Due to limitation in downlink, is expected to be perform rarely: 4-scan mosaic at the Jupiter closest approach 3-scan mosaics during Jupiter eclipses Latitudinal coverage 30°S-30°N range can be extended pole to pole with the MAJIS scanner for distances larger than 106 km; at smaller distances, S/C scans are required according to MAJIS_JUP_DISK_SLEW mode. 50 min (TBD) is the maximum time between the end of acquisition for the (n)-th MAJIS cube and the start of acquisition of (n+1)-th MAJIS cube to avoid gaps in longitudinal coverage SC scan (continuous slew) mode with a rate compatible with the 2 sec repetition time is possible; in this case, no scan activated which shall reduce the power to 35.73 W (Table 3 of technical budget report v2.1). Caveats: Turnaround and stabilization times after each swath