Spatial & Temporal Variations in the UV Emission from the Atmosphere of Io

Details Spatial & Temporal Variations in the UV Emission from the Atmosphere of Io Spatial & Temporal Variations in the UV Emission from the Atmosphere of Io

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7583r&link_type=abstract

HST Proposal ID #7583

Physics

Hst Proposal Id #7583 Solar System

Scientific paper

Measurements of the spatial distribution of Io's hydrogen, sulfur and oxygen FUV emissions will be obtained using STIS spectroscopic and imaging modes. This coordinated program uses 10 orbits of STIS GTO time, 5 orbits from PI W. Moos {program 7582} and 5 orbits from PI F. Roesler {prog. 7583}. During Visit 1, MAMA FUV spectroscopy and imaging will be performed when Io is west of Jupiter. Visit 2 will perform MAMA FUV spectroscopy when Io is east of Jupiter. Visit 3 is devoted to emission line measurements of the spatial and velocity distribution of the atomic oxygen doublet OI 1356A/1359A and the atomic sulfur multiplet SI 1479A. TIME-TAG mode is used for all observations to monitor the temporal variability of the emissions.

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