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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-20-14377-2020</article-id><title-group><article-title>Properties of ice cloud over Beijing from surface Ka-band radar observations during 2014–2017</article-title><alt-title>Properties of ice cloud over Beijing from surface Ka-band radar observations</alt-title>
      </title-group><?xmltex \runningtitle{Properties of ice cloud over Beijing from surface Ka-band radar observations}?><?xmltex \runningauthor{J. Huo et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Huo</surname><given-names>Juan</given-names></name>
          <email>huojuan@iap.ac.cn</email>
        <ext-link>https://orcid.org/0000-0003-3241-3021</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Tian</surname><given-names>Yufang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Wu</surname><given-names>Xue</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0427-782X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Han</surname><given-names>Congzheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Liu</surname><given-names>Bo</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5945-5075</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Bi</surname><given-names>Yongheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Duan</surname><given-names>Shu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Lyu</surname><given-names>Daren</given-names></name>
          
        </contrib>
        <aff id="aff1"><institution>Key Laboratory of Middle Atmosphere and Global Environment Observation, Chinese Academy of Sciences, Beijing, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Juan Huo (huojuan@iap.ac.cn)</corresp></author-notes><pub-date><day>27</day><month>November</month><year>2020</year></pub-date>
      
      <volume>20</volume>
      <issue>22</issue>
      <fpage>14377</fpage><lpage>14392</lpage>
      <history>
        <date date-type="received"><day>24</day><month>January</month><year>2020</year></date>
           <date date-type="rev-request"><day>2</day><month>March</month><year>2020</year></date>
           <date date-type="rev-recd"><day>27</day><month>September</month><year>2020</year></date>
           <date date-type="accepted"><day>5</day><month>October</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 </copyright-statement>
        <copyright-year>2020</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="d1e141">The physical properties and radiative role of ice clouds
remain one of the uncertainties in the Earth–atmosphere system. In this
study, we present a detailed analysis of ice cloud properties based on 4 years of surface millimeter-wavelength radar measurements in Beijing, China,
where the summer monsoon from the ocean and the winter monsoon from the continent
prevail alternately, resulting in various ice clouds. More than 6300 ice
cloud clusters were studied to quantify the properties of ice clouds, such
as the height, optical depth and horizontal extent, which can serve as a
reference for parameterization and characterization in global climate
models. In addition, comparison between ice cloud clusters formed under the
summer monsoon and the winter monsoon indicates the different formation and
evolution mechanisms of cirrus clouds. Statistically, temperatures of more than
95 % of ice radar bins are below <inline-formula><mml:math id="M1" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 <inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and more than 80 %
of ice clouds are above 7 km. The dependence of the radar reflectivity of
ice particles on height and temperature was also observed in this study,
indicating that the reflectivity of ice bins increases (decreases) as the
temperature (height) increases. In addition, it is found that there is a
strong linear relationship between the mean reflectivity and the ice cloud
depth. Due to various synoptic circumstances, the ice clouds in summer are
warmer, higher and thicker, with larger reflectivity than that in winter;
in particular, the mean cloud-top height of ice clouds in summer is 2.2 km
higher than that in winter. Our analysis indicates that in spring, in situ-origin
cirrus clouds are more common than liquid-origin cirrus clouds, while in summer
liquid-origin cirrus clouds are more frequent; in autumn and winter, most cirrus
clouds are of in situ origin.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e169">The radiative role of ice clouds in the Earth–atmosphere system is known to
be significant; however, uncertainties remain with respect to the net effects
since ice clouds contain various types of nonspherical ice crystals (Yang
et al., 2015). For example, ice clouds absorb the outgoing infrared
radiation from Earth's surface and lower atmosphere while reflecting a
portion of the incident sunlight back to outer space. When ice clouds are
thin enough for the sun to be seen through them, the net impact on the
planetary radiation balance is generally one of warming; thicker ice clouds
reflect more sunlight and generally result in net cooling (Heymsfield et
al., 2017; Kärcher, 2018; Kox et al., 2014). Cirrus clouds consist solely
of ice crystals. Their occurrence frequency exhibits latitudinal variability
ranging from 50 % in the equatorial regions of Africa to 7 % in the
polar regions (Stubenrauch et al., 2006; Hahn and Warren, 2007; Sassen et
al., 2008, 2009). Ice clouds cover over 50 % of the globe's surface (Hong
and Liu, 2015). Dolinar et al. (2019) reported that single-layer ice clouds
have a global occurrence frequency of about 18 %. Ice clouds are an
important component of the planetary radiation budget in terms of magnitude;
plus, they influence hydrological and climate sensitivities and affect
surface climate (Runheng and Liou, 1985; Yang et al., 2015; Gultepe and
Heymsfield, 2016; Lawson et al., 2019).</p>
      <p id="d1e172">The physical and optical properties of ice clouds, such as ice crystal size,
ice shape, particle concentration, cloud-top height (CTH) and optical
depth, are heterogeneously and diversely distributed over the globe
(Jensen et al., 1996; Mace et al., 2006; Yang and Fu, 2009; Adhikari et
al., 2012; Cotton et al., 2013; Heymsfield et al., 2013; Luebke et al.,
2016; Wolf et al., 2018; Ge et al., 2019). Recent studies show that cirrus
clouds remain one of the largest sources of<?pagebreak page14378?> uncertainty in global climate
models (GCMs), due to the deficiencies in representing their observed
spatial and temporal variability (Zelinka et al., 2012; Joos et al.,
2014; Muhlbauer et al., 2014). According to an IPCC report (Boucher
et al., 2013), “Especially for ice clouds, and for interactions between
aerosols and clouds, our understanding of the basic microscale physics is
not yet adequate, although it is improving”. Understanding the
microphysical and macrophysical properties of ice clouds, as well as their
relationships with atmospheric states, such as temperature, wind velocity
and relative humidity, is important for advancing our fundamental
understanding of the formation and life cycles of ice cloud. It is also an
essential step toward reducing the uncertainties in estimates of the
climatic impact of cirrus clouds and improving the representation of ice clouds in
GCMs. A better understanding of ice clouds is important for improving
climate simulations and numerical weather predictions.</p>
      <p id="d1e175">Millimeter-wavelength radar is a powerful method for observing the
macroscopic and microphysical properties of vertical cloud profiles owing to
its ability to penetrate the interior of clouds. Because of radar systems' short
wavelengths, they are sensitive to small cloud droplets and ice crystals,
meaning they detect all types of nonprecipitating clouds well
(Kollias et al., 2007). Radar can perform long continuous
observations, and the data have a high temporal resolution (i.e., detecting
three profiles per second with the vertically pointing mode), which is more
advantageous than aircraft in understanding the characteristics of daily
changes and the formation and development of clouds. Regular calibration of
radar instruments can ensure the stability of data and support long-term data for cloud
climatology research. This study used long-term, continuous, surface Ka-band
radar data to study and understand the microphysical and macrophysical
properties of ice clouds over Beijing, China, in the northern midlatitude
region. Beijing (39.96<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 116.37<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) is in the
subtropical monsoon zone with a typical continental monsoon climate. Winds
from the southeast ocean prevail in summer, while winds from the northwest
continent dominate in winter, resulting in hot and rainy summers but cold
and dry winters. The formation, evolution and life cycle of ice clouds
present regional and distinctive traits, which are created by the regional
climate and, to a certain extent, the global climate too. This paper
presents the features of ice clouds over midlatitude monsoon regions
through detailed analysis based on long-term radar data and serves as a
reference for cloud parameterization in GCMs.</p>
      <p id="d1e196">Section 2 of this paper briefly introduces the Ka-band radar data, the
identification method for ice clouds and other auxiliary datasets. Section 3 describes the macrophysical properties of ice clouds. Details of the
microphysical properties of ice clouds are presented in Sect. 4. In
Sect. 5, the formation types of cirrus clouds in four seasons are investigated.
Conclusions are given in Sect. 6.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and method</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Ka-band radar</title>
      <p id="d1e214">The ice clouds analyzed in this study are from observations of a Ka-band
polarization Doppler radar (KPDR) situated at the Institute of Atmospheric
Physics (IAP; 39.967<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 116.367<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), Beijing, China.
The KPDR was set up in 2010 and works at a frequency of 35.075 GHz (wavelength
of 8.55 mm; Huo et al., 2019), measuring the equivalent
reflectivity factor (<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, hereinafter simply “reflectivity”; units
