Saturn's zonal wind profile in 2004-2009 from Cassini ISS images and its long-term variability

Details Saturn's zonal wind profile in 2004-2009 from Cassini ISS images and its long-term variability Saturn's zonal wind profile in 2004-2009 from Cassini ISS images and its long-term variability

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..215...62g&link_type=abstract

Icarus, Volume 215, Issue 1, p. 62-74.

Computer Science

Scientific paper

We retrieved Saturn's winds from ISS Cassini CB and MT images from 2004 to 2009. Differences between CB and MT zonal winds are due to vertical thermal wind shear. We supply tabular data of the ISS Cassini CB and MT Cassini wind profiles. Outside the equator zonal winds have remained stable during a complete Saturn's year. There is a major change in the equatorial winds possibly after the 1990 GWS event.

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