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UVS_SAT_TRANSIT
UVS satellite transit observation
Measure absorption of Jupiter airglow by satellite atmospheres as they transit Jupiter's disk, to constrain satellite atmospheric composition and variability.
Pointing: nadir (Point slit N-S on Jupiter's disk and wait for moon to transit)
UVS

Pointing

track
Ring and satellites

Advanced

10 Europa transits and 10 Io transits during the tour. Dayside transits with the largest satellite angular diameter are highest priority
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
N/A
conditions that make the observation not possible (e.g. thruster firing)

Commanding