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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-17-3083-2017</article-id><title-group><article-title>Enhanced trans-Himalaya pollution transport to the Tibetan Plateau by
cut-off low systems</article-title>
      </title-group><?xmltex \runningtitle{Enhanced trans-Himalaya pollution transport}?><?xmltex \runningauthor{R. Zhang et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Ruixiong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Wang</surname><given-names>Yuhang</given-names></name>
          <email>yuhang.wang@eas.gatech.edu</email>
        <ext-link>https://orcid.org/0000-0002-7290-2551</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2">
          <name><surname>He</surname><given-names>Qiusheng</given-names></name>
          <email>heqs@tyust.edu.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Chen</surname><given-names>Laiguo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Yuzhong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Qu</surname><given-names>Hang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Smeltzer</surname><given-names>Charles</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Li</surname><given-names>Jianfeng</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1091-9753</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Alvarado</surname><given-names>Leonardo M. A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4802-3872</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4 aff5 aff6">
          <name><surname>Vrekoussis</surname><given-names>Mihalis</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8292-8352</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Richter</surname><given-names>Andreas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3339-212X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Wittrock</surname><given-names>Folkard</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Burrows</surname><given-names>John P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1547-8130</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>School of Earth and Atmospheric Sciences, Georgia Institute of
Technology, Atlanta, GA, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>School of Environment and Safety, Taiyuan University of Science and
Technology, Taiyuan, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Urban Environment and Ecology Research Center, South China Institute
of Environmental Sciences (SCIES),<?xmltex \hack{\newline}?> Ministry of Environmental Protection
(MEP), Guangzhou, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute of Environmental Physics and Remote Sensing, University of
Bremen, Bremen, Germany</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Center of Marine Environmental Sciences – MARUM, University of
Bremen, Bremen, Germany</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Energy, Environment and Water Research Center (EEWRC), The Cyprus
Institute, Nicosia, Cyprus</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yuhang Wang (yuhang.wang@eas.gatech.edu) and Qiusheng He
(heqs@tyust.edu.cn)</corresp></author-notes><pub-date><day>28</day><month>February</month><year>2017</year></pub-date>
      
      <volume>17</volume>
      <issue>4</issue>
      <fpage>3083</fpage><lpage>3095</lpage>
      <history>
        <date date-type="received"><day>3</day><month>August</month><year>2016</year></date>
           <date date-type="rev-request"><day>28</day><month>September</month><year>2016</year></date>
           <date date-type="rev-recd"><day>20</day><month>December</month><year>2016</year></date>
           <date date-type="accepted"><day>1</day><month>February</month><year>2017</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>Long-range transport followed by deposition of black
carbon on glaciers of Tibet is one of the key issues of climate research
as it induces changes on radiative forcing and subsequently impacting the melting
of glaciers. The transport mechanism, however, is not well understood. In
this study, we use short-lived reactive aromatics as proxies to diagnose
transport of pollutants to Tibet. In situ observations of short-lived
reactive aromatics across the Tibetan Plateau are analyzed using a regional
chemistry and transport model. The model performance using the current
emission inventories over the region is poor due to problems in the
inventories and model transport. Top-down emissions constrained by satellite
observations of glyoxal are a factor of 2–6 higher than the a priori
emissions over the industrialized Indo-Gangetic Plain. Using the top-down
emissions, agreement between model simulations and surface observations of
aromatics improves. We find enhancements of reactive aromatics over Tibet by
a factor of 6 on average due to rapid transport from India and nearby
regions during the presence of a high-altitude cut-off low system. Our
results suggest that the cut-off low system is a major pathway for
long-range transport of pollutants such as black carbon. The modeling
analysis reveals that even the state-of-the-science high-resolution
reanalysis cannot simulate this cut-off low system accurately, which
probably explains in part the underestimation of black carbon deposition
over Tibet in previous modeling studies. Another model deficiency of
underestimating pollution transport from the south is due to the complexity
of terrain, leading to enhanced transport. It is therefore challenging for
coarse-resolution global climate models to properly represent the effects of
long-range transport of pollutants on the Tibetan environment and the
subsequent consequence for regional climate forcing.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The Tibetan Plateau, commonly referred as the Third Pole and the last
pristine land of the Earth, has drawn much attention in environmental and
climate research in recent years (Menon et al., 2002). Although Tibet appears
to be isolated from industrialized regions due in part to the transport
barrier by its being a plateau and its pollutant concentrations being
generally low, the Third Pole is vulnerable to regional climate change. Areas
of the Tibetan Plateau over 4 km in altitude are warming at a rate of
0.3 <inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C per decade, twice as fast as the global average (Xu et al.,
2009). In addition to the increase of greenhouse gases (GHGs) and the
associated global warming, black carbon (BC) is likely another important
contributor to the warming of the Tibetan Plateau. The deposition of BC on
the vast glaciers of the Tibetan Plateau will decrease the surface albedo,
accompanied by increased sunlight absorption and subsequent enhanced melting
(Hansen and Nazarenko, 2004; Ramanathan and Carmichael, 2008; Ming et al.,
2009; Yasunari et al., 2010). Increasing BC concentrations have previously
been found in ice core and lake sediment records (Xu et al., 2009; Cong et al.,
2013). The dwindling of glaciers over Tibet is a major concern for
freshwater supply to a large portion of the Asian population through the Indus
River, Ganges River, Yarlung Tsangpo River, Yangtze River, and Yellow River
(Singh and Bengtsson, 2004; Barnett et al., 2005; Lutz et al., 2014). Though
melting glaciers favor river runoff temporarily, mass loss of glaciers
endangers water supply during the dry season in the future (Yao et al., 2004;
Kehrwald et al., 2008).</p>
      <p>Besides narrowing the uncertainties of BC emissions, aging, and deposition,
better understanding the transport pathways is equally important in this
region. Surrounded by the largest BC sources of East Asia and South Asia
(Bond et al., 2007; Ohara et al., 2007), Tibet is primarily affected by
pollutant transport from these two regions (Kopacz et al., 2011; Lu et al.,
2012; Zhao et al., 2013; Wang et al., 2015, 2016; Zhang et al., 2015; Li et al.,
2016;  Kang et al., 2016). Kopacz et al. (2011) attempted
to identify the sources of BC over glaciers in the Himalayas and the Tibetan
Plateau (HTP) using the adjoint model of GEOS-Chem. Lu et al. (2012)
developed a novel back-trajectory model with BC emissions,
hydrophilic-to-hydrophobic aging, and deposition and found that South Asia
and East Asia account for 67 and 17 % of BC over the HTP, respectively. Using source
tagging, biofuel and biomass burning emissions from South Asia are found to
be the largest sources of BC in HTP, followed by fossil fuel combustion
emissions (Zhang et al., 2015). Hindman and Upadhyay (2002) suggested that
the vertical lifting due to convection and subsequent horizontal
mountain-valley wind lead to the transport of aerosols from Nepal to Tibet.
