UVCS MISSION LOG ---------------- Date: 11 July 2008 ----- Last revision: 14 July 2008 (Wu) -------------- File Name: 2008.07.12.a.log ---------- Compiled by: M. Uzzo ------------ UVCS Activity: North Polar Coronal Hole OVI Observation for -------------- 12 - 13 July 2008 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 08.07.11.15:10:30.cmd.log Activity: --------- 1) North Polar Coronal Hole Observations Sequence: 08.01_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: 2008.07.12.19:30 end: 2008.07.13.18:30 ONUMs = 24595 (318 exps) 24596 (348 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50111) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 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: q08.07.12.19:29:56.ovi.dat q08.07.13.06:31:16.ovi.dat GAP between 07/13/08|08:20:13( 6379) and 07/13/08|08:21:15( 6476)