<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<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-22-15767-2022</article-id><title-group><article-title>Equilibrium climate sensitivity increases with aerosol concentration due to changes in precipitation efficiency</article-title><alt-title>Equilibrium climate sensitivity</alt-title>
      </title-group><?xmltex \runningtitle{Equilibrium climate sensitivity}?><?xmltex \runningauthor{G. Dagan}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Dagan</surname><given-names>Guy</given-names></name>
          <email>guy.dagan@mail.huji.ac.il</email>
        <ext-link>https://orcid.org/0000-0002-8391-6334</ext-link></contrib>
        <aff id="aff1"><institution>Fredy and Nadine Herrmann Institute of Earth Sciences, Hebrew
University, Jerusalem, Israel</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Guy Dagan (guy.dagan@mail.huji.ac.il)</corresp></author-notes><pub-date><day>16</day><month>December</month><year>2022</year></pub-date>
      
      <volume>22</volume>
      <issue>24</issue>
      <fpage>15767</fpage><lpage>15775</lpage>
      <history>
        <date date-type="received"><day>10</day><month>August</month><year>2022</year></date>
           <date date-type="rev-request"><day>22</day><month>August</month><year>2022</year></date>
           <date date-type="rev-recd"><day>13</day><month>November</month><year>2022</year></date>
           <date date-type="accepted"><day>3</day><month>December</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</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="d1e79">How Earth's climate reacts to anthropogenic forcing is one of the most
burning questions faced by today's scientific community. A leading source of
uncertainty in estimating this sensitivity is related to the response of
clouds. Under the canonical climate-change perspective of forcings and
feedbacks, the effect of anthropogenic aerosols on clouds is categorized
under the forcing component, while the modifications of the radiative
properties of clouds due to climate change are considered in the feedback
component. Each of these components contributes the largest portion of
uncertainty to its relevant category and is largely studied separately from
the other. In this paper, using idealized cloud-resolving radiative–convective-equilibrium simulations, with a slab ocean model, we
show that aerosol–cloud interactions could affect cloud feedback.
Specifically, we show that equilibrium climate sensitivity increases under
high aerosol concentration due to an increase in the short-wave cloud
feedback. The short-wave cloud feedback is enhanced under high-aerosol
conditions due to a stronger increase in the precipitation efficiency with
warming, which can be explained by higher sensitivity of the droplet size
and the cloud water content to the CO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration rise. These
results indicate a possible connection between cloud feedback and
aerosol–cloud interactions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e100">Estimating Earth's equilibrium climate sensitivity (ECS), defined as the
steady-state global-mean temperature increase for a doubling of CO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, is
considered to be a first-order, fundamental milestone on the way to
understanding and predicting anthropogenically driven climate change (Sherwood
et al., 2020). Decades of research have tried to accurately quantify ECS,
with only limited success. The most probable current ECS estimates are in
the range of 2.3–4.5 K (Sherwood et al., 2020). The largest source of
uncertainty in estimating ECS is related to the response of clouds to the
externally forced warming and the feedback of these changes on the climate
system (Sherwood et al., 2020; Ceppi et al., 2017; Schneider et al., 2017).