Dumka et al. (2010) also stressed the important role of mountain-valley
wind in the BC concentration in the central Himalayas. Cong et al. (2015) suggested
that both the large-scale westerlies from South Asia and the local
mountain-valley wind from South Asia are major transport pathways. The
synoptic-scale trough and ridge can potentially lead to the trespassing of
atmospheric brown clouds from South Asia to the Tibetan Plateau (Lüthi
et al., 2015). Ji et al. (2015) indicated that the southwesterlies during
monsoon season favor aerosol transport across the Himalayas from South
Asia. Aerosol observations in previous studies are mostly limited to the
southern and northern slopes of the Himalayas (Hindman and Upadhyay, 2002;
Dumka et al., 2010; Cong et al., 2015), with very few in situ sites (e.g.,
Namco, Linzhi) inside Tibet (Kopacz et al., 2011; Ji et al., 2015; Lüthi
et al., 2015; Zhang et al., 2015). Considering the complex topography
(Lawrence and Lelieveld, 2010; Ménégoz et al., 2013; He et al.,
2014; Kumar et al., 2015) and scarce observations (Maussion et al., 2011),
it is crucial to evaluate model-simulated transport performance over the
Tibetan Plateau using available observations with a good spatial coverage.
Observation-constrained modeling is needed to better understand potential
model biases due to the uncertainties of model-simulated transport from
South Asia to Tibet.</p>
      <p>In this study, we use short-lived reactive aromatics as proxies to diagnose
transport of pollutants to Tibet. In situ observations of short-lived
reactive aromatics across the Tibetan Plateau are analyzed (Sect. 2.1).
Anthropogenic emissions including fossil fuel combustion, gasoline
evaporation, and solvent use constitute the main sources of atmospheric
aromatics (Sack et al., 1992; Fu et al., 2008; Henze et al., 2008; Cagliari
et al., 2010; Cabrera-Perez et al., 2016). Biofuel and biomass burning is
another important source (Fu et al., 2008; Henze et al., 2008). The main sink
of aromatics is OH oxidation with lifetimes ranging from hours to days
(Atkinson, 2000; Liu et al., 2012b). We use satellite observations to
minimize the biases of emission inventories for upwind regions of Tibet
(Sect. 2.2, 2.3 and 2.4) and then apply a regional chemistry and transport
model constrained by high-resolution reanalysis meteorological data to
understand missing transport processes in model simulations (Sect. 3). On the
basis of these results, we examine the implications for global climate
modeling studies of anthropogenically driven changes over the Tibetan Plateau
(Sect. 4).</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
<sec id="Ch1.S2.SS1">
  <title>In situ aromatic data</title>
      <p>Whole-air samples were collected in 2 L electro-polished stainless-steel
canisters, which had been cleaned and vacuumed according to the TO-15 method
issued by the US EPA before shipment to the sampling sites. The restricted grab
sampler (39-RS-x; Entech), which has a 5 <inline-formula><mml:math id="M2" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m Silonite-coated metal
particulate filter, was placed on the inlet of the canister to completely
filter out dust and other particulates during sampling. These samples were
taken in daytime from 08:00 to 19:00 LT (Beijing time, GMT <inline-formula><mml:math id="M3" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 8) with an interval of 1 to
2 h. The sampling time was 5 min to fill the vacuumed canisters. The filled
canisters were transported back to the laboratory of the Guangzhou Institute of
Geochemistry, Chinese Academy of Science. Each air sample was analyzed for 65
light non-methane hydrocarbons (NMHCs) species. The samples were pretreated
by an Entech Model 7100 Preconcentrator (Entech Instruments Inc., California,
USA) and analyzed by a gas chromatography–mass selective detector
(GC-MSD/FID, Agilent 7890A/5973N, USA) using dual columns and dual detectors
to simultaneously analyze both low- and high-boiling-point volatile organic compounds (VOCs) with each
injection. The detailed analytical procedure is described by Zhang et
al. (2012).</p>
      <p>In this study, we analyze 65 measurements of aromatics (benzene, toluene,
ethyl-benzene, and m/p/o-xylene) and wind speed measurements taken across Tibet
during October 2010 (Fig. 1a). Care was taken in sampling such that there are
no direct urban, industrial, or road emissions in the upwind direction of the
sampling location. The lifetimes of toluene, ethyl-benzene, and m/p/o-xylene are
relatively short (2–20 h), and these reactive aromatic compounds therefore
provide observational constraints for transport from India and nearby regions
to Tibet. We group the samples into three periods based on the time and
locations of the measurements, i.e., period 1 from 13 to 17 October 2010 to
the north of the Himalayas along the southern border of Tibet, period 2 from
19 to 24 October across the interior of the Tibetan Plateau, and period 3 of
25 October to the west of the Yarlung Tsangpo Grand Canyon in southeastern
Tibet (Fig. 1a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Overview of regions involved in this study. Locations of
