UVCS MISSION LOG ---------------- Date: 15 July 2003 ----- Last revision: 20 July 2003 (Wu) -------------- File Name: 2003.07.19.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Synoptic for 19 - 20 July 2003 -------------- Coronal Jet Study for 20 July 2003 SOHO Activity: -------------- EOF Staff: D. Dobrzycka: Lead Scientist ---------- M. Uzzo: Commander Y.-K. Ko: Planner R. Wu Command file: 03.07.18.13:03:48.cmd.log Activity: --------- 1) Synoptic Sequence Load and Start Sequence: SynopticA:Start 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: 2003.07.19.15:34 end: 2003.07.20.05:30 ONUMs = 42640 (56 exps) 42641 (56 exps) 42642 (37 exps) 42643 (37 exps) 42644 (37 exps) 42645 (37 exps) 42646 (37 exps) 42647 (37 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: NE: STR1A, N: STR1A, NW: STR2B, W: STR2B, SW: STR2B, S: STR2B, SE: STR2B, E: STR2B, - Mirror/Occulter: STR1A: 3.5, 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR2B: 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR3A: 3.5, 3.0 Ro STR4B: 4.0 Ro STR5A: 2.1, 1.9, 1.75, 1.6 Ro STR6B: 2.5 Ro STR7B: 3.0 Ro CH1A: 1.9, 1.75, 1.6 Ro CH2A: 2.1 Ro CH2B: 2.1 Ro CH3B: 2.5 Ro CH4A: 1.75, 1.6 Ro CH5B: 1.9 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75, 1.9, 2.1, 2.5, 3.0, 3.5, 4.0 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (STR1A, STR2B, STR3A, STR4B, CH1A, CH2A, CH2B, CH3B) 100 um (CH4A, CH5B) 75 um (STR5A, STR6B, STR7B) - LYA GRTPOS: 128000 - OVI GRTPOS: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z03.07.19.15:33:40.lya.dat z03.07.19.15:33:40.ovi.dat z03.07.19.15:33:40.vld.dat z03.07.19.17:50:47.lya.dat z03.07.19.17:50:47.ovi.dat z03.07.19.17:50:47.vld.dat z03.07.19.20:07:26.lya.dat z03.07.19.20:07:26.ovi.dat z03.07.19.20:07:26.vld.dat z03.07.19.21:42:06.lya.dat z03.07.19.21:42:06.ovi.dat z03.07.19.21:42:06.vld.dat z03.07.19.23:16:35.lya.dat z03.07.19.23:16:35.ovi.dat z03.07.19.23:16:35.vld.dat z03.07.20.00:51:27.lya.dat z03.07.20.00:51:27.ovi.dat z03.07.20.00:51:27.vld.dat z03.07.20.02:25:54.lya.dat z03.07.20.02:25:54.ovi.dat z03.07.20.02:25:54.vld.dat z03.07.20.04:00:33.lya.dat z03.07.20.04:00:33.ovi.dat z03.07.20.04:00:33.vld.dat 2) Coronal Jet Study Sequence: 03.06_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: 6965 Duration: start: 2003.07.20.05:57 end: 2003.07.20.15:47 ONUMs = 20085 (80 exps) 20086 (80 exps) 20087 (80 exps) 20088 (32 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 345.0 Degrees (48820) - 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: q03.07.20.05:56:44.lya.dat q03.07.20.05:56:44.ovi.dat q03.07.20.05:56:44.vld.dat q03.07.20.08:50:26.lya.dat q03.07.20.08:50:26.ovi.dat q03.07.20.08:50:26.vld.dat q03.07.20.11:44:06.lya.dat q03.07.20.11:44:06.ovi.dat q03.07.20.11:44:06.vld.dat q03.07.20.14:37:49.lya.dat q03.07.20.14:37:49.ovi.dat q03.07.20.14:37:49.vld.dat