A comparison of red spots in the atmosphere of Jupiter

Details A comparison of red spots in the atmosphere of Jupiter A comparison of red spots in the atmosphere of Jupiter

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icar...67...96b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 67, July 1986, p. 96-105.

Astronomy and Astrophysics

Astronomy

19

Astronomical Photometry, Jupiter Atmosphere, Jupiter Red Spot, Zonal Flow (Meteorology), Anticyclones, Astronomical Photography, Latitude, Ultraviolet Absorption

Scientific paper

Voyager, Pioneer and ground-based astronomical and broadband photometric images of Jupiter are analyzed to compare the Great Red Spot (GRS) with the Little Red Spots (LRS) observed in the North Tropical Zone in 1976. Attention is given to the size and latitudinal positions and the color profiles. The red ovals are found to absorb strongly at blue and UV wavelengths, unlike red-brown belts. The movements of the GRS and the LRS coincided strongly with zonal wind profiles of the regions in which they are embedded. The meridional gradient of the zonal wind is the controlling factor in the lifetime of the red spots.

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