UVCS MISSION LOG ---------------- Date: 17 March 2009 ----- Last revision: 19 March 2009 (Wu) -------------- File Name: 2009.03.17.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Equatorial Coronal Observation for 17 March 2009 -------------- Equatorial Coronal Observation for 17 - 18 March 2009 Flush and Abort Equatorial Coronal Observation for 17 March 2009 Load and Start Equatorial Coronal Observation for 17 - 18 March 2009 Load Equatorial Coronal Observation for 18 March 2009 SOHO Activity: -------------- EOF Staff: M. Uzzo: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: 09.03.16.13:09:00.cmd.log 09.03.17.15:59:00.cmd.log Activity: --------- 1) Equatorial Coronal Observation Sequence: 09.03_StrProfOVI.tcl, sw = 17, n11 = 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...Nonthermal Velocities Sub Obj: Plasma Properties...Proton Temperature OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2009.03.17.05:33 end: 2009.03.18.16:02 ONUMs = 25235 (20 exps) 25236 (284 exps) ; aborted Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 75 Degrees (32425) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600, 235900 - OVI MCP Voltage: 205 - OVI mask: OVI_str_Prof09 in slot 5 Fits Files: q09.03.17.05:32:31.ovi.dat q09.03.17.06:14:58.ovi.dat 2) Equatorial Coronal Observation Sequence: 09.03_StrProfOVI.tcl, sw = 30, n11 = 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...Nonthermal Velocities Sub Obj: Plasma Properties...Proton Temperature OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2009.03.17.16:25 end: 2009.03.18.04:42 ONUMs = 25240 (20 exps) 25241 (336 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 263 Degrees (1104) - Mirror/Occulter: 3.00 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600, 235900 - OVI MCP Voltage: 205 - OVI mask: OVI_str_Prof09 in slot 5 Fits Files: q09.03.17.16:25:22.ovi.dat q09.03.17.17:07:49.ovi.dat 3) Equatorial Coronal Observation Sequence: 09.03_StrProfOVI.tcl, sw = 40, n11 = 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...Nonthermal Velocities Sub Obj: Plasma Properties...Proton Temperature OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2009.03.18.04:44 end: 2009.03.18.17:01 ONUMs = 25242 (20 exps) 25243 (333 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 263 Degrees (1104) - Mirror/Occulter: 4.00 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600, 235900 - OVI MCP Voltage: 205 - OVI mask: OVI_str_Prof09 in slot 5 Fits Files: q09.03.18.04:44:02.ovi.dat q09.03.18.05:26:29.ovi.dat GAP between 03/18/09|06:02:31(11760) and 03/18/09|06:03:35(11864)