UVCS MISSION LOG ---------------- Date: 02 February 2004 ----- Last revision: 16 February 2004 (Wu) -------------- File Name: 2004.02.01.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Streamer Study for 01 - 02 February 2004 -------------- Streamer Study for 02 February 2004 OVI Synoptic for 02 February 2004 SOHO Activity: -------------- EOF Staff: L. Strachan: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 04.01.30.15:20:56.cmd.log Activity: --------- 1) Streamer Properties Over the Solar Cycle Sequence: 04.01_StrObsV1.tcl, sw = 5 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: Coronal Dynamics...Outflow Velocities Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2004.02.01.13:41 end: 2004.02.02.00:06 ONUMs = 20907 (16 exps) 20908 (269 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 40 Degrees (58833) - Mirror/Occulter: 5.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 188940, 225000 - OVI MCP Voltage: 200 - OVI mask: OVI_str_188_225 in slot 5 Fits Files: q04.02.01.13:40:19.ovi.dat q04.02.01.13:40:19.vld.dat q04.02.01.14:16:02.ovi.dat q04.02.01.14:16:02.vld.dat GAP between 02/01/04|20:30:22( 1285) and 02/01/04|20:32:07( 1454) 2) Streamer Properties Over the Solar Cycle Sequence: 04.01_StrObsV1.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: Coronal Dynamics...Outflow Velocities Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2004.02.02.00:09 end: 2004.02.02.01:36 ONUMs = 20909 (8 exps) 20910 (32 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 30 Degrees (57012) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 128000 - OVI GRTPOS: 188940, 225000 - OVI MCP Voltage: 200 - OVI mask: OVI_str_188_225 in slot 5 Fits Files: q04.02.02.00:07:27.ovi.dat q04.02.02.00:07:27.vld.dat q04.02.02.00:25:59.ovi.dat q04.02.02.00:25:59.vld.dat 3) OVI Synoptic Sequence Load and Start Sequence: SynopticOVI:Start SCI_SPEC: Synoptic studies. LYA HV & Power off / OVI voltage at 200, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2004.02.02.01:41 end: 2004.02.02.14:41 ONUMs = 44310 (56 exps) 44311 (36 exps) 44312 (37 exps) 44313 (37 exps) 44314 (37 exps) 44315 (37 exps) 44316 (37 exps) 44317 (37 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: NE: STR1A, N: STR2B, NW: STR2B, W: STR2B, SW: STR2B, S: STR2B, SE: STR2B, E: STR2B - Mirror/Occulter: STR1A: 3.50, 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro STR2B: 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro STR4B: 4.00 Ro CH1A: 1.90, 1.75, 1.60 Ro 1.5 mm overocculting (1.60 Ro) 2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00, 3.50, 4.00 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (STR1A, STR2B, STR4B, CH1A) - LYA GRTPOS: 128000 - OVI GRTPOS: 228200 - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_230 in slot 1 Fits Files: z04.02.02.01:40:07.ovi.dat z04.02.02.01:40:07.vld.dat z04.02.02.03:56:15.ovi.dat z04.02.02.03:56:15.vld.dat z04.02.02.05:28:59.ovi.dat z04.02.02.05:28:59.vld.dat z04.02.02.07:01:51.ovi.dat z04.02.02.07:01:51.vld.dat z04.02.02.08:34:47.ovi.dat z04.02.02.08:34:47.vld.dat z04.02.02.10:07:43.ovi.dat z04.02.02.10:07:43.vld.dat z04.02.02.11:40:27.ovi.dat z04.02.02.11:40:27.vld.dat z04.02.02.13:13:11.ovi.dat z04.02.02.13:13:11.vld.dat 4) Streamer Properties Over the Solar Cycle Sequence: 04.01_StrObsV1.tcl, sw = 2 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. This observation was flushed before it began. OBS_PROG: Primary: Spectral Resolution Sub Obj: Spatial Resolution SCI_OBJ: Coronal Dynamics...Outflow Velocities Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2004.02.02. end: 2004.02.02. ONUMs = 20911 (216 exps) ; not run 20912 (3 VL exps) ; not run 20913 (120 exps) ; not run 20914 (16 exps) ; not run 20915 (88 exps) ; not run Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 40 Degrees (58833) - Mirror/Occulter: 2.5 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 235800, 111000, 188940, 225000 - OVI MCP Voltage: 200 - OVI mask: msk_000303_OVI in slot 3 OVI_str_188_225 in slot 5 Fits Files: