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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 GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-15-12065-2015</article-id><title-group><article-title>The regional distribution characteristics of aerosol optical depth
over the Tibetan Plateau</article-title>
      </title-group><?xmltex \runningtitle{The regional distribution characteristics of AOD}?><?xmltex \runningauthor{C. Xu et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3 aff4">
          <name><surname>Xu</surname><given-names>C.</given-names></name>
          <email>xuchao@itpcas.ac.cn</email>
        <ext-link>https://orcid.org/0000-0003-1242-556X</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3 aff4">
          <name><surname>Ma</surname><given-names>Y. M.</given-names></name>
          <email>ymma@itpcas.ac.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>You</surname><given-names>C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Zhu</surname><given-names>Z. K.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Key Laboratory of Tibetan Environment Changes and Land
Surface Processes, Institute of Tibetan Plateau Research,<?xmltex \hack{\newline}?> CAS Center for
Excellence in Tibetan Plateau Earth Sciences, Chinese Academy of Sciences,
Beijing 100101, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>University of Chinese Academy of Sciences, Beijing
100049, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Qomolangma Station for Atmospheric Environmental
Observation and Research, Chinese Academy of Sciences,<?xmltex \hack{\newline}?> Dingri 858200, Tibet,
China</institution>
        </aff>
        <aff id="aff4"><label>a</label><institution>now at: Institute of Tibetan Plateau Research, CAS Center for Excellence in Tibetan Plateau Earth Sciences, Chinese Academy of Sciences, Beijing, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Y. M. Ma (ymma@itpcas.ac.cn) and C. Xu
(xuchao@itpcas.ac.cn)</corresp></author-notes><pub-date><day>30</day><month>October</month><year>2015</year></pub-date>
      
      <volume>15</volume>
      <issue>20</issue>
      <fpage>12065</fpage><lpage>12078</lpage>
      <history>
        <date date-type="received"><day>4</day><month>May</month><year>2015</year></date>
           <date date-type="rev-request"><day>11</day><month>June</month><year>2015</year></date>
           <date date-type="rev-recd"><day>17</day><month>October</month><year>2015</year></date>
           <date date-type="accepted"><day>23</day><month>October</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>


      <abstract>
    <p>The Tibetan Plateau (TP) is representative of typical clean atmospheric
conditions. Aerosol optical depth (AOD) retrieved by the Multi-angle Imaging
SpectroRadiometer (MISR) is higher over Qaidam Basin than the rest of the TP
throughout the year. Different monthly variation patterns of AOD are observed over
the southern and northern TP, whereby the aerosol load is usually higher in
the northern TP than in the southern part. The aerosol load over the northern
part increases from April to June, peaking in May. The maximum concentration
of aerosols over the southern TP occurs in July. Aerosols appear to be more
easily transported to the main body of the TP across the northern edge rather
than the southern edge. This is maybe partly because the altitude is lower
at the northern edge than that of the Himalayas located along the southern
edge of the TP. Three-dimensional distributions of dust, polluted dust,
polluted continental aerosol and smoke are also investigated, based on Cloud-Aerosol
Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) data. Dust is
found to be the most prominent aerosol type on the TP, and other types of
aerosols affect the atmospheric environment slightly. A dividing line of
higher dust occurrence in the northern TP and lower dust occurrence in the
southern TP can be observed clearly at an altitude of 6–8 km above sea level,
especially in spring and summer. This demarcation appears around
33–35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the middle of the plateau, and it is possibly
associated with the high-altitude terrain in the same geographic location.
Comparisons of CALIPSO and MISR data show that the vertical dust occurrences
are consistent with the spatial patterns of AOD. The different seasonal
variation patterns between the northern and southern TP are primarily driven
by atmospheric circulation, and are also related to the emission
characteristics over the surrounding regions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The Tibetan Plateau (TP), located in central eastern Eurasia, is the most
prominent and complex terrain feature on the Earth. It has the world's
highest average elevation (about 4000 m), with some surface features even
reaching into the mid-troposphere (Fig. 1). The TP is surrounded by several
deserts, including the Taklamakan Desert in the Tarim Basin, Gobi Desert and the
deserts in southwest Asia and the Middle East. The Indo-Gangetic Plain is located
to the south of the TP, with high aerosol loading (Gautam et al., 2011). Several
mountains are located on the TP, including the Himalayas, Gangdise, Nyainqêntanglha, Tanggula and Kunlun mountains.
The elevation differences of these mountains are at least 500 m and usually
1000 m or even more compared with the surrounding areas. Due to its
topographic characteristics, the TP surface absorbs high quantities of solar
radiation with corresponding impacts on surface heat or water fluxes (Ma et
al., 2014a, b). The east Asian monsoon and the eastern part of the south
Asian monsoon systems are mainly controlled by the thermal forcing of the TP
(Wu et al., 2007, 2012).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>The topography (in meters) of the Tibetan Plateau and main mountain
ranges on the Tibetan Plateau.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f01.png"/>

