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contributor authorWelch, Ronald M.
contributor authorWielicki, Bruce A.
date accessioned2017-06-09T14:28:56Z
date available2017-06-09T14:28:56Z
date copyright1989/05/01
date issued1988
identifier issn0022-4928
identifier otherams-20072.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156260
description abstractReflected fluxes are calculated for broken cloudiness (i.e., nonplane parallel) as a function of cloud cover, cloud optical depth, solar zenith angle and surface albedo. These calculations extend previous results for broken cloud reflected fluxes over a black surface. The present study demonstrates that not only radiances but also radiative fluxes over high albedo surfaces may be decreased by the presence of broken cloudiness. Conventional wisdom states that cloud radiances(brightnesses) are always greater than the background. While most cloud retrieval schemes are built around this assumption, it is incorrect for clouds over high albedo surfaces such as found in polar regions. However, the most startling and counterintuitive conclusion of this study is that nonabsorbing finite clouds over a highly reflecting surface will decrease the system albedo. As a result, surface absorption is increased, the result of multiple scattering between surface and cloud layer, controlled by cloud morphology and cloud optical thickness. A simple parameterization of the effects of cloud contamination upon retrieved albedo is given in terms of solar zenith angle, cloud optical depth, surface albedo, cloud cover, and plane-parallel could albedo. In this way, the effects of broken cloudiness are modeled in terms of easily computed plane-parallel values.
publisherAmerican Meteorological Society
titleReflected Fluxes for Broken Clouds over a Lambertian Surface
typeJournal Paper
journal volume46
journal issue10
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1989)046<1384:RFFBCO>2.0.CO;2
journal fristpage1384
journal lastpage1395
treeJournal of the Atmospheric Sciences:;1988:;Volume( 046 ):;issue: 010
contenttypeFulltext


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