Clouds strongly modulate Earth's radiation budget by reflecting the incoming
short-wave radiation from the sun and by absorbing and re-emitting the
terrestrial long-wave radiation (Loeb et al., 2018). Thus, changes in the
cloud macro-physical properties (such as coverage and vertical extent) and
micro-physical properties (such as liquid/ice partition and hydrometeors
size) due to anthropogenically driven climate change could significantly alter
the climate system's response (Gettelman and Sherwood, 2016; Nuijens and
Siebesma, 2019; Schneider et al., 2017).</p>
      <p id="d1e112">An important factor in determining cloud feedback magnitude is the
sensitivity of the precipitation efficiency (<inline-formula><mml:math id="M3" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>) (Lutsko and Cronin, 2018; Lutsko et al.,
2021; Li et al., 2022). <inline-formula><mml:math id="M4" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> quantifies the
fraction of condensed water in a cloud to reach the surface as
precipitation. Using idealized cloud-resolving simulations, it was shown
that <inline-formula><mml:math id="M5" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> is expected to increase with temperature (Lutsko and
Cronin, 2018). The increase in <inline-formula><mml:math id="M6" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> with warming was shown to be
mostly driven by an increase in the efficiency with which cloud condensate
is converted into precipitation, while changes in the evaporation of falling
precipitation were shown to play a smaller role (Lutsko and Cronin, 2018).</p>
      <p id="d1e143">An increase in <inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> with warming represents more efficient depletion
of the water from the clouds, thus affecting the radiation budget. On the
one hand, increase in <inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> with warming was suggested to reduce the
anvil cloud coverage and hence increase the outgoing long-wave radiation
(Lindzen et al., 2001; Mauritsen and Stevens, 2015), thus producing negative
feedback. On the other hand, however, it was recently shown that the
long-wave effect of an <inline-formula><mml:math id="M9" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> increase is over-compensated for by
changes in the short-wave flux (Li et al., 2019); i.e. a large reduction in
the cloud optical depth, driving a reduction in the short-wave cooling effect
of clouds, dominates the response.</p>
      <p id="d1e167">The efficiency with which cloud condensate is converted into precipitation
is closely linked to the micro-physical properties of the clouds. The
autoconversion of cloud droplets into rain becomes significant when liquid
water amount and/or droplet radii reach a critical threshold (Freud and
Rosenfeld, 2012). An important factor influencing the droplet radii (and
also the liquid water amount, to some degree) is the amount of available
cloud condensation nuclei (CCN). Generally, an increase in aerosol
concentration drives an increase in CCN concentration, which results in more
numerous and smaller droplets in the cloud (Twomey, 1974; Warner and Twomey,
1967). The smaller droplets require longer time (or equivalently larger
vertical distance) in the clouds to grow by diffusion to the critical size
enabling precipitation, thus delaying the initial warm-rain formation
(Rosenfeld, 2000; Dagan et al., 2015b). In addition, aerosols were suggested
to enhance the vertical velocities and the cloud top heights of deep
convective clouds (due to the so-called invigoration mechanism; Abbott and
Cronin, 2021; Koren et al., 2005; Rosenfeld et al., 2008), which in turn
can result in precipitation enhancement (Koren et al., 2012). Therefore,
aerosols could affect <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> (Khain, 2009).</p>
      <p id="d1e178">In addition to the effect on rain, aerosols could modify the radiative
properties of clouds by modifying the droplet concentration and size
distribution (Twomey, 1974) and by affecting the clouds' macro-physical
properties (Albrecht, 1989; Bellouin et al., 2019). These changes to the
radiative properties of clouds result in radiative forcing that could affect
the sea surface temperature (SST; Bellouin et al., 2019). Using
cloud-resolving radiative–convective-equilibrium simulations with
interactive SST, Khairoutdinov and Yang (2013) showed that the surface
temperature decreases by 1.5 K with each 10-fold increase in aerosol
concentration, an effect quite comparable to a 2.1–2.3 K SST warming
obtained in a simulation with given (low-)aerosol conditions but doubled
CO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration.</p>
      <p id="d1e190">It has been suggested that cloud feedback and aerosol forcing are not
independent of each other (Mülmenstädt and Feingold, 2018; Igel and
van den Heever, 2021). In addition, the strong links between <inline-formula><mml:math id="M12" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> and
cloud feedback and between <inline-formula><mml:math id="M13" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> and aerosol concentration merit a
dedicated study on the potential mutual CO<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and aerosol effect on
clouds and thus also on ECS, which is the aim of the current study.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Model description and experimental design</title>
      <p id="d1e231">The model used herein is the System of Atmospheric Modeling (SAM;
Khairoutdinov and Randall, 2003) version 6.11.7. Subgrid-scale fluxes are
parameterized using Smagorinsky's eddy diffusivity model, and gravity waves
are damped at the top of the domain. The microphysics scheme used is the two-moment bulk microphysics of Morrison et al. (2005). The cloud droplet number
concentration (CDNC) source assumes that the number of activated CCN depends on the
super-saturation (<inline-formula><mml:math id="M15" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> – which is estimated diagnostically in the model as the
model assumes saturation adjustment) according to a power law: CDNC <inline-formula><mml:math id="M16" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:msup><mml:mi>S</mml:mi><mml:mi>k</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M18" 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 the prescribed concentration of CCN active at
