Spatial Distribution of Io's Extended UV Emissions

Details Spatial Distribution of Io's Extended UV Emissions Spatial Distribution of Io's Extended UV Emissions

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7582m&link_type=abstract

HST Proposal ID #7582

Physics

Hst Proposal Id #7582 Solar System

Scientific paper

Measurements of the spatial distribution of Io's sulfur and oxygen UV emissions will be obtained using STIS spectroscopic modes. This coordinated program uses 6 orbits of STIS GTO time, 3 orbits from PI W. Moos {program 7582} and 3 orbits from PI F. Roesler {prog. 7583}. During Visit 1, MAMA FUV spectroscopy will be performed when Io is near western elongation. Visit 2, also near west Io elongation, is devoted to emission line measurements to measure the spatial distribution of the atomic sulfur doublet SI 1900A/1915A and the atomic oxygen doublet OI 1356A/1359A. TIME-TAG mode is used for all observations to monitor the temporal variability of the emissions.

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