mm<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M9" 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>; dBZ <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>), Doppler velocity, spectral width
and linear depolarization ratio of cloud. It is equipped with a
magnetron-type transmitter with a minimum sensitivity of <inline-formula><mml:math id="M11" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45 dBZ for cloud
determination. For comparison, the 94 GHz cloud profiling radar (CPR) on
CloudSat has a sensitivity of approximately <inline-formula><mml:math id="M12" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30 dBZ. Calculations or
measurements of radar reflectivity in previous studies reveal that the
reflectivity of ice clouds over midlatitude regions are mostly larger than
<inline-formula><mml:math id="M13" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30 dBZ (Deng et al., 2010; Pokharel and Vali, 2011; Matrosov and
Heymsfield, 2017). Therefore, the KPDR is capable of detecting most ice clouds
over Beijing. However, the Ka-band radar is more sensitive to larger
particles in a cloud target since the reflectivity is proportional to the
<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msup><mml:mi>D</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M15" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is particle size). For the CPR, thin ice clouds with ice water
content (IWC) lower than approximately 0.4 mg m<inline-formula><mml:math id="M16" 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> are invisible (Wu et
al., 2009). It is possible that the KPDR misses some thin ice clouds when they
consist of small ice crystals (i.e., <inline-formula><mml:math id="M17" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> less than 20 <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m) or the IWC is
smaller than 0.4 mg m<inline-formula><mml:math id="M19" 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>. The pulse width of the KPDR is 0.2 <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>s, and the
beamwidth is 0.4<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Its repetition frequency is 3.5 kHz, and its
vertical resolution is 30 m. The KPDR has operated daily since 2012, mostly in
the vertically pointing mode. During special events – for example,
short-term collaborative observations with other instruments – the scanning
mode changes to the plane position indicator or radar height indicator mode.
In 2013 and 2018, the KPDR was nonoperational during almost the whole of the
summer period. The radar data used in this paper were observed from 1 January 2014 to 31 December 2017. During these 4 years, the valid
operational time of the radar in the vertically pointing mode occupied more
than 80 % of the total time. Namely, there are more than 28 000 h of
radar measurements in the vertically pointing mode during the period 2014–2017.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Ice and cirrus cloud identification</title>
      <?pagebreak page14379?><p id="d1e393">Ice clouds are composed of various types of ice crystals and are usually
thin. Cirrus clouds also consist of ice crystals. Definitions of cirrus
clouds in previous publications provide us with references for ice cloud
identification with the KPDR. For example, in the cloud classification algorithm
developed for the CPR on the CloudSat satellite, the average temperature at
the largest <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the average height of the maximum
<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the cloud-base height (CBH), etc. are combined to determine cirrus
cloud (Wang and Sassen, 2001b). Sassen et al. (2008) classified
cloud layers as cirrus via defining two criteria: namely, the visible
optical depth should be less than 3.0 and the cloud-top temperature should
be lower than <inline-formula><mml:math id="M24" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 <inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, categorizing cirrus clouds via cloud
physical and optical parameters. Deng et al. (2010) identified cirrus layers
by cloud-top and cloud-base temperature (<inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">top</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M27" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M28" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 <inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">base</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M31" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M32" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 <inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C). In some recent studies,
cirrus clouds are defined as ice clouds with temperatures <inline-formula><mml:math id="M34" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M35" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Krämer et al., 2016; Luebke et al., 2016; Heymsfield et
al., 2017). Ge et al. (2019) used two temperature criteria to identify
cirrus cloud: the temperature of the cloud top should be less than <inline-formula><mml:math id="M37" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30 <inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and the temperature at the maximum <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> layer and at the
cloud base should be less than 0 <inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The KPDR has a cloud clustering
and classification algorithm, a detailed description of which has been
presented by Huo et al. (2019). Here, we briefly describe it as
follows. Firstly, the KPDR cloud profiles are grouped as clusters based on a
combination of a time–height clustering method and a <inline-formula><mml:math id="M41" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-means clustering
method. After each cloud cluster is determined, a fuzzy-logic method is
applied using multiple cloud properties, such as CBH, cloud depth (CD) and
radar reflectivity, to classify the cloud cluster into nine types: Cs,
Cc, Ac, As, St, Sc, Ns, Cu and Cb clouds. According to the definitions and
identification approaches in previous studies, we use two criteria to
identify ice clouds from KPDR data after the clustering and classification
algorithm is performed. Namely, a cloud cluster for which the mean cloud-top
temperature is less than <inline-formula><mml:math id="M42" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 <inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and the maximum cloud-base
temperature is less than <inline-formula><mml:math id="M44" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 <inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is determined as ice cloud. Ice cloud with a cloud-base temperature below <inline-formula><mml:math id="M46" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 <inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is regarded
as cirrus cloud in this paper. It should be noted that supercooled water
might exist in ice clouds with a temperature above <inline-formula><mml:math id="M48" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 <inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and
thus what the radar measures should indicate different physical properties
from that of ice particles. In this paper, the supercooled water is not
distinguished, and its proportion and properties will be investigated in the
future.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Other datasets</title>
      <p id="d1e644">This study also used some other datasets to complement the investigation of
the properties of ice and cirrus cloud, such as the temperature profile,
water vapor, wind velocity and cloud optical thickness. The research
datasets of cloud optical thickness (produced from Himawari-8) used in this
paper were supplied by the P-Tree System of the Japan Aerospace Exploration
Agency (<uri>https://www.eorc.jaxa.jp/ptree/index.html</uri>, last access: 6 January
2020). Other meteorological reanalysis data employed were from the European
Centre for Medium-Range Weather Forecasts (ECMWF) ERA5 datasets
(<uri>https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5</uri>, last
access: 6 January 2020).</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Macrophysical properties</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Ice cloud samples under the summer and winter monsoon</title>
      <p id="d1e670">Ice clouds can be vertically and horizontally extensive, with their various
appearances dependent on the diverse range of associated atmospheric
movements and processes. The KPDR is located in the north of the North China
Plain, where to the west and north there are mountains and to the south and
east is the Bohai Sea. In the region's hot summers, the monsoon from the sea
brings large quantities of water vapor, whereas the dry and cold monsoon from
the northern continent dominates this region in winter. These different
monsoon types support various atmospheric conditions, such as increasing
relative humidity, cooling and updrafts, required for the formation of
ice clouds, ultimately resulting in distinct cirrus distributions. Figure 1
presents a typical example of an ice cloud distribution collected by the KPDR in
1 month of winter (January 2016) and 1 month of summer (August 2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e675">Ice clouds occurring in <bold>(a)</bold> January 2016 (winter) and <bold>(b)</bold> August 2015 (summer). The mean cloud-top height, mean base height and lifetime of each ice cluster forms an ice cloud “rectangle”. Its mean radar reflectivity is illustrated with different colors. Dark red
rectangles on the horizontal axis indicate periods without vertically
pointing radar measurements. The surface temperature (<inline-formula><mml:math id="M50" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>; left-hand <inline-formula><mml:math id="M51" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) and total water vapor (TWV; right-hand <inline-formula><mml:math id="M52" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) in the 2 months are presented in panel <bold>(c)</bold>.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f01.png"/>

