UVCS MISSION LOG ---------------- Date: 21 October 2003 ----- Last revision: 31 October 2003 (Wu) -------------- File Name: 2003.10.21.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Coronal Jet Study for -------------- 21 - 22 October 2003 using Batch Queue Time Tagged Commands via Background Queue Load Mini-Synoptic for 22 October 2003 using Batch Queue Time Tagged Commands via Background Queue SOHO Activity: -------------- EOF Staff: D. Dobrzycka: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner D. Phillips: Planner M. Uzzo Command file: UVCS31021.BCK Activity: --------- 1) Coronal Jet Study Sequence: 03.10_danuta.tcl SCI_SPEC: Study of the dynamic jet structures originating in the polar coronal holes. The polar jets were originally observed at solar minimum when the polar holes were large, dominating structures in the corona. At the current declining phase of the solar cycle the polar holes appeared again as permanent structures. The purpose of the observations is to study counterparts of solar minimum polar coronal jets. OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Coverage SCI_OBJ: Coronal Structure...Fine Structure OBJ: Coronal Hole CMP_NAME: Polar Coronal Jets; UVCS; CDS; EIT; LASCO; TRACE (JOP 155) CMP_NUM: 6992 Duration: start: 2003.10.21.17:42 end: 2003.10.22.13:23 ONUMs = 20422 (80 exps) 20423 (80 exps) 20424 (80 exps) 20425 (80 exps) 20426 (80 exps) 20427 (80 exps) 20428 (63 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 0.0 Degrees (18762) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: q03.10.21.17:42:00.lya.dat q03.10.21.17:42:00.ovi.dat q03.10.21.17:42:00.vld.dat q03.10.21.20:35:43.lya.dat q03.10.21.20:35:43.ovi.dat q03.10.21.20:35:43.vld.dat q03.10.21.23:29:32.lya.dat q03.10.21.23:29:32.ovi.dat q03.10.21.23:29:32.vld.dat q03.10.22.02:23:12.lya.dat q03.10.22.02:23:12.ovi.dat q03.10.22.02:23:12.vld.dat q03.10.22.05:17:01.lya.dat q03.10.22.05:17:01.ovi.dat q03.10.22.05:17:01.vld.dat q03.10.22.08:10:41.lya.dat q03.10.22.08:10:41.ovi.dat q03.10.22.08:10:41.vld.dat q03.10.22.11:04:30.lya.dat q03.10.22.11:04:30.ovi.dat q03.10.22.11:04:30.vld.dat 2) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 215, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2003.10.22.13:34 end: 2003.10.22.17:00 ONUMs = 43560 (9 exps) 43561 (9 exps) 43562 (9 exps) 43563 (9 exps) 43564 (9 exps) 43565 (9 exps) 43566 (9 exps) 43567 (9 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: W, NW, N, NE, E, SE, S, SW - Mirror/Occulter: 1.6, 1.75 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75 Ro) - LYA Slits: 50 um - OVI Slits: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z03.10.22.13:33:33.lya.dat z03.10.22.13:33:33.ovi.dat z03.10.22.13:33:33.vld.dat z03.10.22.14:00:15.lya.dat z03.10.22.14:00:15.ovi.dat z03.10.22.14:00:15.vld.dat z03.10.22.14:26:44.lya.dat z03.10.22.14:26:44.ovi.dat z03.10.22.14:26:44.vld.dat z03.10.22.14:53:13.lya.dat z03.10.22.14:53:13.ovi.dat z03.10.22.14:53:13.vld.dat z03.10.22.15:19:42.lya.dat z03.10.22.15:19:42.ovi.dat z03.10.22.15:19:42.vld.dat z03.10.22.15:46:04.lya.dat z03.10.22.15:46:04.ovi.dat z03.10.22.15:46:04.vld.dat z03.10.22.16:12:39.lya.dat z03.10.22.16:12:39.ovi.dat z03.10.22.16:12:39.vld.dat z03.10.22.16:39:00.lya.dat z03.10.22.16:39:00.ovi.dat z03.10.22.16:39:00.vld.dat