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### By Prime Segment

### By trajectories

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 |

G_IS_3G3 | Ganymede in-situ observations around closest approach | Working Group 3 |

JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |

G_IS_4G4 | Working Group 3 | |

JM_PE35 | Working Group 3 | |

JM_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |

JM_PE31 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |

JM_PE29 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |

JM_PE27 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |

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 |

TOR_RS | Working Group 3 | |

JM_INCL | Working Group 3 | |

JM_PE_P4_noDL | Working Group 3 | |

JM_PE_P4 | Perijoves with WG3 prime (--> 20/09/18: modified (discussion with OW). assuming ~2 times what is produced in G4-G5 scenario (~6.5-7 Gb). Corresponds roughly to 19kbps, copied from JA_INCL) RS rate assumes no D/L suspension (case 2) | Working Group 3 |

JM_CB | Working Group 3 | |

JM_ENA | Working Group 3 | |

JM_GM | Working Group 3 | |

JM_PE | 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) | Working Group 3 |

G_IS | Working Group 3 | |

E_IS | Working Group 3 | |

C_IS | Working Group 3 |

29 segment definitions