UVCS MISSION LOG ---------------- Date: 17 June 2007 ----- Last revision: 20 June 2007 (Wu) -------------- File Name: 2007.06.18.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: North Coronal Hole OVI Observations for -------------- 18 - 19 June 2007 Load North Coronal Hole OVI Observations for 19 - 20 June 2007 Load North Coronal Hole OVI Observations for 20 - 21 June 2007 Load North Coronal Hole OVI Observations for 21 - 22 June 2007 Load OVI Detector Diagnostic for 22 June 2007 Load North Coronal Hole OVI Observations for 22 - 23 June 2007 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 07.06.17.14:39:39.cmd.log Activity: --------- 1) North Coronal Hole OVI Observations Sequence: 06.08_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0 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=0 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: 2007.06.18.11:30 end: 2007.06.19.10:31 ONUMs = 23440 (320 exps) 23441 (348 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 354.381 Degrees (50528) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: q07.06.18.11:30:12.ovi.dat q07.06.18.22:31:32.ovi.dat