UVCS MISSION LOG ---------------- Date: 09 May 2001 ----- Last revision: 10 May 2001 (Ko) -------------- File Name: 2001.05.09.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Load & Run High-latitude Coronal Hole Study for -------------- 9 May - 10 May 2001 Load Mini Synoptic for 10 May 2001 Load High-latitude Coronal Hole Study for 10 May - 11 May 2001 Load Mini Synoptic for 11 May 2001 SOHO Activity: -------------- EOF Staff: M.-P. Miralles: Lead Scientist ---------- Y.-K. Ko: D. H. Phillips: Planner S. Mancuso M. Uzzo: Commander, Planner Command file: 01.05.09.13:10:24.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: 2001.05.09.18:31 end: 2001.05.10.04:41 ONUMs = 16144 (27 exps) 16145 (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: q01.05.09.18:20:46.lya.dat q01.05.09.18:20:46.ovi.dat q01.05.09.18:20:46.vld.dat q01.05.09.22:27:47.lya.dat q01.05.09.22:27:47.ovi.dat q01.05.09.22:27:47.vld.dat GAP between 05/09/01|23:37:14(11408) and 05/09/01|23:38:51(11573) 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: 2001.05.10.04:43 end: 2001.05.10.14:37 ONUMs = 16146 (6 exps) 16147 (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: q01.05.10.04:41:47.lya.dat q01.05.10.04:41:47.ovi.dat q01.05.10.04:41:47.vld.dat q01.05.10.05:16:15.lya.dat q01.05.10.05:16:15.ovi.dat q01.05.10.05:16:15.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: 2001.05.10.14:47 end: 2001.05.10.18:14 ONUMs = 35138 (9 exps) 35139 (9 exps) 35140 (9 exps) 35141 (9 exps) 35142 (9 exps) 35143 (9 exps) 35144 (9 exps) 35145 (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: z01.05.10.14:46:26.lya.dat z01.05.10.14:46:26.ovi.dat z01.05.10.14:46:26.vld.dat z01.05.10.15:12:51.lya.dat z01.05.10.15:12:51.ovi.dat z01.05.10.15:12:51.vld.dat z01.05.10.15:39:20.lya.dat z01.05.10.15:39:20.ovi.dat z01.05.10.15:39:20.vld.dat z01.05.10.16:05:55.lya.dat z01.05.10.16:05:55.ovi.dat z01.05.10.16:05:55.vld.dat z01.05.10.16:32:26.lya.dat z01.05.10.16:32:26.ovi.dat z01.05.10.16:32:26.vld.dat z01.05.10.16:59:01.lya.dat z01.05.10.16:59:01.ovi.dat z01.05.10.16:59:01.vld.dat z01.05.10.17:25:30.lya.dat z01.05.10.17:25:30.ovi.dat z01.05.10.17:25:30.vld.dat z01.05.10.17:52:06.lya.dat z01.05.10.17:52:06.ovi.dat z01.05.10.17:52:06.vld.dat