UVCS MISSION LOG ---------------- Date: 20 March 2003 ----- Last revision: 22 March 2003 (Wu) -------------- File Name: 2003.03.21.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: High Latitude Coronal Hole Observation for -------------- 21 - 22 March 2003 Load High Latitude Coronal Hole Observation for 22 March 2003 Load High Latitude Coronal Hole Observation for 22 March 2003 Load Mini-Synoptic for 22 March 2003 Load High Latitude Coronal Hole Observation for 22 - 23 March 2003 Load High Latitude Coronal Hole Observation for 23 March 2003 Load Mini-Synoptic for 23 March 2003 Load High Latitude Coronal Hole Observation for 23 - 24 March 2003 Load Synoptic for 24 March 2003 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 03.03.20.17:08:40.cmd.log 03.03.21.17:03.00.cmd.log Activity: --------- 1) Observation of the High Latitude Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the southern coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=238 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: 2003.03.21.12:19 end: 2003.03.21.22:29 ONUMs = 18696 (27 exps) 18697 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 230.09, 231.27, 232.38 Degrees (60670, 60884, 61087) - 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: q03.03.21.12:17:19.lya.dat q03.03.21.12:17:19.ovi.dat q03.03.21.12:17:19.vld.dat q03.03.21.16:15:47.lya.dat q03.03.21.16:15:47.ovi.dat q03.03.21.16:15:47.vld.dat 2) Observation of the High Latitude Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of the southern coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=238 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: 2003.03.21.22:31 end: 2003.03.22.08:25 ONUMs = 18698 (6 exps) 18699 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 230.09, 232.38 Degrees (60670, 61087) - 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: q03.03.21.22:29:53.lya.dat q03.03.21.22:29:53.ovi.dat q03.03.21.22:29:53.vld.dat q03.03.21.23:04:28.lya.dat q03.03.21.23:04:28.ovi.dat q03.03.21.23:04:28.vld.dat GAP between 03/22/03|03:18:03(10734) and 03/22/03|03:19:51(10911) GAP between 03/22/03|04:00:03(14770) and 03/22/03|04:01:46(14934) 3) Observation of the High Latitude Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of the southern coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=238 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: 2003.03.22.08:27 end: 2003.03.22.14:11 ONUMs = 18700 (6 exps) 18701 (30 exps) Instrument configuration: - Pointing: Sun center - Roll: 230.09, 232.38 Degrees (60670, 61087) - 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: q03.03.22.08:25:11.lya.dat q03.03.22.08:25:11.ovi.dat q03.03.22.08:25:11.vld.dat q03.03.22.08:59:45.lya.dat q03.03.22.08:59:45.ovi.dat q03.03.22.08:59:45.vld.dat 4) 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: 2003.03.22.14:45 end: 2003.03.22.18:12 ONUMs = 41680 (9 exps) 41681 (9 exps) 41682 (9 exps) 41683 (9 exps) 41684 (9 exps) 41685 (9 exps) 41686 (9 exps) 41687 (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: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z03.03.22.14:44:37.lya.dat z03.03.22.14:44:37.ovi.dat z03.03.22.14:44:37.vld.dat z03.03.22.15:11:16.lya.dat z03.03.22.15:11:16.ovi.dat z03.03.22.15:11:16.vld.dat z03.03.22.15:37:45.lya.dat z03.03.22.15:37:45.ovi.dat z03.03.22.15:37:45.vld.dat z03.03.22.16:04:14.lya.dat z03.03.22.16:04:14.ovi.dat z03.03.22.16:04:14.vld.dat z03.03.22.16:30:43.lya.dat z03.03.22.16:30:43.ovi.dat z03.03.22.16:30:43.vld.dat z03.03.22.16:57:20.lya.dat z03.03.22.16:57:20.ovi.dat z03.03.22.16:57:20.vld.dat z03.03.22.17:23:55.lya.dat z03.03.22.17:23:55.ovi.dat z03.03.22.17:23:55.vld.dat z03.03.22.17:50:22.lya.dat z03.03.22.17:50:22.ovi.dat z03.03.22.17:50:22.vld.dat