Longitudinal Variation and Waves in Jupiter's South Equatorial Wind Jet

Details Longitudinal Variation and Waves in Jupiter's South Equatorial Wind Jet Longitudinal Variation and Waves in Jupiter's South Equatorial Wind Jet

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1104s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1104

Physics

Scientific paper

Jupiter's south equatorial winds and clouds are consistent with a high
frequency, gravity-inertia, wave. A second, westward-moving, Rossby wave
was also identified. Asymmetry with the north equatorial clouds are
likely due to the Great Red Spot.

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