UVCS MISSION LOG ---------------- Date: 22 December 2005 ----- Last revision: 23 December 2005 (Wu) -------------- File Name: 2005.12.22.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start North Coronal Hole LyA Observation for -------------- 22 December 2005 Load North Coronal Hole OVI Observation for 22 - 23 December 2005 Load OVI Synoptic for 23 December 2005 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 05.12.22.14:56:30.cmd.log Activity: --------- 1) North Polar Coronal Hole Observation Sequence: 05.12_hole2LyA.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=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: 2005.12.22.16:11 end: 2005.12.22.18:09 ONUMs = 22046 (56 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 352.093, 353.585 degrees (50112, 50383) - Mirror/Occulter: 1.7, 2.1 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q05.12.22.15:57:21.ovi.dat 2) North Polar Coronal Hole Observation Sequence: 05.12_hole2OVI.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=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: 2005.12.22.18:10 end: 2005.12.23.04:10 ONUMs = 22047 (74 exps) 22048 (216 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 352.093, 353.585 degrees (50112, 50383) - Mirror/Occulter: 1.7, 2.1 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.12.22.18:09:30.ovi.dat q05.12.22.20:42:58.ovi.dat 3) 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: 2005.12.23.04:17 end: 2005.12.23.18:30 ONUMs = 49190 (49 exps) 49191 (47 exps) 49192 (49 exps) 49193 (49 exps) 49194 (49 exps) 49195 (47 exps) 49196 (49 exps) 49197 (49 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: NE: os, N: oc, NW: os, W: os, SW: os, S: oc, SE: os, E: 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: z05.12.23.04:16:15.ovi.dat z05.12.23.06:04:55.ovi.dat z05.12.23.07:48:23.ovi.dat z05.12.23.09:37:02.ovi.dat z05.12.23.11:25:42.ovi.dat z05.12.23.13:14:22.ovi.dat z05.12.23.14:57:50.ovi.dat z05.12.23.16:46:29.ovi.dat