UVCS MISSION LOG ---------------- Date: 10 June 2008 ----- Last revision: 13 June 2008 (Wu) -------------- File Name: 2008.06.10.a.log ---------- Compiled by: M. Uzzo ------------ UVCS Activity: Flush and Abort IQ -------------- Transmit LyA Exposure 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 10 June 2007 Load and Start Streamer Study OVI Observations for 10 June 2008 Load Streamer Study OVI Observations for 10 June 2008 Load Streamer Study OVI Observations for 10 - 11 June 2008 SOHO Activity: -------------- EOF Staff: M. Uzzo: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 08.06.10.11:57:53.cmd.log Activity: --------- 1) OVI Stimulus Pulse Test Sequence: TakeUV_TxN.tcl SCI_SPEC: Calibration OBS_PROG: Calibration SCI_OBJ: Calibration OBJ: CMP_NAME: CMP_NUM: Duration: start: 2008.06.10.16:08 end: 2008.06.10.16:12 ONUMs = 24459 (2 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35156) - 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 - OVI mask: OVI_303_8x2 in slot 3 Fits Files: q08.06.10.16:04:27.ovi.dat 2) OVI Detector Diagnostic Sequence: OVI_164_chk.tcl SCI_SPEC: Instrument Diagnostics OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.06.10.16:31 end: 2008.06.10.17:32 ONUMs = 24460 (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: 150 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: q08.06.10.16:20:58.ovi.dat 3) Streamer Study OVI Observations Sequence: 08.02_StrObsOVI.tcl, sw = 17 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: 2008.06.10.17:42 end: 2008.06.10.19:22 ONUMs = 24461 (8 exps) 24462 (40 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35156) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600, 223500 - OVI MCP Voltage: 200 - OVI mask: OVI_Str_Prof in slot 5 Fits Files: q08.06.10.17:40:32.ovi.dat q08.06.10.17:58:03.ovi.dat 4) Streamer Study OVI Observations Sequence: 08.02_StrObsOVI.tcl, sw = 17 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: 2008.06.10.19:23 end: 2008.06.10.21:04 ONUMs = 24463 (8 exps) 24464 (40 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35156) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600, 223500 - OVI MCP Voltage: 200 - OVI mask: OVI_Str_Prof in slot 5 Fits Files: q08.06.10.19:22:20.ovi.dat q08.06.10.19:39:58.ovi.dat 5) Streamer Study OVI Observations Sequence: 08.02_StrObsOVI.tcl, sw = 0 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: 2008.06.10.21:05 end: 2008.06.11.19:08 ONUMs = 24465 (320 exps) 24466 (320 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35165) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 200 um - LYA GRTPOS: 100000 - OVI GRTPOS: 232100 - OVI MCP Voltage: 200 - OVI mask: OVI_303_8x2 in slot 3 Fits Files: q08.06.10.21:04:29.ovi.dat q08.06.11.08:06:48.ovi.dat