      </fig>

      <p>Many studies have focused on environmental and climate change over the TP (Xu
et al., 2009; Ma et al., 2011; Lin et al., 2012; Yao et al., 2012; Sheng et
al., 2013), and the TP environment is greatly affected by natural and
anthropogenic aerosols from the surrounding regions (Z. Liu et al., 2008;
Bucci et al., 2014; Cong et al., 2015). Therefore, studying tropospheric
aerosols and their effects on the TP is of great importance (King et al.,
1999; Kaufman et al., 2002; Li et al., 2011). Vernier et al. (2011) reported
the presence of an aerosol layer at the tropopause level above Asia during
the monsoon season. The Taklamakan and Gobi deserts are two major dust
sources with long-range transport mainly occurring in spring (D. Liu et al.,
2008). Summertime Tibetan airborne dust plumes were detected from the
Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO)
satellite (Huang et al., 2007), and Xia et al. (2008) suggested that the
aerosol load in summer over the TP was mainly associated with the Taklamakan
Desert. Dust above the TP appears to be largely related to source regions to
the north and on the eastern part of the TP (Z. Liu et al., 2008). The impact
of aerosols above and around the TP during pre-monsoon season was also
investigated; however, a strong elevated heating which could influence
large-scale monsoonal circulations was not found (Kuhlmann and Quaas, 2010).
Atmospheric brown clouds over south Asia, resulting from biomass burning and
fossil fuel consumption, are recognized as a serious environmental problem
(Ramanathan et al., 2005). These carbonaceous aerosols lead to a large
reduction of solar radiation at the surface, an increase of solar heating in
the atmosphere and a weaker hydrological cycle (Ramanathan et al., 2001).
Anthropogenic emissions from strong pollution events can occasionally be
transported to the central TP by prevailing southwesterly winds (Xia et al.,
2011). The high altitudes of the Himalayas appear to block most BC particles
intruding into the TP, but the Yarlung Tsangpo River valley serves as a
“leak” by which contaminants can reach the southeast TP (Cao et al., 2010).
Results from precipitation isotope observations revealed that the northward
maximum extent of the southwest monsoon over the Tibetan Plateau is located
around 34–35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N (Tian et al., 2007). The southern and northern TP
are under the control of different climate systems during the monsoon season
(Yao et al., 2013). Some previous studies have indicated that the southern and
northern TP possibly present different variations in aerosol properties,
e.g., different temporal variations in dust storm records (Wu et al., 2013).
However, the mechanisms of those differences still need further study.</p>
      <p>Although the aerosol load is relatively low, aerosols over the TP have
unique characteristics. In this study, the seasonal variations and spatial
distributions of aerosols over the TP are presented based on the Multi-angle
Imaging SpectroRadiometer (MISR) data. The seasonal vertical distributions
of dust, polluted dust, polluted continental aerosol and smoke are also
investigated using CALIPSO data. This study might indicate that a natural
demarcation of aerosols between the northern and southern TP exists in the
middle of the plateau. In addition to that, the spatial patterns of aerosol loading
are consistent with the vertical distributions of aerosols. We preliminarily
propose the possible mechanisms for the aerosol distributions.</p>
</sec>
<sec id="Ch1.S2">
  <title>Data and methodology</title>
      <p>The MISR was successfully launched into Sun-synchronous polar orbit aboard
Terra, NASA's first Earth Observing System (EOS) spacecraft, on
18 December 1999. Viewing the sunlit Earth simultaneously at nine
widely spaced angles, MISR provides radiometrically and geometrically
calibrated images in four spectral bands at each of the angles. MISR observes
the entire Earth about once per week. The spatial resolution of the
operational MISR aerosol retrieval algorithm is 17.6 km <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 17.6 km.
The retrieval region has 16 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 16 subregions, and each subregion
covers a 1.1 km <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.1 km area. One of the key issues for satellite
aerosol products is cloud contamination, including MISR data (Kahn et al.,
2010). Three cloud-mask products are used in the aerosol preprocessing. The
MISR standard products include three separate MISR-derived cloud masks:
Radiometric Camera-by-camera Cloud Mask (RCCM) (Yang et al., 2007),
Stereo-Derived Cloud Mask (SDCM) (Moroney et al., 2002) and Angular-Signature
Cloud Mask (ASCM) (Di Girolamo and Wilson, 2003). Based on collocated MISR
and Moderate Resolution Imaging Spectroradiometer (MODIS) data, Shi et
al. (2014) suggested that cloud contamination existed in both over-water and
over-land MISR AOD data, with heavier cloud contamination occurring over the
high-latitude southern hemispheric oceans. MISR aerosol retrievals have been
evaluated by many studies (Martonchik et al., 2004; Kahn, 2005; Witek et al.,
2013). The accuracy of MISR AOD was much better than MODIS AOD over land
(Abdou et al., 2005). Xia et al. (2008) made comparisons of MISR AOD with
ground-based hazemeter measurements made at Lhasa and Haibei stations on the
TP, which showed a high correlation coefficient and a low root-mean-square error.
The Level 3 aerosol product is a summary of the Level 2 aerosol product. In
this study, daily Level 3 MISR aerosol data from March 2000 to December 2014
are used to investigate the aerosol spatial distribution, and the spatial
resolution of MISR data is 0.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>
      <p>Monthly variations of AOD at 558 nm are analyzed over the TP. If there was
