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Geological Interpretations of the Topography of Selected Regions of Venus from Arecibo to Goldstone Radar InterferometryRadar interferometry using Arecibo to transmit and three antennas at the Goldstone to receive was conducted on 14 dates in Spring, 2001. This data has been used so far to generate DEMs (digital elevation models) for several of the dates with pixel resolution of 0.5-1.0 km. Additional information is contained in the original extended abstract.
Document ID
20020045965
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Jurgens, R. F. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Margot, J-L. (California Inst. of Tech. Pasadena, CA United States)
Simons, M. (California Inst. of Tech. Pasadena, CA United States)
Pritchard, M. E. (California Inst. of Tech. Pasadena, CA United States)
Slade, M. A. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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