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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>8</volume_number>
		<issue_number>16</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acp-8-4759-2008</doi>
	<article_url>http://www.atmos-chem-phys.net/8/4759/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/8/4759/2008/acp-8-4759-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/8/4759/2008/acp-8-4759-2008.pdf</fulltext_pdf>
	<start_page>4759</start_page>
	<end_page>4786</end_page>
	<publication_date>2008-08-19</publication_date>
	<article_title content_type="html">Validation of ACE-FTS N&lt;sub&gt;2&lt;/sub&gt;O measurements</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>K. Strong</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>M. A. Wolff</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>T. E. Kerzenmacher</name>
		</author>
		<author numeration="4" affiliations="1,2">
			<name>K. A. Walker</name>
		</author>
		<author numeration="5" affiliations="2,3">
			<name>P. F. Bernath</name>
		</author>
		<author numeration="6" affiliations="4">
			<name>T. Blumenstock</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>C. Boone</name>
		</author>
		<author numeration="8" affiliations="5">
			<name>V. Catoire</name>
		</author>
		<author numeration="9" affiliations="6">
			<name>M. Coffey</name>
		</author>
		<author numeration="10" affiliations="7">
			<name>M. De MaziÃ¨re</name>
		</author>
		<author numeration="11" affiliations="8">
			<name>P. Demoulin</name>
		</author>
		<author numeration="12" affiliations="8">
			<name>P. Duchatelet</name>
		</author>
		<author numeration="13" affiliations="2">
			<name>E. Dupuy</name>
		</author>
		<author numeration="14" affiliations="6">
			<name>J. Hannigan</name>
		</author>
		<author numeration="15" affiliations="4">
			<name>M. HÃ¶pfner</name>
		</author>
		<author numeration="16" affiliations="4">
			<name>N. Glatthor</name>
		</author>
		<author numeration="17" affiliations="9">
			<name>D. W. T. Griffith</name>
		</author>
		<author numeration="18" affiliations="10">
			<name>J. J. Jin</name>
		</author>
		<author numeration="19" affiliations="9">
			<name>N. Jones</name>
		</author>
		<author numeration="20" affiliations="11">
			<name>K. Jucks</name>
		</author>
		<author numeration="21" affiliations="12">
			<name>H. Kuellmann</name>
		</author>
		<author numeration="22" affiliations="12,21">
			<name>J. Kuttippurath</name>
		</author>
		<author numeration="23" affiliations="13">
			<name>A. Lambert</name>
		</author>
		<author numeration="24" affiliations="8">
			<name>E. Mahieu</name>
		</author>
		<author numeration="25" affiliations="10">
			<name>J. C. McConnell</name>
		</author>
		<author numeration="26" affiliations="14">
			<name>J. Mellqvist</name>
		</author>
		<author numeration="27" affiliations="4">
			<name>S. Mikuteit</name>
		</author>
		<author numeration="28" affiliations="14">
			<name>D. P. Murtagh</name>
		</author>
		<author numeration="29" affiliations="12">
			<name>J. Notholt</name>
		</author>
		<author numeration="30" affiliations="15">
			<name>C. Piccolo</name>
		</author>
		<author numeration="31" affiliations="16">
			<name>P. Raspollini</name>
		</author>
		<author numeration="32" affiliations="17">
			<name>M. Ridolfi</name>
		</author>
		<author numeration="33" affiliations="5">
			<name>C. Robert</name>
		</author>
		<author numeration="34" affiliations="4">
			<name>M. Schneider</name>
		</author>
		<author numeration="35" affiliations="18">
			<name>O. Schrems</name>
		</author>
		<author numeration="36" affiliations="10">
			<name>K. Semeniuk</name>
		</author>
		<author numeration="37" affiliations="7">
			<name>C. Senten</name>
		</author>
		<author numeration="38" affiliations="4">
			<name>G. P. Stiller</name>
		</author>
		<author numeration="39" affiliations="14">
			<name>A. Strandberg</name>
		</author>
		<author numeration="40" affiliations="1">
			<name>J. Taylor</name>
		</author>
		<author numeration="41" affiliations="19">
			<name>C. TÃ©tard</name>
		</author>
		<author numeration="42" affiliations="1">
			<name>M. Toohey</name>
		</author>
		<author numeration="43" affiliations="14">
			<name>J. Urban</name>
		</author>
		<author numeration="44" affiliations="12">
			<name>T. Warneke</name>
		</author>
		<author numeration="45" affiliations="20">
			<name>S. Wood</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Department of Physics, University of Toronto, Toronto, Ontario, Canada</affiliation>
		<affiliation numeration="2" content_type="html">Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada</affiliation>
		<affiliation numeration="3" content_type="html">Department of Chemistry, University of York, York, UK</affiliation>
