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MAJ_JUP_RING
Radial (and azimuthal) structure of the main rings region (low elevation (~<0.5deg) at a given phase angle
Observations of the main rings (2 ansa) at a given phase (backscattering to forward scattering light), no tracking of azimuthal structure, no spatial binning to increase spatial resolution
MAJIS

Pointing

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Advanced

Low elevation (~<2°), near 0° highly preferred, eclipse, 2 ansa
Acquisition at far distance (>8.105 km at closest approach) to mitigate the spikes issue (<1 e- impacts/s) constraining the resolution (IFOV>=120 km before binning)
100 kHz readout mode (lowest RON < 30 e-)
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)
Source: JUI-IAS-MAJ-TN-104. Update 23/12/2025.

Commanding