observations for period 1 (13–17 October 2010, triangle), period 2
(19–24 October 2010, circle), and period 3 (25 October 2010, square) are
shown in <bold>(a)</bold>. White polygon in <bold>(b)</bold> represents the model
domain margin of REAM. Altitude data from Global Topographic Data (GTOPO30,
courtesy of the US Geological Survey) are shown as colored background.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <title>SCIAMACHY CHOCHO measurements</title>
      <p>The SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY
(SCIAMACHY) onboard Environmental Satellite (ENVISAT) operated from 2002 to
2012 (Burrows et al., 1995; Bovensmann et al., 1999), with an overpass time
at about 10:00 local time. SCIAMACHY made passive remote-sensing
measurements of the upwelling radiation from the top of the atmosphere in
alternate nadir and limb-viewing geometry. Mathematical inversion of the
measurements of SCIAMACHY yields a variety of data products including glyoxal
(CHOCHO) vertical column densities (VCDs; unit: molecules cm<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). The
retrieval uses the differential optical absorption spectroscopy (DOAS)
technique (Wittrock et al., 2006; Vrekoussis et al., 2009; Alvarado et al.,
2014). The CHOCHO retrieval used in this study is based on the algorithm
developed in Alvarado et al. (2014), which includes corrections for the
interferences with nitrogen dioxide (NO<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> over the regions with high
NO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions as well as liquid water over oceans (Alvarado, 2016). The
detection limit for SCIAMACHY CHOCHO VCD is about <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. The overall monthly uncertainty of CHOCHO
VCDs (<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msubsup><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext><mml:mtext>SCIAMACHY</mml:mtext></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the selected region during
October 2010 is given by <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>×</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext><mml:mtext>SCIAMACHY</mml:mtext></mml:msubsup><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>,
where the value of <inline-formula><mml:math id="M12" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is in a range of 0.1 to 0.3. Following the
method as described by Liu et al. (2012b), we derive a top-down aromatic
emission estimate for South Asia constrained by CHOCHO retrievals described
in Sect. 2.4.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>3-D REAM model</title>
      <p>We use the 3-D Regional chEmical trAnsport Model (REAM) to examine the
chemistry evolution and regional transport of aromatics. REAM has been used in
previous studies, including large-scale transport (Wang et al., 2006; Zhao et
al., 2009b, 2010), vertical transport (Zhao et al., 2009a; Zhang et al.,
2014, 2016), emission estimates (Zhao and Wang, 2009; Liu et al., 2012b; Gu
et al., 2013, 2014, 2016), and other air quality studies (Zeng et al., 2003,
2006; Choi et al., 2005, 2008a, b; Wang et al., 2007; Liu et al., 2010,
2012a, 2014; Gray et al., 2011; Yang et al., 2011; Zhang and Wang, 2016).</p>
      <p>REAM has a horizontal resolution of 36 km with 30 vertical levels in the
troposphere and 5 vertical levels in the stratosphere covering adjacent
regions of China (Fig. 1b). The model top is at 10 hpa. Meteorological
fields in REAM are obtained from the Weather Research and Forecasting model
(WRF) assimilations constrained by National Centers for Environmental
Prediction Climate Forecast System Reanalysis (NCEP CFSR; Saha et al., 2010)
6-hourly products, which have a horizontal resolution of T382
(<inline-formula><mml:math id="M13" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 38 km). We run the WRF model with the same resolution as in REAM
with a domain larger than that of REAM by 10 grid cells on each side.
Meteorological inputs related to convective transport are updated every
5 min, while the others are updated every 30 min. The recent update of REAM
expands the GEOS-Chem standard chemical mechanism (V9-02) to include a
detailed description of aromatic chemistry (Bey et al., 2001; Liu et al.,
2010, 2012b). Aromatics are lumped into three species based on reactivity,
i.e., ARO1 (toluene, ethyl-benzene), ARO2 (m/p/o-xylene), and benzene. The
atmospheric lifetimes of the three aromatic tracers against OH are 18 h,
4.2 h, and 3.9 days during the study period (13–25 October 2010),
respectively. Due to the long atmospheric lifetime of benzene, it is more
difficult to track and identify its sources; thus we do not explicitly
discuss benzene in this study. We focus our analysis on reactive aromatics
(toluene, ethyl-benzene, and m/p/o-xylene).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>SCIAMACHY-observed CHOCHO VCDs <bold>(a)</bold>, REAM-simulated CHOCHO VCDs <bold>(b)</bold>, the low bias of simulated CHOCHO
VCDs <bold>(c)</bold>, simulated isoprene <bold>(d)</bold>, and aromatic <bold>(e)</bold>
contributions to CHOCHO VCDs using the a priori emissions for October 2010.