		<affiliation numeration="4" content_type="html">Forschungszentrum Karlsruhe and University of Karlsruhe, Institute for Meteorology and Climate Research (IMK), Karlsruhe, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Laboratoire de Physique et Chimie de L&apos;Environment CNRS â€“ UniversitÃ© d&apos;OrlÃ©ans, OrlÃ©ans, France</affiliation>
		<affiliation numeration="6" content_type="html">National Center for Atmospheric Research, Boulder, CO, USA</affiliation>
		<affiliation numeration="7" content_type="html">Belgian Institute for Space Aeronomy, Brussels, Belgium</affiliation>
		<affiliation numeration="8" content_type="html">Institute of Astrophysics and Geophysics, University of LiÃ¨ge, LiÃ¨ge, Belgium</affiliation>
		<affiliation numeration="9" content_type="html">School of Chemistry, University of Wollongong, Wollongong, Australia</affiliation>
		<affiliation numeration="10" content_type="html">Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada</affiliation>
		<affiliation numeration="11" content_type="html">Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA</affiliation>
		<affiliation numeration="12" content_type="html">Institute for Environmental Physics, University of Bremen, Bremen, Germany</affiliation>
		<affiliation numeration="13" content_type="html">Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA</affiliation>
		<affiliation numeration="14" content_type="html">Department of Radio and Space Science, Chalmers University of Technology, Gothenburg, Sweden</affiliation>
		<affiliation numeration="15" content_type="html">Department of Physics, University of Oxford, Oxford, UK</affiliation>
		<affiliation numeration="16" content_type="html">Institute of Applied Physics &quot;Nello Carrara&quot;, National Research Center, Firenze, Italy</affiliation>
		<affiliation numeration="17" content_type="html">Dipartimento di Chimica Fisica e Inorganica, UniversitÃ  di Bologna, Bologna, Italy</affiliation>
		<affiliation numeration="18" content_type="html">Alfred Wegener Institute for Polar and Marine Research, Bremerhaven, Germany</affiliation>
		<affiliation numeration="19" content_type="html">Laboratoire d&apos;Optique AtmosphÃ©rique, UniversitÃ© des sciences et technologies de Lille, Villeneuve d&apos;Ascq, France</affiliation>
		<affiliation numeration="20" content_type="html">National Institute of Water and Atmospheric Research Ltd., Lauder, New Zealand</affiliation>
		<affiliation numeration="21" content_type="html">now at: LMD/CNRS Ecole Polytechnique, Palaiseau Cedex, France</affiliation>
	</affiliations>
	<abstract content_type="html">The Atmospheric Chemistry Experiment (ACE), also known as SCISAT, was launched
on 12 August 2003, carrying two instruments that measure vertical profiles of
atmospheric constituents using the solar occultation technique. One of these
instruments, the ACE Fourier Transform Spectrometer (ACE-FTS), is measuring volume
mixing ratio (VMR) profiles of nitrous oxide (N&lt;sub&gt;2&lt;/sub&gt;O) from the upper troposphere
to the lower mesosphere at a vertical resolution of about 3â€“4 km. In this study,
the quality of the ACE-FTS version 2.2 N&lt;sub&gt;2&lt;/sub&gt;O data is assessed through comparisons
with coincident measurements made by other satellite, balloon-borne, aircraft,
and ground-based instruments. These consist of vertical profile comparisons with
the SMR, MLS, and MIPAS satellite instruments, multiple aircraft flights of ASUR,
and single balloon flights of SPIRALE and FIRS-2, and partial column comparisons
with a network of ground-based Fourier Transform InfraRed spectrometers (FTIRs).
Between 6 and 30 km, the mean absolute differences for the satellite comparisons lie between &amp;minus;42 ppbv and
+17 ppbv, with most within &amp;plusmn;20 ppbv. This corresponds to relative deviations
from the mean that are within &amp;plusmn;15%, except for comparisons with MIPAS near
30 km, for which they are as large as 22.5%. Between 18 and 30 km, the mean
absolute differences for the satellite comparisons are generally within &amp;plusmn;10 ppbv.
From 30 to 60 km, the mean absolute differences are
within &amp;plusmn;4 ppbv, and are mostly between &amp;minus;2 and +1 ppbv. Given the small
N&lt;sub&gt;2&lt;/sub&gt;O VMR in this region, the relative deviations from the mean are therefore
large at these altitudes, with most suggesting a negative bias in the ACE-FTS
data between 30 and 50 km. In the comparisons with the FTIRs, the mean relative
differences between the ACE-FTS and FTIR partial columns (which cover a mean altitude range of 14 to 27 km)
are within &amp;plusmn;5.6% for eleven of the twelve contributing stations. This mean relative difference is
negative at ten stations, suggesting a small negative bias in the ACE-FTS partial
columns over the altitude regions compared. Excellent correlation (&lt;i&gt;R&lt;/i&gt;=0.964) is
observed between the ACE-FTS and FTIR partial columns, with a slope of 1.01 and
an intercept of &amp;minus;0.20 on the line fitted to the data.</abstract>
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</article>

