| 3GM_DESIGNER_OBSERVATION | | 3GM |
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| 3GM_OBSERVATION | | 3GM |
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| 3GM_PRIME_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | 3GM |
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| 3GM_RIDER_OBSERVATION | Placeholder Segment to accomodate the detailed scenario observation plan generation process. | 3GM |
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| 508_Pas | Test opportunity segment Pasiphae | Working Group 2 |
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| ASTRO_INNER | Astrometry inner moons | Working Group 2 |
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| ASTRO_IRR_ELARA | | Working Group 2 |
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| ASTRO_IRR1_CARPO | Astrometry irregular moon CARPO | Working Group 2 |
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| ASTRO_IRR1_CHALDENE | Astrometry irregular moon CHALDENE | Working Group 2 |
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| ASTRO_IRR1_HIMALIA | Astrometry irregular moon HIMALIA | Working Group 2 |
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| ASTRO_IRR1_KALLICHORE | Astrometry irregular moon KALLICHORE | Working Group 2 |
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| ASTRO_IRR1_LEDA | Astrometry irregular moon LEDA | Working Group 2 |
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| ASTRO_IRR1_LYSITHEA | Astrometry irregular moon LYSITHEA | Working Group 2 |
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| ASTRO_IRR1_MEGACLITE | ASTRO_IRR1_MEGACLITE | Working Group 2 |
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| ASTRO_IRR1_TAYGETE | Astrometry irregular moon TAYGETE | Working Group 2 |
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| ASTRO_IRR1_THEMISTO | Astrometry irregular moon THEMISTO | Working Group 2 |
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| ASTRO_IRR2_ANANKE | Astrometry irregular moon Ananke | Working Group 2 |
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| ASTRO_IRR2_CARME | Astrometry irregular moon Carme | Working Group 2 |
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| ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
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| ASTRO_IRR2_SINOPE | | Working Group 2 |
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| 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 |
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| C_distant | | Working Group 2 |
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| C_GPH | | Working Group 1 |
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| C_GPH_10C2 | test 3_2 | Working Group 1 |
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| C_GPH_10C3 | C_GPH_10C3 | Working Group 1 |
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| C_GPH_10C4 | | Working Group 1 |
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| C_GPH_11C3 | test 3_2 | Working Group 1 |
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| C_GPH_11C4 | C_GPH_11C4 | Working Group 1 |
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| C_GPH_11C5 | | Working Group 1 |
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| C_GPH_12C4 | Test 3_2 | Working Group 1 |
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| C_GPH_12C5 | C_GPH_12C5 | Working Group 1 |
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| C_GPH_13C5 | test 3_2 | Working Group 1 |
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| C_GPH_13C6 | C_GPH_13C6 | Working Group 1 |
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| C_GPH_13C7 | | Working Group 1 |
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| C_GPH_14C6 | test 3_2 | Working Group 1 |
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| C_GPH_14C7 | C_GPH_14C7 | Working Group 1 |
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| C_GPH_14C8 | | Working Group 1 |
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| C_GPH_15C7 | crema 3_2 | Working Group 1 |
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| C_GPH_15C8 | C_GPH_15C8 | Working Group 1 |
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| C_GPH_15C9 | | Working Group 1 |
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| C_GPH_16C10 | | Working Group 1 |
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| C_GPH_16C8 | test 3_2 | Working Group 1 |
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| C_GPH_16C9 | C_GPH_16C9
Geophysics prime segment, defined based on GALA (transmitting) operational range of altitude above Callisto < 2000 km.
Assumed Nadir pointing | Working Group 1 |
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| C_GPH_17C10 | | Working Group 1 |
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| C_GPH_18C10 | test 3_2 | Working Group 1 |
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| C_GPH_18C11 | C_GPH_18C11 | Working Group 1 |
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| C_GPH_19C11 | | Working Group 1 |
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| C_GPH_19C12 | C_GPH_19C12 | Working Group 1 |
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| C_GPH_20C13 | C_GPH_20C13 | Working Group 1 |
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| C_GPH_21C13 | | Working Group 1 |
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| C_GPH_21C14 | C_GPH_21C14 | Working Group 1 |
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| C_GPH_22C11 | test 3_2 | Working Group 1 |
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| C_GPH_22C15 | C_GPH_22C15 | Working Group 1 |
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| C_GPH_23C16 | C_GPH_23C13 | Working Group 1 |
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| C_GPH_24C17 | C_GPH_24C17 | Working Group 1 |
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| C_GPH_25C18 | C_GPH_25C18 | Working Group 1 |
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| C_GPH_26C19 | C_GPH_26C19 | Working Group 1 |
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| C_GPH_28C19 | C_GPH_28C19 | Working Group 1 |
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| C_GPH_29C20 | C_GPH_29C20 | Working Group 1 |
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| C_GPH_5C1 | | Working Group 1 |
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| C_GPH_8C1 | test 3_2 | Working Group 1 |
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| C_GPH_8C2 | | Working Group 1 |
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| C_GPH_9C3 | | Working Group 1 |
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| C_GPH_OBS | Callisto geophysics generic containing obs database link | Working Group 1 |
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| C_IS | | Working Group 3 |
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| C_IS_OBS | C_IS_OBS | Working Group 3 |
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| C_RS | | Working Group 2 |
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| C_RS_10C2 | test 3_2 | Working Group 2 |
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| C_RS_10C3 | C_RS_10C3 | Working Group 2 |
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| C_RS_10C4 | | Working Group 2 |
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| C_RS_11C3 | test 3_2 | Working Group 2 |
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| C_RS_11C4 | C_RS_11C4 | Working Group 2 |
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| C_RS_11C5 | | Working Group 2 |
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| C_RS_12C4 | test 3_2 | Working Group 2 |
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| C_RS_12C5 | C_RS_12C5 | Working Group 2 |
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| C_RS_12C6 | | Working Group 2 |
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| C_RS_13C5 | test 3_2 | Working Group 2 |
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| C_RS_13C6 | C_RS_13C6 | Working Group 2 |
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| C_RS_13C7 | | Working Group 2 |
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| C_RS_14C6 | test 3_2 | Working Group 2 |
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| C_RS_14C7 | C_RS_14C7 | Working Group 2 |
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| C_RS_14C8 | | Working Group 2 |
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| C_RS_15C7 | test 3_2 | Working Group 2 |
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| C_RS_15C8 | C_RS_15C8 | Working Group 2 |
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| C_RS_15C9 | | Working Group 2 |
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| C_RS_16C10 | | Working Group 2 |
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| C_RS_16C8 | test 3_2 | Working Group 2 |
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| C_RS_16C9 | C_RS_16C9: Prime surface and exosphere segment defined as 24 hours centered at CA.
WG1 (gravity) is rider.
Pointing is mainly surface and/or limb (details TBD) | Working Group 2 |
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| C_RS_17C10 | C_RS_17C10 | Working Group 2 |
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| C_RS_17C9 | test 3_2 | Working Group 2 |
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| C_RS_18C10 | test 3_2 | Working Group 2 |
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| C_RS_18C11 | C_RS_18C11 | Working Group 2 |
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| C_RS_19C11 | | Working Group 2 |
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| C_RS_19C12 | C_RS_19C12 | Working Group 2 |
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| C_RS_20C12 | | Working Group 2 |
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| C_RS_20C13 | C_RS_20C13 | Working Group 2 |
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| C_RS_21C13 | | Working Group 2 |
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| C_RS_21C14 | C_RS_21C14 | Working Group 2 |
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| C_RS_22C11 | test 3_2 | Working Group 2 |
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| C_RS_22C15 | C_RS_22C15 | Working Group 2 |
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