UVCS MISSION LOG ---------------- Date: 30 December 2005 ----- Last revision: 17 February 2006 (Wu) -------------- File Name: 2006.01.01.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Equatorial Coronal Hole LyA Observation for -------------- 01 January 2006 Equatorial Coronal Hole LyA Observation for 01 January 2006 Equatorial Coronal Hole OVI Observation for 01 January 2006 Equatorial Coronal Hole OVI Observation for 01 - 02 January 2006 Equatorial Coronal Hole OVI Observation for 02 January 2006 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 05.12.30.19:23:12.cmd.log Activity: --------- 1) Equatorial Coronal Hole Observation Sequence: 06.01_hole1LyA.tcl SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=275 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: 2006.01.01.05:02 end: 2006.01.01.09:37 ONUMs = 22070 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 267.09, 267.92, 269.14 degrees (34626, 34777, 34999) - Mirror/Occulter: 1.7, 1.9, 2.3 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q06.01.01.04:48:39.ovi.dat 2) Equatorial Coronal Hole Observation Sequence: 06.01_hole1LyA.tcl SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=275 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: 2006.01.01.09:38 end: 2006.01.01.14:12 ONUMs = 22071 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 267.09, 267.92, 269.14 degrees (34626, 34777, 34999) - Mirror/Occulter: 1.7, 1.9, 2.3 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q06.01.01.09:37:07.ovi.dat 3) Equatorial Coronal Hole Observation Sequence: 06.01_hole1OVI.tcl SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=270 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: 2006.01.01.14:14 end: 2006.01.01.23:40 ONUMs = 22072 (105 exps) 22073 (164 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 267.09, 267.92, 269.14 degrees (34626, 34777, 34999) - Mirror/Occulter: 1.7, 1.9, 2.3 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q06.01.01.14:12:51.ovi.dat q06.01.01.17:51:45.ovi.dat GAP between 01/01/06|21:16:38( 9773) and 01/01/06|21:25:08(10589) 4) Equatorial Coronal Hole Observation Sequence: 06.01_hole1OVI.tcl SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=270 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: 2006.01.01.23:41 end: 2006.01.02.09:07 ONUMs = 22074 (105 exps) 22075 (168 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 267.09, 267.92, 269.14 degrees (34626, 34777, 34999) - Mirror/Occulter: 1.7, 1.9, 2.3 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q06.01.01.23:40:06.ovi.dat q06.01.02.03:18:52.ovi.dat 5) Equatorial Coronal Hole Observation Sequence: 06.01_holexOVI.tcl, n50min = 8 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=270 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: 2006.01.02.09:08 end: 2006.01.02.16:40 ONUMs = 22076 (14 exps) 22077 (132 exps) 22078 (72 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 267.09, 269.14 degrees (34626, 34999) - Mirror/Occulter: 1.7, 2.3 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50, 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q06.01.02.09:07:13.ovi.dat q06.01.02.09:37:19.ovi.dat q06.01.02.14:10:50.ovi.dat