only one satellite observation for a month then this grid value in that
particular month was excluded for that year, since there would be too few
observations to represent the monthly average. The monthly means that
represent the aerosol long-term distribution are calculated by averaging the
observation data for that month in each year. To analyze aerosol zonal
average, only aerosol retrievals over the TP (27–40<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
75–105<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) at elevations higher than 3000 m are used. In this
study, the northern part of the TP is defined as the region north of
33–34<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, and the southern part of the TP is defined as the region
south of 33–34<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. The reason for selecting 33–34<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N is
based on the distributions of aerosols, which appear to show different
patterns to the north and south of this latitude.</p>
      <p>The Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation
(CALIPSO) satellite provides new insight into clouds and atmospheric aerosols
(Winker et al., 2007, 2010). The CALIPSO satellite was launched into a
Sun-synchronous orbit on 28 April 2006, with a 16-day repeating cycle. The
lidar Level 3 aerosol product is a quality-screened aggregation of Level 2
aerosol profile data. A series of filters are designed to eliminate samples
and layers that were detected or classified with very low confidence or that
have untrustworthy extinction retrievals (Winker et al., 2013). The CALIPSO
version 1.00 and version 1.30 Level 3 aerosol profile data from March 2007 to
February 2015 are used in this study. Nighttime all-sky data are used,
because the instrument is more sensitive during nighttime than daytime
without solar background illumination (Winker et al., 2013). The spatial
resolution of Level 3 data is 5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
(longitude–latitude), and the vertical resolution is 60 m observed from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.5 to 12 km above sea level (a.s.l.; all altitudes hereafter also refer to
a.s.l.
where no other specification is given) in the troposphere. The primary variable of
aerosol type is used, and this variable counts the number of aerosol samples
of each aerosol type for each latitude/longitude/altitude grid cell. Six
aerosol types including clean marine, dust, polluted continental aerosol, clean
continental aerosol, polluted dust, and smoke are classified. From the data product
descriptions, the composition of six aerosol types can be known. Clean marine
is a hygroscopic aerosol that consists primarily of sea salt (NaCl). Dust is
mostly mineral soil. Polluted continental aerosol is background aerosol with a
substantial fraction of urban pollution. Clean continental aerosol is a lightly
loaded aerosol consisting of sulfates (SO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, nitrates
(NO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, organic carbon (OC) or ammonium (NH<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Polluted dust
is a mixture of desert dust and smoke or urban pollution. Smoke aerosol
consists primarily of soot and OC. Mixtures of two aerosol types are not
assigned to one aerosol sample. Dust, polluted dust, polluted continental aerosol and
smoke possibly influence the TP (Kuhlmann and Quaas, 2010). The aerosol
samples for these major types in each season were calculated by accumulating
the detected samples for the season in each latitude/longitude/altitude grid
cell. The multi-year aerosol samples for each season are obtained by averaging
across multiple years. The classification algorithms use the integrated
attenuated backscatter measurements, the volume depolarization ratio
measurements, surface type and layer altitude to determine aerosol type (Omar
et al., 2009). The similarity of the optical properties between polluted
continental aerosol and smoke makes the classification of these two aerosol
types difficult (Omar et al., 2009). Mielonen et al. (2009) made comparisons
of Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) Level 2 aerosol
types and those derived from Aerosol Robotic Network (AERONET) inversion
data. The results revealed the greatest agreement for the dust type (91 %
of the cases), moderate agreement for the polluted dust type (53 % of the
cases), and poorer agreement for smoke (37 % of the cases) and for
polluted and clean continental aerosol combined (22 % of the cases). Burton et
al. (2013) made comparisons of aerosol types between CALIPSO and airborne
High Spectral Resolution Lidar, which showed the best agreement for desert
dust (80 % of the cases) and marine aerosols (62 % of the cases),
moderate agreement for the polluted continental aerosols (53 % of the
cases), but relatively poor agreement for polluted dust (35 % of the
cases) and smoke (13 % of the cases). Although previous studies showed
different results of quantitative validations, these research studies indicated that the
classifications for dust aerosols were reliable. Moreover, it is necessary to
state that the classifications of smoke aerosols presented here are subject
to large uncertainty. There are uncertainties associated with incorrect
aerosol type classification, and these uncertainties further affect aerosol
extinction. Aerosol extinction coefficients are not analyzed due to
values that are too low, with high uncertainties over the TP. In this study, four common
seasons are defined, respectively, as March to May (spring), June to August
(summer), September to November (autumn) and December to February the following
year (winter).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Monthly variations of AOD over the Tibetan Plateau. White shading
indicates insufficient available data.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f02.png"/>

