order to obtain further process level insights, we decompose dCRE to three contributions: <inline-formula><mml:math id="M252" 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> (dCRE<inline-formula><mml:math id="M253" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula>), LWP (dCRE<inline-formula><mml:math id="M254" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:math></inline-formula>), and <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (dCRE<inline-formula><mml:math id="M256" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula>). We follow the procedure laid out in <xref ref-type="bibr" rid="bib1.bibx15" id="text.57"/> and <xref ref-type="bibr" rid="bib1.bibx12" id="text.58"/>. The dCRE decomposition is written as
              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M257" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{7.5}{7.5}\selectfont$\displaystyle}?><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">in</mml:mi></mml:msub><mml:mo mathsize="2.5em" mathvariant="italic">{</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub><mml:mfenced close="]" open="["><mml:mrow><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">pl</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:msub><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:munder></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub><mml:mfenced close="]" open="["><mml:mrow><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">pl</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:msub><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:mrow></mml:munder></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">pl</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">clr</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">clr</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mrow><mml:msub><mml:mi mathvariant="normal">dCRE</mml:mi><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:munder><mml:mo mathsize="2.5em" mathvariant="italic">}</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">clr</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the clear-sky albedo; <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi mathvariant="normal">cld</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the cloud albedo contribution from <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> or alternatively LWP; <inline-formula><mml:math id="M261" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> is cloud fraction; <inline-formula><mml:math id="M262" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is plume fraction; and the 0<inline-formula><mml:math id="M263" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>, pl, and bg subscripts indicate the baseline case, in-plume track, and off track (background), respectively. Note that dCRE<inline-formula><mml:math id="M264" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> has contributions from both <inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> adjustments, which is an outcome of the multiplicative nature of the contributions from <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M268" 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> to CRE (<inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:mo>∝</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). For instance, strong changes in <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are typically associated with precipitation. Under these conditions, LWP and <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and consequently <inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, are not constant. Therefore, dCRE<inline-formula><mml:math id="M273" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> has contributions from <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">cld</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that are not captured in the other two components (dCRE<inline-formula><mml:math id="M275" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> and dCRE<inline-formula><mml:math id="M276" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:math></inline-formula>). The residual from this budget is calculated as RES <inline-formula><mml:math id="M277" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> dCRE <inline-formula><mml:math id="M278" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> dCRE<inline-formula><mml:math id="M279" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M280" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> dCRE<inline-formula><mml:math id="M281" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M282" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> dCRE<inline-formula><mml:math id="M283" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula>. Note that the budget model (Eq. <xref ref-type="disp-formula" rid="Ch1.E1"/>) is based on mean-field properties, and does not account for the presence of inhomogeneities within the domain. Thus, the residual is a measure of the accuracy of the dCRE budget and of the inhomogeneities within the domain <xref ref-type="bibr" rid="bib1.bibx21" id="paren.59"/>.</p>
      <p id="d1e4560">Figure <xref ref-type="fig" rid="Ch1.F6"/>b–d show the time series of individual contributions to dCRE from <inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWP, and <inline-formula><mml:math id="M285" 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>, respectively. Table <xref ref-type="table" rid="Ch1.T1"/> provides averaged values between sunrise and sunset for each day. Below, percentage contributions of the three components to dCRE are calculated as 100 <inline-formula><mml:math id="M286" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> dCRE<inline-formula><mml:math id="M287" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M288" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> dCRE using the data from Table <xref ref-type="table" rid="Ch1.T1"/>. The dCRE<inline-formula><mml:math id="M289" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> component is positive and substantial on days 2 (over 100 %) and 3 (70 %–100 %). In the cases where no additional aerosol is injected after the first pulse, the dCRE<inline-formula><mml:math id="M290" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> component increases from day 2 to day 3 in the single-sprayer configuration (e.g., 5<inline-formula><mml:math id="M291" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 or 1<inline-formula><mml:math id="M292" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100), whereas in the twin-sprayer configuration (e.g., 5<inline-formula><mml:math id="M293" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200), the contributions are similar in magnitude, with a slightly higher contribution on day 3 because of the suppression of precipitation in the morning. In the single-sprayer configuration, apart from the effect of precipitation suppression, the greater areal coverage of the plume on day 3 results in a higher