UVCS MISSION LOG ---------------- Date: 11 October 2005 ----- Last revision: 17 November 2005 (Wu) -------------- File Name: 2005.10.11.a.log ---------- Compiled by: R. Wu, Y.-K. Ko ------------ UVCS Activity: Equatorial Coronal Hole OVI Observation for -------------- 11 October 2005 OVI Synoptic for 11 - 12 October 2005 Flush, Modify OVI Slit Width and Reload rest of OVI Synoptic for 11 -12 October 2005 Load Equatorial Coronal Hole LyA Observation for 12 October 2005 Load Equatorial Coronal Hole OVI Observation for 12 October 2005 Load Equatorial Coronal Hole OVI Observation for 12 October 2005 Load Mini-Synoptic for 12 - 13 October 2005 Load Equatorial Coronal Hole LyA Observation for 13 October 2005 Load Equatorial Coronal Hole OVI Observation for 13 October 2005 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko: Commander Command file: 05.10.07.19:52:00.cmd.log 05.10.09.21:00:00.cmd.log Activity: --------- 1) Equatorial Coronal Hole Observation Sequence: 05.09_holexOVI.tcl, n50min=5 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=270 degrees. NOTE: Slit closed too far following Mini-Synoptic for 10 - 11 October 2005!!! 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: 2005.10.11.06:36 end: 2005.10.11.11:38 ONUMs = 21810 (105 exps) 21811 (168 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 262.09, 264.38 degrees (938, 1355) - Mirror/Occulter: 1.7, 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: 42, 67 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.10.11.06:34:26.ovi.dat q05.10.11.07:04:41.ovi.dat 2) OVI Synoptic Sequence Load and Start Sequence: SynopticD:Start SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage at 200. NOTE: Slit closed too far following Mini-Synoptic for 10 - 11 October 2005!!! OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2005.10.11.11:41 end: 2005.10.12.02:01 ONUMs = 48790 (49 exps) 48791 (49 exps) 48792 (47 exps) 48793 (49 exps) 48794 (49 exps) 48795 (49 exps) 48796 (47 exps) 48797 (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) 192, 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: z05.10.11.11:40:09.ovi.dat z05.10.11.13:28:49.ovi.dat z05.10.11.15:24:14.ovi.dat z05.10.11.17:07:41.ovi.dat z05.10.11.18:56:21.ovi.dat z05.10.11.20:45:01.ovi.dat z05.10.11.22:33:41.ovi.dat z05.10.12.00:17:08.ovi.dat