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UVS_JUP_HP_FEATURE_SCAN
UVS Jupiter HP Feature Scan
To assess the evolution of discrete phenomena (e.g., H Ly-alpha bulge, plumes, auroral features,…) using the HP port and pixellist mode.
UVS

Pointing

nadir
Jupiter atmosphere

Advanced

Specific cadence for a given period during the tour, to be constrained by 1 Gbit/week data downlink. - Synergistic observations with MAJIS and JANUS. Note: Integration time is ¼ of Jupiter’s rotation period and the total data volume is thus 42 Mbits (8 spectral bins, 512 spatial bins, 16 bit value, and 0.001s time 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