UVCS MISSION LOG ---------------- Date: 07 November 2005 ----- Last revision: 07 November 2005 (Wu) -------------- File Name: 2005.11.04.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Polar Coronal Hole LyA Observation for -------------- 04 November 2005 Load Polar Coronal Hole OVI Observation for 04 - 05 November 2005 Load Polar Coronal Hole OVI Observation for 05 November 2005 Load Mini-Synoptic for 05 Novebmer 2005 Load Polar Coronal Hole OVI Observation for 05 - 06 November 2005 Load Polar Coronal Hole OVI Observation for 06 November 2005 Load Mini-Synoptic for 06 Novebmer 2005 Load Polar Coronal Hole LyA Observation for 07 November 2005 Load Polar Coronal Hole OVI Observation for 07 November 2005 Load Polar Coronal Hole OVI Observation for 07 November 2005 Load LyA Synoptic for 07 - 08 November 2005 Load OVI Synoptic for 08 November 2005 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander Y.-K. Ko: Planner R. Wu Command file: 05.11.04.16:29:00.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=195 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: 2005.11.04.18:43 end: 2005.11.04.23:17 ONUMs = 21898 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 187.093, 188.267, 189.381 degrees (52842, 53056, 53259) - 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: q05.11.04.18:33:37.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=195 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: 2005.11.04.23:19 end: 2005.11.05.02:57 ONUMs = 21899 (98 exps) 21900 (164 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 187.093, 188.267, 189.381 degrees (52842, 53056, 53259) - 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: q05.11.04.23:17:57.ovi.dat q05.11.05.02:56:54.ovi.dat 3) Polar Coronal Hole Observation Sequence: 05.09_holexOVI.tcl, n50min = 10 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=195 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: 2005.11.05.08:46 end: 2005.11.05.17:57 ONUMs = 21101 (14 exps) 21102 (132 exps) 21103 (120 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 187.093, 189.381 degrees (52842, 53259) - 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: q05.11.05.08:45:15.ovi.dat q05.11.05.09:15:22.ovi.dat q05.11.05.13:48:54.ovi.dat 4) Mini-Synoptic Sequence Load and Start Sequence: SynopticD:Start SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage at 200, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2005.11.05.18:02 end: 2005.11.05.23:04 ONUMs = 48940 (9 exps) 48941 (35 exps) 48942 (9 exps) 48943 (9 exps) 48944 (9 exps) 48945 (35 exps) 48946 (9 exps) 48947 (9 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: SW: ms, S: mc, SE: ms, E: ms, NE: ms, N: mc, NW: ms, W: ms - 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: 50 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: z05.11.05.18:01:38.ovi.dat z05.11.05.18:26:34.ovi.dat z05.11.05.19:45:14.ovi.dat z05.11.05.20:10:10.ovi.dat z05.11.05.20:35:06.ovi.dat z05.11.05.21:00:02.ovi.dat z05.11.05.22:18:42.ovi.dat z05.11.05.22:43:37.ovi.dat