UVCS MISSION LOG ---------------- Date: 16 December 2002 ----- Last revision: 17 December 2002 (Wu) -------------- File Name: 2002.12.16.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Southern Coronal Hole Study for 16 - 17 December 2002 -------------- Southern Coronal Hole Study for 17 December 2002 Mini-Synoptic for 17 December 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 02.12.16.14:40:06.cmd.log Activity: --------- 1) Observation of a Southern Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of a 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=158 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: 2002.12.16.18:19 end: 2002.12.17.04:29 ONUMs = 18346 (27 exps) 18347 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 150.093, 151.267, 152.381 Degrees (46107, 46320, 46523) - 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: q02.12.16.18:10:27.lya.dat q02.12.16.18:10:27.ovi.dat q02.12.16.18:10:27.vld.dat q02.12.16.22:15:27.lya.dat q02.12.16.22:15:27.ovi.dat q02.12.16.22:15:27.vld.dat 2) Observation of a Southern Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of a 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=158 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: 2002.12.17.04:31 end: 2002.12.17.14:24 ONUMs = 18348 (6 exps) 18349 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 150.093, 152.381 Degrees (46107, 46523) - 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: q02.12.17.04:29:30.lya.dat q02.12.17.04:29:30.ovi.dat q02.12.17.04:29:30.vld.dat q02.12.17.05:03:53.lya.dat q02.12.17.05:03:53.ovi.dat q02.12.17.05:03:53.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: 2002.12.17.14:49 end: 2002.12.17.18:16 ONUMs = 40730 (9 exps) 40731 (9 exps) 40732 (9 exps) 40733 (9 exps) 40734 (9 exps) 40735 (9 exps) 40736 (9 exps) 40737 (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: z02.12.17.14:48:51.lya.dat z02.12.17.14:48:51.ovi.dat z02.12.17.14:48:51.vld.dat z02.12.17.15:15:24.lya.dat z02.12.17.15:15:24.ovi.dat z02.12.17.15:15:24.vld.dat z02.12.17.15:42:12.lya.dat z02.12.17.15:42:12.ovi.dat z02.12.17.15:42:12.vld.dat z02.12.17.16:08:32.lya.dat z02.12.17.16:08:32.ovi.dat z02.12.17.16:08:32.vld.dat z02.12.17.16:35:09.lya.dat z02.12.17.16:35:09.ovi.dat z02.12.17.16:35:09.vld.dat z02.12.17.17:01:38.lya.dat z02.12.17.17:01:38.ovi.dat z02.12.17.17:01:38.vld.dat z02.12.17.17:28:07.lya.dat z02.12.17.17:28:07.ovi.dat z02.12.17.17:28:07.vld.dat z02.12.17.17:54:35.lya.dat z02.12.17.17:54:35.ovi.dat z02.12.17.17:54:35.vld.dat