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UVS_IO_TORUS_SCAN
UVS IO_TORUS_SCAN
Map emissions from the Io torus. Slit aligned parallel with Jupiter's rotation pole, scanned E-W across the torus
UVS

Pointing

Slew
Plasma

Advanced

- At least once per day during the tour, to be constrained by 1 Gbit/week data downlink. - Observations including when distance to Jupiter R>20 Rj - To assess temporal evolution requires repetitive observations, including over short periods to look for changes over short timescales. - Synergistic observations with MAJIS and JANUS
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