1 % super-saturation, and <inline-formula><mml:math id="M19" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> is a constant (set in this study to 0.4 – a
typical value for maritime conditions). Changes in <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> serve as a proxy
for the change in aerosol concentration. Three levels of <inline-formula><mml:math id="M21" 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> are
considered here, covering an extreme range of conditions – 20, 200 and 2000 cm<inline-formula><mml:math id="M22" 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>. While this wide range of conditions is unlikely to exist at any
given geographical location, they are used here in order to cover the range
of possible conditions at different locations and to maximize the effect for
establishing better physical understanding. The activation of CCN at the
cloud base is parameterized following Twomey (1959), using the vertical
velocity and CCN spectrum parameters. The model is configured to pass cloud
water and ice-crystal effective radii from the microphysics scheme to the
radiation scheme; thus, the Twomey effect (Twomey, 1977) of both liquid and
ice is considered. Direct interactions between aerosols and radiation are
not considered here.</p>
      <p id="d1e317">The simulations are conducted in a radiative–convective-equilibrium (RCE)
mode and generally follow the RCEMIP (RCE Model Intercomparison Project;
Wing et al., 2018) small-domain instructions (but with interactive SST and
changes in the CO<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and aerosol concentration). The simulations were
performed on a square, doubly periodic domain. In this case, we want to
avoid the effect of convective self-aggregation on <inline-formula><mml:math id="M24" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>; thus, the
domain size is set to <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mn mathvariant="normal">96</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">96</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>, which was shown to be small enough to
prevent convective self-aggregation (Muller and Held, 2012; Lutsko and
Cronin, 2018; Yanase et al., 2020). The horizontal grid spacing is set to
1 km, and 68 vertical levels are used, between 25 m and 31 km, with vertical
grid spacing increasing from 50 m near the surface to roughly 1 km at the
domain top. We note that while shallow clouds are present in the
simulations, the grid spacing used here is too coarse for a full
representation of these clouds. A time step of 10 s is used, and radiative
fluxes are calculated every 5 min using the CAM radiation scheme (Collins et
al., 2006). The output resolution for all fields is 1 h (3-D fields are saved
as snapshots, while domain statistics are saved as hourly averages). The
incoming solar radiation is fixed at 551.58 W m<inline-formula><mml:math id="M27" 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>, with a zenith angle of
42.05<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Wing et al., 2018), producing a net insolation close to
the tropical-mean value. Convection is initialized with a small thermal
noise added near the surface at the beginning of the simulation. The initial
conditions for the simulations are as in Wing et al. (2018).</p>
      <p id="d1e379">Greenhouse gases are varied for three different levels: pre-industrial level
(280 ppm; <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), 2 times the pre-industrial level (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and 4 times
the pre-industrial level (<inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>). As in the case of the aerosol
concentrations, the large range of CO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> conditions covered here are used
to examine the clouds' sensitivity to greenhouse gas concentrations under a
wide range of conditions. Nine different simulations, with all possible
combinations of <inline-formula><mml:math id="M36" 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 CO<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations, were conducted. The
O<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> vertical profile is similar to Wing et al. (2018) and represents a
typical tropical atmosphere. The effect of other trace gases (such as
CH<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and N<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O) is neglected for simplicity.</p>
      <p id="d1e497">In all simulations, the SST is interactive and predicted by a slab ocean
model (SOM). The SOM's mixed layer depth is set to 5 m, which represented a
compromise between a relatively deep layer (<inline-formula><mml:math id="M41" display="inline"><mml:mo lspace="0mm">≥</mml:mo></mml:math></inline-formula> 10 m), which reduces SST
noise (Khairoutdinov and Yang, 2013), and a relatively shallow layer (<inline-formula><mml:math id="M42" display="inline"><mml:mo lspace="0mm">≪</mml:mo></mml:math></inline-formula> 1 m), which requires a shorter computation time for equilibrium (Romps,
2020). As in Romps (2020), the SOM is cooled at a rate of 112 W m<inline-formula><mml:math id="M43" 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> in
order to ensure that the simulations with <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M45" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are kept at around the
initial SST of 300 K (Fig. 1). Each simulation was run for 1800 d, which
is sufficient for reaching close to equilibrium (the surface energy
imbalance is <inline-formula><mml:math id="M46" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 0.1 W m<inline-formula><mml:math id="M47" 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> in all simulations during the last 150 d). The last 150 d of each run is used for statistical sampling (grey
shading in Fig. 1).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e568"><bold>(a)</bold> The sea surface temperature (SST) along time for the different
simulations conducted under different aerosol and CO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations.
