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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 GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-6-4427-2006</article-id>
<title-group>
<article-title>Simulations of preindustrial, present-day, and 2100 conditions in the NASA GISS composition and climate model G-PUCCINI</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shindell</surname>
<given-names>D.&amp;nbsp;T.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Faluvegi</surname>
<given-names>G.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Unger</surname>
<given-names>N.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Aguilar</surname>
<given-names>E.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Schmidt</surname>
<given-names>G.&amp;nbsp;A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Koch</surname>
<given-names>D.&amp;nbsp;M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</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>Bauer</surname>
<given-names>S.&amp;nbsp;E.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Miller</surname>
<given-names>R.&amp;nbsp;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-group><aff id="aff1">
<label>1</label>
<addr-line>NASA Goddard Institute for Space Studies, New York, NY, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Center for Climate Systems Research, Columbia University, NY, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Dept. of Geophysics, Yale University, New Haven, USA</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Dept. of Applied Physics and Applied Math, Columbia University, NY, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>04</day>
<month>10</month>
<year>2006</year>
</pub-date>
<volume>6</volume>
<issue>12</issue>
<fpage>4427</fpage>
<lpage>4459</lpage>
<permissions>
<license license-type="open-access">
<license-p>This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use,  distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
</license>
</permissions>
<self-uri xlink:href="http://www.atmos-chem-phys.net/6/4427/2006/acp-6-4427-2006.html">This article is available from http://www.atmos-chem-phys.net/6/4427/2006/acp-6-4427-2006.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/6/4427/2006/acp-6-4427-2006.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/6/4427/2006/acp-6-4427-2006.pdf</self-uri>
<abstract>
<p>A model of atmospheric composition and climate has been developed at the
NASA Goddard Institute for Space Studies (GISS) that includes composition
seamlessly from the surface to the lower mesosphere. The model is able to
capture many features of the observed magnitude, distribution, and seasonal
cycle of trace species. The simulation is especially realistic in the
troposphere. In the stratosphere, high latitude regions show substantial
biases during period when transport governs the distribution as meridional
mixing is too rapid in this model version. In other regions, including the
extrapolar tropopause region that dominates radiative forcing (RF) by ozone,
stratospheric gases are generally well-simulated. The model&apos;s
stratosphere-troposphere exchange (STE) agrees well with values inferred
from observations for both the global mean flux and the ratio of Northern (NH) to
Southern Hemisphere (SH) downward fluxes.

&lt;P&gt;

Simulations of preindustrial (PI) to present-day (PD) changes show
tropospheric ozone burden increases of 11% while the stratospheric burden
decreases by 18%. The resulting tropopause RF values are &amp;minus;0.06 W/m&lt;sup&gt;2&lt;/sup&gt;
from stratospheric ozone and 0.40 W/m&lt;sup&gt;2&lt;/sup&gt; from tropospheric ozone. Global
mean mass-weighted OH decreases by 16% from the PI to the PD. STE of
ozone also decreased substantially during this time, by 14%. Comparison
of the PD with a simulation using 1979 pre-ozone hole conditions for the
stratosphere shows a much larger downward flux of ozone into the troposphere
in 1979, resulting in a substantially greater tropospheric ozone burden than
that seen in the PD run. This implies that reduced STE due to stratospheric
ozone depletion may have offset as much as 2/3 of the tropospheric ozone
burden increase from PI to PD. However, the model overestimates the downward
flux of ozone at high Southern latitudes, so this estimate is likely an
upper limit.

&lt;P&gt;

In the future, the tropospheric ozone burden increases by 101% in 2100 for
the A2 scenario including both emissions and climate changes. The primary
reason is enhanced STE, which increases by 124% (168% in the SH
extratropics, and 114% in the NH extratropics). Climate plays a minimal
role in the SH increases, but contributes 38% in the NH.
Chemistry and dry deposition both change so as to reduce tropospheric ozone,
partially in compensation for the enhanced STE, but the increased ozone influx
dominates the burden changes. The net RF due to
projected ozone changes is 0.8 W/m&lt;sup&gt;2&lt;/sup&gt; for A2.
The influence of climate change alone is &amp;minus;0.2 W/m&lt;sup&gt;2&lt;/sup&gt;, making it a substantial
contributor to the net RF. The tropospheric
oxidation capacity increases seven percent in the full A2 simulation, and 36%
due to A2 climate change alone.</p>
</abstract>
<counts><page-count count="33"/></counts>
</article-meta>
</front>
<body/>
<back>
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