UVCS MISSION LOG ---------------- Date: 20 July 2007 ----- Last revision: 23 July 2007 (Wu) -------------- File Name: 2007.07.20.a.log ---------- Compiled by: M. Uzzo, R. Wu, Y.-K. Ko ------------ UVCS Activity: Load and Start South Polar Coronal Hole OVI Observation -------------- for 20 - 21 July 2007 Load South Polar Coronal Hole OVI Observation for 21 - 22 July 2007 Load OVI Detector Diagnostic for July 22 2007 Load Equatorial Coronal Hole LyA Observations for 22 July 2007 Load Equatorial Coronal Hole LyA Observations for 22 July 2007 Load Equatorial Coronal Hole LyA Observations for 22 July 2007 Load Equatorial Coronal Hole OVI Observations for 22 July 2007 Load Equatorial Coronal Hole OVI Observations for 22 July 2007 Load Equatorial Coronal Hole OVI Observations for 22 - 23 July 2007 Load Equatorial Coronal Hole LyA Observations for 23 July 2007 Load Equatorial Coronal Hole LyA Observations for 23 July 2007 Load Equatorial Coronal Hole LyA Observations for 23 July 2007 Load Equatorial Coronal Hole OVI Observations for 23 July 2007 Load Equatorial Coronal Hole OVI Observations for 23 July 2007 Load Equatorial Coronal Hole OVI Observations for 23 - 24 July 2007 Load Equatorial Coronal Hole LyA Observations for 24 July 2007 Load Equatorial Coronal Hole LyA Observations for 24 July 2007 Load Equatorial Coronal Hole LyA Observations for 24 July 2007 Load Equatorial Coronal Hole OVI Observations for 24 July 2007 Load Equatorial Coronal Hole OVI Observations for 24 July 2007 Load Equatorial Coronal Hole OVI Observations for 24 - 25 July 2007 Load OVI Detector Diagnostic for July 25 2007 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 07.07.20.17:03:38.cmd.log Activity: --------- 1) South Polar Coronal Hole OVI Observations Sequence: 06.08_hole.tcl, n = 4, 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=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: 2007.07.20.17:10 end: 2007.07.21.05:09 ONUMs = 23510 (348 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: 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: q07.07.20.17:10:11.ovi.dat GAP between 07/20/07|18:52:23(10900) and 07/20/07|18:53:42(11031)