White areas denote missing satellite data or ocean. For each valid SCIAMACHY
data point, a corresponding model value is sampled in <bold>(b, c)</bold>.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f02.png"/>

        </fig>

      <p>Initial and boundary conditions for chemical tracers are taken from GEOS-Chem
(V9-02) 2<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M15" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation (Bey et al., 2001).
Anthropogenic emissions are from the MIX inventory for October 2010 (Li et
al., 2017). MIX is a mosaic Asian anthropogenic emission inventory with the
Multi-resolution Emission Inventory for China (MEIC) and several
other emission inventories for other Asian countries. In addition to the MIX
inventory, we also conduct sensitivity simulations using the Intercontinental
Chemical Transport Experiment-Phase B (INTEX-B) emissions inventory (Zhang et
al., 2009; Li et al., 2014), which was developed for the year 2006. We find
that, compared to the in situ observations of aromatics, the simulation
results using the INTEX-B emissions are better. The main reason for the
simulation improvements is the emissions of aromatics in South Asia.
Given the large uncertainties in the emissions of aromatics (e.g., Liu et
al., 2012b), this result is not surprising. Since MEIC and INTEX-B
inventories are developed by the same group, we replace MIX aromatic
emissions outside China with INTEX-B data such that aromatic emissions in
the model are consistent. The improvements of model simulations compared to
in situ observations are shown in Fig. S1 in the Supplement. Since satellite
observations are used to improve aromatic emissions (next section), using
either MIX or INTEX-B emissions in this work gives the same conclusions.
Biogenic VOC emissions are computed with the Model of Emissions of Gases and
Aerosols from Nature (MEGAN) algorithm (v2.1; Guenther et al., 2012), and
outdoor biomass burning emissions of CHOCHO and other species are based on
Global Fire Emissions Database Version 4.1 with small fires (GFED4.1s; van
der Werf et al., 2010; Andreae and Merlet, 2001; Lerot et al., 2010). Indoor
burning CHOCHO emissions of India are computed using emission factors from
Pettersson et al. (2011) and Li et al. (2014). Rural and urban population
distributions of India for the year 2010 are used as spatial proxies (Balk et
al., 2006; CIESIN, 2011, 2016). We adopt the energy consumptions for rural
and urban inhabitants on the basis of the National Sample Survey Office of
India (NSSO, 2012a, b). Compared with satellite-observed CO and NO<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
VCDs, REAM performs reasonably well in the study region during October 2010
(Fig. S2 in the Supplement). For general model evaluations of REAM, we refer
the readers to the papers cited early in this section.</p>
      <p>We updated the INTEX-B emission inventory in South Asian countries through
inverse modeling constrained by SCIAMACHY CHOCHO VCDs (next section). We run
REAM simulations with the a priori and top-down emission inventories, and we
compare the results with observations in Sect. 3.1 and 3.2, respectively. We
find that some of the model low bias is likely due to emission
underestimation. We further carried out three model sensitivity tests to
calculate the contributions to surface aromatics from emissions over Tibet,
other provinces of China, and South Asia (India and nearby regions). Each
simulation is run with only the aromatic emissions from the corresponding
region. The OH concentrations in each simulation are specified to the
archived values of the full model simulation. The results for two sub-periods
of period 2 are examined in Sect. 3.3.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Top-down aromatic emission estimation</title>
      <p>Compared with SCIAMACHY data, REAM using the original emission inventories
archived at the overpass time of SCIAMACHY underestimates CHOCHO VCDs in the
populated regions of India (Fig. 2). This underestimation is especially
significant in the Indo-Gangetic Plain located south of the Himalayas
(Fig. 2c). We thus derive the top-down aromatic emissions for these regions
constrained by SCIAMACHY CHOCHO data (Liu et al., 2012b; Alvarado, 2016).</p>
      <p>First, we calculate the difference between observed
(<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msubsup><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext><mml:mtext>SCIAMACHY</mml:mtext></mml:msubsup></mml:mrow></mml:math></inline-formula>, Fig. 2a) and modeled
(<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msubsup><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext><mml:mtext>REAM</mml:mtext></mml:msubsup></mml:mrow></mml:math></inline-formula>, Fig. 2b) CHOCHO VCDs with original emissions
(<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext><mml:mtext>SCIAMACHY</mml:mtext></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext><mml:mtext>REAM</mml:mtext></mml:msubsup></mml:mrow></mml:math></inline-formula>,
Fig. 2c). This discrepancy greatly exceeds the uncertainties of SCIAMACHY
retrieval. We then discuss the potential reasons for the difference, i.e.,
primary emissions from biomass burning and secondary sources from isoprene,
acetylene, ethylene, and aromatics (Fu et al., 2008; Liu et al., 2012b).</p>
      <p>Biomass burning is often a major primary source of CHOCHO (Myriokefalitakis
et al., 2008). GFED4.1s inventories, as well as fire hot spots observed by
MODIS on board the Terra and Aqua satellites, indicate only a small number of
fire occurrences during this period in South Asia, with the exception of crop
residue burning in Punjab, an agricultural state in north India. The
contribution to CHOCHO VCDs from outdoor biomass burning (Fig. S3a in the
Supplement) differs greatly from that of <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>C</mml:mi><mml:mtext>CHOCHO</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 2c),
which is large over the industrialized Indo-Gangetic Plain. Simulated indoor
burning contribution to CHOCHO VCDs is lower by a factor of about 15 than the
CHOCHO VCD discrepancy between satellite retrieval and model simulation
(Fig. S3b in the Supplement). The uncertainty of the indoor burning CHOCHO
emissions mainly results from that of the emission factor. Even if we assume
this uncertainty to be 300 %, indoor burning cannot explain the low bias
