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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-16-10063-2016</article-id><title-group><article-title>Effects of aerosol–radiation interaction on precipitation during
biomass-burning season in East China</article-title>
      </title-group><?xmltex \runningtitle{Aerosol--radiation interaction of biomass burning}?><?xmltex \runningauthor{X.~Huang et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Huang</surname><given-names>Xin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0922-5014</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Ding</surname><given-names>Aijun</given-names></name>
          <email>dingaj@nju.edu.cn</email>
        <ext-link>https://orcid.org/0000-0003-4481-5386</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Liu</surname><given-names>Lixia</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Liu</surname><given-names>Qiang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Ding</surname><given-names>Ke</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Niu</surname><given-names>Xiaorui</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Nie</surname><given-names>Wei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Xu</surname><given-names>Zheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Chi</surname><given-names>Xuguang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Wang</surname><given-names>Minghuai</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9179-228X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Sun</surname><given-names>Jianning</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7683-1674</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Guo</surname><given-names>Weidong</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0299-6393</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Fu</surname><given-names>Congbin</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Joint International Research Laboratory of Atmospheric and Earth
System Sciences, Nanjing University,<?xmltex \hack{\newline}?> Nanjing, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institute for Climate and Global Change Research &amp; School of
Atmospheric Sciences, <?xmltex \hack{\newline}?>Nanjing University, Nanjing, 210023, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Collaborative Innovation Center of Climate Change, Jiangsu province,
China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Aijun Ding (dingaj@nju.edu.cn)</corresp></author-notes><pub-date><day>9</day><month>August</month><year>2016</year></pub-date>
      
      <volume>16</volume>
      <issue>15</issue>
      <fpage>10063</fpage><lpage>10082</lpage>
      <history>
        <date date-type="received"><day>30</day><month>March</month><year>2016</year></date>
           <date date-type="rev-request"><day>6</day><month>April</month><year>2016</year></date>
           <date date-type="rev-recd"><day>15</day><month>July</month><year>2016</year></date>
           <date date-type="accepted"><day>19</day><month>July</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</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>
    <p>Biomass burning is a main source for primary carbonaceous particles in the
atmosphere and acts as a crucial factor that alters Earth's energy budget and
balance. It is also an important factor influencing air quality, regional
climate and sustainability in the domain of Pan-Eurasian Experiment (PEEX).
During the exceptionally intense agricultural fire season in mid-June 2012,
accompanied by rapidly deteriorating air quality, a series of
meteorological anomalies was observed, including a large decline in
near-surface air temperature, spatial shifts and changes in precipitation in
Jiangsu province of East China. To explore the underlying processes that link
air pollution to weather modification, we conducted a numerical study with
parallel simulations using the fully coupled meteorology–chemistry model
WRF-Chem with a high-resolution emission inventory for agricultural fires.
Evaluation of the modeling results with available ground-based measurements
and satellite retrievals showed that this model was able to reproduce the
magnitude and spatial variations of fire-induced air pollution. During the
biomass-burning event in mid-June 2012, intensive emission of absorbing
aerosols trapped a considerable part of solar radiation in the atmosphere and
reduced incident radiation reaching the surface on a regional scale, followed
by lowered surface sensible and latent heat fluxes. The perturbed energy
balance and re-allocation gave rise to substantial adjustments in vertical
temperature stratification, namely surface cooling and upper-air heating.
Furthermore, an intimate link between temperature profile and small-scale
processes like turbulent mixing and entrainment led to distinct changes in
precipitation. On the one hand, by stabilizing the atmosphere below and reducing
the surface flux, black carbon-laden plumes tended to dissipate daytime cloud
and suppress the convective precipitation over Nanjing. On the other hand,
heating aloft increased upper-level convective activity and then favored
convergence carrying in moist air, thereby enhancing the nocturnal
precipitation in the downwind areas of the biomass-burning
plumes.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Biomass burning, defined as open or quasi-open combustion of non-fossilized
vegetative or organic fuel, is widely used by humans to manage and transform
land cover for many purposes and has been identified as one of the most
important disturbance agents in world's terrestrial ecosystems (Fearnside,
2000). It is a major source of many trace gases and particulate matters on a
regional and even a global scale (Andreae and Merlet, 2001; van der Werf et al.,
2006; Ito et al., 2007), contributing significantly to the budgets of trace
gases, greenhouse gases and atmospheric aerosols (Langenfelds et al., 2002).
For instance, biomass burning is estimated to be responsible for almost half
of global carbon monoxide (CO) emission and more than one third of total
black carbon (BC) emission (Bergamaschi et al., 2000; Bond et al., 2013).
With tremendous and intensive emission of atmospheric pollutants, it has
been recognized as one of the culprits of regional air pollution (Wiedinmyer
et al., 2006; Ryu et al., 2007) and an important disturber of biogeochemical
cycles, especially for those of carbon and nitrogen (Crutzen and Andreae,
1990; Kuhlbusch, 1998). In the Eurasian continent, i.e., the main domain of the
Pan-Eurasian Experiment (PEEX) (Kulmala et al., 2015), biomass burning is a
very important source influencing air quality, regional climate change and
sustainability (Chi et al., 2013; Ding et al., 2013a, b; Lappalainen et al.,
2016). In East China, the impact of biomass burning to air quality and
regional climate change is particularly interesting because of the mixing of
biomass-burning plumes with pollutant from fossil fuel combustion sources
(Ding et al., 2013a; Nie et al., 2015; Xie et al., 2015; Lappalainen et al.,
2016).</p>
      <p>Biomass burning, including forest fires, savanna fires, peat burning and
crop residue burning in field, generally features a high emission rate of
light-absorbing carbonaceous aerosols (Reid et al., 1998; Schwarz et al.,
2008). The most important one is BC, which is intensively emitted during
biomass-burning events due to incomplete combustions (Reid et al., 2005;
Akagi et al., 2011). As the dominant absorber of solar radiation in the
atmosphere, BC warms the Earth–atmospheric system and alters the
partitioning of energy between the ground surface and the atmosphere,
thereby modifying atmospheric thermodynamic structures and modulating
hydrological cycles (Krishnan and Ramanathan, 2002; Ramanathan et al., 2005;
Ding et al., 2016). These modifications induced by biomass burning have been
detected in many regions, especially for those during forest fires. Surface
temperature decline was extensively observed during forest fires in North
America, Asia and Africa (Robock, 1988, 1991; Procopio et al., 2004; Kolusu
et al., 2015). The dimming around ground surface and heating in the
upper atmosphere, especially in the upper boundary layer, could cause the
suppression of daytime mixing height and result in an enhancement of surface
air pollution through aerosol–boundary-layer–radiation feedbacks (Ding et
al., 2013a, 2016). This effect was named as the “dome effect”
of BC by Ding et al. (2016). By cooling the surface and stabilizing the
