UVCS MISSION LOG ---------------- Date: 11 December 2006 ----- Last revision: 27 December 2006 (Wu) -------------- File Name: 2006.12.12.a.log ---------- Compiled by: M. Uzzo, R .Wu ------------ UVCS Activity: Ramp Down and Power off LYA Detector -------------- Turn on OVI Detector Conduct OVI Stimulus Pulse Test Ramp Up OVI Detector HV Load and Start OVI Detector Diagnostic for 12 December 2006 Load Streamer Study OVI Observation for 12 - 14 December 2006 Flush Streamer Study OVI Observation for 12 - 14 December 2006 Reload Streamer Study OVI Observation for 12 - 14 December 2006 with corrected roll angle SOHO Activity: -------------- EOF Staff: M. Uzzo: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 06.12.12.14:51:15.cmd.log 06.12.13.13:44:59.cmd.log Activity: --------- 1) OVI Stimulus Pulse Test Sequence: TakeUV_TxN.tcl SCI_SPEC: OBS_PROG: SCI_OBJ: OBJ: CMP_NAME: CMP_NUM: Duration: start: 2006.12.12.19:30 end: 2006.12.12.19:34 ONUMs = 22933 (2 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 60 Degrees (62474) - Mirror/Occulter: 2.50 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 0 - OVI MCP Voltage: 0 - OVI mask: OVI_303_8x2 in slot 3 Fits Files: q06.12.12.19:26:50.ovi.dat 2) 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: 2006.12.12.19:48 end: 2006.12.12.20:49 ONUMs = 22934 (12 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: q06.12.12.19:41:21.ovi.dat 3) Streamer Study Sequence: 06.10_StrObsOVI.tcl, sw = 2 SCI_SPEC: A comprehensive study of several streamer properties including the outflow velocities, abundances, electron densities and temperatures. The spatial distribution of these physical properties are analyzed at multiple heights within several streamers examined over the course of the solar cycle. Note: Final ONUM loaded 13 December 2006 OBS_PROG: Primary: Spectral Resolution Sub Obj: Spatial Resolution SCI_OBJ: Primary: Coronal Dynamics...Outflow Velocities Sub Obj: Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2006.12.12.20:57 end: 2006.12.14.21:47 ONUMs = 22935 (16 exps) 22936 (120 exps) 22937 (320 exps) 22938 (320 exps) 22939 (320 exps) 22940 (319 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 70 Degrees (64294) - Mirror/Occulter: 2.50 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50, 150 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600, 223500, 232100 - OVI MCP Voltage: 200 - OVI mask: OVI_Str_Prof in slot 5 OVI_303_8x2 in slot 3 Fits Files: q06.12.12.20:55:56.ovi.dat q06.12.12.21:29:59.ovi.dat q06.12.13.01:39:04.ovi.dat q06.12.13.12:41:34.ovi.dat q06.12.13.23:42:54.ovi.dat q06.12.14.10:44:46.ovi.dat