UVCS MISSION LOG ---------------- Date: 30 January 2007 ----- Last revision: 06 February 2007 (Ko) -------------- File Name: 2007.01.31.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Observations of Polar Coronal Holes for -------------- 31 - 01 February 2007 Load OVI Detector Diagnostic for 2 February 2007 Load Observations of Polar Coronal Holes for 02 - 03 February 2007 Load Observations of Polar Coronal Holes for 03 - 04 February 2007 SOHO Activity: Received via email Thursday, 01 February 2007, -------------- 05:02:55 GMT: OBT DISTRIBUTED TO UVCS BY FOT EOF Staff: D. Telloni: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 07.01.29.16:46:00.cmd.log 07.01.31.15:12:01.cmd.log Activity: --------- 1) Observations of Polar Coronal Holes Sequence: 07.01_Daniele.tcl n = 8, m = 3, r = 0 SCI_SPEC: Main scientific objective is to make some comparisons between coronal hole and streamer observations in order to study plasma properties varying with time. OBS_PROG: Primary: Temporal Coverage Sub Obj: Temporal Resolution SCI_OBJ: Primary: Plasma Properties Sub Obj: Ion Temperatures OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2007.01.31.17:42 end: 2007.02.01.17:48 ONUMs = 23079 (223 exps) 23080 (228 exps) 23081 (156 exps) 23082 (60 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180 Degrees (18762) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: q07.01.31.17:42:19.ovi.dat GAP between 01/31/07|23:20:20(12125) and 01/31/07|23:34:32(13485) GAP between 02/01/07|00:18:49( 1361) and 02/01/07|00:26:30( 2095) GAP between 02/01/07|00:38:16( 3226) and 02/01/07|00:51:57( 4540) q07.02.01.01:58:19.ovi.dat GAP between 02/01/07|09:53:32( 7421) and 02/01/07|10:23:31(10304) q07.02.01.10:14:18.ovi.dat q07.02.01.15:44:58.ovi.dat