UVCS MISSION LOG ---------------- Date: 23 December 2003 ----- Last revision: 28 December 2003 (Wu) -------------- File Name: 2003.12.24.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: North Coronal Hole Observations for ------------- 24 - 25 December 2003 Load North Coronal Hole Observations for 25 December 2003 Load Mini-Synoptic for 25 December 2003 Load North Coronal Hole Observations for 25 - 26 December 2003 Load Synoptic for 26 December 2003 Load North Coronal Hole Observations for 26 - 27 December 2003 via Background Queue (to be uplinked between 10:00 and 11:00 UT 26 December 2003) Load North Coronal Hole Observations for 27 December 2003 using Batch Queue Time Tagged Commands via Background Queue (to be uplinked between 10:00 and 11:00 UT 26 December 2003) Load North Coronal Hole Observations for 27 - 28 December 2003 using Batch Queue Queue Time Tagged Commands via Background Queue (to be uplinked between 10:00 and 11:00 UT 26 December 2003) Load North Coronal Hole Observations for 28 December 2003 using Batch Queue Time Tagged Commands via Background Queue (to be uplinked between 10:00 and 11:00 UT 26 December 2003) Load North Coronal Hole Observations for 28 December 2003 using Batch Queue Time Tagged Commands via Background Queue (to be uplinked between 10:00 and 11:00 UT 26 December 2003) Load Mini-Synoptic for 29 December 2003 using Batch Queue Time Tagged Commands via Background Queue (to be uplinked between 10:00 and 11:00 UT 26 December 2003) SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner D. H. Phillips: Planner M. Uzzo Command file: 03.12.23.16:37:00.cmd.log 03.12.24.17:15:00.cmd.log Activity: --------- 1) Observation of the North Coronal Hole Sequence: 03.10_hole1.tcl SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=357 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2003.12.24.17:00 end: 2003.12:25.03:08 ONUMs = 20682 (105 exps) 20683 (163 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 349.093, 350.267, 351.381 degrees (16776, 16990, 17193) - Mirror/Occulter: 1.7, 2.0, 2.4 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 5 Fits Files: q03.12.24.16:47:57.lya.dat q03.12.24.16:47:57.ovi.dat q03.12.24.16:47:57.vld.dat q03.12.24.20:55:05.lya.dat q03.12.24.20:55:05.ovi.dat q03.12.24.20:55:05.vld.dat GAP between 12/25/03|00:46:45( 4285) and 12/25/03|00:59:43( 5531) 2) Observation of the North Coronal Hole Sequence: 03.10_hole5.tcl SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=357 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2003.12.25.03:10 end: 2003.12:25.13:01 ONUMs = 20684 (14 exps) 20685 (132 exps) 20686 (120 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 349.093, 351.381 degrees (16776, 17193) - Mirror/Occulter: 1.7, 2.4 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 5 Fits Files: q03.12.25.03:08:36.lya.dat q03.12.25.03:08:36.ovi.dat q03.12.25.03:08:36.vld.dat q03.12.25.03:42:43.lya.dat q03.12.25.03:42:43.ovi.dat q03.12.25.03:42:43.vld.dat q03.12.25.08:35:33.lya.dat q03.12.25.08:35:33.ovi.dat q03.12.25.08:35:33.vld.dat 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 215, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2003.12.25.13:11 end: 2003.12.25.16:39 ONUMs = 44160 (9 exps) 44161 (9 exps) 44162 (9 exps) 44163 (9 exps) 44164 (9 exps) 44165 (9 exps) 44166 (9 exps) 44167 (9 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - 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: z03.12.25.13:11:14.lya.dat z03.12.25.13:11:14.ovi.dat z03.12.25.13:11:14.vld.dat z03.12.25.13:37:35.lya.dat z03.12.25.13:37:35.ovi.dat z03.12.25.13:37:35.vld.dat z03.12.25.14:04:12.lya.dat z03.12.25.14:04:12.ovi.dat z03.12.25.14:04:12.vld.dat z03.12.25.14:30:41.lya.dat z03.12.25.14:30:41.ovi.dat z03.12.25.14:30:41.vld.dat z03.12.25.14:57:09.lya.dat z03.12.25.14:57:09.ovi.dat z03.12.25.14:57:09.vld.dat z03.12.25.15:23:38.lya.dat z03.12.25.15:23:38.ovi.dat z03.12.25.15:23:38.vld.dat z03.12.25.15:50:07.lya.dat z03.12.25.15:50:07.ovi.dat z03.12.25.15:50:07.vld.dat z03.12.25.16:16:49.lya.dat z03.12.25.16:16:49.ovi.dat z03.12.25.16:16:49.vld.dat