UVCS MISSION LOG ---------------- Date: 09 September 2009 ----- Last revision: 17 September 2009 (Wu) -------------- File Name: 2009.09.10.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start North Coronal Hole Study (LyA Primary) -------------- for 10 - 11 September 2009 Load North Coronal Hole Study (LyA Primary) for 11 September 2009 Load North Coronal Hole Study (LyA Primary) for 11 September 2009 Load LYA Detector Dark Diagnostic for 11 September 2009 Load Proton Velocity Distribution Measurements Observation for 11 - 13 September 2009 Load Proton Velocity Distribution Measurements Observation for 13 September 2009 Load LYA Detector Dark Diagnostic for 13 September 2009 Load HERSCHEL Sounding Rocket Launch Observations for 13 September 2009 Load HERSCHEL Sounding Rocket Launch Observations for 13 September 2009 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 09.09.09.13:32:03.cmd.log Activity: --------- 1) North Coronal Hole Study (LyA Primary) Sequence: 09.09_LYAhole.tcl, ro = 17, n = 1, m = 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: 2009.09.10.21:51 end: 2009.09.11.00:36 ONUMs = 25796 (63 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: Hi Res center at 0 Degrees (21584) - 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: q09.09.10.21:50:50.lya.dat GAP between 09/10/09|23:25:04( 7376) and 09/11/09|00:00:36(10791) 2) North Coronal Hole Study (LyA Primary) Sequence: 09.09_LYAhole.tcl, ro = 20, n = 1, m = 1, 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: 2009.09.11.00:37 end: 2009.09.11.04:04 ONUMs = 25797 (100 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: Hi Res center at 0 Degrees (21165) - Mirror/Occulter: 2.0 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: q09.09.11.00:37:17.lya.dat 3) North Coronal Hole Study (LyA Primary) Sequence: 09.09_LYAhole.tcl, ro = 24, m = 5, r = 0, e = 2 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: 2009.09.11.04:05 end: 2009.09.11.10:58 ONUMs = 25798 (199 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: Hi Res center at 0 (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: 195 - LYA mask: LYA_VEX_4x1 in slot 2 Fits Files: q09.09.11.04:05:02.lya.dat 4) LYA Detector Dark Rate Diagnostic Sequence: LYA_dark_chk.tcl SCI_SPEC: Calibration OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2009.09.11.11:00 end: 2009.09.11.12:01 ONUMs = 25799 (12 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 0 Degrees (18762) - Mirror/Occulter: 5.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 210000 - LYA Filter Engaged - LYA MCP Voltage: 200 - LYA mask: LYA_chk_1xfull in slot 6 Fits Files: q09.09.11.11:00:23.lya.dat