UVCS MISSION LOG ---------------- Date: 17 July 2006 ----- Last revision: 20 July 2006 (Wu) -------------- File Name: 2006.07.17.a.log ---------- Compiled by: R .Wu ------------ UVCS Activity: Ramp Down and Power off LYA Detector -------------- Turn on OVI Detector Conduct OVI Stimulus Pulse Test Ramp Up OVI Detector HV Load and Start OVI Detector Diagnostic for 17 July 2006 Load North Polar Coronal Hole LyA Observation for 17 - 18 July 2006 Load North Polar Coronal Hole OVI Observation for 18 - 19 July 2006 Load North Polar Coronal Hole OVI Observation for 19 - 20 July 2006 Load North Polar Coronal Hole OVI Observation for 20 - 21 July 2006 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist --------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 06.07.17.19:36:00.cmd.log Activity: --------- 1) OVI Stimulus Pulse Test Sequence: TakeUV_TxN.tcl SCI_SPEC: OBS_PROG: SCI_OBJ: OBJ: CMP_NAME: CMP_NUM: Duration: start: 2006.07.17.19:50 end: 2006.07.17.19:54 ONUMs = 22615 (2 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 2.2 Ro 1.5 mm Overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 0 - OVI MCP Voltage: 0 - OVI mask: msk_000303_OVI in slot 3 Fits Files: q06.07.17.19:44:59.ovi.dat 2) OVI Detector Diagnostic Sequence: 06.02_OVI_164_chk.tcl SCI_SPEC: OBS_PROG: Spatial Resolution SCI_OBJ: OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2006.07.17.20:18 end: 2006.07.17.21:18 ONUMs = 22616 (12 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 1.75 Ro 1.5 mm Overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: q06.07.17.20:15:47.ovi.dat 3) North Coronal Hole Observations Sequence: 06.06_hole.tcl 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 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=180 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: 2006.07.17.21:38 end: 2006.07.18.04:36 ONUMs = 22617 (202 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 174.38 Degrees (17739) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 75 um - OVI Slit: 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp2_164 in slot 4 Fits Files: q06.07.17.21:38:20.ovi.dat