Excitation Processes for the Outer Planet UV Emissions: Future-Cycle Continuation

Details Excitation Processes for the Outer Planet UV Emissions: Future-Cycle Continuation Excitation Processes for the Outer Planet UV Emissions: Future-Cycle Continuation

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3618m&link_type=abstract

HST Proposal ID #3618

Physics

Hst Proposal Id #3618

Scientific paper

A set of observations of Jupiter (Cycle 1) and Saturn (Cycle2) in the far-ultraviolet spectral region will be used to determine the process(es) exciting UV ('electroglow') emissions in the upper atmospheres of these planets. Utilizing the increased sensitivity and spectral resolution of the ST/FOS over IUE and Voyager systems, emission lines from 1200-1800A will be used to distinguish between the two suggested processes of electron excitation and fluorescence.

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