The rotation of the upper atmosphere of Venus

Details The rotation of the upper atmosphere of Venus The rotation of the upper atmosphere of Venus

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979crasb.289..107b&link_type=abstract

Academie des Sciences (Paris), Comptes Rendus, Serie B - Sciences Physiques, vol. 289, no. 5, Sept. 24, 1979, p. 107-110. In Fre

Physics

2

Rotating Environments, Upper Atmosphere, Venus Atmosphere, Histograms, Space Exploration

Scientific paper

Photographs and drawings of Venus made over a period of 85 years are analyzed in order to determine the rotation period of the ultraviolet markings observed. Examination of 204 documents made from 1893 to 1978 indicates that a synodic statistical retrograde rotation period of 4.02185 days leads to a flat longitudinal distribution of the forked markings, while one of 3.99525 days reveals a concentration of 70 percent of the markings in one hemisphere, in agreement with data obtained by Mariner 10. The precision of the determination is confirmed by a statistical analysis, and a previous estimate of 4.0285 days is attributed to the effects of averaging between the rotation speeds of the upper and lower portions of the Venus atmosphere.

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