The shaded grey area is referred to as equilibrium conditions. <bold>(b)</bold> Change in
equilibrium SST due to a change in CO<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (compared to the
<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> case of each aerosol concentration), for the different aerosol
concentrations (the different curves).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f01.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e628">Figure 1 presents the SST of the different simulations along time (panel a)
and the change in the equilibrium SST with the CO<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration for
the different <inline-formula><mml:math id="M53" 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> cases (panel b). As expected, the equilibrium SST (grey
shading in Fig. 1a) increases with the CO<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration and decreases
with <inline-formula><mml:math id="M55" 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> concentration. However, the rate of increase in equilibrium SST
with CO<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration increases under extremely high <inline-formula><mml:math id="M57" 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>
concentrations (2000 cm<inline-formula><mml:math id="M58" 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 with the low and medium <inline-formula><mml:math id="M59" 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>
concentrations (20 and 200 cm<inline-formula><mml:math id="M60" 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>, respectively; Fig. 1b). Calculating
the average ECS based on the three combinations available for each <inline-formula><mml:math id="M61" 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>
condition (<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M64" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M69" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
(<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M74" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>) demonstrates that it increases with <inline-formula><mml:math id="M77" 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> from
3.0 K at the lowest <inline-formula><mml:math id="M78" 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> to 3.7 K at the highest <inline-formula><mml:math id="M79" 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> (i.e. a 23 %
increase; Table 1).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e921">Average equilibrium climate sensitivity (ECS), cloud feedback
parameter (<inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), hydrological sensitivity (<inline-formula><mml:math id="M81" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula>) and change in precipitation efficiency (<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi></mml:mrow></mml:math></inline-formula>) of the three combinations available for each
<inline-formula><mml:math id="M83" 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> condition (<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M86" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M91" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M93" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M95" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M96" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M98" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>). For the calculation of the average ECS, the
difference between <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M100" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is divided by 2. The rest of
the quantities are normalized by the SST change between the relevant
simulations. Please refer to the text for the definitions of these
quantities.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="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:thead>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M103" 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></oasis:entry>
         <oasis:entry colname="col2">ECS</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M105" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">[cm<inline-formula><mml:math id="M107" 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>]</oasis:entry>
         <oasis:entry colname="col2">[K]</oasis:entry>
         <oasis:entry colname="col3">[W m<inline-formula><mml:math id="M108" 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> K<inline-formula><mml:math id="M109" 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>]</oasis:entry>
         <oasis:entry colname="col4">[% K<inline-formula><mml:math id="M110" 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>]</oasis:entry>
         <oasis:entry colname="col5">[% K<inline-formula><mml:math id="M111" 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>]</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">20</oasis:entry>
         <oasis:entry colname="col2">3.0</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M112" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.45</oasis:entry>
         <oasis:entry colname="col4">3.8</oasis:entry>
         <oasis:entry colname="col5">1.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">200</oasis:entry>
         <oasis:entry colname="col2">3.1</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M113" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.38</oasis:entry>
         <oasis:entry colname="col4">4.3</oasis:entry>
         <oasis:entry colname="col5">1.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2000</oasis:entry>
         <oasis:entry colname="col2">3.7</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M114" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.08</oasis:entry>
         <oasis:entry colname="col4">4.6</oasis:entry>
         <oasis:entry colname="col5">2.7</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1360">Figure 2 presents the time- and domain-mean vertical profiles of temperature
and water vapour mixing ratio (<inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in the different simulations (panels a
and b) and their difference from the simulation with the lowest <inline-formula><mml:math id="M116" 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
CO<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations (panels c and d). It demonstrates, as expected, that
the vertical profile of air temperature is set by the surface temperature
(increases with CO<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and decreases with <inline-formula><mml:math id="M119" 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>) with an
amplification of the change at the upper troposphere, as the profiles follow
the moist adiabatic lapse rate. It also shows that <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> increases with the
temperature, as expected (Held and Soden, 2006).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1429">Time- and domain-mean vertical profiles of air temperature and
water vapour mixing ratio (<inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in the different simulations <bold>(a, b)</bold> and
how they differ from the simulation with the lowest <inline-formula><mml:math id="M122" 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 CO<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations <bold>(c, d)</bold>.</p></caption>
        <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f02.png"/>

      </fig>

      <p id="d1e1475">In order to understand the increase in ECS with <inline-formula><mml:math id="M124" 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>, we next examine the
top-of-atmosphere (TOA) energy budget. Figure 3 presents the change in the
net short-wave and long-wave TOA energy gain (<inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>,
respectively) with the CO<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration for the different <inline-formula><mml:math id="M128" 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>
conditions. In addition, Fig. 3 presents the change in the cloud radiative
effect (CRE) with increasing the CO<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, where CRE is
computed by subtracting the clear-sky from the all-sky TOA radiative fluxes
(<inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mtext>clear-sky</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>), again for the short wave and long wave separately
(CRE<inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:math></inline-formula> and CRE<inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:math></inline-formula>, respectively). Figure 3a and b demonstrate that
under equilibrium conditions <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> increases, while <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> decreases with
the CO<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration. However, the rate of change in both <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> is much faster under the high-<inline-formula><mml:math id="M138" 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> conditions than under the low-
and medium-<inline-formula><mml:math id="M139" 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> conditions. The trend in CRE<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:math></inline-formula> under the different
<inline-formula><mml:math id="M141" 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> conditions (Fig. 3c) resembles the trend in <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, suggesting that
the clouds' response dominates the changes in the TOA short-wave fluxes.
