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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-15-13519-2015</article-id><title-group><article-title>OMI tropospheric NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> profiles from cloud slicing: constraints
on surface emissions, convective transport and lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula></article-title>
      </title-group><?xmltex \runningtitle{OMI tropospheric NO${}_{{2}}$ profiles from cloud slicing}?><?xmltex \runningauthor{M.~Belmonte Rivas et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Belmonte Rivas</surname><given-names>M.</given-names></name>
          <email>belmonte@knmi.nl</email>
        <ext-link>https://orcid.org/0000-0003-0528-3858</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Veefkind</surname><given-names>P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Eskes</surname><given-names>H.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8743-4455</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Levelt</surname><given-names>P.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Technical University of Delft, Delft, the Netherlands</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Royal Netherlands Meteorology Institute, De Bilt, the Netherlands</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">M. Belmonte Rivas (belmonte@knmi.nl)</corresp></author-notes><pub-date><day>9</day><month>December</month><year>2015</year></pub-date>
      
      <volume>15</volume>
      <issue>23</issue>
      <fpage>13519</fpage><lpage>13553</lpage>
      <history>
        <date date-type="received"><day>2</day><month>February</month><year>2015</year></date>
           <date date-type="rev-request"><day>17</day><month>March</month><year>2015</year></date>
           <date date-type="rev-recd"><day>30</day><month>October</month><year>2015</year></date>
           <date date-type="accepted"><day>20</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/.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>We derive annual and seasonal global climatologies of tropospheric NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
profiles from OMI cloudy observations for the year 2006 using the cloud-slicing method on six pressure levels centered at about 280, 380, 500, 620, 720
and 820 hPa. A comparison between OMI and the TM4 model tropospheric
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> profiles reveals striking overall similarities, which confer great
confidence to the cloud-slicing approach to provide details that pertain to
annual as well as seasonal means, along with localized discrepancies that
seem to probe into particular model processes. Anomalies detected at the
lowest levels can be traced to deficiencies in the model surface emission
inventory, at mid-tropospheric levels to convective transport and horizontal
advective diffusion, and at the upper tropospheric levels to model lightning
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production and the placement of deeply transported NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> plumes
such as from the Asian summer monsoon. The vertical information contained in
the OMI cloud-sliced NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> profiles provides a global observational
constraint that can be used to evaluate chemistry transport models (CTMs) and
guide the development of key parameterization schemes.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\allowdisplaybreaks}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Global maps of tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical column densities (VCDs)
derived from satellite UV–vis nadir sounders such as OMI, GOME and SCIAMACHY
have contributed to the development of a variety of applications. Clear-sky
observations of tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs, those with cloud fractions
typically below 25 %, have been used to constrain surface NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission
inventories (Martin et al., 2003; Mijling and van der A, 2012; Miyazaki
et al., 2012), detect and monitor point source emission trends (Richter
et al., 2005; van der A et al., 2008) and constrain surface <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
lifetimes (Beirle et al., 2011), to cite a few examples. Still, cloudy
conditions predominate, which prevent the detection of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
concentrations at the surface. For OMI, more than 70 % of the
measurements collected in the extratropics are affected by clouds and
typically discarded, with the consequent loss of information. The utilization
of cloudy data from satellite IR and UV–vis nadir sounders provides access to
a large repository of observations with potential to reveal information about
trace gas concentrations at different altitudes and to constrain the
parameterizations of a number of cloud-related processes.</p>
      <p>Clouds are introduced in general circulation models (GCMs) because of their
broadband radiative effects and direct relation with the water vapor
feedbacks and precipitation (Jakob, 2003). Clouds also affect the
redistribution of trace gases via convection and interaction with chemistry,
which are essential elements in chemistry transport models (CTMs). Convective
transport of polluted plumes (including NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, but also HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, CO and
non-methane hydrocarbons – NMHCs) from the boundary layer can cause substantial
enhancement of upper tropospheric ozone, an important anthropogenic
greenhouse gas (Pickering et al., 1992). At high altitudes, enhanced chemical
lifetimes and stronger winds are also responsible for the long-range
transport of pollutants. Still, the exchange between environment and cloud air
that determines the way that convective columns evolve (i.e., the entrainment
and detrainment rates in mass flux schemes) remains uncertain. The presence
of convective clouds not only transports pollutants vertically but also
removes soluble species (like <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) by precipitation, and modulates
photolysis rates by altering the actinic fluxes above and below the cloud
(Tie et al., 2003). Associated with the deepest convective clouds, the
production of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> by lightning is a key component of the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
budget in the upper troposphere, not only because of its relation with
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production but also because it affects the general oxidizing capacity
of the atmosphere and the lifetimes of tracers destroyed by reactions with OH
– like CO, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Yet the source strength and spatial
distribution of lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions remain uncertain – with a global
best estimate of <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Tg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">a</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (Schumann and Huntrieser,
2007).</p>
      <p>In large-scale global CTMs, convection and other cloud-related processes such
as scavenging and lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production are represented by subgrid
parameterizations. Most convective parameterizations are tested against
temperature and humidity profiles from radiosondes (Folkins et al., 2006),
but chemical tracers provide additional constraints. A number of studies have
tried to quantify the effect of different convective schemes on tropospheric
CO and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles using satellite-based climatologies for comparison
with model data (Mahowald et al., 1995; Barret et al., 2010; Hoyle et al.,
2011), finding the largest discrepancies in the tropical middle and upper
troposphere. Even though <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> may appear unsuitable as a tracer of air
motion because of its high reactivity with other NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> members (such as
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, PAN, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>) and the
presence of time-varying sources (mainly surface emissions and lightning
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, but also aircraft and stratospheric inflows), its short lifetime
makes it attractive to study very fast transport mechanisms like convection.
A number of studies have demonstrated the capabilities of satellite UV–vis
sounders to estimate the source strength and 3-D distribution of lightning
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> over cloudy scenes (Boersma et al., 2005; Beirle et al., 2006; Martin
et al., 2007; Miyazaki et al., 2014). These studies have found good agreement
between modeled and observed lightning <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over the tropical
continents – albeit with discrepancies in the geographical and vertical
distributions. Other studies have compared the performance of lightning
parameterizations against satellite lightning flash densities, like Tost
et al. (2007) and Murray et al. (2012), concluding that it is difficult to
find a good combination of convective and lightning scheme that accurately
reproduces the observed lightning distributions – leaving the problem of the
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> yield per flash aside. Thus there is a clear need for measurements with
which the development of model parameterizations of convective transport and
lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> schemes can be guided.</p>
      <p>In this paper, we use a variation of the cloud-slicing technique first
developed by Ziemke et al. (2001) for tropospheric ozone, and later
exploited by Liu et al. (2014) for tropospheric CO and Choi
et al. (2014) for tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, based on the increments of
gas vertical column density above cloud as a function of cloud
pressure within a certain longitude/latitude/time cell. Obviously,
large cloud fractions and some degree of cloud height diversity within
the cell are conditions required for this technique to produce useful
results. The cloud-slicing approach applied by Choi et al. (2014) on
OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> data was able to find signatures of uplifted
anthropogenic and lightning <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in their global
free-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations, as well as in a number
of tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles over selected regions. In this
work, global annual and seasonal <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> volume mixing ratio (VMR) profiles are generated at
a spatial resolution of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> on pressure
levels centered at about 280, 380, 500, 620, 720 and 820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>. We
give particular consideration to the scattering sensitivity of the OMI
measurements above the cloud, as well as to the representativity of
the cloud-sliced profiles with regard to a cloudy atmosphere. We
report on results from this methodology as well as its direct
applicability as an observational constraint using a state-of-the-art
chemical transport model.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methodology</title>
      <p>The methodology to produce observed and modeled climatologies
of tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR profiles under cloudy scenes begins
with a description of the OMI and TM4 data sets involved. We introduce
the pre-processing steps required to estimate <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above
cloud from OMI slant column measurements, followed by the upscaling
steps required to bring the spatial resolution of the satellite
observations in line with the TM4 model grid for comparison.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Cloud pressure intervals and mean cloud pressure levels used for
cloud slicing (hPa): the VCD pressure interval gives the boundaries of the
cloud pressure bin. The VMR pressure interval refers to where the VMR is
assumed constant after the pressure difference.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">VCD pressure interval</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> VCD pressure <inline-formula><mml:math display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">VMR pressure interval</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> VMR pressure <inline-formula><mml:math display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Level 1</oasis:entry>  
         <oasis:entry colname="col2">Tropopause–380</oasis:entry>  
         <oasis:entry colname="col3">330</oasis:entry>  
         <oasis:entry colname="col4">Tropopause–330</oasis:entry>  
         <oasis:entry colname="col5">280</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Level 2</oasis:entry>  
         <oasis:entry colname="col2">380–500</oasis:entry>  
         <oasis:entry colname="col3">450</oasis:entry>  
         <oasis:entry colname="col4">330–450</oasis:entry>  
         <oasis:entry colname="col5">380</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Level 3</oasis:entry>  
         <oasis:entry colname="col2">500–620</oasis:entry>  
         <oasis:entry colname="col3">570</oasis:entry>  
         <oasis:entry colname="col4">450–570</oasis:entry>  
         <oasis:entry colname="col5">500</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Level 4</oasis:entry>  
         <oasis:entry colname="col2">620–720</oasis:entry>  
         <oasis:entry colname="col3">670</oasis:entry>  
         <oasis:entry colname="col4">570–670</oasis:entry>  
         <oasis:entry colname="col5">620</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Level 5</oasis:entry>  
         <oasis:entry colname="col2">720–820</oasis:entry>  
         <oasis:entry colname="col3">770</oasis:entry>  
         <oasis:entry colname="col4">670–770</oasis:entry>  
         <oasis:entry colname="col5">720</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Level 6</oasis:entry>  
         <oasis:entry colname="col2">820–1000</oasis:entry>  
         <oasis:entry colname="col3">870</oasis:entry>  
         <oasis:entry colname="col4">770–870</oasis:entry>  
         <oasis:entry colname="col5">820</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<sec id="Ch1.S2.SSx1" specific-use="unnumbered">
  <?xmltex \opttitle{OMI NO${}_{2}$ products}?><title>OMI NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> products</title>
      <p>The <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> slant columns used in this work are retrieved by the UV–vis
spectrometer OMI (Ozone Monitoring Instrument; Levelt et al., 2006) according
to KNMI DOMINO version 2.0 (Boersma et al., 2007, 2011). The data files,
which include total and stratospheric slant columns, averaging kernel
information, cloud fraction, cloud pressure and assimilated trace gas
profiles from the TM4 model, are available at
<uri>http://www.temis.nl/airpollution/no2.html</uri>.</p>
      <p>Of particular importance to this study are the cloud pressures and fractions
retrieved by the OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud algorithm (Acarreta et al.,
2004). The OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud algorithm uses an optically thick
Lambertian cloud model with a fixed albedo of 0.8; the fraction of this
Lambertian cloud model covering the pixel is called effective cloud fraction
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mtext>eff</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mtext>obs</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mtext>cloudy</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mtext>clear</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>), where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mtext>cloudy</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mtext>clear</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> are
modeled clear- and cloudy-sky reflectances, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mtext>obs</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the
observed continuum reflectance – i.e., the reflectance with the
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> absorption line removed), which is not the same as the
geometric cloud fraction but an equivalent amount that yields the same
top-of-atmosphere (TOA) reflectance as observations; the altitude level of the
Lambertian cloud model is then adjusted so that it results in the same amount
of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> absorption as in observations (Stammes et al.,
2008). The OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud pressure refers to the optical
radiative cloud pressure near the mid-level of the cloud and below the MODIS
infrared-based cloud top, which is about 250 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> higher than OMI for
deep convective clouds or about 50–70 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> higher for extratropical
mid-level clouds. The OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud pressure has been
validated against PARASOL with a mean difference below 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> and
a SD below 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> (Stammes et al., 2008). The OMI
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud fraction has been validated against MODIS with
a mean difference of 0.01 and SD of 0.12 over cloudy scenes (effective cloud
fractions larger than 50 % without surface snow or ice) (Sneep et al.,
2008). In this paper, we use the cloud radiance fraction defined as CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mtext>eff</mml:mtext></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>R</mml:mi><mml:mtext>cloudy</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mtext>obs</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> – which represents the
weight of the air mass factor of the cloudy part.</p>
</sec>
<sec id="Ch1.S2.SSx2" specific-use="unnumbered">
  <title>TM4 model</title>
      <p>The TM4 chemistry transport model has a spatial resolution of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">3</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> with 35 sigma pressure levels up to 0.38 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> (and
approximately 15 levels in the troposphere) driven by temperature and winds
from ECMWF reanalyses and assimilated OMI stratospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
information from previous orbits. The tropospheric chemistry scheme is based
on Houweling et al. (1998) using the POET emissions (Olivier et al., 2003)
database based on the EDGAR inventory for anthropogenic sources, which are
typical of years 1990–1995, with biomass emissions of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> based on ATSR
fire counts over 1997–2003 and released in the lowest model layers. The
photolysis rates are calculated as in Landgraf and Crutzen (1998) and
modified as in Krol and van Weele  (1997). In the TM4 model, the physical
parameterization for convective tracer transport is calculated with a mass
flux scheme that accounts for shallow, mid-level and deep convection
(Tiedtke, 1989). Large-scale advection of tracers is performed by using the
slopes scheme of Russell and Lerner (1981). The lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production
is parameterized according to Meijer et al. (2001) using a linear
relationship between lightning intensity and convective precipitation, with
marine lightning 10 times less active than continental lightning and scaled
to a total annual of 5 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Tg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">N</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (Boersma et al., 2005). The
vertical lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> profile for injection into the model is an
approximation of the outflow profile suggested by <?xmltex \hack{\mbox\bgroup}?>Pickering<?xmltex \hack{\egroup}?> et al. (1998).
Including free-tropospheric emissions from air traffic and lightning, the
total NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions for 1997 amount to 46 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Tg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">N</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. More
about this model may be found in Boersma et al. (2011) and references
therein.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Latitude–height section of annual zonal mean OMI cloud frequencies
(CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> %) – observed during daytime around 13:45 LST. On the left
in red, the bottom pressure boundaries for the calculation of annual mean
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above cloud (after Table 1). On the right in blue, the
approximate pressure for the resulting <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR after differentiation
of VCDs (also after Table 1).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS1">
  <title>Cloud slicing</title>
      <p>A technique initially developed for estimating upper tropospheric
ozone using nadir sounders (Ziemke et al., 2001), cloud slicing
consists in arranging collections of trace gas VCDs measured above
clouds against cloud pressure over a certain area and time period in
order to estimate a gas VMR via the pressure
derivative as

