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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-6-3535-2006</article-id>
<title-group>
<article-title>Probing stratospheric transport and chemistry with new balloon and aircraft observations of the meridional and vertical N&lt;sub&gt;2&lt;/sub&gt;O isotope distribution</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kaiser</surname>
<given-names>J.</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>Engel</surname>
<given-names>A.</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>Borchers</surname>
<given-names>R.</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>RÃ¶ckmann</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Atmospheric Physics Division, Max Planck Institute for Nuclear  Physics, Heidelberg, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institute for Atmosphere and Environment, J. W. Goethe University,  Frankfurt, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Planets and Comets Department, Max Planck Institute for Solar System  Research, Katlenburg-Lindau, Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>now at: School of Environmental Sciences, University of East  Anglia, Norwich, UK</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>now at: Institute for Marine and  Atmospheric Research Utrecht, Utrecht University, The Netherlands</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>08</month>
<year>2006</year>
</pub-date>
<volume>6</volume>
<issue>11</issue>
<fpage>3535</fpage>
<lpage>3556</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/6/3535/2006/acp-6-3535-2006.html">This article is available from http://www.atmos-chem-phys.net/6/3535/2006/acp-6-3535-2006.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/6/3535/2006/acp-6-3535-2006.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/6/3535/2006/acp-6-3535-2006.pdf</self-uri>
<abstract>
<p>A comprehensive set of stratospheric balloon and aircraft samples was analyzed
for the position-dependent isotopic composition of nitrous oxide (N&lt;sub&gt;2&lt;/sub&gt;O).
Results for a total of 220 samples from between 1987 and 2003 are presented,
nearly tripling the number of mass-spectrometric N&lt;sub&gt;2&lt;/sub&gt;O isotope measurements
in the stratosphere published to date. Cryogenic balloon samples were obtained
at polar (Kiruna/Sweden, 68&amp;deg; N), mid-latitude (southern France,
44&amp;deg; N) and tropical sites (Hyderabad/India, 18&amp;deg; N). Aircraft
samples were collected with a newly-developed whole air sampler on board of the
high-altitude aircraft M55 Geophysica during the EUPLEX 2003 campaign. For
mixing ratios above 200 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, relative isotope enrichments
(&amp;delta; values) and mixing ratios display a compact relationship,
which is nearly independent of latitude and season and which can be explained
equally well by Rayleigh fractionation or mixing. However, for mixing ratios
below 200 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt; this compact relationship gives way to meridional,
seasonal and interannual variations. A comparison to a previously published
mid-latitude balloon profile even shows large zonal variations, justifying the
use of three-dimensional (3-D) models for further data interpretation.

&lt;P&gt;

In general, the magnitude of the apparent fractionation constants (i.e.,
apparent isotope effects) increases continuously with altitude and decreases
from the equator to the North Pole. Only the latter observation can be
understood qualitatively by the interplay between the time-scales of N&lt;sub&gt;2&lt;/sub&gt;O
photochemistry and transport in a Rayleigh fractionation framework. Deviations
from Rayleigh fractionation behavior also occur where polar vortex air mixes
with nearly N&lt;sub&gt;2&lt;/sub&gt;O-free upper stratospheric/mesospheric air (e.g., during the
boreal winters of 2003 and possibly 1992). Aircraft observations in the polar
vortex at mixing ratios below 200 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt; deviate from isotope
variations expected for both Rayleigh fractionation and two-end-member mixing, but
could be explained by continuous weak mixing between intravortex and extravortex
air (Plumb et al., 2000). However, it appears that none of the simple approaches
described here can capture all features of the stratospheric N&lt;sub&gt;2&lt;/sub&gt;O isotope
distribution, again justifying the use of 3-D models. Finally, correlations
between &lt;sup&gt;18&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O and average &lt;sup&gt;15&lt;/sup&gt;N/&lt;sup&gt;14&lt;/sup&gt;N isotope ratios or
between the position-dependent &lt;sup&gt;15&lt;/sup&gt;N/&lt;sup&gt;14&lt;/sup&gt;N isotope ratios show that
photo-oxidation makes a large contribution to the total N&lt;sub&gt;2&lt;/sub&gt;O sink in the
lower stratosphere (possibly up to 100% for N&lt;sub&gt;2&lt;/sub&gt;O mixing ratios above
300 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt;). Towards higher altitudes, the temperature dependence of
these isotope correlations becomes visible in the stratospheric observations.</p>
</abstract>
<counts><page-count count="22"/></counts>
</article-meta>
</front>
<body/>
<back>
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