CRE<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:math></inline-formula>, on the other hand, decreases at a similar rate with CO<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration for the different <inline-formula><mml:math id="M145" 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> conditions (Fig. 3d). Thus, the
different decrease rates in <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> with CO<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration for the
different <inline-formula><mml:math id="M148" 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> conditions (Fig. 3b) must be driven by clear-sky changes
(specifically, the plank, the lapse rate and the water vapour feedbacks;
see Fig. 2 above).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1745">The change in the net top-of-atmosphere energy gain (<inline-formula><mml:math id="M149" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) in the
short wave <bold>(a)</bold> and in the long wave <bold>(b)</bold> and the change in the cloud radiative
effect (CRE) in the short wave <bold>(c)</bold> and in the long wave <bold>(d)</bold>, due to a change
in the CO<inline-formula><mml:math id="M150" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (compared to the <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M152" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> case of each
aerosol concentration), for the different aerosol concentrations (the
different curves).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f03.png"/>

      </fig>

      <p id="d1e1802">In Table 1 above, we estimate the average cloud radiative feedback
(<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) as the change in CRE with increasing surface
temperature, i.e. <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> dCRE <inline-formula><mml:math id="M155" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> d<inline-formula><mml:math id="M156" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, for the different
<inline-formula><mml:math id="M157" 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> conditions. The table shows that <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> becomes less
negative with the increase in <inline-formula><mml:math id="M159" 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>, leading to higher climate sensitivity.
The differences in the values of <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> between the different
<inline-formula><mml:math id="M161" 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> conditions are mostly derived from the short-wave part of the spectrum
(Fig. 3).</p>
      <p id="d1e1899">Thus far, we have seen that the ECS increases with <inline-formula><mml:math id="M162" 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> (Fig. 1 and Table 1) and that this increase can be explained by changes in <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Table 1) and specifically in CRE<inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:math></inline-formula> (Fig. 3). To understand
the changes in the cloud properties driving the changes in <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and hence also in ECS, under the different <inline-formula><mml:math id="M166" 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> conditions,
in Fig. 4 we present the change in cloud liquid water path (CWP), ice water
path (IWP), rainwater path (RWP) and cloud fraction (CF) with increasing
CO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations for the different <inline-formula><mml:math id="M168" 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> conditions. The figure
shows that the CWP decreases with the CO<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at a much
faster rate (about 3 times faster) under the highest-<inline-formula><mml:math id="M170" 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> conditions
compared to the low- and medium-<inline-formula><mml:math id="M171" 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> conditions (Fig. 4a). The changes in
the IWP, on the other hand, are about an order of magnitude smaller than the
changes in CWP and are not consistent in sign for the different <inline-formula><mml:math id="M172" 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>
conditions (Fig. 4b). The RWP increases with the CO<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at
a slightly faster rate (about 20 % faster) under the highest-<inline-formula><mml:math id="M174" 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>
conditions compared to the low- and medium-<inline-formula><mml:math id="M175" 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> conditions (however the
response is non-monotonic with <inline-formula><mml:math id="M176" 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>; Fig. 4c). The CF decreases with the
CO<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at a similar rate for the different <inline-formula><mml:math id="M178" 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>
conditions (about 1.5 % decrease in CF for each doubling of the CO<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations; Fig. 4d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2094">The change in <bold>(a)</bold> cloud liquid water path (CWP), <bold>(b)</bold> ice water path
(IWP), <bold>(c)</bold> rainwater path (RWP) and <bold>(d)</bold> cloud fraction (CF) due to a change
in the CO<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (compared to the <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> case of each
aerosol concentration), for the different aerosol concentrations (the
different curves).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f04.png"/>

      </fig>

      <p id="d1e2144">The faster decrease in CWP with CO<inline-formula><mml:math id="M183" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations under high-<inline-formula><mml:math id="M184" 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>
conditions drives the faster increase in CRE<inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:math></inline-formula> as the clouds become
less opaque in the short wave. We note that the difference in CRE<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">SW</mml:mi></mml:msup></mml:math></inline-formula>
trend under different <inline-formula><mml:math id="M187" 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> conditions could not be explained by the minor
differences in the CF trends. In addition, the small differences in the IWP
between the different <inline-formula><mml:math id="M188" 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> conditions are consistent with the small
differences in the CRE<inline-formula><mml:math id="M189" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">LW</mml:mi></mml:msup></mml:math></inline-formula> seen above. The general increase in RWP with
CO<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations is consistent with an increase in precipitation efficiency