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mtext>VMR</mml:mtext><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>=</mml:mo><mml:mn>0.1</mml:mn><mml:mi>g</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>A</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mtext>VCD</mml:mtext></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mo>=</mml:mo><mml:mn>9.8</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn>28.97</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">mol</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>6.022</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>23</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">molec</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">mol</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> with VCD
expressed in <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">molec</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and cloud pressure expressed in hPa. The
method determines an average trace gas volume mixing ratio over a certain
area, time period and cloud pressure interval (Choi et al., 2014). In this
paper, annual average tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD lat–long grids from OMI and
TM4 are produced for six tropospheric layers with bottom cloud pressures
located within pressure intervals centered at about 330, 450, 570, 670, 770
and 870 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>. The cloud pressure intervals used for cloud slicing were
chosen after several trial runs and are laid out in Table 1 and Fig. 1. An
annual climatology of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR profiles is then estimated after
differencing the annual tropospheric VCD arrays above cloud with respect to
pressure.</p>
      <p>Figure 1 shows the latitude–height section of annual zonal mean OMI
cloud frequency for the year 2006, showing that cloud slicing does not
provide uniform global sampling. Most high clouds (mainly deep
cumulus, since cirrus clouds pass generally undetected by OMI) occur along
the Intertropical Convergence Zone (ITCZ) near the Equator and over
tropical continents, but can also be seen in the mid-latitude storm
track regions and over mid-latitude continents in the summer;
mid-level clouds are prominent in the mid-latitude storm tracks, usually
guided by the tropospheric westerly jets, and some occur in the ITCZ; and
low clouds, including shallow cumulus and stratiform clouds, occur
essentially over the oceans but are most prevalent over cooler
subtropical oceans and in polar regions (Boucher et al., 2013). In
summary, cloud sampling proves best at low to mid-altitudes in the
extratropics and mid- to high altitudes in the deep tropics. However, cloud sampling is typically poor off the west coasts of
subtropical (Pacific, Atlantic and Indian) landmasses at high
altitudes – which are areas of large-scale subsidence with persistent
low stratocumulus, and at low altitudes over the tropical landmasses,
particularly the Amazon Basin and central Africa.</p>
<sec id="Ch1.S2.SS1.SSS1">
  <?xmltex \opttitle{NO${}_{{2}}$ above cloud}?><title>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> above cloud</title>
      <p>The tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical column density above the cloud,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, for an instrument like OMI is defined here
as a function of the total slant column, SCD, as

                  <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mtext>SCD</mml:mtext><mml:mo>-</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>strat</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>strat</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the stratospheric slant column,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> accounts for the slant surface component leaked
from below the cloud (i.e., the amount of surface signal that seeps through
the cloud for partially cloudy conditions), and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>
denotes the scattering sensitivity above the cloud. The stratospheric slant
column arises from TM4 model stratospheric profiles assimilated to OMI
observations over unpolluted areas (Belmonte Rivas et al., 2014). The
below-cloud leaked component is defined as

                  <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>=</mml:mo></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>ground</mml:mtext><mml:mtext>CLP</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mtext>corr</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where CRF is the cloud radiance fraction, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the clear-sky component of the scattering sensitivity (purely dependent on Rayleigh
scattering and surface albedo), <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the a priori trace gas profile
(i.e., the TM4 model), and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>corr</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the OMI temperature correction
defined below. Note that the summation goes from the ground to the cloud
level pressure, CLP (see Fig. 2), where the cloud level is given by the OMI
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud pressure.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Schematic diagram of the scattering sensitivity above and below the
cloud (normalized by the geometric air mass factor): CLP is the cloud level
pressure, and <inline-formula><mml:math display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> is the total scattering sensitivity, usually defined as
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:mtext>CRF</mml:mtext><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloudy</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. The red curve
illustrates a residual sensitivity to <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> contents below the cloud
when conditions are partially cloudy.</p></caption>
            <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f02.png"/>

          </fig>

      <p>The scattering sensitivity above the cloud, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, is
defined as (see Appendix)

                  <disp-formula id="Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>m</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mtext>corr</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> is the total scattering sensitivity (usually defined as
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:mtext>CRF</mml:mtext><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloudy</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> as in Boersma
et al., 2004). Note that the summation in this case goes from cloud level to
the tropopause (see Fig. 2). The total scattering sensitivity <inline-formula><mml:math display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> has been
derived from the averaging kernel <inline-formula><mml:math display="inline"><mml:mrow><mml:mtext>AK</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> as

                  <disp-formula id="Ch1.E5" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>m</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mtext>AK</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mtext>AMF</mml:mtext></mml:mrow><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>corr</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where AMF is the total air mass factor (used to compute the total vertical
column VCD <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> SCD <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> AMF from the total slant column SCD, and different
from the tropospheric air mass factor <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> used to
compute <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>). The temperature correction is defined as in
Boersma et al. (2004) and accounts for the temperature dependence of the
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> absorption cross section and its influence on the retrieved slant
column using ECMWF temperatures:

                  <disp-formula id="Ch1.E6" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>corr</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mn>220</mml:mn><mml:mo>-</mml:mo><mml:mn>11.4</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mo>[</mml:mo><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn>11.4</mml:mn><mml:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>The elements of the averaging kernel contain the height dependent
sensitivity of the satellite observation to changes in tracer
concentrations and they are calculated with a version of the Doubling
Adding KNMI (DAK) radiative transfer model in combination with TM4-simulated tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles. Of central importance to
our cloud-slicing approach is that a below-cloud leaked component
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>) is removed from the tropospheric slant
column, and a scattering sensitivity above the cloud
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>) is used to estimate the vertical column
density above the cloud, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. This is in
contrast with the methodology applied in Choi et al. (2014), where
below-cloud leakages are neglected (making tropospheric estimates more
sensitive to surface contamination, particularly at low cloud
fractions), and the scattering sensitivity above the cloud is assumed
equal to the geometric air mass factor.</p>
      <p>As far as model quantities are concerned, the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column above
the cloud in TM4 is simply calculated as