        </fig>

      <p id="d1e715">There are more ice clouds in August than in January, and the mean radar
reflectivity of ice cloud in August is higher than that in January. Ice
clouds in August also show larger vertical dimensions than in January. The
temperature and amount of water vapor are two key parameters in the
formation of clouds, especially in plain areas where orographic uplift is
negligible. The strong contrast in the climatic circumstances between a
month in summer and a month in winter generates a diverse range of ice
clouds (Fig. 1c). Thus, to better understand the physical or optical
properties of ice clouds, statistical analyses were carried out in this
study for different seasons. Such comparisons of the ice clouds among the
four seasons benefit our understanding of the dominant formation origins of
ice clouds when a region is governed alternately by different monsoon types.
In this study, 4 years of radar observations presented more than 6300 ice
cloud clusters for our analysis.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Monthly and hourly occurrence frequency</title>
      <p id="d1e726">Radar data collected in vertically viewing mode were used to calculate the
occurrence frequency of all clouds (<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), which is the ratio of cloudy
profiles to all profiles in a certain time range (i.e., an hour or a month),
as well as the occurrence frequency of ice clouds (<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), which is the
ratio of profiles determined as ice clouds to all radar profiles:

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M55" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the number of cloudy profiles, <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the number of all
radar profiles and <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the number of ice cloud profiles. Figure 2
shows the monthly occurrence frequency of all clouds and ice clouds in 4 years. In addition, the occurrence frequency of cirrus clouds is also
presented for contrast. September has the maximum <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> among all months,
and summer/winter has the maximum/minimum <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> among the four seasons.
Relative to <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> decreases to 33 %–50 %, and in winter
<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is about 33 % of <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The average <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in April and June
is about 20 %, whereas in winter<?pagebreak page14380?> (December–February) it is no more than
10 %. The average <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the 4 years is 14 %, which is lower than
the ice cloud coverage of 24 % reported by Hahn and Warren (2007) based on
satellite measurements over North China. This might be associated with the
observation location and the field of view (FOV) of the KPDR. Large
quantities of water vapor over the sea areas and orographic-lift movements
over mountain areas provide advantageous conditions for the formation of
clouds, meaning more clouds occur over these areas relative to plain areas.
Therefore, the occurrence frequency calculated from the KPDR data with a
small FOV is lower than the cloud coverage calculated from data with a
broad FOV. For cirrus clouds, the largest occurrence frequency (4 %)
occurs in April. Spring, but not summer, has the most cirrus clouds.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e938">Monthly occurrence frequencies of all clouds (<inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">all</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), ice clouds (<inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and cirrus clouds <bold>(a)</bold>, along with the diurnal <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the four seasons <bold>(b)</bold>.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f02.png"/>

        </fig>

      <p id="d1e986">The KPDR operates continuously and thus allows the diurnal variation in
<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to be studied, which illustrates the potential relationship with
local thermal convection caused by solar heating. As shown in Fig. 2a, the
three highest <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values in spring, summer, autumn and winter occur at
20:00/22:00/19:00, 21:00/23:00/22:00, 00:00/22:00/21:00 and
14:00/13:00/17:00 LT (UTC+8), respectively. The hourly variations in <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the
four seasons are different; in spring, summer and autumn, larger <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
values appear at night, whereas larger <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values in winter appear
during the daytime. The diurnal variation in <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> seems to be insensitive to
solar heating, which drives the development of regional thermal convection.
Here, the presence of ice clouds over the KPDR is not closely related to local
air-updraft activities, indicating that these ice clouds may mostly not be
generated locally by thermal convections. It is interesting that <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi mathvariant="normal">ic</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
decreases from 00:00 to 02:00 LT and then increases after that in the four
seasons. Is there a decay process in ice clouds during this period? Is the
decrease caused by wind, vertical movement or turbulence? Further analysis
is required in the future to answer these questions.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Height, depth and extent</title>
      <p id="d1e1075">The top height of ice cloud, especially cirrus cloud, indicates the highest
condensation level in the troposphere, above which clouds cannot form
because of the nonconducive condensation conditions. The base height of ice
clouds indicates the lowest level required for ice formation. In this study,
the CTH and CBH were calculated for each ice cloud cluster; specifically,
the CTH and CBH are the mean values of all cloudy profiles in an ice cloud
cluster. The distributions of the mean CTH and CBH of all ice clouds in the
four seasons are presented in Fig. 3, and Table 1 presents the quantified
statistical results.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1080">Distribution of cloud-top height <bold>(a)</bold>, cloud-base height <bold>(b)</bold>, cloud depth <bold>(c)</bold> and horizontal extent (EXT; <bold>d</bold>) in the four seasons. In panel <bold>(d)</bold>, EXT is shown as log10 values.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f03.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1107">Statistical results for the cloud-top height (CTH),
cloud-base height (CBH), cloud depth (CD), horizontal extent (EXT) and cloud optical depth (COD) in the
four seasons. The “trimmean” is the 10 % trimmed mean of portion clusters, excluding 10 % of clusters with the highest and lowest values (unit: km).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Season</oasis:entry>
         <oasis:entry colname="col2">Parameters</oasis:entry>
         <oasis:entry colname="col3">Mean</oasis:entry>
         <oasis:entry colname="col4">Median</oasis:entry>
         <oasis:entry colname="col5">Trimmean</oasis:entry>
         <oasis:entry colname="col6">Maximum</oasis:entry>
         <oasis:entry colname="col7">Minimum</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Spring</oasis:entry>
         <oasis:entry colname="col2">CTH</oasis:entry>
         <oasis:entry colname="col3">8.16</oasis:entry>
         <oasis:entry colname="col4">8.17</oasis:entry>
         <oasis:entry colname="col5">8.15</oasis:entry>
         <oasis:entry colname="col6">11.74</oasis:entry>
         <oasis:entry colname="col7">5.73</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CBH</oasis:entry>
         <oasis:entry colname="col3">7.68</oasis:entry>
         <oasis:entry colname="col4">7.68</oasis:entry>
         <oasis:entry colname="col5">7.68</oasis:entry>
         <oasis:entry colname="col6">11.43</oasis:entry>
         <oasis:entry colname="col7">5.43</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CD</oasis:entry>
         <oasis:entry colname="col3">0.35</oasis:entry>
         <oasis:entry colname="col4">0.27</oasis:entry>
         <oasis:entry colname="col5">0.32</oasis:entry>
         <oasis:entry colname="col6">2.1</oasis:entry>
         <oasis:entry colname="col7">0.06</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">EXT</oasis:entry>
         <oasis:entry colname="col3">61.5</oasis:entry>
         <oasis:entry colname="col4">17.34</oasis:entry>
         <oasis:entry colname="col5">35.6</oasis:entry>
         <oasis:entry colname="col6">2824.9</oasis:entry>
         <oasis:entry colname="col7">0.18</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">COD</oasis:entry>
         <oasis:entry colname="col3">4.27</oasis:entry>
         <oasis:entry colname="col4">3.22</oasis:entry>
         <oasis:entry colname="col5">3.81</oasis:entry>
         <oasis:entry colname="col6">–</oasis:entry>
         <oasis:entry colname="col7">0.06</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Summer</oasis:entry>
         <oasis:entry colname="col2">CTH</oasis:entry>
         <oasis:entry colname="col3">9.27</oasis:entry>
         <oasis:entry colname="col4">9.38</oasis:entry>
         <oasis:entry colname="col5">9.30</oasis:entry>
         <oasis:entry colname="col6">12.86</oasis:entry>
         <oasis:entry colname="col7">6.10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CBH</oasis:entry>
         <oasis:entry colname="col3">8.73</oasis:entry>
         <oasis:entry colname="col4">8.97</oasis:entry>
         <oasis:entry colname="col5">8.78</oasis:entry>
         <oasis:entry colname="col6">12.42</oasis:entry>
         <oasis:entry colname="col7">5.64</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CD</oasis:entry>
         <oasis:entry colname="col3">0.39</oasis:entry>
         <oasis:entry colname="col4">0.30</oasis:entry>
         <oasis:entry colname="col5">0.35</oasis:entry>
         <oasis:entry colname="col6">2.45</oasis:entry>
         <oasis:entry colname="col7">0.06</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">EXT</oasis:entry>
         <oasis:entry colname="col3">43.0</oasis:entry>
         <oasis:entry colname="col4">16.1</oasis:entry>
         <oasis:entry colname="col5">29.6</oasis:entry>
         <oasis:entry colname="col6">725.1</oasis:entry>
         <oasis:entry colname="col7">0.13</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">COD</oasis:entry>
         <oasis:entry colname="col3">6.07</oasis:entry>
         <oasis:entry colname="col4">4.28</oasis:entry>
         <oasis:entry colname="col5">5.64</oasis:entry>
         <oasis:entry colname="col6">–</oasis:entry>
         <oasis:entry colname="col7">0.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Autumn</oasis:entry>
         <oasis:entry colname="col2">CTH</oasis:entry>
         <oasis:entry colname="col3">8.23</oasis:entry>
         <oasis:entry colname="col4">8.27</oasis:entry>
         <oasis:entry colname="col5">8.24</oasis:entry>
         <oasis:entry colname="col6">11.25</oasis:entry>
         <oasis:entry colname="col7">5.69</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CBH</oasis:entry>
         <oasis:entry colname="col3">7.74</oasis:entry>
         <oasis:entry colname="col4">7.80</oasis:entry>
         <oasis:entry colname="col5">7.77</oasis:entry>
         <oasis:entry colname="col6">11.07</oasis:entry>
         <oasis:entry colname="col7">5.31</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CD</oasis:entry>
