UVCS MISSION LOG ---------------- Date: 01 May 2001 ----- Last revision: 02 May 2001 (Mancuso) -------------- File Name: 2001.05.01.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load Mid-latitude Coronal Hole Study for -------------- 01 May - 02 May 2001 Load Mini Synoptic for 02 May 2001 SOHO Activity: -------------- EOF Staff: M.-P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner D. H. Phillips: Planner S. Mancuso M. Uzzo Command file: 01.05.01.15:55:36.cmd.log Activity: --------- 1) Observation of Mid-Latitude Coronal Hole Sequence: 01.01_hole1a.tcl SCI_SPEC: Characterization of a mid-latitude 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. Roll positions are VL-corrected for PA=208 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: 2001.05.01.21:03 end: 2001.05.02.07:17 ONUMs = 16122 (27 exps) 16123 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 55209, 55423, 55625 (200.093, 201.267, 202.381) - 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_168MPM in slot 1 Fits Files: q01.05.01.21:03:07.lya.dat q01.05.01.21:03:07.ovi.dat q01.05.01.21:03:07.vld.dat q01.05.02.01:03:25.lya.dat q01.05.02.01:03:25.ovi.dat q01.05.02.01:03:25.vld.dat GAP between 05/02/01|00:44:17( 8800) and 05/02/01|01:14:16(11683) 2) Observation of Mid-Latitude Coronal Hole Sequence: 01.04_hole5a.tcl SCI_SPEC: Characterization of a mid-latitude 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. Roll positions are VL-corrected for PA=208 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: 2001.05.02.07:17 end: 2001.05.02.17:41 ONUMs = 16124 (6 exps) 16125 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 55209, 55625 (200.093, 202.381) - 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_168MPM in slot 1 Fits Files: q01.05.02.07:17:19.lya.dat q01.05.02.07:17:19.ovi.dat q01.05.02.07:17:19.vld.dat q01.05.02.07:51:53.lya.dat q01.05.02.07:51:53.ovi.dat q01.05.02.07:51:53.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: 2001.05.02.17:41 end: 2001.05.02.21:10 ONUMs = 35060 (9 exps) 35061 (9 exps) 35062 (9 exps) 35063 (9 exps) 35064 (9 exps) 35065 (9 exps) 35066 (9 exps) 35067 (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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_CME_168 in slot 4 Fits Files: z01.05.02.17:41:43.lya.dat z01.05.02.17:41:43.ovi.dat z01.05.02.17:41:43.vld.dat z01.05.02.18:08:09.lya.dat z01.05.02.18:08:09.ovi.dat z01.05.02.18:08:09.vld.dat z01.05.02.18:34:42.lya.dat z01.05.02.18:34:42.ovi.dat z01.05.02.18:34:42.vld.dat z01.05.02.19:01:11.lya.dat z01.05.02.19:01:11.ovi.dat z01.05.02.19:01:11.vld.dat z01.05.02.19:27:47.lya.dat z01.05.02.19:27:47.ovi.dat z01.05.02.19:27:47.vld.dat z01.05.02.19:54:34.lya.dat z01.05.02.19:54:34.ovi.dat z01.05.02.19:54:34.vld.dat z01.05.02.20:21:07.lya.dat z01.05.02.20:21:07.ovi.dat z01.05.02.20:21:07.vld.dat z01.05.02.20:47:34.lya.dat z01.05.02.20:47:34.ovi.dat z01.05.02.20:47:34.vld.dat