                  <disp-formula id="Ch1.E7" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the a priori trace gas profile (i.e., the TM4 model). Note
that the a priori gas profiles, originally reported on hybrid sigma pressure
grids, have been resampled onto a uniform pressure grid with steps of
23.75 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> to simplify averaging operations. The cloud level pressure
(CLP) that defines the model above-cloud <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns in
Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) is the same OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud pressure used
for cloud slicing. Using OMI's cloud information to sample the TM4 model
amounts to assuming that cloud altitudes and fractions in the model are
identical to those observed by OMI. We know that differences between
instantaneous model and observed cloud fields can be notable, but we also
know that current model cloud fields are able to reproduce the average
geographical and vertical distribution of observed cloud amounts reasonably
well (Boersma et al., 2015), albeit with reports of underestimation of the
low-level cloud fractions in the marine stratocumulus regions, underestimation of
the mid-level cloud fractions everywhere, and slight overestimation of the
high-level cloud fraction over the deep tropics (Nam et al., 2014) – errors that
are likely related to the microphysical cloud and convection
parameterizations. Therefore, using an observed cloud field to probe into
model cloud processes, though probably suboptimal in case-by-case studies, is
likely to be fine in an average sense.</p>
</sec>
<sec id="Ch1.S2.SS1.SSS2">
  <title>Spatial averaging</title>
      <p>A comparison of OMI observations with a model such as TM4 should also
take into account the inhomogeneity of the tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
field, which is usually large due to the presence of strong point
sources and weather-scale variability. The model <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns
should be viewed as areal averages, given that the limit of scales
represented in the model is given by its resolution. Thus it is
important to aggregate OMI observations to attain the same spatial
resolution used by the model. The OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD above-cloud
observations (with a nominal spatial resolution of
13 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> at the swath center) are
aggregated onto daily <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">1</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">1</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>
longitude–latitude bins – later spatially smoothed to <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> – before comparison with the afternoon TM4 model
outputs defined on a <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">3</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> grid on a daily
basis as in Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>). The aggregated OMI product collects all
VCDs observed within a specified period (1 day) with solar zenith
angle less than 70<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, surface albedo less than 30 % and CRF
larger than 20 % at the OMI pixel level (roughly equivalent to an
effective cloud fraction of 10 %, which is a minimum condition for
cloud fraction and pressure to be properly reported by OMI). No
weighting is applied. At this point, populating the grid bins with as
many OMI measurements as possible is important in order to avoid
spatial representation errors between the two records (a partially
filled bin may not be representative of what occurs over the entire
cell, which is what the model represents). The aggregated CRFs (and all
other OMI and model quantities) are then evaluated at grid resolution,
and a CRF threshold of 50 % at cell level is applied to both
observations and model data. The annual mean tropospheric VCD above
cloud is then calculated per pressure layer using the CLP thresholds
specified in Table 1 on daily gridded OMI and TM4 <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD
outputs, provided there are at least 30 measurements in a bin.</p>
</sec>
<sec id="Ch1.S2.SS1.SSS3">
  <title>Error analysis</title>
      <p>In the cloud-slicing method, the derivation of annual mean VMR
profiles from annual layered VCD amounts above cloud follows as

                  <disp-formula id="Ch1.E8" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mtext>VMR</mml:mtext><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>C</mml:mi><mml:mfenced close=")" open="("><mml:mo>〈</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>〉</mml:mo><mml:mo>-</mml:mo><mml:mo>〈</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo></mml:mfenced></mml:mrow><mml:mrow><mml:mfenced close=")" open="("><mml:mo>〈</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>〉</mml:mo><mml:mo>-</mml:mo><mml:mo>〈</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is defined as <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>0.1</mml:mn><mml:mi>g</mml:mi><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as
in Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) and the index <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> refers to the cloud level. We term these
objects VMR pseudoprofiles because they are constructed on the conditional
provision of cloud presence, and the presence of cloud modifies the
underlying <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profile: either directly via chemical or dynamical
processes such as lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production, advection of (clean/polluted)
air from below, suppression of biomass burning or decreased photolysis under
the cloud, or more indirectly via selective sampling of seasonal features,
such as entangling a wet season column of enhanced lightning at high altitude
with a dry season column of enhanced biomass burning at low altitude. One can
appreciate that the effect of cloud presence on the profile varies with cloud
altitude, which is unfortunate, because we use changes in cloud altitude to
sample the underlying profile. This state of affairs introduces a source of
systematic error between the cloud-slicing estimate (i.e., the pseudoprofile)
and the actual underlying profile, which we term pseudoprofile error. One may
evaluate (and further compensate for) the pseudoprofile error associated with
conditional cloud sampling by comparing the model VMR profile sampled using
the cloud-slicing technique against the underlying “true” mean <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
VMR profile from the same model, as described below. Other sources of
systematic error may also intervene, including uncertainties in the a priori
corrections and errors in the stratospheric column. The effect of
uncertainties in the a priori corrections is limited by the impact that a
priori corrections have on pseudoprofiles, which is itself limited (see
Supplement). The effect of errors in the stratospheric column is expected to
be small, since stratospheric columns only show a small additive bias
(Belmonte Rivas et al., 2014) that is bound to cancel via the pressure
difference. One could also include temporal representativity errors from
mismatched collocations between model and OMI clouds in this category, which
Boersma et al. (2015) estimate to lie around 10 %. In this section we
provide a brief description of the retrieval error that may be expected from
instrumental random noise properties alone, followed by an estimate of
pseudoprofile error that is based on model behavior.</p>
</sec>
<sec id="Ch1.S2.SS1.SSSx1" specific-use="unnumbered">
  <title>Retrieval error</title>
      <p>The retrieval error in the annual mean cloud-slicing profiles is assumed
random and calculated by standard error propagation of Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>). Note that we do not
compute VMRs on daily or orbital basis (since one does not achieve the necessary cloud
height diversity but in exceptional circumstances), but from the difference of annual mean
VCDs. The derivation follows as

                  <disp-formula specific-use="align"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mtext>VMR</mml:mtext></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mn>0.1</mml:mn><mml:mi>g</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>A</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">δ</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>annual</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>annual</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mn>0.1</mml:mn><mml:mi>g</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>A</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced open="(" close=""><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mfenced close=")" open="("><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced open="." close=")"><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mfenced open="(" close=")"><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mfenced open="(" close=")"><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">δ</mml:mi><mml:mfenced close=")" open="("><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mn>0.1</mml:mn><mml:mi>g</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>A</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close="" open="("><mml:mn mathvariant="normal">2</mml:mn><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>annual</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced open="." close=")"><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mfenced close=")" open="("><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mfenced open="(" close=")"><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">δ</mml:mi><mml:msub><mml:mi>p</mml:mi><mml:mtext>annual</mml:mtext></mml:msub></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p>where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are all mean
annual quantities estimated for contiguous pressure levels. Assuming random
Gaussian errors in the determination of single OMI observations with an
uncertainty (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>VCD) of 50 % in the OMI vertical column density
(Boersma, 2004) and an uncertainty (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:math></inline-formula>) of 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in
O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> cloud pressure (Stammes et al., 2008), the standard error of the
mean annual quantity (VCD or pressure) is the standard error of the single
retrieval divided by the square root of the number of OMI measurements
collected per grid cell <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>grid</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> in a year:

                  <disp-formula specific-use="gather"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>annual</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mtext>VCD</mml:mtext><mml:mo>/</mml:mo><mml:msqrt><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>grid</mml:mtext></mml:msub></mml:mrow></mml:msqrt></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msub><mml:mi>p</mml:mi><mml:mtext>annual</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>p</mml:mi><mml:mo>/</mml:mo><mml:msqrt><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>grid</mml:mtext></mml:msub></mml:mrow></mml:msqrt><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

              Thus we obtain

                  <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E9"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mtext>VMR</mml:mtext><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mn>0.1</mml:mn><mml:mi>g</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>air</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>A</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mn mathvariant="normal">2</mml:mn><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mtext>VCD</mml:mtext></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>VCD</mml:mtext></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:msqrt><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mtext>grid</mml:mtext></mml:msub></mml:mrow></mml:msqrt></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S2.SS1.SSSx2" specific-use="unnumbered">
  <title>Pseudoprofile (systematic) error</title>
      <p>The extent to which cloud-slicing profiles remain
physical and accurate representations of an average cloudy atmosphere
is limited by the assumptions that underlie the cloud-slicing
difference, which can be expressed as

                  <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E10"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mtext>VMR</mml:mtext><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mo>(</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>∝</mml:mo><mml:mtext>VCD</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mtext>VCD</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p>In cloud slicing, the mean VMR between the pressure levels
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is given by the difference between
the VCD above cloud pressure <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, provided there is cloud
at <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and the VCD above cloud pressure <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>,
provided there is cloud at <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> too. The problem is that
the presence of cloud modifies the profile. One may think that the
column difference in Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>) is an approximation to what
happens when clouds are located at <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, somewhere between
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. But assuming that the trace gas
concentration profile does not change with small changes in cloud
altitude (which are otherwise necessary to estimate the VMR slope)
entails some error. Ideally, we would like to calculate

                  <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E11"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>true</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>∝</mml:mo><mml:mtext>VCD</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mtext>VCD</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p>Now we have a unique (and physically plausible) cloud condition behind
the difference, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and a VMR estimate
that is representative of gas concentration provided that there are
clouds at the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> level. Yet if we would like to obtain
a VMR estimate that is representative of trace gas concentration in
a general cloudy atmosphere, then we would calculate

                  <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E12"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>mid</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>∝</mml:mo><mml:mtext>VCD</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>dn</mml:mtext></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:mo>∀</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mtext>VCD</mml:mtext><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>up</mml:mtext></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:mo>∀</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p> </p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f03-part01.jpg"/>

          </fig>

<?xmltex \hack{\addtocounter{figure}{-1}}?><?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p><bold>(a)</bold> OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above cloud – average quantities
for the year 2006: for high-altitude clouds (top row, 330 and
450 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>), mid-altitude clouds (middle row, 570 and 670 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>)
and low clouds (bottom row, 770 and 870 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>). Gray means no data
available (i.e., insufficient number of cloud detections in the cell).
<bold>(b)</bold> Same as <bold>(a)</bold> but for TM4.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f03-part02.jpg"/>

          </fig>

      <p>That is, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> represents a mean VMR profile
provided that there are clouds anywhere in the column, i.e., regardless
of cloud altitude. We refer to the difference between VMR and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>true</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> as sampling error, because the cloud diversity
necessary to estimate the trace gas concentration is distorting the
underlying profile. We refer to the difference between
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>true</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> as
representation error, because a profile measured under high-cloud
conditions is not representative of a profile under low-cloud
conditions, nor in general representative of an average cloudy
state. The sum of the sampling and representation errors, that is,
the difference between the cloud-sliced VMR pseudoprofile and
the average profile in a cloudy atmosphere <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>,
is what we call the pseudoprofile error. All VMR,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>true</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> profiles can
be calculated on account of the TM4 CTM, so that a model-based
estimation of the sampling and representation (pseudoprofile)
systematic errors becomes available. The general pattern of
pseudoprofile errors (see Sect. 3.3) indicates that biases are small
in the upper three levels, largely positive (100–200 %) over
tropical and extratropical outflows in the lower two levels, and
negative (up to 100 %) over the continents for the lower three
levels (particularly over central and South America, Australia, Canada
and Siberia). One way to bypass this systematic error is to scale the
observed VMR pseudoprofiles by the model profile-to-pseudoprofile
ratio as

