UVCS MISSION LOG ---------------- Date: 16 February 2005 ----- Last revision: 22 February 2005 (Wu) -------------- File Name: 2005.02.17.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Load mask OVI_Syn_188 in slot 2 -------------- Load mask OVI_str_164_225 in slot 4 Load and Start Vignetting Function Measurement for 17 February 2005 Load Streamer Study for 17 - 18 February 2005 Flush IQ and Reload Observations SOHO Activity: -------------- EOF Staff: L. Gardner: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 05.02.17.12:58:48.cmd.log Activity: -------- 1) Detector Characterization: Vignetting Function Measurement : Part 2 Sequence: 05.02_cal_occ.tcl, 05.02_cal_occ_mini.tcl, r = 2, 3 SCI_SPEC: Vignetting function tests. Observe signal in OVI channel as a function of occulter position for several fixed mirror positions: mirror 2.5 Ro scan occulter 1.3 - 2.3 Ro (0.8-8.7 mm) mirror 3.5 Ro " " 2.1 - 3.3 Ro (7.12-16.62mm) mirror 4.5 Ro " " 3.0 - 4.3 Ro (14.24-24.53mm) This test is to determine the change of mirror efficiency with time. OBS_PROG: Calibration SCI_OBJ: Calibration...Vignetting OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2005.02.17.13:03 end: 2005.02.17.19:14 ONUMs = 22126 (26 exps) 22127 (33 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 140 Degrees (11480) @ r=2.5 35 Degrees (57923) @ r=3.5 - Mirror/Occulter: 2.5 Ro: 8.70, 0.80, 1.58, 3.16, 5.50, 7.12, 8.70, 0.80, 1.58, 3.16, 5.50, 7.12, 8.70 mm 3.5 Ro: 16.62, 7.12, 8.70, 11.08, 12.66, 16.62, 7.12, 8.70, 11.08, 12.66, 16.62 mm - LYA Slit: 50 um - OVI Slit: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 188100 - OVI MCP Voltage: 200 - OVI mask: msk_000303_OVI in slot 3 Fits Files: q05.02.17.13:02:46.ovi.dat q05.02.17.16:21:16.ovi.dat 2) Streamer Properties Over the Solar Cycle Sequence: 05.02_StrObsV2.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: 2005.02.17.19:16 end: 2005.02.18.20:11 ONUMs = 22130 (350 exps) 22131 (80 exps) 22132 (40 exps) 22133 (193 exps) 22134 (8 exps) 22135 (40 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 35 Degrees (57923) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100, 50 um - LYA GRTPOS: 128000 - OVI GRTPOS: 232100, 86600, 67500, 46000, 164600, 223500 - OVI MCP Voltage: 200 - OVI mask: msk_000303_OVI in slot 3 OVI_str_164_225 in slot 4 Fits Files: q05.02.17.19:14:34.ovi.dat q05.02.18.07:23:06.ovi.dat q05.02.18.10:10:36.ovi.dat q05.02.18.11:34:16.ovi.dat GAP between 02/18/05|13:39:57( 2290) and 02/18/05|13:41:42( 2456) GAP between 02/18/05|13:44:25( 2718) and 02/18/05|13:47:29( 3013) q05.02.18.18:29:10.ovi.dat q05.02.18.18:46:59.ovi.dat