UVCS MISSION LOG ---------------- Date: 15 September 2008 ----- Last revision: 15 September 2008 (Wu) -------------- File Name: 2008.09.13.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: LYA Detector Diagnostic for 13 September 2008 -------------- Physical Parameters of the Slow and Fast Solar Wind Across the Sonic Point for 13 - 14 September 2008 SOHO Activity: -------------- EOF Staff: D. Telloni: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: 08.09.12.11:15:00.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: 2008.09.13.01:14 end: 2008.09.13.01:45 ONUMs = 24708 (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: q08.09.13.01:04:41.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: 2008.09.13.01:56 end: 2008.09.14.01:54 ONUMs = 24709 (360 exps) 24710 (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: q08.09.13.01:54:47.lya.dat q08.09.13.14:19:30.lya.dat