         <oasis:entry colname="col3">0.35</oasis:entry>
         <oasis:entry colname="col4">0.28</oasis:entry>
         <oasis:entry colname="col5">0.33</oasis:entry>
         <oasis:entry colname="col6">1.82</oasis:entry>
         <oasis:entry colname="col7">0.06</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">EXT</oasis:entry>
         <oasis:entry colname="col3">86.10</oasis:entry>
         <oasis:entry colname="col4">23.5</oasis:entry>
         <oasis:entry colname="col5">55.17</oasis:entry>
         <oasis:entry colname="col6">2863.8</oasis:entry>
         <oasis:entry colname="col7">0.47</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">COD</oasis:entry>
         <oasis:entry colname="col3">4.62</oasis:entry>
         <oasis:entry colname="col4">3.05</oasis:entry>
         <oasis:entry colname="col5">4.01</oasis:entry>
         <oasis:entry colname="col6">–</oasis:entry>
         <oasis:entry colname="col7">0.01</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Winter</oasis:entry>
         <oasis:entry colname="col2">CTH</oasis:entry>
         <oasis:entry colname="col3">7.02</oasis:entry>
         <oasis:entry colname="col4">6.90</oasis:entry>
         <oasis:entry colname="col5">7.00</oasis:entry>
         <oasis:entry colname="col6">9.94</oasis:entry>
         <oasis:entry colname="col7">5.50</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CBH</oasis:entry>
         <oasis:entry colname="col3">6.63</oasis:entry>
         <oasis:entry colname="col4">6.57</oasis:entry>
         <oasis:entry colname="col5">6.63</oasis:entry>
         <oasis:entry colname="col6">9.75</oasis:entry>
         <oasis:entry colname="col7">5.30</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CD</oasis:entry>
         <oasis:entry colname="col3">0.28</oasis:entry>
         <oasis:entry colname="col4">0.21</oasis:entry>
         <oasis:entry colname="col5">0.26</oasis:entry>
         <oasis:entry colname="col6">2.13</oasis:entry>
         <oasis:entry colname="col7">0.04</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">EXT</oasis:entry>
         <oasis:entry colname="col3">72.7</oasis:entry>
         <oasis:entry colname="col4">19.3</oasis:entry>
         <oasis:entry colname="col5">41.4</oasis:entry>
         <oasis:entry colname="col6">1695.2</oasis:entry>
         <oasis:entry colname="col7">1.50</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">COD</oasis:entry>
         <oasis:entry colname="col3">4.52</oasis:entry>
         <oasis:entry colname="col4">2.80</oasis:entry>
         <oasis:entry colname="col5">4.10</oasis:entry>
         <oasis:entry colname="col6">–</oasis:entry>
         <oasis:entry colname="col7">0.21</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1649">It is shown that the CTH of ice clouds varies in the range of 5.5–12.9 km
(Fig. 3a). The difference between the maximum and the minimum is about 6 km
in each season, indicating the ranges of the condensation level and various
formation mechanisms of ice clouds. Besides, differences in the CTH between
the four seasons are also apparent. Both the maximum (12.9 km) and the
highest mean (9.27 km) CTH<?pagebreak page14381?> are found in summer, whereas winter has the
minimum CTH (9.94 km) and lowest mean CTH (7.02 km). In summer, 85 % of
ice clouds have a CTH greater than 8 km and 29 % are greater than 10 km.
In winter, 71 % of ice clouds have a CTH larger than 8 km and those with
a CTH higher than 6 km account for 97 %. The mean CTH in summer is 2.2 km
higher than that in winter, which means the average condensation level in
summer is also 2.2 km higher. Spring and autumn are two transition seasons
and their CTHs are 8.16 and 8.23 km, respectively, which are between
those of summer and winter.</p>
      <p id="d1e1652">Figure 3b shows that the CBH changes within a range of 5.3–12.4 km, and the
minimum CBHs in the four seasons are close to each other, ranging between
5.3 and 5.7 km. However, the mean CBH in summer is the highest (8.7 km)
among the four seasons, while the lowest (6.6 km) is in winter. The
difference in CBH between summer and winter is 2.1 km.<?pagebreak page14382?> The mean CBHs in
spring and autumn are both 7.7 km. In summer, the percentage of ice clouds
with a CBH larger than 8 km is 72 %, while it is only 65 % in winter. In
summer and winter, 95 % of ice clouds have a CBH greater than 6 km.</p>
      <p id="d1e1655">It is shown that the mean CDs of ice clouds in the four seasons are close,
with the depths of most clusters being less than 1 km (Fig. 3c).
Statistically, in the four seasons, 68 % of clusters have a CD of less
than 0.5 km, 90 % have a CD of less than 1 km and 96 % have a CD of less than 1.5 km. It should
be noted that the CTH, CBH and CD here are the mean values of an ice cloud
cluster. It is therefore possible that there are some instances of CTH, CBH
and CD that are greater than their corresponding mean values.</p>
      <p id="d1e1658">The horizontal extent (EXT) of ice clouds indicates the clouds' lifetimes and their
formation mechanism type. For the KPDR, the EXT of an ice cloud cluster is
computed as follows:
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M77" display="block"><mml:mrow><mml:mi mathvariant="normal">EXT</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">hw</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">ci</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">hw</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mean velocity of horizontal wind calculated from the
ECMWF-ERA5 dataset and <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">ci</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the continuous time during which an ice
cluster moves over the KPDR. It is found that the maximum EXT of ice clouds
reaches 2800 km, in April 2017, and the maximum <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">ci</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is 21 h, in March 2016. The EXT ranges through orders of magnitude
from low values of less than 0.1 km to over 2800 km. Summer has the minimum
mean, median and trimmed mean EXT, while ice clouds in autumn have the
maximum mean, median and trimmed mean EXT. Statistically, about 75 % of
ice clouds have an EXT of less than 50 km and 87 % have an EXT of less than 100 km. The
statistically quantified structural properties of ice clouds in the four
seasons are presented in Table 1.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Optical depth</title>
      <p id="d1e1726">Cloud optical depth (COD) is relatively independent of wavelength throughout
the visible spectrum. In the visible portion of the spectrum, the COD is
almost entirely due to scattering by droplets or crystals of clouds
(American Meteorological Society, 2019). Therefore, the CODs of ice clouds
depend directly on the CD, the IWC and the size distribution of the ice
crystals, indicating a cooling effect or warming effect in the energy
budget.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1731">The cloud optical depth (COD) of ice clouds in terms of
the cloud depth in spring <bold>(a)</bold>, summer <bold>(b)</bold>, autumn <bold>(c)</bold>, and winter <bold>(d)</bold>. Colors indicate the mean reflectivity of those radar profiles within 10 min of the AHI (Advanced Himawari Imager) observation time. Cases with cloud-base temperatures lower than <inline-formula><mml:math id="M81" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 <inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C are illustrated with purple edges. Panel <bold>(e)</bold> presents the probability density distribution of the COD in the four seasons.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f04.png"/>

