UVCS MISSION LOG ---------------- Date: 30 October 2007 ----- Last revision: 20 November 2007 (Wu) -------------- File Name: 2007.11.01.a.log ---------- Compiled by: M. Uzzo, R. Wu, Y.-K. Ko ------------ UVCS Activity: Load SOHO / Hinode Polar Plumes OVI Campaign for -------------- 01 - 02 November 2007 Load SOHO / Hinode Polar Plumes LYA Campaign for 02 November 2007 SOHO Activity: -------------- EOF Staff: G. Poletto: Lead Scientist ---------- Y.-K. Ko: Planner M. Uzzo: Commander Command file: 07.11.01.12:03:47.cmd.log Activity: --------- 1) SOHO/Hinode Polar Plumes Campaign, JOP197 Sequence: 07.10_Plume_ovi.tcl, n3h = 7, n50m = 2, n21m = 0 SCI_SPEC: To characterize the physical parameters (densities, temperatures, abundance, flows) of coronal hole plumes with coordinated multi-spacecraft observations, and relate changes in the photospheric magnetic fields with changes in the observed plasma properties in order to understand the physical processes that lead to the formation of these stable structures. Roll angle is such that row 290 is at the target angle of PA = 0 degrees OBS_PROG: Primary: Temporal Coverage Sub Obj: Spatial Coverage SCI_OBJ: Primary: Coronal Structure...Fine Structure Sub Obj: Coronal Dynamics...Outflow Velocities OBJ: Polar Plume CMP_NAME: Multi-wavelength observations of coronal hole plumes at solar minimum, JOP197 CMP_NUM: 7243 Duration: start: 2007.11.01.21:10 end: 2007.11.02.18:07 ONUMs = 23798 (240 exps) 23799 (240 exps) 23800 (128 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 20.0 Degrees (22400) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 200 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_Plume_217 in slot 1 Fits Files: q07.11.01.21:10:19.ovi.dat q07.11.02.05:26:19.ovi.dat q07.11.02.13:42:19.ovi.dat 2) SOHO/Hinode Polar Plumes Campaign, JOP197 Sequence: 07.10_Plume_lyared.tcl SCI_SPEC: To characterize the physical parameters (densities, temperatures, abundance, flows) of coronal hole plumes with coordinated multi-spacecraft observations, and relate changes in the photospheric magnetic fields with changes in the observed plasma properties in order to understand the physical processes that lead to the formation of these stable structures. Roll angle is such that row 290 is at the target angle of PA = 0 degrees OBS_PROG: Primary: Temporal Coverage Sub Obj: Spatial Coverage SCI_OBJ: Primary: Coronal Structure...Fine Structure Sub Obj: Coronal Dynamics...Outflow Velocities OBJ: Polar Plume CMP_NAME: Multi-wavelength observations of coronal hole plumes at solar minimum, JOP197 CMP_NUM: 7243 Duration: start: 2007.11.02.18:08 end: 2007.11.02.20:08 ONUMs = 23801 (58 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 20.0 Degrees (22400) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 200 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp2_164 in slot 4 Fits Files: q07.11.02.18:08:07.ovi.dat