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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-15-13145-2015</article-id><title-group><article-title>A potential vorticity-based determination of the transport barrier in the Asian summer monsoon anticyclone</article-title>
      </title-group><?xmltex \runningtitle{Monsoon transport barrier}?><?xmltex \runningauthor{F.~Ploeger et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Ploeger</surname><given-names>F.</given-names></name>
          <email>f.ploeger@fz-juelich.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Gottschling</surname><given-names>C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Griessbach</surname><given-names>S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3792-3573</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Grooß</surname><given-names>J.-U.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9485-866X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Guenther</surname><given-names>G.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4111-6221</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Konopka</surname><given-names>P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Müller</surname><given-names>R.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5024-9977</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Riese</surname><given-names>M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6398-6493</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Stroh</surname><given-names>F.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4492-2977</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Tao</surname><given-names>M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ungermann</surname><given-names>J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9095-8332</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Vogel</surname><given-names>B.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9763-3055</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>von Hobe</surname><given-names>M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6034-6562</ext-link></contrib>
        <aff id="aff1"><institution>Institute for Energy and Climate research: Stratosphere (IEK–7), Forschungszentrum Jülich, Jülich, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">F. Ploeger (f.ploeger@fz-juelich.de)</corresp></author-notes><pub-date><day>27</day><month>November</month><year>2015</year></pub-date>
      
      <volume>15</volume>
      <issue>22</issue>
      <fpage>13145</fpage><lpage>13159</lpage>
      <history>
        <date date-type="received"><day>20</day><month>February</month><year>2015</year></date>
           <date date-type="rev-request"><day>13</day><month>April</month><year>2015</year></date>
           <date date-type="rev-recd"><day>28</day><month>October</month><year>2015</year></date>
           <date date-type="accepted"><day>15</day><month>November</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/15/13145/2015/acp-15-13145-2015.html">This article is available from https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015.pdf</self-uri>