                  <disp-formula id="Ch1.E13" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref,OMI</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>OMI</mml:mtext></mml:msub><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref,TM4</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>TM4</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>This model-based pseudoprofile correction (applied in Sect. 3.4)
remains subject to the accuracy with which the model represents its
own profiles, and should be treated with caution.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <?xmltex \opttitle{NO${}_{2}$ VCD above cloud}?><title>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCD above cloud</title>
      <p>Figure 3a shows the annual mean tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD aggregates
on <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">1</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">1</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> grids observed by OMI for the year
2006 above clouds with mean pressures centered at around 330, 450, 570,
670, 770 and 870 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> – see Fig. 1 and Table 1. A similar set
of annual mean <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above cloud has been extracted from
the TM4 model using identical cloud sampling (i.e., using the cloud
fraction and cloud pressure from OMI) for comparison (see Fig. 3b).</p>
      <p>Most of the lightning <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions are expected above clouds
higher than 450 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> (i.e., the upper two levels in Fig. 3a),
although some deep convection may also be present over strong
industrial sources (like the northeastern USA, Europe, China, and the
Johannesburg, South Africa, area) or biomass burning sources in central Africa, the
Amazon Basin or northeastern India, complicating the problem of process
attribution.</p>
      <p>The two middle levels in Fig. 3a are expected to carry, along with the
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> burden inherited from the upper levels, additional
signatures from frontal uplifting into the mid-troposphere by conveyor
belts over major industrial sources in the northeastern USA, central Europe
and China, as well as convective transport of biomass burning sources
over central Africa, South America, Indonesia and northern
Australia. The strong convective signatures of surface industrial and
biomass burning sources, along with their low tropospheric outflows,
dominate the two lowest levels in Fig. 3a. Note the extensive lack of
data over the tropical continents at low altitudes, a region where
persistent high cloud precludes penetration into the lowest levels,
and over the subtropical subsidence areas.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Tropospheric scattering sensitivities above cloud level
(AMF<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mtext>above</mml:mtext></mml:msub><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula> AMF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>geo</mml:mtext></mml:msub></mml:math></inline-formula> in Eq. <xref ref-type="disp-formula" rid="Ch1.E4"/>): for high-altitude clouds (top row, 330 and 450 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>), mid-altitude clouds
(middle row, 570 and 670 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) and low clouds (bottom row, 770 and
870 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f04.jpg"/>

        </fig>

      <p>By differencing the annual average VCD arrays with respect to
pressure, we expect to separate the contributions from different
altitudes to the total tropospheric column. But before that, let us take a look
at the scattering sensitivities above cloud and the effects of
correcting for below-cloud leakage in these results. Figure 4 shows the
annual mean tropospheric scattering sensitivity above cloud level
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> in Eq. <xref ref-type="disp-formula" rid="Ch1.E4"/>) applied to generate the
OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs shown in Fig. 3a. Globally, the tropospheric
scattering sensitivity above the cloud does not deviate by more than 10 % from the geometric air mass factor at most cloud altitudes,
except at the lowest levels, where it suffers reductions of up to
30 %. This reduction in scattering sensitivity at the lowest cloud
levels may come as a surprise, particularly when clouds are known to
boost the scattering sensitivity just above the cloud top. However,
the pronounced decrease in scattering sensitivity at the lowest cloud
levels is related to penetration of substantial amounts of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
(from strong or elevated surface sources) into the cloud mid-level,
where extinction acts to reduce the scattering sensitivity. Other than
the extinction effect, the variability in scattering sensitivity is
governed by changes in the observation geometry
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> decreases as the sun angle increases) and
the temperature correction introduced in Eq. (<xref ref-type="disp-formula" rid="Ch1.E6"/>), which is
responsible for the subtropical bands and the variability at high
southern latitudes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p> </p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f05-part01.jpg"/>

        </fig>

<?xmltex \hack{\addtocounter{figure}{-1}}?><?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p> </p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f05-part02.jpg"/>

        </fig>

      <p>The corrections for the surface leaked component introduced in
Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) are largest (see Supplement) over polluted regions for the
highest clouds (up to 50–66 %) and smallest over clean areas
like the oceans. In order to verify that the model-based below-cloud
leak corrections do not appreciably change the OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs
arrays, we have performed a separate trial run where the CRF threshold
(at grid level) is increased from 50 to 80 % (see Supplement) to conclude that none
of the prominent VCD signatures seen in Fig. 3a (or none of the VMR
features that we will see later) changes appreciably in the restricted
CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>80</mml:mn></mml:mrow></mml:math></inline-formula> % case. Results from the CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>80</mml:mn></mml:mrow></mml:math></inline-formula> % trial run
include notably diminished cloud frequencies and spatial coverage,
seriously thinning the population that produces the annual averages
and generally damaging their representativity. This effect is
particularly notable in the upper two levels (280 and 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>)
and to lesser extent over the large-scale subsidence area in the
lowest level, since deep convective and low marine stratocumulus
clouds are not particularly extensive but have a preference for low
effective cloud fractions. Excluding the contributions from these
cloud types in the CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>80</mml:mn></mml:mrow></mml:math></inline-formula> % case does not change the
mid-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> patterns relative to the CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> % case, but it biases the OMI aggregates in the upper
troposphere low relative to the modeled average, which is not
particularly sensitive to this change. In summary, the CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>80</mml:mn></mml:mrow></mml:math></inline-formula> %
trial run does not show any clear signs of a priori information constraining
the results, but it provides hints of results being influenced detrimentally
by the lower sampling densities afforded by a higher CRF threshold.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <?xmltex \opttitle{NO${}_{2}$ VMR pseudoprofiles}?><title>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VMR pseudoprofiles</title>
      <p>The annual mean tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR pseudoprofiles observed
by OMI for the year 2006 are compared against their TM4 model
counterparts in Fig. 5a–c. Note that pseudoprofile errors do not
affect this comparison, since both observed and modeled pseudoprofiles
are observing identical (if somewhat unphysical, because of sampling
and representation issues) atmospheric states. After the pressure difference,
there remain some instances where negative VMRs are found, but these are
mainly associated with poorly populated cells (such as at high latitudes, near
the tropics at low altitudes, or around subsidence regions). These instances are
identified and dealt with by recourse to information from nearby cells, when available,
or otherwise ignored.</p>
      <p>Many of the cloud-slicing features observed at the upper two levels
(280 and 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) in Fig. 5a can be attributed to actual
biomass burning, lightning and deep convection. It may be difficult to
separate these components clearly without a proper seasonal analysis
(deferred to Sect. 3.6), although one can identify areas of predominant lightning production as
those regions that do not seem connected via convection to surface
sources underneath and use the LIS-OTD flash rate climatology and the
ATSR fire counts (see Fig. 6 below) as interpretation aids for
attribution. Positive anomalies (observations larger than modeled
amounts) are detected in Fig. 5a over all major industrial areas
(eastern USA, central Europe and eastern China) both at 280 and
380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> levels, suggesting that deep transport of boundary
layer <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> may be too weak in the model. However, there
are extensive negative anomalies (meaning observations lower than
modeled amounts) in background upper tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> both at
280 and 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>, which is consistent with reports of model
overestimation of the amount of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> attributed to lightning
over the tropical oceans in Boersma (2005).</p><?xmltex \hack{\addtocounter{figure}{-1}}?><?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p><bold>(a)</bold> Upper cloud levels (280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> left,
380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> right): OMI vs. model <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMRs (OMI top, TM4 middle,
difference bottom) average quantities for the year 2006. <bold>(b)</bold> Same as
<bold>(a)</bold> but for middle cloud levels (500 hPa left, 620 hPa right).
<bold>(c)</bold> Same as <bold>(a)</bold> but for lower cloud levels
(720 hPa left, 820 hPa right).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f05-part03.png"/>

        </fig>

      <p>Negative anomalies in Fig. 5a are particularly large over Siberia,
Amazonia and the Bay of Bengal. The negative anomaly over eastern
Siberia, an area of predominant biomass burning, could be related to
excessive fire-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission over boreal forests in the
model (Huijnen et al., 2012). In South America, lightning <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
contributions seen by OMI appear confined mostly to the western
equatorial coast (Peru, Ecuador and Colombia) on the one hand, and
southern Brazil and off the east coast of Uruguay on the other hand
(more in line with the LIS-OTD flash climatology shown in Fig. 6) –
in stark contrast with model amounts, which locate the lightning
maximum further to the north over the Brazilian Matto Grosso, where
the maxima in precipitation related to the South American monsoon
system usually takes place. It is worth noting that the lightning
intensity in the TM4 model is solely driven by convective
precipitation, although Albrecht et al. (2011) report that convective
precipitation is not always well correlated with lightning in this
area, showing that the most efficient storms in producing lightning
per rainfall are located in the south regions of Brazil. The negative
anomaly over Amazonia is therefore very likely related to problems
with the TM4 lightning scheme. The negative anomaly over the Bay of Bengal, an area of maxima in precipitation related to the Indian monsoon,
could also be a reflection of excess model lightning linked to
convection.</p>
      <p>Other notable discrepancies in Fig. 5a include positive anomalies over
central Africa and northeastern India at 280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.
Over central Africa, the pattern of positive anomalies
bears only partial resemblance to the pattern of biomass burning
emission underneath (see mid-level OMI VMRs in Fig. 5b) – suggesting
that upper level positive anomalies in central Africa may be related
more to deficiencies in the lightning scheme than to convective
transport. Actually, Barret et al. (2010) report that lightning flash
frequencies simulated by TM4 are lower than measured by the LIS
climatology over the southern Sahel, which is consistent with our
observations. On the other hand, the large positive anomaly observed
over the Tibetan Plateau at 280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>, which significantly
deviates from the LIS-OTD flash rate climatology in the area (confined
to the Himalayan foothills only), is very likely an effect of deep
transport associated with the Asian monsoon. The model does show an
enhancement in upper tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over India, but not
moving far enough north into the Tibetan Plateau and failing to
reproduce the strong enhancements in upper tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
over northeastern India and southern China related to the Asian summer
monsoon plume – which Kar et al. (2004) also detected in the MOPITT
CO profiles.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>Interpretation aids for process attribution: mean flash rate climatology
(1998–2010) from the LIS-OTD sensor (left; Cecil et al., 2014) and fire count
climatology (1997–2003) from the ATSR sensor (right; Arino et al., 2012).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f06.png"/>

        </fig>

      <p>The cloud-slicing features observed at the mid-tropospheric levels
(500 and 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) in Fig. 5b may be mostly attributed to
mid-tropospheric convection of strong surface sources and their
associated outflows. We observe a remarkable agreement between model
and observations on the localization and intensity of major convective
signals over industrial sources (eastern USA, central Europe, China and
India) as well as over typical biomass burning sources in central
Africa, Indonesia and South America. Contrary to what is observed in
the upper levels (see prevalent negative anomalies in Fig. 5a), there
are extensive positive anomalies (meaning observations larger than
modeled amounts) in background middle tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> both at
500 and 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in Fig. 5b, particularly over the tropics and
subtropics – which is indicative of deficient model mid-tropospheric
outflows at these levels. Positive anomalies over the continents are
particularly large over China (with an outflow-related positive
anomaly downwind over the Pacific), the central USA, and the biomass
burning regions in central Africa and South America. While it may be
more or less clear that enhanced mid-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
concentrations observed over the oceans are related to enhanced
convective inflows into this level (without definitely discarding
a problem with <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> lifetime), the origin of the convective
anomalies remains ambiguous. A cursory look at the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
concentrations observed at lower levels might help determine
whether flux anomalies into the mid-troposphere are related to
deficiencies in model-prescribed surface emissions or problems with
the convective transport scheme, or both.</p>
      <p>For example, the pattern of anomalies over China at lowest levels (see
Fig. 5c) is prominently positive, but it carries a dipolar positive–negative
(China–Japan) pattern that is no longer observed at
higher levels. Thus, while it is possible that some of the
mid-tropospheric convective anomalies are a response to flux anomalies
carried from underneath (i.e., a deficiency in the originally
prescribed surface emission), as happens over the eastern USA and
Europe, where negative anomalies are carried upwards (see Fig. 5b),
the overall effect does not exclude net deficiencies in model
convective transport. As far as biomass burning is concerned, the
pattern of anomalies over central Africa and South America in the
lowest tropospheric levels (see Fig. 5c) is unfortunately not as
evident (given the lack of low-cloud detections) as over China but
mostly neutral or slightly negative, indicating that mid-tropospheric
positive anomalies in this area respond to either a convective
transport scheme that is too weak or a model injection height that is
too low.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p><bold>(a)</bold> Classification EOFs: surface source, outflow, high/low outflow, and middle outflow.
<bold>(b)</bold> Model-based classes based on EOF decomposition of
model <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles under cloudy conditions: black (primary industrial),
red (secondary industrial), orange (biomass burning), ochre (Baykal Highway),
yellow (Indostan), light green (Middle East), green (tropical outflow), turquoise
(tropical subsidence), cyan (extratropical outflow), blue (boreal outflow),
and dark blue (clear background). Gray means unclassified.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f07.jpg"/>

