UVCS MISSION LOG ---------------- Date: 25 January 2002 ----- Last revision: 28 January 2002 (Wu) -------------- File Name: 2002.01.26.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Active Region Streamer Study for 01/26/02 - 01/27/02 -------------- Mini Synoptic for 01/27/02 Active Region Streamer Study for 01/27/02 SOHO Activity: -------------- EOF Staff: John Raymond: Lead Scientist ---------- M. Uzzo: Planner, Commander R. Wu Command file: 02.01.25.13:42:02.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: 2002.01.26.16:53 end: 2002.01.27.02:52 ONUMs = 17076 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 110 degrees (38797) - 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: q02.01.26.16:52:24.lya.dat q02.01.26.16:52:24.ovi.dat q02.01.26.16:52:24.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: 2002.01.27.03:16 end: 2002.01.27.06:40 ONUMs = 37580 (8 exps) 37581 (9 exps) 37582 (9 exps) 37583 (9 exps) 37584 (9 exps) 37585 (9 exps) 37586 (9 exps) 37587 (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: z02.01.27.03:12:59.lya.dat z02.01.27.03:12:59.ovi.dat z02.01.27.03:12:59.vld.dat z02.01.27.03:39:24.lya.dat z02.01.27.03:39:24.ovi.dat z02.01.27.03:39:24.vld.dat z02.01.27.04:05:52.lya.dat z02.01.27.04:05:52.ovi.dat z02.01.27.04:05:52.vld.dat z02.01.27.04:32:21.lya.dat z02.01.27.04:32:21.ovi.dat z02.01.27.04:32:21.vld.dat z02.01.27.04:58:42.lya.dat z02.01.27.04:58:42.ovi.dat z02.01.27.04:58:42.vld.dat z02.01.27.05:25:19.lya.dat z02.01.27.05:25:19.ovi.dat z02.01.27.05:25:19.vld.dat z02.01.27.05:51:47.lya.dat z02.01.27.05:51:47.ovi.dat z02.01.27.05:51:47.vld.dat z02.01.27.06:18:14.lya.dat z02.01.27.06:18:14.ovi.dat z02.01.27.06:18:14.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: 2002.01.27.06:53 end: 2002.01.27.16:52 ONUMs = 17077 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 110 degrees (38797) - 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: q02.01.27.06:51:45.lya.dat q02.01.27.06:51:45.ovi.dat q02.01.27.06:51:45.vld.dat