UVCS MISSION LOG ---------------- Date: 30 January 2002 ----- Last revision: 01 February 2002 (Wu) -------------- File Name: 2002.01.30.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Active Region Streamer Study for -------------- 30 - 31 January 2002 Load Mini Synoptic for 31 January 2002 Load Active Region Streamer Study for 31 January 2002 SOHO Activity: CELIAS recovery status: MTOF recovered yesterday, STOF -------------- recovery today from ~16-20 UT. CTOF recovery is planned to begin sometime after STOF have been recovered. EOF Staff: Y.-K. Ko: Lead Scientist, Planner ---------- R. Wu: Commander M. Uzzo Command file: 02.01.30.14:34:01.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: 2002.01.30.16:21 end: 2002.01.31.02:20 ONUMs = 17080 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 262 degrees (922) - 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: q02.01.30.16:20:17.lya.dat q02.01.30.16:20:17.ovi.dat q02.01.30.16:20:17.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: 2002.01.31.02:24 end: 2002.01.31.05:50 ONUMs = 37621 (9 exps) 37622 (9 exps) 37623 (8 exps) 37624 (9 exps) 37625 (9 exps) 37626 (9 exps) 37627 (9 exps) 37628 (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: z02.01.31.02:22:58.lya.dat z02.01.31.02:22:58.ovi.dat z02.01.31.02:22:58.vld.dat z02.01.31.02:49:26.lya.dat z02.01.31.02:49:26.ovi.dat z02.01.31.02:49:26.vld.dat z02.01.31.03:15:55.lya.dat z02.01.31.03:15:55.ovi.dat z02.01.31.03:15:55.vld.dat z02.01.31.03:42:23.lya.dat z02.01.31.03:42:23.ovi.dat z02.01.31.03:42:23.vld.dat z02.01.31.04:08:52.lya.dat z02.01.31.04:08:52.ovi.dat z02.01.31.04:08:52.vld.dat z02.01.31.04:35:21.lya.dat z02.01.31.04:35:21.ovi.dat z02.01.31.04:35:21.vld.dat z02.01.31.05:01:57.lya.dat z02.01.31.05:01:57.ovi.dat z02.01.31.05:01:57.vld.dat GAP between 01/31/02|05:02:03( 9834) and 01/31/02|05:04:28(10065) z02.01.31.05:28:27.lya.dat z02.01.31.05:28:27.ovi.dat z02.01.31.05:28:27.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: 2002.01.31.06:23 end: 2002.01.31.16:22 ONUMs = 17081 (169 exps) Instrument configuration: - Pointing: Sun center - Roll: 262 degrees (922) - 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: q02.01.31.06:22:02.lya.dat q02.01.31.06:22:02.ovi.dat q02.01.31.06:22:02.vld.dat