UVCS MISSION LOG ---------------- Date: 01 July 2009 ----- Last revision: 10 July 2009 (Wu) -------------- File Name: 2009.07.09.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: North Coronal Hole Study for 09 - 10 July 2009 -------------- Flush IQ & BQ Abort North Coronal Hole Study for 09 - 10 July 2009 Load Patrol_Safe_Test as Embedded Sequence ID=2137.FP=3252 Set ID=2137.FP=3252 as PStart Sequence Load North Coronal Hole Study for 09 July 2009 Load OVI Detector Dark Rate Diagnostic for 09 July 2009 Load OVI Detector Rate Diagnostic for 09 July 2009 Sent Patrol Start Command but UVCS Failed to Execute Embedded Routine Load and Start North Coronal Hole Study for 09 - 10 July 2009 Load North Coronal Hole Study for 10 - 11 July 2009 Load OVI Detector Dark Rate Diagnostic for 11 July 2009 Load North Coronal Hole Study for 11 - 12 July 2009 Load North Coronal Hole Study for 12 - 13 July 2009 Load OVI Detector Dark Rate Diagnostic for 13 July 2009 Load North Coronal Hole Study for 13 - 14 July 2009 SOHO Activity: -------------- EOF Staff: M. P. Miralles / J. Kohl / L. Gardner: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 09.07.06.12:10:56.cmd.log 09.07.09.13:06:06.cmd.log Activity: --------- 1) North Polar Coronal Hole Study Sequence: 09.07_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: 2009.07.09.09:52 end: 2009.07.09.13:08 ONUMs = 25611 (95 exps) ; aborted Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50331) - Mirror/Occulter: 2.1 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 232100 - OVI MCP Voltage: 205 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q09.07.09.09:51:41.ovi.dat 2) North Polar Coronal Hole Study Sequence: 09.07_hole.tcl, n = 0, m = 3, p = 0, r = 0, 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: 2009.07.09.13:50 end: 2009.07.09.15:54 ONUMs = 25612 (60 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50331) - Mirror/Occulter: 2.1 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 232100 - OVI MCP Voltage: 205 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q09.07.09.13:49:39.ovi.dat 3) OVI Detector Dark Rate Diagnostic Sequence: OVI_dark_chk.tcl SCI_SPEC: Determine Dark count rate for OVI detector. Instrument rolled to coronal hole, 5.0 Ro with 0.8 mm exposed mirror. Script engages OVI filter and then disengages it at end. OBS_PROG: Calibration SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2009.07.09.15:56 end: 2009.07.09.16:57 ONUMs = 25613 (12 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 5.0 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - OVI Filter Engaged - OVI MCP Voltage: 205 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: q09.07.09.15:56:05.ovi.dat GAP between 07/09/09|16:04:08( 7021) and 07/09/09|16:06:10( 7216) 4) OVI Detector Diagnostic Sequence: OVI_164_chk.tcl SCI_SPEC: Instrument Diagnostics Attempted to start Patrol function which would have interrupted this observation but function failed to do so. OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2009.07.09.16:58 end: 2009.07.09.17:59 ONUMs = 25614 (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: 205 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: q09.07.09.16:56:59.ovi.dat 5) North Polar Coronal Hole Study Sequence: 09.07_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: 2009.07.09.18:07 end: 2009.07.10.17:08 ONUMs = 25615 (320 exps) 25616 (348 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 352.09 Degrees (50331) - Mirror/Occulter: 2.1 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 232100 - OVI MCP Voltage: 205 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q09.07.09.18:07:27.ovi.dat GAP between 07/10/09|04:11:15(11340) and 07/10/09|04:12:31(11464) q09.07.10.05:08:47.ovi.dat