        </fig>

      <p>The lower tropospheric levels (720 and 820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
sampled by the cloud-slicing technique are shown in Fig. 5c. These
levels sustain the highest <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations in the vicinity
of major industrial hubs (eastern USA, central Europe and China) and
the strongest anomalies as well, which in this case can be linked
directly to deficiencies in prescribed surface emissions. All major
features in the anomaly patterns at these levels can be matched
unambiguously to the pattern of OMI to TM4 total tropospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column differences for clear-sky conditions shown later in
Fig. 12, characterized by positive anomalies over the northeastern USA,
central Europe and Japan, and negative anomalies over China. These low-level signatures are consistent with <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increases over China,
India and the Middle East, and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> decreases over the eastern USA
and central Europe, which are not reflected in the model emission
inventory. Other salient features at these levels include an
interesting band of negative anomalies along the ITCZ (perhaps related
to rapid convective mixing of relative “clean” air from the boundary
layer) and extensive positive anomalies over the oceans (more so at
720 than at 820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) – revealing deficient model outflows at
high latitudes and suggesting that poleward transport of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
in the model may not be vigorous enough (a problem likely related to
horizontal diffusion in the model).</p>
      <p>In summary, there is remarkable agreement between observed and modeled
upper/middle/lower tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts, their main distributions
resembling each other at continental scale, with localized differences
suggesting that the cloud-slicing technique holds promise for testing model
features related to anthropogenic emission, convection and uplift, horizontal
advection and lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p>Model-based source and outflow class definitions based on EOF decomposition.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Class label</oasis:entry>  
         <oasis:entry colname="col2">Main condition</oasis:entry>  
         <oasis:entry colname="col3">Extra condition</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Primary industrial</oasis:entry>  
         <oasis:entry colname="col2">EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">USA, Europe, China</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Secondary industrial</oasis:entry>  
         <oasis:entry colname="col2">100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">USA, Europe, China</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Biomass burning</oasis:entry>  
         <oasis:entry colname="col2">100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">geographic</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Baykal highway</oasis:entry>  
         <oasis:entry colname="col2">100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">geographic</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Indostan</oasis:entry>  
         <oasis:entry colname="col2">100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">geographic</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Middle East</oasis:entry>  
         <oasis:entry colname="col2">100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">geographic</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Tropical outflow</oasis:entry>  
         <oasis:entry colname="col2">EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula>, EOF2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">EOF3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, EOF4 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Tropical subsidence</oasis:entry>  
         <oasis:entry colname="col2">EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula>, EOF2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">EOF3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Extratropical outflow</oasis:entry>  
         <oasis:entry colname="col2">EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula>, EOF2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">EOF3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, EOF4 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Boreal outflow</oasis:entry>  
         <oasis:entry colname="col2">EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula>, EOF2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">EOF3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≫</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Clean background</oasis:entry>  
         <oasis:entry colname="col2">EOF1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula>, EOF2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">pptv</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S3.SS3">
  <title>Classification</title>
      <p>In the previous section, we studied the geographical distribution of
observed and modeled <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts on different pressure
layers. In this section, we focus on the vertical dimension by looking
at <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR amounts across pressure layers. In order to
simplify the analysis, we have defined a set of geographical classes
based on the amount of variance contained in the TM4 model
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles. These classes characterize how much of the
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> content in the profile can be apportioned to surface
sources and how much to outflows – further subdivided into outflows
with low-, mid- or high-altitude components. Annual mean <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR
profiles are plotted for each class, along with reference to
pseudoprofile error. A standard empirical orthogonal function (EOF)
decomposition of the reference TM4 profiles (VMR<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>ref</mml:mtext></mml:msub></mml:math></inline-formula> in
Eq. <xref ref-type="disp-formula" rid="Ch1.E12"/>) is employed to characterize the geographical variance
of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical profiles under cloudy conditions and identify
major spatial patterns. The first four EOF eigenvectors (out of
a total of six) are shown in Fig. 7a. The first EOF represents
profiles with higher concentrations near the surface – a profile over
a surface source. The second EOF represents profiles with
concentrations uniformly distributed across the column – a profile
for a generic outflow type. The third and fourth EOF eigenvectors
divide the generic outflow type into subtypes with stronger high-altitude (EOF3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), low-altitude (EOF3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) or mid-tropospheric
(EOF4 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) components. The classes that result from applying masks
based on the conditions defined in Table 2 are shown in
Fig. 7b. According to the TM4 model, the classes containing all
primary and secondary industrial sources (i.e., strong projections on
EOF1) are mainly confined to the USA, Europe and China. Other secondary
industrial sources relate to India, the Middle East and the Baykal
Highway (a major road connecting Moscow to Irkutsk, passing through
Chelyabinsk, Omsk and Novosibirsk). Major biomass burning sources
include large sectors in Africa and South America, Indonesia, New
Guinea, and northern Australia. <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> outflows over the tropics
(i.e., strong projections on EOF2) are subdivided into generic tropical
outflows (with strong upper and mid-tropospheric components, or larger
projections on EOF3 and EOF4) and outflows over large-scale subsidence
areas (with stronger lower tropospheric components, or negative
projections on EOF3). The extratropical outflows differ from the
tropical outflows in that the sign of the mid-tropospheric projection
is reversed, so that extratropical profiles are more C-shaped
(according to the model). The boreal outflow differs from the
extratropical outflow in that it has an extremely large upper
tropospheric component (i.e., a very large projection on
EOF3). Finally, we have defined a separate class, labeled clean
background, including all those areas without significant projections
on either source or outflow eigenvectors.</p>
      <p>The average tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles estimated using the
cloud-slicing method on OMI and TM4 data sets for all the 11 classes
(15 classes when primary and secondary industrial regions are
subdivided geographically into China, USA and Europe subclasses)
defined in Table 2 and Fig. 7b are shown next in Figs. 8 and 9. These
plots compare the OMI and TM4 VMR pseudoprofile estimates calculated
in a cloud-slicing fashion as in Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>), along with the
reference TM4 <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> profile calculated as in
Eq. (<xref ref-type="disp-formula" rid="Ch1.E12"/>) for an average cloudy atmosphere. Recall that the
difference between the TM4 VMR and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VMR</mml:mtext><mml:mtext>ref</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> profiles
gives an indication of pseudoprofile error – or the representativity
of the cloud-slicing estimate relative to a general cloudy
situation. The OMI VMR cloud-slicing estimate is bounded by error bars
calculated from standard error propagation as in Eq. (<xref ref-type="disp-formula" rid="Ch1.E9"/>), and
scaling by the square root of the number of profiles collected per
grid cell – also shown in right subpanels in Figs. 8 and 9.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F11" specific-use="star"><caption><p>Cloud-slicing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR profiles for the year 2006 by class
(OMI pseudoprofile, dashed red line; TM4 pseudoprofile, dashed black line;
TM4 profile for cloudy conditions, continuous black line). The error bars show
random retrieval errors. The differences between continuous and dashed black
lines show systematic pseudoprofile errors. The subpanels on the right show the
average number of OMI observations collected per grid cell per year for that class.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f08.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p>Cloud-slicing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR profiles for year 2006 by class:
all primary sources (left), all secondary sources (middle) and all outflow
classes (right). (OMI pseudoprofile, dashed red line; TM4 pseudoprofile,
dashed black line; TM4 profile for cloudy conditions, continuous black line).
The error bars show random retrieval errors. The differences between continuous
and dashed black lines show systematic pseudoprofile errors.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f09.png"/>

