UVCS MISSION LOG ---------------- Date: 31 January 2008 ----- Last revision: 07 March 2008 (Wu) -------------- File Name: 2008.01.31.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Flush and Abort Streamer Study OVI Observations for -------------- 31 January 2008 Load and Start Streamer Study OVI Observations for 31 January 2008 Load Streamer Study OVI Observations for 31 January - 01 February 2008 Load Streamer Study OVI Observations for 01 February 2008 SOHO Activity: Received via email Friday, 01 February 2008, -------------- 04:59:43 GMT: OBT DISTRIBUTED TO UVCS BY FOT EOF Staff: M. Uzzo: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 08.01.31.15:25:47.cmd.log 08.02.01.14:16:56.cmd.log Activity: --------- 1) Streamer Study OVI Observations Sequence: 08.01_StrObsOVI.tcl, sw = 21 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: 2008.01.31.15:35 end: 2008.01.31.20:18 ONUMs = 24035 (16 exps) 24036 (116 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35156) - Mirror/Occulter: 2.5 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: q08.01.31.15:34:22.ovi.dat GAP between 01/31/08|15:59:17( 4085) and 01/31/08|16:00:39( 4209) q08.01.31.16:08:32.ovi.dat GAP between 01/31/08|16:25:01( 6559) and 01/31/08|16:31:10( 7141) 2) Streamer Study OVI Observations Sequence: 08.02_StrObsOVI.tcl, sw = 22 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: 2008.01.31.20:19 end: 2008.02.01.08:03 ONUMs = 24037 (20 exps) 24038 (320 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35156) - Mirror/Occulter: 2.5 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: q08.01.31.20:18:09.ovi.dat q08.01.31.21:00:34.ovi.dat 3) Streamer Study OVI Observations Sequence: 08.02_StrObsOVI.tcl, sw = 22 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: 2008.02.01.08:05 end: 2008.02.01.16:53 ONUMs = 24039 (20 exps) 24040 (235 exps) ; aborted Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 270 Degrees (35156) - Mirror/Occulter: 2.5 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: q08.02.01.08:03:30.ovi.dat q08.02.01.08:45:55.ovi.dat GAP between 02/01/08|09:29:49( 6708) and 02/01/08|09:30:51( 6805)