UVCS MISSION LOG ---------------- Date: 01 July 2009 ----- Last revision: 02 July 2009 (MU) -------------- File Name: 2009.07.01.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: North Coronal Hole Study for 01 - 02 July 2009 -------------- Load OVI Detector Rate Diagnostic for 02 July 2009 Load North Coronal Hole Study for 02 - 03 July 2009 Load North Coronal Hole Study for 03 - 04 July 2009 Load OVI Detector Rate Diagnostic for 04 July 2009 Load North Coronal Hole Study for 04 - 05 July 2009 Load North Coronal Hole Study for 05 - 06 July 2009 Load OVI Detector Rate Diagnostic for 06 July 2009 Load North Coronal Hole Study for 06 - 07 July 2009 SOHO Activity: Received via email Thursday, 02 July 2009, -------------- 03:01:15 GMT: OBT DISTRIBUTED TO UVCS BY FOT EOF Staff: M. P. Miralles / J. Kohl: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: 09.06.26.12:41:51.cmd.log Activity: --------- 1) North Polar Coronal Hole Study Sequence: 09.07_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: 2009.07.01.13:18 end: 2009.07.01.12:18 ONUMs = 25591 (319 exps) 25592 (347 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50331) - Mirror/Occulter: 2.1 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 232100 - OVI MCP Voltage: 205 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q09.07.01.13:17:49.ovi.dat q09.07.02.00:19:09.ovi.dat