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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-9-8377-2009</article-id>
<title-group>
<article-title>NO&lt;sub&gt;x&lt;/sub&gt; production by lightning in Hector: first airborne measurements during SCOUT-O3/ACTIVE</article-title>
</title-group>
<contrib-group><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="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Schlager</surname>
<given-names>H.</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>Lichtenstern</surname>
<given-names>M.</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>Roiger</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>Stock</surname>
<given-names>P.</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>Minikin</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>HÃ¶ller</surname>
<given-names>H.</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>Schmidt</surname>
<given-names>K.</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>Betz</surname>
<given-names>H.-D.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Allen</surname>
<given-names>G.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Viciani</surname>
<given-names>S.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ulanovsky</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ravegnani</surname>
<given-names>F.</given-names>
</name>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Brunner</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institut fÃ¼r Physik der AtmosphÃ¤re, Deutsches Zentrum fÃ¼r Luft- und Raumfahrt (DLR), Oberpfaffenhofen, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>nowcast GmbH, MÃ¼nchen, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Physics Department, University of Munich, Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>School of Earth, Atmospheric &amp; Environmental Sciences, University of Manchester, UK</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Istituto Nazionale di Ottica Applicata (CNR-INOA), Firenze, Italy</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Central Aerological Observatory, Moscow, Russia</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>Institute of Atmospheric Sciences and Climate (CNR-ISAC), Bologna, Italy</addr-line>
</aff>
<aff id="aff8">
<label>8</label>
<addr-line>Laboratory for Air Pollution and Environmental Technology, Empa, Swiss Federal Laboratories for Materials Testing and Research, DÃ¼bendorf, Switzerland</addr-line>
</aff>
<pub-date pub-type="epub">
<day>05</day>
<month>11</month>
<year>2009</year>
</pub-date>
<volume>9</volume>
<issue>21</issue>
<fpage>8377</fpage>
<lpage>8412</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/9/8377/2009/acp-9-8377-2009.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/9/8377/2009/acp-9-8377-2009.pdf</self-uri>
<abstract>
<p>During the SCOUT-O3/ACTIVE field phase in Novemberâ€“December 2005, airborne in
situ measurements were performed inside and in the vicinity of thunderstorms
over northern Australia with several research aircraft (German &lt;i&gt;Falcon&lt;/i&gt;,
Russian M55 &lt;i&gt;Geophysica&lt;/i&gt;, and British
&lt;i&gt;Dornier-228&lt;/i&gt;. Here a case study from 19 November is presented in
detail on the basis of airborne trace gas measurements (NO, NO&lt;sub&gt;y&lt;/sub&gt;,
CO, O&lt;sub&gt;3&lt;/sub&gt;) and stroke measurements from the German LIghtning
Location NETwork (LINET), set up in the vicinity of Darwin
during the field campaign. The anvil outflow from three different types of
thunderstorms was probed by the Falcon aircraft: (1) a continental
thunderstorm developing in a tropical airmass near Darwin, (2) a mesoscale
convective system (MCS), known as Hector, developing within the tropical
maritime continent (Tiwi Islands), and (3) a continental thunderstorm developing
in a subtropical airmass ~200 km south of Darwin. For the first
time detailed measurements of NO were performed in the Hector outflow. The
highest NO mixing ratios were observed in Hector with peaks up to 7 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt;
in the main anvil outflow at ~11.5â€“12.5 km altitude. The
mean NO&lt;sub&gt;x&lt;/sub&gt; (=NO+NO&lt;sub&gt;2&lt;/sub&gt;) mixing ratios during these penetrations (~100 km width)
varied between 2.2 and 2.5 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. The NO&lt;sub&gt;x&lt;/sub&gt;
contribution from the boundary layer (BL), transported upward with the
convection, to total anvil-NO&lt;sub&gt;x&lt;/sub&gt; was found to be minor (&lt;10%). On the
basis of Falcon measurements, the mass flux of lightning-produced NO&lt;sub&gt;x&lt;/sub&gt;
(LNO&lt;sub&gt;x&lt;/sub&gt;) in the well-developed Hector system was estimated to 0.6â€“0.7 kg(N) s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;.
The highest average stroke rate of the probed thunderstorms was
observed in the Hector system with 0.2 strokes s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (here only strokes
with peak currents &amp;ge;10 kA contributing to LNO&lt;sub&gt;x&lt;/sub&gt; were considered). The
LNO&lt;sub&gt;x&lt;/sub&gt; mass flux and the stroke rate were combined to estimate the LNO&lt;sub&gt;x&lt;/sub&gt;
production rate in the different thunderstorm types. For a better comparison
with other studies, LINET strokes were scaled with Lightning
Imaging Sensor (LIS) flashes. The LNO&lt;sub&gt;x&lt;/sub&gt; production
rate per LIS flash was estimated to 4.1â€“4.8 kg(N) for the well-developed
Hector system, and to 5.4 and 1.7 kg(N) for the continental thunderstorms
developing in subtropical and tropical airmasses, respectively. If we assume,
that these different types of thunderstorms are typical thunderstorms
globally (LIS flash rate ~44 s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;), the annual global LNO&lt;sub&gt;x&lt;/sub&gt;
production rate based on Hector would be ~5.7â€“6.6 Tg(N) a&lt;sup&gt;&amp;minus;1&lt;/sup&gt; and
based on the continental thunderstorms developing in subtropical and tropical
airmasses ~7.6 and ~2.4 Tg(N) a&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, respectively. The
latter thunderstorm type produced much less LNO&lt;sub&gt;x&lt;/sub&gt; per flash compared to the
subtropical and Hector thunderstorms, which may be caused by the shorter mean
flash component length observed in this storm. It is suggested that the
vertical wind shear influences the horizontal extension of the charged
layers, which seems to play an important role for the flash lengths that may
originate. In addition, the horizontal dimension of the anvil outflow and the
cell organisation within the thunderstorm system are probably important
parameters influencing flash length and hence LNO&lt;sub&gt;x&lt;/sub&gt; production per flash.</p>
</abstract>
<counts><page-count count="36"/></counts>
</article-meta>
</front>
<body/>
<back>
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