      </fig>

      <p>The meridional circulations are examined using ERA-Interim monthly mean
reanalysis data, produced by the European Centre for Medium-Range Weather
Forecasts (ECMWF). The spatial resolution of ERA-Interim reanalysis data is
0.75<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.75<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, and the vertical layers at 32
different pressure levels are used (i.e., 1000, 975, 950, 925, 900, 875,
850, 825, 800, 775, 750, 700, 650, 600, 550, 500, 450, 400, 350, 300, 250,
225, 200, 175, 150, 125, 100, 70, 50, 30, 20, 10 hPa). Data are analyzed
from March 2000 to February 2014.</p>
</sec>
<sec id="Ch1.S3">
  <title>Results and analysis</title>
<sec id="Ch1.S3.SS1">
  <title>Aerosol distribution characteristics</title>
      <p>Monthly variations of AOD over the Tibetan Plateau are shown in Fig. 2.
Seasonal variations of AOD are significant. The monthly average of AOD for
the <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15-year study period was less than <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.50 over the whole
TP in spring and summer, but less than 0.25 in autumn and winter. The highest
AOD is shown over the Qaidam Basin on the TP in each month. Frequent dust
storms mainly lead to the high AOD (Zhang et al., 2003; Wang et al., 2004).
Human activities, including those such as fossil fuel combustion and industrial
emissions over the Qaidam Basin, also contribute to the increasing aerosol
concentrations to some extent (Streets et al., 2003; Zhang et al., 2009; Liu
et al., 2015). The aerosol load increases gradually from March to May over
the northern part of the TP, while it decreases from June to August. The
areas with higher aerosol loads (<inline-formula><mml:math display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.25) expand gradually in April and
reach their maximum extent in May, which indicates that AOD is highest in May. AOD
is higher to the north of 33–34<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N than to the south for the whole year.
The east–west-trending mountains on the TP seem to act as a major natural
barrier for the transport of atmospheric aerosols from north to south. The
aerosol load increases slightly to the south of 30<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in summer. The
aerosol load over the southern TP may be associated with the Indo-Gangetic
Plain. A possible explanation of this phenomenon may be the peaks in
anthropogenic emissions in the Indo-Gangetic Plain during summer coupled
with suitable atmospheric circulation. Alpine valleys along the Himalayas
(e.g., the Pulan Valley in the western Himalayas and the Yadong Valley in the
middle Himalayas) may act as channels along which aerosols can be transported
into the southern part of the TP during the monsoon season. In autumn and
winter, AOD over the whole TP is mostly lower than 0.20, except in the Qaidam
Basin. AOD even decreases below 0.10 over most regions of the TP from
November to January. Unfortunately, AOD over the southeast TP cannot always
be determined in each season due to thick cloud.</p>
      <p>In summary, AOD is usually higher over the Qaidam Basin than over the other
parts of the TP, throughout the year. Obvious seasonal variations of AOD are
observed over the TP. Dust or anthropogenic emissions may pass through the
northern edge of the TP, especially the Qaidam Basin, to intrude into the
TP.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Zonal variations in aerosol properties over the TP</title>
      <p>Although the aerosol load is quite low over the TP, the zonal distribution
pattern can be seen clearly. Figure 3 shows the zonal monthly means of AOD
for a period of over 15 years. Monthly variations in the northern TP are
different from those in the southern TP. The aerosol load is relatively high
over the northern TP during April to June, while it is high over the southern
TP during June to August. Single monthly peak occurs over both the northern
and southern TP. The monthly peak is observed in May and July, respectively.
Moreover, the monthly zonal peak of AOD in the northern TP is about 1.5 times
that in the southern part. Previous studies showed similar results based on
surface observations (Gobbi et al., 2010; Xu et al., 2014). The zonal means
over the whole TP are even below 0.10 during November to January.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Zonal average of AOD over the Tibetan Plateau in each month. White
shading indicates insufficient available data.</p></caption>
          <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f03.png"/>

        </fig>

      <p>Overall, AOD shows clear zonal distributions. Different monthly variation
patterns of AOD are shown in the northern part and southern part of TP. The
maximum aerosol concentration is observed during April to June to the region
north of 33–34<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, with maximum levels in May. Aerosols can be
clearly transported to the south of about 30<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N over the TP, with
maximum levels in July.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Vertical distributions of aerosols</title>
      <p>Dust, polluted dust, polluted continental aerosol and smoke retrieved by CALIPSO are
the major aerosol types, possibly influencing the environment over the TP.
The seasonal vertical distributions of these aerosol types are discussed
in relation to the latitudinal transects. The regions from 80 to 100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E
covering most of the TP are selected to represent aerosol three-dimensional
distributions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>The detected accumulated dust samples for four seasons over the
Tibetan Plateau and surrounding areas for four longitudinal transects
(80–85, 85–90, 90–95 and 95–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). Black areas represent
mountain profiles along the transects. MAM denotes March to May, JJA denotes
June to August, SON denotes September to November and DJF denotes December to
February the following year (the following season divisions are the same).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f04.png"/>

