UVCS MISSION LOG ---------------- Date: 12 February 2001 ----- Last revision: 24 February 2001 (Wu) -------------- File Name: 2001.02.12.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load & Run mid-latitude coronal hole for -------------- 02/12/01-02/13/01 Load mid-latitude coronal hole for 02/13/01 Load Mini-Synoptic 02/13/01 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- M. Uzzo: Commander, Planner D. Phillips: Planner S. Mancuso Y.-K. Ko R. Wu Command file: 01.02.12.15:56:08.cmd.log Activity: --------- 1) Observation of Low-Latitude Coronal Hole Sequence: 01.01_hole1.tcl SCI_SPEC: Characterization of an Equatorial Coronal Hole. Goal is to measure the properties of a mid-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. 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: 2001.02.12.18:44 end: 2001.02.13.04:55 ONUMs = 15880 (27 exps) 15881 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 357.8, 359.1, 0.2 Degrees (18369, 18593, 18804) - 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: 175500 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_175500MPM in slot 1 Fits Files: q01.02.12.18:34:47.lya.dat q01.02.12.18:34:47.ovi.dat q01.02.12.18:34:47.vld.dat q01.02.12.22:41:05.lya.dat q01.02.12.22:41:05.ovi.dat q01.02.12.22:41:05.vld.dat 2) Observation of Low-Latitude Coronal Hole Sequence: 01.01_hole2.tcl SCI_SPEC: Characterization of an Equatorial Coronal Hole. Goal is to measure the properties of an equatorial 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. 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: 2001.02.13.04:56 end: 2001.02.13.14:47 ONUMs = 15882 (57 exps) Instrument configuration: - Pointing: Sun center - Roll: 1.1 Degrees (18954) - Mirror/Occulter: 2.8 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 175500 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_175500MPM in slot 1 Fits Files: q01.02.13.04:55:03.lya.dat q01.02.13.04:55:03.ovi.dat q01.02.13.04:55:03.vld.dat 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 205, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2001.02.13.14:58 end: 2001.02.13.18:25 ONUMs = 34335 (9 exps) 34336 (9 exps) 34337 (9 exps) 34338 (9 exps) 34339 (9 exps) 34340 (9 exps) 34341 (9 exps) 34342 (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: 175500 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_175500 in slot 2 Fits Files: z01.02.13.14:57:30.lya.dat z01.02.13.14:57:30.ovi.dat z01.02.13.14:57:30.vld.dat z01.02.13.15:23:55.lya.dat z01.02.13.15:23:55.ovi.dat z01.02.13.15:23:55.vld.dat z01.02.13.15:50:23.lya.dat z01.02.13.15:50:23.ovi.dat z01.02.13.15:50:23.vld.dat z01.02.13.16:16:52.lya.dat z01.02.13.16:16:52.ovi.dat z01.02.13.16:16:52.vld.dat GAP between 02/13/01|16:40:36( 8282) and 02/13/01|16:44:59( 8697) z01.02.13.16:43:29.lya.dat z01.02.13.16:43:29.ovi.dat z01.02.13.16:43:29.vld.dat z01.02.13.17:10:04.lya.dat z01.02.13.17:10:04.ovi.dat z01.02.13.17:10:04.vld.dat z01.02.13.17:36:33.lya.dat z01.02.13.17:36:33.ovi.dat z01.02.13.17:36:33.vld.dat z01.02.13.18:03:00.lya.dat z01.02.13.18:03:00.ovi.dat z01.02.13.18:03:00.vld.dat