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<article language="en">
	<journal>
		<journal_title>Atmospheric Measurement Techniques Discussions</journal_title>
		<journal_url>www.atmos-meas-tech-discuss.net</journal_url>
		<eissn>1867-8610</eissn>
		<volume_number>2</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/amtd-2-303-2009</doi>
	<article_url>http://www.atmos-meas-tech-discuss.net/2/303/2009/</article_url>
	<abstract_html>http://www.atmos-meas-tech-discuss.net/2/303/2009/amtd-2-303-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-meas-tech-discuss.net/2/303/2009/amtd-2-303-2009.pdf</fulltext_pdf>
	<start_page>303</start_page>
	<end_page>342</end_page>
	<publication_date>2009-02-09</publication_date>
	<article_title content_type="html">Retrieval of SO&lt;sub&gt;2&lt;/sub&gt; from thermal infrared satellite measurements: correction procedures for the effects of volcanic ash</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>S. Corradini</name>
			<email>corradini@ingv.it</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>L. Merucci</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>A. J. Prata</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Istituto Nazionale di Geofisica e Vulcanologia,Via di Vigna Murata 605, 00143 Roma, Italy</affiliation>
		<affiliation numeration="2" content_type="html">Norwegian Institute for Air Research, Instituttveien 18 Kjeller, 2027, Norway</affiliation>
	</affiliations>
	<abstract content_type="html">The simultaneous presence of SO&lt;sub&gt;2&lt;/sub&gt; and ash in a volcanic plume can lead to a
significant error in the SO&lt;sub&gt;2&lt;/sub&gt; columnar abundance retrieval when multispectral
Thermal InfraRed (TIR) data are used. The ash particles within the plume with
effective radii (from 1 to 10 Î¼m) reduce
the Top Of Atmosphere (TOA) radiance in the entire TIR spectral range, including
the channels used for SO&lt;sub&gt;2&lt;/sub&gt; retrieval. The net effect is a significant
SO&lt;sub&gt;2&lt;/sub&gt; overestimation.

&lt;br&gt;&lt;br&gt;
In this work the interference of ash is discussed and two correction
procedures for satellite SO&lt;sub&gt;2&lt;/sub&gt; volcanic plume
retrieval in the TIR spectral range are developed to achieve an
higher computation speed and a better accuracy.

&lt;br&gt;&lt;br&gt;
The ash correction can be applied when the
sensor spectral range includes the 7.3 and/or 8.7 Î¼m SO&lt;sub&gt;2&lt;/sub&gt;
absorption bands, and the split window bands centered around 11 and 12 Î¼m required
for ash retrieval. This allows the possibility of a simultaneous estimation
of both volcanic SO&lt;sub&gt;2&lt;/sub&gt; and ash in the same data set.
The proposed ash correction procedures have been applied to
the Moderate Resolution Imaging Spectroradiometer
(MODIS) and the Spin Enhanced Visible and Infrared Imager (SEVIRI)
measurements. Data collected during the 24
November 2006 Mt. Etna eruption have been used to illustrate the technique.
The SO&lt;sub&gt;2&lt;/sub&gt; and ash estimations are carried out by using a least
squares fit method and the Brightness Temperature Difference (BTD) procedures,
respectively. The simulated TOA radiance Look-Up Table
(LUT) needed for the SO&lt;sub&gt;2&lt;/sub&gt; columnar abundance and the ash retrievals have
been computed using the MODTRAN 4 Radiative Transfer Model.

&lt;br&gt;&lt;br&gt;
The results show the importance of the ash correction
on SO&lt;sub&gt;2&lt;/sub&gt; retrieval at 8.7 Î¼m â€“ the SO&lt;sub&gt;2&lt;/sub&gt; columnar abundance corrected
by the ash influence is less than one half of the values retrieved
without the correction. The ash correction on SO&lt;sub&gt;2&lt;/sub&gt; retrieval at 7.3 Î¼m
is much less important and only significant for low SO&lt;sub&gt;2&lt;/sub&gt; columnar abundances.
Results also show that the simplified and faster correction procedure
underestimates the ash correction compared with the more time consuming but
more accurate correction procedure.
Such underestimation is greater
for instruments having better ground pixel resolution, i.e. greater for MODIS
than for SEVIRI.</abstract>
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</article>