dCRE<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> component. On day 4, the dCRE<inline-formula><mml:math id="M295" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> is less than 20 % of dCRE. The dCRE<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:math></inline-formula> component is much lower than that of dCRE<inline-formula><mml:math id="M297" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> on day 2, but the two are comparable in magnitude on day 3. Additionally, the LWP contribution is positive in the morning and negative in the afternoon. On day 3, the positive contribution is an outcome of precipitation suppression in the morning. Some of these positive contributions are offset by the effects of entrainment, which explains the lack of a consistent trend in the 5<inline-formula><mml:math id="M298" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases. For instance, case 5<inline-formula><mml:math id="M299" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-220 has the strongest precipitation suppression (Fig. <xref ref-type="fig" rid="Ch1.F2"/>e), but cases 5<inline-formula><mml:math id="M300" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 and 5<inline-formula><mml:math id="M301" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 exhibit higher LWP and dCRE<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:math></inline-formula> in the morning. However, in the afternoon, the dCRE<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LWP</mml:mi></mml:msub></mml:math></inline-formula> is negative, with the highest magnitude for cases 5<inline-formula><mml:math id="M304" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 and 5<inline-formula><mml:math id="M305" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200, due to the negative LWP adjustment from enhanced SW absorption. The higher LWP in these cases in the morning makes them susceptible to SW absorption, as is evident from the weakly negative dCRE in the afternoon. A similar conclusion was obtained in an earlier study <xref ref-type="bibr" rid="bib1.bibx42" id="paren.60"/>. On the morning of day 4, the LWP component is negative and comparable in magnitude to the <inline-formula><mml:math id="M306" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> component. Both of their contributions to dCRE are low (<inline-formula><mml:math id="M307" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 20 %). On this day most of the contribution to dCRE is from the changes in <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> due to precipitation suppression.</p>
      <p id="d1e4824">From day 2 to day 4, the decoupling of the cloud layer from the surface increases, which favors the development of cumulus clouds. Moreover, the onset of precipitation further reduces the homogeneity within the domain. All of these<?pagebreak page1927?> contribute towards an increase in the magnitude of residual from day 2 to day 4 (column RES in Table <xref ref-type="table" rid="Ch1.T1"/>).</p>
</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>NA50: pristine system</title>
      <p id="d1e4838">Figure <xref ref-type="fig" rid="Ch1.F7"/>, analogous to Fig. <xref ref-type="fig" rid="Ch1.F2"/>, shows the evolution of cloud and aerosol properties in the system with <inline-formula><mml:math id="M309" 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> <inline-formula><mml:math id="M310" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 50 mg<inline-formula><mml:math id="M311" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. The lower initial <inline-formula><mml:math id="M312" 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> leads to an early onset of precipitation, even before the introduction of the first aerosol pulse (Fig. <xref ref-type="fig" rid="Ch1.F7"/>e), which leads to a very different aerosol plume and MBL evolution. In the baseline case, the precipitation-induced transition results in an open-cellular cloud structure. This structure is maintained until the end of the simulation. Note that the boundary layer is quite shallow, which supports the open cellular structure (Fig. <xref ref-type="fig" rid="Ch1.F7"/>f). This makes the transition reversible through aerosol addition <xref ref-type="bibr" rid="bib1.bibx20" id="paren.61"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e4896">As in Fig. <xref ref-type="fig" rid="Ch1.F2"/> but for case NA50.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f07.png"/>

        </fig>

      <p id="d1e4907">Figure <xref ref-type="fig" rid="Ch1.F7"/>a shows the evolution of plume area coverage. Qualitatively, its evolution is similar to the NA150 system with a monotonic increase in time. However, the spread rate in the current system is higher. For instance, case 5<inline-formula><mml:math id="M313" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 in NA150 attained a plume area fraction of 0.9 on day 2 around 12:00 LT. The same case in NA50 attains a similar plume area fraction on day 2 by 03:00 LT. A higher spread rate in NA50 is related to the flow patterns in the precipitating and precipitation-suppressed regions, which is discussed further in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS1"/> below.</p>
      <p id="d1e4922"><?xmltex \hack{\newpage}?>Figure <xref ref-type="fig" rid="Ch1.F7"/>b, c, and d show the cloud properties LWP, <inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M315" 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>, respectively.  In the baseline case, <inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> decrease after the onset of precipitation. The (cloudy-average) LWP shows an increasing trend, as expected in broken cumulus. The stronger updrafts associated with the convergence of surface flows form deeper clouds with higher LWP, although at the cost of low <inline-formula><mml:math id="M318" 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> <xref ref-type="bibr" rid="bib1.bibx53" id="paren.62"/>.</p>
      <p id="d1e4987">In all the perturbed cases, the impact of the seeding is visible in the <inline-formula><mml:math id="M319" 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> time series immediately and in the LWP and <inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> time series after about 20:00 LT on day 1. Injection of aerosol increases <inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M322" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and lowers the LWP relative to the baseline case for much of the duration of the simulation. These reductions in LWP are attributed to the deepening of the MBL (Fig. <xref ref-type="fig" rid="Ch1.F7"/>f) and manifest more strongly because of the reduction in <inline-formula><mml:math id="M323" 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>. After the initial increases in <inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> while the sprayers are active, there is a strong decline (especially in the strong perturbation cases). This decline continues until the aerosol plume spreads across the domain (approximately the middle of day 2). This reduction is due to the ongoing collision–coalescence along the plume track boundaries.</p>
