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SWI_SPECTRAL_SCAN_CTS_FS_V1
SWI SPECTRAL SCAN CTS FS V1
Same as SWI SPECTRAL SCAN CTS PS, except a frequency-switch calibration
mode is used instead of position-switch. It enables spending  100% of the integration
time on-source. If the purity of the spectral band is good enough, there is an option to precompute
ON-OFF for the CTS before downlink. A single execution can cover up to 9 tunings.
SWI

Pointing

nadir
-

Advanced

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