        </fig>

      <p>The cloud-slicing estimates for the annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles
over primary industrial centers in the eastern USA, Europe and China are shown in
the first row in Fig. 8. There is a remarkably good correspondence between
observed and modeled tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles over these strongly
emitting areas, particularly over central Europe, attesting to the accuracy
and representativity of the cloud-slicing estimates for yearly means.
Pseudoprofile errors are small in these areas, so that cloud-slicing
estimates remain a good representation of average cloudy conditions. The OMI
to TM4 VMR differences at the lowest levels are consistent with known
deficiencies in model-prescribed surface emissions (OMI smaller than TM4
over the eastern USA and central Europe, but larger over China). These low-level
anomalies are carried upwards to a level of 500–600 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>, above which
the effects of enhanced convective mid-tropospheric and deep transport start
to dominate regardless of the signature of the surface difference. The second
row in Fig. 8 shows the annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles over
secondary industrial centers around eastern USA, Europe and China. The low-level features related to surface emission are identical to those of the
primary centers, but the signature of enhanced mid-tropospheric convection is
clearer – indicating that vertical transport in the model is too weak or
lifetime too short, regardless of the sign of the surface anomaly. The sign
of the OMI to TM4 difference is reversed in the upper two levels, in line
with the generalized model overestimation of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the upper
troposphere. The third row in Fig. 8 shows the cloud-slicing estimate for the
annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles over secondary industrial pollution
centers in India, the Middle East and the Baykal Highway – note that
pseudoprofile errors are larger in this case. For India, the differences
between OMI and TM4 profiles at low levels point to a large underestimation
of model surface emissions, and model overestimation of upper tropospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts – this upper level anomaly related to the misplaced
Asian summer monsoon signal, which in observations appears located over the
Tibetan Plateau. For the Middle East, the difference between OMI and TM4
profiles points to large differences at mid-tropospheric level (OMI larger
than TM4). The agreement between OMI and TM4 profiles for the Baykal Highway
class is reasonably good – allowing for a small underestimation of model
surface emissions. After deep transport in China, this is the class with
higher upper level <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts, most likely related to fire-induced
convection from boreal fires. The left panel in the fourth row in Fig. 8
shows the cloud-slicing estimate for the annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
profile over tropical biomass burning regions, featuring positive anomalies
at middle levels and negative anomalies at lower and upper levels, again
pointing at defective model convective transport into the mid-troposphere (or
issues with the pyro-convection height). The cloud-slicing estimates for
annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles over typical outflow regions are
shown in the middle and right panels in the fourth row (tropical and tropical
subsidence outflows) and left and middle panels in the fifth row
(extratropical and boreal outflows) in Fig. 8. As a salient feature, all of
the outflow profiles share a prominent mid-tropospheric plume centered at around
620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in the tropics and a little lower in the extratropics, around
720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>, with <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts much smaller than the model in the
upper troposphere and general agreement at the lowest level, producing
profiles which are generally S-shaped (instead of C-shaped as in the model).
The mid-tropospheric plume is likely related to enhanced convective fluxes of
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over industrial and biomass burning areas (but definitely not
discarding issues with <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> lifetime or substantial chemical NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
recycling from <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and PAN sources at this level). Note also the
generalized model overestimation of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the upper levels (tropical
and extratropical), which is consistent with reports of excess lightning
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production over the tropical oceans in Boersma et al. (2005). The
upper level overestimation is particularly large for the boreal outflow
class, which we also mentioned could be related to the excess fire-induced
convection over Siberia or too large NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factors. Finally, the
cloud-slicing estimate for the annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profile over
the clean Southern Ocean is shown in the right panel of the last row in
Fig. 8, with good agreement at the top levels and gradually increasing model
underestimation towards the surface, suggesting enhanced lateral
contributions at high latitudes from horizontal eddy diffusion.</p>
      <p>The left panel in Fig. 9 shows the annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
profile for all the primary surface sources together (eastern USA,
central Europe and China), indicating that differences at surface
level average out globally, leaving the effects of enhanced observed
mid-tropospheric convection and deep transport to stand out. The
signature of enhanced mid-tropospheric convection becomes even clearer
in the middle panel in Fig. 9, which shows the annual tropospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profile for all secondary surface sources together (around
primary sources, plus India, the Middle East, the Baykal Highway and
the biomass burning areas), where the signature of enhanced deep
transport is in this case replaced by model overestimation of upper
tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The model overestimation of upper level
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> appears clearly in the right panel in Fig. 9, which shows
the annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profile for all the outflow
classes, along with a prominent model underestimation of
mid-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels. In summary, and consistent with
our comments on Fig. 5a–c, the average profiles that result from
applying the cloud-slicing technique on observed OMI and modeled TM4
data sets show striking overall similarities, which confer great
confidence to the cloud-slicing approach, along with more localized
differences that probe into particular model processes and
parameterization schemes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><caption><p><bold>(a)</bold> Latitude–height cross section of annual zonal mean
tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR in logarithmic scale from TM4 (left) and OMI
(right) with CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> %. <bold>(b)</bold> Same as <bold>(a)</bold> but for
the remote Pacific sector (180–135 W).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f10.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><caption><p>Longitudinal cross section of annual mean tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
VMR in logarithmic scale from TM4 (left) and OMI (right) with CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> % over the tropics (10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–20<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f11.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <title>Cross sections</title>
      <p>We would like to wrap up our results in the form of observed and
modeled annual zonal mean and longitudinal <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cross sections
along the tropics (Figs. 10a, b and 11). Note that in order to bypass
pseudoprofile errors, the observed <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pseudoprofiles are
scaled in this section by the model profile-to-pseudoprofile ratio as
in Eq. (<xref ref-type="disp-formula" rid="Ch1.E13"/>) to form what is called the observation update.</p>
      <p>For the annual zonal mean tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the left-to-right panel
comparison in Fig. 10a shows that, although the observation update does not
change the strength of major industrial emission over the northern
mid-latitudes at the lowest levels, the associated convective cloud is
reaching higher in altitude. In the tropics and southern latitudes, vertical
transport of the combination of biomass burning and industrial emissions is
stronger and reaching higher – with a prominent high plume originating from
the Johannesburg area. The observation update does bring notably stronger
midtropospheric outflows distributed over a broader latitude band and weaker
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> signatures at high altitude. The enhanced mid-tropospheric plume
is best appreciated in Fig. 10b, which shows the annual zonal mean
tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> averaged over the Pacific Ocean sector
(180–135 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">W</mml:mi></mml:math></inline-formula>) – the dominant sources of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over the oceans
are thought to include the long-range transport from continental source
regions, as well as chemical recycling of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and PAN sources
(Staudt et al., 2003). Schultz et al. (1999) actually show that the
decomposition of PAN originating from biomass burning actually accounts for
most of the mid-tropospheric NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the remote southern Pacific, suggesting
that enhanced convective flux from surface sources may not be the only agent
responsible for the enhanced mid-tropospheric outflows observed by OMI.</p>
      <p>Figure 11 shows a picture for the annual longitudinal <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
cross section for tropical latitudes between 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and
20<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, where the observation update raises the convective
plumes from major biomass burning areas in South America, central
Africa and Indonesia/northern Australia to higher altitude, between
500 and 600 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>, with a slight westward tilt and longer
downstream transport of cloud outflow at upper levels caused by the
tropical easterly jet, and generally weaker <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> signatures at
high altitude.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15"><caption><p>Annual clear-sky OMI tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> total columns in
logarithmic scale for the year 2006.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f12.png"/>

        </fig>

      <p>In summary, the OMI cloud-slicing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles seem to suggest that
raising the polluted plumes to higher altitudes allows for much longer
residence and chemical lifetimes, and longer and more widely distributed
horizontal transport of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (following poleward advection and
dispersion by the subtropical jet and by baroclinic waves at lower levels) in
the mid-troposphere. These observations are in line with reports in Williams
et al. (2010) showing that the underestimation of upper tropospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in TM4 relative to observations over Africa may be linked to a too
weak convective uplift using the Tiedtke scheme. The studies of Tost
et al. (2007), Barret et al. (2010) and Hoyle et al. (2011) corroborate this
finding, indicating that the vertical extent of tropical convection and
associated transport of CO and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the middle and upper troposphere
is underestimated in Tiedtke-based models. Accurately constraining the
convective transport in CTMs should contribute to the determination of the
vertical distribution of lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, since knowledge of the extent of
mixing of air into the cloud as a function of altitude is required to
separate the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> produced by lightning from that produced by upward
transport (Dickerson, 1984).</p>
</sec>
<sec id="Ch1.S3.SS5">
  <title>Consistency check</title>
      <p>Because of the annual and global character of the OMI annual tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
profile climatology estimates, we do not have any
direct means to validate them in the same way as has been done,
for example, in Choi et al. (2014). But we can check their
consistency by demanding that the total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
column from the cloud-slicing technique does not deviate significantly
from the total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column observed in clear-sky
conditions (see Fig. 12). The total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column
from the cloud-slicing technique, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>slicing</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>,
is calculated as the sum of partial vertical
column densities obtained from the annual mean pseudoprofile VMR as

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E14"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>slicing</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mtext>lat</mml:mtext><mml:mo>,</mml:mo><mml:mtext>lon</mml:mtext><mml:mo>)</mml:mo><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mn mathvariant="normal">6</mml:mn></mml:munderover><mml:msub><mml:mtext>VMR</mml:mtext><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mtext>lat</mml:mtext><mml:mo>,</mml:mo><mml:mtext>lon</mml:mtext><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:mo>〈</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>〉</mml:mo><mml:mo>-</mml:mo><mml:mo>〈</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi>C</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is the same constant defined in Eq. (<xref ref-type="disp-formula" rid="Ch1.E8"/>). Note that absent VMR
grid values (such as at high altitude over subsidence regions, or at low
altitude over the tropical continents) are ignored without provision of a priori information.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16" specific-use="star"><caption><p>Total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns differences between cloudy
(CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> %) and clear (CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>25</mml:mn></mml:mrow></mml:math></inline-formula> %) conditions for TM4 (left) and OMI (right).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f13.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><caption><p>Total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column differences (OMI–TM4) in clear
(left) and cloudy (right) conditions for the year 2006.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f14.png"/>

        </fig>

      <p>We do, however, know that there are some basic differences between <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
profiles observed under clear and cloudy conditions. In the TM4
model, the differences between cloudy (CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> %) and clear
(CRF <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>25</mml:mn></mml:mrow></mml:math></inline-formula> %) profile climatologies (see left panel in Fig. 13
below) show strong negative anomalies over the biomass burning areas
(central Africa, southern America, northern Australia, southern India,
but also in the Persian Gulf and Turkestan) most likely related to
fire suppression during the wet/cloudy season. Over industrial areas
(USA, Europe and China) a more complex pattern of anomalies arises
that likely results from the competing effects of suppressed
photolysis under clouds (small positive anomaly), venting by passing
fronts (large negative anomalies) and accumulation patterns dependent
on a predominant synoptic weather type (cyclonic or anticyclonic, Pope
et al., 2014). This pattern of differences between cloudy and clear
annual <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profile climatologies is well reproduced by OMI
observations (see right panel in Fig. 13 below). The sole difference
is that OMI sees larger outflows at higher latitudes in the cloudy
case – perhaps a deficiency of the model in redistributing its
horizontal flows under frontal conditions.</p>
      <p>Another more direct way to perform this consistency check is to look at the
differences in total <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns between model (TM4) and observations
(OMI) for the clear and cloudy cases separately, as shown in Fig. 14. For the
clear-sky case (see left panel in Fig. 14) the pattern of anomalies that
arises is consistent with existing long-term satellite <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trend
studies (van der A et al., 2008; Richter et al., 2005) that report
significant reductions in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in Europe and eastern parts of the
United States as well as strong increases in China, along with evidence of decreasing
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in Japan and increasing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in India, the Middle East, and
central Russia – as well as over some spots in the central USA and South Africa.
The differences between model and clear-sky OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> total columns are
being used to update the surface emission inventories (Mijling and van der A,
2012; Ding et al., 2015). What is comforting is that a similar pattern of
differences arises in the cloudy case (using the cloud-slicing TM4 and OMI
profiles), and with a similar amplitude, verifying that the OMI cloud-slicing
columns are internally consistent with the clear-sky OMI observations in
detecting anomalies that can be ultimately related to outdated model emission
inventories.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F18" specific-use="star"><caption><p>African sector at 280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>: seasonal variability in OMI (top row)
versus TM4 model (bottom row) average <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR pseudoprofiles for the year 2006.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f15.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F19" specific-use="star"><caption><p>Same as Fig. 15 but at 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f16.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F20" specific-use="star"><caption><p>Same as Fig. 15 but at 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f17.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F21" specific-use="star"><caption><p>Same as Fig. 15 but at 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f18.jpg"/>

