UVCS MISSION LOG ---------------- Date: 08 April 2004 ----- Last revision: 12 April 2004 (Wu) -------------- File Name: 2004.04.09.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: South Coronal Hole LyA Observation for -------------- 09 - 10 April 2004 Load OVI Synoptic for 10 April 2004 Load South Coronal Hole LyA Observation for 10 April 2004 Load South Coronal Hole OVI Observation for 10 - 11 April 2004 Load South Coronal Hole OVI Observation for 11 April 2004 Load Mini-Synoptic for 11 April 2004 Load OVI Synoptic for 11 - 12 April 2004 Load LyA Synoptic for 12 April 2004 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: 04.04.08.12:09:00.cmd.log 04.04.09.14:51:00.cmd.log Activity: --------- 1) South Coronal Hole Observation Sequence: 04.02_holexOVI.tcl, n53min = 7 SCI_SPEC: Characterization of a south 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=175 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: 2004.04.09.15:47 end: 2004.02.09.22:55 ONUMs = 21100 (14 exps) 21101 (132 exps) 21102 (48 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 167.09, 169.38 degrees (49201, 49618) - Mirror/Occulter: 1.7, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 4 Fits Files: q04.04.09.15:40:23.ovi.dat q04.04.09.15:40:23.vld.dat q04.04.09.16:19:00.ovi.dat q04.04.09.16:19:00.vld.dat q04.04.09.21:09:55.ovi.dat q04.04.09.21:09:55.vld.dat 2) OVI Synoptic Sequence Load and Start Sequence: SynopticC:Start SCI_SPEC: Synoptic studies. 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: 2004.04.09.23:03 end: 2004.04.10.14:08 ONUMs = 44800 (49 exps) 44801 (47 exps) 44802 (49 exps) 44803 (49 exps) 44804 (48 exps) 44805 (47 exps) 44806 (49 exps) 44807 (49 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: SW: os, S: oc, SE: os, E: os, NE: os, N: oc, NW: os, W: 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: 50 um - OVI Slits: 150 um (LyA Synoptic) 200 um (OVI, and Mini Synoptic) - LYA GRTPOS: 128000 - OVI GRTPOS: 177596 (LyA Synoptic) 229000 (OVI, and Mini Synoptic) - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_178 in slot 2 (LyA Synoptic) OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic) Fits Files: z04.04.09.23:02:41.ovi.dat z04.04.09.23:02:41.vld.dat z04.04.10.00:58:20.ovi.dat z04.04.10.00:58:20.vld.dat z04.04.10.02:46:31.ovi.dat z04.04.10.02:46:31.vld.dat z04.04.10.04:42:02.ovi.dat z04.04.10.04:42:02.vld.dat z04.04.10.06:37:35.ovi.dat z04.04.10.06:37:35.vld.dat GAP between 04/10/04|07:44:02( 3726) and 04/10/04|07:45:29( 3860) z04.04.10.08:33:03.ovi.dat z04.04.10.08:33:03.vld.dat z04.04.10.10:21:22.ovi.dat z04.04.10.10:21:22.vld.dat z04.04.10.12:16:47.ovi.dat z04.04.10.12:16:47.vld.dat