UVCS MISSION LOG ---------------- Date: 01 February 2002 ----- Last revision: 04 February 2002 (Wu) -------------- File Name: 2002.02.02.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Active Region Streamer Study for 02 - 03 February 2002 -------------- Mini Synoptic for 03 February 2002 Active Region Streamer Study for 03 February 2002 SOHO Activity: -------------- EOF Staff: Y.-K. Ko: Lead Scientist, Planner ---------- R. Wu: Commander M. Uzzo Command file: 02.02.01.19:12:01.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: 2002.02.02.13:28 end: 2002.02.02.23:27 ONUMs = 17084 (169 exps) Instrument configuration: - Pointing: Sun center - Roll: 270 degrees (2378) - 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: q02.02.02.13:26:47.lya.dat q02.02.02.13:26:47.ovi.dat q02.02.02.13:26:47.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: 2002.02.02.23:31 end: 2002.02.03.02:56 ONUMs = 37640 (8 exps) 37641 (9 exps) 37642 (9 exps) 37643 (9 exps) 37644 (9 exps) 37645 (9 exps) 37646 (9 exps) 37647 (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: z02.02.02.23:28:28.lya.dat z02.02.02.23:28:28.ovi.dat z02.02.02.23:28:28.vld.dat z02.02.02.23:55:11.lya.dat z02.02.02.23:55:11.ovi.dat z02.02.02.23:55:11.vld.dat z02.02.03.00:21:40.lya.dat z02.02.03.00:21:40.ovi.dat z02.02.03.00:21:40.vld.dat z02.02.03.00:48:09.lya.dat z02.02.03.00:48:09.ovi.dat z02.02.03.00:48:09.vld.dat z02.02.03.01:14:53.lya.dat z02.02.03.01:14:53.ovi.dat z02.02.03.01:14:53.vld.dat z02.02.03.01:41:36.lya.dat z02.02.03.01:41:36.ovi.dat z02.02.03.01:41:36.vld.dat z02.02.03.02:08:05.lya.dat z02.02.03.02:08:05.ovi.dat z02.02.03.02:08:05.vld.dat z02.02.03.02:34:32.lya.dat z02.02.03.02:34:32.ovi.dat z02.02.03.02:34:32.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: 2002.02.03.03:28 end: 2002.02.03.13:27 ONUMs = 17085 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 270 degrees (2378) - 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: q02.02.03.03:27:31.lya.dat q02.02.03.03:27:31.ovi.dat q02.02.03.03:27:31.vld.dat