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SWI_SPECTRAL_SCAN_CTS_FS
SWI SPECTRAL SCAN CTS FS
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
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Advanced

this mode 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
TBD
conditions that make the observation not possible (e.g. thruster firing)
#update2021

Commanding