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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>6</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-10087-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/10087/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/10087/2006/acpd-6-10087-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/10087/2006/acpd-6-10087-2006.pdf</fulltext_pdf>
	<start_page>10087</start_page>
	<end_page>10152</end_page>
	<publication_date>2006-10-11</publication_date>
	<article_title content_type="html">Evaluation of ozonesondes, HALOE, SAGE II and III, Odin-OSIRIS and SMR, and ENVISAT-GOMOS, -SCIAMACHY and -MIPAS ozone profiles in the tropics from SAOZ long duration balloon measurements in 2003 and 2004</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>F. Borchi</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>J.-P. Pommereau</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">CNRS, Service d’Aéronomie, Verrières le Buisson, France</affiliation>
	</affiliations>
	<abstract content_type="html">The performances of satellite and sondes ozone measuring instruments
available in the tropics between 10 and 26 km during the southern hemisphere
summer in 2003 and 2004, have been investigated by comparison with series of
profiles obtained by solar occultation in the visible Chappuis bands using a
SAOZ UV-Vis spectrometer carried by circumnavigating long duration balloons.
When compared to SAOZ, systematic positive or negative altitude shifts could
be observed in satellite profiles, varying from &amp;lt;50 m for the GOMOS
stellar occultation instrument, followed by +100/200 m for solar occultation
systems (SAGE II, HALOE above 22 km), but as large as &amp;minus;900 m or +2000 m for
limb viewing systems (OSIRIS, SCIAMACHY). The ozone relative biases are
generally limited, between &amp;minus;4% and +4%, for measurements in the
visible Chappuis bands (SAGE II and III, GOMOS above 22 km and OSIRIS), the
near IR (HALOE above 22 km) and the ozonesondes, but increase to &amp;minus;7% in
the UV (SCIAMACHY), and +7% in the mid-IR (MIPAS) and the submillimetric
range (SMR). Regarding precision, evaluated statistically from the zonal
variability of ozone concentration, the best measurements are found to be
those of SAGE II (2%), followed by HALOE above 22 km (3&amp;ndash;4%), then
the ozonesondes, SAGE III moon and OSIRIS (4&amp;ndash;5%), GOMOS above 22 km and
SCIAMACHY (~6%), MIPAS (8.5%) and finally SMR (16%).
Overall, all satellite ozone measurements appear little reliable in the
tropical troposphere except those of SAGE II (and eventually SAGE III),
though low biased by 50% and of limited (50%) precision.</abstract>
	<references>
	</references>
</article>

