ECLIPSE_BATTERY_RECOVERY_FAST | Battery recharge after eclipse | GENERIC |
ECLIPSE_BATTERY_RECOVERY_STANDARD | Battery recharge after eclipse
pointing should be default power optimised pointing | GENERIC |
ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
ASTRO_IRR1_THEMISTO | Astrometry irregular moon THEMISTO | Working Group 2 |
ASTRO_IRR1_TAYGETE | Astrometry irregular moon TAYGETE | Working Group 2 |
ASTRO_IRR1_LYSITHEA | Astrometry irregular moon LYSITHEA | Working Group 2 |
ASTRO_IRR1_LEDA | Astrometry irregular moon LEDA | Working Group 2 |
ASTRO_IRR1_KALLICHORE | Astrometry irregular moon KALLICHORE | Working Group 2 |
ASTRO_IRR1_HIMALIA | Astrometry irregular moon HIMALIA | Working Group 2 |
ASTRO_IRR1_CHALDENE | Astrometry irregular moon CHALDENE | Working Group 2 |
ASTRO_IRR1_CARPO | Astrometry irregular moon CARPO | Working Group 2 |
ASTRO_IRR2_CARME | Astrometry irregular moon Carme | Working Group 2 |
ASTRO_IRR2_ANANKE | Astrometry irregular moon Ananke | Working Group 2 |
ASTRO_INNER | Astrometry inner moons | Working Group 2 |
ASTRO_IRR1_MEGACLITE | ASTRO_IRR1_MEGACLITE | Working Group 2 |
DL_EXT | assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018) | GENERIC |
JMAG_CALROLL | 5 calibration roll needed by JMAG. 2 as soon as possible after JOI. 3 during phase 5: one at the start of phase 5, the last 2 as late as possible before GOI | WGX |
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 |
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 |
IO_MONITORING | - JANUS minimum distance = 7.00e+05 km
- MAJIS minimum distance = 8.00e+05 km
- SWI minimum distance = 6.00e+05 km (able to resolve target when angular size is > 1 mrad)
| Working Group 2 |
PEPLO_DESIGNER_OBSERVATION | | PEPLO |
PEPHI_DESIGNER_OBSERVATION | | PEPHI |
PEPHI_OBSERVATION | | PEPHI |
PEPHI_PRIME_OBSERVATION | | PEPHI |
FLIP_ZAXIS | | GENERIC |
SOC_DESIGNER_OBSERVATION | | SOC |
NAVCAM_DESIGNER_OBSERVATION | | NAVCAM |
RADEM_DESIGNER_OBSERVATION | | RADEM |
GALA_DESIGNER_OBSERVATION | | GALA |
JMAG_DESIGNER_OBSERVATION | | JMAG |
SWI_DESIGNER_OBSERVATION | | SWI |
JANUS_DESIGNER_OBSERVATION | | JANUS |
RIME_DESIGNER_OBSERVATION | | RIME |
STELLAR_UVS_OCC_ET | | GENERIC |
RIME_RIDER_OBSERVATION | | RIME |
SWI_RIDER_OBSERVATION | | SWI |
RINGPHASE | | Working Group 2 |
RECOVERY | | GENERIC |
SOC_OBSERVATION | | SOC |
3GM_OBSERVATION | | 3GM |
SWI_PRIME_OBSERVATION | | SWI |
RIME_PRIME_OBSERVATION | | RIME |
J_SAT_THYONE | | Working Group 2 |
J_SAT_S2017_J9 | | Working Group 2 |
J_SAT_S2017_J7 | | Working Group 2 |
J_SAT_S2017_J6 | | Working Group 2 |
J_SAT_S2017_J5 | | Working Group 2 |
J_SAT_S2017_J3 | | Working Group 2 |
J_SAT_S2017_J2 | | Working Group 2 |
J_SAT_S2016_J1 | | Working Group 2 |
J_SAT_S2011_J2 | | Working Group 2 |
J_SAT_S2010_J2 | | Working Group 2 |
J_SAT_S2010_J1 | | Working Group 2 |
J_SAT_S2003_J9 | | Working Group 2 |
J_SAT_S2003_J4 | | Working Group 2 |
J_SAT_S2003_J19 | | Working Group 2 |
J_SAT_S2003_J16 | | Working Group 2 |
J_SAT_S2003_J12 | | Working Group 2 |
J_SAT_S2003_J10 | | Working Group 2 |
J_SAT_PHILOPHROSYNE | | Working Group 2 |
J_SAT_ORTHOSIE | | Working Group 2 |
J_SAT_MNEME | | Working Group 2 |
J_SAT_KALYKE | | Working Group 2 |
J_SAT_KALE | | Working Group 2 |
J_SAT_EUPORIE | | Working Group 2 |
J_SAT_EUPHEME | | Working Group 2 |
J_SAT_EUKELADE | | Working Group 2 |
J_SAT_EUANTHE | | Working Group 2 |
J_SAT_EIRENE | | Working Group 2 |
J_SAT_DIA | | Working Group 2 |
J_SAT_CARPO | | Working Group 2 |
J_SAT_AITNE | | Working Group 2 |
J_SAT_VALETUDO | | Working Group 2 |
J_SAT_THEMISTO | | Working Group 2 |
J_SAT_TAYGETE | | Working Group 2 |
J_SAT_SINOPE | | Working Group 2 |
J_SAT_PRAXIDIKE | | Working Group 2 |
J_SAT_PASITHEE | | Working Group 2 |
J_SAT_PASIPHAE | | Working Group 2 |
J_SAT_PANDIA | | Working Group 2 |
J_SAT_MEGACLITE | | Working Group 2 |
J_SAT_LYSITHEA | | Working Group 2 |
J_SAT_LEDA | | Working Group 2 |
J_SAT_KALLICHORE | | Working Group 2 |
J_SAT_ISONOE | | Working Group 2 |
J_SAT_IOCASTE | | Working Group 2 |
J_SAT_HIMALIA | | Working Group 2 |
J_SAT_HERSE | | Working Group 2 |
J_SAT_HERMIPPE | | Working Group 2 |
J_SAT_HELIKE | | Working Group 2 |
J_SAT_HEGEMONE | | Working Group 2 |
J_SAT_HARPALYKE | | Working Group 2 |
J_SAT_ERSA | | Working Group 2 |
J_SAT_ERINOME | | Working Group 2 |
J_SAT_ELARA | | Working Group 2 |
J_SAT_CHALDENE | | Working Group 2 |
J_SAT_CARME | | Working Group 2 |
J_SAT_CALLIRRHOE | | Working Group 2 |
J_SAT_AUTONOE | | Working Group 2 |
J_SAT_ARCHE | | Working Group 2 |