atmosphere, intense forest fires may lead to the inhibition of cloud
formation (Andreae et al., 2004; Koren et al., 2004; Feingold et al., 2005),
suppression in precipitation (Rosenfeld, 1999; Sakaeda et al., 2011) and
even temporal shift in onset of monsoon (Liu et al., 2005; Lau et al., 2006;
Zhang et al., 2009). In short, BC has been demonstrated to cause a
significant perturbation in the radiative energy balance and has even led to
regional and global climate change (Penner et al., 1992; Menon et al., 2002;
Ramanathan and Carmichael, 2008).</p>
      <p>Although forest and savanna fires are much less notable in China compared
with tropical America, Africa and Southeast Asia (van der Werf et al.,
2006), it is noteworthy that China is a large country with the world's
top-ranked agricultural production, which is inevitably accompanied by a
tremendous amount of crop residue. Field burning of crop residue is a common
and widespread management practice in China during post-harvest periods for
the purpose of clearing farmland and providing short-lived ash fertilization
for the crop rotation (Gao et al., 2002). It is estimated that about 120 Tg
of crop residue is burned in fields across China every year, far higher than
that burned in forest fires and savanna fires (Yan et al., 2006). Previous
studies have documented that field burning of crop residue led to
deterioration in regional air quality during harvest season (Yang et al.,
2008; Huang et al., 2012b; Li et al., 2014). What is worse, this kind of
pollution occurs periodically in East China, particularly during the harvest
period of wheat in June (Fig. 1). However, studies regarding its effects
on meteorology and climate are still limited. Ding et al. (2013a) reported
that temperature and precipitation were dramatically modified during the
harvest season in 2012 according to ground-based measurements at a regional
background station SORPES in the Yangtze River Delta region in East China
(Ding et al., 2013b). However, there is a lack of a comprehensive picture of
how or through which processes the biomass-burning plumes influenced the air
temperature and precipitation and on what scale the aerosol–weather
interactions happened during this case.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p><bold>(a)</bold> Distribution of 13-year total fire detections by
MOD14A1 during 2003–2015 in the WRF-Chem coarse domain. The black rectangle
represents the inner domain. The top left corner gives a map showing the
geographic location of the model domain. <bold>(b)</bold> Thirteen-year time series of
monthly fire detections in the model coarse domain based on MOD14A1
retrievals.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f01.png"/>

      </fig>

      <p>Here we conducted numerical simulations for the biomass-burning event in
East China during mid-June 2012 based on the online coupled
meteorology–chemistry model WRF-Chem (the Weather Research and Forecasting
model coupled with Chemistry) combined with multiple ground-based
measurements and remote-sensing retrievals. The rest of this paper is
structured as follows: Sect. 2 describes the development of an emission
inventory for field burning of crop residues and how the numerical
simulations are configured and designed; in Sect. 3 we validate the
modeling results using available measurements and then analyze the
perturbations in energy budget and temperature adjustments induced by crop
residue burning; finally, three regions with distinct precipitation changes,
located near or downwind from the burning sites, are selected to be discussed in
detail. Conclusions are drawn in Sect. 4.</p>
</sec>
<sec id="Ch1.S2">
  <title>Data and methodology</title>
<sec id="Ch1.S2.SS1">
  <title>Emission inventory</title>
      <p>Modeling aerosols' radiative effects during this biomass-burning event
first requires accurate quantification and meticulous characterization of
emission from field burning of crop residue. Here, emission intensities of
trace gases and particulate matters, specifically including carbon dioxide
(CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, CO, methane (CH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, non-methane organic compounds (NMOCs),
nitrogen oxides (NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>), ammonia (NH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, sulfur dioxide (SO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, BC,
organic carbon (OC) and particulate matter (PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2.5</mml:mn></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> are
particles with aerodynamic diameter less than 2.5 and 10 microns
respectively), were estimated based on a bottom-up method. According to the
farming season (available at <uri>http://zzys.agri.gov.cn</uri>) and province-level statistics
on crop cultivation (NBSC, 2013), we can deduce that the intensive
agricultural fires in June were mainly related to wheat straw burning as a
consequence of the extensively spreading cultivation mode of “winter
wheat–summer corn/rice” in East China. Burned biomass at province-level was
calculated based on statistical data of crop productions,
residue-to-production ratios and percentages of crop residues burned in the
field. Emissions of various pollutants were derived from the product of
burned mass and experiment results on crop-specific combustion efficiencies
and pollutant-specific emission factors. The detailed methods and involved
datasets are described in our previous work (Huang et al., 2012b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p><bold>(a)</bold> Satellite fire detections in June 2012 and backward
trajectories for NJ (Nanjing), XZ (Xuzhou) and SY (Sheyang). <bold>(b)</bold> Temporal
variations of daily fire occurrences. BC emission rates from <bold>(c)</bold> agricultural
fires and <bold>(d)</bold> anthropogenic activities on 9 June. Note that the
backward trajectories were calculated for an altitude of 2 km over NJ, XZ
and SY from 14:00 LT and 18:00 LT on 10 June and 01:00 LT on 11 June (Draxler and Rolph, 2003). Anhui and
Jiangsu provinces are labeled in gray in Fig. 2a.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f02.png"/>

        </fig>

      <p>To determine the locations and time of crop residue fires, MODIS (Moderate
Resolution Imaging Spectroradiometer, available at https://ladsweb.nascom.nasa.gov/data/) Thermal Anomalies/Fire Daily L3 Global
product (MOD/MYD14A1) combined with burned area product (MCD45A1) were
introduced for the purpose of emission spatiotemporal allocations (Giglio et
al., 2003; Boschetti et al., 2009). MOD/MYD14A1 provides fire identification
by examining the brightness temperature relative to neighboring pixels.
MCD45A1 was also incorporated in this work because its bidirectional
reflectance model-based change detection approach has been proved to be
capable of presenting a more accurate mapping of smaller fragments of burn
scars (Roy and Boschetti, 2009). The Global Land Cover (GLC) product with a
spatial resolution of 1 km was used in this study to identify the burning of
different biomass. Only fire detections that occurred on farmland, i.e.,
land cover classes defined as “farm” and “mosaic of cropping”, were
identified as field burning of crop residue. Emission at province level
estimated using the aforementioned method was then allocated equally to
each fire spot.</p>
      <p>The fire emission estimation developed in this work was compared with the
FINN fire emission dataset. Spatially, these two emission inventories
generally were consistent with each other because the locations for the
fires in both inventories are based on MODIS Thermal Anomalies product
(Fig. S1 in the Supplement). Some inconsistencies, such as the density of fire in central
Jiangsu, are attributed to the different land cover dataset applied for the
identification of underlying biomass type. FINN fire emission estimation
used MODIS Collection 5 Land Cover Type data (Wiedinmyer et al., 2011),
while we employed Global Land Cover data. This inventory differs slightly
from FINN estimation in magnitude. Taking CO emission in the inner model
domain for instance, we estimate that 4.5 Tg CO was emitted while FINN gives
the value of 7.5 Tg during the first half of June 2012. It might be
attributed to different methods to estimate burned biomass. FINN used MODIS
Vegetation Continuous Fields to assign the burned mass. The fuel loading of
farmland was assumed to be 0.5 kg m<inline-formula><mml:math 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> (Wiedinmyer et al., 2006).