with warming (Lutsko and Cronin, 2018), as elaborated below.</p>
      <p id="d1e2226">Figure 4 suggests that the largest difference in the cloud response to
CO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> under different <inline-formula><mml:math id="M192" 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> conditions is due to changes in CWP. The
higher sensitivity of CWP to CO<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration under higher-<inline-formula><mml:math id="M194" 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>
conditions can explain the higher <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and thus also the
larger ECS. Hence, the question arises: what causes the faster reduction in
CWP with CO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration under high-<inline-formula><mml:math id="M197" 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> conditions? A major sink
for CWP is via precipitation. Hence, in Fig. 5 we present the change in the
mean surface precipitation rate, the hydrological sensitivity (<inline-formula><mml:math id="M198" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula> – the
rate of change in the surface precipitation per 1 K increase in surface
temperature) and the precipitation efficiency (<inline-formula><mml:math id="M199" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> – calculated
following Li et al., 2022, as the ratio of surface
precipitation to condensed water path, i.e. CWP <inline-formula><mml:math id="M200" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> IWP <inline-formula><mml:math id="M201" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> RWP). Please note
that the precipitation efficiency definition used here, following Li et al. (2022), is slightly different from the definition used in Lutsko and Cronin (2018). However, the two different definitions were shown to be tightly
correlated (Li et al., 2022); thus, the exact definition used is not
expected to change the main conclusions. In addition, the use of this
definition will enable easier   comparison with observations and global climate
models in the future.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e2331">The change in <bold>(a)</bold> surface precipitation, <bold>(b)</bold> hydrological
sensitivity (<inline-formula><mml:math id="M202" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula>) and <bold>(c)</bold> precipitation efficiency
(<inline-formula><mml:math id="M203" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>) due to a change in the CO<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration
(compared to the <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> case of each aerosol concentration), for the
different aerosol concentrations (the different curves).</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f05.png"/>

      </fig>

      <p id="d1e2392">As expected, Fig. 5 demonstrates that the surface precipitation increases
with CO<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (i.e. <inline-formula><mml:math id="M208" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula> is positive), and so does <inline-formula><mml:math id="M209" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> (Lutsko
and Cronin, 2018). This is true for all <inline-formula><mml:math id="M210" 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> conditions. However, the
rates of increase in surface precipitation and <inline-formula><mml:math id="M211" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> with CO<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration are higher under the highest-<inline-formula><mml:math id="M213" 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> conditions (see also Table 1). We note that the larger rate of increase in surface precipitation under
the highest-<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:mrow></mml:math></inline-formula> conditions is not solely due to the higher surface
temperature increase, as <inline-formula><mml:math id="M215" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula> also increases with <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:mrow></mml:math></inline-formula>.</p>
      <p id="d1e2487">The much larger (more than double; Table 1) rate of increase in <inline-formula><mml:math id="M217" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>
with the CO<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration under the highest-<inline-formula><mml:math id="M219" 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> conditions
represents more efficient depletion of the cloud water from the atmosphere,
leading to a faster reduction in CWP with CO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (Fig. 4),
which in turn leads to higher <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and ECS. The faster
increase in RWP with CO<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration under the highest-<inline-formula><mml:math id="M223" 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>
conditions presented in Fig. 4c is consistent with this explanation.</p>
      <p id="d1e2558">The last open question is why <inline-formula><mml:math id="M224" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> increases faster with CO<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration under the highest-<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> conditions. The increase in <inline-formula><mml:math id="M227" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> with warming was shown to be mostly driven by an increase in the
efficiency with which cloud condensate is converted into precipitation
(Lutsko and Cronin, 2018). As mentioned in the introduction, the
conversion of cloud condensate into precipitation (or autoconversion of
cloud droplets) becomes significant only when liquid water amount and/or
droplet radii reach a critical threshold (Freud and Rosenfeld, 2012). To
understand the faster <inline-formula><mml:math id="M228" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> increases with CO<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration
under the highest-<inline-formula><mml:math id="M230" 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> conditions, we present the histograms over the
domain and time (during the last 150 d of the simulations based on 3-D
output in 1 h resolution) of liquid cloud droplet mixing ratio
(<inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; Fig. 6) and mean cloud droplet radii (<inline-formula><mml:math id="M232" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>; Fig. 7)
around the height of the maximum in cloud droplet effective radii (1950 m)
and its mean sensitivity to doubling of CO<inline-formula><mml:math id="M233" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration for each
<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:mrow></mml:math></inline-formula> condition.</p>
