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Variations in Venus Cloud Particle Properties

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dc.contributor.author Carlson, R. W. en_US
dc.contributor.author Kamp, L. W. en_US
dc.contributor.author Baines, K. H. en_US
dc.contributor.author Pollack, J. B. en_US
dc.contributor.author Grinspoon, G. H. en_US
dc.contributor.author Encrenaz, T. en_US
dc.contributor.author Drossart, P. en_US
dc.contributor.author Taylor, F. W. en_US
dc.date.accessioned 2004-10-06T04:43:48Z
dc.date.available 2004-10-06T04:43:48Z
dc.date.issued 1993 en_US
dc.identifier.citation n/a en_US
dc.identifier.clearanceno 93-1460 en_US
dc.identifier.uri http://hdl.handle.net/2014/35734
dc.description.abstract Using Venus nightside data obtained by the Galileo Near Infrared Mapping spectrometer, we hav studied the correclation of 1.74 and 2.30 <sub>m</sub> radiation which is transmitted through the clouds. en_US
dc.format.extent 432389 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other clouds radiative transfer calculations Venus large particles photochemical processes en_US
dc.title Variations in Venus Cloud Particle Properties en_US


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