UVCS MISSION LOG ---------------- Date: 07 October 2002 ----- Last revision: 09 October 2002 (Wu) -------------- File Name: 2002.10.07.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start Southern Coronal Hole Study for -------------- 07 - 08 October 2002 Load Southern Coronal Hole Study for 08 October 2002 Load Mini-Synoptic for 08 October 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 02.10.07.13:38:03.cmd.log Activity: --------- 1) Observation of the South Polar Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a south 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=185 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: 2002.10.07.17:13 end: 2002.10.08.03:23 ONUMs = 18102 (27 exps) 18103 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 177.093, 178.267, 179.381 Degrees (51022, 51236, 51438) - 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: q02.10.07.17:07:11.lya.dat q02.10.07.17:07:11.ovi.dat q02.10.07.17:07:11.vld.dat q02.10.07.21:09:33.lya.dat q02.10.07.21:09:33.ovi.dat q02.10.07.21:09:33.vld.dat 2) Observation of the South Polar Coronal Hole Sequence: 02.06_hole5.tcl SCI_SPEC: Characterization of a south 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=185 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: 2002.10.08.03:25 end: 2002.10.08.13:18 ONUMs = 18104 (6 exps) 18105 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 177.093, 179.381 Degrees (51022, 51438) - 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: q02.10.08.03:23:30.lya.dat q02.10.08.03:23:30.ovi.dat q02.10.08.03:23:30.vld.dat q02.10.08.03:58:02.lya.dat q02.10.08.03:58:02.ovi.dat q02.10.08.03:58:02.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: 2002.10.08.13:46 end: 2002.10.08.17:13 ONUMs = 40020 (9 exps) 40021 (9 exps) 40022 (6 exps) 40023 (9 exps) 40024 (9 exps) 40025 (9 exps) 40026 (9 exps) 40027 (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: z02.10.08.13:45:35.lya.dat z02.10.08.13:45:35.ovi.dat z02.10.08.13:45:35.vld.dat z02.10.08.14:12:21.lya.dat z02.10.08.14:12:21.ovi.dat z02.10.08.14:12:21.vld.dat z02.10.08.14:39:00.lya.dat z02.10.08.14:39:00.ovi.dat z02.10.08.14:39:00.vld.dat z02.10.08.15:05:33.lya.dat z02.10.08.15:05:33.ovi.dat z02.10.08.15:05:33.vld.dat z02.10.08.15:32:02.lya.dat z02.10.08.15:32:02.ovi.dat z02.10.08.15:32:02.vld.dat z02.10.08.15:58:38.lya.dat z02.10.08.15:58:38.ovi.dat z02.10.08.15:58:38.vld.dat z02.10.08.16:25:14.lya.dat z02.10.08.16:25:14.ovi.dat z02.10.08.16:25:14.vld.dat z02.10.08.16:51:41.lya.dat z02.10.08.16:51:41.ovi.dat z02.10.08.16:51:41.vld.dat