Integrated Dynamical and Spectroscopic Observations of Jupiter and Sat Urn

Details Integrated Dynamical and Spectroscopic Observations of Jupiter and Sat Urn Integrated Dynamical and Spectroscopic Observations of Jupiter and Sat Urn

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3887b&link_type=abstract

HST Proposal ID #3887

Computer Science

Hst Proposal Id #3887

Scientific paper

An integrated set of multispectral images and ultraviolet spectra provides the basis for comparative analysis of the atmospheres of Jupiter and Saturn. The spatial resolution and the spectral range of the Hubble Space Telescope, combined with the ability to continue similar observations for at least 17 years, assure that these data will contribute to a valuable database for interpreting the high resolution data from Voyager, Galileo and Cassini. The basic problems that are addressed with these data are: temporal variations of the ammonia clouds, characterization of convection in the upper tropospheres, meridional stratospheric circulation, variation in the troposphere-stratosphere dynamic coupling and seasonal variability.

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