However, in China, crop straw is used in multiple ways that differ
regionally, like biofuel, biogas production and animal feed supply, which is
highly dependent on crop species. We estimated the emission using a
“bottom-up” method by fully considering crop yields, crop-specific straw
usage and combustion efficiency.</p>
      <p>During this agricultural fire event, the spatial pattern of fire detections
in Fig. 2a indicates that open burning of straw mostly concentrated in
northern parts of Anhui and Jiangsu province and got extremely severe on 9
and 13 June, as displayed in Fig. 2b. Burning of crop residues dominated
local emissions of atmospheric pollutants when compared with corresponding
anthropogenic emissions. Taking BC for instance (Fig. 2c and d), emission
rate from field burning of crop residues far outweighed that from industry,
power plant, residential activity and transportation combined (Li et al.,
2015).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Numerical simulation</title>
      <p>The numerical simulations in this study were conducted using WRF-Chem
version 3.6.1, which is an online-coupled chemical transport model
considering multiple physical and chemical processes, including emission and
deposition of pollutants, advection and diffusion, gaseous and aqueous
chemical transformation, aerosol chemistry and dynamics (Grell  et al.,
2011). The model has been widely utilized to investigate
aerosol–radiation–cloud interactions and aerosol–boundary-layer feedback
(Grell  et al., 2011; Zhao et al., 2013; Fan et al., 2015; Huang et
al., 2015; Ding et al., 2016; Gao et al., 2016). In the present work, we
adopted two nested model domains (Fig. 1a). The coarse domain is centered at 115.0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E,
33.0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N  with a grid resolution of
20 km covered East China and its surrounding areas. The fine resolution of 4 km for the inner one allowed better
characterization of small-scale physical processes, especially those linked
to convective motions, cloud formation and rainfall onset. There were 31
vertical layers from the ground level to the top pressure of 50 hPa, 20 of
which were placed below 4 km to achieve finer vertical resolution within the
boundary layer. The initial and boundary conditions of meteorological fields
were updated from the 6 h NCEP (National Centers for Environmental
Prediction) global final analysis (FNL) data with a 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
spatial resolution. To investigate the aerosols' radiative
effects on 10 June 2012 when the precipitation was substantially modified,
the simulations were conducted for the time period from 20 May to 15 June.
The meteorological initializing date for 10 June was 12:00 UTC on 9 June.
Each run covered 60 h and the last 48 h modeling results were kept for further analysis.
The chemical outputs from the preceding run were used as the initial
conditions for the following run. The first 20 days were regarded as the
model spin-up period for atmospheric chemistry, so as to better characterize
aerosol distributions and minimize the influences of initial conditions and
allow the model to reach a state of statistical equilibrium under the
applied forcing (Berge et al., 2001; Lo et al., 2008).</p>
      <p>Key parameterization options for the WRF-Chem modeling were the Noah land
surface scheme to describe the land–atmosphere interactions (Ek et al.,
2003), the YSU boundary layer scheme (Hong, 2010) and the RRTMG short- and
longwave radiation scheme (Mlawer et al., 1997). The Lin microphysics
scheme that accounts for six forms of hydrometer (Lin et al., 1983) together
with the Grell cumulus parameterization was applied to reproduce the cloud
and precipitation processes (Grell   and Devenyi, 2002) for the coarse
domain. Cumulus parameterization was switched off for the inner domain. For
the numerical representation of atmospheric chemistry, we used the CBMZ
(Carbon Bond Mechanism version Z) photochemical mechanism combined with
MOSAIC (Model for Simulating Aerosol Interactions and Chemistry) aerosol
model (Zaveri and Peters, 1999; Zaveri et al., 2008). Aerosols were assumed
to be spherical particles. The size distribution was divided into four
discrete size bins defined by their lower and upper dry particle diameters
(0.039–0.156, 0.156–0.625, 0.625–2.5 and 2.5–10.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m). Aerosols in
each size bin were assumed to be internally mixed and their optical
properties, including extinction coefficient, single-scattering albedo (SSA)
and asymmetry factor, were computed based on Mie theory (Fast et al., 2006)
using volume averaged refractive indices (Barnard et al., 2010). Similar
model configurations and settings have achieved good performance in our
previous simulations over East China (Huang et al., 2015; Ding et
al., 2016). Detailed configurations and domain settings are listed in Table 1.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><caption><p>WRF-Chem modeling configuration options and settings.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.98}[.98]?><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry namest="col1" nameend="col3" align="center">Domain setting </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Domain 1</oasis:entry>  
         <oasis:entry colname="col3">Domain 2</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Horizontal grid</oasis:entry>  
         <oasis:entry colname="col2">130 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 130</oasis:entry>  
         <oasis:entry colname="col3">160 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 160</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Grid spacing</oasis:entry>  
         <oasis:entry colname="col2">20 km</oasis:entry>  
         <oasis:entry colname="col3">4 km</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Vertical layers</oasis:entry>  
         <oasis:entry colname="col2">31</oasis:entry>  
         <oasis:entry colname="col3">31</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry namest="col1" nameend="col3" align="center">Configuration options </oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Longwave radiation</oasis:entry>  
         <oasis:entry colname="col2">RRTMG</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Shortwave radiation</oasis:entry>  
         <oasis:entry colname="col2">RRTMG</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Land surface</oasis:entry>  
         <oasis:entry colname="col2">Noah</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Boundary layer</oasis:entry>  
         <oasis:entry colname="col2">YSU</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Microphysics</oasis:entry>  
         <oasis:entry colname="col2">Lin et al.</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Cumulus parameterization</oasis:entry>  
         <oasis:entry colname="col2">Grell–Deveny</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">(only for domain 1)</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Photolysis</oasis:entry>  
         <oasis:entry colname="col2">Fast-J</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Gas-phase chemistry</oasis:entry>  
         <oasis:entry colname="col2">CBMZ</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Aerosol scheme</oasis:entry>  
         <oasis:entry colname="col2">MOSAIC</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p>Both natural and anthropogenic emissions were included for the regional
WRF-Chem modeling in the present work. Typical anthropogenic emissions were
obtained from the Multi-resolution Emission Inventory for China (MEIC)
database (Li et al., 2015), in which emissions sources were classified into
five main sectors: power plants, residential combustion, industrial
processes, on-road mobile sources and agricultural activities. This
database covers most of anthropogenic pollutants, such as SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, CO,
volatile organic compounds (VOCs), PM, BC and OC. NH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> emission over
China was derived from Huang et al. (2012a). VOCs emitted from typical
anthropogenic activities and aforementioned crop residue burning were
speciated into model-ready lumped species using profiles for Carbon Bond
Mechanism (Hsu et al., 2006). The biogenic VOC and NO emissions were
calculated online by using the Model of Emissions of Gases and Aerosols from
Nature (MEGAN) that embedded in WRF-Chem (Guenther et al., 2006). More than
20 biogenic species, including isoprene, monoterpenes (e.g., <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene) and sesquiterpenes, were considered and then
involved in the photochemistry calculation. In China, crop residues are
usually burned in piles, which are characterized by short-lived and
small-scale smoldering. Consequently, the plume rise of biomass-burning
plumes was not considered in this study, and the straw fire emission was
placed in the lowest two levels from the surface to around 50 m in this
simulation.</p>
      <p>Previous studies have shown that, under highly polluted conditions, the aerosol–radiation interaction
(ARI)
dominated over the aerosol–cloud interaction (ACI) that is related to
aerosols' ability to act as cloud condensation nuclei (CCN) (e.g., Rosenfeld et al., 2008; Fan et al.,
2015). We also conducted another numerical experiment which included both
ACI and ARI. The ACI-induced radiative perturbations were much less notable
than those caused by ARI both at the surface and in the atmosphere (Fig. S2), implying the dominant role of ARI during this kind of synoptic-scale fire event. Since that
the focus of this study is on ARI and ACI's effect was not that significant,
the prognosed aerosol was disabled to act as CCN
or ice nuclei in the simulations and therefore the effects from ACI
were not accounted for in the following analysis. Accordingly, wet
scavenging of aerosol was disabled too. In order to disentangle aerosols'
role in radiative transfer and subsequent effects on cloud and precipitation
during this biomass-burning event in  mid-June of 2012, we designed three
parallel numerical experiments. Domain settings and model configurations for
these simulations were exactly the same as mentioned before. The control (CTL)
experiment did not include aerosol's effects on either longwave or
shortwave radiation transfer. On the contrary, the other two took account of
aerosols' perturbations on radiation transfer: ARI-A with anthropogenic
emissions (anthropogenic activities refer to power generation,
transportation, industrial and residential activities hereafter) and ARI-AB
that included both anthropogenic activities and biomass-burning emissions.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results and discussions</title>
<sec id="Ch1.S3.SS1">
  <title>Fire-induced pollution and observed anomalies in meteorology</title>
      <p>As demonstrated by existing studies (Andreae et al., 1988; Huang et al.,
2012c; Ding et al., 2013a), air quality  dramatically deteriorated and
the visibility was impeded during biomass-burning events. We compare the
simulated daily averaged PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> concentration with the corresponding
measurements derived from Air Pollution Index (API, available at <uri>http://datacenter.mep.gov.cn/</uri>) in Fig. 3 (if not
mentioned specially, the simulation refers to ARI-AB experiment hereafter).
