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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-12-10945-2012</article-id>
<title-group>
<article-title>Impact of very short-lived halogens on stratospheric ozone abundance and UV radiation in a geo-engineered atmosphere</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tilmes</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>Kinnison</surname>
<given-names>D. E.</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>Garcia</surname>
<given-names>R. R.</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>Salawitch</surname>
<given-names>R.</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>Canty</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>Lee-Taylor</surname>
<given-names>J.</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>Madronich</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>Chance</surname>
<given-names>K.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>National Center for Atmospheric Research, Boulder, Colorado, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>University of Maryland College Park, MD, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>20</day>
<month>11</month>
<year>2012</year>
</pub-date>
<volume>12</volume>
<issue>22</issue>
<fpage>10945</fpage>
<lpage>10955</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2012 S. Tilmes et al.</copyright-statement>
<copyright-year>2012</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/articles/12/10945/2012/acp-12-10945-2012.html">This article is available from https://acp.copernicus.org/articles/12/10945/2012/acp-12-10945-2012.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/12/10945/2012/acp-12-10945-2012.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/12/10945/2012/acp-12-10945-2012.pdf</self-uri>
<abstract>
<p>The impact of very short-lived (VSL) halogenated source species on the ozone
layer and surface erythemal ultraviolet radiation (UV&lt;sub&gt;ERY&lt;/sub&gt;) is
investigated in the context of geo-engineering of climate by stratospheric
sulfur injection. For a projected 2040 model atmosphere, consideration of VSL
halogens at their upper limit results in lower ozone columns and higher
UV&lt;sub&gt;ERY&lt;/sub&gt; due to geo-engineering for nearly all seasons and
latitudes, with UV&lt;sub&gt;ERY&lt;/sub&gt; rising by 12% and 6% in southern
and northern high latitudes, respectively. When VSL halogen sources are
neglected, future UV&lt;sub&gt;ERY&lt;/sub&gt; increases due to declines in ozone
column are nearly balanced by reductions of UV&lt;sub&gt;ERY&lt;/sub&gt; due to
scattering by the higher stratospheric aerosol burden in mid-latitudes.
Consideration of VSL sources at their upper limit tips the balance, resulting
in annual average increases in UV&lt;sub&gt;ERY&lt;/sub&gt; of up to 5% in mid and
high latitudes. Therefore, VSL halogens should be considered in models that
assess the impact of stratospheric sulfur injections on the ozone layer.</p>
</abstract>
<counts><page-count count="11"/></counts>
</article-meta>
</front>
<body/>
<back>
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