UVCS MISSION LOG ---------------- Date: 10 January 2002 ----- Last revision: 14 January 2002 (Wu) -------------- File Name: 2002.01.10.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load Active Region Streamer Study for 01/10/02 - 01/11/02 -------------- Load Mini Synoptic for 01/11/02 Load Active Region Streamer Study for 01/11/02 SOHO Activity: -------------- EOF Staff: Y.-K. Ko: Lead Scientist, Planner, Commander ---------- M. Uzzo: Commander Command file: 02.01.10.17:04:42.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: 6839 Duration: start: 2002.01.10.17:48 end: 2002.01.11.03:47 ONUMs = 17037 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 78 degrees (32971) - 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: q02.01.10.17:47:03.lya.dat q02.01.10.17:47:03.ovi.dat q02.01.10.17:47:03.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: 2002.01.11.04:06 end: 2002.01.11.07:33 ONUMs = 37450 (9 exps) 37451 (9 exps) 37452 (9 exps) 37453 (9 exps) 37454 (9 exps) 37455 (9 exps) 37456 (9 exps) 37457 (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: z02.01.11.04:05:39.lya.dat z02.01.11.04:05:39.ovi.dat z02.01.11.04:05:39.vld.dat z02.01.11.04:32:03.lya.dat z02.01.11.04:32:03.ovi.dat z02.01.11.04:32:03.vld.dat z02.01.11.04:58:36.lya.dat z02.01.11.04:58:36.ovi.dat z02.01.11.04:58:36.vld.dat z02.01.11.05:25:13.lya.dat z02.01.11.05:25:13.ovi.dat z02.01.11.05:25:13.vld.dat z02.01.11.05:51:48.lya.dat z02.01.11.05:51:48.ovi.dat z02.01.11.05:51:48.vld.dat z02.01.11.06:18:17.lya.dat z02.01.11.06:18:17.ovi.dat z02.01.11.06:18:17.vld.dat z02.01.11.06:44:46.lya.dat z02.01.11.06:44:46.ovi.dat z02.01.11.06:44:46.vld.dat z02.01.11.07:11:21.lya.dat z02.01.11.07:11:21.ovi.dat z02.01.11.07:11:21.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: 6839 Duration: start: 2002.01.11.07:49 end: 2002.01.11.17:48 ONUMs = 17038 (169 exps) Instrument configuration: - Pointing: Sun center - Roll: 78 degrees (32971) - 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: q02.01.11.07:48:11.lya.dat q02.01.11.07:48:11.ovi.dat q02.01.11.07:48:11.vld.dat