      <?pagebreak page1928?><p id="d1e5059">In the 1<inline-formula><mml:math id="M325" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, the rain rate is slightly lower than the baseline for a few hours post-injection (day 1, approximately 20:00 LT). This decrease in precipitation is proportional to the number of injected aerosol particles. During this time the local (plume track) cloud coverage approaches 100 %. By the end of day 1, precipitation in the 1<inline-formula><mml:math id="M326" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases recovers and exceeds the baseline value, while <inline-formula><mml:math id="M327" 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> decreases subsequently, albeit at a slower rate than the baseline case. The higher domain-mean precipitation rate relative to the baseline case is sustained by the generation of non-precipitating or weakly precipitating clouds with lower LWPs and higher <inline-formula><mml:math id="M328" 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> occurring over a larger fraction of the domain (higher <inline-formula><mml:math id="M329" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Over time, as the aerosol plume spreads, <inline-formula><mml:math id="M330" 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> decreases locally within the plume track (not shown in Fig. <xref ref-type="fig" rid="Ch1.F7"/>c). This lowers the colloidal stability of the clouds, resulting in precipitation and subsequent cloud break-up. By the afternoon of day 2, <inline-formula><mml:math id="M331" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the 1<inline-formula><mml:math id="M332" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases is below 0.3 (comparable to the baseline case) with no signs of recovery.</p>
      <p id="d1e5141">For the higher seeded amounts, the injection of aerosol reduces precipitation significantly for the first 2–3 d (depending on the strength of the injection), allowing the boundary layer to establish a stratocumulus layer with <inline-formula><mml:math id="M333" 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> close to 1. Unlike in the 1<inline-formula><mml:math id="M334" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, the number concentration in the aerosol pulse is high enough to suppress precipitation in adjacent cells due to lateral spreading. The suppression of precipitation allows the MBL to deepen, which decreases <inline-formula><mml:math id="M335" 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> as a result of dilution (Fig. <xref ref-type="fig" rid="Ch1.F7"/>f). Subsequent precipitation events towards the end of day 3/day 4 result in a runaway effect and cloud break-up, marking the transition to cumulus clouds.</p>
      <p id="d1e5175">The counteracting effects on <inline-formula><mml:math id="M336" 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> of aerosol injections and MBL deepening play out in an interesting manner in cases 5<inline-formula><mml:math id="M337" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> and 8.6<inline-formula><mml:math id="M338" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>. <xref ref-type="bibr" rid="bib1.bibx55" id="text.63"/> argued that a concentrated injection is more effective than a distributed injection in enhancing the CRE in the presence of strong precipitation. The 8.6<inline-formula><mml:math id="M339" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 case can be considered a more concentrated version of 5<inline-formula><mml:math id="M340" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200. Compared to case 8.6<inline-formula><mml:math id="M341" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100, 5<inline-formula><mml:math id="M342" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 has more aerosol injected into the MBL; however <inline-formula><mml:math id="M343" 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 these two cases is comparable – in fact, <inline-formula><mml:math id="M344" 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 slightly higher for case 8.6<inline-formula><mml:math id="M345" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100. The difference comes from the depth of the MBL (Fig. <xref ref-type="fig" rid="Ch1.F7"/>f). The MBL height in 5<inline-formula><mml:math id="M346" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 is about 100–200 m greater than in 8.6<inline-formula><mml:math id="M347" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100. To leading order, the increase in <inline-formula><mml:math id="M348" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is proportional to the total injected aerosol number. Furthermore, the changes in LHF and sensible heat flux (SHF) in response to aerosol perturbations are broadly consistent with the deepening of the MBL (Fig. <xref ref-type="fig" rid="Ch1.F8"/>). The increased entrainment of drier and warmer free-tropospheric (FT) air enhances LHF and reduces SHF.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e5308">Time series of surface scalar fluxes in all the cases in NA50. See Fig. <xref ref-type="fig" rid="Ch1.F7"/> for legend. <bold>(a)</bold> Sensible heat flux (SHF) and <bold>(b)</bold> latent heat flux (LHF).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f08.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e5327">NA50. <bold>(a, b)</bold> Lagrangian curtains of <inline-formula><mml:math id="M350" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in cases 8.6<inline-formula><mml:math id="M351" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 and 5<inline-formula><mml:math id="M352" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200, respectively. The black curves represent the cloud-base and cloud-top heights. <bold>(c, d)</bold> Vertical profiles of <inline-formula><mml:math id="M353" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at intervals of 8 h in the cases shown in <bold>(a)</bold> and <bold>(b)</bold>.</p></caption>
          <?xmltex \igopts{width=469.470472pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f09.png"/>

        </fig>

