The motion of a white SPOT of Jupiter's south temperate belt

Details The motion of a white SPOT of Jupiter's south temperate belt The motion of a white SPOT of Jupiter's south temperate belt

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978avest..12..124z&link_type=abstract

(Astronomicheskii Vestnik, vol. 12, Apr.-June 1978, p. 124, 125.) Solar System Research, vol. 12, no. 2, Oct. 1978, p. 106, 107.

Astronomy and Astrophysics

Astronomy

Annual Variations, Jupiter Atmosphere, Oscillations, Temperate Regions, Jupiter Red Spot, Longitude, Periodic Variations, Southern Hemisphere

Scientific paper

Annual oscillations with an average period of 12.4 months have been discovered in the motion of a south temperate belt white spot (WS-III) from observations of Jupiter for 1969 through 1976 with the 30-cm Zeiss refractor of the Volgograd planetarium's observatory. A sequence has been noticed of two short periods, with one of them prolonged. The remaining two white spots do not experience noticeable periodic oscillations, and periodic oscillations of the Red Spot's longitude are barely evident.

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