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 |