UVCS MISSION LOG ---------------- Date: 22 January 2002 ----- Last revision: 29 January 2002 (Ko) -------------- File Name: 2002.01.22.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Active Region Streamer Study for 01/22/02 - 01/23/02 -------------- Load Mini Synoptic for 01/23/02 Load Active Region Streamer Study for 01/23/02 SOHO Activity: -------------- EOF Staff: John Raymond: Lead Scientist ---------- M. Uzzo: Planner, Commander R. Wu Command file: 02.01.22.14:49:49.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: 2002.01.22.20:03 end: 2002.01.23.06:03 ONUMs = 17070 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 275 degrees (3288) - 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: q02.01.22.20:02:28.lya.dat q02.01.22.20:02:28.ovi.dat q02.01.22.20:02:28.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: 2002.01.23.06:05 end: 2002.01.23.09:32 ONUMs = 37540 (9 exps) 37541 (9 exps) 37542 (9 exps) 37543 (8 exps) 37544 (9 exps) 37545 (9 exps) 37546 (9 exps) 37547 (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: z02.01.23.06:04:50.lya.dat z02.01.23.06:04:50.ovi.dat z02.01.23.06:04:50.vld.dat z02.01.23.06:31:16.lya.dat z02.01.23.06:31:16.ovi.dat z02.01.23.06:31:16.vld.dat z02.01.23.06:58:00.lya.dat z02.01.23.06:58:00.ovi.dat z02.01.23.06:58:00.vld.dat z02.01.23.07:24:43.lya.dat z02.01.23.07:24:43.ovi.dat z02.01.23.07:24:43.vld.dat z02.01.23.07:51:12.lya.dat z02.01.23.07:51:12.ovi.dat z02.01.23.07:51:12.vld.dat z02.01.23.08:17:41.lya.dat z02.01.23.08:17:41.ovi.dat z02.01.23.08:17:41.vld.dat z02.01.23.08:44:17.lya.dat z02.01.23.08:44:17.ovi.dat z02.01.23.08:44:17.vld.dat z02.01.23.09:10:47.lya.dat z02.01.23.09:10:47.ovi.dat z02.01.23.09:10:47.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: 2002.01.23.10:04 end: 2002.01.23.20:03 ONUMs = 17071 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 275 degrees (3288) - 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: q02.01.23.10:02:57.lya.dat q02.01.23.10:02:57.ovi.dat q02.01.23.10:02:57.vld.dat