      <abstract>
    <p>The Asian summer monsoon provides an important pathway of tropospheric source
gases and pollution into the lower stratosphere. This transport is
characterized by deep convection and steady upwelling, combined with
confinement inside a large-scale anticyclonic circulation in the upper
troposphere and lower stratosphere (UTLS). In this paper, we show that a
barrier to horizontal transport along the 380 K isentrope in the monsoon
anticyclone can be determined from a local maximum in the gradient of
potential vorticity (PV), following methods developed for the polar vortex
<xref ref-type="bibr" rid="bib1.bibx23" id="paren.1"><named-content content-type="pre">e.g.,</named-content></xref>. The monsoon anticyclone is dynamically highly
variable and the maximum in the PV gradient is weak, such that additional
constraints are needed (e.g., time averaging). Nevertheless, PV contours in
the monsoon anticyclone agree well with contours of trace gas mixing ratios
(CO, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) and mean age from model simulations with a Lagrangian chemistry
transport model (CLaMS) and satellite observations from the Microwave Limb
Sounder (MLS) instrument. Hence, the PV-based transport barrier reflects the
separation between air inside the core of the anticyclone and the background
atmosphere well. For the summer season 2011 we find an average PV value of
3.6 PVU for the transport barrier in the anticyclone on the 380 K
isentrope.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>An efficient pathway for anthropogenic pollution and tropospheric source
gases into the stratosphere is linked to the Asian summer monsoon, as has
been shown from satellite observations of HCN <xref ref-type="bibr" rid="bib1.bibx33" id="paren.2"/>. Upward
transport in the monsoon is caused by frequent high-reaching convection
<xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx2" id="paren.3"><named-content content-type="pre">e.g.,</named-content></xref> and slower steady upwelling at higher
levels around the tropopause. In the upper troposphere and lower stratosphere
(UTLS), more precisely in the Tropical Tropopause Layer TTL
<xref ref-type="bibr" rid="bib1.bibx7" id="paren.4"><named-content content-type="pre">e.g.,</named-content></xref>, the Asian monsoon is characterized by a
large-scale anticyclonic circulation system, mainly a response to strong
convective diabatic heating at low levels <xref ref-type="bibr" rid="bib1.bibx9" id="paren.5"/>. The anticyclonic
circulation confines the upward transported air and isolates it, to some
degree, from its surroundings. This confinement leads to positive anomalies
of tropospheric trace gases (e.g., CO, HCN, H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O) and to negative anomalies
of stratospheric trace gases (e.g., ozone) in the anticyclone
<xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx26 bib1.bibx27 bib1.bibx13 bib1.bibx4" id="paren.6"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p>For an improved understanding of the pollution transport by the monsoon,
understanding the confinement of trace gases within the anticyclone is
crucial. However, the Asian monsoon anticyclone is characterized by large
dynamic variability <xref ref-type="bibr" rid="bib1.bibx8" id="paren.7"/>, strong east-west displacements
<xref ref-type="bibr" rid="bib1.bibx16" id="paren.8"/>, frequent shedding of small-scale eddies
<xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx31" id="paren.9"/> and even splits. Moreover, strong diabatic
heating processes play a role in the monsoon and, consequently, potential vorticity (PV) is not
well conserved <xref ref-type="bibr" rid="bib1.bibx10" id="paren.10"><named-content content-type="pre">e.g.,</named-content></xref>. For these reasons, the
confinement of air inside the Asian monsoon anticyclone appears to be much
weaker than in the polar vortex, and it turns out to be very challenging to
locate a barrier to horizontal transport <xref ref-type="bibr" rid="bib1.bibx8" id="paren.11"/>. However, that
such a transport barrier exists, at least to some degree, is reflected in the
observed trace gas anomalies within the anticyclone.</p>
      <p>To date, simplified criteria have been adopted to define this transport
barrier and to separate the core region of the anticyclone from its
surroundings. These criteria are commonly based on the positive geopotential
height anomaly or the negative PV anomaly in the monsoon anticyclone and
assume a fixed geopotential height (on a fixed pressure level) or PV value to
represent the transport barrier <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx3" id="paren.12"><named-content content-type="pre">e.g.,</named-content></xref>.
These criteria have the advantage of being easy to apply, but they lack a
clear physical reasoning.</p>
      <p>In this paper, we present a physically motivated criterion to deduce the
transport barrier in the Asian monsoon anticyclone based on conservation
properties of the flow. This criterion is closely related to a
well-established methodology using PV gradients on isentropic surfaces, which
has been originally developed for the polar vortex
<xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx20 bib1.bibx23" id="paren.13"><named-content content-type="pre">e.g.,</named-content></xref>. The method relies on the
fact that PV is approximately conserved, such that a maximum in the PV
gradient on an isentrope reflects the existence of a barrier to transport. We
emphasize here that the terminology “transport barrier” does not imply
vanishing cross-gradient transport. In fact, the anticyclone transport
barrier turns out to be rather leaky and is better interpreted as a region of
reduced cross-gradient transport (see Sect. <xref ref-type="sec" rid="Ch1.S7"/>).</p>
      <p>We introduce the data, model and methods to be used in
Sect. <xref ref-type="sec" rid="Ch1.S2"/>. In Sect. <xref ref-type="sec" rid="Ch1.S3"/> we motivate the
use of PV as a basis for deducing the anticyclone transport barrier, by
comparing PV to simulated and observed trace gas distributions (CO, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) in
the Asian monsoon region. The criterion for deducing the transport barrier is
presented in Sect. <xref ref-type="sec" rid="Ch1.S4"/>, and validated by comparison to
simulated CO, ozone and mean age in Sect. <xref ref-type="sec" rid="Ch1.S5"/>. We
finally discuss our results and conclude.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
      <p>Meteorological fields to characterize the Asian monsoon anticyclone are taken
from European Centre for Medium-Range Weather Forecasts (ECMWF) ERA-Interim
reanalysis. ERA-Interim covers the period from 1979 until present,
assimilating observational data from several sources to provide a reliable
state of the atmosphere <xref ref-type="bibr" rid="bib1.bibx6" id="paren.14"><named-content content-type="pre">for details, see</named-content></xref>. We used 6-hourly
data on a 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal grid and interpolated
it on potential temperature (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>) levels in the vertical. The presented
analysis focuses on the summer season (June–August, JJA) 2011 and on the
380 K isentropic surface, which is a characteristic level for the Asian
upper-level anticyclone in the UTLS. Note that in the tropics 380 K is close
to the 100 hPa isobaric surface, which has been used in several studies to
analyze transport in the Asian monsoon anticyclone
<xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx3" id="paren.15"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p>The most relevant meteorological fields for this study are Ertel's potential
vorticity (PV), the circulation (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Γ</mml:mi></mml:math></inline-formula>), and the Montgomery stream
function (<inline-formula><mml:math display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>). PV is calculated from the horizontal winds
<xref ref-type="bibr" rid="bib1.bibx10" id="paren.16"><named-content content-type="pre">e.g.,</named-content></xref>:
          <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">PV</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="italic">ζ</mml:mi><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        with <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ζ</mml:mi></mml:math></inline-formula> the relative vorticity, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:math></inline-formula> the Coriolis
parameter, and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>g</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mo>∂</mml:mo><mml:mi mathvariant="italic">θ</mml:mi></mml:msub><mml:mi>p</mml:mi></mml:mrow></mml:math></inline-formula> the isentropic mass
density (<inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> pressure, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> latitude, <inline-formula><mml:math display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> acceleration due to gravity, and
<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Ω</mml:mi></mml:math></inline-formula> the rotation frequency of the Earth). PV is a particularly well-suited quantity for characterizing barriers to transport. In the absence of
friction and diabatic processes the PV of an air parcel is conserved
following its motion <xref ref-type="bibr" rid="bib1.bibx10" id="paren.17"><named-content content-type="pre">e.g.,</named-content></xref>, and thus regions of
enhanced PV gradients are indicative of suppressed transport (transport
barriers). This fact was used for the polar vortex to deduce the transport
barrier based on the gradient of PV along an isentropic surface
<xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx23" id="paren.18"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p>A related quantity, characterizing fluid rotation, is the circulation
<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Γ</mml:mi></mml:math></inline-formula> along a closed contour <inline-formula><mml:math display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> (here, on an isentrope):
          <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>=</mml:mo><mml:munder><mml:mo movablelimits="false">∮</mml:mo><mml:mi>S</mml:mi></mml:munder><mml:mi mathvariant="bold-italic">d</mml:mi><mml:mi>s</mml:mi><mml:mo>⋅</mml:mo><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mo>=</mml:mo><mml:munder><mml:mo movablelimits="false">∫</mml:mo><mml:mi>A</mml:mi></mml:munder><mml:mi>d</mml:mi><mml:mi>a</mml:mi><mml:mi mathvariant="italic">ζ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        with <inline-formula><mml:math display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> the area enclosed by the contour <inline-formula><mml:math display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> the
horizontal wind on an isentropic surface (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">d</mml:mi><mml:mi>s</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mi>a</mml:mi></mml:mrow></mml:math></inline-formula> represent
line and area elements). Therefore, cyclonic flow is characterized by
positive circulation, while anticyclonic flow is characterized by negative
circulation.</p>
      <p>The Montgomery stream function <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mi>T</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi></mml:mrow></mml:math></inline-formula> (with <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Φ</mml:mi></mml:math></inline-formula>
geopotential, <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> temperature, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the specific heat at
constant pressure) is the isentropic analogue of geopotential, which is
frequently used to characterize the monsoon anticyclone
<xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx3" id="paren.19"/>. Under geostrophic approximations the
horizontal flow on an isentrope is along contours of constant <inline-formula><mml:math display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx10" id="paren.20"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p>Due to the anticyclonic nature of the upper-level circulation, the Asian
monsoon in the UTLS is characterized by strongly negative, anomalously low PV
(see Fig. <xref ref-type="fig" rid="Ch1.F1"/>), and anomalously high Montgomery stream
function values. To the north, the anticyclone is bounded by the subtropical
westerly jet, to the south by the equatorial easterly jet. Furthermore, the
monsoon region is characterized by an elevated thermal tropopause which, from
a climatological point of view, exceeds the zonal mean tropopause by more
than 1 km (Fig. <xref ref-type="fig" rid="Ch1.F1"/>), corresponding to <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>20</mml:mn></mml:mrow></mml:math></inline-formula> K
in potential temperature.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Meteorological conditions in the Asian monsoon anticyclone (based on
ERA–Interim reanalysis). Color shading shows the PV anomaly of the monsoon
longitude section (60–120<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) with respect to the zonal mean,
averaged over summer (June-August). Also shown is zonal wind (thick black,
solid/dashed positive/negative) and potential temperature (thin black)
averaged between 60–120<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. The first thermal tropopause
<xref ref-type="bibr" rid="bib1.bibx38" id="paren.21"><named-content content-type="pre">calculated using the definition of</named-content></xref> zonally averaged over
0–360<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E is shown as dark-blue, averaged over 60–120<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E
as cyan line. </p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f01.pdf"/>

