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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-5-8879-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/8879/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/8879/2005/acpd-5-8879-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/8879/2005/acpd-5-8879-2005.pdf</fulltext_pdf>
	<start_page>8879</start_page>
	<end_page>8923</end_page>
	<publication_date>2005-09-19</publication_date>
	<article_title content_type="html">The direct inversion method for data assimilation using isentropic tracer advection</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>M. N. Juckes</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">British Atmospheric Data Centre, SSTD, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire, OX11 0QX, UK</affiliation>
	</affiliations>
	<abstract content_type="html">A new data assimilation algorithm is applied to MIPAS
and SBUV measurements of stratospheric ozone.
The results are validated against  HALOE, POAM III,
SAGE II and III, OSIRIS and ozonesonde data.
The new assimilation algorithm has the
accuracy of the Kalman smoother but is,
for the systems studied here with up to 200 000  variables
per time step and 61 million control variables in total,
many orders of magnitude less computationally expensive.
The analysis produced minimises a single penalty function
evaluated over an analysis window of over one month.
The cost of the analysis is found to increase nearly linearly
with the number of control variables.
Compared with 850 profiles from Electrochemical
Concentration Cell sondes at 29 sites the analysis is found
to be merely 0.1% high at 420 K, rising to 0.4% at 650 K (813 sonde profiles).
Comparison against the other satellites imply that the bias remains small
up to 1250 K (38 km) and then increases to around &amp;minus;10% at 1650 K (44 km).
Between 20 and 35 km the root-mean-square difference relative to HALOE,
SAGE II and III, and POAM is in the 5 to 10% range, with
larger discrepancies relative to other instruments.
Outside this height range rms differences are generally larger,
though agreement with HALOE remains good up to 50 km.</abstract>
	<references>
	</references>
</article>

