UVCS MISSION LOG ---------------- Date: 30 June 2008 ----- Last revision: 03 July 2008 (Wu) -------------- File Name: 2008.06.30.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start Polar Plume Observations for 30 June 2008 -------------- Load Polar Plume Observations for 30 June - 01 July 2008 Load Polar Plume Observations for 01 July 2008 Load Polar Plume Observations for 01 July 2008 Load Eruptive and Quiescent Prominences Atlas Observation for 01 July 2008 Flush and Reload Polar Plume Observations for 01 July 2008 Load Eruptive and Quiescent Prominences Atlas Observation for 01 July 2008 SOHO Activity: Received via email Tuesday, 01 July 2008, -------------- 03:59:43 GMT: OBT DISTRIBUTED TO UVCS BY FOT EOF Staff: G. Poletto / S. Parenti: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 08.06.30.12:44:15.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: 2008.06.30.20:01 end: 2008.06.30.22:05 ONUMs = 24556 (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: q08.06.30.20:01:27.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: 2008.06.30.22:06 end: 2008.07.01.00:52 ONUMs = 24557 (79 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: q08.06.30.22:06:23.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: 2008.07.01.00:53 end: 2008.07.01.06:48 ONUMs = 24558 (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: q08.07.01.00:52:38.lya.dat 4) 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: 2008.07.01.06:49 end: 2008.07.01.08:53 ONUMs = 24559 (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: q08.07.01.06:49:14.lya.dat 5) Eruptive and Quiescent Prominences Atlas Observation Sequence: 08.06_JOP207.tcl, m = 15, r = 1, e = 0 SCI_SPEC: OBS_PROG: Primary: Sub Obj: SCI_OBJ: Primary: Sub Obj: OBJ: CMP_NAME: Eruptive and Quiescent Prominences Atlas, CDS; SUMER; UVCS; Hinode-EIS (S/C); Hinode-SOT (S/C); Hinode-XRT (S/C) CMP_NUM: 7280 Duration: start: 2008.07.01.09:08 end: 2008.07.01.19:44 ONUMs = 24560 (240 exps) 24561 (68 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 341.5 (326 target) Degrees (48183) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 50 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: q08.07.01.09:07:47.lya.dat q08.07.01.17:23:47.lya.dat