FLIP_ZAXIS | | GENERIC |
STELLAR_UVS_OCC_ET | | GENERIC |
RIME_RIDER_OBSERVATION | | RIME |
ECLIPSE_BATTERY_RECOVERY_STANDARD | Battery recharge after eclipse
pointing should be default power optimised pointing | GENERIC |
ECLIPSE_BATTERY_RECOVERY_FAST | Battery recharge after eclipse | GENERIC |
FB_BATTERY_RECOVERY_STANDARD | Segment to allow for battery recharge.
Attitude should be default power optimised. | GENERIC |
FB_BATTERY_RECOVERY_FAST | Segment to allow for battery recharge.
Pointing should be default power optimised | GENERIC |
JUPITER_CP | In situ Jupiter corotation breakdown region and plasma transport observation. Maximize the intervals for which co-rotation is measured to build spatial and temporal coverage of corotation profiles across the magnetosphere and also in the local moon environments.
CP stands for corotation profile | Working Group 3 |
RINGMOSAIC | RINGMOSAIC (Janus definition). impression of the extent of the whole ring
system | Working Group 2 |
RINGPHASE | | Working Group 2 |
RECOVERY | | GENERIC |
RINGSPIRAL_MP | RINGSPIRAL_MP (medium phase: JANUS Def) | Working Group 2 |
RINGSPIRAL_HP | RINGSPIRAL_HP (high phase, Janus def) | Working Group 2 |
SHADOWEDGE | rings SHADOWEDGE. Imaging of the ring region intersected by the planetary shadow at moderate
elevation and very high phase. Especially for the very faint gossamer rings and the Thebe
extension | Working Group 2 |
SOC_PRIME_OBSERVATION | Placeholder for SOC Prime Observation | SOC |
SOC_OBSERVATION | | SOC |
JUICE_PRIME_OBSERVATION | Placeholder for JUICE SOC Observations. | JUICE |
GALA_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | GALA |
GALA_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | GALA |
3GM_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | 3GM |
3GM_OBSERVATION | | 3GM |
RPWI_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | RPWI |
RPWI_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | RPWI |
JMAG_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | JMAG |
JMAG_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | JMAG |
SWI_PRIME_OBSERVATION | | SWI |
SWI_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | SWI |
RIME_PRIME_OBSERVATION | | RIME |
PEP_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | PEPLO |
PEP_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | PEPLO |
UVS_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | UVS |
UVS_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | UVS |
NAVCAM_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | NAVCAM |
NAVCAM_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | NAVCAM |
RADEM_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | RADEM |
RECOVERY_FLYBY | 15.15 hours recovery segments to be scheduled after flybys/eclipse, when standard instrument mode is assumed
Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+Analysis
Pointing should be power optimized | GENERIC |
BATTERY_RECHARGE | 20.5 hour recovery segments to be scheduled after very demanding periods. For the moment only after flybys and eclipses.
Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+Analysis | GENERIC |
ECLIPSE | SUN OCCULTATION BY JUPITER CONVERTED INTO ECLIPSE SEGMENTS | GENERIC |
IO_MAJ_HOTSPOTS | IO_MAJ_HOTSPOTS | Working Group 2 |
IO_MAJ_COMPOSITION | IO_MAJ_COMPOSITION | Working Group 2 |
MAJIS_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | MAJIS |
MAJIS_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | MAJIS |
JANUS_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | JANUS |
JANUS_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | JANUS |
ASTRO_IRR1_MEGACLITE | ASTRO_IRR1_MEGACLITE | Working Group 2 |
RINGMATTER | RINGMATTER. Observations of the main rings and the gossamer rings, imaging the ring ansae from moderately large elevation.