      </fig>

      <p>To confirm the deduced location of the transport barrier, which will be based
on PV, we consider different trace gas species (carbon monoxide, ozone) from
model simulations with the Chemical Lagrangian Model of the Stratosphere
CLaMS <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx21 bib1.bibx14" id="paren.22"/>, driven by ERA-Interim
meteorological data. We further consider simulated mean age of air, the
average transit time for transport through the stratosphere, calculated from
an inert tracer with a linearly increasing source in the model boundary layer
<xref ref-type="bibr" rid="bib1.bibx37" id="paren.23"><named-content content-type="pre">e.g., </named-content></xref>. CLaMS is a Lagrangian chemistry transport model
(CTM), based on 3-D forward trajectories, with an additional parameterization
for small-scale mixing, which depends on the deformation in the large-scale
flow. Vertical transport in the model is purely diabatic above about
300 hPa, with the total diabatic heating rates taken from ERA-Interim
forecast data. The vertical model resolution around the tropopause is about
400 m. For the simulation of CO, a lower boundary condition from MOPITT
(Measurements of Pollution in the Troposphere satellite experiment) is used
and chemical loss due to reaction with OH is included as described in
<xref ref-type="bibr" rid="bib1.bibx30" id="text.24"/>. CLaMS ozone includes a zero mixing ratio lower boundary
condition and a simplified chemistry comprising photolytical production and
loss due to the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> driven catalytic ozone loss cycle in the lower
stratosphere. For further details about this specific CLaMS simulation see
<xref ref-type="bibr" rid="bib1.bibx30" id="text.25"/>. In the UTLS, CLaMS CO and ozone agree well with various
observations, as shown in several recent publications
<xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx15" id="paren.26"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p>In addition, results will be compared to ozone observations from the
Microwave Limb Sounder (MLS) instrument onboard the Aura satellite version 3
data <xref ref-type="bibr" rid="bib1.bibx19" id="paren.27"><named-content content-type="pre">see e.g.,</named-content><named-content content-type="post">and
<uri>http://mls.jpl.nasa.gov/data/v3_data_quality_document.pdf</uri></named-content></xref>.
MLS scans about 3500 profiles per day providing a dense sampling of the
global atmosphere, including the Asian monsoon region. The vertical
resolution of MLS ozone is about 3 km. For MLS CO, a standard tropospheric
tracer for Asian monsoon studies, the vertical resolution is coarser
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>4.5</mml:mn></mml:mrow></mml:math></inline-formula> km) and therefore we focus on ozone for this study. MLS
profiles are originally on pressure levels and were interpolated to potential
temperature surfaces for the purpose of this study. For further details about
MLS data, see <xref ref-type="bibr" rid="bib1.bibx19" id="text.28"/>.</p>
</sec>
<sec id="Ch1.S3">
  <title>Trace gas confinement in the anticyclone and PV</title>
      <p>Figure <xref ref-type="fig" rid="Ch1.F2"/>a and b show the distributions of CLaMS CO and
ozone in the monsoon region on the 380 K isentrope on 6 July 2011. Clearly
visible is the positive anomaly of the tropospheric tracer CO and the
negative anomaly of the stratospheric tracer ozone in the monsoon
anticyclone, characteristic for strong tropospheric impact and confinement
within the anticyclone. Note that extratropical stratospheric air is advected
around the eastern flank of the anticyclone, transporting CO-poor and
ozone-rich air equatorwards. This transport has recently been shown to
strongly affect the ozone seasonality in the tropics
<xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx28 bib1.bibx1" id="paren.29"/>. Furthermore, poleward transport
of CO-rich air affects the trace gas composition of the lowermost
stratosphere and crucially depends on the CO lifetime
<xref ref-type="bibr" rid="bib1.bibx11" id="paren.30"><named-content content-type="pre">e.g.,</named-content></xref>. To create a similar map from ozone measurements,
we bin ozone observations from MLS between 4 and 8 July 2011 (using
version 3.3 data), in order to obtain sufficiently dense observations
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>c). Lower ozone mixing ratios in the model
compared to MLS are likely related to the broad satellite averaging kernel
and the zero mixing ratio boundary condition at the surface in the model
<xref ref-type="bibr" rid="bib1.bibx30" id="paren.31"/>. However, the patterns of the low ozone anomaly in the
monsoon anticyclone reliably agree between model simulations and observations
(note the 5-day average for the satellite data).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Maps of <bold>(a)</bold> CLaMS CO and <bold>(b)</bold> CLaMS ozone on the
380 K isentrope on 6 July 2011 within the Asian monsoon region. Selected
potential vorticity contours are shown in black (4, 7 PVU) and Montgomery
stream function contours in white (<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>3.6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>3.615</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). Arrows show horizontal wind. <bold>(c)</bold> Same but
for MLS ozone data sampled during the period 4–8 July 2011, with the MLS
data binned into 3<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> 6<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude/longitude bins
(bins without measurements are left white). Meteorological data are taken
from ERA-Interim. (Note the logarithmic color scale for
ozone.)</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f02.png"/>

      </fig>

      <p>Overlaid on the trace gas mixing ratios in Fig. <xref ref-type="fig" rid="Ch1.F2"/> are
contours of PV and Montgomery stream function. Both meteorological quantities
show strong anomalies within the monsoon. However, when compared to the trace
gas mixing ratio contours the PV contours agree better than the Montgomery
stream function contours, in particular for small-scale variations. Even the
separation of a smaller eddy to the east of the main anticyclone is well
reflected in the PV distribution. These small-scale eddies, frequently shed
from the main anticyclone, have the potential to transport air masses with
elevated mixing ratios of tropospheric trace gases (e.g., CO, H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O) rapidly
into the middle and high latitude lower stratosphere
<xref ref-type="bibr" rid="bib1.bibx29 bib1.bibx36" id="paren.32"><named-content content-type="pre">e.g.,</named-content></xref>. A close relation between the
distributions of CO and PV in the monsoon was already found by
<xref ref-type="bibr" rid="bib1.bibx8" id="text.33"/>. For these reasons, we use PV as a basis for defining a
criterion for the transport barrier in the Asian monsoon.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p><bold>(a)</bold> Ozone from MLS (solid) and CLaMS (dashed) vs. potential
vorticity in the Asian monsoon region (10–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and
10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) at 380 K, averaged over the period
4–8 June 2011. <bold>(b)</bold> Same but for the ozone gradient with respect to
potential vorticity. Red lines show the transport barrier determined from PV
(see text).</p></caption>
        <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f03.pdf"/>

      </fig>

      <p><?xmltex \hack{\newpage}?>Motivated by studies of the polar vortex where the transport barrier is
characterized by particularly steep gradients of conserved tracers, we map
MLS and CLaMS ozone vs. potential vorticity (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). This
mapping was carried out by binning all data from the Asian monsoon region at
380 K (10–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) with respect
to potential vorticity (bin size 0.1 PVU). Figure <xref ref-type="fig" rid="Ch1.F3"/> shows
that, despite the offset between CLaMS and MLS ozone mentioned above, there
is agreement in the main structure, with low ozone in the core of the
anticyclone (at low PV values) and higher mixing ratios towards higher PV. In
particular, there is evidence from model and observations for a two-step
increase of ozone mixing ratios, resulting in two separate maxima in the
gradient of ozone with respect to PV. The stronger maximum around 7 PVU is
related to the transport barrier at the subtropical jet <xref ref-type="bibr" rid="bib1.bibx17" id="paren.34"/>. The
secondary maximum occurs around 4 PVU. In the following, we will provide
evidence that this secondary maximum may be interpreted as the transport
barrier of the Asian monsoon anticyclone (red line shows the transport
barrier PV value, objectively determined using the criterion derived in the
following section).</p>
</sec>
<sec id="Ch1.S4">
  <title>A PV-gradient criterion for the Asian monsoon</title>
      <p>Motivated by the good agreement between the PV and trace gas variability in
the monsoon region (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) and the fact that PV is an
approximately conserved quantity, we follow the approach developed for the
polar vortex for deducing a transport barrier
<xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx20 bib1.bibx23" id="paren.35"><named-content content-type="pre">e.g.,</named-content></xref>. <xref ref-type="bibr" rid="bib1.bibx23" id="text.36"/> defined
the transport barrier of the vortex edge as the location of the largest
(isentropic) change in PV, with the additional constraint of close proximity
to a strong zonal jet. Recently, <xref ref-type="bibr" rid="bib1.bibx17" id="text.37"/> deduced the location of the
transport barrier for the subtropical jet using an analogous approach.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Illustration of the calculation of monsoon-centered equivalent
latitude from the area within PV-contours (see text for details). Color-coded
is the PV-field within the Asian monsoon region at 380 K (10–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N
and 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) averaged for 5–7 July 2011, with the
thick white contour highlighting 4 PVU. The thin white contour encloses the
region of lowest PV (<inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 2.2 PVU) indicating the anticyclone center. The
black contours show PV globally.</p></caption>
        <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f04.pdf"/>

