UVCS MISSION LOG ---------------- Date: 11 May 2001 ----- Last revision: 14 May 2001 (Wu) -------------- File Name: 2001.05.11.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Load Mask & Embeded Routines -------------- Load & Run High-latitude Coronal Hole Study for 11 May - 12 May 2001 Load Mini Synoptic for 12 May 2001 Load & Run High-latitude Coronal Hole Study for 12 May - 13 May 2001 Load Mini Synoptic for 13 May 2001 Load & Run High-latitude Coronal Hole Study for 13 May - 14 May 2001 Load 14 hour Synoptic for 14 May 2001 Load JOP139 May 14 - 15 2001 SOHO Activity: -------------- EOF Staff: M.-P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner D. H. Phillips: Planner S. Mancuso Y.-K. Ko Command file: 01.05.11.12:46:36.cmd.log Activity: --------- 1) Observation of High-Latitude Coronal Hole Sequence: 01.05_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=0 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: 2001.05.11.19:14 end: 2001.05.12.05:24 ONUMs = 16152 (27 exps) 16153 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 17323, 17536, 17739 (352.093, 353.267, 354.381 deg) - 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: 170700 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170700MPM in slot 1 Fits Files: q01.05.11.19:03:48.lya.dat q01.05.11.19:03:48.ovi.dat q01.05.11.19:03:48.vld.dat q01.05.11.23:10:45.lya.dat q01.05.11.23:10:45.ovi.dat q01.05.11.23:10:45.vld.dat 2) Observation of High-Latitude Coronal Hole Sequence: 01.05_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=0 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: 2001.05.12.05:26 end: 2001.05.12.15:20 ONUMs = 16154 (6 exps) 16155 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 17323, 17739 (352.093, 354.381 deg) - 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: 170700 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170700MPM in slot 1 Fits Files: q01.05.12.05:24:45.lya.dat q01.05.12.05:24:45.ovi.dat q01.05.12.05:24:45.vld.dat q01.05.12.05:59:13.lya.dat q01.05.12.05:59:13.ovi.dat q01.05.12.05:59:13.vld.dat GAP between 05/12/01|11:19:58(11559) and 05/12/01|11:29:10(12442) 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: 2001.05.12.15:30 end: 2001.05.12.18:57 ONUMs = 35154 (9 exps) 35155 (9 exps) 35156 (9 exps) 35157 (9 exps) 35158 (9 exps) 35159 (9 exps) 35160 (9 exps) 35161 (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: 194500 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194500 in slot 2 Fits Files: z01.05.12.15:29:22.lya.dat z01.05.12.15:29:22.ovi.dat z01.05.12.15:29:22.vld.dat z01.05.12.15:55:49.lya.dat z01.05.12.15:55:49.ovi.dat z01.05.12.15:55:49.vld.dat z01.05.12.16:22:18.lya.dat z01.05.12.16:22:18.ovi.dat z01.05.12.16:22:18.vld.dat z01.05.12.16:49:01.lya.dat z01.05.12.16:49:01.ovi.dat z01.05.12.16:49:01.vld.dat z01.05.12.17:15:30.lya.dat z01.05.12.17:15:30.ovi.dat z01.05.12.17:15:30.vld.dat z01.05.12.17:41:59.lya.dat z01.05.12.17:41:59.ovi.dat z01.05.12.17:41:59.vld.dat z01.05.12.18:08:28.lya.dat z01.05.12.18:08:28.ovi.dat z01.05.12.18:08:28.vld.dat z01.05.12.18:34:48.lya.dat z01.05.12.18:34:48.ovi.dat z01.05.12.18:34:48.vld.dat