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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>4</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-5183-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/5183/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/5183/2005/acpd-5-5183-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/5183/2005/acpd-5-5183-2005.pdf</fulltext_pdf>
	<start_page>5183</start_page>
	<end_page>5221</end_page>
	<publication_date>2005-07-22</publication_date>
	<article_title content_type="html">Effects of column density on I&lt;sub&gt;2&lt;/sub&gt; spectroscopy and a determination of I&lt;sub&gt;2&lt;/sub&gt; absorption cross section at 500 nm</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>P. Spietz</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>J. C. Gómez Martín</name>
		</author>
		<author numeration="3" affiliations="">
			<name>J. P. Burrows</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Environmental Physics (IUP), University of Bremen, PO Box 330440, 28334 Bremen, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The use of ro-vibronic spectra of I&lt;sub&gt;2&lt;/sub&gt; in the region of 543 nm to 578 nm as
reference spectra for atmospheric Differential Optical Absorption
Spectroscopy is studied. In this study it is shown that the retrieval of
atmospheric column densities with Differential Optical Absorption
Spectroscopy set-ups at FWHM at and above 1nm depends critically on the
column density, under which the used reference spectrum was recorded.
Systematic overestimation of the comparatively low atmospheric column
density of I&lt;sub&gt;2&lt;/sub&gt; of the order of 13% is possible. Under low pressure
conditions relevant in laboratory studies, the systematic deviations may
grow up to 45%. To avoid such effects with respect to field measurements,
new reference spectra of I&lt;sub&gt;2&lt;/sub&gt; were determined under column density of the
order of 10&lt;sup&gt;16&lt;/sup&gt; molec/cm&lt;sup&gt;2&lt;/sup&gt; close to that expected for the atmospheric
measurement. Thereby the described systematic deviations are avoided. Two
typical configurations of Differential Optical Absorption Spectroscopy,
which use grating spectrometers, were chosen for the spectroscopic set-up.
One spectrum was recorded at similar resolution (0.25 nm FWHM) but finer
binning (0.035 nm/pixel) than previously published data. For the other (0.59 nm
FWHM, 0.154 nm/pixel) no previously published spectra exist. Wavelength
calibration is accurate to &amp;plusmn;0.04 nm and &amp;plusmn;0.11 nm respectively. The
absorption cross section for the recordings was determined under low column
density with an accuracy of &amp;plusmn;4% and &amp;plusmn;3% respectively. The
absolute absorption cross section of I&lt;sub&gt;2&lt;/sub&gt; at 500 nm (in standard air) in
the continuum absorption region was determined using a method independent of
iodine vapour pressure. Obtained was &amp;sigma;&lt;sub&gt;I&lt;sub&gt;2&lt;/sub&gt;&lt;/sub&gt;(500 nm)=(2.186&amp;plusmn;0.021)&amp;middot;10&lt;sup&gt;&amp;minus;18&lt;/sup&gt; cm&lt;sup&gt;2&lt;/sup&gt;&amp;middot;molec&lt;sup&gt;&amp;minus;1&lt;/sup&gt; in very good agreement
with previously published results, but at 50% smaller uncertainty. From
this and previously published results a weighted average of &amp;sigma;&lt;sub&gt;I&lt;sub&gt;2&lt;/sub&gt;&lt;/sub&gt;(500 nm)=(2.191&amp;plusmn;0.02)
&amp;middot;10&lt;sup&gt;&amp;minus;18&lt;/sup&gt; cm&lt;sup&gt;2&lt;/sup&gt;&amp;middot;molec&lt;sup&gt;&amp;minus;1&lt;/sup&gt; is determined.</abstract>
	<references>
	</references>
</article>