      </fig>

      <p>The PV distribution on 6 July 2011 is shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/>,
illustrating the anomalously low PV in the Asian monsoon anticyclone. In a
first step, we restrict all fields to a region including the monsoon
anticyclone, which we define as 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>≤</mml:mo></mml:mrow></mml:math></inline-formula> 60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>≤</mml:mo></mml:mrow></mml:math></inline-formula> 160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> latitude, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> longitude) to eliminate
the interfering influence of low PV values near the equator. The PV
distribution on 6 July 2011 within this region is shown in
Fig. <xref ref-type="fig" rid="Ch1.F5"/>a (top). A similar definition of the Asian monsoon
area was used by <xref ref-type="bibr" rid="bib1.bibx8" id="text.38"/>. The chosen latitude–longitude range
includes the anticyclone for all days during summer 2011. Slight variations
to this range cause no significant change to our results.</p>
      <p>Following <xref ref-type="bibr" rid="bib1.bibx5" id="text.39"/>, we define a monsoon-centered equivalent
latitude <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of a given PV contour in the anticyclone as the
latitude of a circle around the North Pole enclosing the same area, as
illustrated in Fig. <xref ref-type="fig" rid="Ch1.F4"/> (here, the 4 PVU contour is mapped to
about <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 65<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). Hence, for a PV contour enclosing an
area <inline-formula><mml:math display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula>, the equivalent latitude is defined by <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">E</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>sin⁡</mml:mi><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">E</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being the Earth's radius.
Consequently, the center of the monsoon occurs at a monsoon equivalent
latitude of 90<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, corresponding to the location of minimum PV. In this
sense, PV and equivalent latitude are related to each other, exhibiting a
unique functional dependence PV(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) as shown in
Fig. <xref ref-type="fig" rid="Ch1.F5"/>a (bottom). As already noted above, PV increases
monotonically from low values in the center of the anticyclone to higher
values at its edge.</p>
      <p>For 6 July 2011, the gradient of PV with respect to <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>,
namely <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">PV</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, shows no clear
maximum which could be indicative for the anticyclone transport barrier,
besides the maximum around 50<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> equivalent latitude (about 7–8 PVU)
related to the subtropical jet <xref ref-type="bibr" rid="bib1.bibx17" id="paren.40"/>. The absence of a clear
secondary maximum, representing the anticyclone transport barrier, has
recently been attributed to the large dynamical variability of the anticyclone
<xref ref-type="bibr" rid="bib1.bibx8" id="paren.41"/>. However, if this variability is damped by averaging the PV
field over a time window of 3 days between 5 and 7 July 2011, a clear
secondary maximum in the PV gradient emerges around 65<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> equivalent
latitude (Fig. <xref ref-type="fig" rid="Ch1.F5"/>b, bottom). In the following, we
interpret this maximum as the transport barrier of the Asian monsoon
anticyclone, and show its physical significance by comparison to trace gas
distributions in Sect. <xref ref-type="sec" rid="Ch1.S5"/>.</p>
      <p>To calculate the time-averaged PV for different dates we use a variable time
window. Therefore, we define an optimal window for each date as the smallest
number of days (<inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>3 days at most) such that the PV-gradient maximum
exceeds the adjacent minima by 30 %. Figure <xref ref-type="fig" rid="Ch1.F6"/> illustrates
this procedure for the example of the 6 July 2011, confirming that for this
date a <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1-day average (3-day time window) results in the clearest
gradient maximum. If the time window chosen is too large (e.g., <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>3 days
in Fig. <xref ref-type="fig" rid="Ch1.F6"/>), the maximum in the PV gradient degrades again
because different dynamical conditions contribute to the average. For that
reason, we restrict the maximum averaging period to 7 days (given date
<inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>3 days). Notably, for some dates no time averaging is necessary to
determine a PV-gradient maximum.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p><bold>(a)</bold> Potential vorticity map at 380 K on 6 July 2011, in
the Asian monsoon region between 10–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and
10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (upper panel), and PV as a function of the
monsoon centered equivalent latitude (lower panel). Monsoon equivalent
latitude <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is calculated from the area within PV contours
(see text). Shown is PV(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) (black) together with the
respective PV gradient <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">PV</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
(red). Low PV and large <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> indicate the anticyclone center.
<bold>(b)</bold> Same as panel <bold>(a)</bold> but for the PV-field averaged between
5 and 7 July 2011. The anticyclone transport barrier, deduced from a local
maximum in the PV gradient (see text), is shown as white thick contours
(upper panels) and red solid vertical lines (lower panels), respectively.
White thin contours (upper panels) and red dashed lines (lower panels) show
5 PVU. Black dashed lines (lower panels) highlight particular PV values. The
PV-value of the barrier is given in the grey box.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f05.pdf"/>

      </fig>

      <p>We apply an additional constraint to exclude the subtropical jet from the
calculation, which generally shows much larger PV-gradient values than the
anticyclone transport barrier. Empirically, for the summer 2011 a PV-limit of
5 PVU reliably separates the monsoon transport barrier from the subtropical
jet at 380 K, as illustrated in Fig. <xref ref-type="fig" rid="Ch1.F5"/>b for 6 July. A
physical motivation for this constraint can be deduced from the horizontal
circulation (also averaged over <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 day, see Fig. <xref ref-type="fig" rid="Ch1.F7"/>), as
described in the following. Necessarily, the anticyclone transport barrier is
located within the region of anticyclonic motion (negative relative
vorticity), and hence in the equivalent latitude range where the circulation
decreases when moving away from the anticyclone center (hence, with
decreasing monsoon equivalent latitude). Consequently, the PV-gradient
maximum of the anticyclone transport barrier needs to be located at
equivalent latitudes larger than the minimum
circulation (4.8 PVU in Fig. <xref ref-type="fig" rid="Ch1.F7"/>). This circulation constraint
generally excludes the subtropical jet from the transport barrier
calculation. For simplicity, we use 5 PVU as an upper PV-limit for the
transport barrier calculation at 380 K in the following, which is a good
approximation of the circulation minimum. Note in addition that the second
derivative of the circulation with respect to equivalent latitude <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mo>∂</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula> is related to the first derivative of PV
(see Eq. <xref ref-type="disp-formula" rid="Ch1.E2"/>). Therefore, the transport barrier related to the
local maximum in the PV gradient can be approximated by the local maximum in
the second derivative of <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Γ</mml:mi></mml:math></inline-formula> (see Fig. <xref ref-type="fig" rid="Ch1.F7"/>, bottom),
providing a consistency check of our procedure.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6"><caption><p><bold>(a)</bold> Potential vorticity with respect to monsoon centered
equivalent latitude on the 380 K isentrope, with the PV field averaged over
different periods centered around 6 July 2011. <bold>(b)</bold> The corresponding
gradients of PV with respect to equivalent latitude. Vertical lines show the
PV-gradient maximum.</p></caption>
        <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f06.pdf"/>

