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<article language="en">
	<journal>
		<journal_title>Atmospheric Measurement Techniques Discussions</journal_title>
		<journal_url>www.atmos-meas-tech-discuss.net</journal_url>
		<eissn>1867-8610</eissn>
		<volume_number>3</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/amtd-3-3971-2010</doi>
	<article_url>http://www.atmos-meas-tech-discuss.net/3/3971/2010/</article_url>
	<abstract_html>http://www.atmos-meas-tech-discuss.net/3/3971/2010/amtd-3-3971-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-meas-tech-discuss.net/3/3971/2010/amtd-3-3971-2010.pdf</fulltext_pdf>
	<start_page>3971</start_page>
	<end_page>3986</end_page>
	<publication_date>2010-08-30</publication_date>
	<article_title content_type="html">Observation of the exhaust plume from the space shuttle main engine using the Microwave Limb Sounder</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>H. C. Pumphrey</name>
			<email>h.c.pumphrey@ed.ac.uk</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>A. Lambert</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>N. J. Livesey</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of GeoSciences, The University of Edinburgh, Edinburgh, UK</affiliation>
		<affiliation numeration="2" content_type="html">NASA Jet Propulsion Laboratory, Pasadena, CA, USA</affiliation>
	</affiliations>
	<abstract content_type="html">A space shuttle launch deposits 700 t of water in the
atmosphere. Some of this water is released into the upper mesosphere
and lower thermosphere where it may be directly detected by a limb
sounding satellite instrument. We report measurements of water vapour
plumes from shuttle launches made by the Microwave Limb Sounder (MLS)
on the Aura satellite. Approximately 50% of shuttle launches are
detected by MLS. The signal appears at a similar level across the
upper 10 km of the MLS limb scan, suggesting that the bulk of the
observed water is above the top of the scan. Only a small fraction at
best of smaller launches (Ariane, Proton) are detected. We conclude
that the sensitivity of MLS is only just great enough to detect a
shuttle sized launch, but that a suitably designed instrument of the
same general type could detect the exhausts from a large proportion of
heavy-lift launches.</abstract>
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</article>

