View observation definition

SWI_5POINT_CROSS_PS
SWI 5POINT CROSS PS
Investigation of the Jovian and Galilean moon atmospheric composition, and Galilean surface properties by means of rough raster mapping. The stepsize is such that the opposite ends of the cross are separated by the size of the target in the given direction. For Jupiter, two CTS spectra are recorded every 60 seconds over 10000 channels (16 bits coding). For moon monitoring, two CTS spectra are recorded every 30 seconds over 210 channels (16 bits coding). For both cases, and in parallel, two CCH measurements (20 bits coding) are recorded every 0.1 second. Position-switch calibration method.
SWI

Pointing

nadir
-

Advanced

This mode is particularly meant for daily monitoring the moons during the Jupiter Tour. It can also be used for rough mapping of Jupiter and calibration purposes from long distances. Expected to be used when the target angular size is 1 to 2 x the FWHM.
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