        </fig>

      <p>Figure 4 shows latitudinal transects of accumulated dust samples in each
season. The features of aerosol three-dimensional distributions can be
concluded to seasonal variability and spatial differences. Dust generation
and lofting is always active over the Tarim Basin and Hexi Corridor all
year around, while dust occurs frequently over the northern Indian peninsula
only in spring. Detected dust over the TP increases significantly in spring
and summer, and dust occurs much less frequently in autumn and winter. This
phenomenon possibly indicates that dust can be transported into the TP in
spring and summer, while dust only occurs in Qaidam Basin in autumn and
winter. Much less dust is detected on-plateau than off-plateau, which
indicates that the TP acts as a large barrier for the transport of dust.
Furthermore, dust occurrence decreases from the surface to the high altitude
over the TP. Most Tibetan airborne dust is concentrated at a height of
less than 7 km during spring and summer. Obvious differences of detected
dust exist between the southern and northern TP in spring and summer. Dust
occurs more frequently over the northern part of TP than the southern part.
The demarcation between high dust occurrence over the northern TP and
relatively low dust occurrence over the southern TP is clear along each
longitudinal cross section. The demarcation runs east to west across the TP,
which appears to be in accord with the distributions of monthly MISR AOD.
After climbing the northern edge of the TP, dust reduces substantially. The
extreme high mountains over the TP include the Kunlun and the Tanggula. When
dust encounters these major mountains one by one, the detected dust aerosols
passing through the mountains decrease gradually along the longitudinal zones
from north to south in each season. The dust layer has the greatest depth
over all the longitudinal zones in spring, followed by summer. In spring,
dust layer extends from the surface to 11–12 km over the TP. Dust can be
generated and lofted to a similar altitude over the Tarim Basin and Hexi
Corridor in spring, whereas the dust layer exhibits a lesser thickness and
extends to 6–8 km over the northern Indian peninsula. The detected aerosol
layer even reaches up to upper troposphere and lower stratosphere over the TP
and the regions north of the TP. Frequent dust activities and little
precipitation may be favorable for dust intrusion in stratosphere.
Stratosphere–troposphere exchange is currently a widely studied topic, and
aerosols intruding into the stratosphere will lead to a negative radiative
forcing (Solomon et al., 2011). Previous studies have mainly focused on deep fast
convective transport of polluted air from the atmospheric boundary layer into
the upper troposphere and lower stratosphere during Asian summer monsoon
season (Fu et al., 2006; Randel et al., 2010). The non-volcanic aerosol layer
near the tropopause was detected vertically from 13 to 18 km based on
CALIPSO observations during the Asian summer monsoon, and AOD here has
increased 3 times since the late 1990s (Vernier et al., 2015). However, our
results suggest the TP and the regions north of the TP may also act as
alternative pathways for aerosols from the troposphere to the stratosphere during the
spring period. The mechanisms of spring dust transport from the atmospheric
boundary layer into the upper troposphere and lower stratosphere need further
rigorous studies and discussions. The demarcation of dust occurrence between
the northern and southern TP can be seen clearly from the surface to a height of
about 6–8 km during spring, while it becomes unapparent at high altitudes.
The dust layer can only extend to the altitudes of 8–10 km over the TP during
summer, and the demarcation appears to be obvious at an altitude of less than
7 km. This phenomenon may indicate that dust seems to be transported more easily
through the northern edge of TP than the southern edge during spring and
summer. The dust layer is usually at altitudes of less than 8 km over the TP in
autumn and winter. Due to low dust occurrence, the differences of detected
dust between the northern and southern TP are not obvious in autumn and
winter.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><caption><p>The detected accumulated polluted dust samples for four seasons over
the Tibetan Plateau and surrounding areas for four longitudinal transects
(80–85, 85–90, 90–95 and 95–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). Black areas represent
mountain profiles along the transects.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f05.png"/>

        </fig>

      <p>Figure 5 shows latitudinal transects of accumulated polluted dust samples in
each season. Polluted dust also affects the environment of the TP.
Nevertheless, the effect of polluted dust is not as significant as dust over
the TP. High occurrence of polluted dust is observed over the northern Indian
peninsula, except in summer, possibly due to large precipitation. The
occurrence of polluted dust is higher than dust over the northern Indian
peninsula except in spring. The polluted dust is confined to the lower 5 km
of the atmosphere over the northern Indian peninsula in spring and summer,
while polluted dust is concentrated at a height of less than 4 km in autumn
and winter. The maximum height seems to be crucial to the long-range
transport of polluted dust, considering that it is comparable to or lower
than the altitude of the TP. Polluted dust cannot be transported onto the TP,
when its maximum height is lower than the southern edge. Polluted dust also
occurs to the north of the TP, but the effect is not obvious. Polluted dust
decreases dramatically on-plateau relative to off-plateau regions. Only a
small amount of polluted dust can be detected over the TP, and the number of
polluted dust samples is a bit larger in spring and summer than in autumn and
winter. The polluted dust layer also exhibits a relatively greater thickness
over the TP in spring and summer. Differences of occurrence between the
northern and southern part of TP also seem to be unapparent. Polluted dust
rarely occur in autumn and winter, especially along the longitudinal cross
section of 80–85, 85–90 and 90–95<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6" specific-use="star"><caption><p>The detected accumulated polluted continental samples for four
seasons over the Tibetan Plateau and surrounding areas for four longitudinal
transects (80–85, 85–90, 90–95 and 95–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). Black areas
represent mountain profiles along the transects.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f06.png"/>

