UVCS MISSION LOG ---------------- Date: 15 Dec 2010 ----- Last revision: 21 Apr 2010 (RR) -------------- File Name: 2010.12.15.a.log ---------- Compiled by: R. Rosati ------------ UVCS Activity: Attempt to locate the star Theta Oph unsuccessful, NRT duration -------------- too short today. Load South Coronal Hole OVI Observations for 15 Dec 2010 - 29 Dec 2010 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Rosati: Commander Command file: 10.12.16.02:49:56.cmd.log Activity: --------- 1) South Coronal hole weekly observation Sequence: HoleOVIweek 26723 20072 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2010.12.15.20:51 end: 2010.12.22.23:50 ONUMs = 26723 (80 exps) 26724 (177 exps) 26725 (40 exps) 26726 (271 exps) 26727 (134 exps) 26728 (30 exps) 26729 (53 exps) 26730 (123 exps) 26731 (161 exps) 26738 (131 exps) 26739 (99 exps) 26740 (94 exps) 26741 (19 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 82.7 Degrees (20083) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting 2.0 Ro 1.5 mm overocculting 2.4 Ro 1.5 mm overocculting 5.0 Ro 0.8 mm exposed mirror - LYA Slit: 50 um - OVI Slit: 50, 75, 100 um - LYA GRTPOS: 83040 - OVI GRTPOS: 98000 - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 OVI_chk_1xfull in slot 6 OVI_Hole_BG1 in slot 1 Fits Files: q10.12.16.01:51:20.ovi.dat q10.12.16.04:37:50.ovi.dat q10.12.16.15:40:20.ovi.dat q10.12.16.18:26:50.ovi.dat q10.12.17.08:13:30.ovi.dat q10.12.17.22:00:53.ovi.dat q10.12.17.23:04:26.ovi.dat q10.12.18.01:50:56.ovi.dat q10.12.18.15:37:36.ovi.dat q10.12.21.19:04:36.ovi.dat q10.12.22.08:51:16.ovi.dat q10.12.22.22:37:56.ovi.dat q10.12.23.04:08:36.ovi.dat 2) South Coronal hole weekly observation Sequence: HoleOVIweek 26742 20045 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2010.12.23.02:33 end: 2010.12.30.03:32 ONUMs = 26742 (12 exps) 26743 (139 exps) 26744 (46 exps) 26745 (216 exps) 26746 (247 exps) 26747 (30 exps) 26748 (44 exps) 26749 (160 exps) 26750 (168 exps) 26751 (243 exps) 26752 (198 exps) 26753 (73 exps) 26755 (180 exps) 26756 (195 exps) 26757 (187 exps) 26758 (171 exps) 26759 (54 exps) 26760 (30 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 83 Degrees (20045) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting 2.0 Ro 1.5 mm overocculting 2.4 Ro 1.5 mm overocculting 5.0 Ro 0.8 mm exposed mirror - LYA Slit: 50 um - OVI Slit: 50, 75, 100 um - LYA GRTPOS: 83040 - OVI GRTPOS: 98000 - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 OVI_chk_1xfull in slot 6 OVI_Hole_BG1 in slot 1 Fits Files: q10.12.23.05:12:24.ovi.dat q10.12.23.07:58:54.ovi.dat q10.12.23.19:01:24.ovi.dat q10.12.23.21:47:54.ovi.dat q10.12.24.11:34:34.ovi.dat q10.12.25.01:21:57.ovi.dat q10.12.25.02:25:30.ovi.dat q10.12.25.05:12:00.ovi.dat q10.12.25.18:58:40.ovi.dat q10.12.26.08:45:20.ovi.dat q10.12.26.22:32:00.ovi.dat q10.12.27.12:18:40.ovi.dat q10.12.27.18:52:20.ovi.dat q10.12.28.08:39:00.ovi.dat q10.12.28.22:25:40.ovi.dat q10.12.29.12:12:20.ovi.dat q10.12.30.01:59:00.ovi.dat q10.12.30.07:29:40.ovi.dat