      <p id="d1e2668">Figure 6 demonstrates that the cut-off of the <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> distribution (the
mixing ratio for which the probability density function starts to decrease
sharply) increases with the CO<inline-formula><mml:math id="M236" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration and decreases with the
aerosol concentration. However, the sensitivity of the relatively large
<inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to CO<inline-formula><mml:math id="M238" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration is significantly larger under high
aerosol concentrations compared to the lower aerosol concentrations (Fig. 6b). The larger relative increase in high <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> promotes the autoconversion
process and hence enhances <inline-formula><mml:math id="M240" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>, more so under high aerosol
concentrations than under low aerosol concentrations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e2732">Probability density functions (PDFs) of the cloud droplet mixing
ratio (<inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) for the different simulations <bold>(a)</bold> and the mean sensitivity
of the <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> PDF to a doubling of the CO<inline-formula><mml:math id="M243" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration based on the
three combinations available for each <inline-formula><mml:math id="M244" 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> condition
(<inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M246" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M247" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M249" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M251" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M252" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M254" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and (<inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M256" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M257" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M259" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>) <bold>(b)</bold>, calculated for the heights around which the cloud droplet effective
radii reach a maximum (1950 m) and using 3-D files output every hour of the
last 150 d of the simulations. Note the logarithmic scales for the <inline-formula><mml:math id="M261" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axes
of <bold>(a)</bold>.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f06.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e2950">Probability density functions (PDFs) of cloud droplet mean radii
(<inline-formula><mml:math id="M262" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>) for the different simulations <bold>(a)</bold> and the mean sensitivity
of the <inline-formula><mml:math id="M263" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> PDF to a doubling of the CO<inline-formula><mml:math id="M264" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration based on
the three combinations available for each <inline-formula><mml:math id="M265" 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> condition
(<inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M267" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M268" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M270" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M272" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M273" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M275" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and (<inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M277" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M278" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math id="M280" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>)
<bold>(b)</bold>, calculated for the heights around which the cloud droplet effective
radii reach a maximum (1950 m) and using 3-D files output every hour of the
last 150 d of the simulations. Note the logarithmic scales for the <inline-formula><mml:math id="M282" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axes
of <bold>(a)</bold>.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15767/2022/acp-22-15767-2022-f07.png"/>

      </fig>

      <p id="d1e3173">Figure 7 demonstrates, in line with expectations, that <inline-formula><mml:math id="M283" 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> has a strong
effect on <inline-formula><mml:math id="M284" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>. In addition, it shows that under all <inline-formula><mml:math id="M285" 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>
conditions, <inline-formula><mml:math id="M286" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> increases with the CO<inline-formula><mml:math id="M287" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration. This
could be explained by the increase in the availability of water vapour (Fig. 2), which, for given <inline-formula><mml:math id="M288" 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> conditions, enables larger diffusional growth
of the droplets. This trend could also be understood from the increase in
<inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> with warming (Fig. 6; Lutsko and Cronin, 2018), which under given
<inline-formula><mml:math id="M290" 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> conditions implies larger <inline-formula><mml:math id="M291" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>. Here again, the highest-<inline-formula><mml:math id="M292" 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> conditions demonstrate the largest sensitivity of <inline-formula><mml:math id="M293" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> to
CO<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, especially on the right-hand side of the
distribution (Fig. 7b). This could be explained by the fact that under these
high-<inline-formula><mml:math id="M295" 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> conditions, the cloud droplet growth is primarily limited by the
availability of water vapour, as a large number of droplets compete for the
available water vapour (Koren et al., 2014; Dagan et al., 2015a; Reutter et
al., 2009). Thus, an increase in the availability of water vapour with
CO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (Fig. 2) under polluted conditions results in a
larger increase in <inline-formula><mml:math id="M297" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> compared with clean conditions. However,
the reasons behind this trend, as well as behind the larger increase in
<inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in high-<inline-formula><mml:math id="M299" 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> simulations, deserve further exploration in the future.
