Excitation Processes for the Outer Planet UV Emissions: Cycle 1 Observations

Details Excitation Processes for the Outer Planet UV Emissions: Cycle 1 Observations Excitation Processes for the Outer Planet UV Emissions: Cycle 1 Observations

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.2625m&link_type=abstract

HST Proposal ID #2625

Physics

Hst Proposal Id #2625

Scientific paper

A set of observations of Jupiter in the far-ultraviolet spectral region will be used to determine the process(es) exciting UV ('electroglow') emissions in the upper atmosphere. Utilizing the increased sensitivity and spectral resolution of the ST/HRS over IUE and Voyager systems, emission lines in two 35A bandpasses centered at 1254A and 1594A will be used to distinguishbetween the suggested processes of electron excitation and fluorescence.

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