        </fig>

      <p id="d1e1772">The Advanced Himawari Imager (AHI), on board the geostationary meteorological
Himawari-8 satellite operated by the Japan Meteorological Agency,
observes the Beijing area every 10 min and began releasing COD and
cloud-type products in July 2015 with a spatial resolution of 5 km. The CODs
are retrieved by using nonabsorbing visible wavelengths (i.e., 0.51 or 0.64 <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m) and water-absorbing, near-infrared wavelengths (i.e., 1.6 or 2.3 <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m; Nakajima and Nakajma, 1995; Kawamoto et al., 2001). Quantified
uncertainties in the AHI CODs have not been reported, so we use them here
directly. The data nearest to the KPDR that the AHI determines as<?pagebreak page14383?> cirrus cloud and
the KPDR determines as ice cloud are selected, and their CODs are investigated.
Those collocated CODs (collected from the year 2016 to 2017) combined with
the mean CDs and mean reflectivity, which are calculated from all cloudy
KPDR bins observed within 10 min of the AHI observing time, are presented in
Fig. 4.</p>
      <p id="d1e1792">In the four seasons, CODs show an increasing tendency with increasing CD.
The mean reflectivity shows a similar tendency, meaning thicker ice clouds
generally contain larger particles and a greater number density of ice
particles. The probability density distributions of CODs in the four seasons
show a higher probability occurring at lower CODs. The mean COD in spring,
summer, autumn and winter is 4.27, 6.07, 4.62 and 4.52, respectively. The
proportions of CODs lower than 3 in spring, summer, autumn and winter are
46 %, 36 %, 49 % and 52 %, respectively. The proportions of CODs
lower than 10 in the four seasons are 91 %, 79 %, 87 % and 90 %,
respectively. In Fig. 4, KPDR cirrus clouds are shown with purple circles.
The proportions of CODs for cirrus clouds lower than 3 in spring, summer,
autumn and winter are 70 %, 55 %, 77 % and 79 %, respectively. The
proportions of CODs lower than 6 in the four seasons are 93 %, 77 %,
94 % and 98 %, respectively. As shown in previous studies, the primary
cirrus optical depth is below 3 (Kienast-Sjögren et al., 2016; Sassen et
al., 2008). Here, our analysis shows larger CODs, indicating possible
mixed-phase clouds. Also, it might be related to the uncertainty in CODs,
as the uncertainties in AHI CODs and the different FOV between the KPDR and the AHI
may cause the employed CODs to differ from the real CODs. The results here
present statistical features of the CODs of ice clouds over Beijing based on
a COD dataset of limited accessibility. For cirrus clouds, lidar should
provide accurate COD measurements.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Microphysical properties</title>
      <?pagebreak page14384?><p id="d1e1804">The most important microphysical quantities of ice clouds are the ice
particle size distribution, the IWC and the clouds' shapes (Heymsfield et al.,
2017). It is known that the radar equivalent (or effective) reflectivity
factor can be expressed as
          <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M85" display="block"><mml:mtable rowspacing="0.2ex" columnspacing="1em" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mfenced close="|" open="|"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi>m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mrow><mml:msup><mml:mi>m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo movablelimits="false">∫</mml:mo><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mo movablelimits="false">∫</mml:mo><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mo movablelimits="false">∫</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi></mml:mrow></mml:mfenced><mml:mi>N</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi></mml:mrow></mml:mfenced><mml:mi mathvariant="normal">d</mml:mi><mml:mi>D</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
        where <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">∅</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is the backscattering
cross section with maximum dimension <inline-formula><mml:math id="M87" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> and an axial direction <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">∅</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> with respect to the radar beam, <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">∅</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is the number density, <inline-formula><mml:math id="M90" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> is the wavelength,
and <inline-formula><mml:math id="M91" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> is the complex index of refraction of the scattering target. To date,
numerous empirical relationships between <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and cloud properties
(<inline-formula><mml:math id="M93" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>) – e.g., IWC, snow precipitation rate – have been developed, usually in
the power-law form of
          <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M94" display="block"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>A</mml:mi><mml:msup><mml:mi>P</mml:mi><mml:mi>B</mml:mi></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M95" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> is the prefactor coefficient and <inline-formula><mml:math id="M96" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> is the exponent derived in terms of
calculated or measured datasets (Liu and Illingworth, 2000; Wang and
Sassen, 2001a; Heymsfield et al., 2008; Austin et al., 2009; Delanoë and
Hogan, 2010; Deng et al., 2015; Matrosov and Heymsfield, 2017; Heymsfield et
al., 2018). Delanoë and Hogan (2008, 2010) proposed a different
method using a forward model to retrieve the IWC and the effective radius by
combination with the COD. Also, the basic principles of this method are
applied in the CloudSat–CALIPSO cloud microphysical retrieval algorithm.
However, the use of empirical relations such as in Eq. (5) is still common in
many practical measurements, and the correspondence between the IWC and
<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is related to the particle size distribution (the gamma
distribution is mostly used for ice clouds).</p>
      <p id="d1e2069">For the KPDR, the development of the IWC and particle size retrieval
algorithm is in progress but has not been tested completely. In this paper,
we use the measured radar reflectivity factor <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> directly, not the
retrieved microphysical quantities, to study and characterize the
microphysical properties of ice clouds. It can be found from Eq. (2) that
reflectivity increases when <inline-formula><mml:math id="M99" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M100" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> increase; in other words, a
larger reflectivity normally indicates a larger <inline-formula><mml:math id="M101" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M102" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> and IWC.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Reflectivity and height dependence</title>
      <p id="d1e2118">The KPDR detects clouds at a 30 m vertical resolution. All ice radar bins
collected from 2014 to 2017 were counted according to their reflectivity and
height, and the relative frequencies (counts; calculated at 0.25 dBZ and 30 m intervals within 15 km) are shown separately in Fig. 5. As presented, ice
clouds exist below the height of 13 km. In summer, the reflectivity mostly
varies between <inline-formula><mml:math id="M103" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 and <inline-formula><mml:math id="M104" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 dBZ, while most of the reflectivity falls
within the range of <inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 to <inline-formula><mml:math id="M106" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20 dBZ in winter. In spring and autumn, the
reflectivity primarily ranges between <inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 and <inline-formula><mml:math id="M108" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 dBZ. The range of
variation in reflectivity in summer is the biggest among the four seasons,
while it is the smallest in winter. Statistically, at the same height where ice
clouds exist in the four seasons, the mean reflectivity of winter is 5 dBZ
less than that of spring or autumn and it is 10 dBZ less than that of
summer. In the four seasons, the mean reflectivity declines as the height
increases below 11 km, with a similar slope. At the height above 11 km, the
relationship between reflectivity and the height varies greatly among the four
seasons, which might be due to the small sample counts. It can also be seen
that the ice bins in summer are located at higher heights than in winter.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e2166">The frequency of reflectivity versus height in spring <bold>(a)</bold>, summer <bold>(b)</bold>, autumn <bold>(c)</bold> and winter <bold>(d)</bold>. Colors are the log number of the
counts (calculated at 0.25 dBZ and 30 m intervals). The mean reflectivity
calculated at various heights and the corresponding standard deviation (SD)
are presented in panels <bold>(e)</bold> and <bold>(f)</bold>, respectively.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Temperature dependence</title>
      <p id="d1e2202">Temperature plays a key role in the formation, evolution and lifetime of ice
clouds. Activation of liquid water drops does not happen below
<inline-formula><mml:math id="M109" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 <inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C because the relative humidity where the ice forms is
below water saturation. At temperatures higher than <inline-formula><mml:math id="M111" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 <inline-formula><mml:math id="M112" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C,
primary ice clouds form only when aided by ice-nucleating particles
(Kanji et al., 2017). The summer monsoon and winter monsoon
in Beijing support distinct temperatures, water vapor, etc., i.e., the
conditions necessary for the formation of ice clouds, resulting in
distributions of reflectivity with different features corresponding to
temperature. The frequencies (counts; calculated at 0.25 dBZ and 1 <inline-formula><mml:math id="M113" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C intervals) are shown separately in Fig. 6.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e2248">As in Fig. 5 but for temperature, and the colors are the
log number of the counts (calculated at 0.25 dBZ and 1 <inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
intervals).</p></caption>
          <?xmltex \igopts{width=406.874409pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f06.png"/>

