UVCS MISSION LOG ---------------- Date: 04 September 2008 ----- Last revision: 08 September 2008 (Wu) -------------- File Name: 2008.09.06.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: LYA Detector Diagnostic for 06 September 2008 -------------- Physical Parameters of the Slow and Fast Solar Wind Across the Sonic Point for 06 - 07 September 2008 SOHO Activity: -------------- EOF Staff: D. Telloni: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 08.09.04.11:20:35.cmd.log Activity: --------- 1) LYA Detector Diagnostic Sequence: LYA_100_chk.tcl SCI_SPEC: Instrument Diagnostics OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.09.06.22:48 end: 2008.09.06.23:18 ONUMs = 24693 (6 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 0 Degrees (18762) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_chk_1xfull in slot 6 Fits Files: q08.09.06.22:38:26.lya.dat 2) Physical Parameters of Coronal Holes Across the Sonic Point Sequence: 08.09_sonic.tcl, n50min = 29 SCI_SPEC: Main scientific objective is to study plasma properties varying with time. Note: Pixel 300 at 90 Degrees OBS_PROG: Primary: Temporal Coverage Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Ion Temperatures OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2008.09.06.23:29 end: 2008.09.07.23:27 ONUMs = 24694 (360 exps) 24695 (336 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 94.4 Degrees (35957) - Mirror/Occulter: 5.7 Ro 1.5 mm overocculting - LYA Slit: 300 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_VEX_4x1 in slot 2 Fits Files: q08.09.06.23:28:15.lya.dat q08.09.07.11:52:58.lya.dat