UVCS MISSION LOG ---------------- Date: 16 January 2007 ----- Last revision: 19 January 2007 (Wu) -------------- File Name: 2007.01.16.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start South Coronal Hole Observation for -------------- 16 - 17 January 2007 Load South Coronal Hole Observation for 17 January 2007 Flush IQ Reload and Start South Coronal Hole Observation for 16 - 17 January 2007 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander Y.-K. Ko: Planner R. Wu Command file: 07.01.16.14:38:24.cmd.log Activity: --------- 1) South Coronal Hole Observations Sequence: 07.01_pch.tcl, n50min = 30 SCI_SPEC: Study of the energy and dynamics of polar plumes and their relation to polar jets. Hinode/XRT has recently observed jets in reconnection regions within and near coronal hole boundaries at the poles. These hot jets have been seeing in X-rays up to 1.7 Ro. In this study, we will search for counterparts to the polar X-ray jets and follow the polar plume distribution. OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Coverage & Sensitivity SCI_OBJ: Primary: Coronal Structure...Fine Structure Sub Obj: Plasma Properties...Proton Temperature OBJ: Polar Plume and Coronal Hole CMP_NAME: Polar Coronal Hole Study, UVCS; LASCO; CDS; EIT; Hinode (S/C); TRACE (S/C); STEREO (S/C) CMP_NUM: 7197 Duration: start: 2007.01.16.16:15 end: 2007.01.16.17:04 ONUMs = 23030 (24 exps) ; flushed 23031 ( exps) ; not run Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180 Degrees (18762) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 300 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_str_4x1 in slot 2 Fits Files: q07.01.16.16:14:07.lya.dat 2) South Coronal Hole Observations Sequence: 07.01_pch.tcl, n50min = 37 SCI_SPEC: Study of the energy and dynamics of polar plumes and their relation to polar jets. Hinode/XRT has recently observed jets in reconnection regions within and near coronal hole boundaries at the poles. These hot jets have been seeing in X-rays up to 1.7 Ro. In this study, we will search for counterparts to the polar X-ray jets and follow the polar plume distribution. OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Coverage & Sensitivity SCI_OBJ: Primary: Coronal Structure...Fine Structure Sub Obj: Plasma Properties...Proton Temperature OBJ: Polar Plume and Coronal Hole CMP_NAME: Polar Coronal Hole Study, UVCS; LASCO; CDS; EIT; Hinode (S/C); TRACE (S/C); STEREO (S/C) CMP_NUM: 7197 Duration: start: 2007.01.16.17:05 end: 2007.01.17.23:40 ONUMs = 23031 (360 exps) 23032 (360 exps) 23033 (168 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: 300 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_str_4x1 in slot 2 Fits Files: q07.01.16.17:04:37.lya.dat q07.01.17.05:29:20.lya.dat q07.01.17.17:53:20.lya.dat