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    Microwave Brightness Temperatures from Tilted Convective Systems

    Source: Journal of Applied Meteorology:;2000:;volume( 039 ):;issue: 007::page 983
    Author:
    Hong, Ye
    ,
    Haferman, Jeffrey L.
    ,
    Olson, William S.
    ,
    Kummerow, Christian D.
    DOI: 10.1175/1520-0450(2000)039<0983:MBTFTC>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Aircraft and ground-based radar data from the Tropical Ocean and Global Atmosphere Coupled Ocean?Atmosphere Response Experiment show that convective systems are not always vertical. Instead, many are tilted from vertical. Satellite passive microwave radiometers observe the atmosphere at an oblique angle. For example, the Special Sensor Microwave Imager on Defense Meteorological Satellite Program satellites and the Tropical Rainfall Measurement Mission (TRMM) Microwave Imager (TMI) on the TRMM satellite view at an incident angle of about 50°. Thus, the brightness temperature measured from one direction of tilt may be different than that viewed from the opposite direction because of the different optical path. This paper presents an investigation of passive microwave brightness temperatures upwelling from tilted convective systems. To account for the effect of tilt, a 3D backward Monte Carlo radiative transfer model has been applied to a simple tilted cloud model and a dynamically evolving cloud model to derive the brightness temperature. The radiative transfer results indicate that brightness temperature varies when the viewing angle changes because of the different optical path. The tilt increases the displacements between the high 19-GHz brightness temperature (Tb19) due to liquid emission from the lower level of cloud and the low 85-GHz brightness temperature (Tb85) due to ice scattering from the upper level of cloud. As the resolution degrades, the difference of brightness temperature due to the change of viewing angle decrease dramatically. The displacement between Tb19 and Tb85, however, remains prominent. The successful launch and operation of the TRMM satellite provide an opportunity to examine tilted convective systems using collocated radar and radiometer data. TMI observations of tilted systems indicate that displacement between Tb19 and Tb85 can be as far as 100 km. Such displacement not only poses a problem to rainfall retrieval algorithms that use only scattering information but also causes large uncertainty in rainfall retrieval from multichannel retrieval algorithms. This study suggests that combined radar and radiometer data are needed to reduce the effect of tilt and to improve surface rainfall retrieval.
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      Microwave Brightness Temperatures from Tilted Convective Systems

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4148244
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    contributor authorHong, Ye
    contributor authorHaferman, Jeffrey L.
    contributor authorOlson, William S.
    contributor authorKummerow, Christian D.
    date accessioned2017-06-09T14:07:27Z
    date available2017-06-09T14:07:27Z
    date copyright2000/07/01
    date issued2000
    identifier issn0894-8763
    identifier otherams-12859.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4148244
    description abstractAircraft and ground-based radar data from the Tropical Ocean and Global Atmosphere Coupled Ocean?Atmosphere Response Experiment show that convective systems are not always vertical. Instead, many are tilted from vertical. Satellite passive microwave radiometers observe the atmosphere at an oblique angle. For example, the Special Sensor Microwave Imager on Defense Meteorological Satellite Program satellites and the Tropical Rainfall Measurement Mission (TRMM) Microwave Imager (TMI) on the TRMM satellite view at an incident angle of about 50°. Thus, the brightness temperature measured from one direction of tilt may be different than that viewed from the opposite direction because of the different optical path. This paper presents an investigation of passive microwave brightness temperatures upwelling from tilted convective systems. To account for the effect of tilt, a 3D backward Monte Carlo radiative transfer model has been applied to a simple tilted cloud model and a dynamically evolving cloud model to derive the brightness temperature. The radiative transfer results indicate that brightness temperature varies when the viewing angle changes because of the different optical path. The tilt increases the displacements between the high 19-GHz brightness temperature (Tb19) due to liquid emission from the lower level of cloud and the low 85-GHz brightness temperature (Tb85) due to ice scattering from the upper level of cloud. As the resolution degrades, the difference of brightness temperature due to the change of viewing angle decrease dramatically. The displacement between Tb19 and Tb85, however, remains prominent. The successful launch and operation of the TRMM satellite provide an opportunity to examine tilted convective systems using collocated radar and radiometer data. TMI observations of tilted systems indicate that displacement between Tb19 and Tb85 can be as far as 100 km. Such displacement not only poses a problem to rainfall retrieval algorithms that use only scattering information but also causes large uncertainty in rainfall retrieval from multichannel retrieval algorithms. This study suggests that combined radar and radiometer data are needed to reduce the effect of tilt and to improve surface rainfall retrieval.
    publisherAmerican Meteorological Society
    titleMicrowave Brightness Temperatures from Tilted Convective Systems
    typeJournal Paper
    journal volume39
    journal issue7
    journal titleJournal of Applied Meteorology
    identifier doi10.1175/1520-0450(2000)039<0983:MBTFTC>2.0.CO;2
    journal fristpage983
    journal lastpage998
    treeJournal of Applied Meteorology:;2000:;volume( 039 ):;issue: 007
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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