UVCS MISSION LOG ---------------- Date: 01 October 2002 ----- Last revision: 02 October 2002 (Wu) -------------- File Name: 2002.10.01.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Southern Coronal Hole Study for -------------- 01 - 02 October 2002 Load Southern Coronal Hole Study for 02 October 2002 Load Mini-Synoptic for 02 October 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 02.09.30.14:43:00.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=130 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: 2002.10.01.17:40 end: 2002.10.02.03:50 ONUMs = 18084 (27 exps) 18085 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 122.093, 123.267, 124.381 Degrees (40998, 41212, 41415) - 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: q02.10.01.17:29:02.lya.dat q02.10.01.17:29:02.ovi.dat q02.10.01.17:29:02.vld.dat q02.10.01.21:36:34.lya.dat q02.10.01.21:36:34.ovi.dat q02.10.01.21:36:34.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=130 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: 2002.10.02.03:52 end: 2002.10.02.13:46 ONUMs = 18086 (6 exps) 18087 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 122.093, 124.381 Degrees (40998, 41415) - 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: q02.10.02.03:50:44.lya.dat q02.10.02.03:50:44.ovi.dat q02.10.02.03:50:44.vld.dat q02.10.02.04:25:16.lya.dat q02.10.02.04:25:16.ovi.dat q02.10.02.04:25:16.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: 2002.10.02.14:09 end: 2002.10.02.17:37 ONUMs = 39960 (9 exps) 39961 (9 exps) 39962 (9 exps) 39963 (9 exps) 39964 (9 exps) 39965 (9 exps) 39966 (9 exps) 39967 (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: z02.10.02.14:08:51.lya.dat z02.10.02.14:08:51.ovi.dat z02.10.02.14:08:51.vld.dat z02.10.02.14:35:20.lya.dat z02.10.02.14:35:20.ovi.dat z02.10.02.14:35:20.vld.dat z02.10.02.15:02:04.lya.dat z02.10.02.15:02:04.ovi.dat z02.10.02.15:02:04.vld.dat z02.10.02.15:28:47.lya.dat z02.10.02.15:28:47.ovi.dat z02.10.02.15:28:47.vld.dat z02.10.02.15:55:16.lya.dat z02.10.02.15:55:16.ovi.dat z02.10.02.15:55:16.vld.dat z02.10.02.16:21:45.lya.dat z02.10.02.16:21:45.ovi.dat z02.10.02.16:21:45.vld.dat z02.10.02.16:48:21.lya.dat z02.10.02.16:48:21.ovi.dat z02.10.02.16:48:21.vld.dat z02.10.02.17:14:55.lya.dat z02.10.02.17:14:55.ovi.dat z02.10.02.17:14:55.vld.dat