UVCS MISSION LOG ---------------- Date: 09 November 2006 ----- Last revision: 16 November 2006 (Wu) -------------- File Name: 2006.11.09.a.log ---------- Compiled by: R. Wu, Y.-K. Ko ------------ UVCS Activity: Streamer Study OVI Observation for 09 - 10 November 2006 -------------- Flush and Abort Streamer Study Ramp Down and Power off OVI Detector Turn on LYA Detector Conduct LYA Stimulus Pulse Test Ramp Up LYA Detector HV Load and Start LYA Detector Diagnostic for 09 November 2006 Load Suprathermal Seed Particle Populations in the Extended Corona (Streamer Study) for 09 - 10 November 2006 Load Suprathermal Seed Particle Populations in the Extended Corona (Streamer Study) for 10 - 14 November 2006 SOHO Activity: -------------- EOF Staff: L. Strachan / J. Kohl: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Commander, Planner M. Uzzo: Planner Command file: 06.11.08.19:04:00.cmd.log 06.11.09.21:07:01.cmd.log Activity: --------- 1) Streamer Study Sequence: 06.10_StrObsOVI.tcl, sw = 1 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. 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: 2006.11.09.10:37 end: 2006.11.09.21:28 ONUMs = 22893 (8 exps) 22894 (40 exps) 22895 (266 exps) ; aborted 22896 ( exps) ; flushed Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 135 Degrees (43348) - Mirror/Occulter: 1.75 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: q06.11.09.10:35:51.ovi.dat q06.11.09.10:53:29.ovi.dat q06.11.09.12:17:14.ovi.dat 2) LYA Stimulus Pulse Test Sequence: TakeUV_TxN.tcl SCI_SPEC: OBS_PROG: SCI_OBJ: OBJ: CMP_NAME: CMP_NUM: Duration: start: 2006.11.09.21:50 end: 2006.11.09.21:54 ONUMs = 22897 (2 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 135 Degrees (43348) - 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: 0 - OVI MCP Voltage: 0 - LYA mask: msk_000303 in slot 3 Fits Files: q06.11.09.21:45:57.lya.dat 3) LYA Detector Diagnostic Sequence: 06.05_LYA_chk.tcl SCI_SPEC: OBS_PROG: Spatial Resolution SCI_OBJ: OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2006.11.09.22:10 end: 2006.11.09.22:40 ONUMs = 22898 (6 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: 210000 - LYA MCP Voltage: 195 - LYA mask: LYA_chk_1xfull in slot 6 Fits Files: q06.11.09.22:04:42.lya.dat 4) Suprathermal Seed Particle Population Measurements Sequence: 06.11_SeedLyA_r3.tcl, n12hr = 1, n6hr = 0, n50min = 4 SCI_SPEC: OBS_PROG: Primary: Spectral Resolution Sub_Obj: Sensitivity SCI_OBJ: Primary: Plasma Properties...Density Sub_Obj: Plasma Properties...Proton Temperature OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2006.11.09.22:55 end: 2006.11.10.14:07 ONUMs = 22899 (180 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 252 degrees (64658) - Mirror/Occulter: 3.00 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_wing_100 in slot 5 Fits Files: q06.11.09.22:54:46.lya.dat