UVCS MISSION LOG ---------------- Date: 21 July 2006 ----- Last revision: 25 July 2006 (MU) -------------- File Name: 2006.07.30.a.log ---------- Compiled by: M. Uzzo ------------ UVCS Activity: North Polar Coronal Hole OVI Observation for -------------- 30 - 31 July 2006 OVI Detector Diagnostic for 31 July 2006 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist --------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 06.07.25.18:25:20.cmd.log Activity: --------- 1) 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: 2006.07.30.1 end: 2006.07.31.1 ONUMs = 22647 (320 exps) 22648 ( exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 174.38 Degrees (17739) - Mirror/Occulter: 2.0 Ro 1.5 mm overocculting - LYA Slit: 75 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: 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: 2006.07.31.1 end: 2006.07.31.1 ONUMs = 22649 (12 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: 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: