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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 Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-4-1237-2004</article-id>
<title-group>
<article-title>Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: &lt;sup&gt;14&lt;/sup&gt;N&lt;sup&gt;14&lt;/sup&gt;NO, &lt;sup&gt;15&lt;/sup&gt;N&lt;sup&gt;14&lt;/sup&gt;NO, &lt;sup&gt;14&lt;/sup&gt;N&lt;sup&gt;15&lt;/sup&gt;NO and &lt;sup&gt;15&lt;/sup&gt;N&lt;sup&gt;15&lt;/sup&gt;NO</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>von Hessberg</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>Kaiser</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Enghoff</surname>
<given-names>M. B.</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>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>Sorensen</surname>
<given-names>S. L.</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>Röckmann</surname>
<given-names>T.</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>Johnson</surname>
<given-names>M. S.</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 Chemistry, University of Copenhagen, Copenhagen, Denmark</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Max-Planck Institute for Nuclear Physics, Atmospheric Physics Division, Heidelberg, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Air Quality Research Branch, Meteorological Service of Canada, Toronto, Ontario, Canada</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Synchrotron Radiation Research, Lund University, Lund, Sweden</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>now at Department of Geosciences, Princeton University, Princeton, New Jersey, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>10</day>
<month>08</month>
<year>2004</year>
</pub-date>
<volume>4</volume>
<issue>5</issue>
<fpage>1237</fpage>
<lpage>1253</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 P. von Hessberg et al.</copyright-statement>
<copyright-year>2004</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/articles/4/1237/2004/acp-4-1237-2004.html">This article is available from https://acp.copernicus.org/articles/4/1237/2004/acp-4-1237-2004.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/4/1237/2004/acp-4-1237-2004.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/4/1237/2004/acp-4-1237-2004.pdf</self-uri>
<abstract>
<p>The isotopically substituted nitrous oxide species &lt;sup&gt;14&lt;/sup&gt;N&lt;sup&gt;14&lt;/sup&gt;NO, &lt;sup&gt;15&lt;/sup&gt;N&lt;sup&gt;14&lt;/sup&gt;NO,
&lt;sup&gt;14&lt;/sup&gt;N&lt;sup&gt;15&lt;/sup&gt;NO and &lt;sup&gt;15&lt;/sup&gt;N&lt;sup&gt;15&lt;/sup&gt;NO were investigated by
ultra-violet (UV) absorption spectroscopy. High precision cross sections
were obtained for the wavelength range 181 to 218nm at temperatures of 233
and 283K. These data are used to calculate photolytic isotopic
fractionation constants as a function of wavelength. The fractionation
constants were used in a three-dimensional chemical transport model in order
to simulate the actual fractionation of N&lt;sub&gt;2&lt;/sub&gt;O in the stratosphere, and
the results were found to be in good agreement with field studies.</p>
</abstract>
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