        </fig>

      <p id="d1e2266">In spring, summer and autumn, ice clouds occur mostly at temperatures within
the range of <inline-formula><mml:math id="M115" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 to <inline-formula><mml:math id="M116" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>55 <inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, relative to which ice
clouds in winter occur at lower temperatures. Statistically, the percent of
ice bins with temperatures less than <inline-formula><mml:math id="M118" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 <inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is 99 %, 95 %,
95 % and 99 % in spring, summer, autumn and winter, respectively; the
percent of ice bins with temperatures less than <inline-formula><mml:math id="M120" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25 <inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is
85 %, 71 %, 72 % and 92 % in spring, summer, autumn and winter,
respectively; and the percent of ice bins with temperatures less than
<inline-formula><mml:math id="M122" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 <inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is 52 %, 36 %, 35 % and 60 % in spring, summer,
autumn and winter, respectively. The reflectivity shows a dependence on the
temperature, increasing when temperature increases. Statistically, the mean
temperature of ice clouds in winter is lower than that in other seasons,
even though these ice clouds appear at lower heights. As the temperature
decreases, the difference in reflectivity between winter and summer
declines. At the same temperature, the mean reflectivity in summer is higher
than that in winter. The slopes among the four seasons are close to each
other when temperature is above <inline-formula><mml:math id="M124" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50 <inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, demonstrating a
determinative effect of the temperature on the cloud particle properties.
The slopes in the four seasons disperse at temperatures lower than
<inline-formula><mml:math id="M126" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50 <inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, which might be because the small sample counts influence
the representativeness of statistical results.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Depth dependence</title>
      <p id="d1e2383">Based on all the ice clusters in the 4 years, we calculated the mean
reflectivity and the mean depth of each cluster (Fig. 7), and it was
interesting to find that there is a strong linear relationship between the
mean reflectivity and the CD. Specifically, the mean reflectivity increases
as the CD increases. The linear equation shown in Fig. 7 represents a method
that can be used to estimate the mean reflectivity (or CD) if the CD (or
reflectivity) is known, which should be useful for cloud parameterization in
GCMs.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e2388">The mean reflectivity of ice clouds as a function of
cloud depth (CD).</p></caption>
          <?xmltex \igopts{width=389.802756pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f07.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
<?pagebreak page14385?><sec id="Ch1.S5">
  <label>5</label><title>Origination type of cirrus clouds</title>
      <p id="d1e2409">Krämer et al. (2016) and Luebke et al. (2016) classified two types of
cirrus cloud according to their formation mechanism; namely, in situ- and
liquid-origin cirrus cloud. The in situ-origin cirrus type forms directly as
cirrus clouds, while the liquid-origin type originates from mixed-phase clouds that
are completely frozen until they are lifted to temperatures of <inline-formula><mml:math id="M128" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M129" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 <inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Krämer et al. (2016) and Luebke et al. (2016) reported that the in situ-origin cirrus clouds are mostly thin,
with a lower IWC, while liquid-origin cirrus clouds tend to be thicker with a higher
IWC. Also, liquid-origin cirrus clouds tend to have larger ice crystals than in situ-origin
cirrus clouds. Various prefactor coefficients dependent on temperature have been
derived and applied in the <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–IWC power-law relationship (i.e., Eq. 5) since the distribution of reflectivity has a dependence on temperature,
just as shown above in Sect. 4.2 (Hogan et al., 2006; Heymsfield et
al., 2013, 2018; Matrosov and Heymsfield, 2017).
Therefore, the reflectivity of in situ-origin cirrus clouds should generally be less than
that of liquid-origin cirrus clouds.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e2448">Normalized frequency of the reflectivity at different
temperatures (<inline-formula><mml:math id="M132" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>) in spring. The solid line is the frequency calculated from
all cirrus clouds. The dashed line is the frequency calculated from cirrus clouds with a
mean <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M134" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M135" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ. The dash-dotted line is the frequency
calculated from cirrus clouds with a mean <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> above <inline-formula><mml:math id="M137" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ. The dashed line corresponds to the in situ-origin type, and the dotted line corresponds to the liquid-origin type. <inline-formula><mml:math id="M138" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the maximum number used to normalize the frequency.</p></caption>
        <?xmltex \igopts{width=423.946063pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f08.png"/>

