| J_SAT_S2017_J2 | | Working Group 2 |
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| J_SAT_S2016_J1 | | Working Group 2 |
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| J_SAT_S2011_J2 | | Working Group 2 |
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| J_SAT_S2010_J2 | | Working Group 2 |
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| J_SAT_S2010_J1 | | Working Group 2 |
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| J_SAT_S2003_J9 | | Working Group 2 |
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| J_SAT_S2003_J4 | | Working Group 2 |
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| J_SAT_S2003_J19 | | Working Group 2 |
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| J_SAT_S2003_J16 | | Working Group 2 |
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| J_SAT_S2003_J12 | | Working Group 2 |
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| J_SAT_PHILOPHROSYNE | | Working Group 2 |
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| J_SAT_ORTHOSIE | | Working Group 2 |
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| J_SAT_MNEME | | Working Group 2 |
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| J_SAT_KALYKE | | Working Group 2 |
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| J_SAT_KALE | | Working Group 2 |
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| J_SAT_EUPORIE | | Working Group 2 |
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| J_SAT_EUPHEME | | Working Group 2 |
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| J_SAT_EUKELADE | | Working Group 2 |
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| J_SAT_EIRENE | | Working Group 2 |
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| J_SAT_DIA | | Working Group 2 |
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| J_SAT_CARPO | | Working Group 2 |
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| J_SAT_AITNE | | Working Group 2 |
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| J_SAT_VALETUDO | | Working Group 2 |
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| J_SAT_THEMISTO | | Working Group 2 |
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| J_SAT_TAYGETE | | Working Group 2 |
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| J_SAT_SINOPE | | Working Group 2 |
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| J_SAT_PASITHEE | | Working Group 2 |
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| J_SAT_PASIPHAE | | Working Group 2 |
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| J_SAT_PANDIA | | Working Group 2 |
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| J_SAT_MEGACLITE | | Working Group 2 |
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| J_SAT_LYSITHEA | | Working Group 2 |
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| J_SAT_LEDA | | Working Group 2 |
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| 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 |
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| 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_CARME | | Working Group 2 |
|---|
| J_SAT_AUTONOE | | Working Group 2 |
|---|
| J_SAT_ARCHE | | Working Group 2 |
|---|
| J_SAT_AOEDE | | Working Group 2 |
|---|
| J_SAT_ANANKE | | Working Group 2 |
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| G_RS_1G1 | | Working Group 2 |
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| G_RS_5G5 | | Working Group 2 |
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| RING_PHASECURV_170 | | Working Group 2 |
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| RING_PHASECURV_160 | | Working Group 2 |
|---|
| RING_PHASECURV_150 | | Working Group 2 |
|---|
| RING_PHASECURV_140 | | Working Group 2 |
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| RING_PHASECURV_130 | | Working Group 2 |
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| RING_PHASECURV_120 | | Working Group 2 |
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| RING_PHASECURV_110 | | Working Group 2 |
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| RING_PHASECURV_100 | | Working Group 2 |
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| RING_PHASECURV_90 | | Working Group 2 |
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| RING_PHASECURV_80 | | Working Group 2 |
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| RING_PHASECURV_70 | | Working Group 2 |
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| RING_PHASECURV_60 | | Working Group 2 |
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| RING_PHASECURV_50 | | Working Group 2 |
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| RING_PHASECURV_40 | | Working Group 2 |
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| RING_PHASECURV_30 | | Working Group 2 |
|---|
| RING_PHASECURV_20 | | Working Group 2 |
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| EUROPA_DISTANT | | Working Group 2 |
|---|
| J_SAT_INN_AST_A | | Working Group 2 |
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| J_SAT_IRR_AST_E | | Working Group 2 |
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| J_SAT_INN_CHAR_A | | Working Group 2 |
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| J_SAT_INN_AST_T | | Working Group 2 |
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| J_SAT_IRR_CHAR_E | | Working Group 2 |
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| G_RS_4G4 | | Working Group 2 |
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| G_RS_2G2 | | Working Group 2 |
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| IO_RS | | Working Group 2 |
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| J_RING | | Working Group 2 |
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| G_distant | | Working Group 2 |
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| E_RS | | Working Group 2 |
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| E_distant | | Working Group 2 |
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| C_distant | | Working Group 2 |
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| ASTRO_IRR2_SINOPE | | Working Group 2 |
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| ASTRO_IRR_ELARA | | Working Group 2 |
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| CALLISTO_DISTANT | | Working Group 2 |
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| CHARACTERIZATION_IRR2_CARME | | Working Group 2 |
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| GANYMEDE_DISTANT | | Working Group 2 |
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| JM_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE31 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE29 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE27 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE25 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE23 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE21 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE19 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE17 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE15 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE13 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |
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| JUPITER_TAIL | In situ search for signatures of local magnetic reconnection in the Jovian magnetotail | Working Group 3 |
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| JUPITER_GM | In situ mapping of global configuration and monitoring dynamics of the Jovian magnetospheric environment.
corotation should be in the FoV of PEP/JDC or PEP/JEI.
Conditions for coverage:
◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation
◦ Boresight angle of JDC or JEI less than ˜90 deg
Conditions for ideal coverage:
◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation
◦ Boresight angle less than ˜75 deg (JEI) or 70 deg (JDC): corotation away from the FoV edge
JDC is preferred for monitoring corotation, over JEI, when possible. | Working Group 3 |
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