UVCS MISSION LOG ---------------- Date: 21 April 2008 ----- Last revision: 28 July 2008 (MU) -------------- File Name: 2008.04.20.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Physical Parameters of Coronal Holes Across the -------------- Sonic Point for 20 - 21 April 2008 LyA Detector Diagnostic for 21 April 2008 SOHO Activity: -------------- EOF Staff: D. Telloni: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: 08.04.18.17:45:00.cmd.log Activity: --------- 1) Physical Parameters of Coronal Holes Across the Sonic Point Sequence: 08.04_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: 2008.04.20.18:59 end: 2008.04.21.18:58 ONUMs = 24378 (360 exps) 24379 (336 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 96.7 Degrees (36376) - Mirror/Occulter: 3.7 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_VEX_4x1 in slot 2 Fits Files: q08.04.20.18:58:39.lya.dat q08.04.21.07:23:22.lya.dat 2) LYA Detector Diagnostic Sequence: LYA_100_chk.tcl SCI_SPEC: OBS_PROG: Spatial Resolution SCI_OBJ: OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.04.21.19:07 end: 2008.04.21.19:38 ONUMs = 24380 (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: q08.04.21.18:57:46.lya.dat