      </fig>

      <p>A necessary condition for the transport barrier criterion to hold is the
existence of a strong PV anomaly. Therefore, the applicability is restricted
to a shallow layer around 380 K (see Fig. <xref ref-type="fig" rid="Ch1.F1"/>).
Figure <xref ref-type="fig" rid="Ch1.F8"/> compares PV and its gradient with respect to monsoon
equivalent latitude at different levels for 6 July 2011 (<inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 day). The PV-gradient based transport barrier turns out to be clearest at the 380 K
level, still detectable at 370 and 390 K, but becomes undetectable below
(360 K) and above (400 K). Strongest PV gradients at 380 K emerge not only
for the 6 July, but during the whole summer (not shown). Note that the
corresponding PV values change between different levels, due to the strong
dependence of PV on altitude. At levels of the subtropical jet core around
360 K, the strong jet to the north of the monsoon masks the existence of the
anticyclone transport barrier <xref ref-type="bibr" rid="bib1.bibx8" id="paren.42"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>Relative vorticity map at 380 K, in the Asian monsoon region
between 10–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E averaged over
5–7 July 2011 (upper panel). The lower panel shows the horizontal
circulation (calculated from area-integrated relative vorticity) as function
of the monsoon centered equivalent latitude (black) and the respective second
derivative (red). PV-values corresponding to the minimum circulation are
shown as thin grey contour (upper panel) and red dashed line (lower), and
PV-values corresponding to the maximum in the second derivative of the
circulation as thick grey contour (upper) and red solid line (lower). The
black contour (upper panel) shows the transport barrier PV deduced from the
maximum PV-gradient, for comparison. (See text for further
details).</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f07.pdf"/>

      </fig>

      <p>The tropopause within the monsoon is located at particularly high altitudes
(see Fig. <xref ref-type="fig" rid="Ch1.F1"/>). Compared to the zonal mean, the
tropopause is upward bulging in the monsoon anticyclone by about 20 K
potential temperature (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). Therefore, the
detectable PV-gradient-based transport barrier around 380 K is likely
related to the tropopause, with air masses inside the anticyclone being
tropospheric and surrounding air masses stratospheric. Consequently, the
diagnosed transport barrier can also be interpreted as a PV-based tropopause
definition. Although enhanced PV gradients as a measure for confinement of
air are detectable only within a shallow layer around the tropopause, the
transport processes in the Asian monsoon occur throughout a thick layer from
the surface to the lower stratosphere. As pointed out by <xref ref-type="bibr" rid="bib1.bibx32" id="text.43"/>,
the anticyclone at upper levels is strongly related to convective variability
below.</p>
      <p>To summarize, the minimum circulation (largest negative circulation values at
approximately 5 PVU) defines the <italic>anticyclone boundary</italic>. The
<italic>anticyclone transport barrier</italic> is then calculated from the
time-averaged PV field as the maximum PV gradient at PV values smaller than
5 PVU. The procedure is illustrated in Fig. <xref ref-type="fig" rid="Ch1.F9"/>, and generally
results in a well-defined PV-value (e.g., 4 PVU for 6 July 2011, see
Fig. <xref ref-type="fig" rid="Ch1.F5"/>b) characterizing the transport barrier for the
Asian monsoon anticyclone for most days between about mid-June and mid-August
2011. For some days during the summer season, however, no clear maximum
emerges in the PV-gradient even after averaging over a few days (see also
Fig. <xref ref-type="fig" rid="Ch1.F12"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p><bold>(a)</bold> Potential vorticity with respect to monsoon centered
equivalent latitude for 6 July 2011 (calculated from the 5–7 July average),
on different levels (360, 370, 380, 390, 400 K isentropes). <bold>(b)</bold> The
corresponding PV-gradients with respect to equivalent latitude. Vertical
lines show the gradient maxima (transport barriers).</p></caption>
        <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f08.pdf"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Method to localize the PV-based transport barrier in the Asian
monsoon anticyclone (at 380 K), summarized in four steps.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f09.pdf"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p><bold>(a)</bold> Potential vorticity maps at 380 K on 6, 9, 12, 15, 18,
and 21 July 2011. The thick white contour shows the calculated anticyclone
transport barrier (maximum PV gradient), the thin white contour 5 PVU.
<bold>(b)</bold> Maps of CO from CLaMS on the same days, with PV-based transport
barrier included as white contours.</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f10.png"/>

      </fig>

</sec>
<sec id="Ch1.S5">
  <title>PV-based transport barrier and relation to trace gases</title>
      <p>To investigate whether the diagnosed transport barrier is physically
meaningful, in the sense of separating air masses of different chemical
characteristics, we compare it to simulated CO in the Asian monsoon region.
Figure <xref ref-type="fig" rid="Ch1.F10"/> shows PV and CO maps at 380 K for the 6, 9, 12,
15, 18 and 21 July 2011, overlaid with the PV contours of the transport
barrier (thick white), as deduced for each date following the procedure
described in Sect. <xref ref-type="sec" rid="Ch1.S4"/>. First, the barrier calculated from the
time-averaged fields results in reasonable PV values also when compared to
the instantaneous PV maps on the particular days. Second, in the CO
distributions the diagnosed barrier separates the high mixing ratios in the
center of the anticyclone from the lower values around.</p>
      <p>The sequence of plots in Fig. <xref ref-type="fig" rid="Ch1.F10"/> illustrates the large
variability of the anticyclone, with frequent shedding of smaller scale
eddies (9 July) and even splits of the anticyclone (21 July). Also for days
of particularly large variability the diagnosed barrier separates well the core
region of the anticyclone, characterized by high CO mixing ratios, from
its surroundings. Even the shedding of the smaller eddy and the vortex split
are reflected in the transport barrier. It should be further noted that the
agreement between PV and CO is not perfect and that high CO mixing ratios may
extend outside the PV contour (e.g., on 18 July at the northeastern edge of
the anticyclone), a potential indication of the leakiness of the anticyclone
transport barrier.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p><bold>(a)</bold> Map of CO from CLaMS on the 380 K isentrope, with the
thick white contour showing the PV-value of maximum CO-gradient, the black
contour showing the PV-value of maximum PV-gradient (thin white line shows
5 PVU), averaged between 5 and 7 July 2011 at 380 K. The bottom panel shows
CO from CLaMS vs. monsoon centered equivalent latitude (black), and the
respective gradient (red). <bold>(b)</bold> Same for ozone from CLaMS, and
<bold>(c)</bold> for mean age from CLaMS. (The PV values of the maximum gradient
are given in the upper panels.)</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f11.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><caption><p><bold>(a)</bold> Time evolution of the gradient of PV with respect to
monsoon centered equivalent latitude <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as a function of PV
for the period 20 June to 20 August 2011 at 380 K (note the logarithmic
color scale). The same is shown for panels <bold>(b)</bold> CO, <bold>(c)</bold>
O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and <bold>(d)</bold> mean age. Symbols show the PV-gradient maximum (grey
diamonds), and the CO-gradient maximum (green crosses). The dashed line
highlights 5 PVU. Dates without a clear gradient maximum are left
white.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f12.pdf"/>

