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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<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>3</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/acpd-3-3411-2003</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/3/3411/2003/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/3/3411/2003/acpd-3-3411-2003.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/3/3411/2003/acpd-3-3411-2003.pdf</fulltext_pdf>
	<start_page>3411</start_page>
	<end_page>3449</end_page>
	<publication_date>2003-07-03</publication_date>
	<article_title content_type="html">Global distribution of total ozone and lower stratospheric temperature variations</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>W. Steinbrecht</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>B. Hassler</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>H. Claude</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>P. Winkler</name>
		</author>
		<author numeration="5" affiliations="2">
			<name>R. S. Stolarski</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">German Weather Service, Hohenpeissenberg, Germany</affiliation>
		<affiliation numeration="2" content_type="html">NASA, Goddard Space Flight Center, Greenbelt, Maryland, USA</affiliation>
	</affiliations>
	<abstract content_type="html">This study gives an overview of interannual variations of total ozone
      and 50hPa temperature. It is based on newer and longer records from the 1979 to 2001 Total Ozone Monitoring Spectrometer (TOMS) and Solar Backscatter
      Ultraviolet (SBUV) instruments, and on US National Center for Environmental
      Prediction (NCEP) reanalyses. Multiple linear least squares regression is used
      to quantify various natural and anthropogenic influences. For most influences
      the total ozone and 50hPa temperature responses look very similar, reflecting a
      very close coupling. As a rule of thumb, a 10 Dobson Unit (DU) change in total ozone corresponds to a
      1K change of 50hPa temperature. Large influences come from the linear trend term, up to
      &amp;minus;30 DU or &amp;minus;1.5 K/decade, from terms related to polar vortex strength, up to
      50 DU or 5 K (typical, minimum to maximum), from tropospheric meteorology, up to
      30 DU or 3 K, or from the Quasi-Biennial Oscillation (QBO), up to 25 DU or
      2.5 K. The 11-year solar cycle, up to 25 DU or 2.5 K, El Niño/Southern Oscillation
      (&lt;i&gt;ENSO&lt;/i&gt;), up to 10 DU or 1 K, are somewhat smaller influences. Stratospheric aerosol after
      the 1991 Pinatubo eruption lead to warming up to 3 K at low latitudes and to
      ozone depletion up to 40 DU at high latitudes. Response to QBO, polar vortex
      strength, and to a lesser degree to &lt;i&gt;ENSO&lt;/i&gt;, exhibit an inverse correlation between
      low latitudes and higher latitudes. Responses to the solar cycle or 400 hPa
      temperature, however, have the same sign over most of the globe. Responses are
      usually zonally symmetric at low and mid-latitudes, but asymmetric at high
      latitudes. There, solar cycle, QBO or &lt;i&gt;ENSO&lt;/i&gt; influence position and strength of the stratospheric
      anti-cyclones over the Aleutians and south of Australia.</abstract>
	<references>
	</references>
</article>

