UVCS MISSION LOG ---------------- Date: 04 January 2002 ----- Last revision: 05 January 2002 (Ko) -------------- File Name: 2002.01.03.a.log ----------- Compiled by: M. Uzzo, Y.-K. Ko ------------ UVCS Activity: Active Region Streamer Study -------------- for 01/03/02 - 01/04/02 Mini Synoptic for 01/04/02 Active Region Streamer Study for 01/04/02 SOHO Activity: -------------- EOF Staff: Y.-K. Ko: Lead Scientist / Planner ---------- M. Uzzo: Commander / Planner D. Phillips Command file: 02.01.02.14:15:58.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: 2002.01.03.16:06 end: 2002.01.04.02:05 ONUMs = 17011 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 77 degrees (32789) - 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: q02.01.03.16:04:36.lya.dat q02.01.03.16:04:36.ovi.dat q02.01.03.16:04:36.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: 2002.01.04.02:23 end: 2002.01.04.05:50 ONUMs = 37391 (9 exps) 37392 (9 exps) 37393 (9 exps) 37394 (9 exps) 37395 (9 exps) 37396 (9 exps) 37397 (9 exps) 37398 (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: z02.01.04.02:22:19.lya.dat z02.01.04.02:22:19.ovi.dat z02.01.04.02:22:19.vld.dat z02.01.04.02:48:50.lya.dat z02.01.04.02:48:50.ovi.dat z02.01.04.02:48:50.vld.dat z02.01.04.03:15:33.lya.dat z02.01.04.03:15:33.ovi.dat z02.01.04.03:15:33.vld.dat z02.01.04.03:42:17.lya.dat z02.01.04.03:42:17.ovi.dat z02.01.04.03:42:17.vld.dat z02.01.04.04:08:46.lya.dat z02.01.04.04:08:46.ovi.dat z02.01.04.04:08:46.vld.dat z02.01.04.04:35:15.lya.dat z02.01.04.04:35:15.ovi.dat z02.01.04.04:35:15.vld.dat z02.01.04.05:01:52.lya.dat z02.01.04.05:01:52.ovi.dat z02.01.04.05:01:52.vld.dat z02.01.04.05:28:25.lya.dat z02.01.04.05:28:25.ovi.dat z02.01.04.05:28:25.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: 2002.01.04.06:09 end: 2002.01.04.16:08 ONUMs = 17012 (170 exps) Instrument configuration: - Pointing: Sun center - Roll: 77 degrees (32789) - 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: q02.01.04.06:08:06.lya.dat q02.01.04.06:08:06.ovi.dat q02.01.04.06:08:06.vld.dat