of the simulated CHOCHO VCDs. Therefore, the large model underestimation of
CHOCHO over the Indo-Gangetic Plain is unlikely due to outdoor biomass
burning or indoor burning during our analysis period.</p>
      <p>Direct anthropogenic emissions of CHOCHO are small (Volkamer et al., 2005;
Stavrakou et al., 2009; Liu et al., 2012b). CHOCHO is produced primarily from
the photochemical oxidation of biogenic compounds (e.g., isoprene and
terpenes) and hydrocarbon released by anthropogenic activities (e.g.,
acetylene, ethylene, and aromatics) (Fu et al., 2008). Due to the long
atmospheric lifetime of acetylene and ethylene, their contributions to CHOCHO
concentrations are quite small in South Asia during October 2010. The most
significant secondary sources of CHOCHO in South Asia are isoprene (Fig. 2d)
and aromatics (Fig. 2e). Biogenic isoprene emissions depend on vegetation,
sunlight, and temperature. The high isoprene contribution to CHOCHO VCDs is
to the southeast of the Indo-Gangetic Plain, where CHOCHO VCDs are high in
both the observations and model simulations. In comparison, aromatic
oxidation dominates CHOCHO over the Indo-Gangetic Plain, where model
underestimation is largest (Fig. 2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Comparison between REAM-simulated reactive aromatic concentrations
(<inline-formula><mml:math id="M22" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) and in situ observations (<inline-formula><mml:math id="M23" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis). REAM results are archived
corresponding to the time and location of the observations. Linear regression
results for three periods are shown in red (slope <inline-formula><mml:math id="M24" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.14, <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.04</mml:mn></mml:mrow></mml:math></inline-formula>),
blue (slope <inline-formula><mml:math id="M26" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.56, <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.83</mml:mn></mml:mrow></mml:math></inline-formula>), and green (slope <inline-formula><mml:math id="M28" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.15,
<inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M30" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.02) dashed lines, respectively.</p></caption>
          <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f03.png"/>

        </fig>

      <p>We apply the approach by Liu et al. (2012b) to estimate the top-down
emissions of aromatics based on SCIAMACHY CHOCHO VCDs. As found by Liu et
al. (2012b), domain-wide inversion is impractical since model results
correlate poorly with gridded satellite data, most likely reflecting the
problems in the spatial distribution of a priori emissions. We therefore
determine the emissions by inversion for each grid cell at the overpass time
of SCIAMACHY as Liu et al. (2012b) and find similar results for India and
nearby regions as Liu et al. (2012b) did for eastern China. The top-down
biogenic isoprene emissions are essentially the same as the a priori
emissions. However, the top-down anthropogenic emissions of aromatics
(Fig. S4 in the Supplement) increase by a factor of 2–6. The improved model
comparison with in situ observations will be discussed in the next section.
One caveat with respect to the top-down emission estimate is that we have to
assume that the speciation of aromatics in the a priori emission inventory is
correct. Since the purpose of this work is to study transport pathways to the
Tibetan Plateau on the basis of in situ observations, we examine lumped
reactive aromatics (defined as the sum of toluene, ethyl-benzene, and
m/p/o-xylene) in the model evaluation (next section). Satellite observations
cannot be used for this purpose since CHOCHO VCDs over Tibet are below or
around the detection limit.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <title>Observed and simulated reactive aromatics</title>
      <p>The average of observed reactive aromatic surface concentration
(59 <inline-formula><mml:math id="M31" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 63 pptv) over the Tibetan Plateau is considerably lower than the
values found for megacities of China, such as Beijing (8.04 ppbv) and
Shanghai (5.2 ppbv) (Liu et al., 2012b). Higher aromatic levels were
measured during period 1 (76 <inline-formula><mml:math id="M32" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 39 pptv) and period 3
(169 <inline-formula><mml:math id="M33" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 57 pptv) than in period 2 (26 <inline-formula><mml:math id="M34" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 39 pptv). The model
simulation using the a priori emissions in general compares poorly with the
in situ observations (Fig. 3). The best performance is during the
low-concentration period 2 when the model underestimates the observations by
about a factor of 2. However, the relatively high correlation coefficient
(<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.83</mml:mn></mml:mrow></mml:math></inline-formula>) suggests that atmospheric transport and emission distribution
are reasonably simulated. This is in sharp contrast to periods 1 and 3 when
the model underestimates the observations by a factor of 7 with very low
correlations between the model and the observations (slope <inline-formula><mml:math id="M36" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.14 and
0.15, <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.04</mml:mn></mml:mrow></mml:math></inline-formula> and 0.02 for period 1 and 3, respectively). We discuss the
different reasons for the model performance for periods 1, 2, and 3 in the next
three sections.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Improvements due to top-down emissions</title>
      <p>Figures 2 and S4 in the Supplement show that SCIAMACHY observations of
CHOCHO suggest much higher industrial emissions of aromatics over the
Indo-Gangetic Plain than the a priori emissions. We derive top-down emissions
on the basis of SCIAMACHY CHOCHO VCDs (Sect. 2.4). Top-down emissions are
higher than the a priori emissions by a factor of 2–6 over the Indo-Gangetic
Plain, which is the upwind region of the Tibetan Plateau. Figure 4 shows the
resulting improvement in the model simulation. The large underestimations of
CHOCHO VCDs over the Indo-Gangetic Plain are corrected as expected (Fig. 4a).
