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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>6</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acpd-6-12301-2006</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/6/12301/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/6/12301/2006/acpd-6-12301-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/6/12301/2006/acpd-6-12301-2006.pdf</fulltext_pdf>
	<start_page>12301</start_page>
	<end_page>12345</end_page>
	<publication_date>2006-11-29</publication_date>
	<article_title content_type="html">Near-real time retrieval of tropospheric NO&lt;sub&gt;2&lt;/sub&gt; from OMI</article_title>
	<authors>
		<author numeration="1" affiliations="1,3">
			<name>K. F. Boersma</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>H. J. Eskes</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>J. P. Veefkind</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>E. J. Brinksma</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>R. J. van der A</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>M. Sneep</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>G. H. J. van der Oord</name>
		</author>
		<author numeration="8" affiliations="1">
			<name>P. F. Levelt</name>
		</author>
		<author numeration="9" affiliations="1">
			<name>P. Stammes</name>
		</author>
		<author numeration="10" affiliations="2">
			<name>J. F. Gleason</name>
		</author>
		<author numeration="11" affiliations="2">
			<name>E. J. Bucsela</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">KNMI, De Bilt, The Netherlands</affiliation>
		<affiliation numeration="2" content_type="html">NASA GSFC, Greenbelt, Maryland, USA</affiliation>
		<affiliation numeration="3" content_type="html">now at: Harvard University, Cambridge, USA</affiliation>
	</affiliations>
	<abstract content_type="html">We present a new algorithm for the near-real time retrieval &amp;ndash; within 3 h
of the actual satellite measurement &amp;ndash; of tropospheric NO&lt;sub&gt;2&lt;/sub&gt; columns
from the Ozone Monitoring Instrument (OMI). The retrieval system is based on
the combined retrieval-assimilation-modelling approach developed at KNMI for
off-line tropospheric NO&lt;sub&gt;2&lt;/sub&gt; from the GOME and SCIAMACHY satellite
instruments. We have adapted the off-line system such that the required a
priori information ndash; profile shapes and stratospheric background
NO&lt;sub&gt;2&lt;/sub&gt; ndash; is now immediately available upon arrival of the OMI
NO&lt;sub&gt;2&lt;/sub&gt; slant columns and cloud data at KNMI. Slant column NO&lt;sub&gt;2&lt;/sub&gt;
and cloud information arrives at KNMI typically within 80 min of actual
OMI observations. Slant columns for NO&lt;sub&gt;2&lt;/sub&gt; are retrieved using
differential optical absorption spectroscopy (DOAS) in the 405&amp;ndash;465 nm
range. Cloud fraction and cloud pressure are provided by a new cloud
retrieval algorithm that uses the absorption of the O&lt;sub&gt;2&lt;/sub&gt;&amp;ndash;O&lt;sub&gt;2&lt;/sub&gt; collision
complex near 477 nm. On-line availability of stratospheric slant
columns and NO&lt;sub&gt;2&lt;/sub&gt; profiles is achieved by running the TM4 chemistry
transport model (CTM) forward in time based on forecast ECMWF meteo and
assimilated NO&lt;sub&gt;2&lt;/sub&gt; information from all previously observed orbits. OMI
NO&lt;sub&gt;2&lt;/sub&gt; slant columns, after correction for spurious across-track
variability, show a random error for individual pixels of approximately
0.7&amp;times;10&lt;sup&gt;15&lt;/sup&gt;molec.cm&lt;sup&gt;&amp;ndash;2&lt;/sup&gt;.
As NO&lt;sub&gt;2&lt;/sub&gt; retrievals are very sensitive to clouds, we evaluated the
consistency of cloud fraction and cloud pressure from the new O&lt;sub&gt;2&lt;/sub&gt;&amp;ndash;O&lt;sub&gt;2&lt;/sub&gt;
(OMI) algorithm and from the Fast Retrieval Scheme for Cloud Observables
(FRESCO). Cloud parameters from the O&lt;sub&gt;2&lt;/sub&gt;&amp;ndash;O&lt;sub&gt;2&lt;/sub&gt; (OMI) algorithm have
similar frequency distributions as cloud parameters retrieved from
FRESCO (SCIAMACHY) for August 2006. On average, OMI cloud fractions are higher by 0.011, and OMI
cloud pressures exceed FRESCO cloud pressures by 60 hPa. As a
consistency check, we intercompared OMI near-real time NO&lt;sub&gt;2&lt;/sub&gt; columns
measured at 13:45 h local time to SCIAMACHY off-line NO&lt;sub&gt;2&lt;/sub&gt; columns
measured at 10:00 h local time. In August 2006, both instruments observe
very similar spatial patterns of tropospheric NO&lt;sub&gt;2&lt;/sub&gt; columns, and small
differences for most locations on Earth where tropospheric NO&lt;sub&gt;2&lt;/sub&gt;
columns are small. For regions that are strongly polluted, SCIAMACHY observes
higher tropospheric NO&lt;sub&gt;2&lt;/sub&gt; columns than OMI.</abstract>
	<references>
	</references>
</article>