Both observations and simulations manifested the fact that intensive
agricultural fires led to the severe pollution in mid-June. Since 9 June,
when the detected fire spots became intense and extensive, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula>
concentrations in northern Anhui and northwestern Jiangsu province began to
increase, especially for those regions near the fire location. For instance,
the observed daily mean PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> concentrations reached up to around 250 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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>
at Fuyang (FY) and Xuzhou (XZ) and even exceeded 400 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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>
at Bengbu (BB) on 9 June (the locations of cities mentioned in
this article are labeled in Fig. 2). Although the simulated temporal
variations agree with observations, model-predicted PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> concentrations at
FY and BB were 196 and 168 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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. The underestimation might be due to the fact that rapid formation of
secondary aerosol like sulfate and secondary organic matters is not so well
described in current atmospheric chemical transport models (Capes et al.,
2008; Xie et al., 2015). XZ and BB suffered from the second-round fire smoke
2 days later, with a maximum daily mean concentration of 548 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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>
observed at BB. Figure 4 illustrates the satellite-retrieved
660 nm aerosol optical depth (AOD) and SSA from MODIS Aerosol Product
MOD04_L2 (daily level 2 data produced at the spatial
resolution of 10 km, Collection 6) around 11:00 local time (LT) on 9 June
when the first round of extensive fire pollution broke out. Their
comparisons with ARI-AB modeled spatial distributions of PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2.5</mml:mn></mml:msub></mml:math></inline-formula> and BC
column-integrated mass loadings further confirm model's ability to
reproduce
atmospheric pollution for this event. The AOD observation shows that high
aerosol loadings were concentrating in northeast Anhui and the north-central
Jiangsu, shaping a belt of pollution from the fire sites to the downwind
areas. A similar pattern was also simulated by the model. The PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2.5</mml:mn></mml:msub></mml:math></inline-formula>
mass loading was found to exceed 200 mg m<inline-formula><mml:math 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> near BB, NJ and most parts
of central Jiangsu. This strap-shaped pollution was particularly obvious in
terms of BC column concentrations, which was also consistent with a
relatively lower SSA along BB, Yangzhou (YZ) and Taizhou (TZ). While solely
including anthropogenic emissions, ARI-A experiment failed to represent the
spatial pattern of high AOD in the northern Anhui and Jiangsu and the low
SSA value near BB (Fig. 4a, d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Measurements of 24 h averaged PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> concentrations and
corresponding PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> simulations at <bold>(a)</bold> FY (Fuyang), <bold>(b)</bold> BB (Bengbu),
<bold>(c)</bold> XZ (Xuzhou) and <bold>(d)</bold> HF (Hefei).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Spatial distributions of simulated PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2.5</mml:mn></mml:msub></mml:math></inline-formula> mass loading by
<bold>(a)</bold> ARI-A and <bold>(b)</bold> ARI-AB experiments and <bold>(c)</bold> satellite-derived 660 nm AOD at
11:00 LT, 9 June. Simulated BC mass loading by <bold>(d)</bold> ARI-A and <bold>(e)</bold> ARI-AB
experiments and <bold>(f)</bold> satellite-derived SSA at that time.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f04.png"/>

        </fig>

      <p>Along with the severe air pollution and poor visibility, anomalies in
meteorology occurred on 9–10 June. Ding et al. (2013a) found that, during
these 2 days, a sharp decline existed in the observed air temperature in
NJ and YZ compared with weather forecast results and NCEP FNL data, but the
simulations and observations showed a good agreement when the heavy air
pollution was not present before 9 June and after 10 June. At YZ the temperature difference
was as high as 5.9 and 9.2 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C on 9 and 10 June respectively.
Simultaneously, measured solar radiation intensity and sensible heat flux
showed very low values on 10 June in comparison with non-episode days.
Moreover, local meteorological agency forecasted a convective rainfall to
occur in NJ and surrounding areas in the afternoon of 10 June, with the
rainfall center passing by NJ around 14:00 LT. However, this forecasted
rainfall never happened that day.</p>
      <p>On the basis of ground-based measurements, vertical sounding data,
remote-sensing images and their comparisons with numerical simulations, we
found that agricultural fires worsen regional air quality to a large extent
and caused a series of anomalies in temperature and precipitation in the
mid-June of 2012. How the biomass-burning plumes influenced the air
temperature and precipitation will be the main issue to be addressed in the
following discussions.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Perturbations in energy budget and temperature responses</title>
      <p>To better understand aerosols' role in the energy re-allocation on 10 June
when precipitation was evidently modified, radiative forcing in the
atmosphere and at the ground surface was estimated by differentiating the
CTL, ARI-A and ARI-AB simulations (Fig. 5). At the surface, daily mean
incident shortwave radiation was weakened by 45.5 W m<inline-formula><mml:math 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> (averaged over
the inner domain) as the extinction of aerosol was quite large with a
satellite-observed 660 nm AOD exceeding 2.0 (Fig. 4b). Meanwhile, about
60.4 W m<inline-formula><mml:math 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> shortwave energy was blocked in the atmosphere over the inner
domain due to the fact that absorbing aerosols were accumulated on that day.
A positive domain-averaged radiative forcing of <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>14.9 W m<inline-formula><mml:math 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> was
simulated at the top of the atmosphere on 10 June. Comparatively,
radiative perturbations caused by agricultural fires (ARI-AB minus ARI-A)
were more substantial than those due to anthropogenic emissions (ARI-A minus
CTL) in magnitude, particularly in the atmosphere, as presented in Fig. 5.