      </fig>

      <p id="d1e2515">In this section, based on the frequency statistics in Sect. 4.2, we
calculated the distribution of reflectivity (similar to the probability
density function, PDF) at several temperatures to investigate the origin
type of cirrus clouds in Beijing. Figures 8–11 show the normalized frequency of
reflectivity at central temperatures of <inline-formula><mml:math id="M139" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65, <inline-formula><mml:math id="M140" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60, <inline-formula><mml:math id="M141" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>55, <inline-formula><mml:math id="M142" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50, <inline-formula><mml:math id="M143" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45 and
<inline-formula><mml:math id="M144" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 <inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C within <inline-formula><mml:math id="M146" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1 <inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in spring, summer, autumn
and winter, respectively. The maximum counts, <inline-formula><mml:math id="M148" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, used to normalize the
frequency is also presented in the figures.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e2596">As in Fig. 8 but for summer. No cirrus clouds are found when
temperature is at or below <inline-formula><mml:math id="M149" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65 <inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in summer.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f09.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e2623">As in Fig. 8 but for autumn. No cirrus clouds are found when the
temperature is at or below <inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65 <inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in autumn.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f10.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e2650">As in Fig. 8 but for winter.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/14377/2020/acp-20-14377-2020-f11.png"/>

      </fig>

      <?pagebreak page14386?><p id="d1e2659">Cirrus clouds present diverse reflectivity frequency distributions in terms
of temperature in the four seasons. There is no cirrus cloud detected in
summer and autumn (see Figs. 9a and 10a) at or below <inline-formula><mml:math id="M153" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65 <inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.
The number of cirrus cloud bins at <inline-formula><mml:math id="M155" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65 <inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in spring and autumn
is very small when compared to other temperatures above <inline-formula><mml:math id="M157" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50 <inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.
This might be because the frequency of atmospheric temperature <inline-formula><mml:math id="M159" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M160" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65 <inline-formula><mml:math id="M161" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C within the troposphere over Beijing is small, so cirrus
clouds at and below this temperature are few. Cirrus clouds also occur
little in summer and autumn at <inline-formula><mml:math id="M162" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60 <inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, due to the higher average
temperature than in the other two seasons. Above <inline-formula><mml:math id="M164" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>55 <inline-formula><mml:math id="M165" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, the
peak frequency center in winter is located at a smaller reflectivity value than
that in summer, indicating smaller particles and a smaller number density than in
summer. In the four seasons, the <inline-formula><mml:math id="M166" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> value at <inline-formula><mml:math id="M167" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45 <inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is the biggest
among all temperatures, indicating that cirrus cloud appears more frequently
at <inline-formula><mml:math id="M169" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45 <inline-formula><mml:math id="M170" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C than at other temperatures. The reason is that at
these altitudes both in situ-origin and liquid-origin cirrus clouds appear, whereas
at colder temperatures only in situ-origin cirrus clouds exist (Krämer et al.,
2020). Spring has the biggest <inline-formula><mml:math id="M171" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> value at each temperature, indicating that
cirrus clouds in spring are the most frequent, which has also been shown in
Fig. 2.</p>
      <?pagebreak page14387?><p id="d1e2814">A bimodal PDF is found at some temperatures – for example, at
<inline-formula><mml:math id="M172" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60 and <inline-formula><mml:math id="M173" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>65 <inline-formula><mml:math id="M174" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in spring and at <inline-formula><mml:math id="M175" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45 <inline-formula><mml:math id="M176" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in autumn. However, most PDFs show a unimodal feature. One possibility is
that only one origin type exists in Beijing. Another possibility is that the
difference between the two origin types is not clearly distinguished. It
might be related to the measurement specialties of radar since the
<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> indicates the backscattering from numerous particles and the
<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is more sensitive to the larger particles in a cloud target.</p>
      <p id="d1e2880">We divided cirrus clouds into two groups using a mean-<inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> threshold to
study whether cirrus clouds over Beijing also originate from different
mechanisms. If the PDFs of the two separate groups exhibit distinct
features, it is possible that they form from different mechanisms. It is
found that the cirrus clouds in spring and summer (Figs. 8 and 9) can be
separated clearly into two groups by a threshold of <inline-formula><mml:math id="M180" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ, and the two
groups demonstrate different PDFs after applying each threshold between
<inline-formula><mml:math id="M181" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>32 dBZ and <inline-formula><mml:math id="M182" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38 dBZ. The full width at half maxima and the peak center
are different. In addition, the proportions of the two groups are
comparable. However, in autumn and winter, cirrus clusters with a mean
reflectivity of less than <inline-formula><mml:math id="M183" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ contribute the absolute majority of all
cirrus clusters when compared with the cirrus clusters with a reflectivity larger than
<inline-formula><mml:math id="M184" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ, illustrating different PDFs from those in spring and summer. It
is possible that the differences in the PDFs among the four seasons are due to
the different origin types. For a mean <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mo>-</mml:mo></mml:mrow></mml:math></inline-formula>34 dBZ, a cirrus cloud
is likely to be an in situ-origin cirrus cloud; for a mean <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M187" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M188" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ, a cirrus cloud is likely to be a liquid-origin cirrus cloud. From Figs. 8 and 9, it can be seen that spring has more in situ-origin cirrus clouds,<?pagebreak page14389?> while summer has
more liquid-origin cirrus clouds. In winter and autumn, cirrus clouds with a mean <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mo>-</mml:mo></mml:mrow></mml:math></inline-formula>34 dBZ dominate, which means that the dominant cirrus clouds in winter
and autumn are in situ-origin cirrus clouds. Summer has more convective movements and
water vapor resulting in dominant liquid-origin cirrus clouds.</p>
      <p id="d1e2985">As mentioned above, there might be another possibility, which is that only one origin
type dominates over Beijing, since most PDFs are unimodal. Large-scale
synoptic and dynamic analysis should be carried out to distinguish the
dominant origin type. At present, however, we prefer the view that there are
two origin types in Beijing, since this is consistent with the basic
weather characteristics in the four seasons. Nonetheless, more work will be
performed in the future to confirm the current assumptions. On the whole,
the formation mechanisms of cirrus clouds in spring and summer in Beijing
illustrate different features to those in autumn and winter. It can also be
found that the distribution of reflectivity depends not only on the
temperature but also on the origin type.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Summary and discussion</title>
      <p id="d1e2996">Ice clouds are an important component of the planetary radiation budget and
remain an uncertainty source in GCMs. This study used 4 years of
vertically pointing Ka-band radar measurements in Beijing to characterize
the physical and optical properties of ice clouds and to investigate the
origination type of cirrus clouds. The goal was to present the quantified
properties of ice clouds over the subtropical monsoon zone, which can be
represented in GCMs to move toward a better understanding of the relationships
between temperature and radar reflectivity under different formation
conditions in various monsoon climates.</p>
      <p id="d1e2999">The winter monsoon and summer monsoon prevail alternately over Beijing,
resulting in four distinct seasons. Ice clouds in winter and summer show
strikingly different features. The specific findings about the properties of
ice clouds can be summarized as follows:
<list list-type="order"><list-item>
      <p id="d1e3004">The occurrence frequency, height, temperature and mean reflectivity of ice
clouds in winter are lower than in summer. The average occurrence frequency
over Beijing is 14 %, and it is 20 % in summer but less than 10 % in
winter. The diurnal variation in the occurrence frequency is not obvious,
indicating an insensitive response to solar heating.</p></list-item><list-item>
      <p id="d1e3008">The CTHs of ice clouds range within 5.5–12.9 km, and the difference between
the maximum and minimum reaches 6 km in every season. The mean CTH in summer
is 2.2 km higher than in winter. The CBHs range within 5–12.4 km, and the
difference in the mean CBH between summer and winter is 2.1 km. In total,
86 % of ice clouds are above 7 km in summer and 81 % are above 7 km in
winter. Statistically, in the four seasons, 68 % of clusters have a depth
of less than 0.5 km, 90 % have a depth of less than 1 km, and 96 % have a depth of less than 1.5 km.</p></list-item><list-item>
      <p id="d1e3012">The EXT ranges through orders of magnitude from low values of less than 0.1 km to over 2800 km. Summer has the minimum mean, median and trimmed mean
EXT, whereas ice clouds in autumn have the maximum mean, median and trimmed
mean EXT. Statistically, about 75 % of ice clouds have an EXT of less than 50 km and 87 % have an EXT of less than 100 km. In addition, the mean COD in spring, summer,
autumn and winter is 4.3, 6.1, 4.6 and 4.5, respectively.</p></list-item><list-item>
      <p id="d1e3016">The radar reflectivity of ice clouds is dependent on the height,
temperature and CD. The reflectivity mostly varies between <inline-formula><mml:math id="M190" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 and <inline-formula><mml:math id="M191" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 dBZ, and the mean reflectivity in summer is 10 dBZ higher than in winter.
More than 95 % of ice bins are below the temperature of <inline-formula><mml:math id="M192" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 <inline-formula><mml:math id="M193" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and the mean temperature of ice cloud in winter is the lowest among the
four seasons. It was found that there is a strong linear relationship
between the mean reflectivity and the CD.</p></list-item><list-item>
      <p id="d1e3050">Cirrus cloud occurs more frequently at <inline-formula><mml:math id="M194" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45 <inline-formula><mml:math id="M195" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C than at other
temperatures over Beijing, and cirrus clouds in spring are the most frequent
among the four seasons.</p></list-item></list></p>
      <p id="d1e3069">The PDFs of reflectivity for cirrus cloud with respect to various
temperatures were also investigated. It was found that the PDFs in the four
seasons illustrate striking differences. A preliminary analysis indicates
that cirrus clouds with mean reflectivity lower than <inline-formula><mml:math id="M196" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>34 dBZ are likely to
be of the in situ-origin type. Most cirrus clouds are of the in situ-origin type in winter
and autumn; the in situ-origin cirrus clouds are more frequent than
liquid-origin cirrus clouds in spring, while summer features more
liquid-origin cirrus clouds. It should be noted that the current analysis and
results might have limitations due to the KPDR's limited ability to identify
possible supercooled layers in clouds. In our recent work (Huo
et al., 2020), the cirrus clouds are separated into three types via
cloud-base temperature to study their particle reflectivity and movements,
since there are differences among previous studies in the knowledge of the
temperature range of cirrus clouds. Besides seasonal variation, cirrus
clouds with different cloud-base temperatures also have different
microphysical characteristics. In future work, we intend to further
investigate the formation mechanisms of cirrus clouds in Beijing, as well as
in other areas, for the purposes of parameterization in GCMs and the
development of a locally adaptive <inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–IWC relationship.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <?pagebreak page14390?><p id="d1e3094">The ERA5 hourly data on pressure levels from 1979 to the present are available through the Copernicus Climate Change Service (<ext-link xlink:href="https://doi.org/10.24381/cds.bd0915c6" ext-link-type="DOI">10.24381/cds.bd0915c6</ext-link>, Hersbach et al., 2018). The AHI cloud property research product (produced from Himawari-8) that was used in this paper was supplied by the P-Tree System, Japan Aerospace Exploration Agency (<uri>https://www.eorc.jaxa.jp/ptree/userguide.html</uri>; Bessho et al., 2016.). The radar data used here are available by special request to the corresponding author (huojuan@mail.iap.ac.cn).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3106">JH designed the study and carried it out. YT, CH,
XW, YB, DL, SD and BL prepared some of the datasets. JH prepared the manuscript with contributions from all co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3112">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3118">We appreciate the valuable suggestions and insightful
instructions from the reviewers. We also thank the ECMWF ERA5 and AHI
science teams for sharing their product datasets. We also acknowledge our
Ka-radar team for their maintenance service during long-term measurements
that made our research possible.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3123">This research has been supported by the National Natural Science Foundation of China (grant no. 41775032).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3129">This paper was edited by Martina Krämer and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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<abstract-html><p>The physical properties and radiative role of ice clouds
remain one of the uncertainties in the Earth–atmosphere system. In this
study, we present a detailed analysis of ice cloud properties based on 4 years of surface millimeter-wavelength radar measurements in Beijing, China,
where the summer monsoon from the ocean and the winter monsoon from the continent
prevail alternately, resulting in various ice clouds. More than 6300 ice
cloud clusters were studied to quantify the properties of ice clouds, such
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reference for parameterization and characterization in global climate
models. In addition, comparison between ice cloud clusters formed under the
summer monsoon and the winter monsoon indicates the different formation and
evolution mechanisms of cirrus clouds. Statistically, temperatures of more than
95&thinsp;% of ice radar bins are below −15&thinsp;°C and more than 80&thinsp;%
of ice clouds are above 7&thinsp;km. The dependence of the radar reflectivity of
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indicating that the reflectivity of ice bins increases (decreases) as the
temperature (height) increases. In addition, it is found that there is a
strong linear relationship between the mean reflectivity and the ice cloud
depth. Due to various synoptic circumstances, the ice clouds in summer are
warmer, higher and thicker, with larger reflectivity than that in winter;
in particular, the mean cloud-top height of ice clouds in summer is 2.2&thinsp;km
higher than that in winter. Our analysis indicates that in spring, in situ-origin
cirrus clouds are more common than liquid-origin cirrus clouds, while in summer
liquid-origin cirrus clouds are more frequent; in autumn and winter, most cirrus
clouds are of in situ origin.</p></abstract-html>
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