UVCS MISSION LOG ---------------- Date: 16 January 2002 ----- Last revision: 17 January 2002 (Wu) -------------- File Name: 2002.01.16.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start South Hemisphere Coronal -------------- Hole Study for 15 - 16 January 2002 Load South Hemisphere Coronal Hole Study for 17 January 2002 Load Mini Synoptic for 17 January 2002 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 02.01.16.16:32:50.cmd.log Activity: --------- 1) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 01.06_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=230 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: 2002.01.16.17:22 end: 2002.01.17.03:32 ONUMs = 17054 (27 exps) 17055 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 222.09, 223.27, 224.38 Degrees (59214, 59428, 59630) - 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_168MPM in slot 1 Fits Files: q02.01.16.17:20:28.lya.dat q02.01.16.17:20:28.ovi.dat q02.01.16.17:20:28.vld.dat GAP between 01/16/02|21:07:11( 9803) and 01/16/02|21:08:13( 9904) q02.01.16.21:18:38.lya.dat q02.01.16.21:18:38.ovi.dat q02.01.16.21:18:38.vld.dat 2) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 01.06_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=230 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: 2002.01.17.03:34 end: 2002.01.17.13:28 ONUMs = 17055 (6 exps) 17056 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 222.09, 224.38 Degrees (59214, 59630) - 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_168MPM in slot 1 Fits Files: q02.01.17.03:32:45.lya.dat q02.01.17.03:32:45.ovi.dat q02.01.17.03:32:45.vld.dat q02.01.17.04:07:19.lya.dat q02.01.17.04:07:19.ovi.dat q02.01.17.04:07:19.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: 2002.01.17.14:01 end: 2002.01.17.17:28 ONUMs = 37850 (9 exps) 37851 (9 exps) 37852 (8 exps) 37853 (9 exps) 37854 (9 exps) 37855 (9 exps) 37856 (9 exps) 37857 (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: 184200 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_184 in slot 2 Fits Files: z02.01.17.14:00:46.lya.dat z02.01.17.14:00:46.ovi.dat z02.01.17.14:00:46.vld.dat z02.01.17.14:27:24.lya.dat z02.01.17.14:27:24.ovi.dat z02.01.17.14:27:24.vld.dat z02.01.17.14:54:07.lya.dat z02.01.17.14:54:07.ovi.dat z02.01.17.14:54:07.vld.dat z02.01.17.15:20:36.lya.dat z02.01.17.15:20:36.ovi.dat z02.01.17.15:20:36.vld.dat z02.01.17.15:47:05.lya.dat z02.01.17.15:47:05.ovi.dat z02.01.17.15:47:05.vld.dat z02.01.17.16:13:34.lya.dat z02.01.17.16:13:34.ovi.dat z02.01.17.16:13:34.vld.dat z02.01.17.16:40:10.lya.dat z02.01.17.16:40:10.ovi.dat z02.01.17.16:40:10.vld.dat z02.01.17.17:06:40.lya.dat z02.01.17.17:06:40.ovi.dat z02.01.17.17:06:40.vld.dat