Spatially, radiative effects due to anthropogenic activities concentrated in
the economically developed Yangtze River Delta region while agricultural
fires exerted significant impact on radiation balance in northern and
central Jiangsu and the northern part of Anhui. Table 2 compares the radiative
perturbations caused by anthropogenic activities and biomass-burning
emissions over three regions with distinct precipitation changes (marked in
Fig. 8). As shown, both of them tended to heat the atmosphere and cool the
ground surface. Fire plumes dominated the radiative effect in terms of
atmospheric warming. Radiation measurements collected at Hefei (HF) and
sensible and latent heat flux recorded at Lishui (in South Nanjing) are
compared with the diurnal variations of corresponding simulations in Fig. 6,
which supports that significant radiative perturbations took place at NJ
and HF. Substantially weakened daytime solar irradiance was observed on 10 June, when the peak value of downwelling shortwave radiation was 618.3 W m<inline-formula><mml:math 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>
at HF and was only 309.7 W m<inline-formula><mml:math 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> at NJ. Taking aerosol's effect
on radiation into account tended to predict lower downwards solar radiation,
which was closer to observation for both cities. Reduction in shortwave
energy hitting the surface in turn decreased outgoing heat fluxes and
therefore simulated sensible and latent heat fluxes at 12:00 LT on 10 June
in ARI-AB experiment decreased by 89.3 and 76.1 W m<inline-formula><mml:math 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>, respectively,
compared to the CTL experiment.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Radiative forcing <bold>(a)</bold> at the surface and <bold>(b)</bold> in the atmosphere due
to anthropogenic aerosols on 10 June. Radiative forcing of aerosol <bold>(c)</bold> at
the surface and <bold>(d)</bold> in the atmosphere due to biomass-burning emissions on 10 June. Aerosol-induced changes in air temperature and wind fields <bold>(e)</bold> near
the surface and <bold>(f)</bold> at the altitude of 2 km.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f05.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p>Radiative perturbations at the surface (SUR) and in the atmosphere
(ATM) caused by anthropogenic activities and agricultural fires for three
zones with distinct precipitation changes.</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="center"/>
     <oasis:colspec colnum="3" colname="col3" align="center" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:colspec colnum="5" colname="col5" align="center"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" namest="col2" nameend="col3" colsep="1">SUR </oasis:entry>  
         <oasis:entry rowsep="1" namest="col4" nameend="col5">ATM </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Anthropogenic activities</oasis:entry>  
         <oasis:entry colname="col3">Agricultural   fires</oasis:entry>  
         <oasis:entry colname="col4">Anthropogenic activities</oasis:entry>  
         <oasis:entry colname="col5">Agricultural   fires</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Zone 1</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>27.3</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35.1</oasis:entry>  
         <oasis:entry colname="col4">36.3</oasis:entry>  
         <oasis:entry colname="col5">41.1</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Zone 2</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33.3</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>41.7</oasis:entry>  
         <oasis:entry colname="col4">31.9</oasis:entry>  
         <oasis:entry colname="col5">45.6</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Zone 3</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23.8</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>14.8</oasis:entry>  
         <oasis:entry colname="col4">27.7</oasis:entry>  
         <oasis:entry colname="col5">21.1</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>Overall, the magnitude of the radiative forcing on 10 June was comparable in
northern Anhui and central Jiangsu, differing from the distribution pattern
of fire-induced air pollution that remarkably concentrated in northern
Anhui. As revealed in our previous estimation, among all components of the
ambient aerosols, BC is the most important disturber of shortwave radiation
transfer at the surface and in the atmosphere as well (Huang et al., 2015;
Ding et al., 2016). Although fire emission mostly concentrated in the
northern Anhui and resulted in a high BC concentration of 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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>
there, high-altitude BC was spread much more broadly. At an altitude of 2 km,
BC concentration around 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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> stretched from northern Anhui
to central Jiangsu (Fig. S3). Such distinct distributions between two
layers were partly attributed to the stagnant condition near the surface and
stronger horizontal transport in the upper level. It is emphasized that
upper-level BC has higher absorbing efficiency (Ding et al., 2016). That is
why the distributions of both positive radiative forcing in the atmosphere
and negative forcing at the surface were generally consistent with BC's spatial
pattern in the upper air.</p>
      <p>The perturbations in the energy budget and the following re-allocation gave
rise to substantial modulation in vertical stratification of air
temperature. In comparison with the CTL experiment, ARI-AB experiment predicted
an obvious decline in near-surface temperature by considering the effects of
aerosol–radiation interaction. Hourly observed 2 m air temperature was
compared with corresponding simulations by two experiments during the time
period from 8 to 15 June. Model-performance statistics including mean bias, mean error and root mean square error are presented in
Table 3. As shown, CTL simulation had a systematic positive bias in 2 m
temperature and ARI-AB predicted lower temperature for both areas near fire
locations (BB and XZ) and downwind regions (NJ and SY). The decreases in
temperature were pronounced in BB and XZ with a large difference of
approximately 1.2 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, which notably narrowed the gaps with
observations. On 10 June when the fire-induced pollution became intensive,
the magnitude of surface cooling was remarkably high near the fire sites.
Temperature response in Fig. 5e support this cooling effect. For instance,
compared to CTL, simulated near-surface temperature by ARI-A and ARI-AB
experiment at XZ was cooled by almost 1.2 and 8.0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C at 20:00 LT
on 10 June (Fig. 7b). In addition to the cooling tendency of near-surface
temperature, aerosols' radiative effects also increased air temperature at a
higher altitude, which were more apparent over the downwind areas (Fig. 5f).
According to the comparisons between simulated temperature profiles by
the three parallel experiments in Fig. 7, the warming of air temperature
was particularly evident around an altitude of 2 km at SY with a maximum of
3.0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and the biomass-burning aerosols played a leading role.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Diurnal variations of simulated and observed downwelling
shortwave radiation at <bold>(a)</bold> HF (Hefei) and <bold>(b)</bold> NJ (Nanjing) on 9–10 June.
Comparisons of  <bold>(c)</bold> simulated sensible and <bold>(d)</bold> latent heat fluxes  with the
measurements at NJ. Blue, green and red lines present the CTL, ARI-A and ARI-AB
experiments. Black circles mark the observations.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Comparisons between the observed and modeled air temperature
profiles for <bold>(a)</bold> NJ (Nanjing) at 08:00 LT and <bold>(b)</bold> XZ (Xuzhou) and <bold>(c)</bold> SY
(Sheyang) at 20:00 LT, 10 June. Black circles denote sounding observations.
Blue, green and red solid lines are experiments without (CTL) and with
radiative effects of aerosols from anthropogenic emissions (ARI-A) and
additional fire emissions (ARI-AB) respectively.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p>Modeled precipitation during the period from 00:00 UTC, 10 June,
to 00:00 UTC, 11 June, while excluding and considering radiative effects of
aerosols in <bold>(a)</bold> CTL and <bold>(b)</bold> ARI-AB experiments, corresponding
to
<bold>(c)</bold> TRMM-observed precipitation. Three regions with notable changes in
precipitation are marked in rectangles: Zone 1 (red dashed line), Zone 2
(green dashed line) and Zone 3 (yellow dashed line).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f08.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3"><caption><p>Statistical analyses of the simulated 2 m temperature and the
corresponding observations at four different cities.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.97}[.97]?><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:colspec colnum="5" colname="col5" align="center" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="center"/>
     <oasis:colspec colnum="7" colname="col7" align="center"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" namest="col2" nameend="col3" align="center" colsep="1">MB<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry rowsep="1" namest="col4" nameend="col5" colsep="1">ME<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry rowsep="1" namest="col6" nameend="col7">RMSE<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">CTL</oasis:entry>  
         <oasis:entry colname="col3">ARI-AB</oasis:entry>  
         <oasis:entry colname="col4">CTL</oasis:entry>  
         <oasis:entry colname="col5">ARI-AB</oasis:entry>  
         <oasis:entry colname="col6">CTL</oasis:entry>  
         <oasis:entry colname="col7">ARI-AB</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">NJ</oasis:entry>  
         <oasis:entry colname="col2">0.85</oasis:entry>  
         <oasis:entry colname="col3">0.37</oasis:entry>  
         <oasis:entry colname="col4">1.70</oasis:entry>  
         <oasis:entry colname="col5">1.66</oasis:entry>  
         <oasis:entry colname="col6">2.39</oasis:entry>  