      <?pagebreak page1929?><p id="d1e5399">Figure <xref ref-type="fig" rid="Ch1.F9"/>a and b show the Lagrangian evolution of the vertical profiles of <inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in cases 8.6<inline-formula><mml:math id="M355" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 and 5<inline-formula><mml:math id="M356" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200. A few snapshots at intervals of 8 h are shown in Fig. <xref ref-type="fig" rid="Ch1.F9"/>c and d for further clarity. The earlier and stronger precipitation suppression in 5<inline-formula><mml:math id="M357" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 starts deepening the MBL by the morning of day 2, which strengthens the decoupling of the cloud layer from the surface. This is evident from the time series of the BFI (Fig. <xref ref-type="fig" rid="Ch1.F10"/>). Furthermore, the deepening of the MBL enhances the LHF and reduces the SHF (Fig. <xref ref-type="fig" rid="Ch1.F8"/>). The corresponding increase in LWP is higher in 5<inline-formula><mml:math id="M358" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 compared to 8.6<inline-formula><mml:math id="M359" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100, which is evident in the afternoon of day 2 (Fig. <xref ref-type="fig" rid="Ch1.F7"/>b). Furthermore, the dilution associated with the deepening of the cloud layer and weaker net aerosol vertical transport from the surface layer maintains a lower <inline-formula><mml:math id="M360" 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 5<inline-formula><mml:math id="M361" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200. Note that <inline-formula><mml:math id="M362" 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 higher in case 5<inline-formula><mml:math id="M363" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 close to the surface. Thus, the differences in the final cloud break-up time in these cases is a manifestation of the differences in the boundary layer structure post-aerosol injection.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e5505">Negative buoyancy flux integral in the sub-cloud layer in cases 8.6<inline-formula><mml:math id="M364" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 and 5<inline-formula><mml:math id="M365" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f10.png"/>

        </fig>

<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Transverse circulation</title>
      <p id="d1e5535">The faster dispersal of the injected aerosol plume in NA50 is associated with the formation of a transverse circulation across the aerosol plume track <xref ref-type="bibr" rid="bib1.bibx54" id="paren.64"/>. The cross-sectional snapshots at different times in Fig. <xref ref-type="fig" rid="Ch1.F11"/> show the flow patterns in the plume-affected region and its neighborhood for case 8.6<inline-formula><mml:math id="M366" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100. Note that the vectors represent the velocity component after the mean horizontal wind has been removed. The <inline-formula><mml:math id="M367" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M368" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> cross sections in Fig. <xref ref-type="fig" rid="Ch1.F11"/>a, c, and e show the organization of the flow-field from the circulation near the cloud top along the plume track and its brief evolution in time (about 9 h). This circulation is created by the presence of a gradient in the rain rate across the plume track, which causes a corresponding buoyancy gradient that directs the circulation (filled contours in Fig. <xref ref-type="fig" rid="Ch1.F11"/>b, d, and f). Initially, the plume track exhibits slightly positive buoyancy, which is contrasted by strongly negative buoyant regions outside the plume track associated with evaporating precipitation. The strong convergence near the surface along the track is associated with the outflows from the adjacent precipitating cells that supply moisture to the plume track, making it more positively buoyant (Fig. <xref ref-type="fig" rid="Ch1.F11"/>b, d). Hence, the injected aerosol particles are lofted to the cloud layer within strong updrafts with velocities around 1–3 m s<inline-formula><mml:math id="M369" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F11"/>b, d). This suppresses precipitation, which causes strong outflows near the cloud top at the top of the plume track. These outflows spread horizontally until they encounter a counter flow from a neighboring cloud cell (<inline-formula><mml:math id="M370" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M371" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 60 km in Fig. <xref ref-type="fig" rid="Ch1.F11"/>d). This deflects the polluted outflow towards the cloud base in the neighboring cell (Fig. <xref ref-type="fig" rid="Ch1.F11"/>d, f), aiding in the faster dispersal of aerosol. Note that the spread rate of the plume is affected by the strength of the perturbation, with the 5<inline-formula><mml:math id="M372" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases having a faster spread rate compared to the 1<inline-formula><mml:math id="M373" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases. This is an outcome of the difference in the strength of the transverse circulations. The positive feedback associated with stronger in-track precipitation suppression and subsequent moisture convergence results in a stronger circulation. A detailed discussion about this precipitation gradient-induced mesoscale circulation is provided in <xref ref-type="bibr" rid="bib1.bibx54" id="text.65"><named-content content-type="post">Fig. 9b therein</named-content></xref>. Note that the meteorology and large-scale forcing in the current simulation are very different from those in <xref ref-type="bibr" rid="bib1.bibx54" id="text.66"/>, which supports the generality of this mechanism in the presence of aerosol gradients in a precipitating shallow boundary layer.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e5629"><bold>(a, c, e)</bold> <inline-formula><mml:math id="M374" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M375" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> cross sections of <inline-formula><mml:math id="M376" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <bold>(b, d, f)</bold> <inline-formula><mml:math id="M377" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M378" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> cross sections of buoyancy, for the case 8.6<inline-formula><mml:math id="M379" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100. The vectors represent the planar velocity field after subtracting the horizontal mean wind. <inline-formula><mml:math id="M380" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M381" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> cross sections are at <inline-formula><mml:math id="M382" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M383" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 700 m, and <inline-formula><mml:math id="M384" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M385" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> cross sections are at <inline-formula><mml:math id="M386" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M387" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 64 km. The green contour lines in the panels to the right indicate liquid water content of value 0.01 g kg<inline-formula><mml:math id="M388" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, and black contour lines (dashed) represent values of <inline-formula><mml:math id="M389" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M390" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 100 and 200 mg<inline-formula><mml:math id="M391" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. <bold>(a, b)</bold> <inline-formula><mml:math id="M392" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M393" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> day 0, 22:00 LT; <bold>(c, d)</bold> <inline-formula><mml:math id="M394" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M395" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> day 1, 01:00 LT; <bold>(e, f)</bold> <inline-formula><mml:math id="M396" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M397" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> day 1, 07:00 LT.</p></caption>
