UVCS MISSION LOG ---------------- Date: 16 July 2002 ----- Last revision: 21 July 2002 (Wu) -------------- File Name: 2002.07.16.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Polar Coronal Hole Study for ------------ 16 - 17 July 2002 Load Mini-Synoptic for 17 July 2002 Load Polar Coronal Hole Study for 17 July 2002 Load Long Synoptic For 17 - 18 July 2002 SOHO Activity: -------------- EOF Staff: L. Zangrilli: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 02.07.16.15:59:01.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: 2002.07.16.16:12 end: 2002.07.17.02:09 ONUMs = 17745 (113 exps) Instrument configuration: - Pointing: Sun center - Roll: 180 degrees (51551) - 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: q02.07.16.16:01:29.lya.dat q02.07.16.16:01:29.ovi.dat q02.07.16.16:01:29.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: 2002.07.17.02:38 end: 2002.07.17.06:05 ONUMs = 39221 (9 exps) 39222 (9 exps) 39223 (9 exps) 39224 (9 exps) 39225 (9 exps) 39226 (9 exps) 39227 (9 exps) 39228 (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: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z02.07.17.02:37:18.lya.dat z02.07.17.02:37:18.ovi.dat z02.07.17.02:37:18.vld.dat z02.07.17.03:03:49.lya.dat z02.07.17.03:03:49.ovi.dat z02.07.17.03:03:49.vld.dat z02.07.17.03:30:33.lya.dat z02.07.17.03:30:33.ovi.dat z02.07.17.03:30:33.vld.dat z02.07.17.03:57:01.lya.dat z02.07.17.03:57:01.ovi.dat z02.07.17.03:57:01.vld.dat z02.07.17.04:23:30.lya.dat z02.07.17.04:23:30.ovi.dat z02.07.17.04:23:30.vld.dat z02.07.17.04:49:59.lya.dat z02.07.17.04:49:59.ovi.dat z02.07.17.04:49:59.vld.dat z02.07.17.05:16:35.lya.dat z02.07.17.05:16:35.ovi.dat z02.07.17.05:16:35.vld.dat z02.07.17.05:43:11.lya.dat z02.07.17.05:43:11.ovi.dat z02.07.17.05:43:11.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: 2002.07.17.06:12 end: 2002.07.17.16:09 ONUMs = 17746 (114 exps) Instrument configuration: - Pointing: Sun center - Roll: 180 degrees (51551) - 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: q02.07.17.06:06:01.lya.dat q02.07.17.06:06:01.ovi.dat q02.07.17.06:06:01.vld.dat