UVCS MISSION LOG ---------------- Date: 05 January 2002 ----- Last revision: 07 January 2002 (MU) -------------- File Name: 2002.01.05.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load mask Comet_192 in slot 5 -------------- load mask OVI_184_red1pxl in slot 6 Load Active Region Streamer Study for 01/05/02 - 01/06/02 Load Mini Synoptic for 01/06/02 Load Active Region Streamer Study for 01/06/02 Load 21 hour synoptics for 01/06/02 - 01/07/02 Load Comet Machholz Background Study for 01/07/02 SOHO Activity: -------------- EOF Staff: Y.-K. Ko: Lead Scientist, Planner, Commander ---------- M. Uzzo Command file: 02.01.05.21:33:22.cmd.log Activity: --------- 1) Active Region Streamer Study Sequence: 01.12_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 CMP_NUM: 6839 Duration: start: 2002.01.05.22:16 end: 2002.01.06.08:15 ONUMs = 17014 (170 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, 236700 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: msk_000303_OVI in slot 3 Fits Files: q02.01.05.22:15:32.lya.dat.Z q02.01.05.22:15:32.ovi.dat.Z q02.01.05.22:15:32.vld.dat.Z 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: 2002.01.06.08:17 end: 2002.01.06.11:44 ONUMs = 37410 (9 exps) 37411 (9 exps) 37412 (9 exps) 37413 (9 exps) 37414 (9 exps) 37415 (9 exps) 37416 (9 exps) 37417 (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: z02.01.06.08:17:25.lya.dat z02.01.06.08:17:25.ovi.dat z02.01.06.08:17:25.vld.dat z02.01.06.08:44:03.lya.dat z02.01.06.08:44:03.ovi.dat z02.01.06.08:44:03.vld.dat z02.01.06.09:10:32.lya.dat z02.01.06.09:10:32.ovi.dat z02.01.06.09:10:32.vld.dat z02.01.06.09:37:15.lya.dat z02.01.06.09:37:15.ovi.dat z02.01.06.09:37:15.vld.dat z02.01.06.10:03:44.lya.dat z02.01.06.10:03:44.ovi.dat z02.01.06.10:03:44.vld.dat z02.01.06.10:30:13.lya.dat z02.01.06.10:30:13.ovi.dat z02.01.06.10:30:13.vld.dat z02.01.06.10:56:42.lya.dat z02.01.06.10:56:42.ovi.dat z02.01.06.10:56:42.vld.dat z02.01.06.11:23:17.lya.dat z02.01.06.11:23:17.ovi.dat z02.01.06.11:23:17.vld.dat 3) Active Region Streamer Study Sequence: 01.12_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 CMP_NUM: 6839 Duration: start: 2002.01.06.12:16 end: 2002.01.06.22:16 ONUMs = 17015 (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, 236700 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: msk_000303_OVI in slot 3 Fits Files: q02.01.06.12:16:00.lya.dat.Z q02.01.06.12:16:00.ovi.dat.Z q02.01.06.12:16:00.vld.dat.Z