UVCS MISSION LOG ---------------- Date: 19 October 2005 ----- Last revision: 17 November 2005 (Wu) -------------- File Name: 2005.10.19.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start Polar Coronal Hole LyA Observation -------------- for 19 October 2005 Load Polar Coronal Hole OVI Observation for 19 - 20 October 2005 Load Polar Coronal Hole OVI Observation for 20 October 2005 Load Synoptic for 20 October 2005 Load Polar Coronal Hole LyA Observation for 20 - 21 October 2005 Load Polar Coronal Hole OVI Observation for 21 October 2005 Load Polar Coronal Hole OVI Observation for 21 October 2005 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 05.10.19.11:57:19.cmd.log Activity: --------- 1) Polar Coronal Hole Observation Sequence: 05.09_hole1LyA.tcl SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar 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 non-polar coronal holes. Roll positions are VL-corrected for PA=8 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: 2005.10.19.13:07 end: 2005.10.19.17:41 ONUMs = 21845 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 0.093, 1.267, 2.381 degrees (18779, 18993, 19195) - Mirror/Occulter: 1.7, 2.0, 2.4 Ro 1.5 mm overocculting (1.7, 2.0 Ro) 2.0 mm overocculting (2.4 Ro) - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q05.10.19.12:58:00.ovi.dat 2) Polar Coronal Hole Observation Sequence: 05.09_hole1OVI.tcl SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar 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 non-polar coronal holes. Roll positions are VL-corrected for PA=8 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: 2005.10.19.17:43 end: 2005.10.20.03:08 ONUMs = 21846 (105 exps) 21847 (167 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 0.093, 1.267, 2.381 degrees (18779, 18993, 19195) - Mirror/Occulter: 1.7, 2.0, 2.4 Ro 1.5 mm overocculting (1.7, 2.0 Ro) 2.0 mm overocculting (2.4 Ro) - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.10.19.17:41:42.ovi.dat q05.10.19.21:20:39.ovi.dat GAP between 10/20/05|02:53:26(11604) and 10/20/05|02:54:56(11750) 3) Polar Coronal Hole Observation Sequence: 05.09_holexOVI.tcl, n50min = 2 SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar 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 non-polar coronal holes. Roll positions are VL-corrected for PA=8 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: 2005.10.20.03:10 end: 2005.10.20.05:44 ONUMs = 21848 (14 exps) 21849 (60 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 0.093, 2.381 degrees (18779, 19195) - Mirror/Occulter: 1.7, 2.4 Ro 1.5 mm overocculting (1.7 Ro) 2.0 mm overocculting (2.4 Ro) - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.10.20.03:08:43.ovi.dat q05.10.20.03:38:51.ovi.dat 4) OVI Synoptic Sequence Load and Start Sequence: SynopticD:Start SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage at 200. OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2005.10.20.05:54 end: 2005.10.20.20:07 ONUMs = 48860 (49 exps) 48861 (49 exps) 48862 (47 exps) 48863 (49 exps) 48864 (49 exps) 48865 (49 exps) 48866 (47 exps) 48867 (49 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: W: os, NW: os, N: oc, NE: os, E: os, SE: os, S: oc, SW: os - Mirror/Occulter: ls: 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro lc: 2.10, 1.90, 1.75, 1.60 Ro os: 3.00, 2.10, 1.90, 1.75, 1.60 Ro oc: 1.90, 1.75, 1.60 Ro ms: 2.10, 1.75, 1.60 Ro mc: 1.90, 1.75, 1.60 Ro 1.5 mm overocculting (1.60 Ro) 2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00 Ro) - LYA Slits: 100 um - OVI Slits: 150 um (LyA Synoptic) 200 um (OVI, and Mini Synoptic) - LYA GRTPOS: 100000 - OVI GRTPOS: 187260 (LyA Synoptic) 229000 (OVI, and Mini Synoptic) - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_188 in slot 2 (LyA Synoptic) OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic) Fits Files: z05.10.20.05:53:19.ovi.dat z05.10.20.07:41:59.ovi.dat z05.10.20.09:30:39.ovi.dat z05.10.20.11:14:06.ovi.dat z05.10.20.13:02:46.ovi.dat z05.10.20.14:51:26.ovi.dat z05.10.20.16:40:06.ovi.dat z05.10.20.18:23:33.ovi.dat