            <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f11.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Cloud radiative effect</title>
      <p id="d1e5865">Figure <xref ref-type="fig" rid="Ch1.F12"/>a shows the time series of dCRE for the NA50 cases. In all the cases, we see a dominant peak in the morning around 10:00 LT, similar to the dCRE profiles in NA150. In the 1<inline-formula><mml:math id="M398" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, an enhancement in CRE is evident only on the morning of day 2. In the 5<inline-formula><mml:math id="M399" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> and 8.6<inline-formula><mml:math id="M400" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, a substantial enhancement in CRE is evident on days 2 and 3. On day 4, the enhancement in CRE is significant but substantially weaker in comparison to the earlier days. This is due to the precipitation-related decrease in <inline-formula><mml:math id="M401" 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>. Table <xref ref-type="table" rid="Ch1.T2"/> and Fig. <xref ref-type="fig" rid="Ch1.F7"/>b, c, and d show the contributions to dCRE from <inline-formula><mml:math id="M402" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWP, and <inline-formula><mml:math id="M403" 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>, respectively. Note that the <inline-formula><mml:math id="M404" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-axis range is different for each panel. As in case N150, the percentage contributions of the three components to dCRE can be calculated from Table <xref ref-type="table" rid="Ch1.T2"/> as 100 <inline-formula><mml:math id="M405" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> dCRE<inline-formula><mml:math id="M406" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">LWP</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M407" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> dCRE. The dominant contribution to CRE derives from the changes to <inline-formula><mml:math id="M408" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the strong perturbation cases. The contribution from <inline-formula><mml:math id="M409" 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 positive, and its magnitude is less than 20 %–30 % of dCRE<inline-formula><mml:math id="M410" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula>. In contrast, the contribution from LWP is negative and is comparable in magnitude to that of dCRE<inline-formula><mml:math id="M411" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> on days 2 and 3. Similarly, in the 1<inline-formula><mml:math id="M412" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> cases, the <inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWP components are comparable in magnitude but of opposite sign.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e6046">Time series of changes to CRE (dCRE) and its contributions for case NA50. <bold>(a)</bold> dCRE, <bold>(b)</bold> <inline-formula><mml:math id="M414" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE, <bold>(c)</bold> LWP contribution to dCRE, and <bold>(d)</bold> <inline-formula><mml:math id="M415" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution to dCRE. <inline-formula><mml:math id="M416" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> is the cloud optical thickness. The legend is shown in panel <bold>(d)</bold>. Note that the <inline-formula><mml:math id="M417" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-axis range is different for each panel.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f12.png"/>

          </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
</sec>
<?pagebreak page1930?><sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e6119">In the previous section, we explored the impact of aerosol perturbation on the SCT. We considered two SCT scenarios, one in which strong precipitation only occurs in the afternoon of day 3 (NA150 – polluted) and the other in which strong precipitation occurs in the afternoon of day 1 (NA50 – pristine). The simulation results suggest that an aerosol perturbation delays the onset of the SCT in both scenarios. To leading order, the delay in the transition is proportional to the number of injected aerosol particles prior to the onset of the transition in both scenarios, which is broadly consistent with the results of <xref ref-type="bibr" rid="bib1.bibx63" id="text.67"/>.</p>
      <p id="d1e6125">In the polluted system, the transition is affected mainly by the total number of injected particles prior to the transition and not by the time sequence of the injections. This is evident from the fact that cases 1<inline-formula><mml:math id="M418" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-110 and 1<inline-formula><mml:math id="M419" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-101 follow a similar trajectory (except for the time when the plume is still spreading) for all the cloud properties (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) and break up around the same time. Additionally, the 5<inline-formula><mml:math id="M420" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 case and the delayed version of 5<inline-formula><mml:math id="M421" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100 (5 h delay in seeding) to leading order have similar evolution in cloud properties. A similar conclusion was drawn from the simulations in <xref ref-type="bibr" rid="bib1.bibx42" id="text.68"/> wherein a non-precipitating cloud system was subjected to a range of aerosol perturbations by varying the injection rate and duration of the perturbation. It was concluded that after the initial transient, the cloud system properties were determined only by the total number of aerosol particles injected into the cloud layer. Note that the cloud layer in the polluted simulations qualifies as a non-precipitating system until the morning of day 3, and all the aerosol pulses are active before this time. Furthermore, the addition of aerosol delays this onset of precipitation.</p>
