UVCS MISSION LOG ---------------- Date: 03 April 2006 ----- Last revision: 11 April 2006 (Wu) -------------- File Name: 2006.04.07.a.log ---------- Compiled by: M. Uzzo, Y.-K. Ko ------------ UVCS Activity: Plume Observations in LyA at the South Coronal Hole for -------------- 07 April 2006 Plume Observations in OVI at the South Coronal Hole for 07 - 08 April 2006 OVI Detector Diagnostic for 08 April 2006 Load Plume Observations in LyA at the South Coronal Hole for 08 April 2006 Load Plume Observations in OVI at the South Coronal Hole for 08 - 09 April 2006 Load South Coronal Hole Observations in LyA for 09 April 2006 Load South Coronal Hole Observations in OVI for 09 - 10 April 2006 Load South Coronal Hole Observations in OVI for 10 - 11 April 2006 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist --------- Y.-K. Ko: Planner, Commander Command file: 06.04.05.15:38:52.cmd.log 06.04.07.20:37:59.cmd.log Activity: --------- 1) Plume Observations at the South Coronal Hole Sequence: 06.04_plumeLyA.tcl SCI_SPEC: The observations will focus on determinations of O5+ outflow speeds in polar plumes and determinations of the electron density. Roll angle is corrected to put row 55 at target angle. Target angle = 180 OBS_PROG: Primary: Spatial Resolution Sub Obj: Spectral Coverage SCI_OBJ: Primary: Coronal Structure...Fine Structure Sub Obj: Coronal Dynamics...Outflow Velocities Sub Obj: Plasma Properties...Density OBJ: Polar Plume CMP_NAME: Plume Observations at the South Coronal Hole, UVCS; LASCO CMP_NUM: 7176 Duration: start: 2006.04.07.14:59 end: 2006.04.07.18:05 ONUMs = 22367 (90 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 147 Degrees (45544) - Mirror/Occulter: 1.6 Ro 1.5 mm overocculting - LYA Slits: 100 um - OVI Slits: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp2_164 in slot 4 Fits Files: q06.04.07.14:58:14.ovi.dat 2) Plume Observations at the South Coronal Hole Sequence: 06.04_plumeOVI.tcl SCI_SPEC: The observations will focus on determinations of O5+ outflow speeds in polar plumes and determinations of the electron density. Roll angle is corrected to put row 55 at target angle. Target angle = 180 OBS_PROG: Primary: Spatial Resolution Sub Obj: Spectral Coverage SCI_OBJ: Primary: Coronal Structure...Fine Structure Sub Obj: Coronal Dynamics...Outflow Velocities Sub Obj: Plasma Properties...Density OBJ: Polar Plume CMP_NAME: Plume Observations at the South Coronal Hole, UVCS; LASCO CMP_NUM: 7176 Duration: start: 2006.04.07.18:07 end: 2006.04.08.16:10 ONUMs = 22368 (320 exps) 22369 (318 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 147 Degrees (45544) - Mirror/Occulter: 1.6 Ro 1.5 mm overocculting - LYA Slits: 100 um - OVI Slits: 150 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_Eclipse06_215 in slot 1 Fits Files: q06.04.07.18:07:06.ovi.dat q06.04.08.05:08:26.ovi.dat 3) OVI Detector Diagnostic Sequence: 06.02_OVI_164_chk.tcl SCI_SPEC: Instrument Diagnostics OBS_PROG: Spatial Resolution SCI_OBJ: OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2006.04.08.16:14 end: 2006.04.08.17:15 ONUMs = 22370 (12 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 180 degrees (51551) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: q06.04.08.16:09:57.ovi.dat