12 | | 21 January: The BM1 periods at the inbound magnetopause crossings were deleted, following the SOWG meeting. Some BM1 periods around the magnetic equator were proposed, requiring individual timings for each satellite, and some BM2 periods for EQUA. It was also decided that NM3 should be used on C1 during the Blanco-Cano long NM1 sessions, and a 1h BM1 period on C1 for the inbound Bow Shock should be inserted. The D0 (no-data-taking) periods were removed for the orbits which involved the Blanco-Cano requests. New Bryant plots, single SC BM and D0 lists, and updated by-orbit analysis are attached. |
| 12 | 21 January: The BM1 periods at the inbound magnetopause crossings were deleted, following the SOWG meeting. Some BM1 periods around the magnetic equator were proposed, requiring individual timings for each satellite, and some BM2 periods for EQUA. It was also decided that NM3 should be used on C1 during the Blanco-Cano long NM1 sessions, and a 1h BM1 period on C1 for the inbound Bow Shock should be inserted. The D0 (no-data-taking) periods were removed for the orbits which involved the Blanco-Cano requests. New Bryant plots, single SC BM, NM3 and D0 lists, and updated by-orbit analysis are attached. |