      <p id="d1e6162">In the pristine system, all the aerosol pulses are active after the onset of precipitation. We see that the distribution in space and time of aerosol pulses plays an important role in the evolution of the cloud system. For instance, 1<inline-formula><mml:math id="M422" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-110 and 1<inline-formula><mml:math id="M423" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 have the same number of aerosol particles injected into the MBL; however their cloud properties have very different trajectories. Until the afternoon of day 2, <inline-formula><mml:math id="M424" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are higher for 1<inline-formula><mml:math id="M426" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200, after which the reverse is true. Note<?pagebreak page1931?> that the timing of this switch-over is consistent with the injection of the second pulse in 1<inline-formula><mml:math id="M427" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-110. The enhancement of precipitation post-aerosol perturbation in 1<inline-formula><mml:math id="M428" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 reduces the injected aerosol concentration within the MBL; however the enhancement in CRE is not significant in either of these cases after day 2. This illustrates the complexity in the evolution of the MBL properties in this system and is reinforced by the fact that the onset of SCT is not delayed the most for the strongest perturbation (5<inline-formula><mml:math id="M429" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200) but by a slightly weaker perturbation (8.6<inline-formula><mml:math id="M430" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100). The key difference is the depth of the inversion layer, which is proportional to the magnitude of the precipitation suppression. This enhanced depth dilutes <inline-formula><mml:math id="M431" 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> and also strengthens the decoupling of the cloud layer from the surface. The increased LHF due to entrainment deepening and stronger cumulus clouds trigger precipitation that results in the earlier transition in 5<inline-formula><mml:math id="M432" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 compared to 8.6<inline-formula><mml:math id="M433" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100.</p>
      <?pagebreak page1932?><p id="d1e6263">The CRE in both the polluted and pristine systems is enhanced post-aerosol perturbation. No substantial darkening tendency is evident in any of the simulations. The decomposition of CRE offers insights into the contributions from <inline-formula><mml:math id="M434" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWP, and <inline-formula><mml:math id="M435" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. In the polluted system, the dCRE increases from day 2 to day 4. The contributions from the negative LWP adjustment are around 10 %–30 % of <inline-formula><mml:math id="M436" 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>. On day 3, the positive adjustment in LWP in the morning is due to precipitation suppression, some of which is offset by the entrainment adjustment. The negative LWP adjustment in the afternoon is due to enhanced SW absorption. These counteracting effects reduce the net contribution from the LWP component (see Table <xref ref-type="table" rid="Ch1.T1"/>). Note that the negative adjustment in LWP due to entrainment (dominant during the night) is not significant in this system due to fairly high free-tropospheric humidity (<inline-formula><mml:math id="M437" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 3.5 g kg<inline-formula><mml:math id="M438" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). On day 4, the enhancement in CRE is largely a result of the changes to <inline-formula><mml:math id="M439" 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> associated with precipitation suppression, and its peak magnitude is approximately 75 % more than the dCRE peak on day 3. In the pristine system, the SCT is delayed the most in case 8.6<inline-formula><mml:math id="M440" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-100, resulting in the highest dCRE on day 4. However, the net brightness is not the highest for this case as the dCRE in case 5<inline-formula><mml:math id="M441" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>-200 is substantially higher on days 2 and 3. Additionally, the dominant contribution to dCRE is from the changes to <inline-formula><mml:math id="M442" 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> associated with precipitation suppression, which is consistent with earlier LES studies on MCB <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx29 bib1.bibx12 bib1.bibx42" id="paren.69"/>. On day 2, the contribution from <inline-formula><mml:math id="M443" 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 also substantial and comparable to <inline-formula><mml:math id="M444" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><?xmltex \opttitle{CRE vs. $N_{\mathrm{d}}$}?><title>CRE vs. <inline-formula><mml:math id="M445" 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></title>
      <p id="d1e6402">Using satellite data, <xref ref-type="bibr" rid="bib1.bibx24" id="text.70"/> showed recently that in spite of the saturation in cloud brightening that occurs at higher <inline-formula><mml:math id="M446" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (the albedo effect), CRE increases linearly with increasing <inline-formula><mml:math id="M447" 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>. This linear relationship is an outcome of the effect of <inline-formula><mml:math id="M448" 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> on <inline-formula><mml:math id="M449" 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> via delayed precipitation. This is consistent with our simulations where we see a proportionate delay in SCT with increasing aerosol injection. Figure <xref ref-type="fig" rid="Ch1.F13"/> shows that the CRE increases with <inline-formula><mml:math id="M450" 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 is a strong function of the solar zenith angle (SZA). <xref ref-type="bibr" rid="bib1.bibx24" id="text.71"/> do not account for the variability in SZA and use the average insolation. The peak values in CRE on each day occur between 08:00 and 10:00 LT in all cases. In the NA150 and NA50 cases (top and bottom panels in Fig. <xref ref-type="fig" rid="Ch1.F13"/>) we see a linear increase in CRE peaks with <inline-formula><mml:math id="M451" 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> on day 2. This is an outcome of the spreading of the plume areal coverage (<inline-formula><mml:math id="M452" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and CRE is directly proportional to <inline-formula><mml:math id="M453" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">AF</mml:mi><mml:mi mathvariant="normal">pl</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (see Eq. <xref ref-type="disp-formula" rid="Ch1.E1"/>). On day 3 in the NA150 cases, we see a