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contributor authorPrabhakara, C.
contributor authorYoo, Jung-Moon
contributor authorDalu, Giuseppe
contributor authorFraser, R. S.
date accessioned2017-06-09T14:03:21Z
date available2017-06-09T14:03:21Z
date copyright1990/12/01
date issued1990
identifier issn0894-8763
identifier otherams-11633.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4146883
description abstractThe spectral data obtained by the Infrared Interferometer Spectrometer (IRIS) flown on Nimbus 4 satellite in 1970 indicated the existence of optically thin ice clouds in the upper troposphere that probably extended into lower stratosphere, in the polar regions, during winter and early spring. The spectral features of these clouds differ somewhat from that of the optically thin cirrus clouds in the tropics. From theoretical simulation of the infrared spectra in the 8?25 ?m region, we infer that these polar clouds have a vertical stratification in particle size, with larger particles (?12 ?m) in the bottom of the cloud and smaller ones (?1 ?m) aloft. Radiative transfer calculations also suggest that the equivalent ice-water content of these polar clouds is of the order of 1 mg cm?2.
publisherAmerican Meteorological Society
titleDeep Optically Thin Cirrus Clouds in the Polar Regions. Part I: Infrared Extinction Characteristics
typeJournal Paper
journal volume29
journal issue12
journal titleJournal of Applied Meteorology
identifier doi10.1175/1520-0450(1990)029<1313:DOTCCI>2.0.CO;2
journal fristpage1313
journal lastpage1329
treeJournal of Applied Meteorology:;1990:;volume( 029 ):;issue: 012
contenttypeFulltext


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