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UVS_DISK_SCAN
UVS_DISK_SCAN
Construct spectral image cubes of multiple atmospheric emission line features (up to 1024 selectable spectral bins with a minimum of 3 key emissions: H Lya, OI 130.4 nm, OI 135.6 nm), with repeated scans to investigate highly time-variable auroral dynamics.
UVS

Pointing

Slew
-

Advanced

8 per flyby - 4 before and 4 after c/a. Scans should be approximately evenly spaced in either time or distance from closest approach
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
TBW
conditions that make the observation not possible (e.g. thruster firing)
#update2021-11-25

Commanding