      </fig>

      <p>To investigate more quantitatively to what degree the transport barrier
deduced from PV is reflected in the CO distribution, we apply the barrier
calculation to CO, exemplarily for 6 July 2011. Therefore, we restrict the CO
field to the monsoon region, average over <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 days (5–7 July 2011),
transform to PV-based monsoon centered equivalent latitude
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, restrict to the anticyclonic region and calculate the
PV-value of the maximum CO gradient
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">CO</mml:mi><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.
Figure <xref ref-type="fig" rid="Ch1.F11"/>a shows that a clear CO-gradient maximum
emerges around 65<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, equivalent to a PV value of 4 PVU, in agreement
with the transport barrier deduced from the maximum PV-gradient. Likewise,
distributions of simulated ozone and mean age of air reflect the PV-based
transport barrier within the Asian monsoon region
(Fig. <xref ref-type="fig" rid="Ch1.F11"/>b, c).</p>
      <p>The PV-gradient based transport barrier for the Asian monsoon anticyclone has
been calculated for all days between 20 June and 20 August 2011. Before this
period and afterwards, almost no barrier could be found. CLaMS CO fields show
trace gas confinement inside the anticyclone from mid-June 2011 onwards, but
obviously the transport barrier during this early phase is not strong enough
to be detectable by our method. Likewise, following the main monsoon season
first the PV-gradient maximum vanishes (by mid–end of August) but trace gas
anomalies remain for a few weeks until mid-September. Hence, the degree of
confinement inside the anticyclone is strong enough for a PV-gradient maximum
to be detected only during the main monsoon season.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F12"/> (top) shows the evolution of the PV-gradient at
380 K over the summer season. Although the gradient maximum related to the
anticyclone barrier appears weaker during some periods, it shows smooth
subseasonal variability, with higher PV values (around 4 PVU) at the beginning
of July and the beginning of August and lower PV values (around 3.2 PVU) in mid
July and mid August. Significant subseasonal dynamic variability of the Asian
monsoon, occurring with a frequency of about 30 days, has been recently noted
by <xref ref-type="bibr" rid="bib1.bibx8" id="text.44"/>. Only for a few days (end of June and beginning of
August) no transport barrier could be deduced because no clear maximum in the
PV gradient emerged.</p>
      <p>The evolution of the gradients of CO, ozone and mean age over the summer
(Fig. <xref ref-type="fig" rid="Ch1.F12"/>b–d) consistently shows a local maximum throughout
most of the season, coinciding well with the PV-based transport barrier.
However, by the end of July and after 15 August, there is additional
structure in the trace gas distributions at PV values above 4 PVU, which is
not reflected in the PV gradients. During these periods, the maximum trace
gas gradients are located at higher PV values than the PV-based transport
barrier. To what degree the strength of the anticyclone transport barrier can
be related to convection <xref ref-type="bibr" rid="bib1.bibx32" id="paren.45"><named-content content-type="pre">which increases the area of low PV values,
see</named-content></xref> and to other dynamical processes is beyond the scope of
this paper and needs to be further studied.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><caption><p>Transport barrier PV values for the Asian monsoon anticyclone at
380 K calculated from maximum PV and CO gradients and maximum-minimum ranges
for the years 2011–2013 (averages over all dates between 20 June and
20 August of each year where the transport barrier criterion holds).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">2011</oasis:entry>  
         <oasis:entry colname="col3">2012</oasis:entry>  
         <oasis:entry colname="col4">2013</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">PV–barrier/PVU</oasis:entry>  
         <oasis:entry colname="col2">3.6 (3.0–4.4)</oasis:entry>  
         <oasis:entry colname="col3">3.8 (2.6–4.4)</oasis:entry>  
         <oasis:entry colname="col4">3.5 (2.6–4.4)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">CO–barrier/PVU</oasis:entry>  
         <oasis:entry colname="col2">3.7 (3.2–4.4)</oasis:entry>  
         <oasis:entry colname="col3">3.7 (2.4–4.6)</oasis:entry>  
         <oasis:entry colname="col4">3.6 (2.6–4.2)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><caption><p><bold>(a)</bold> Occurrence frequency of the Asian monsoon anticyclone
at 380 K (in percentage of days) for the period between 20 June and
20 August 2011, calculated from the area covered by PV values lower than the
anticyclone transport barrier. Red contours show selected percentage values
(20, 40, 60, 80 %), the thick cyan contour shows the average PV value of
the barrier in the average PV field (average over the period considered). The
bottom panel shows the projection of anticyclone occurrence frequency onto
the longitude axis (bin size 2.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). <bold>(b)</bold> Occurrence frequency
for PV values below 0.5 PVU at 360 K isentrope, for the same period (cyan
contour shows 0.5 PVU in the average PV field).</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f13.pdf"/>

