UVCS MISSION LOG ---------------- Date: 28 October 2002 ----- Last revision: 29 October 2002 (Wu) -------------- File Name: 2002.10.28.a.log ----------- Compiled by: M. Uzzo, Y.-K. Ko, R. Wu ------------ UVCS Activity: Load and Start SOHO-Ulysses Elemental Abundance Study -------------- JOP112 for 28-29 October 2002 Load Mini-Synoptic for 29 October 2002 Load SOHO-Ulysses Elemental Abundance Study JOP112 for 29 October 2002 Flush, abort and reload above SOHO-Ulysses Elemental Abundance observations at 20:17 UT to change PA to 23 degrees. SOHO Activity: -------------- EOF Staff: S. Parenti: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko: Commander R. Wu Command file: 02.10.28.13:07:39.cmd.log Activity: --------- 1) SOHO-Ulysses Elemental Abundance Study JOP112 Sequence: 02.10_parenti.tcl SCI_SPEC: The program involves the observations of coronal hole - streamer boundary at several solar distances. The purpose is to determine the variation of the elements composition accross this interface. With these data we try to estimate the FIP effect in the two regions and establish their contribution to the fast and slow solar wind. OBS_PROG: Primary: Temporal Coverage Sub Obj: Spatial Coverage SCI_OBJ: Abundances...Electron Temperature and Ionization State OBJ: Streamer Boundary CMP_NAME: JOP112 SOHO-Ulysses Elemental Abundance Study CDS, LASCO, SUMER, UVCS, Ulysses (S/C) CMP_NUM: 6905 Duration: start: 2002.10.28.16:43 end: 2002.10.28.20:06 ONUMs = 18160 (16 exps) 18161 (77 exps) ; aborted 18162 (80 exps) ; flushed 18163 (80 exps) ; flushed 18164 (16 exps) ; flushed Instrument configuration: - Pointing: Sun center - Roll: 337 Degrees (14575) - Mirror/Occulter: 1.6 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 173000, 100000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_SP_173 in slot 5 OVI_SP_100 in slot 4 Fits Files: q02.10.28.16:41:43.lya.dat q02.10.28.16:41:43.ovi.dat q02.10.28.16:41:43.vld.dat q02.10.28.17:18:37.lya.dat q02.10.28.17:18:37.ovi.dat q02.10.28.17:18:37.vld.dat 2) SOHO-Ulysses Elemental Abundance Study JOP112 Sequence: 02.10_parenti.tcl SCI_SPEC: The program involves the observations of coronal hole - streamer boundary at several solar distances. The purpose is to determine the variation of the elements composition accross this interface. With these data we try to estimate the FIP effect in the two regions and establish their contribution to the fast and slow solar wind. OBS_PROG: Primary: Temporal Coverage Sub Obj: Spatial Coverage SCI_OBJ: Abundances...Electron Temperature and Ionization State OBJ: Streamer Boundary CMP_NAME: JOP112 SOHO-Ulysses Elemental Abundance Study CDS, LASCO, SUMER, UVCS, Ulysses (S/C) CMP_NUM: 6905 Duration: start: 2002.10.28.20:19 end: 2002.10.29.06:12 ONUMs = 18162 (16 exps) 18163 (80 exps) 18164 (80 exps) 18165 (80 exps) 18166 (16 exps) Instrument configuration: - Pointing: Sun center - Roll: 23 Degrees (22949) - Mirror/Occulter: 1.6 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 173000, 100000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_SP_173 in slot 5 OVI_SP_100 in slot 4 Fits Files: q02.10.28.20:17:52.lya.dat q02.10.28.20:17:52.ovi.dat q02.10.28.20:17:52.vld.dat q02.10.28.20:54:50.lya.dat q02.10.28.20:54:50.ovi.dat q02.10.28.20:54:50.vld.dat q02.10.28.23:48:33.lya.dat q02.10.28.23:48:33.ovi.dat q02.10.28.23:48:33.vld.dat q02.10.29.02:42:23.lya.dat q02.10.29.02:42:23.ovi.dat q02.10.29.02:42:23.vld.dat q02.10.29.05:36:06.lya.dat q02.10.29.05:36:06.ovi.dat q02.10.29.05:36:06.vld.dat 3) 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: 2002.10.29.06:26 end: 2002.10.29.09:52 ONUMs = 40220 (9 exps) 40221 (9 exps) 40222 (9 exps) 40223 (9 exps) 40224 (9 exps) 40225 (9 exps) 40226 (9 exps) 40227 (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: z02.10.29.06:25:04.lya.dat z02.10.29.06:25:04.ovi.dat z02.10.29.06:25:04.vld.dat z02.10.29.06:51:40.lya.dat z02.10.29.06:51:40.ovi.dat z02.10.29.06:51:40.vld.dat z02.10.29.07:18:10.lya.dat z02.10.29.07:18:10.ovi.dat z02.10.29.07:18:10.vld.dat z02.10.29.07:44:45.lya.dat z02.10.29.07:44:45.ovi.dat z02.10.29.07:44:45.vld.dat z02.10.29.08:11:14.lya.dat z02.10.29.08:11:14.ovi.dat z02.10.29.08:11:14.vld.dat z02.10.29.08:37:50.lya.dat z02.10.29.08:37:50.ovi.dat z02.10.29.08:37:50.vld.dat z02.10.29.09:04:26.lya.dat z02.10.29.09:04:26.ovi.dat z02.10.29.09:04:26.vld.dat z02.10.29.09:30:56.lya.dat z02.10.29.09:30:56.ovi.dat z02.10.29.09:30:56.vld.dat 4) SOHO-Ulysses Elemental Abundance Study JOP112 Sequence: 02.10_parenti.tcl SCI_SPEC: The program involves the observations of coronal hole - streamer boundary at several solar distances. The purpose is to determine the variation of the elements composition accross this interface. With these data we try to estimate the FIP effect in the two regions and establish their contribution to the fast and slow solar wind. OBS_PROG: Primary: Temporal Coverage Sub Obj: Spatial Coverage SCI_OBJ: Abundances...Electron Temperature and Ionization State OBJ: Streamer Boundary CMP_NAME: JOP112 SOHO-Ulysses Elemental Abundance Study CMP_NUM: 6905 Duration: start: 2002.10.29.10:14 end: 2002.10.29.20:06 ONUMs = 18167 (16 exps) 18168 (80 exps) 18169 (80 exps) 18170 (80 exps) 18171 (16 exps) Instrument configuration: - Pointing: Sun center - Roll: 23 Degrees (22949) - Mirror/Occulter: 1.6 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 173000, 100000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_SP_173 in slot 5 OVI_SP_100 in slot 4 Fits Files: q02.10.29.10:12:30.lya.dat q02.10.29.10:12:30.ovi.dat q02.10.29.10:12:30.vld.dat q02.10.29.10:49:28.lya.dat q02.10.29.10:49:28.ovi.dat q02.10.29.10:49:28.vld.dat q02.10.29.13:43:04.lya.dat q02.10.29.13:43:04.ovi.dat q02.10.29.13:43:04.vld.dat q02.10.29.16:36:50.lya.dat q02.10.29.16:36:50.ovi.dat q02.10.29.16:36:50.vld.dat q02.10.29.19:30:36.lya.dat q02.10.29.19:30:36.ovi.dat q02.10.29.19:30:36.vld.dat