The moderatly large elevation will reveal azimuthal structure in the rings and the presence of clumps at the resolution limit of the imaging. | Working Group 2 |
STAR_OCC_OBS | STAR_OCC_OBS | Working Group 4 |
E_IS_OBS | E_IS_OBS | Working Group 3 |
C_IS_OBS | C_IS_OBS | Working Group 3 |
G_IS_OBS | G_IS_OBS | Working Group 3 |
J_SAT_OBS | J_SAT_OBS | Working Group 2 |
ECLIPSE_JUPITER_THERMAL | ECLIPSE_JUPITER_THERMAL | GENERIC |
FB_THERMAL | FB_THERMAL | GENERIC |
DEFAULT_THERMAL | DEFAULT_THERMAL | GENERIC |
J_SAT_515_Adr | J_SAT_515_Adr | Working Group 2 |
J_SAT_514_The | J_SAT_514_The | Working Group 2 |
J_SAT_505_Ama | J_SAT_505_Ama | Working Group 2 |
J_SAT_IRR_SEARCH | J_SAT_IRR_SEARCH
discover new irregular moons | Working Group 2 |
J_SAT_520_Tay | J_SAT_520_Tay | Working Group 2 |
J_SAT_559_17J1 | J_SAT_559_17J1 | Working Group 2 |
J_SAT_55503_3J9 | J_SAT_55503_3J9 | Working Group 2 |
J_SAT_548_Cyl | J_SAT_548_Cyl | Working Group 2 |
J_SAT_566_17J5 | J_SAT_566_17J5 | Working Group 2 |
J_SAT_556_11J2 | J_SAT_556_11J2 | Working Group 2 |
J_SAT_568_17J7 | J_SAT_568_17J7 | Working Group 2 |
J_SAT_569_17J8 | J_SAT_569_17J8 | Working Group 2 |
J_SAT_562_Val | J_SAT_562_Val | Working Group 2 |
J_SAT_567_17J6 | J_SAT_567_17J6 | Working Group 2 |
J_SAT_564_17J3 | J_SAT_564_17J3 | Working Group 2 |
J_SAT_543_Arc | J_SAT_543_Arc | Working Group 2 |
J_SAT_537_Kle | J_SAT_537_Kle | Working Group 2 |
J_SAT_538_Pst | J_SAT_538_Pst | Working Group 2 |
J_SAT_554_16J1 | J_SAT_554_16J1 | Working Group 2 |
J_SAT_542_Tlx | J_SAT_542_Tlx | Working Group 2 |
J_SAT_541_Aoe | J_SAT_541_Aoe | Working Group 2 |
J_SAT_522_Har | J_SAT_522_Har | Working Group 2 |
J_SAT_561_3J19 | J_SAT_561_3J19 | Working Group 2 |
J_SAT_540_Mne | J_SAT_540_Mne | Working Group 2 |
J_SAT_557_Eir | J_SAT_557_Eir | Working Group 2 |
J_SAT_547_Euk | J_SAT_547_Euk | Working Group 2 |
J_SAT_530_Her | J_SAT_530_Her | Working Group 2 |
J_SAT_532_Eyd | J_SAT_532_Eyd | Working Group 2 |
J_SAT_523_Klk | J_SAT_523_Klk | Working Group 2 |
J_SAT_572_11J1 | J_SAT_572_11J1 | Working Group 2 |
J_SAT_55506_3J16 | J_SAT_55506_3J16 | Working Group 2 |
J_SAT_552_10J2 | J_SAT_552_10J2 | Working Group 2 |
J_SAT_525_Eri | J_SAT_525_Eri | Working Group 2 |
J_SAT_533_Eua | J_SAT_533_Eua | Working Group 2 |
J_SAT_536_Spo | J_SAT_536_Spo | Working Group 2 |
J_SAT_528_Aut | J_SAT_528_Aut | Working Group 2 |
J_SAT_527_Pra | J_SAT_527_Pra | Working Group 2 |
J_SAT_529_Thy | J_SAT_529_Thy | Working Group 2 |
J_SAT_555_3J18 | J_SAT_555_3J18 | Working Group 2 |
J_SAT_519_Meg | J_SAT_519_Meg | Working Group 2 |
J_SAT_55504_3J10 | J_SAT_55504_3J10 | Working Group 2 |
J_SAT_539_Heg | J_SAT_539_Heg | Working Group 2 |
J_SAT_517_Clh | J_SAT_517_Clh | Working Group 2 |
J_SAT_55505_3J12 | J_SAT_55505_3J12 | Working Group 2 |
J_SAT_546_Crp | J_SAT_546_Crp | Working Group 2 |
J_SAT_551_10J1 | J_SAT_551_10J1 | Working Group 2 |