The 4-day rotation of the upper atmosphere of venus

Details The 4-day rotation of the upper atmosphere of venus The 4-day rotation of the upper atmosphere of venus

Sep 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21.1559b&link_type=abstract

Planetary and Space Science, Volume 21, Issue 9, p. 1559-1561.

Physics

6

Scientific paper

Near u.v. photographs of Venus have been analysed. Evidence is presented that so-called Y- and ψ-shaped markings accelerate from local sunrise to some time during local afternoon; mean horizontal velocities are 83 msec-1 (morning) and 122 msec-1 (afternoon). Possibly these configurations are more stable than a normal cloud system. `Irregular' features do not seem to share this acceleration; they circulate at higher altitudes, sometimes covering or distorting the stable configurations.

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