EVENT DATE TIME (PST/SCET)
Start Encounter 14 Dec 96 16:00
End last Europa-4 Io torus obs. (UVS) 15 02:19
OTM-16 18:30
Jupiter auroral map (UVS) 16 02:00
First hot spot observation (PPR) 17 06:48
Io eclipse ingress observation (NIMS) 11:09
Io eclipse thermal observation (SSI) 11:46
Io eclipse egress observation (NIMS) 13:27
Amalthea imaging (SSI) 23:13
Thebe imaging (SSI) 18 00:10
Europa global observation (PPR) 11:55
Io C/A (range = 321000km) 13:37
Europa global mosaic (NIMS) 17:19
Jupiter C/A (range = 655000km) 19:22
Adrastea imaging (SSI) 19:30
Europa maculae region (SSI) 19:40
Europa wake crossing recording (F&P) 22:20
Europa Double Line area (NIMS) 22:27
Start Solar occultation by Europa 22:51
Start Earth occultation by Europa
Europa C/A (range = 2270 km) 22:53
End Solar occultation by Europa 23:08
End Earth occultation by Europa 23:09
Ganymede C/A (range = 792000 km) 19 12:12
Science Turn (high-phase Jupiter) 20:00
First high-phase Jupiter observation (SSI) 22:34
Callisto C/A (range = 1490000km) 05:32
Last high-phase Jupiter observation (NIMS) 08:50
Last hot spot observation (UVS) 08:53
Jupiter rings observation (NIMS) 09:11
Turn to return to Earth point 10:23
Himalia observation (UVS) 21:57
Atmospheric profile during occultation (RS) 21 08:17
Start Earth occultation by Jupiter 09:43
End Europa-4 real-time survey (F&P) 11:00
End Earth occultation by Jupiter 16:37
Start Solar occultation by Jupiter 18:52
End Solar occultation by Jupter 22 02:52
Start Playback 05:00
OTM-17 23 01:45
Turn for attitude maintenance 26 12:38
OTM-18 04 Jan 1997 06:30
Turn for attitude maintenance 08 06:53
Start Solar conjunction* 10 14:14
End Solar conjunction 28 07:09
OTM-19 06 Feb 05:00
First Europa-6 approach OPNAV 09 17:00
Turn for attitude maintenance 10 10:38
Last Europa-6 approach OPNAV 15 22:49
End Playback 16 16:00
* Solar conjunction contains a phasing orbit fly through the Jovian system.
Refer to Jupiter - Orbit 5 supplement.
** Closest approach distances are with respect to the center
of the target body.
*** Due to anomaly, PPR will be observing in only one filter.
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