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Radio Interferometry of Venus at Short Wavelengths

Published online by Cambridge University Press:  14 August 2015

Michael A. Janssen
Michael A. Janssen*
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, Calif., U.S.A.

Abstract

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From short wavelength (γ < 4 cm) interferometry of Venus interpreted on the basis of the physical structure and bulk composition of its atmosphere as given by spacecraft measurements, evidence for the presence of a source of opacity in addition to CO2 is found. This opacity presumably is due to unknown minor constituents of the atmosphere of Venus.

Type
Part II Terrestrial Planets
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 161 - 169
Copyright
Copyright © Reidel 1974 

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