UVCS MISSION LOG ---------------- Date: 02 July 2008 ----- Last revision: 07 July 2008 (Wu) -------------- File Name: 2008.07.03.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start Polar Plume Observations for 03 July 2008 -------------- Load Polar Plume Observations for 03 - 04 July 2008 Load Polar Plume Observations for 04 July 2008 Load Polar Plume Observations for 04 July 2008 Load LyA Detector Diagnostic for 04 July 2008 Load Suprathermal Seed Particle Observations for 04 - 05 July 2008 Load Suprathermal Seed Particle Observations for 05 July 2008 Load Suprathermal Seed Particle Observations for 05 - 06 July 2008 Load Suprathermal Seed Particle Dark Count Observations for 06 - 07 July 2008 SOHO Activity: -------------- EOF Staff: G. Poletto: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 08.07.03.11:59:31.cmd.log Activity: --------- 1) Polar Plume Observations Sequence: 08.06_Poletto.tcl, sw = 17 SCI_SPEC: Plume vs. interplume observations with the aim of 1) defining plume properties, with the help of other coordinated observations from TRACE, STEREO, possibly HINODE, 2) check whether wind originates preferentially from plume or interplume regions. Targeting high resolution portion of detector at 180 deg. OBS_PROG: Primary: Spatial Resolution Sub Obj: Temporal Coverage SCI_OBJ: Primary: Coronal Dynamics...Outflow Velocities Sub Obj: Coronal Structure...Fine Structure OBJ: Polar Plume CMP_NAME: Polar Plume Observations, UVCS; SUMER CMP_NUM: 7276 Duration: start: 2008.07.03.19:54 end: 2008.07.03.21:58 ONUMs = 24574 (60 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 195.5 Degrees (21584) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 75 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 200 - LYA mask: LYA_VEX_4x1 in slot 2 Fits Files: q08.07.03.19:53:40.lya.dat 2) Polar Plume Observations Sequence: 08.06_Poletto.tcl, sw = 20 SCI_SPEC: Plume vs. interplume observations with the aim of 1) defining plume properties, with the help of other coordinated observations from TRACE, STEREO, possibly HINODE, 2) check whether wind originates preferentially from plume or interplume regions. Targeting high resolution portion of detector at 180 deg. OBS_PROG: Primary: Spatial Resolution Sub Obj: Temporal Coverage SCI_OBJ: Primary: Coronal Dynamics...Outflow Velocities Sub Obj: Coronal Structure...Fine Structure OBJ: Polar Plume CMP_NAME: Polar Plume Observations, UVCS; SUMER CMP_NUM: 7276 Duration: start: 2008.07.03.21:59 end: 2008.07.04.00:44 ONUMs = 24575 (80 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 193.2 Degrees (21165) - Mirror/Occulter: 2.0 Ro 1.5 mm overocculting - LYA Slit: 75 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 200 - LYA mask: LYA_VEX_4x1 in slot 2 Fits Files: q08.07.03.21:58:35.lya.dat 3) Polar Plume Observations Sequence: 08.06_Poletto.tcl, sw = 24 SCI_SPEC: Plume vs. interplume observations with the aim of 1) defining plume properties, with the help of other coordinated observations from TRACE, STEREO, possibly HINODE, 2) check whether wind originates preferentially from plume or interplume regions. Targeting high resolution portion of detector at 180 deg. OBS_PROG: Primary: Spatial Resolution Sub Obj: Temporal Coverage SCI_OBJ: Primary: Coronal Dynamics...Outflow Velocities Sub Obj: Coronal Structure...Fine Structure OBJ: Polar Plume CMP_NAME: Polar Plume Observations, UVCS; SUMER CMP_NUM: 7276 Duration: start: 2008.07.04.00:45 end: 2008.07.04.06:40 ONUMs = 24576 (172 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 191.1 Degrees (20783) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 75 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 200 - LYA mask: LYA_VEX_4x1 in slot 2 Fits Files: q08.07.04.00:44:49.lya.dat 4) Polar Plume Observations Sequence: 08.06_Poletto.tcl, sw = 30 SCI_SPEC: Plume vs. interplume observations with the aim of 1) defining plume properties, with the help of other coordinated observations from TRACE, STEREO, possibly HINODE, 2) check whether wind originates preferentially from plume or interplume regions. Targeting high resolution portion of detector at 180 deg. OBS_PROG: Primary: Spatial Resolution Sub Obj: Temporal Coverage SCI_OBJ: Primary: Coronal Dynamics...Outflow Velocities Sub Obj: Coronal Structure...Fine Structure OBJ: Polar Plume CMP_NAME: Polar Plume Observations, UVCS; SUMER CMP_NUM: 7276 Duration: start: 2008.07.04.06:41 end: 2008.07.04.19:46 ONUMs = 24577 (360 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 188.9 Degrees (20382) - Mirror/Occulter: 3.0 Ro 1.5 mm overocculting - LYA Slit: 75 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 200 - LYA mask: LYA_VEX_4x1 in slot 2 Fits Files: q08.07.04.06:41:12.lya.dat 5) LYA Detector Diagnostic Sequence: LYA_100_chk.tcl SCI_SPEC: Calibration OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.07.04.19:48 end: 2008.07.04.20:19 ONUMs = 24578 (6 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180 Degrees (18762) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 200 (Nominal +5) - LYA mask: LYA_chk_1xfull in slot 6 Fits Files: q08.07.04.19:46:46.lya.dat