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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys.net/inc/acp/copernicus.dtd">
<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>4</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acp-4-231-2004</doi>
	<article_url>http://www.atmos-chem-phys.net/4/231/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/4/231/2004/acp-4-231-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/4/231/2004/acp-4-231-2004.pdf</fulltext_pdf>
	<start_page>231</start_page>
	<end_page>254</end_page>
	<publication_date>2004-02-09</publication_date>
	<article_title content_type="html">Multi axis differential optical absorption spectroscopy (MAX-DOAS)</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>G. Hönninger</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. von Friedeburg</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>U. Platt</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Umweltphysik, Universität Heidelberg, Heidelberg, Germany</affiliation>
		<affiliation numeration="2" content_type="html">now at: Meteorological Service of Canada, Toronto, Canadanals.ne</affiliation>
	</affiliations>
	<abstract content_type="html">Multi Axis Differential Optical Absorption Spectroscopy
      (MAX-DOAS) in the atmosphere is a novel measurement technique that represents a significant advance on the well-established zenith
      scattered sunlight DOAS instruments which are mainly sensitive to stratospheric absorbers.
      MAX-DOAS utilizes scattered sunlight received from multiple viewing directions. The spatial
      distribution of various trace gases close to the instrument can be derived by combining several
      viewing directions. Ground based MAX-DOAS is highly sensitive to absorbers in the lowest few
      kilometres of the atmosphere and vertical profile information can be retrieved by combining the
      measurements with Radiative Transfer Model (RTM) calculations. The potential of the technique for
      a wide variety of studies of tropospheric trace species and its (few) limitations are discussed. A
      Monte Carlo RTM is applied to calculate Airmass Factors (AMF) for the various viewing geometries
      of MAX-DOAS. Airmass Factors can be used to quantify the light path length within the absorber
      layers. The airmass factor dependencies on the viewing direction and the influence of several
      parameters (trace gas profile, ground albedo, aerosol profile and type, solar zenith and azimuth
      angles) are investigated. In addition we give a brief description of the instrumental
      MAX-DOAS systems realised and deployed so far. The results of the RTM studies are compared to several
      examples of recent MAX-DOAS field experiments and an outlook for future possible applications is
      given.</abstract>
	<references>
	</references>
</article>

