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UVS_JUP_AP_SCAN_MAP
UVS Jupiter AP Scan Map
Scan the UVS slit in the cross slit direction across a region (e.g., auroral (N or S)) or entire disk using the Airglow (AP) port, scan at a constant rate across Jupiter to produce a map. Observation performed in pixel list mode to reach a time resolution of 0.001 s.
UVS

Pointing

Slew
-

Advanced

- Specific cadence for a given period during the tour, to be constrained by 1 Gbit/week data downlink. - Distance to Jupiter R<20 Rj - 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