deviation from the linear increase in CRE with <inline-formula><mml:math id="M454" 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>, which is related to the albedo effect (proportional to <inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:msubsup><mml:mi>N</mml:mi><mml:mi mathvariant="normal">d</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:mrow></mml:math></inline-formula>). During this time, the contribution from <inline-formula><mml:math id="M456" 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 negligible (see Table <xref ref-type="table" rid="Ch1.T1"/>). On day 4 in NA150, as well as day 3 in NA50, we see a near-linear increase in CRE with <inline-formula><mml:math id="M457" 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>. This is an outcome of precipitation suppression and corresponding changes to <inline-formula><mml:math id="M458" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. However, we see a weak hint of saturation in the NA150 cases on day 4, which could be related to higher <inline-formula><mml:math id="M459" 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 the NA150 cases. Note that the <inline-formula><mml:math id="M460" 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> range considered in <xref ref-type="bibr" rid="bib1.bibx24" id="text.72"/> is rather small (<inline-formula><mml:math id="M461" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 100 cm<inline-formula><mml:math id="M462" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) compared to the range considered here (between 25 and 500 cm<inline-formula><mml:math id="M463" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).<?pagebreak page1933?> Furthermore, the saturation in CRE could be related to the reduction in LWP from enhanced SW absorption and cloud-top entrainment, effects which were not taken into account in the satellite data analysis of <xref ref-type="bibr" rid="bib1.bibx24" id="text.73"/>. Currently, we do not have enough data to confirm this hypothesis. Thus, more studies under different meteorological conditions are required to ascertain the nature of the relationship between CRE and <inline-formula><mml:math id="M464" 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 the SCT.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e6645">CRE vs. <inline-formula><mml:math id="M465" 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> for each day in NA150 <bold>(a–c)</bold> and NA50 <bold>(d–f)</bold>. The color code for the top and bottom panel figures is the same as Figs. <xref ref-type="fig" rid="Ch1.F6"/> and <xref ref-type="fig" rid="Ch1.F12"/>, respectively. The separation between consecutive symbols indicates a time difference of 24 min. The black line connects the maximum values in CRE for each case.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f13.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>MCB and SCT</title>
      <p id="d1e6683">These insights indicate that if one considers deliberate injections of aerosol into NEP clouds where precipitation is not imminent (moderately to very polluted clouds), the focus should be to inject as many aerosol particles as possible into the MBL (until coagulation losses start to dominate; see <xref ref-type="bibr" rid="bib1.bibx4" id="altparen.74"/>) to enhance the brightness of the cloud deck. The aerosol perturbation should be performed while the ocean surface temperature is relatively cold as advection towards warmer waters strengthens the decoupling of the cloud layer from the surface, which reduces the efficiency of the vertical transport of the injected aerosol. Furthermore, since the spread rate of the aerosol plume is low under these conditions, a more widely distributed injection would aid in a faster dispersal of the injected aerosol. In the context of the pristine system, a high aerosol injection rate is required for a successful implementation of MCB. Since the aerosol plume spread rate in this system is high, the number of sprayers required could be lower. Additionally, if targeted brightening is considered, the pristine system would be more effective due to the substantial enhancement in the CRE due to rapid and strong <inline-formula><mml:math id="M466" 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> increases soon after aerosol injection ends. However, the frequency of occurrence of such clean boundary layers closer to the coast is very low <xref ref-type="bibr" rid="bib1.bibx57" id="paren.75"/>. With the new shipping regulations and a projected reduction in emissions <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx14" id="paren.76"/>, the frequency of occurrence of such cleaner boundary layers near the coast may increase. In the polluted system, strong changes in CRE are evident only after several hours post-aerosol perturbation. However, combined with their significantly greater frequency of occurrence, the net brightness enhancement from these cloud systems could be substantial. A more systematic analysis is required to confirm this and will be addressed in future studies.</p>
      <p id="d1e6706">A key question that arises from the results and the discussion here is as follows: to what extent can the SCT be delayed through aerosol perturbations? Additionally, if a substantially higher aerosol concentration is injected into the MBL, would that result in the classic SCT scenario where the transition is due to the warming of the ocean surface and not due to precipitation? The injection of aerosol enhances the colloidal stability of the cloud layer and suppresses precipitation, but it also enhances the entrainment rate of free-tropospheric air, which reduces LWP. However, higher aerosol concentrations deepen the cloud layer and thus have a tendency to enhance LWP <xref ref-type="bibr" rid="bib1.bibx48" id="paren.77"/>. The significance of these competing effects may vary on a case-by-case basis. Therefore, a wider variety of simulations under different conditions are required to address these questions.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Summary and outlook</title>
