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UVS_SAT_DISK_SCAN_HP
UVS satellite HP 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
Ring and satellites

Advanced

Occasionally replaces UVS_SAT_DISK_SCAN_AP when illumination is good, to achieve improved spatial resolution
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