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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>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-7-1683-2007</article-id>
<title-group>
<article-title>Lightning-produced NO&lt;sub&gt;2&lt;/sub&gt; observed by two ground-based UV-visible spectrometers at Vanscoy, Saskatchewan in August 2004</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fraser</surname>
<given-names>A.</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>Goutail</surname>
<given-names>F.</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>McLinden</surname>
<given-names>C. A.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Melo</surname>
<given-names>S. M. L.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Strong</surname>
<given-names>K.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Physics, University of Toronto, Toronto, Ontario, Canada</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Service d&apos;Aéronomie du Centre Nationale de la Recherche Scientifique, Verrières le Buisson, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Environment Canada, Downsview, Ontario, Canada</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Space Science, Canadian Space Agency, Saint-Hubert, Québec, Canada</addr-line>
</aff>
<pub-date pub-type="epub">
<day>28</day>
<month>03</month>
<year>2007</year>
</pub-date>
<volume>7</volume>
<issue>6</issue>
<fpage>1683</fpage>
<lpage>1692</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>
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<self-uri xlink:href="http://www.atmos-chem-phys.net/7/1683/2007/acp-7-1683-2007.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/7/1683/2007/acp-7-1683-2007.pdf</self-uri>
<abstract>
<p>Ground-based measurements of ozone and NO&lt;sub&gt;2&lt;/sub&gt; differential slant columns by the SAOZ
(Système d&apos;Analyse par Observations Zénithales) and UT-GBS (University of
Toronto Ground-Based Spectrometer) instruments during the MANTRA 2004 field
campaign are presented herein. During the afternoon of 28 August, a
thunderstorm passed over the instruments, which were installed at Vanscoy,
Saskatchewan (52&amp;deg; N, 107&amp;deg; W). Enhanced differential slant columns of ozone and
NO&lt;sub&gt;2&lt;/sub&gt; were observed by both instruments during the storm, with maximum
values of two and 25 times the expected clear sky columns, respectively. The enhanced
ozone differential slant columns are primarily due to the longer path traversed by the
solar radiation caused by multiple scattering inside the thick cloud layer
associated with the thunderstorm. The enhanced NO&lt;sub&gt;2&lt;/sub&gt; columns are partly attributed
to NO&lt;sub&gt;x&lt;/sub&gt; production by lightning. Two new methods are used to separate
the NO&lt;sub&gt;2&lt;/sub&gt; enhancements into contributions from the longer path length and
production by lightning. Combining the observed excess NO&lt;sub&gt;2&lt;/sub&gt; with lightning
flash data from the Canadian Lightning Detection Network and Environment
Canada Doppler radar measurements, the production of NO&lt;sub&gt;2&lt;/sub&gt; molecules per
lightning flash is determined. Using these two methods, the best estimate of
the production rate is found to be (7.88&amp;plusmn;2.52)&amp;times;10&lt;sup&gt;26&lt;/sup&gt; molecules
NO&lt;sub&gt;2&lt;/sub&gt;/flash from the UT-GBS and (6.81&amp;plusmn;2.17)&amp;times;10&lt;sup&gt;26&lt;/sup&gt; molecules
NO&lt;sub&gt;2&lt;/sub&gt;/flash from SAOZ. These results are consistent with the range of previous estimates reported in the literature.</p>
</abstract>
<counts><page-count count="10"/></counts>
</article-meta>
</front>
<body/>
<back>
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