         <oasis:entry colname="col7">2.15</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">BB</oasis:entry>  
         <oasis:entry colname="col2">2.19</oasis:entry>  
         <oasis:entry colname="col3">0.98</oasis:entry>  
         <oasis:entry colname="col4">2.51</oasis:entry>  
         <oasis:entry colname="col5">1.65</oasis:entry>  
         <oasis:entry colname="col6">3.27</oasis:entry>  
         <oasis:entry colname="col7">2.16</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">XZ</oasis:entry>  
         <oasis:entry colname="col2">1.67</oasis:entry>  
         <oasis:entry colname="col3">0.51</oasis:entry>  
         <oasis:entry colname="col4">2.37</oasis:entry>  
         <oasis:entry colname="col5">2.19</oasis:entry>  
         <oasis:entry colname="col6">3.32</oasis:entry>  
         <oasis:entry colname="col7">2.89</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">SY</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.28</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.46</oasis:entry>  
         <oasis:entry colname="col4">1.97</oasis:entry>  
         <oasis:entry colname="col5">1.65</oasis:entry>  
         <oasis:entry colname="col6">2.52</oasis:entry>  
         <oasis:entry colname="col7">2.03</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table><?xmltex \begin{scaleboxenv}{.97}[.97]?><table-wrap-foot><p><?xmltex \hack{\vspace{2mm}}?><inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula> MB, ME and RMSE refer to mean bias, mean error and root-mean-square
error respectively.</p></table-wrap-foot><?xmltex \end{scaleboxenv}?></table-wrap>

      <p>The different temperature responses over the source region of fire emission
and downwind areas could be partially interpreted by the fact that, near the
fire locations, pronounced surface cooling counteracted part of the
atmospheric warming, which would otherwise elevate upper-air temperature,
through vertical mixing; for the downwind area where the surface was
less radiatively cooled, the atmosphere was prone to being warmed. As a
result of surface cooling and atmospheric heating, vertical convective
motions were weakened, triggering perturbations in pressure and wind fields
(Fig. 5e and f). It is obvious that suppressed convection was generally
along with the resultant wind convergence around 2 km and surface
divergence, which may further play a significant role in water vapor
transport, entrainment and also cloud formation.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Effects on cloud and precipitation</title>
      <p>In addition to the attenuation of solar radiation and the modulation in
temperature gradients, precipitation also showed many disparities between
CTL and ARI-AB simulations. The satellite observation from Tropical Rainfall
Measuring Mission (TRMM) Multisatellite Precipitation Analysis product
(3B42), which provides merged-infrared precipitation information at a
0.25 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial resolution and has been demonstrated
to perform well in East China (Simpson et al., 1988; Zhao and Yatagai,
2014), was used to evaluate the simulated precipitation. As demonstrated in
Fig. 8, ARI-AB experiment agrees better with TRMM observations than CTL
experiment in terms of precipitation intensities and also spatial pattern on
10 June. Specifically, CTL and ARI-A simulation suggested a convective rain
in Zone 1 (NJ and its adjacent areas) around 14:00 LT (the locations of zones 1–3 are marked in Fig. 8); however the ARI-AB simulation did not show any
precipitation then, consistent with the TRMM observations. Besides, ARI-AB
displayed enhanced precipitation in northern Jiangsu province. A
precipitation with the intensity of 3 and 5 mm h<inline-formula><mml:math 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> was predicted by ARI-AB
experiment in Zone 2 (XZ and its adjacent areas) and Zone 3 (SY and its
adjacent areas), which, however, never occurred in the CTL and ARI-A experiments.
Concerning temporal variations, 3 h precipitation rates for these three
zones derived from TRMM 3B42 retrievals are plotted in Fig. 9. Compared to
the
CTL and ARI-A experiments, the ARI-AB experiment, which considered radiative
effects of aerosol from both anthropogenic and biomass-burning emissions,
succeeded in capturing the approximate onset time for all the three regions.</p>
<sec id="Ch1.S3.SS3.SSS1">
  <title>Suppressed daytime precipitation</title>
      <p>Over Zone 1, CTL and ARI-A simulations produced a convective rainfall event
in the afternoon that actually did not happen, while ARI-AB simulation with
no precipitation was closer to the observations. According to the energy
budget and radiation flux calculation (Fig. 5), on 10 June more than 6 MJ m<inline-formula><mml:math 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>
solar radiation that was supposed to reach the surface was blocked in
the atmosphere over Zone 1, most of which was caused by biomass-burning
aerosol. The presence of light-absorbing aerosols reduced sensible heat flux
and evapotranspiration at the surface (Fig. 6). Large-eddy simulation for
biomass-burning regions of Brazil deduced that the peak reductions in
sensible and latent heat flux were 60 and 70 W m<inline-formula><mml:math 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> (Feingold et al.,
2005), which are quantitatively similar to those near NJ estimated in this
work. It was shown that reduced surface flux alone was sufficient to explain
the observed cloud dissipation during the biomass-burning event in Brazil.
For this case, this convective rain  disappeared merely by nudging 2 m
temperature in the WRF modeling run by Ding et al. (2013a), highlighting
the importance of surface flux modification in the development of these
convective clouds.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Simulated hourly precipitation while considering (ARI-A experiment
in green dashed lines; ARI-AB experiment in red dashed lines) and excluding
(blue solid lines, CTL) radiative effects of aerosols and their comparisons
with TRMM observations (black circles) for <bold>(a)</bold> Zone 1, <bold>(b)</bold> Zone 2 and
<bold>(c)</bold> Zone 3.</p></caption>
            <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f09.png"/>

          </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F10" specific-use="star"><caption><p><bold>(a)</bold> Temporal evolutions of BC vertical profile and changes in air
temperature (K); <bold>(b)</bold> perturbations in RH (%) and cloud water (g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
over Zone 1. <bold>(c)</bold> Longitude–height cross sections of BC concentrations and
aerosol-induced temperature changes at 14:00 LT, 10 June. <bold>(d)</bold> Same as
<bold>(c)</bold> but for water vapor (g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and wind fields (m s<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Note that the
vertical wind speed was multiplied by a factor of 100. Red and black lines
in <bold>(d)</bold> outline cloud coverage (cloud water mass ratio greater than 10<inline-formula><mml:math 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> g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
in ARI-AB and CTL simulations. In this case, the condensate mass
ratio was less than 10<inline-formula><mml:math 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> g kg<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula> for the whole column in
ARI-AB; thus no red line is presented in Fig. 10d. <bold>(e)</bold> Vertical profile of
zone-averaged potential temperature (PT) and MSE and <bold>(f)</bold> updraft velocity
predicted by CTL (blue), ARI-A (green) and ARI-AB (red) at 14:00 LT. Shadows
in Fig. 10f represent 25–75th percentile range of simulated updraft velocity.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f10.png"/>

          </fig>

      <p>To figure out the role of vertical thermal behaviors in Zone 1, temporal
variations of zone-averaged differences in temperature, relative humidity
(RH) profiles between ARI-AB and CTL experiments are illustrated in
Fig. 10a and b. From 09:00 LT in the morning, a 1 km thick belt with BC-laden
smoke approached Zone 1 and covered  the boundary layer top. The
radiative extinction by the elevated smoke layer led to a cooling effect at
the surface, which reduced the boundary layer height and decreased the air
temperature in the boundary layer. Simultaneously, relatively strong warming
effect between the altitudes of 1–3 km increased the air temperature above
the boundary layer. The cooling at the lower altitude and warming at the
upper altitude made the stability significantly increase, especially near
the top of the boundary layer, which further suppressed the development of
boundary layer. For the perturbations in humidity, the enhanced atmospheric
stability reduced the boundary layer height and hindered the upward
transport of water vapor to a higher altitude, while the heating aloft
decreased RH by increasing the air temperature there. These led to a
resultant decrease of more than 20 % in RH above the boundary layer. A
more stable and shallower boundary layer in ARI-AB experiment had a tendency
to reduce convective mixing and effectively cut off the cloud layer from its
source of moisture, subsequently desiccating the cloud layer, and leading to
substantially weakened vertical motions. Accordingly, ARI-AB simulated
updraft velocity above 1 km was only one-tenth that of CTL experiment in the
afternoon of 10 June, as demonstrated in Fig. 10f. Even though
anthropogenic aerosol also weakened convective motions in ARI-A experiment,
the potential temperature profile was hardly changed and the weakening
effect of convection was not comparable with that caused by biomass-burning
aerosols. Therefore, compared with CTL and ARI-A experiment, much less moist
static energy (MSE) was carried upwards and the excess MSE accumulated in a
shallower boundary layer due to much weaker convection in ARI-AB experiment
(Fig. 10e).</p>
      <p>In addition to Zone 1, this warmed belt was also blanketing a wider range
from 116 to 120<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E at the moment when the CTL-predicted rainfall
started (Fig. 9a shows that the rainfall occurred around 14:00 LT), as
shown in the longitude–height cross sections of temperature difference
between the CTL and ARI-AB experiments in Fig. 10c. In the CTL run, a cumulus cloud
layer appeared above the inversion, capping the boundary layer (Fig. 10d).
