UVCS MISSION LOG ---------------- Date: 28 January 2004 ----- Last revision: 29 January 2004 (Wu) -------------- File Name: 2004.01.28.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Flush and Abort Streamer Study for 29 January 2004 -------------- Begin ESR Simulation Stop ESR Simulation Load and Start Streamer Study for 28 - 29 January 2004 Load Streamer Study for 29 January 2004 SOHO Activity: -------------- EOF Staff: L. Strachan: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 04.01.28.13:15:50.cmd.log Activity: --------- 1) ESR Simulation Sequence: Manual SCI_SPEC: The detectors are switched off and the door was SUPPOSED to be partially closed but was not to simulate a condition UVCS would be in if an ESR occured. The detectors are switched on for a short period at intervals of approximately 1 hour and all of the temperatures are recorded. The purpose is to determine how the temperatures fall during an ESR which occurs during long gaps in contact and substitution heaters can not be turned on by the FOT. OBS_PROG: UVCS Temperature Response SCI_OBJ: OBJ: CMP_NAME: CMP_NUM: Duration: start: 2004.01.28.13:35 end: 2004.01.28.15:59 ONUMs = 20874 (0 exps) ; ABORTED due to door being left open Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 275 Degrees (36066) - Mirror/Occulter: 5.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 225000 - OVI mask: OVI_str_188_225 in slot 5 Fits Files: 2) Streamer Properties Over the Solar Cycle Sequence: 04.01_StrObsV1.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: Coronal Dynamics...Outflow Velocities Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2004.01.28.16:02 end: 2004.01.29.02:03 ONUMs = 20878 (111 exps) 20879 (9 VL exps) 20880 (56 exps) 20881 (56 exps) 20882 (8 exps) 20883 (32 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 220 Degrees (26044) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 235800, 229000, 111000, 188940, 225000 - OVI MCP Voltage: 200 - OVI mask: msk_000303_OVI in slot 3 OVI_str_188_225 in slot 5 Fits Files: q04.01.28.16:00:58.ovi.dat q04.01.28.16:00:58.vld.dat q04.01.28.20:04:36.vld.dat q04.01.28.20:29:05.ovi.dat q04.01.28.20:29:05.vld.dat q04.01.28.22:31:20.ovi.dat q04.01.28.22:31:20.vld.dat q04.01.29.00:34:14.ovi.dat q04.01.29.00:34:14.vld.dat q04.01.29.00:52:52.ovi.dat q04.01.29.00:52:52.vld.dat 3) Streamer Properties Over the Solar Cycle Sequence: 04.01_StrObsV1.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: Coronal Dynamics...Outflow Velocities Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2004.01.28.02:06 end: 2004.01.29.13:02 ONUMs = 20885 (8 exps) 20886 (32 exps) 20887 (8 exps) 20888 (87 exps) 20889 (16 exps) 20890 (149 exps) ; aborted Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 275 Degrees (36066) - Mirror/Occulter: 1.75, 2.5, 3.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 188940, 225000 - OVI MCP Voltage: 200 - OVI mask: OVI_str_188_225 in slot 5 Fits Files: q04.01.29.02:04:13.ovi.dat q04.01.29.02:04:13.vld.dat q04.01.29.02:22:48.ovi.dat q04.01.29.02:22:48.vld.dat q04.01.29.03:33:06.ovi.dat q04.01.29.03:33:06.vld.dat q04.01.29.03:51:29.ovi.dat q04.01.29.03:51:29.vld.dat q04.01.29.07:03:01.ovi.dat q04.01.29.07:03:01.vld.dat q04.01.29.07:38:44.ovi.dat q04.01.29.07:38:44.vld.dat