        </fig>

      <p>Figure 6 shows latitudinal transects of accumulated polluted continental
samples in each season. Much less polluted continental samples are detected
relative to dust or polluted dust over the study regions. This result does
not mean that there is less urban air pollution in essence. Urban pollution
mixed with dust is classified as polluted dust. Polluted continental
aerosols seem to happen more frequently in autumn and winter over the
northern Indian peninsula. Polluted continental aerosols hardly have any
impact on the TP in each season.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>The detected accumulated smoke samples for four seasons over the
Tibetan Plateau and surrounding areas for four longitudinal transects
(80–85, 85–90, 90–95 and 95–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). Black areas represent
mountain profiles along the transects.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f07.png"/>

        </fig>

      <p>Figure 7 shows latitudinal transects of accumulated smoke samples in each
season. Smoke consisting of soot and OC can be transported to the main body
of the TP. More smoke samples are detected over the Indo-Gangetic Plain
rather than the areas north of the TP. The altitude of smoke aerosol layer is
higher in summer than other seasons over the Indo-Gangetic Basin. Although the
heavy summer rains remove a large amount of soluble gases and aerosols, less-soluble species can be lifted to the upper troposphere in deep convective
clouds and then be transported away from the Indo-Gangetic Plain by strong upper
tropospheric winds. In spring, few smoke samples are detected above the TP,
and do not show a continuous vertical distribution. This indicates that smoke
released during big fires can be occasionally uplifted above the atmospheric
boundary layer and further transported to the TP. Detected smoke samples
increase lightly over the TP during summer, and they are also not continuous
in column. Although smoke does not occur during summer as frequently as
autumn or winter over the northern Indian peninsula, strong southerly winds
blow towards the TP only during summer. Smoke can even suspend at an altitude
of 12 km over the TP in summer. Detected smoke samples are a bit higher in
the central TP in summer, which may be due to local emission. Detected smoke
samples decrease again in autumn, and smoke usually occurs less than 7 km
over the TP. Smoke occurrence is a bit higher in the southern part of the TP
than the northern part in summer and autumn. Smoke appears to be more likely
transported from the northern Indian peninsula to the TP in summer and
autumn, because higher occurrence of smoke is shown in the adjacent regions
of the southern edge. No smoke samples are detected over the TP in winter.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p>The meridional circulation at 95<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E in the four seasons.
The black shading shows the altitudes of the Tibetan Plateau at
95<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f08.png"/>

        </fig>

      <p>In summary, pure dust is found to be the main aerosol type above the TP, and
dust mixed with pollution or smoke occasionally occurs. Smoke only has a
little effect on the TP in summer, while urban pollution does not contaminate
the environment of the TP individually. Much fewer aerosols are detected
on-plateau than off-plateau, which indicates that the TP acts as a natural
barrier. Dust and polluted dust exhibit more thickness in spring and summer
above the TP. The bulk of dust is concentrated at a height of less than 7 km
during spring and summer. Different dust occurrences between the northern and
southern TP can be found clearly in spring and summer. No significant
differences are found in the occurrences of polluted dust, smoke or polluted
continental aerosols over the northern and southern TP. Smoke aerosols may be
more likely to come from the northern Indian peninsula in summer.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Possible factors contributing to the aerosol distribution pattern</title>
      <p>The TP has quite pristine atmospheric conditions; that is to say, few
aerosols come from local contributions. Zhang et al. (2015) showed that local
emissions contributed only a small percentage of BC in the Himalayas and
Tibetan Plateau. There are no obvious sources of biomass burning on the TP
(Mouillot and Field, 2005). As the most prominent aerosol type on the TP,
airborne dust on the TP mostly comes from the surrounding regions. A negative
or significant negative relationship between AOD and wind speed was found
over most regions of the TP based on previous results (Ge et al., 2014).
Therefore, long-range transport of aerosols primarily impacts the atmospheric
environment over the TP, and this study is not focused on the contribution of
inner sources on the TP. The aerosol load has significant seasonal
variations. Interestingly, the pattern of seasonal variations over the
northern TP is different to that of the southern part; this could be due to
many factors, including the emission sources, high-altitude terrain and
atmospheric circulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>Spatial distribution of wind at 500 hPa over the Tibetan Plateau in
the four seasons.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/12065/2015/acp-15-12065-2015-f09.png"/>