However, the absorbing aerosol in ARI-AB run heated the atmosphere aloft and
stabilized the sub-cloud layer. The decrease in specific humidity was
collocated with warmed upper air since that atmospheric heating and surface
cooling weakened vertical convection and further reduced the vertical
transport of water vapor. Lower entrainment rate together with higher
saturation pressure resulted in daytime decoupling and thinning of the cloud
layer all along the longitude from 116 to 120<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. This effect
might be further strengthened by a positive feedback loop as described by
Jacobson (2002), in which cloud loss leads to an increasing opportunity for
BC's light absorption.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F11" specific-use="star"><caption><p><bold>(a)</bold> Temporal evolutions of BC vertical profile and changes in air
temperature (K); <bold>(b)</bold> perturbations in RH (%) and cloud water (g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
over Zone 2. <bold>(c)</bold> Longitude–height cross sections of BC concentrations and
aerosol-induced temperature changes at 18:00 LT, 10 June. <bold>(d)</bold> Same as
<bold>(c)</bold> but for water vapor (g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and wind fields (m s<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Note that the
vertical wind speed was multiplied by a factor of 100. Red and black lines
in <bold>(d)</bold> outline cloud coverage (cloud water mass ratio greater than 10<inline-formula><mml:math 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> g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
in ARI-AB and CTL simulations. <bold>(e)</bold> Vertical profile of
zone-averaged potential temperature (PT) and MSE and <bold>(f)</bold> updraft velocity
predicted by CTL (blue), ARI-A (green) and ARI-AB (red) at 18:00 LT. Shadows
in f represent 25–75th percentile range of simulated updraft velocity.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f11.png"/>

          </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F12" specific-use="star"><caption><p><bold>(a)</bold> Temporal evolutions of BC vertical profile and changes in air
temperature (K); <bold>(b)</bold> perturbations in RH (%) and cloud water (g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
over Zone 3. <bold>(c)</bold> Longitude–height cross sections of BC concentrations and
aerosol-induced temperature changes at 01:00 LT, 11 June. <bold>(d)</bold> Same as <bold>(c)</bold> 
but for water vapor (g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and wind fields (m s<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Note that the
vertical wind speed was multiplied by a factor of 100. Red and black lines
in <bold>(d)</bold> outline cloud coverage (cloud water mass ratio greater than 10<inline-formula><mml:math 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> g kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
in ARI-AB and CTL simulations. In this case, the condensate mass
ratio was less than 10<inline-formula><mml:math 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> g kg<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula> for the whole column in CTL,
thus no black line is presented in Fig.12d. <bold>(e)</bold> Vertical profile of
zone-averaged potential temperature (PT) and MSE and <bold>(f)</bold> updraft velocity
predicted by CTL (blue), ARI-A (green) and ARI-AB (red) at 01:00 LT. Shadows
in Fig. 12f represent 25–75th percentile range of simulated updraft velocity.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/10063/2016/acp-16-10063-2016-f12.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <title>Enhanced nocturnal precipitation</title>
      <p>A precipitation rate of over 2.5 mm h<inline-formula><mml:math 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> was observed around 19:00–20:00 LT on
10 June in XZ and its surrounding areas (Zone 2). Only ARI-AB simulation
captured this precipitation event. As shown in Fig. 11a, there existed two
layers with a high BC concentration of up to 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math 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> during
daytime over Zone 2. One was near the surface and peaked around 18:00 LT,
which could be linked to local fire emissions. The other one was lying over
the boundary layer top, which was apparent at an altitude of 0.8 km before
the boundary layer developed and at 2 km after 15:00 LT. It was very likely
associated with the transport of upstream fire pollution. Owing to
strong radiative heating effect of BC, a warmer layer was formed above 1 km
during daytime with temperature increase over 1.0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. In contrast, near-surface temperature kept decreasing. The decline reached
its maximum around 20:00 LT. It was also supported by Fig. 7b in which the
near-surface temperature decreased by almost 8.0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C at XZ.
Until 16:00 LT, the upper-air warming due to radiative absorption was
gradually compensated by cooling from the surface through vertical mixing.
Changes in RH were almost opposite of those in air temperature. Around
18:00 LT, RH at 3 km altitude started to increase and then a precipitating cloud
formed there.</p>
      <p>To get a better insight into the dynamical processes that contribute to
precipitation change, longitude–height cross section of zonal mean responses
of temperature, water vapor and wind profile just before the onset time of
precipitation are demonstrated in Fig. 11c and d. Noteworthy is that
warmed upper air between 117 and 119<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E led to less
condensation there. More water vapor accumulated below 1 km and was then
transported toward Zone 2 by the prevailing east wind near the surface,
leading to  excess water vapor over Zone 2 in the ARI-AB experiment (Fig. 11e).
Simultaneously, radiatively heated air parcel with a temperature
increase of 0.5 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C was found around 2 km over Zone 2. The
warmer layer around 2–3 km combined with large drops in temperature beneath
resulted in a buoyancy-driven lifting force. Moreover, horizontal
heterogeneity in atmospheric heating provided the low-level convergence for
maintaining convection in a conditionally unstable atmosphere around 3 km.
The zone-averaged updraft velocity in ARI-AB experiment tripled that
predicted by CTL and ARI-A at the altitude of 3 km when the precipitation
began (Fig. 11f). Understandably, what made the precipitating cloud form
around 3 km over Zone 2 was the accumulated MSE near the surface and
anomalous updraft of the air that favored the vertical uplift of MSE. The
release of latent heat may increase the upper-air instability and in turn
enhance the precipitation.</p>
      <p>For the downwind region Zone 3, the warming effect caused by
aerosol–radiation interaction was evident for the air column above 0.5 km
all day long on 10 June (Fig. 12a). The warming pattern was coincident
with the distribution of BC concentration. As a result of increased
air temperature, RH decreased substantially during daytime. Late at night,
an extra precipitating cloud formed above 2 km over Zone 3 in ARI-AB
simulation, leading to a nocturnal precipitation with a strength of
approximately 6 mm h<inline-formula><mml:math 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 01:00 LT on 11 June. What triggered this rainfall
event is a bit more complicated than that over Zone 2. First, the whole air
column was  cooling at the moment when the precipitation took place,
inevitably raising the RH value. The RH increase was quite apparent at the
altitude of 3–4 km. Second, daytime radiative absorption by BC-laden plumes
around 2 km heated the surrounding air. Relatively warmer layer at the
altitude of <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 km generated a positive buoyant updraft
(Figure 12f) hence the air parcel there was displaced upwards along with
enhanced convergence carrying in moist air. This effect has been proposed by
Fan et al. (2015) as part of termed “enhanced conditional instability”, by
which absorbing aerosols escalate convection downwind of a heavily polluted
area and promote precipitation. Comparatively, radiative heating of biomass-burning aerosol was the main contributor to the significant enhancement of
upper-level updraft. Last but not the least, spatially heterogeneous
aerosol-related heating was associated with greater horizontal temperature
lapse, resulting in a convergence flow above 3 km with an additional onshore
wind (Fig. 12d). Zone 3 is only about 20 km from the Yellow Sea. It is
plausible that more water vapor-saturated air masses originating from the
ocean brought in excess water vapor and consequently elevated the humidity
above 3 km. More MSE accumulated above 3 km in the ARI-AB experiment compared
with that simulated by the CTL and ARI-A experiments before the precipitation
also support this view (Fig. 12e). We suggest that these precipitating
clouds formed because of instability at the top of the smoke layer, driven
by the strong radiation absorption that warmed the surrounding air.
