A model for the dependence of MSU brightness temperature on lapse rate
An analytical model is developed for microwave sounding unit (MSU) channel 2 radiance that is both simple and accurate. The basis of the model is a parameterization of the pressure and temperature dependence of the absorption coefficient of oxygen in the 60 GHz band. The parameterization allows a cl...
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Veröffentlicht in: | Journal of quantitative spectroscopy & radiative transfer 2001-04, Vol.69 (2), p.159-170 |
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container_title | Journal of quantitative spectroscopy & radiative transfer |
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creator | O'Brien, D.M. |
description | An analytical model is developed for microwave sounding unit (MSU) channel 2 radiance that is both simple and accurate. The basis of the model is a parameterization of the pressure and temperature dependence of the absorption coefficient of oxygen in the 60 GHz band. The parameterization allows a closed expression to be derived for the brightness temperature at the top of an atmosphere consisting of layers within each of which the lapse rate is constant. The model may be inverted to derive the lapse rate of the troposphere in terms of the MSU brightness temperature and surface temperature and, therefore, provides a framework within which the two temperature records may be interpreted. |
doi_str_mv | 10.1016/S0022-4073(00)00074-1 |
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The basis of the model is a parameterization of the pressure and temperature dependence of the absorption coefficient of oxygen in the 60 GHz band. The parameterization allows a closed expression to be derived for the brightness temperature at the top of an atmosphere consisting of layers within each of which the lapse rate is constant. 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The model may be inverted to derive the lapse rate of the troposphere in terms of the MSU brightness temperature and surface temperature and, therefore, provides a framework within which the two temperature records may be interpreted.</description><subject>Brightness temperature</subject><subject>Lapse rate</subject><subject>MSU</subject><issn>0022-4073</issn><issn>1879-1352</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LxDAQhoMoWFd_gpCT6KE6ado0PcmyuCqseFj3HNJk4lb6ZdIV_Pe2u-LV0zDM874wDyGXDG4ZMHG3BkiSOIWcXwPcAECexuyIREzmRcx4lhyT6A85JWchfIwQ50xEZDmnTWexpq7zdNgitdhja7E1SDtHX9YbWvrqfTu0GAIdsOnR62Hnx2tLa90HpOOO5-TE6Trgxe-ckc3y4W3xFK9eH58X81VsOJdDXJhUa-mEEKnlwroEciazXKdaygQc6MQIbsvCGinzTJaltUxqlzsUiAUYPiNXh97ed587DINqqmCwrnWL3S4oJnkqEsFGMDuAxncheHSq91Wj_bdioCZram9NTUoUgNpbU1Pu_pDD8YuvCr0Kppps2MqjGZTtqn8afgAsI3Ou</recordid><startdate>20010415</startdate><enddate>20010415</enddate><creator>O'Brien, D.M.</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20010415</creationdate><title>A model for the dependence of MSU brightness temperature on lapse rate</title><author>O'Brien, D.M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c338t-9c4aa8f6664d36df2071857a4a8820f0a2c63db9dc88758bbdd18af7fe6ee90c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>Brightness temperature</topic><topic>Lapse rate</topic><topic>MSU</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>O'Brien, D.M.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Journal of quantitative spectroscopy & radiative transfer</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>O'Brien, D.M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A model for the dependence of MSU brightness temperature on lapse rate</atitle><jtitle>Journal of quantitative spectroscopy & radiative transfer</jtitle><date>2001-04-15</date><risdate>2001</risdate><volume>69</volume><issue>2</issue><spage>159</spage><epage>170</epage><pages>159-170</pages><issn>0022-4073</issn><eissn>1879-1352</eissn><abstract>An analytical model is developed for microwave sounding unit (MSU) channel 2 radiance that is both simple and accurate. The basis of the model is a parameterization of the pressure and temperature dependence of the absorption coefficient of oxygen in the 60 GHz band. The parameterization allows a closed expression to be derived for the brightness temperature at the top of an atmosphere consisting of layers within each of which the lapse rate is constant. The model may be inverted to derive the lapse rate of the troposphere in terms of the MSU brightness temperature and surface temperature and, therefore, provides a framework within which the two temperature records may be interpreted.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/S0022-4073(00)00074-1</doi><tpages>12</tpages></addata></record> |
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subjects | Brightness temperature Lapse rate MSU |
title | A model for the dependence of MSU brightness temperature on lapse rate |
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