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Optical search for lightning on VenusElectrical signals attributed to lightning events on Venus have been observed by instruments aboard Veneras 11 and 12 and aboard the Pioneer Venus Orbiter. This paper reports the results of a search for optical pulses from the dark side of Venus made with the star sensor aboard the Pioneer Venus Orbiter. A comparison of both the frequency and amplitude distributions of received pulses with those of control experiments in which the star sensor observed deep space showed no statistically significant differences. Based on observations made during orbits 300 through 345, an upper limit of 30 flashes/sq km/yr has been derived for the average lightning frequency on the dark side of Venus. This value assumes that the amplitude distribution of lightning and the attenuation of the optical pulse by clouds on Venus are not substantially different from that occurring on earth.
Document ID
19810044076
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Borucki, W. J.
(NASA Ames Research Center Theoretical and Planetary Studies Branch, Moffett Field, Calif., United States)
Dyer, J. W.
(NASA Ames Research Center Pioneer Projects Office, Moffett Field, Calif., United States)
Thomas, G. Z.
(Hughes Aircraft Co. Los Angeles, Calif., United States)
Jordan, J. C.
(Informatics, Inc. Palo Alto, Calif., United States)
Comstock, D. A.
(De Anza College Cupertino, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
March 1, 1981
Publication Information
Publication: Geophysical Research Letters
Volume: 8
Subject Category
Lunar And Planetary Exploration
Accession Number
81A28480
Funding Number(s)
CONTRACT_GRANT: NAS2-8300
Distribution Limits
Public
Copyright
Other

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