At the same time, in situ observations during period 2 are much better
reproduced by the model with the slope increasing from 0.56 to 0.91 and a
similar <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> value (0.66) (Fig. 4b). In contrast, model simulations for
periods 1 and 3 are not improved using top-down emission estimates with low
biases similar to the original model simulation. This indicates that the
reasons for the discrepancies in periods 1 and 3 are probably not related to
the uncertainties in emissions but could be linked to deficiencies in model
transport in this area.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>REAM-simulated CHOCHO VCDs with top-down emissions <bold>(a)</bold> and
comparison of simulated and observed reactive aromatic concentrations during
period 2 <bold>(b)</bold>. Blue and red circles in panel <bold>(b)</bold> represent
REAM simulation with a priori (slope <inline-formula><mml:math id="M39" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.56, <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.83</mml:mn></mml:mrow></mml:math></inline-formula>) and with
top-down (slope <inline-formula><mml:math id="M41" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.91, <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.66</mml:mn></mml:mrow></mml:math></inline-formula>) emissions, respectively.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f04.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Rapid trans-Himalaya transport due to a high-level cut-off low
system</title>
      <p>Observed and simulated reactive aromatic concentrations show large
variabilities during period 2 (Fig. 4b). An investigation of these data shows
that a major contributor is meteorology. Observed concentrations of reactive
aromatics during 19–20 October are generally lower (6.6 <inline-formula><mml:math id="M43" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.4 pptv)
than those during 21–24 October (37 <inline-formula><mml:math id="M44" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 45 pptv). The
concentration difference during the two time periods is captured by model
simulations with top-down emissions (Fig. 5). Analysis of WRF-simulated
surface wind speed shows an increase by a factor of 2–4 from 19–20 October
(Fig. 5a) to 21–24 October (Fig. 5b),
corresponding well to increasing transport of aromatics from the
Indo-Gangetic Plain.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Distributions of WRF-simulated surface wind and REAM-simulated
concentrations of reactive aromatics over the Tibetan Plateau during
19–20 October 2010 <bold>(a)</bold> and 21–24 October 2010 <bold>(b)</bold>.
Circles show the observed reactive aromatic concentrations. Composite
distributions of simulated reactive aromatic concentrations and surface wind
over Tibet, corresponding to sampling time of the observations, are shown in
color and by arrows, respectively. Corresponding WRF-simulated 300 hPa
geopotential height fields are shown by contour lines. The border of the Tibet
Autonomous Region is colored green.</p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f05.png"/>

        </fig>

      <p>To further analyze the difference between the two time periods, we conduct
sensitivity simulations as described in Sect. 2.3. We compute the source
attributions for emissions over Tibet, India and nearby regions, and China
excluding Tibet (Fig. 6). During 19–20 October, reactive aromatics are due
to Tibetan emissions. With the exception of one data point, the
concentrations are <inline-formula><mml:math id="M45" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 7 pptv. On 21 October, emissions from India and
nearby regions become dominant while the concentrations are still low
(7–21 pptv). During 22–24 October, however, emissions from India and
nearby regions contribute much higher concentrations (10–137 pptv). The
only exception is one data point sampled 30 km east of Lhasa, where about
one-fifth of the population of Tibet resides. The contribution of emissions
from India and nearby regions to this data point is <inline-formula><mml:math id="M46" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 pptv, still
much higher than during 19–20 October. The contribution of emissions from
China (excluding Tibet) is negligible (<inline-formula><mml:math id="M47" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 %) for this period.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Reactive aromatics emitted from Tibet (red), India and nearby
regions (“South Asia”, blue), and China excluding Tibet (“China w/o
Tibet”, green) corresponding to the in situ observations in the REAM
simulation with top-down emissions. Contributions from the other regions are
negligible.</p></caption>
          <?xmltex \igopts{width=128.037402pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f06.png"/>

        </fig>

      <p>The rise of the Tibetan Plateau is a natural barrier for pollution transport
(Fig. 1). Considering the high altitude of the Tibetan Plateau, we analyze
the 300 hPa geopotential height field in order to understand the change of wind
circulation over the region (Fig. 5). During 19–20 October, the upper
troposphere shows a northward gradual pressure decrease, which does not
promote near-surface forcing of trans-Himalaya transport (Fig. 5a). During
21–24 October, the presence of a southeastward-moving upper-tropospheric
cut-off low system induces increasingly stronger surface wind from India to
Tibet (Fig. 5b, Hoskins et al., 1985). The cut-off low system is a closed
low-pressure system detached from the westerlies. It began to form on 21 October
and started to dissipate on 24 October. Trans-Himalaya air mass flux in
the lower atmosphere shows an increase by a factor of 2 to 5 (Fig. S5 in the
Supplement). Accompanying this transport, large amounts of pollutants such as
reactive aromatics analyzed here are transported to the Tibetan Plateau,
leading to much higher surface concentrations.</p>
      <p>The cut-off low system provides a more rapid and efficient pollutant
transport pathway than transport pathways previously proposed by
other studies, such as westerlies (Cong et al., 2015; Ji et al., 2015) and
mountain-valley winds (Hindman and Upadhyay, 2002; Dumka et al., 2010).