      </fig>

      <p>At 380 K, the PV value at the determined transport barrier is generally
found between about 3 and 4 PVU, and shows intraseasonal variability. The
mean PV value of the transport barrier over the summer 2011 is 3.6 PVU (at
380 K), in very good agreement with the mean PV of the related CO-gradient
maximum (Table <xref ref-type="table" rid="Ch1.T1"/>). We calculated the transport barrier PV
values also for summers 2012 and 2013 (see Table <xref ref-type="table" rid="Ch1.T1"/>) and
found some weak interannual variability which needs to be further
investigated. Note that the interannual variability and model-projected
future changes of the Asian monsoon anticyclone are largely uncertain,
hitherto <xref ref-type="bibr" rid="bib1.bibx18" id="paren.46"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
</sec>
<sec id="Ch1.S6">
  <title>Anticyclone location probability</title>
      <p>The location probability for the region enclosed by the transport barrier
(“anticyclone core region”, in the following) is shown in
Fig. <xref ref-type="fig" rid="Ch1.F13"/>. Presented is the local frequency of occurrence
for PV values lower than the anticyclone barrier value, in units of
percentage of days during summer 2011 (20 June to 20 August 2011). Clearly,
the largest probability of being located inside the anticyclone core occurs
around 70<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E/30<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N (above 80 % of the considered days).
The whole region between about 25–40<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 20–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E is
located within the anticyclone core for more than 50 % of the days. Note
that the anticyclone location probability may show significant interannual
variability (e.g., a broader distribution in longitude in 2012 compared to
2011 and 2013) which needs to be further studied.</p>
      <p><xref ref-type="bibr" rid="bib1.bibx40" id="text.47"/> and <xref ref-type="bibr" rid="bib1.bibx39" id="text.48"/> found an enhanced probability for the
anticyclone center (estimated as geopotential height maximum) to occur at
longitudes of the Tibetan (around 70–100<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) and the Iranian
(around 45–65<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) plateaus, resulting in a bimodal longitude
occurrence frequency. Figure <xref ref-type="fig" rid="Ch1.F13"/>a shows no enhanced
probability for the anticyclone core region to be located in these two
regions. However, if projected onto the longitude axis, the anticyclone
location probability indicates two weak maxima
(Fig. <xref ref-type="fig" rid="Ch1.F13"/>a/bottom), located at about 55 and 85<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E.
To what degree the bimodality in the longitudinal geopotential height maximum
distribution found by <xref ref-type="bibr" rid="bib1.bibx40" id="text.49"/> has a physical basis, originating
from enhanced occurrence probability in particular geographic regions, or is
an artifact of the projection needs to be further studied.</p>
      <p>Note that the large zonal extent of the anticyclone occurrence probability at
380 K in Fig. <xref ref-type="fig" rid="Ch1.F13"/>a is related to frequent eddy shedding
events, with the above analysis not distinguishing between the main
anticyclone and westward and eastward traveling eddies. Also note that at
lower levels (e.g., at 360 K in Fig. <xref ref-type="fig" rid="Ch1.F13"/>b) the region of
lowest PV values is more confined and located further eastward and southward
above the Tibetan plateau and Northern India, within the region of the
vertical conduit for upward transport in the monsoon proposed by
<xref ref-type="bibr" rid="bib1.bibx3" id="text.50"/>.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S7">
  <title>Discussion</title>
      <p>Recently, <xref ref-type="bibr" rid="bib1.bibx3" id="text.51"/> showed evidence for upward transport in the
Asian monsoon occurring in a vertical conduit separated from the main
anticyclone. Hence, it is not the anticyclone itself but this conduit which
defines the most efficient pathway of polluted surface air to higher
altitudes. However, as the air is released from the conduit at greater
altitudes, it stays confined and chemically isolated, at least to some
degree, inside the anticyclone, as shown from trace gas observations
<xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx27" id="paren.52"><named-content content-type="pre">e.g.,</named-content></xref>. Therefore, a complete understanding of
pollution transport from the boundary layer into the stratosphere requires
understanding of the confinement inside the upper level anticyclone.</p>
      <p>In this paper, we investigated to what extent meteorological fields and trace
gas distributions reflect the existence of a barrier to (quasi-) horizontal
transport along isentropic surfaces in the Asian monsoon anticyclone. We
refined the methodology developed for the polar vortex by additional
constraints (e.g., time averaging, restriction to anticyclone) and found a
secondary maximum besides the subtropical jet maximum in the gradient of
potential vorticity with respect to a monsoon-centered equivalent latitude
(related to the area enclosed within PV contours). We interpreted this
PV-gradient maximum as the transport barrier in the monsoon anticyclone. This
PV-gradient based transport barrier for the monsoon is deducible in a layer
around the tropopause (around 380 K) for most days between mid-June to mid-August 2011.</p>
      <p>However, the PV-gradient based transport barrier, and hence the related
confinement of air masses, in the monsoon anticyclone appears much weaker
than the transport barrier at the edge of the polar vortex
<xref ref-type="bibr" rid="bib1.bibx23" id="paren.53"><named-content content-type="pre">e.g.,</named-content></xref> and also weaker than the barrier at the subtropical
jet <xref ref-type="bibr" rid="bib1.bibx17" id="paren.54"><named-content content-type="pre">see</named-content></xref>, likely related to the large dynamic variability
of the monsoon anticyclone. Daily maps of the anticyclone show large
displacements in east-west direction, shedding of smaller-scale eddies and
even splits (Fig. <xref ref-type="fig" rid="Ch1.F10"/>), frequently causing air masses to be
torn out of the anticyclone. In particular the strong diabatic heating
related to deep convection over South Asia affects the anticyclonic monsoon
circulation <xref ref-type="bibr" rid="bib1.bibx32" id="paren.55"/> and potentially the strength of the
transport barrier (e.g., Fig. <xref ref-type="fig" rid="Ch1.F12"/>). Hence, the anticyclone
transport barrier turns out to be leaky, allowing cross-barrier transport to
some degree, and the maximum PV gradient is better interpreted as a measure
of the degree of confinement of the air masses than describing a rigid
barrier to the flow. Nonetheless, for the sake of clear terminology we use
the term “barrier” throughout this study.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14"><caption><p>Time evolution of the gradient of ozone from MLS with respect to
monsoon equivalent latitude (based on ERA-Interim PV) for June–August 2011
at 380 K (note the logarithmic color scale). At each date, MLS measurements
from 2 days before to 2 days later have been collected, to yield a sufficient
coverage of the monsoon region. Grey symbols show the PV-gradient
maximum.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f14.pdf"/>