        </fig>

      <p>Much higher aerosol loads are observed over the surrounding regions of the
TP. AOD peaks during spring and summer over Tarim Basin. Strong anticyclonic
wind anomaly at 500 hPa and enhanced easterly wind at 850 hPa over the
Tarim Basin during spring and summer are good for dust entrainment, vertical
lofting, and horizontal transport (Ge et al., 2014). The Indo-Gangetic Basin,
encompassing most of northern India peninsula, extends from Pakistan in the
west to Bangladesh in the east. The Indo-Gangetic Basin is one of the most
heavily populated regions of the world. There are a large quantity of
emissions of biomass burning and fossil fuel over south Asia, adjacent to the TP (Ramanathan et al., 2005). AOD over the Indo-Gangetic
Basin can reach extremely high values throughout the year, peaking during
spring and summer due to enhanced emission of natural aerosols (Dey and Di
Girolamo, 2010). Furthermore, aerosol layers exist above the TP over the
northern Indian peninsula and Tarim Basin during spring and summer. Dust and
polluted dust layers exhibit a relatively greater thickness over the regions
north of the TP than the regions south of the TP during spring and summer.
The aerosol concentrations and the heights of aerosol layers over the
surrounding regions have a great influence on the transport of aerosols.</p>
      <p>The high terrain acts as a natural barrier for the transport of atmospheric
aerosols from the surrounding polluted regions to the main body of the TP due
to its topographic characteristics. Therefore, AOD over the TP is much lower
than that of surrounding regions, such as the Taklamakan Desert and the
Indo-Gangetic Plain. The aerosol distributions are impacted by the mountain
ranges on the TP. The high aerosol load occurring over the northern part
seems to be associated with lower altitudes, and a relatively low aerosol
load along the southern edge seems to be associated with the higher
altitudes. The aerosol layer firstly needs to be present higher than the TP
elevation, which is a requirement for aerosol transport to the TP. The
southern edge is much higher than the northern edge of the TP. The transport
of aerosols from north of the TP seems easier than from south of the TP.
Aerosols may only pass through alpine valleys along the Himalayas to intrude
into the TP, while a broader northeastern edge – especially the Qaidam Basin
– seems to provide transmission channels. When aerosols pass across the
northern edge, the major natural obstacles they encounter are several
mountains. The Kunlun and the Tanggula mountains act as barriers which block
aerosols. It is then difficult for aerosols to spread further southward. The
Gangdise and the Nyainqêntanglha mountains are located around
30–31<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N on the southern TP. These mountains possibly act as a
natural barrier for aerosols passing across the southern edge, and curb the
spread of pollution further northward to the main body of the TP. The
demarcation extending to 6–8 km seems to exist only in dust aerosols, while
it is not apparent in other types of aerosols due to their small amounts. The
high-altitude terrain located around 33–35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the middle of the
plateau appears to be geographically identical to this natural demarcation.
Not only does the whole TP block the atmospheric aerosols, but also the
extreme high mountains on the TP cause an obstruction to the transport of
aerosols.</p>
      <p>Atmospheric circulation also greatly impacts the seasonal aerosol variations.
Figure 8 shows the annual average vertical wind fields, and Fig. 9 shows the wind
vector field at 500 hPa. A longitude of 95<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, corresponding to the
Qaidam Basin, is chosen to analyze the vertical atmospheric circulations.
During the spring period, the northern air flows and southern air flows
intersect at about 31–32<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N over the TP. Aerosols above the TP are
mostly from the northern side of the TP in spring, and aerosols originating
from the Indo-Gangetic Basin may only affect the area south of 31–32<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N on
the TP. Northwesterly and westerly winds at 500 hPa prevail over the
Indo-Gangetic Plain during spring. Although high aerosol load occurs and
aerosol layer exists at 5 km during spring, this atmospheric circulation
does not benefit to the transport of air pollutants from the northern India
to the TP. Kuhlmann and Quaas (2010) reported that around 40 % of
elevated desert dust or polluted dust from Iran and Pakistan can be advected
towards the southern slope of TP. During summer, the airflows originating
from both the northern and southern sides of the TP carry aerosols to the
main body of the TP. The Indo-Gangetic Basin is dominated by a cyclonic
circulation system at 500 hPa. In addition, vertical circulation indicates
strong updrafts below 200 hPa to the south of the TP. Updrafts are also
shown on the whole TP. With the summer monsoon developing, the southwesterly
winds at 500 hPa reach the northward maximum extent over the TP.
Furthermore, the northern atmospheric circulation system and south Asian
monsoonal system meet around 34–35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the middle of the TP. The
atmospheric circulation promotes the transport of aerosols from the Tarim
Basin, Qaidam Basin and Indo-Gangetic Basin to the main body of the TP. It
might be reasonably deduced that atmospheric circulation possibly leads to
the formation of different seasonal variation patterns of aerosols between the
northern and southern TP. Dust particles coated by pollution acids can
provide the predominant source of cloud condensation nuclei (Ma et al.,
2010). Urban emissions consisting of hygroscopic compounds could be deposited
by heavy precipitation and reduce substantially over the northern Indian