Compared to aromatics, BC is also subject to wet scavenging, which greatly
reduces its transport efficiency by convection. In-cloud BC scavenging is due
to cloud activation or ice nucleation and subsequent removal by
precipitation, and below-cloud scavenging is due to collision with rain
droplets (e.g., Taylor et al., 2014). During our analysis period, the cut-off
low system and the associated precipitation are to the northwest of Tibet
(Fig. S6 in the Supplement). Precipitation south of Tibet is weak, and thus
the subsequent removal of BC during trans-Himalaya transport is limited.</p>
      <p>To examine the sensitivity of trans-Himalaya transport to the distribution of
emission sources, we redistribute the INTEX-B total aromatic emissions over
China and other South Asia countries on the basis of the MIX BC emission
distributions. We conduct a sensitivity simulation using the redistributed
emissions and compare the results to the original simulation. The
trans-Himalaya transport from South Asia clearly dominates, and it is strongly
affected by the presence of a cut-off low system during our analysis period
(Fig. S7 in the Supplement). Our analysis implies that BC transported in the
presence of an upper-tropospheric cut-off low is potentially a major
contributor to BC deposition to Tibetan glaciers.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Missing cut-off low system and complex terrain</title>
      <p>Compared to period 2, model performance for periods 1 and 3 is very poor with
severe low biases (Fig. 3). Transport deficiency appears to be the main
problem. Figure 7 shows the histograms of observed and simulated surface wind
speed for the three periods. The observed and simulated wind speed distributions
are similar for period 2 (Fig. 7c). In comparison, the simulated wind speed
distribution differs drastically for the other two periods (Fig. 7a and d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>Histograms of observed and simulated surface wind speed for
period 1 <bold>(a)</bold>, period 2 <bold>(c)</bold>, and period 3 <bold>(d)</bold>.
Panel <bold>(b)</bold> shows the wind histogram of 23 October with an
upper-tropospheric cut-off low system. Model results are sampled at the same time
and location as the observations. In <bold>(b)</bold>, the date information is
not used. Wind speed is binned at a 1 m s<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> interval.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f07.png"/>

        </fig>

      <p>The wind speed distributions are more similar between periods 1 and 2 in the
observations than model simulations. The underestimation of wind speed in
period 1 leads to slower transport of pollutants from the Indo-Gangetic Plain
and consequently to a low bias in surface reactive aromatics in the model.
Examination of the 300 hPa geopotential height field during 13–17 October
of period 1 shows a weak trough northeast of Kazakhstan in CSFR reanalysis
and WRF simulation results (Fig. S8 in the Supplement). A strong upper-tropospheric
low-pressure system, akin to the cut-off low system of Fig. 5b,
will induce stronger lower-troposphere wind circulation. The lack of
radiosonde observations over the interior of the Tibetan Plateau to constrain
the meteorological reanalysis is the plausible reason (Fig. S9 in the
Supplement). The horizontal scale of the Rossby wave at northern
midlatitudes is thousands of kilometers, which can be reasonably represented by
the density of the existing radiosonde network. We hypothesize that the
smaller-scale cut-off low system, not simulated in the reanalysis, is more
likely the reason for the model–observation discrepancy during period 1. We
resample surface wind speed of 23 October, when a cut-off low system leads to
rapid trans-Himalaya transport in period 2 as analyzed in the previous section.
At the same time of the day and location as the observations, the simulated
wind speed histogram is in good agreement with the observations (Fig. 7b).
The corresponding air mass flux across the Himalayas would have been much
stronger in the presence of a cut-off low system (Fig. S10 in the
Supplement).</p>
      <p>During period 3, the observed wind speed histogram is skewed to very low wind
speed (0–1 m s<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) compared to the simulations (Fig. 7d). Sampling
bias to avoid locations with strong wind is a possible reason. Another reason
is that these samples were taken at lower altitudes in valleys compared to
higher altitudes in the other two periods. Inspection of Fig. 1 shows the
complex terrain surrounding the valleys of period 3 sampling. Using
high-resolution (<inline-formula><mml:math id="M50" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km) terrain data from the US Geological Survey
(USGS) Global 30 Arc-Second Elevation (GTOPO30) dataset, we find that the
standard deviation of altitude in the 7 km <inline-formula><mml:math id="M51" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7 km region centered
at the corresponding observation location correlates well with the observed
reactive aromatics with a <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> value of 0.55 (Fig. 8), which suggests that
pollution transport is strongly enhanced by the effects of complex terrain.
The horizontal resolution of 36 km used in this study is inadequate to
simulate this effect. Model resolution as high as 1 km appears to be
necessary to capture the observed feature, but the computational resource
requirement will be exceptionally large for a global model such as that used
for CFSR. Other issues related to complex terrains in this region were also
discussed by previous studies (Maussion et al., 2011; Ménégoz et al.,
2013; He et al., 2014; Kumar et al., 2015). The effects of complex terrain
may have also affected the observations of periods 1 and 2 but to a smaller
extent since the terrain variation is lower and sampling altitude is higher
in those periods.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p>Observed reactive aromatics as a function of terrain complex during
period 3. The latter is computed as the standard deviation of altitude in a
7 km <inline-formula><mml:math id="M53" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7 km region centered at the sampling location. The dash
line denotes a least-squares regression.</p></caption>
          <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/3083/2017/acp-17-3083-2017-f08.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions and implications for climate studies</title>
      <p>We apply the REAM model to analyze in situ observations of reactive aromatics
across the Tibetan Plateau. Top-down estimate using SCIAMACHY CHOCHO
observations suggests that the a priori inventory for aromatic emissions is
low by a factor of 2 to 6 over the industrialized Indo-Gangetic Plain.
