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SWI_SPECTRAL_SCAN_ACS_PS_V1
SWI SPECTRAL SCAN ACS PS V1
Investigation of the atmospheric composition of Jupiter and the Galilean
moons. The whole frequency range available to SWI is scanned. This mode is nominally meant
for deep integrations and requires numerous repetitions (e.g. monitoring of the moons). Two
ACS spectra are recorded for 60 seconds over 1024 channels. Position-switch calibration method.
A single execution can cover up to 16 tunings.
SWI

Pointing

nadir
-

Advanced

Scheduling: can be used from any JUICE-Jupiter distance, and from
anywhere for Galilean moons. Repetition: One full spectral scan for Jupiter in the equatorial
phase and another one in the high inclination phase (SWI LIMB SPECTRAL SCAN preferred),
one full spectral scan for all Galilean moons.
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