UVCS MISSION LOG ---------------- Date: 10 May 2005 ----- Last revision: 11 May 2005 (Wu) -------------- File Name: 2005.05.10.a.log ---------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Flush and Reload Mini Synoptic at SW for 10 May 2005 -------------- Load North Polar Coronal Hole OVI Observation for 10 - 11 May 2005 Load North Polar Coronal Hole OVI Observation for 11 May 2005 Load OVI Synoptic for 11 May 2005 Load IPS Campaign LyA Observations for 12 May 2005 Load IPS Campaign OVI Observations for 12 - 13 May 2005 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 05.05.10.17:44:01.cmd.log Activity: --------- 1) North Polar Coronal Hole Observation Sequence: 05.02_hole1OVI.tcl SCI_SPEC: Characterization of the North 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=351 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: 2005.05.10.19:05 end: 2005.05.11.04:31 ONUMs = 22342 (105 exps) 22343 (168 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 343.09, 344.27, 345.38 degrees (15684, 15898, 16101) - Mirror/Occulter: 1.7, 2.0, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.05.10.18:54:42.ovi.dat q05.05.10.22:43:11.ovi.dat 2) North Polar Coronal Hole Observation Sequence: 05.02_holexOVI.tcl, n50min=5 SCI_SPEC: Characterization of the North 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=351 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: 2005.05.11.04:32 end: 2005.05.11.09:35 ONUMs = 22344 (14 exps) 22345 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 343.09, 345.38 degrees (15684, 16101) - Mirror/Occulter: 1.7, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.05.11.04:31:12.ovi.dat q05.05.11.05:01:20.ovi.dat