        </fig>

      <p>In Fig. 14, note that the model total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns
over clean remote areas (i.e., tropical and extratropical outflow
regions over the oceans) in the cloudy case do not deviate in general
by more than <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>0.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">molec</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> from
observations. This is a good result, showing that the estimate of the
stratospheric column (by data assimilation) does not produce
significant cloud-cover dependent biases in the tropospheric
column. If we recall that the observed cloud-slicing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
profile over clean remote areas is S-shaped, with a much stronger
mid-tropospheric component and a much reduced upper tropospheric load
than in the model, then we can infer that there has been as much gain
in the mid-tropospheric component as there has been loss at high
altitude, which is another form of closure.</p>
</sec>
<sec id="Ch1.S3.SS6">
  <title>Seasonal analysis</title>
      <p>The seasonal mean tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR pseudoprofiles for the DJF,
MAM, JJA and SON periods observed by OMI over the year 2006 compared
against their TM4 model counterparts are shown next. These plots (Figs. 15–33)
have been generated using the same cloud-slicing grid and CRF threshold
configurations applied for the annual means, with a required minimum of 7
measurements collected per bin during each season (instead of 30 for the
annual means). This section is not intended to provide a thorough analysis of
seasonal variability in (observed or modeled) tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles
but rather to demonstrate the potential of the cloud-slicing technique to provide details
that pertain to seasonal as well as to annual means.</p>
      <p>The largest signatures of seasonal variability expected to appear in these
figures are (a) a seasonal cycle in lightning activity in the upper levels
(280–380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) that shifts in latitude following the Sun's
declination; (b) a seasonal cycle of biomass burning in the mid-levels
(500–620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>) basically opposite to that of lightning in case of
man-made fires during the dry season, otherwise in phase with lightning; and
(c) a seasonal cycle over industrial areas at lower levels
(720–820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>), featuring minimum <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels in the summer
months due to changes in the lifetime of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (van der A et al., 2008). The
seasonal cycle in lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions may be verified against the
climatology of lightning flashes observed by LIS-OTD (data set available
online, <uri>ftp://ghrc.nsstc.nasa.gov/pub/lis/climatology</uri>; see Cecil et
al., 2014). The seasonal cycle in biomass burning may be verified against the
climatology of ATSR and AVHRR fire counts from Dwyer et al. (2000) and
Schultz (2002).</p>
</sec>
<sec id="Ch1.S3.SSx1" specific-use="unnumbered">
  <title>Africa</title>
      <p>Over Africa, persistent lightning activity at upper levels is expected to take
place about the Equator (the Congo Basin) all year long, shifting southward towards South
Africa in SON and DJF, and northward towards the Gulf of Guinea, the Sahel and Sudan in
MAM and JJA, features which are all captured by OMI in Fig. 15 (in reasonable agreement
with TM4, though some discrepancies are apparent too). These lightning signatures are not
to be confused with traces of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> lifted from biomass burning underneath, which
feature a precisely opposite phase. Remarkable biomass burning signatures can be
appreciated throughout the entire tropospheric column in Figs. 15–18 as <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
enhancements north of the Equator (Sahel) in DJF and south of the Equator (Angola and Zambia)
in JJA, shifting eastward towards Mozambique and Madagascar in SON (best seen at 500
and 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in Figs. 17–18). We note that the penetration of seasonal biomass burning
signatures into 280–500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> is stronger in OMI than in TM4. In addition, note the strong
enhancement in lightning activity seen by OMI off the southeast coast of Africa in MAM and JJA
at 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in Fig. 16, in connection with the confluence of the warm Agulhas and the
cold Antarctic Circumpolar Current, which is virtually missed by TM4.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F22" specific-use="star"><caption><p>South American sector at 280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>: seasonal variability in OMI
(top row) versus TM4 model (bottom row) average <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR pseudoprofiles for the year 2006.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f19.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F23" specific-use="star"><caption><p>Same as Fig. 19 but at 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f20.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F24" specific-use="star"><caption><p>Same as Fig. 19 but at 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f21.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F25" specific-use="star"><caption><p>Same as Fig. 19 but at 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f22.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F26" specific-use="star"><caption><p>Same as Fig. 19 but at 720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in logarithmic scale.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f23.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SSx2" specific-use="unnumbered">
  <title>South America</title>
      <p>Over South America, a maximum in lightning activity is expected to occur over
central Brazil in SON, as captured by OMI in Figs. 19–20 (in agreement with TM4, though some
discrepancies persist relative to the location of the lightning maximum, as we mentioned when
describing the annual means), migrating towards the southeast in DJF. Lightning and
precipitation are persistent in the northwest (Colombia, Venezuela and Central America) all
year round, intensifying in MAM and JJA, as reasonably captured by OMI in Fig. 19, along with
some persistent <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> enhancements over La Plata Basin and off into the
Brazil–Malvinas Confluence Zone. The lightning signatures at upper levels may be partly overlapped
by those from biomass burning lifted from underneath, but their separation is more difficult in
this case. For instance, the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> enhancements detected by OMI at 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>
over Brazil in SON and DJF in Fig. 21 correlate well with the lightning signatures at
380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>, but they also correlate with the biomass burning signals at 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>,
indicating that both processes may be occurring at the
same time in separate but nearby locations (e.g., combining the start of the wet season in the
Amazon Basin in DJF, with the end of the burning season in eastern Brazil). The cycle of
biomass burning in South America, which takes place over the dry season, starts in southern
Brazil in JJA, finding a maximum in SON eastward towards the coastal states, as OMI captures
in Figs. 21–23 (in reasonable agreement with TM4). In DJF, some activity may persist in eastern
Brazil and new activity develops over the lower slopes of the Argentinian Andes during the
austral summer, generally complicating attribution. Finally, it is interesting to note in Fig. 23 the
remarkable decrease in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels at 720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> over the Amazon Basin during
the rainy season in DJF and MAM, as if in connection with an efficient <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> removal
mechanism.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F27" specific-use="star"><caption><p>Asian sector at 280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>: seasonal variability in OMI (top row)
versus TM4 model (bottom row) average <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR pseudoprofiles for the year 2006.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f24.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F28" specific-use="star"><caption><p>Same as Fig. 24 but at 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f25.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F29" specific-use="star"><caption><p>Same as Fig. 24 but at 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f26.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F30" specific-use="star"><caption><p>Same as Fig. 24 but at 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f27.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F31" specific-use="star"><caption><p>Same as Fig. 24 but at 720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in logarithmic scale.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f28.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SSx3" specific-use="unnumbered">
  <title>Southeast Asia and Australia</title>
      <p>At upper levels, one should expect to see some persistent lightning activity
over Indonesia all year round, as qualitatively observed by OMI in Fig. 24 (and in
agreement with TM4), migrating northward towards South Asia in MAM and JJA,
and southward towards Australia in SON and DJF. These lightning signatures may
be mixed to greater or lesser degree with <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> lifted from biomass burning and/or
anthropogenic sources underneath. Over South Asia, biomass burning is expected
to reach its maximum in MAM, as OMI captures in Figs. 26–28 particularly over northern
India and Myanmar. These emissions are likely responsible for a large part of the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
enhancement observed around India at upper levels in MAM. The very strong <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
enhancement observed over South Asia at upper levels in JJA (Figs. 24–25) is very likely
related to deep transport of surface emissions (biomass and industrial) during the
monsoon season, which TM4 locates over the Indo-Gangetic area and OMI locates further
east over the Tibetan Plateau. Over Indonesia and northern Australia, a maximum in biomass
burning activity is expected be reached in SON, as OMI captures reasonably well in
Figs. 26–28, indicating that the strong <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> enhancement seen by OMI over northern
Australia at 280 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in SON may well be tainted by deep transport of biomass burning.</p>
      <p>Over a major industrial hub like China, near-surface concentrations of
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> around 720–820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> are expected to reach
minimum/maximum levels in JJA/DJF, just on account of increased/reduced
exposure to sunlight (i.e., reduced/increased NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> lifetime), as shown by
both OMI and TM4 in Fig. 28. At mid-tropospheric levels though, other effects
such as vertical transport intervene. Note in Figs. 26–27 that the TM4 model
registers maximum mid-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels over China in JJA, and
minimum in DJF. However, OMI observes stronger mid-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
levels in DJF than in JJA. According to OMI, surface emissions from China
(and also from Europe and the USA, as we shall see next) are being
transported in larger quantities and to higher altitudes than in the model,
particularly during the winter months.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F32" specific-use="star"><caption><p>North American and European sectors at 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>: seasonal
variability in OMI (left column) versus TM4 model (right column) average
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR pseudoprofiles for the year 2006.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f29.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F33" specific-use="star"><caption><p>Same as Fig. 29 but at 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f30.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F34" specific-use="star"><caption><p>Same as Fig. 29 but at 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f31.jpg"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F35" specific-use="star"><caption><p>Same as Fig. 29 but at 720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in logarithmic scale.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f32.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F36" specific-use="star"><caption><p>Same as Fig. 29 but at 820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in logarithmic scale.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/13519/2015/acp-15-13519-2015-f33.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SSx4" specific-use="unnumbered">
  <title>Europe and North America</title>
      <p>In connection with summer convection, lightning activity
at northern mid-latitudes is expected to be strongest in JJA. Enhancements in
upper tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are observed by OMI (and TM4) in Fig. 29 over the
eastern Mediterranean in JJA and SON. Enhanced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels over Siberia
in JJA may also be related to summer convection and increased biomass burning.
In the USA, lightning activity is expected to reach a maximum in JJA and shift southward
towards the Gulf of Mexico in SON and DJF, features which are all registered by OMI
in Fig. 29 (in reasonable agreement with TM4, though some discrepancies are apparent
in DJF). Figures 30–31 reveal an interesting discrepancy between the OMI and TM4
pseudoprofiles regarding the intensity and reach of convective penetration at 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>
of anthropogenic <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> above major industrial areas. As already noted for China, the
TM4 model is placing enhancements of mid-tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over central Europe
and the eastern USA in MAM and JJA, whereas OMI registers a more uniform distribution of
mid-tropospheric signatures across the year, showing maxima in DJF and SON. This
disagreement is suggestive of problems with the model convective scheme, possibly
related to frontal uplift by conveyor belts in the wintertime. At levels closest to the
surface, the variation in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration over major industrial areas (Europe
and the USA, but also China, India and the Middle East) registered by OMI in Figs. 19–20 shows
minima in JJA and maxima in DJF, just as expected and in agreement with TM4.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Summary and conclusions</title>
      <p>In this paper, we derive annual and seasonal global climatologies of tropospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles from OMI cloudy measurements for the year 2006
using the cloud-slicing method on six pressure levels centered at
about 280, 380, 500, 620, 720 and 820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>. The cloud-slicing
profiles have been estimated after differencing annual and seasonal tropospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns above cloud with respect to pressure, using mean
cloud pressures located at about 330, 450, 570, 670, 770 and
870 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>. We term these objects pseudoprofiles, since the
required presence of a probing cloud necessarily draws the cloud-slicing estimate away
from the underlying <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profile. The systematic error between the
cloud-sliced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pseudoprofile and the actual average <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
profile in a cloudy atmosphere is called pseudoprofile error, which
can be evaluated (and possibly corrected) using a CTM.</p>
      <p>The total tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> content in the cloud-slicing
profiles is consistent with the OMI clear-sky total tropospheric column
for the same year, after making allowance for a natural change in the
global <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> distribution that occurs in passing from clear to
cloudy conditions. This change includes suppression of biomass burning
during the wet/cloudy season, suppressed <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> photolysis under
clouds, venting by weather fronts and accumulation patterns dependent
on the predominant (clear or cloudy sky) synoptic weather type. The
internal consistency between OMI clear-sky and cloud-slicing
tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns confirms the capability of cloud-slicing profiles to detect CTM model anomalies that can be ultimately
related to problems in model emission inventories but with additional
vertical information that allows distinction between surface,
mid-tropospheric and upper-tropospheric processes.</p>
      <p>The vertical information contained in OMI tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles
derived from the cloud-slicing technique provides a wealth of information
that can be used to evaluate global chemistry models and provide guidance in
the development of subgrid model parameterizations of convective transport,
fire-induced injection, horizontal advective diffusion and lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
production. Overlapping processes (i.e., the effects of deep convection and
lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the upper troposphere, the effects of mid-tropospheric
convection and anomalies in surface emissions in the mid-troposphere) as well
as uncertainties in the chemical degradation and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> recycling rates
currently limit the degree to which discrepancies between observations and
simulations can be unambiguously attributed to a single process, although the
availability of observational constraints definitely constitutes an
improvement.</p>
      <p>To give an example of such an application, we have performed a comparison between
cloud-slicing tropospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles from OMI and the TM4 model.
In the upper troposphere (280 and 380 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> levels), observed
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration anomalies reveal excessive model background
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts which are consistent with too strong model lightning
emissions over the oceans (and/or too long lifetimes) combined with misplaced
lightning <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over central Africa and South America, which is
indicative of limitations in the convectively driven model lightning NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
scheme of Meijer et al. (2001). Other anomalies suggest observed enhanced
deep transport of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from major industrial centers relative to TM4,
including a prominent signal from the Asian summer monsoon plume that the
model fails to place accurately, and probable excess model fire-induced
convection over Siberia.</p>
      <p>In the mid-troposphere (500 and 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> levels), observed <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
concentration anomalies reveal deficient model background <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts
suggestive of too small model convective inflows into this level, with
deficits particularly large over China, the central USA and Europe during the
winter months, and the biomass burning regions in central Africa and South
America, combined with extensive outflows over the oceans that are stronger
and more widely distributed in latitude than in the model. This is consistent
with independent reports of underestimation of vertical transport by
convective clouds in Tiedtke-based models. Raising the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> plumes to
higher altitudes allows for much longer residence and chemical lifetimes, and
longer and more widely distributed horizontal transport of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
following poleward advection and dispersion by the subtropical jet in the
mid-troposphere, all of which end up producing typical outflow profiles over
the oceans that are generally S-shaped with a prominent mid-tropospheric
plume centered at around 620 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in the tropics and around
720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> in the extratropics. The role that the recycled NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
component may play in the enhanced mid-tropospheric outflows observed by OMI
over remote ocean regions is unclear at this stage, but the cloud-slicing
technique shows promise to study such effects.</p>
      <p>In the lower troposphere (720 and 820 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>), observed
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration anomalies show a pattern that is consistent
with deficiencies in model surface emissions related to known
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trends characterized by <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increases over China,
India and the Middle East, and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> decreases over the eastern USA,
central Europe and Japan. The lower levels also show extensive
positive anomalies over the oceans (particularly at 720 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula>),
which are indicative of deficient model outflows at low altitudes
(and/or too short model lifetimes) with deficient poleward diffusion
of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at low to mid-tropospheric levels, and an interesting
band of negative anomalies along the ITCZ.</p>
      <p>On a seasonal basis, both the OMI and TM4 model pseudoprofiles
show seasonal features that are consistent with the available lightning
flash and fire count climatologies, and complementary to the results
obtained for the annual means. On a finer scale, we observe some
significant differences on lightning distribution (at upper levels over
Africa and South America, or over the Agulhas and Brazil–Malvinas
ocean current confluence zones), and the intensity and reach of convective transport
over strong biomass or industrial sources – whose detailed examination
deserves future work. For example, we note that the penetration of seasonal
biomass burning signatures into 280–500 hPa over Africa is stronger in OMI
than in TM4. Also, the penetration of industrial emissions into mid-tropospheric
levels over Europe, China and the USA reaches a maximum in MAM and JJA
according to TM4, whereas OMI registers a more uniform distribution of
mid-tropospheric signatures across the year with maxima in DJF and SON,
which is suggestive of problems with the model convective scheme, possibly
related to frontal uplift by conveyor belts in the wintertime.</p>
      <p>Note that support from a CTM (TM4 in our case) is required to make
provision for the cloud-slicing technique in order to determine the a priori
corrections for below-cloud leakage, so that a level of trust must initially be
placed in the model. When comparing the resulting pseudoprofiles
against the a priori information, a number of discrepancies arise which
work against our initial trust in the model. This conflicting outcome
should be understood and justified to the extent that a priori corrections
only have a limited impact on the cloud-slicing profiles. Correcting for
pseudoprofile errors using model-based profile-to-pseudoprofile ratios
is an entirely different matter. The presence of systematic pseudoprofile
error in cloud-slicing estimates and their general predominance over
random instrumental error suggest that the vertical information contained
in cloudy pixels may be best extracted by an assimilation procedure that
updates the atmospheric state (i.e., the model profile shape) at the right
time and place using the averaging kernel of the observation. Most data
assimilation experiments using OMI <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> observations have
focused to this date on exploiting clear-sky measurements only: our results provide
strong motivation to put cloudy pixels to good use as well, as done by, for example, Miyazaki et al. (2014).</p><?xmltex \hack{\clearpage}?>
</sec>

