UVCS MISSION LOG ---------------- Date: 09 September 2002 ----- Last revision: 10 September 2002 (Wu) -------------- File Name: 2002.09.09.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load and Start Polar Coronal Jets Study for ------------- 09 - 10 September 2002 Load Mini Synoptic for 10 September 2002 Load Polar Coronal Jets Study for 10 September 2002 SOHO Activity: -------------- EOF Staff: D. Dobrzycka: Lead Scientist ---------- Y.-K. Ko: Commander, Planner D. H. Phillips: Planner M. Uzzo R. Wu Command file: 02.09.09.14:48:15.cmd.log Activity: --------- 1) Polar Coronal Jets Study Sequence: 02.09_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: JOP155 - Polar Coronal Jets at the Declining Phase of the Solar Cycle, UVCS, EIT, LASCO, CDS, TRACE (S/C) CMP_NUM: 6894 Duration: start: 2002.09.09.16:56 end: 2002.09.10.02:47 ONUMs = 17990 (80 exps) 17991 (80 exps) 17992 (80 exps) 17993 (32 exps) Instrument configuration: - Pointing: Sun center - Roll: 340 Degrees (15121) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_CME_173 in slot 4 Fits Files: q02.09.09.16:56:08.lya.dat q02.09.09.16:56:08.ovi.dat q02.09.09.16:56:08.vld.dat q02.09.09.19:49:52.lya.dat q02.09.09.19:49:52.ovi.dat q02.09.09.19:49:52.vld.dat q02.09.09.22:43:41.lya.dat q02.09.09.22:43:41.ovi.dat q02.09.09.22:43:41.vld.dat q02.09.10.01:37:22.lya.dat q02.09.10.01:37:22.ovi.dat q02.09.10.01:37:22.vld.dat 2) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 210, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2002.09.10.02:56 end: 2002.09.10.06:23 ONUMs = 39740 (9 exps) 39741 (9 exps) 39742 (9 exps) 39743 (9 exps) 39744 (9 exps) 39745 (9 exps) 39746 (9 exps) 39747 (9 exps) Instrument configuration: - Pointing: Sun center - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.09.10.02:55:00.lya.dat z02.09.10.02:55:00.ovi.dat z02.09.10.02:55:00.vld.dat z02.09.10.03:21:29.lya.dat z02.09.10.03:21:29.ovi.dat z02.09.10.03:21:29.vld.dat z02.09.10.03:47:59.lya.dat z02.09.10.03:47:59.ovi.dat z02.09.10.03:47:59.vld.dat z02.09.10.04:14:34.lya.dat z02.09.10.04:14:34.ovi.dat z02.09.10.04:14:34.vld.dat z02.09.10.04:41:03.lya.dat z02.09.10.04:41:03.ovi.dat z02.09.10.04:41:03.vld.dat z02.09.10.05:07:39.lya.dat z02.09.10.05:07:39.ovi.dat z02.09.10.05:07:39.vld.dat z02.09.10.05:34:24.lya.dat z02.09.10.05:34:24.ovi.dat z02.09.10.05:34:24.vld.dat z02.09.10.06:00:57.lya.dat z02.09.10.06:00:57.ovi.dat z02.09.10.06:00:57.vld.dat 3) Polar Coronal Jets Study Sequence: 02.09_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: JOP155 - Polar Coronal Jets at the Declining Phase of the Solar Cycle, UVCS, EIT, LASCO, CDS, TRACE (S/C) CMP_NUM: 6894 Duration: start: 2002.09.10.06:48 end: 2002.09.10.16:38 ONUMs = 17994 (80 exps) 17995 (80 exps) 17996 (80 exps) 17997 (32 exps) Instrument configuration: - Pointing: Sun center - Roll: 340 Degrees (15121) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_CME_173 in slot 4 Fits Files: q02.09.10.06:47:49.lya.dat q02.09.10.06:47:49.ovi.dat q02.09.10.06:47:49.vld.dat q02.09.10.09:41:28.lya.dat q02.09.10.09:41:28.ovi.dat q02.09.10.09:41:28.vld.dat q02.09.10.12:35:17.lya.dat q02.09.10.12:35:17.ovi.dat q02.09.10.12:35:17.vld.dat q02.09.10.15:28:58.lya.dat q02.09.10.15:28:58.ovi.dat q02.09.10.15:28:58.vld.dat