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SWI_MOON_LIMB_STARE_PS_V1
SWI MOON LIMB STARE PS V1
Investigation of Galilean Moons’ atmospheric composition, temperature,
and winds). Flyby: Two CTS spectra are recorded for 30 sec over 210 channels (16 bits coding).
GCO: Two CTS spectra are recorded for 30 sec over 130 channels (16 bits coding) and a different
altitude (5, 10, 20, 40, and 50 km) is scanned every orbit. Position-switch calibration method.
SWI

Pointing

nadir
-

Advanced

This mode will be used during phases I and III of the flybys,
between -4.5hrs and -3hrs and between +4.5hrs to +6hrs from CA. During the whole GCO-
500 phase, this mode will be used continuously for 5 orbits (i.e. 16-hrs) and then cycled equally
with SWI MOON LIMB SCAN PS, SWI MOON NADIR STARE PS, and SWI 2D MAP PS.
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
TBD
conditions that make the observation not possible (e.g. thruster firing)
#update2024Oct02

Commanding