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

<app id="App1.Ch1.S1">
  <title>Gas columns above and below cloud</title>
      <p>If the tropospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is defined as

              <disp-formula id="App1.Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        where the clear AMF can be expressed as

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.E2"><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>clear</mml:mtext></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mrow><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mtable rowspacing="-4pt" class="array" columnalign="left"><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">clear</mml:mtext></mml:mtd></mml:mtr><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">below</mml:mtext></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mrow><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mtable class="array" rowspacing="-4pt" columnalign="left"><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">clear</mml:mtext></mml:mtd></mml:mtr><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">above</mml:mtext></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the clear-sky scattering sensitivity and
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the model a priori trace gas profile. Similarly, the cloudy
AMF can be expressed as

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.E3"><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>cloud</mml:mtext></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mrow><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mtable class="array" rowspacing="-4pt" columnalign="left"><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">cloud</mml:mtext></mml:mtd></mml:mtr><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">above</mml:mtext></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloudy</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the cloudy-sky scattering
sensitivity. Note that by construction:

              <disp-formula id="App1.Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>tropopause</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>Then the tropospheric AMF can be written, after inserting Eqs. (A2) and (A3)
into Eq. (A1), and rearranging terms relating to above and below components
separately, as

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.E5"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mtext>CRF</mml:mtext><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mrow><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mtable class="array" rowspacing="-4pt" columnalign="left"><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">cloud</mml:mtext></mml:mtd></mml:mtr><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">above</mml:mtext></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mrow><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mtable rowspacing="-4pt" class="array" columnalign="left"><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">clear</mml:mtext></mml:mtd></mml:mtr><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">above</mml:mtext></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:msub></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mrow><mml:mspace linebreak="nobreak" width="-0.125em"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mspace width="-0.125em" linebreak="nobreak"/><mml:mtable rowspacing="-4pt" class="array" columnalign="left"><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">clear</mml:mtext></mml:mtd></mml:mtr><mml:mtr><mml:mtd><?xmltex \hack{\scriptsize}?><mml:mtext mathvariant="normal">below</mml:mtext></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p>From this formulation arise definitions for
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>:

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.E6"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>≡</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:mfenced open="(" close=")"><mml:mtext>CRF</mml:mtext><mml:mo>⋅</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mtext>cloud</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mfenced><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mtext>CLP</mml:mtext><mml:mtext>trop</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="App1.Ch1.E7"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>≡</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mtext>clear</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mtext>CLP</mml:mtext></mml:munderover><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>Now it is straightforward to write

              <disp-formula id="App1.Ch1.Ex13"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        which after substitution of Eq. (A5) becomes

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.E8"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mfenced><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p>This allows the separation of the slant column components above
and below the cloud in Eq. (A8) as

              <disp-formula id="App1.Ch1.E9" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>above</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Now, in Boersma (2005) the above-cloud part
of the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column is retrieved by removing the model predicted
ghost column (integrated from the ground to the cloud level pressure, identical
to <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>) that is implicitly added via the
tropospheric air mass factor as

              <disp-formula id="App1.Ch1.E10" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mtext>CRF</mml:mtext><mml:mo>⋅</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        However, by virtue of Eq. (A4), formulation in Eq. (A10) in Boersma (2005) should be changed to

              <disp-formula id="App1.Ch1.E11" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>above</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mtext>SCD</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mtext>AMF</mml:mtext><mml:mtext>trop</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mtext>VCD</mml:mtext><mml:mtext>below</mml:mtext></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        which is equivalent to Eq. (A9).</p><?xmltex \hack{\clearpage}?><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-15-13519-2015-supplement" xlink:title="pdf">doi:10.5194/acp-15-13519-2015-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
</app>
  </app-group><ack><title>Acknowledgements</title><p>This work has been funded by the Netherlands Space Office (NSO) under
OMI contract.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: M. Van Roozendael</p></ack><ref-list>
    <title>References</title>

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    <!--<article-title-html>OMI tropospheric NO<m:math xmlns="http://www.w3.org/1999/xhtml" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:svg="http://www.w3.org/2000/svg" display="inline"><m:msub level="3"><m:mi/><m:mn mathvariant="normal">2</m:mn></m:msub></m:math> profiles from cloud slicing: constraints
on surface emissions, convective transport and lightning NO<m:math xmlns="http://www.w3.org/1999/xhtml" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:svg="http://www.w3.org/2000/svg" display="inline"><m:msub level="3"><m:mi/><m:mi mathvariant="italic">x</m:mi></m:msub></m:math></article-title-html>
<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">We derive annual and seasonal global climatologies of tropospheric NO<m:math display="inline"><m:msub level="3"><m:mi/><m:mn mathvariant="normal">2</m:mn></m:msub></m:math>
profiles from OMI cloudy observations for the year 2006 using the cloud-slicing method on six pressure levels centered at about 280, 380, 500, 620, 720
and 820 hPa. A comparison between OMI and the TM4 model tropospheric
NO<m:math display="inline"><m:msub level="3"><m:mi/><m:mn mathvariant="normal">2</m:mn></m:msub></m:math> profiles reveals striking overall similarities, which confer great
confidence to the cloud-slicing approach to provide details that pertain to
annual as well as seasonal means, along with localized discrepancies that
seem to probe into particular model processes. Anomalies detected at the
lowest levels can be traced to deficiencies in the model surface emission
inventory, at mid-tropospheric levels to convective transport and horizontal
advective diffusion, and at the upper tropospheric levels to model lightning
NO<m:math display="inline"><m:msub level="3"><m:mi/><m:mi mathvariant="italic">x</m:mi></m:msub></m:math> production and the placement of deeply transported NO<m:math display="inline"><m:msub level="3"><m:mi/><m:mn mathvariant="normal">2</m:mn></m:msub></m:math> plumes
such as from the Asian summer monsoon. The vertical information contained in
the OMI cloud-sliced NO<m:math display="inline"><m:msub level="3"><m:mi/><m:mn mathvariant="normal">2</m:mn></m:msub></m:math> profiles provides a global observational
constraint that can be used to evaluate chemistry transport models (CTMs) and
guide the development of key parameterization schemes.</p></abstract-html>
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