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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>2</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/acpd-2-1403-2002</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/2/1403/2002/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/2/1403/2002/acpd-2-1403-2002.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/2/1403/2002/acpd-2-1403-2002.pdf</fulltext_pdf>
	<start_page>1403</start_page>
	<end_page>1427</end_page>
	<publication_date>2002-09-19</publication_date>
	<article_title content_type="html">The potential of polarization measurements from space at mm and sub-mm wavelengths for determining cirrus cloud parameters</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. Miao</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>K.-P. Johnsen</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>S. Buehler</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>A. Kokhanovsky</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Environmental Physics, University of Bremen, Germany</affiliation>
		<affiliation numeration="2" content_type="html">GKSS Research Center Geesthacht GmbH, Geesthacht, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The millimeter and sub-millimeter waves have been attracting
      a lot of attention recently in the cloud remote sensing community. This is largely because of its potential use in measuring cirrus cloud
      parameters with airborne or space-borne radiometers. In this study, we examine the possibility of using polarization measurements in this
      frequency range to retrieve microphysical parameters of cloud ice particles. By using a simple radiative transfer model, the polarization
      differences of the brightness temperatures measured at the vertical and horizontal polarization channels are calculated at the following seven frequencies:
      90, 157, 220, 340, 463, 683, and 874 GHz. The cirrus clouds are modeled with nearly spherical particles, circular cylinder, and circular plate,
      as well as with mixtures of these types. We found that the polarization difference shows a unique ``resonance&apos;&apos; feature with the change of ice
      particle characteristic size: it has a strong response only in a certain range of ice particle size, beyond that range it approaches zero.
      The size range where this resonance happens depends to a large extent on particle
      shape and aspect ratio, but to a much less extent on particle orientation.
      This resonance feature remains even when the particles are mixed with different shapes, although the magnitude and the position of the resonance
      peak may change, depending on how ice particles are mixed. Oriented particles generally show larger polarization
      difference than randomly oriented ones, and plates have larger polarization difference than cylinders. However, particle
      orientations have a significantly stronger influence on the polarization difference than particle shapes (cylinder or plate). This makes it
      difficult to distinguish particle shapes using millimeter and sub-millimeter radiometric measurements, if there is no information available
      on particle orientations. However, if the state of particle shape mixture can be predetermined by other approaches,
      polarization measurements can help to determine ice particle characteristic
      size and orientation. This information, in turn, will benefit the retrieval of cloud ice water path.</abstract>
	<references>
	</references>
</article>

