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SWI_SPECTRAL_SCAN_CTS_PS
SWI SPECTRAL SCAN CTS PS
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 CTS spectra are recorded for 60 seconds over 10000 channels (16bit coding). Position-switch calibration method. A single execution can cover up to 13 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