UVCS MISSION LOG ---------------- Date: 16 March 2001 ----- Last revision: 19 March 2001 (Wu) -------------- File Name: 2001.03.18.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Mini-Synoptic 03/18/01 -------------- High-latitude coronal hole study 03/18/01 SOHO Activity: -------------- EOF Staff: L. Strachan: Lead Scientist ---------- Y.-K. Ko: Commander, Planner D. Phillips: Planner M. Uzzo R. Wu Command file: 01.03.16.16:51:38.cmd.log Activity: --------- 1) 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: 2001.03.18.15:02 end: 2001.03.18.18:26 ONUMs = 34650 (9 exps) 34651 (9 exps) 34652 (9 exps) 34653 (9 exps) 34654 (9 exps) 34655 (9 exps) 34656 (9 exps) 34657 (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: z01.03.18.14:59:01.lya.dat z01.03.18.14:59:01.ovi.dat z01.03.18.14:59:01.vld.dat z01.03.18.15:25:30.lya.dat z01.03.18.15:25:30.ovi.dat z01.03.18.15:25:30.vld.dat z01.03.18.15:52:06.lya.dat z01.03.18.15:52:06.ovi.dat z01.03.18.15:52:06.vld.dat z01.03.18.16:18:34.lya.dat z01.03.18.16:18:34.ovi.dat z01.03.18.16:18:34.vld.dat z01.03.18.16:45:11.lya.dat z01.03.18.16:45:11.ovi.dat z01.03.18.16:45:11.vld.dat z01.03.18.17:11:40.lya.dat z01.03.18.17:11:40.ovi.dat z01.03.18.17:11:40.vld.dat z01.03.18.17:38:16.lya.dat z01.03.18.17:38:16.ovi.dat z01.03.18.17:38:16.vld.dat z01.03.18.18:04:52.lya.dat z01.03.18.18:04:52.ovi.dat z01.03.18.18:04:52.vld.dat 2) Observation of High-Latitude Coronal Hole Sequence: 01.01_hole4.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. 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: 2001.03.18.18:52 end: 2001.03.19.04:43 ONUMs = 15976 (56 exps) Instrument configuration: - Pointing: Sun center - Roll: 341.141 degrees (15329) - Mirror/Occulter: 3.5 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 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: q01.03.18.18:40:30.lya.dat q01.03.18.18:40:30.ovi.dat q01.03.18.18:40:30.vld.dat GAP between 03/18/01|18:45:59(14676) and 03/18/01|18:49:59(15058) GAP between 03/18/01|18:56:21(15678) and 03/18/01|18:57:59(15827) GAP between 03/19/01|02:06:16( 7831) and 03/19/01|02:07:56( 7982) 3) Observation of High-Latitude Coronal Hole Sequence: 01.01_hole4.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. 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: 2001.03.19.04:44 end: 2001.03.19.14:35 ONUMs = 15977 (57 exps) Instrument configuration: - Pointing: Sun center - Roll: 341.141 degrees (15329) - Mirror/Occulter: 3.5 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 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: q01.03.19.04:43:03.lya.dat q01.03.19.04:43:03.ovi.dat q01.03.19.04:43:03.vld.dat