      <p id="d1e6722">In this study, we explored how the stratocumulus-to-cumulus transition (SCT) is affected by deliberate aerosol perturbations using a Lagrangian large-eddy simulation (LES) model coupled to a two-moment bulk microphysics scheme. We used the average trajectory from <xref ref-type="bibr" rid="bib1.bibx44" id="text.78"/>. The setup of these simulations is directed towards marine cloud brightening (MCB) – the deliberate injection of aerosol particles into the marine boundary layer to enhance the brightness of the marine stratocumulus clouds, thereby exerting a cooling effect on the planet. We considered two different baseline aerosol conditions: a polluted (150 particles mg<inline-formula><mml:math id="M467" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) background and a pristine background (50 particles mg<inline-formula><mml:math id="M468" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). We varied the aerosol injection rates per sprayer, number of sprayers, and number of aerosol pulses to assess the impact of various MCB strategies. Our results showed that the spread rate of the aerosol plume is faster in the pristine system due to the transverse circulation induced by the gradient in rain rate across the plume track. In response to the aerosol perturbation, the SCT is delayed in both polluted and pristine systems. To leading order, in the polluted scenario, the time delay in the transition is proportional to the amount of aerosol injected into the MBL and is only weakly affected by the distribution (in space and time) of the aerosol sprayers. The enhancement in cloud radiative effect (CRE) increases from day 2 to day 4. The changes in CRE are dominated by the albedo effect on days 2 and 3 and cloud fraction (<inline-formula><mml:math id="M469" 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>) adjustments on day 4. In the pristine system, only the strong perturbations make a substantial contribution to MCB. The weak perturbations are dissipated within a day through enhanced precipitation in the aerosol plume track. The time delay in SCT is affected by the total number of aerosol particles injected into the marine boundary layer and their distribution in space and time. A more concentrated but slightly weaker aerosol injection tends to delay the SCT more effectively than splitting it across two sprayers. The enhancement in CRE is dominated by <inline-formula><mml:math id="M470" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and is sustained for 2 d in the strongly perturbed cases.</p>
      <p id="d1e6774">The results presented here are based on the composite trajectory from a 2-year (2006–2007, June–August) climatology. This average trajectory may mask the variability in profiles, which may impact the SCT. For instance, faster advection or a faster SST increase may result in an early transition. In such a scenario, the time required for the aerosol plume to spread and the corresponding cloud adjustment timescales<?pagebreak page1934?> may affect the effectiveness of MCB. In other words, a different aerosol injection rate and sprayer configuration may be required under these conditions for the effective implementation of MCB. Thus, future studies should use more realistic conditions based on instantaneous soundings and forcings. Additionally, the current Lagrangian model does not account for the large-scale feedback associated with aerosol perturbation. Thus, further model improvements are warranted to better constrain the impact of aerosol perturbation <xref ref-type="bibr" rid="bib1.bibx11" id="paren.79"/>.</p>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Aerosol plume identification</title>
      <p id="d1e6791">The aerosol plume is detected by setting a threshold manually on the vertically integrated (0 <inline-formula><mml:math id="M471" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M472" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M473" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M474" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) aerosol concentration. For each of the baseline systems (NA150 and NA50), the same threshold values are used in all the perturbed cases. In the NA150 case, the background aerosol concentration has a variability of <inline-formula><mml:math id="M475" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>10 % about the mean value. We use a spatial Gaussian filter of five pixels width to smooth these fluctuations. This causes artificial broadening of the plume during its initial evolution period. However, with time, the effect of the filter is weakened due to the increase in plume area coverage. In the NA50 system, the signal-to-noise ratio is very high, even for the weak perturbations (1<inline-formula><mml:math id="M476" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>). Thus, no filtering is used in determining the plume area coverage in NA50. The time series of the threshold values used in this study is shown in Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F14"/>. The threshold values change with time due to the changes in the background conditions. In the NA150 system, the threshold value is nearly constant, with minor (within 15 % of the start value) changes during the evolution of the system. On the other hand, in the NA50 system, the threshold value decreases quickly with time to account for the losses from precipitation in the region away from the plume track. Since the threshold values are the same for all the aerosol plume tracks in each system, a sensitivity test on these threshold is not required as the relative trend in the spread rates would be similar.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.S1.F14"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e6845">Time series of the threshold values for identifying plume in NA150 and NA50.</p></caption>
        <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://acp.copernicus.org/articles/24/1919/2024/acp-24-1919-2024-f14.png"/>

      </fig>

</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e6858">The simulations were carried out using SAM  <xref ref-type="bibr" rid="bib1.bibx34" id="paren.80"/>, which is publicly available at the Harvard repository (<uri>https://wiki.harvard.edu/confluence/display/climatemodeling/SAM</uri>, <xref ref-type="bibr" rid="bib1.bibx32" id="altparen.81"/>). The data from the simulations are available from the NOAA Chemical Sciences Laboratory's Clouds, Aerosol, &amp; Climate<?pagebreak page1935?> program at <uri>https://csl.noaa.gov/groups/csl9/datasets/data/cloud_phys/2023-Prabhakaran-etal/</uri> <xref ref-type="bibr" rid="bib1.bibx41" id="paren.82"/>.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e6879">PP, FH, and GF designed the research. PP carried out the simulations and analysis. PP, FH, and GF discussed the results. PP wrote the manuscript with input from FH and GF.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e6885">At least one of the (co-)authors is a member of the editorial board of <italic>Atmospheric Chemistry and Physics</italic>. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e6894">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. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e6900">Marat Khairoutdinov graciously provided the SAM model. Jianhao Zhang, CIRES/NOAA-CSL, provided the data for Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e6907">This research has been supported by the U.S. Department of Commerce (Earth's Radiation Budget grant, NOAA CPO Climate &amp; CI (grant no. 03-01-07-001) and NOAA Cooperative Agreement with CIRES (grant no. NA17OAR4320101)) and the Emmy Noether program of the German Research Foundation (Deutsche Forschungsgemeinschaft, DFG (grant no. HO 6588/1-1)).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e6913">This paper was edited by Hailong Wang and reviewed by two anonymous referees.</p>
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