UVCS MISSION LOG ---------------- Date: 30 January 2002 ----- Last revision: 01 February 2002 (Wu) -------------- File Name: 2002.01.31.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Active Region Streamer Study for -------------- 31 January - 01 February 2002 Load Mini Synoptic for 01 February 2002 Load Active Region Streamer Study for 01 February 2002 Load Long Synoptic for 01 - 02 February 2002 SOHO Activity: CELIAS CTOF Recovery ~ 16:00 - 16:30 UT -------------- EOF Staff: Y.-K. Ko: Lead Scientist, Planner ---------- R. Wu: Commander M. Uzzo Command file: 02.01.31.15:30:38.cmd.log Activity: --------- 1) Active Region Streamer Study Sequence: 02.01_ar.tcl SCI_SPEC: Characterize the electron temperature and elemental abundances in the corona above active regions of various properties (e.g. size, magnetic configurations). OBS_PROG: Primary: Spectral Coverage Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Electron Temperature Abundances OBJ: Streamer (Active Region) CMP_NAME: AR Streamer Study, JOP 151 CMP_NUM: 6844 Duration: start: 2002.01.31.16:41 end: 2002.02.01.02:40 ONUMs = 17082 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 77 degrees (32789) - Mirror/Occulter: 1.6 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 184200, 103000, 225000, 236900 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: msk_000303_OVI in slot 3 Fits Files: q02.01.31.16:39:38.lya.dat q02.01.31.16:39:38.ovi.dat q02.01.31.16:39:38.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: 2002.02.01.02:59 end: 2002.02.01.06:26 ONUMs = 37630 (9 exps) 37631 (9 exps) 37632 (9 exps) 37633 (9 exps) 37634 (9 exps) 37635 (9 exps) 37636 (9 exps) 37637 (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: 184200 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_184 in slot 2 Fits Files: z02.02.01.02:58:24.lya.dat z02.02.01.02:58:24.ovi.dat z02.02.01.02:58:24.vld.dat z02.02.01.03:25:02.lya.dat z02.02.01.03:25:02.ovi.dat z02.02.01.03:25:02.vld.dat z02.02.01.03:51:45.lya.dat z02.02.01.03:51:45.ovi.dat z02.02.01.03:51:45.vld.dat z02.02.01.04:18:14.lya.dat z02.02.01.04:18:14.ovi.dat z02.02.01.04:18:14.vld.dat z02.02.01.04:44:43.lya.dat z02.02.01.04:44:43.ovi.dat z02.02.01.04:44:43.vld.dat z02.02.01.05:11:19.lya.dat z02.02.01.05:11:19.ovi.dat z02.02.01.05:11:19.vld.dat z02.02.01.05:37:55.lya.dat z02.02.01.05:37:55.ovi.dat z02.02.01.05:37:55.vld.dat z02.02.01.06:04:22.lya.dat z02.02.01.06:04:22.ovi.dat z02.02.01.06:04:22.vld.dat 3) Active Region Streamer Study Sequence: 02.01_ar.tcl SCI_SPEC: Characterize the electron temperature and elemental abundances in the corona above active regions of various properties (e.g. size, magnetic configurations). OBS_PROG: Primary: Spectral Coverage Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Electron Temperature Abundances OBJ: Streamer (Active Region) CMP_NAME: AR Streamer Study, JOP 151 CMP_NUM: 6844 Duration: start: 2002.02.01.06:42 end: 2002.02.01.16:41 ONUMs = 17083 (169 exps) Instrument configuration: - Pointing: Sun center - Roll: 77 degrees (32789) - Mirror/Occulter: 1.9 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 184200, 103000, 225000, 236900 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: msk_000303_OVI in slot 3 Fits Files: q02.02.01.06:41:13.lya.dat q02.02.01.06:41:13.ovi.dat q02.02.01.06:41:13.vld.dat