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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