UVCS MISSION LOG ---------------- Date: 08 January 2007 ----- Last revision: 19 January 2007 (Wu) -------------- File Name: 2007.01.08.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Ramp Down and Power off OVI Detector -------------- Turn on LYA Detector Conduct LYA Stimulus Pulse Test Ramp Up LYA Detector HV Load and Start LyA Detector Diagnostic for 08 January 2007 Load South Coronal Hole Observation for 08 - 09 January 2007 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 07.01.08.16:09:00.cmd.log Activity: --------- 1) LYA Stimulus Pulse Test Sequence: TakeUV_TxN.tcl SCI_SPEC: OBS_PROG: SCI_OBJ: OBJ: CMP_NAME: CMP_NUM: Duration: start: 2007.01.08.16:45 end: 2007.01.08.16:49 ONUMs = 23008 (2 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 5.0 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 0 - OVI MCP Voltage: 0 - LYA mask: msk_000303 in slot 3 Fits Files: q07.01.08.16:42:38.lya.dat 2) LYA Detector Diagnostic Sequence: 06.05_LYA_chk.tcl SCI_SPEC: OBS_PROG: Spatial Resolution SCI_OBJ: OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2007.01.08.17:02 end: 2007.01.08.17:32 ONUMs = 23009 (6 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180 Degrees (18762) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_chk_1xfull in slot 6 Fits Files: q07.01.08.17:00:36.lya.dat 3) South Coronal Hole Observations Sequence: 07.01_pch.tcl, n50min = 26 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: 2007.01.08.17:51 end: 2007.01.09.15:20 ONUMs = 23010 (360 exps) 23011 (264 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: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_str_4x1 in slot 2 Fits Files: q07.01.08.17:49:53.lya.dat q07.01.09.06:14:36.lya.dat