UVCS MISSION LOG ---------------- Date: 10 October 2002 ----- Last revision: 15 October 2002 (Wu) -------------- File Name: 2002.10.12.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Southern Coronal Hole Study for 12 - 13 October 2002 -------------- Southern Coronal Hole Study for 13 October 2002 Mini-Synoptic for 13 October 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 02.10.11.12:06:26.cmd.log Activity: --------- 1) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a high-latitude coronal hole. Goal is to measure the properties of a high-latitude 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=258 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: 2002.10.12.20:16 end: 2002.10.13.06:26 ONUMs = 18116 (27 exps) 18117 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 250.093, 251.267, 252.381 Degrees (64311, 64525, 64728) - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.10.12.20:12:35.lya.dat q02.10.12.20:12:35.ovi.dat q02.10.12.20:12:35.vld.dat q02.10.13.00:12:46.lya.dat q02.10.13.00:12:46.ovi.dat q02.10.13.00:12:46.vld.dat 2) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 02.06_hole5.tcl SCI_SPEC: Characterization of a high-latitude coronal hole. Goal is to measure the properties of a high-latitude 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=258 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: 2002.10.13.06:28 end: 2002.10.13.16:22 ONUMs = 18118 (6 exps) 18118 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 250.093, 252.381 Degrees (64311, 64728) - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.10.13.06:26:44.lya.dat q02.10.13.06:26:44.ovi.dat q02.10.13.06:26:44.vld.dat q02.10.13.07:01:14.lya.dat q02.10.13.07:01:14.ovi.dat q02.10.13.07:01:14.vld.dat 3) 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: 2002.10.13.16:56 end: 2002.10.13.20:23 ONUMs = 40070 (9 exps) 40071 (9 exps) 40072 (9 exps) 40073 (9 exps) 40074 (9 exps) 40075 (9 exps) 40076 (9 exps) 40077 (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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.10.13.16:55:53.lya.dat z02.10.13.16:55:53.ovi.dat z02.10.13.16:55:53.vld.dat z02.10.13.17:22:11.lya.dat z02.10.13.17:22:11.ovi.dat z02.10.13.17:22:11.vld.dat z02.10.13.17:48:48.lya.dat z02.10.13.17:48:48.ovi.dat z02.10.13.17:48:48.vld.dat z02.10.13.18:15:16.lya.dat z02.10.13.18:15:16.ovi.dat z02.10.13.18:15:16.vld.dat z02.10.13.18:41:45.lya.dat z02.10.13.18:41:45.ovi.dat z02.10.13.18:41:45.vld.dat z02.10.13.19:08:06.lya.dat z02.10.13.19:08:06.ovi.dat z02.10.13.19:08:06.vld.dat z02.10.13.19:34:43.lya.dat z02.10.13.19:34:43.ovi.dat z02.10.13.19:34:43.vld.dat z02.10.13.20:01:11.lya.dat z02.10.13.20:01:11.ovi.dat z02.10.13.20:01:11.vld.dat