UVCS MISSION LOG ---------------- Date: 18 July 2002 ----- Last revision: 19 July 2002 (Wu) -------------- File Name: 2002.07.18.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Polar Coronal Hole Study for ------------ 18 - 19 July 2002 Load Mini-Synoptic for 19 July 2002 Load Polar Coronal Hole Study for 19 July 2002 Load Long Synoptic For 19 - 20 July 2002 SOHO Activity: -------------- EOF Staff: L. Zangrilli: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner Command file: 02.07.18.14:33:01.cmd.log Activity: --------- 1) Polar Coronal Hole Study Sequence: 02.07_lz1.tcl SCI_SPEC: To study the structure of newborn coronal holes of the new cycle, and to investigate a possible asymmetry between the north and the south poles. OBS_PROG: Primary: Spatial Coverage Sub Obj: Spectral Resolution SCI_OBJ: Primary: Coronal Structure Sub Obj: Large-Scale Structure OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2002.07.18.15:48 end: 2002.07.19.01:45 ONUMs = 17747 (113 exps) Instrument configuration: - Pointing: Sun center - Roll: 0 degrees (18762) - Mirror/Occulter: 1.6, 1.8, 2.0, 2.5, 3.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_LZ_194372 in Slot 4 Fits Files: q02.07.18.15:33:17.lya.dat q02.07.18.15:33:17.ovi.dat q02.07.18.15:33:17.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: 2002.07.19.01:56 end: 2002.07.19.05:23 ONUMs = 39240 (9 exps) 39241 (9 exps) 39242 (9 exps) 39243 (9 exps) 39244 (9 exps) 39245 (9 exps) 39246 (9 exps) 39247 (7 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: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z02.07.19.01:55:33.lya.dat z02.07.19.01:55:33.ovi.dat z02.07.19.01:55:33.vld.dat z02.07.19.02:22:06.lya.dat z02.07.19.02:22:06.ovi.dat z02.07.19.02:22:06.vld.dat z02.07.19.02:48:43.lya.dat z02.07.19.02:48:43.ovi.dat z02.07.19.02:48:43.vld.dat z02.07.19.03:15:18.lya.dat z02.07.19.03:15:18.ovi.dat z02.07.19.03:15:18.vld.dat z02.07.19.03:41:47.lya.dat z02.07.19.03:41:47.ovi.dat z02.07.19.03:41:47.vld.dat z02.07.19.04:08:16.lya.dat z02.07.19.04:08:16.ovi.dat z02.07.19.04:08:16.vld.dat z02.07.19.04:34:53.lya.dat z02.07.19.04:34:53.ovi.dat z02.07.19.04:34:53.vld.dat z02.07.19.05:01:26.lya.dat z02.07.19.05:01:26.ovi.dat z02.07.19.05:01:26.vld.dat 3) Polar Coronal Hole Study Sequence: 02.07_lz2.tcl SCI_SPEC: To study the structure of newborn coronal holes of the new cycle, and to investigate a possible asymmetry between the north and the south poles. OBS_PROG: Primary: Spatial Coverage Sub Obj: Spectral Resolution SCI_OBJ: Primary: Coronal Structure Sub Obj: Large-Scale Structure OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2002.07.19.05:47 end: 2002.07.19.15:44 ONUMs = 17748 (114 exps) Instrument configuration: - Pointing: Sun center - Roll: 0 degrees (18762) - Mirror/Occulter: 3.0, 3.5 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_LZ_194372 in Slot 4 Fits Files: q02.07.19.05:35:08.lya.dat q02.07.19.05:35:08.ovi.dat q02.07.19.05:35:08.vld.dat