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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>5</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-10925-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/10925/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/10925/2005/acpd-5-10925-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/10925/2005/acpd-5-10925-2005.pdf</fulltext_pdf>
	<start_page>10925</start_page>
	<end_page>10946</end_page>
	<publication_date>2005-10-31</publication_date>
	<article_title content_type="html">Detection and measurement of total ozone from stellar spectra: Paper 2. Historic data from 1935–1942</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>R. E. M. Griffin</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Dept. of Earth and Space Sciences and Engineering, York University, 4700 Keele Street, Toronto, ON, M3J 1P3, Canada</affiliation>
		<affiliation numeration="2" content_type="html">Herzberg Institute for Astrophysics, 5071 West Saanich Road, Victoria, BC, V9E 2E7, Canada</affiliation>
	</affiliations>
	<abstract content_type="html">Atmospheric ozone columns are derived from historic stellar spectra observed
between 1935 and 1942 at Mount Wilson Observatory, California.  Comparisons
with contemporary measurements in the Arosa database show a generally close
correspondence.  The results of the analysis indicate that astronomy&apos;s archives
command considerable potential for investigating the natural levels of ozone
and its variability during the decades prior to anthropogenic interference.</abstract>
	<references>
	</references>
</article>

