UVCS MISSION LOG ---------------- Date: 29 November 2002 ----- Last revision: 04 December 2002 (Wu) -------------- File Name: 2002.12.02.a.log ----------- Compiled by: Y.-K. Ko, R. Wu ------------ UVCS Activity: 1st two Position Angles of Synoptic for -------------- 02 - 03 December 2002 Load and Start remaining six Position Angles of Synoptic for 02 - 03 December 2002 Load Eclipse Campaign Support Southern Coronal Hole Study for 03 December 2002 SOHO Activity: Change SOHO Telemetry Submode to 6 -------------- EOF Staff: G. Poletto / J. Kohl: Lead Scientist ---------- Y.-K. Ko: Commander, Planner R. Wu: Commander M. Uzzo / D. H. Phillips: Planner Command file: 02.11.29.15:42:46.cmd.log 02.12.02.20:04:00.cmd.log Activity: --------- 1) Synoptic Sequence Load and Start Sequence: SynopticA:Start 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: 2002.12.02.16:56 end: 2002.12.03.05:34 ONUMs = 40580 (37 exps) 40581 (37 exps) 40582 (37 exps) 40583 (37 exps) 40584 (37 exps) 40585 (37 exps) 40586 (37 exps) 40587 (37 exps) Instrument configuration: - Pointing: Sun center - Roll: W: STR2B, NW: STR2B, N: STR2B, NE: STR2B, E: STR2B, SE: STR2B, S: STR2B, SW: STR2B - Mirror/Occulter: STR1A: 3.5, 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR2B: 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR3A: 3.5, 3.0 Ro STR4B: 4.0 Ro STR5A: 2.1, 1.9, 1.75, 1.6 Ro STR6B: 2.5 Ro STR7B: 3.0 Ro CH1A: 1.9, 1.75, 1.6 Ro CH2A: 2.1 Ro CH2B: 2.1 Ro CH3B: 2.5 Ro CH4A: 1.75, 1.6 Ro CH5B: 1.9 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75, 1.9, 2.1, 2.5, 3.0, 3.5, 4.0 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (STR1A, STR2B, STR3A, STR4B, CH1A, CH2A, CH2B, CH3B) 100 um (CH4A, CH5B) 75 um (STR5A, STR6B, STR7B) - LYA GRTPOS: 128000 - OVI GRTPOS: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z02.12.02.16:56:04.lya.dat z02.12.02.16:56:04.ovi.dat z02.12.02.16:56:04.vld.dat z02.12.02.18:30:42.lya.dat z02.12.02.18:30:42.ovi.dat z02.12.02.18:30:42.vld.dat z02.12.02.20:11:50.lya.dat z02.12.02.20:11:50.ovi.dat z02.12.02.20:11:50.vld.dat z02.12.02.21:46:04.lya.dat z02.12.02.21:46:04.ovi.dat z02.12.02.21:46:04.vld.dat z02.12.02.23:20:43.lya.dat z02.12.02.23:20:43.ovi.dat z02.12.02.23:20:43.vld.dat z02.12.03.00:54:55.lya.dat z02.12.03.00:54:55.ovi.dat z02.12.03.00:54:55.vld.dat z02.12.03.02:29:35.lya.dat z02.12.03.02:29:35.ovi.dat z02.12.03.02:29:35.vld.dat z02.12.03.04:04:13.lya.dat z02.12.03.04:04:13.ovi.dat z02.12.03.04:04:13.vld.dat 2) Eclipse Campaign Observation of the South Polar Coronal Hole Sequence: 02.12_hole_eclipse.tcl SCI_SPEC: The objective of the eclipse support during Dec 3-4, 2002 is intercalibration with eclipse instruments on the ground. Characterization of a south polar coronal hole and a streamer in the NW. Roll positions are VL-corrected for PA=198 degrees. OBS_PROG: Primary: Calibration Sub Obj: Sensitivity SCI_OBJ: Calibration...VLC Stray Light Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2002.12.03.05:40 end: 2002.12.03.17:07 ONUMs = 18294 (105 exps) 18295 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 190.316, 191.267, 192.009 Degrees (53429, 53602, 53737) - Mirror/Occulter: 1.75, 2.00, 2.25 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 1 Fits Files: q02.12.03.05:35:02.lya.dat q02.12.03.05:35:02.ovi.dat q02.12.03.05:35:02.vld.dat q02.12.03.12:09:50.lya.dat q02.12.03.12:09:50.ovi.dat q02.12.03.12:09:50.vld.dat