Similarly to the <inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> case, the larger relative increase in the relatively
large droplets promotes the autoconversion process and hence enhances
<inline-formula><mml:math id="M301" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>, more so under high aerosol concentrations than under lower aerosol
concentrations.</p>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Summary and conclusions</title>
      <p id="d1e3401">The role of clouds in climate change is manifested by two pathways: (1) effects of anthropogenic aerosol on clouds and (2) feedback that clouds
exert on the changing climate. These two pathways are usually studied
separately, and even by different scientific communities. In this paper, we
demonstrate that the two pathways are closely linked to each other and
should be examined concurrently.</p>
      <p id="d1e3404">Using long, idealized RCE simulations over a small domain with a slab ocean
model, we demonstrate that the ECS, i.e. the increase in surface
temperature under equilibrium conditions due to doubling of the CO<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration, increases with the aerosol concentration. The ECS increase is
explained by a faster increase in precipitation efficiency with warming
under high aerosol concentrations, which represents a more efficient
depletion of the water from the cloud and thus is manifested as an increase
in the cloud feedback parameter. The precipitation efficiency increases
faster under high aerosol concentration due to a higher sensitivity of the
relatively high liquid water mixing ratios and the relatively large mean
droplet sizes to a CO<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration increase. We note that the
increase in the total (short wave plus long wave) cloud feedback parameter
with the increase in precipitation efficiency is a result of a stronger
short-wave effect (Li et al., 2019) than a long-wave effect (Lindzen et al.,
2001) in the simulations presented here. Future work should examine the
robustness of this trend in different models and with different
microphysical and radiative schemes. Moreover, the response of precipitation
to changes in aerosol concentration might be microphysical-representation-dependent (White et al., 2017) and hence should be examined in the future
under different microphysical schemes (conceivably in a multi-model
intercomparison project focusing on aerosol effect on RCE simulations).</p>
      <p id="d1e3425">The results presented here are based on idealized simulations over a small
domain. Under more realistic conditions, other processes, not included here,
that could affect the precipitation efficiency and hence the general trend
will be introduced. In particular, convective self-aggregation could be of
interest as, while it is inhibited in the small domain used here, it was
shown to affect precipitation efficiency (Lutsko et al., 2021) and to be
affected by aerosols (Nishant et al., 2019). Other processes that should be
accounted for in future research include the presence of large-scale
circulation and direct aerosol radiative effects (Dagan et al., 2019;
Dingley et al., 2021). In addition, the results presented here suggest that
the sensitivity of ECS to aerosol loading might not be linear (Table 1).
Hence, the dynamical aerosol range present at different geographical
locations would affect the total ECS trend.</p>
      <p id="d1e3428">The results presented here suggest a possible connection between cloud
feedback and aerosol–cloud interactions. The regulation of aerosol emissions
is known to be more effective than the effort to reduce greenhouse gas
emissions. This, together with the short lifetime of aerosols in the
atmosphere, has resulted in a reduction in the value of the global-mean
aerosol effective radiative forcing in recent years (Quaas et al., 2022). If
the conclusions of this paper hold under higher levels of complexity (e.g.
large-scale circulation, convective self-aggregation, etc.) this might mean
that the reduction in global aerosol emissions could lead to a reduction in
ECS, which could compensate, at least partially, for the reduction in the
negative forcing induced by aerosols (Quaas et al., 2022; Bellouin et al.,
2019), thus providing yet additional motivation for reducing aerosol
emissions globally.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e3436">SAM is publicly available at <uri>http://rossby.msrc.sunysb.edu/~marat/SAM/</uri> (Khairoutdinov, 2022).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e3445">The data presented in this study are publicly available at
<ext-link xlink:href="https://doi.org/10.5281/zenodo.7306706" ext-link-type="DOI">10.5281/zenodo.7306706</ext-link> (Dagan, 2022).</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3454">The author has declared that there are no competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e3460">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3466">This research has been supported by the Israel Science Foundation (grant no. 1419/21).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3472">This paper was edited by Anne Perring and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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