UVCS MISSION LOG ---------------- Date: 22 January 2002 ----- Last revision: 24 January 2002 (Wu) -------------- File Name: 2002.01.23.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Active Region Streamer Study for 01/23/02 - 01/24/02 -------------- Load Mini Synoptic for 01/24/02 Load Active Region Streamer Study for 01/24/02 Load 21 hour synoptics for 01/24/02 - 01/25/02 SOHO Activity: -------------- EOF Staff: John Raymond: Lead Scientist ---------- M. Uzzo: Planner, Commander R. Wu Command file: 02.01.23.13:55:33.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: 2002.01.23.20:04 end: 2002.01.24.06:03 ONUMs = 17072 (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: q02.01.23.20:03:08.lya.dat q02.01.23.20:03:08.ovi.dat q02.01.23.20:03:08.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: 2002.01.24.06:06 end: 2002.01.24.09:33 ONUMs = 37550 (9 exps) 37551 (9 exps) 37552 (9 exps) 37553 (9 exps) 37554 (7 exps) 37555 (9 exps) 37556 (9 exps) 37557 (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: z02.01.24.06:05:16.lya.dat z02.01.24.06:05:16.ovi.dat z02.01.24.06:05:16.vld.dat z02.01.24.06:31:53.lya.dat z02.01.24.06:31:53.ovi.dat z02.01.24.06:31:53.vld.dat z02.01.24.06:58:22.lya.dat z02.01.24.06:58:22.ovi.dat z02.01.24.06:58:22.vld.dat z02.01.24.07:24:51.lya.dat z02.01.24.07:24:51.ovi.dat z02.01.24.07:24:51.vld.dat z02.01.24.07:51:28.lya.dat z02.01.24.07:51:28.ovi.dat z02.01.24.07:51:28.vld.dat z02.01.24.08:18:03.lya.dat z02.01.24.08:18:03.ovi.dat z02.01.24.08:18:03.vld.dat z02.01.24.08:44:32.lya.dat z02.01.24.08:44:32.ovi.dat z02.01.24.08:44:32.vld.dat z02.01.24.09:10:59.lya.dat z02.01.24.09:10:59.ovi.dat z02.01.24.09:10:59.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: 2002.01.24.10:04 end: 2002.01.24.20:03 ONUMs = 17073 (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: q02.01.24.10:03:09.lya.dat q02.01.24.10:03:09.ovi.dat q02.01.24.10:03:09.vld.dat