Application of the top-down emission estimate greatly reduces the low bias of
the model during period 2. Model results suggest that the second half of
period 2 is characterized by rapid trans-Himalaya transport from India and
nearby regions driven by the presence of a cut-off low system in the upper
troposphere.</p>
      <p>Model performance for periods 1 and 3 is poor compared to period 2, and
employing top-down emission estimates does not significantly improve the
model simulation of these periods. In situ observations show much stronger
surface wind than simulated in the model during period 1. The lack of
radiosonde observations in the interior of the Tibetan Plateau is likely the
reason that a cut-off low system, the scale of which is much less than the
midlatitude Rossby wave, is not simulated by the T382 (<inline-formula><mml:math id="M54" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 38 km) CSFR
reanalysis. Consequently, trans-Himalaya transport is greatly underestimated
in the model. Sampling of period 3 is in valleys surrounded by complex
terrain. Although observed surface wind is weak, we find that reactive
aromatic concentrations are strongly correlated with the complexity of
surrounding terrain, implying enhanced pollution transport by terrain-driven
mixing. Model simulations at a resolution of 36 km are inadequate for
simulating the terrain effect.</p>
      <p>The height of the Tibetan Plateau is a natural barrier for pollution
transport into this pristine region. This geographical feature is also a
challenge for regional and global model simulations. In this study, we use
short-lived reactive aromatics as proxies to evaluate model-simulated
transport to the Tibetan Plateau on the basis of in situ observations. After
correcting for the emission underestimation using satellite observations,
simulated trans-Himalaya transport of proxy species (using WRF assimilated
meteorological fields) still has significant low biases for two reasons:
(1) poor representation of a cut-off low system and (2) inadequate
representation of terrain effect due to a coarse model resolution. These two
transport-related issues likely exist in global climate models; the coarser
resolution of climate models than our simulations or CSFR may further worsen
the transport biases. Our results imply that pollution transport to the
Tibetan Plateau, such as that of BC, is likely to be greatly underestimated
in climate models, which has been found previously (e.g., He et al., 2014). In
addition to trans-Himalaya transport, BC emissions, chemical transformation,
and wet deposition also require extensive evaluations with the observations
over the region. Further analysis of reanalysis and climate model simulations
is required to quantify potential model biases and the resulting effect of
simulated BC deposition to glaciers on the Tibetan Plateau due to the
transport issues we identified in this study.</p>
</sec>
<sec id="Ch1.S5">
  <title>Data availability</title>
      <p>The modeling data are available at Georgia Institute of Technology website (<uri>http://apollo.eas.gatech.edu/data/trans-Himalaya/</uri>).
The SCIAMACHY CHOCHO data are available at University of Bremen IUP DOAS website (<uri>http://www.iup.uni-bremen.de/doas/glyoxal_data.htm</uri>).
The NCEP CFSR data are available at University Corporation for Atmophseric Research (UCAR) website (<uri>http://rda.ucar.edu/datasets/ds093.0/</uri>).
The MIX and INTEX-b emission inventories are available at  MEIC group website (<uri>http://meicmodel.org</uri>).
The rural and urban population density data are available at CIESIN website (<uri>http://sedac.ciesin.columbia.edu/</uri>).
The GTOPO30 elevation data are available at USGS website (<uri>https://lta.cr.usgs.gov/GTOPO30</uri>).</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/acp-17-3083-2017-supplement" xlink:title="pdf">doi:10.5194/acp-17-3083-2017-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><notes notes-type="competinginterests">

      <p>The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p>The modeling analysis of this work was supported by the Atmospheric Chemistry
Program of the US National Science Foundation. The observation sampling and
analysis were supported by the National Natural Science Foundation of China
(nos. 41472311, 41273107) and the Special Scientific Research Funds for
Environmental Protection Commonwealth Section of China (20603020802L). The
contributions of the University of Bremen scientists to this manuscript were
funded in part by the University of Bremen as well as the state of Bremen, DLR (German Aerospace),
DFG (German Research Foundation), and ESA. Mihalis Vrekoussis acknowledges support from the DFG Research
Center/Cluster of Excellence “The Ocean in the Earth System-MARUM”.
Leonardo M. A. Alvarado gratefully acknowledges the funding support by the
German Academic Exchange Service (DAAD).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: F. Fierli<?xmltex \hack{\newline}?> Reviewed by: two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Enhanced trans-Himalaya pollution transport to the Tibetan Plateau by cut-off low systems</article-title-html>
<abstract-html><p class="p">Long-range transport followed by deposition of black
carbon on glaciers of Tibet is one of the key issues of climate research
as it induces changes on radiative forcing and subsequently impacting the melting
of glaciers. The transport mechanism, however, is not well understood. In
this study, we use short-lived reactive aromatics as proxies to diagnose
transport of pollutants to Tibet. In situ observations of short-lived
reactive aromatics across the Tibetan Plateau are analyzed using a regional
chemistry and transport model. The model performance using the current
emission inventories over the region is poor due to problems in the
inventories and model transport. Top-down emissions constrained by satellite
observations of glyoxal are a factor of 2–6 higher than the a priori
emissions over the industrialized Indo-Gangetic Plain. Using the top-down
emissions, agreement between model simulations and surface observations of
aromatics improves. We find enhancements of reactive aromatics over Tibet by
a factor of 6 on average due to rapid transport from India and nearby
regions during the presence of a high-altitude cut-off low system. Our
results suggest that the cut-off low system is a major pathway for
long-range transport of pollutants such as black carbon. The modeling
analysis reveals that even the state-of-the-science high-resolution
reanalysis cannot simulate this cut-off low system accurately, which
probably explains in part the underestimation of black carbon deposition
over Tibet in previous modeling studies. Another model deficiency of
underestimating pollution transport from the south is due to the complexity
of terrain, leading to enhanced transport. It is therefore challenging for
coarse-resolution global climate models to properly represent the effects of
long-range transport of pollutants on the Tibetan environment and the
subsequent consequence for regional climate forcing.</p></abstract-html>
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