UVCS MISSION LOG ---------------- Date: 01 November 2002 ----- Last revision: 05 November 2002 (Wu) -------------- File Name: 2002.11.04.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Southern Coronal Hole Study for 04 - 05 November 2002 -------------- Southern Coronal Hole Study for 05 November 2002 Mini-Synoptic for 05 November 2002 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- Y.-K. Ko: Planner M. Uzzo: Commander R. Wu Command file: 02.11.01.13:30:47.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: 2002.11.04.15:23 end: 2002.11.05.01:33 ONUMs = 18205 (27 exps) 18206 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 177.09, 178.27, 179.38 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 6 Fits Files: q02.11.04.15:16:54.lya.dat q02.11.04.15:16:54.ovi.dat q02.11.04.15:16:54.vld.dat q02.11.04.19:19:21.lya.dat q02.11.04.19:19:21.ovi.dat q02.11.04.19:19:21.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: 2002.11.05.01:35 end: 2002.11.05.11:28 ONUMs = 18207 (6 exps) 18208 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 177.09, 179.38 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 6 Fits Files: q02.11.05.01:33:15.lya.dat q02.11.05.01:33:15.ovi.dat q02.11.05.01:33:15.vld.dat q02.11.05.02:07:49.lya.dat q02.11.05.02:07:49.ovi.dat q02.11.05.02:07:49.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: 2002.11.05.11:56 end: 2002.11.05:15:23 ONUMs = 40300 (9 exps) 40301 (9 exps) 40302 (9 exps) 40303 (9 exps) 40304 (9 exps) 40305 (8 exps) 40306 (9 exps) 40307 (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: z02.11.05.11:55:23.lya.dat z02.11.05.11:55:23.ovi.dat z02.11.05.11:55:23.vld.dat z02.11.05.12:22:09.lya.dat z02.11.05.12:22:09.ovi.dat z02.11.05.12:22:09.vld.dat z02.11.05.12:48:38.lya.dat z02.11.05.12:48:38.ovi.dat z02.11.05.12:48:38.vld.dat z02.11.05.13:15:07.lya.dat z02.11.05.13:15:07.ovi.dat z02.11.05.13:15:07.vld.dat z02.11.05.13:41:50.lya.dat z02.11.05.13:41:50.ovi.dat z02.11.05.13:41:50.vld.dat z02.11.05.14:08:34.lya.dat z02.11.05.14:08:34.ovi.dat z02.11.05.14:08:34.vld.dat z02.11.05.14:35:03.lya.dat z02.11.05.14:35:03.ovi.dat z02.11.05.14:35:03.vld.dat GAP between 11/05/02|14:14:13(10835) and 11/05/02|14:16:43(11073) GAP between 11/05/02|14:58:30(15093) and 11/05/02|15:01:47(15407) z02.11.05.15:01:30.lya.dat z02.11.05.15:01:30.ovi.dat z02.11.05.15:01:30.vld.dat