      </fig>

      <p>Despite the leakiness of the barrier, diagnosing the corresponding PV-value
offers a method for separating the core of the monsoon anticyclone from its
surroundings. Hence, the size of the anticyclone core may be determined and
air masses may be appropriately tagged. This offers new opportunities for
model studies of Asian monsoon impact and for evaluation of measurements from
the monsoon region. The degree of confinement inside the anticyclone further
determines how effectively air masses from the anticyclone core mix with air
from the anticyclone edge. Air masses from different transport pathways may
be injected into different regions of the anticyclone (e.g., into the core by
convection and upwelling within the conduit <xref ref-type="bibr" rid="bib1.bibx3" id="paren.56"/>, or into the
anticyclone edge by typhoons over Southeast Asia <xref ref-type="bibr" rid="bib1.bibx36" id="paren.57"/>).
Therefore, chemical reactions and lifetimes of short-lived species, and the
effectivity of pollution transport into the stratosphere will depend on the
degree of confinement.</p>
      <p>The smooth evolution of the anticyclone transport barrier over the season
(Fig. <xref ref-type="fig" rid="Ch1.F12"/>) enhances our confidence in its relation to a
physical mechanism. Furthermore, enhanced gradients in CLaMS simulated trace
gas distributions (CO, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and mean age) clearly demonstrate the existence
of the PV-gradient based transport barrier. These enhanced trace gas
gradients are reflected in corresponding minima in mixing ratio PDFs (see
Appendix). However, a proper validation of the meaningfulness of the
diagnosed transport barrier can only be achieved by comparison to trace gas
measurements. Figure <xref ref-type="fig" rid="Ch1.F14"/> compares the gradient (with
respect to monsoon equivalent latitude) of MLS observed ozone in the monsoon
region to the PV-based transport barrier (grey symbols), similarly to
Fig. <xref ref-type="fig" rid="Ch1.F3"/> but for the entire season. Maximum ozone and PV
gradients agree well during the beginning of July and the middle to end of July.
During mid-August, the PV-based barrier is located at higher PV values,
but shows a similar temporal evolution as the maximum ozone gradient.</p>
      <p>The disagreements between the model and MLS are not unexpected, mainly
because of the different resolutions (e.g., vertical resolution around the
tropopause of about 400 m in CLaMS vs. about 3 km in MLS). Nonetheless, MLS
ozone shows enhanced gradients coinciding with the PV value of the transport
barrier over several days, providing further confidence in the PV-based
anticyclone transport barrier. Further analysis of observations of higher
resolution (e.g., in situ observations) would be desirable.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S8" sec-type="conclusions">
  <title>Conclusions</title>
      <p>As shown by anomalies in several trace gas observations, the air inside the
Asian monsoon anticyclone appears, at least to some degree, confined and
isolated from its surroundings. Diagnosing the related transport barrier
offers new opportunities for quantifying the transport of tropospheric source
gases into the UTLS (e.g., determining anticyclone size, tagging air masses).
In this paper, we showed that the potential vorticity field reflects the
existence of a barrier to horizontal transport between the anticyclone and
its surroundings. Although the detection of the transport barrier is hampered
by the large dynamic variability of the anticyclone and the proximity to the
subtropical jet, a refined PV-gradient criterion may be used to deduce the
barrier within the Asian<?xmltex \hack{\vadjust{\newpage}}?> monsoon anticyclone, in a
layer around 380 K. Therefore, we refined the criterion developed for the
polar vortex <xref ref-type="bibr" rid="bib1.bibx23" id="paren.58"><named-content content-type="pre">e.g.,</named-content></xref> and determined the anticyclone
transport barrier from the PV-gradient maximum, after restricting the PV
field to the monsoon region and averaging over a time window around the given
date (summarized in Fig. <xref ref-type="fig" rid="Ch1.F9"/>). Comparison to trace gas
distributions shows that the PV-gradient based transport barrier is
meaningful in the sense of separating air masses of different chemical
characteristics. The deduced PV values (e.g., 3.6 on average for 2011 at
380 K) offer a physically motivated criterion to separate the inner core of
the anticyclone from the surrounding region, crucial for the interpretation
of trace gas observations and for model studies.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <title>Transport barrier from trace gas mixing ratio PDF</title>
      <p>To further increase the confidence in the existence of the PV-gradient
transport barrier, we deduce the anticyclone transport barrier also from
simulated CO using a different methodology based on probability density
functions (PDF) and show its consistency with the PV-based results <xref ref-type="bibr" rid="bib1.bibx34" id="paren.59"><named-content content-type="pre">for
a review of the PDF method, see</named-content></xref>. Therefore, we calculate the
PDF of CLaMS simulated CO mixing ratios in the Asian monsoon region
(10–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–160<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) for a <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1-day time
window around 6 July 2011 (Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/>). The PDF was constructed
after assigning the appropriate area-weighting to the data points. Mean CO
monotonically decreases with increasing PV, with high CO inside the monsoon
(coinciding with low PV) and low CO outside. Minima in the mixing ratio PDF
indicate regions of suppressed horizontal transport <xref ref-type="bibr" rid="bib1.bibx34" id="paren.60"/>.</p>
      <p>The PDF in Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/> shows one minimum at CO mixing ratios around
35–40 ppbv, related to the subtropical jet, and a secondary minimum around
55 ppbv, related to the transport barrier inside the Asian monsoon
anticyclone. From the PDF of PV values corresponding to CO mixing ratios
around the minimum, we find a corresponding PV value of 4.1 PVU, in good
agreement to the 4 PVU emerging from the PV-gradient maximum
(Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/>/bottom).</p>
      <p>For 6 July, the CO PDF shows the anticyclone transport barrier even for the
instantaneous distribution, without averaging over <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 days (not shown).
Note that the PDF approach is related to the PV-gradient method
<xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx25" id="paren.61"><named-content content-type="pre">e.g.,</named-content></xref>.</p><?xmltex \hack{\newpage}?>
      <p><?xmltex \hack{\noindent}?>Still, the comparison between the two methods shows the
robustness of the deduced transport barrier. Similarly to the PV-based
approach, the PDF approach fails in locating a transport barrier at several
days during summer. The use of mixing ratio PDF's offers a simple method to
deduce the anticyclone transport barrier from satellite observations.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F1"><caption><p>Asian monsoon transport barrier at 380 K on 6 July 2011 from the CO
mixing ratio PDF. The main panel (upper left) shows CLaMS CO (monsoon region
average, 5–7 July time average) vs. PV with one standard deviation as grey
shading. The upper right panel shows the corresponding mixing ratio PDF with
the monsoon transport barrier highlighted as red dashed line. The lower panel
shows the PDF of PV-values around the barrier (between the thin red lines in
the upper right panel). (See text for further details.)</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13145/2015/acp-15-13145-2015-f15.pdf"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><ack><title>Acknowledgements</title><p>We thank Bernard Legras for advice, Nicole Thomas for programming support and
the ECWMF for providing reanalysis data. We further thank Gloria Manney and
two anonymous reviewers for their helpful and constructive comments on the
manuscript. F. Ploeger was funded by an HGF postdoc grant, and further thanks
go to the HGF for supporting a research stay at the Laboratoire de Météorologie
Dynamique of the École Normale Supérieure in Paris during which parts of
this work had been carried out.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?>The article
processing charges for this open-access <?xmltex \hack{\newline}?>
publication were
covered by a Research <?xmltex \hack{\newline}?>
Centre of the Helmholtz Association.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: T. J. Dunkerton</p></ack><ref-list>
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<abstract-html><h6 xmlns="http://www.w3.org/1999/xhtml" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:svg="http://www.w3.org/2000/svg">Abstract. </h6><p xmlns="http://www.w3.org/1999/xhtml" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:svg="http://www.w3.org/2000/svg" class="p">The Asian summer monsoon provides an important pathway of tropospheric source
gases and pollution into the lower stratosphere. This transport is
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confinement inside a large-scale anticyclonic circulation in the upper
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potential vorticity (PV), following methods developed for the polar vortex
<cite class="cite">e.g.,</cite>. The monsoon anticyclone is dynamically highly
variable and the maximum in the PV gradient is weak, such that additional
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the monsoon anticyclone agree well with contours of trace gas mixing ratios
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transport model (CLaMS) and satellite observations from the Microwave Limb
Sounder (MLS) instrument. Hence, the PV-based transport barrier reflects the
separation between air inside the core of the anticyclone and the background
atmosphere well. For the summer season 2011 we find an average PV value of
3.6 PVU for the transport barrier in the anticyclone on the 380 K
isentrope.</p></abstract-html>
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