UVCS MISSION LOG ---------------- Date: 11 July 2008 ----- Last revision: 17 July 2008 (Wu) -------------- File Name: 2008.07.11.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Ramp Down and Power off LyA Detector -------------- Turn on OVI Detector Conduct OVI Stimulus Pulse Test Ramp Up OVI Detector HV Load and Start OVI Detector Diagnostic for 11 July 2008 Load North Polar Coronal Hole OVI Observation for 11 July 2008 Load North Polar Coronal Hole OVI Observation for 11 - 12 July 2008 Load North Polar Coronal Hole OVI Observation for 12 - 13 July 2008 Load North Polar Coronal Hole LYA Observation for 13 July 2008 Load North Polar Coronal Hole OVI Observation for 13 - 14 July 2008 Load North Polar Coronal Hole OVI Observation for 14 - 15 July 2008 Load North Polar Coronal Hole OVI Observation for 15 - 16 July 2008 Flush Interactive Queue Ramp Down and Turn off OVI HV Load OVI Detector Mask OVI_EclipSyn_215 into OVI slot 2 Turn on and Ramp Up OVI HV Reload and Start North Polar Coronal Hole OVI Observation for 11 July 2008 Load North Polar Coronal Hole OVI Observation for 11 - 12 July 2008 Load North Polar Coronal Hole OVI Observation for 12 - 13 July 2008 Load North Polar Coronal Hole LYA Observation for 13 July 2008 Load North Polar Coronal Hole OVI Observation for 13 - 14 July 2008 Load North Polar Coronal Hole OVI Observation for 14 - 15 July 2008 Load North Polar Coronal Hole OVI Observation for 15 - 16 July 2008 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner, Commander Command file: 08.07.11.15:10:30.cmd.log Activity: --------- 1) OVI Stimulus Pulse Test Sequence: TakeUV_TxN.tcl SCI_SPEC: Calibration OBS_PROG: Calibration SCI_OBJ: Calibration OBJ: CMP_NAME: CMP_NUM: Duration: start: 2008.07.11.15:29 end: 2008.07.11.15:33 ONUMs = 24589 (2 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 5.0 Ro 0.8 mm occulting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA MCP Voltage: 0 - OVI MCP Voltage: 0 - OVI mask: OVI_303_8x2 in slot 3 Fits Files: q08.07.11.15:25:06.ovi.dat 2) OVI Detector Diagnostic Sequence: OVI_164_chk.tcl SCI_SPEC: Instrument Diagnostics OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.07.11.15:43 end: 2008.07.11.16:44 ONUMs = 24590 (12 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: q08.07.11.15:42:00.ovi.dat 3) North Polar Coronal Hole Observations Sequence: 08.01_hole.tcl, n = 1, m = 0, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=0 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.07.11.16:48 end: 2008.07.11.19:50 ONUMs = 24591 (88 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50111) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp2_164 in slot 4 Fits Files: q08.07.11.16:47:42.ovi.dat 4) North Polar Coronal Hole Observations Sequence: 08.01_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=0 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.07.11.19:51 end: 2008.07.12.20:00 ONUMs = 24592 ( exps) ; aborted Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50111) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: StarFF_4x4 in slot 2 Fits Files: q08.07.11.19:51:21.ovi.dat 5) North Polar Coronal Hole Observations Sequence: 08.01_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=0 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.07.11.20:28 end: 2008.07.12.19:26 ONUMs = 24593 (319 exps) 24594 (347 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50111) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: q08.07.11.20:27:43.ovi.dat q08.07.12.07:29:03.ovi.dat