Cloud-top meridional momentum transports on Saturn and Jupiter

Details Cloud-top meridional momentum transports on Saturn and Jupiter Cloud-top meridional momentum transports on Saturn and Jupiter

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986joat.conf..129s&link_type=abstract

In NASA. Goddard Inst. for Space Studies The Jovian Atmospheres p 129-143 (SEE N87-17598 09-91)

Other

Clouds (Meteorology), Jupiter Atmosphere, Meridional Flow, Momentum Transfer, Saturn Atmosphere, Wind Velocity, Equatorial Regions, Jet Streams (Meteorology), Kinetic Energy, Wind Profiles

Scientific paper

Cloud-tracked wind measurements reported by Sromovsky et al. were analyzed to determine meridional momentum transports in Saturn's northern middle latitudes. Results are expressed in terms of eastward and northward velocity components (u and v), and eddy components u and v. At most latitudes between 13 and 44 deg N (planetocentric), the transport by the mean flow () is measurably southward, tending to support Saturn's large equatorial jet, and completely dominating the eddy transport. Meridional velocities are near zero at the peak of the relatively weak westward jet; along the flanks of that jet, measurements indicate divergent flow out of the jet. In this region the dominant eddy transport () is northward on the north side of the jet, but not resolvable on the south side. Eddy transports at most other latitudes are not significantly different from measurement error. The conversion of eddy kinetic energy to mean kinetic energy, indicated by the correlation between and d/dy (where y is meridional distance) is clearly smaller than various values reported for Jupiter, and not significantly different from zero. Both Jovian and Saturnian results may be biased by the tendency for cloud tracking to favor high contrast features, and thus may not be entirely representative of the cloud level motions as a whole.