peninsula. Some less-soluble species can be lifted to the upper troposphere
in deep convective clouds and then be transported to the TP by strong upper
tropospheric winds. The strong southwesterly winds can provide the dynamical
conditions for the transport of aerosols during monsoon season, which leads to
the highest aerosol load occurring in July over the southern TP. The aerosol
particles continue to reduce drastically after passing through the Himalayas
Mountains due to the physical blocking. Consequently, the aerosol loading and
occurrences are still higher in the northern TP than the southern TP during
summer. Seasonal variations of atmospheric circulations lead to the
relatively higher aerosol loads in spring and summer on the TP. During
autumn, southwesterly winds mainly prevail south of 31–32<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N at
500 hPa on the TP with the retreat of monsoon. During the winter period,
wind fields are similar to autumn but with higher wind velocities. Westerly
winds at 500 hPa gradually prevail over the Indo-Gangetic Basin from autumn
to winter. Moreover, our results reveal that the aerosol layer usually exists
at an altitude of less than 4 km over the Indo-Gangetic Basin during autumn
and winter. Aerosols originating from Indo-Gangetic Basin cannot be lifted to
a height higher than the elevation of the southern edge during autumn and
winter. Conversely, some elevated dust aerosol layers higher than the
northern edge of the TP are observed north of the TP during autumn and
winter. It is difficult for aerosols transported from the Indo-Gangetic Basin to
the TP during autumn and winter seasons. Elevated dust aerosols from the north of
the TP can be possibly transported to the TP coupled with northward winds.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Concluding remarks</title>
      <p>This study identifies the patterns of aerosol variations over the TP using
the 15-year MISR data. Furthermore, the vertical distributions of dust,
polluted dust, polluted continental aerosols and smoke retrieved by 8-year
CALIPSO data are also investigated over the TP. The possible reasons for the
temporal variations and spatial distributions of aerosols are discussed.</p>
      <p>The aerosol load exhibits obvious seasonal variations over the investigated
regions, with higher AOD observed during spring and summer. Two different
kinds of seasonal patterns of AOD are observed over the TP. The maximum
monthly AOD over the northern TP occurs in May, while AOD over the southern
TP peaks in July. AOD shows much higher values over Qaidam Basin than other
parts of the TP throughout the year. Monthly AOD usually shows higher values
over the northern TP than the southern TP. Dust is found to be the major
aerosol type above the TP, while polluted dust and smoke aerosols slightly
affect the atmospheric environment on the TP. Therefore, the seasonal
variation and spatial pattern of aerosol load are largely associated with
dust occurrence. Both the occurrence and the thickness of airborne dust also
reach maximums over the TP in spring. The dust layer over the TP can reach up to
the upper troposphere and lower stratosphere in spring (altitudes of
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 11–12 km), while the altitude of dust layer is much lower in other
seasons. Higher dust occurrence in the northern TP and lower dust occurrence
in the southern TP are observed during spring and summer. This dividing line
is located around 33–35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the middle of the plateau. In
addition, this demarcation extends from the surface to an altitude of
6–8 km. However, this demarcation is not observed in the distributions of
other aerosol types due to their low occurrences.</p>
      <p>The seasonal variations and distribution characteristics of the aerosol load
on the TP are possibly affected by many factors, including emission sources,
the height of aerosol layer, atmospheric circulation and the topography of
the TP. High concentrations of aerosols exist during spring and summer over
the surrounding regions including the Indo-Gangetic Basin and the Tarim Basin.
Furthermore, aerosol layers exist above the TP elevation during these two
seasons. These conditions are favorable for aerosol transport from the
surrounding regions to the TP. Different seasonal variations over the
northern and southern TP are closely associated with atmospheric circulation
system. Atmospheric circulations also greatly control the potential maximum
limit of aerosol transport. However, the actual distribution patterns of
aerosol are not completely consistent with the maximum extent of airflows.
The mountains on the TP may effectively block the transport of aerosols. It
is the possible reason that a dividing line of different dust occurrences
between the southern and northern TP exists in the middle of the TP during
spring and summer.</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>This research was funded by the Chinese Academy of Sciences (XDB03030201),
the National Natural Science Foundation of China (91337212, 41275010, 41375009), the
CMA Special Fund for Scientific Research in the Public Interest
(GYHY201406001) and EU-FP7 projects “CORE-CLIMAX” (313085). This study was also funded by the CAS “Hundred Talent” program (Weiqiang Ma). We would like
to thank the editor and two anonymous referees for their very valuable
comments greatly improving the paper. The MISR data were obtained from the
NASA Langley Research Center Atmospheric Science Data Center. The CALIPSO
data were obtained from the NASA Langley Research Center Atmospheric Science
Data Center. The ERA-Interim data were produced by ECMWF. The first author
would like to acknowledge Changgui Lin, You He and all the other group
members for their help in preparing the paper.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: H. Su</p></ack><ref-list>
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