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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>7</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/acpd-7-10543-2007</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/7/10543/2007/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/7/10543/2007/acpd-7-10543-2007.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/7/10543/2007/acpd-7-10543-2007.pdf</fulltext_pdf>
	<start_page>10543</start_page>
	<end_page>10588</end_page>
	<publication_date>2007-07-23</publication_date>
	<article_title content_type="html">Short- and medium-term atmospheric effects of very large solar proton events</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>C. H. Jackman</name>
			<email>charles.h.jackman@nasa.gov</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>D. R. Marsh</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>F. M. Vitt</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>R. R. Garcia</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>E. L. Fleming</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>G. J. Labow</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>C. E. Randall</name>
		</author>
		<author numeration="8" affiliations="4">
			<name>M. López-Puertas</name>
		</author>
		<author numeration="9" affiliations="4">
			<name>B. Funke</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">NASA/Goddard Space Flight Center, Greenbelt, MD, USA</affiliation>
		<affiliation numeration="2" content_type="html">National Center for Atmospheric Research, Boulder, CO, USA</affiliation>
		<affiliation numeration="3" content_type="html">University of Colorado, Boulder, CO, USA</affiliation>
		<affiliation numeration="4" content_type="html">Instituto de-Astrofisica de Andalucia, CSIC, Granada, Spain</affiliation>
	</affiliations>
	<abstract content_type="html">Solar eruptions sometimes produce protons, which impact the Earth&apos;s
atmosphere. These solar proton events (SPEs) generally last a few days and
produce high energy particles that precipitate into the Earth&apos;s atmosphere.
The protons cause ionization and dissociation processes that ultimately lead
to an enhancement of odd-hydrogen and odd-nitrogen in the polar cap regions
(&amp;gt;60&amp;deg; geomagnetic latitude). We have used the Whole Atmosphere
Community Climate Model (WACCM3) to study the atmospheric impact of SPEs
over the period 1963&amp;ndash;2005. The very largest SPEs were found to be the most
important and caused atmospheric effects that lasted several months to years
after the events. We present the short- and medium-term (days to a few
months) atmospheric influence of the four largest SPEs in the past 45 years
(August 1972; October 1989; July 2000; and October&amp;ndash;November 2003) as
computed by WACCM3 and observed by satellite instruments. The polar effects
can be summarized as follows: 1) Mesospheric NO&lt;sub&gt;x&lt;/sub&gt; (NO+NO&lt;sub&gt;2&lt;/sub&gt;)
increased by over 50 ppbv and mesospheric ozone decreased by over 30%
during these very large SPEs; 2) upper stratospheric and lower mesospheric
NO&lt;sub&gt;x&lt;/sub&gt; increased by over 10 ppbv and was transported during polar night
down to the middle stratosphere in a few weeks; 3) mid- to upper
stratospheric ozone decreased over 20%; and 4) enhancements of HNO&lt;sub&gt;3&lt;/sub&gt;,
HOCl, ClO, ClONO&lt;sub&gt;2&lt;/sub&gt;, and N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; were indirectly caused by the
very large SPEs, although the model results suggest impacts at higher
altitudes than indicated by the measurements for the October&amp;ndash;November 2003 SPE
period.</abstract>
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