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SWI_NADIR_STARE_PS
SWI NADIR STARE PS
Investigation of the atmospheric composition (and temperature) of Jupiter
and the Galilean moons. 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 (16 bits coding). Position-switch calibration method.
SWI

Pointing

nadir
Jupiter atmosphere

Advanced

can be used from any JUICE-Jupiter distance, but preferentially
from large distances, i.e. when the target size is <1   the FWHM. Repetition:  once per
day for Galilean moons from large distances. For Jupiter, SWI JUP LIMB STARE is usually
preferred.
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