Therefore, the heated BC-laden air was ascended and cooled, leading to the
formation of clouds preferentially in the conditionally unstable zone in the
upper air.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Uncertainties</title>
      <p>Though the modeling work here characterized cloud and precipitation
anomalies during the biomass-burning event, we may also question to what
extent the modeling reproduced the relevant processes in the real world. As
widely acknowledged, accurate simulation of smoke plume and prediction of
clouds are both challenging for regional/global models. One contributor to
the uncertainties is the quantification of fire emission. The magnitude
was determined by statistical information and laboratory experiment data,
the accuracy and representativeness of which may introduce some uncertainties. The
spatiotemporal distribution of fire emission was allocated based on MODIS
retrievals. Loss of information due to cloud coverage and poor detection
efficiency of short-lived or small-scale fires are major limitations (Giglio
et al., 2003). Another challenge is quantification of heat release from
biomass burning and subsequent effects on local and regional meteorology.
Furthermore, much attention has been paid to the vertical distribution of
absorbing aerosol, to which the cloud response is highly sensitive (Koch and
Del Genio, 2010). The vertical profile of absorbing aerosol in this
simulation underwent little constrain due to limited observation at that
time. The regional model is hardly capable of precisely presenting turbulent
flows and vertical transport, thus introducing uncertainties in three
dimensional distributions of BC. It also should be noted that BC is
co-emitted with other components such as OC and sulfur dioxide that oxidize
to sulfate (Xie et al., 2015). Mixing with other scattering aerosol would
considerably amplify the absorbing efficiency of BC. A model's ability to
account for the evolution of mixing state and how to quantify its
amplification also affect the simulated radiative behaviors. Besides, poorly
recognized secondary organic carbon formation processes and its light
absorption make it imperative to reassess and redefine the chemical
mechanism and optical properties of OC in models (Saleh et al., 2014). The
large uncertainty in simulating clouds and further aerosol–cloud interaction
is another limitation (e.g., Wang et al., 2011; Tao et al., 2012). To
improve the model performance in all these chemical and physical processes,
more comprehensive measurements and modeling efforts are needed in the
future.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions</title>
      <p>To investigate radiative effects of aerosol–radiation interaction on cloud
and precipitation modifications during the exceptionally active agricultural
fire season in June 2012, a bottom-up emission inventory of crop open burning
was developed and then the fully coupled online WRF-Chem model was applied in
this work. The evaluation of simulation through ground-based observations and
satellite retrievals showed that the model generally captured spatial
patterns and temporal variations of fire pollution, which was predominantly
concentrating over northern Anhui and central-northern Jiangsu. It is evident
that post-harvest burning of crop residues emitted a tremendous amount of
atmospheric pollutants and deteriorated regional air quality to a large
extent in East China. Elevated concentration of aerosols, particularly
light-absorbing BC, would heat the atmosphere and cool the ground surface
through both direct solar radiation attenuation (direct radiative forcing)
and cloud redistribution (semi-direct radiative forcing). These radiative
cooling (heating) effects were distinct close to (downwind from) the source
regions of fire sites. Adjusted temperature stratification was intimately
linked to small-scale processes such as turbulent mixing, entrainment and the
evolution of the boundary layer. Subsequently, over Nanjing and its adjacent
regions, absorbing aerosols immediately above the boundary layer top
increased the inversion beneath, reducing available moisture and leading to a
burn-off effect of cloud. Meanwhile, fire plumes played an enhancement role
in nocturnal precipitation over northern Jiangsu by increasing up-level
convective activity and fostering low-level convergence that carries in more
moist air. Overall, aerosols' radiative effect on precipitation modification
is therefore likely to depend to a large extent on local meteorological
conditions like atmospheric instability and humidity.</p>
</sec>
<sec id="Ch1.S5">
  <title>Data availability</title>
      <p>Meteorological datasets used in this work can be acquired from
<uri>http://rda.ucar.edu/datasets/ds463.3/</uri> and
<uri>http://weather.uwyo.edu/upperair/sounding.html</uri>. Model outputs and
radiation observations are available on request from the corresponding
author.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/acp-16-10063-2016-supplement" xlink:title="pdf">doi:10.5194/acp-16-10063-2016-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>This work was supported by the National Natural Science Foundation of China
(D0512/91544231, D0512/41422504 and D0510/41505109). Part of this work was
supported by the Jiangsu Provincial Science Fund for Distinguished Young
Scholars awarded to Aijun Ding  (no. BK20140021).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by:  V.-M. Kerminen <?xmltex \hack{\newline}?>
Reviewed by:  two anonymous referees</p></ack><ref-list>
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biomass-burning season in East China</article-title-html>
<abstract-html><p class="p">Biomass burning is a main source for primary carbonaceous particles in the
atmosphere and acts as a crucial factor that alters Earth's energy budget and
balance. It is also an important factor influencing air quality, regional
climate and sustainability in the domain of Pan-Eurasian Experiment (PEEX).
During the exceptionally intense agricultural fire season in mid-June 2012,
accompanied by rapidly deteriorating air quality, a series of
meteorological anomalies was observed, including a large decline in
near-surface air temperature, spatial shifts and changes in precipitation in
Jiangsu province of East China. To explore the underlying processes that link
air pollution to weather modification, we conducted a numerical study with
parallel simulations using the fully coupled meteorology–chemistry model
WRF-Chem with a high-resolution emission inventory for agricultural fires.
Evaluation of the modeling results with available ground-based measurements
and satellite retrievals showed that this model was able to reproduce the
magnitude and spatial variations of fire-induced air pollution. During the
biomass-burning event in mid-June 2012, intensive emission of absorbing
aerosols trapped a considerable part of solar radiation in the atmosphere and
reduced incident radiation reaching the surface on a regional scale, followed
by lowered surface sensible and latent heat fluxes. The perturbed energy
balance and re-allocation gave rise to substantial adjustments in vertical
temperature stratification, namely surface cooling and upper-air heating.
Furthermore, an intimate link between temperature profile and small-scale
processes like turbulent mixing and entrainment led to distinct changes in
precipitation. On the one hand, by stabilizing the atmosphere below and reducing
the surface flux, black carbon-laden plumes tended to dissipate daytime cloud
and suppress the convective precipitation over Nanjing. On the other hand,
heating aloft increased upper-level convective activity and then favored
convergence carrying in moist air, thereby enhancing the nocturnal
precipitation in the downwind areas of the biomass-burning
plumes.</p></abstract-html>
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