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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>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>GÃ¶ttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-10-10965-2010</article-id>
<title-group>
<article-title>Direct satellite observation of lightning-produced NO&lt;sub&gt;x&lt;/sub&gt;</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Beirle</surname>
<given-names>S.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Huntrieser</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wagner</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Max-Planck-Institut fÃ¼r Chemie, Mainz, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institut fÃ¼r Physik der AtmosphÃ¤re, Deutsches Zentrum fÃ¼r Luft- und Raumfahrt (DLR), Oberpfaffenhofen, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>24</day>
<month>11</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>22</issue>
<fpage>10965</fpage>
<lpage>10986</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
<self-uri xlink:href="http://www.atmos-chem-phys.net/10/10965/2010/acp-10-10965-2010.html">This article is available from http://www.atmos-chem-phys.net/10/10965/2010/acp-10-10965-2010.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/10/10965/2010/acp-10-10965-2010.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/10/10965/2010/acp-10-10965-2010.pdf</self-uri>
<abstract>
<p>Lightning is an important source of NO&lt;sub&gt;x&lt;/sub&gt; in the free
      troposphere, especially in the tropics, with strong impact on ozone
      production. However, estimates of lightning NO&lt;sub&gt;x&lt;/sub&gt; (LNO&lt;sub&gt;x&lt;/sub&gt;)
      production efficiency (LNO&lt;sub&gt;x&lt;/sub&gt; per flash) are still quite
      uncertain.
&lt;br&gt;&lt;br&gt;
      In this study we present a systematic analysis of NO&lt;sub&gt;2&lt;/sub&gt; column
      densities from SCIAMACHY measurements over active thunderstorms, as
      detected by the World-Wide Lightning Location Network (WWLLN), where
      the WWLLN detection efficiency was estimated using the flash
      climatology of the satellite lightning sensors LIS/OTD. Only events
      with high lightning activity are considered, where corrected WWLLN
      flash rate densities inside the satellite pixel within the last hour
      are above 1 /km&lt;sup&gt;2&lt;/sup&gt;/h.  For typical SCIAMACHY ground pixels of
      30 Ã— 60 km&lt;sup&gt;2&lt;/sup&gt;, this threshold corresponds to 1800 flashes
      over the last hour, which, for literature estimates of lightning
      NO&lt;sub&gt;x&lt;/sub&gt; production, should result in clearly enhanced NO&lt;sub&gt;2&lt;/sub&gt; column densities.
&lt;br&gt;&lt;br&gt;
      From 2004â€“2008, we find 287 coincidences of SCIAMACHY measurements
      and high WWLLN flash rate densities. For some of these events, a clear
      enhancement of column densities of NO&lt;sub&gt;2&lt;/sub&gt; could be observed,
      indeed. But overall, the measured column densities are below the
      expected values by more than one order of magnitude, and in most of
      the cases, no enhanced NO&lt;sub&gt;2&lt;/sub&gt; could be found at all.
&lt;br&gt;&lt;br&gt;
      Our results are in contradiction to the currently accepted range of
      LNO&lt;sub&gt;x&lt;/sub&gt; production per flash of 15
      (2â€“40)&amp;times;10&lt;sup&gt;25&lt;/sup&gt; molec/flash. This probably partly
      results from the specific conditions for the events under
      investigation, i.e. events of high lightning activity in the morning
      (local time) and mostly (for 162 out of 287 events) over ocean.
&lt;br&gt;&lt;br&gt;
      Within the detected coincidences, the highest NO&lt;sub&gt;2&lt;/sub&gt; column
      densities were observed around the US Eastcoast. This might be
      partly due to interference with ground sources of NO&lt;sub&gt;x&lt;/sub&gt; being
      uplifted by the convective systems. However, it could also indicate
      that flashes in this region are particularly productive.
&lt;br&gt;&lt;br&gt;
      We conclude that current estimates of LNO&lt;sub&gt;x&lt;/sub&gt; production might be
      biased high for two reasons. First, we observe a high variability of
      NO&lt;sub&gt;2&lt;/sub&gt; for coincident lightning events. This high variability can
      easily cause a publication bias, since studies reporting on high
      NO&lt;sub&gt;x&lt;/sub&gt; production have likely been published, while studies
      finding no or low amounts of NO&lt;sub&gt;x&lt;/sub&gt; might have been rejected as
      errorneous or not significant. Second, many estimates of LNO&lt;sub&gt;x&lt;/sub&gt;
      production in literature have been performed over the US, which is
      probably not representative for global lightning.</p>
</abstract>
<counts><page-count count="22"/></counts>
</article-meta>
</front>
<body/>
<back>
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