UVCS MISSION LOG ---------------- Date: 28 September 2007 ----- Last revision: 22 October 2007 (Wu) -------------- File Name: 2007.10.01.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Equatorial Coronal Hole LYA Observation for -------------- 01 October 2007 Equatorial Coronal Hole LYA Observation for 01 October 2007 Equatorial Coronal Hole LYA Observation for 01 October 2007 Equatorial Coronal Hole OVI Observation for 01 October 2007 Equatorial Coronal Hole OVI Observation for 01 October 2007 Equatorial Coronal Hole OVI Observation for 01 - 02 October 2007 Load North Coronal Hole OVI Observation for 02 - 03 October 2007 Load North Coronal Hole OVI Observation for 03 - 04 October 2007 Load OVI Detector Diagnostic for 04 October 2007 Load North Coronal Hole LYA Observation for 04 October 2007 Load North Coronal Hole OVI Observation for 04 - 05 October 2007 SOHO Activity: Received via email Wednesday, 02 October 2007, -------------- 04:00:39 GMT: OBT DISTRIBUTED TO UVCS BY FOT EOF Staff: S. Cranmer: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Commander M. Uzzo: Planner Command file: 07.09.29.13:30:00.cmd.log 07.10.01.13:05:36.cmd.log Activity: --------- 1) Equatorial Polar Coronal Hole LYA Observations Sequence: 06.08_hole.tcl, n = 0, m = 1, p = 1, r = 0, e = 0 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of an equatorial 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=245 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: 2007.10.01.09:51 end: 2007.10.01.10:53 ONUMs = 23718 (30 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 237.093 Degrees (61944) - 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: q07.10.01.09:50:36.ovi.dat 2) Equatorial Polar Coronal Hole LYA Observations Sequence: 06.08_hole.tcl, n = 0, m = 2, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of an equatorial 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=245 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: 2007.10.01.10:54 end: 2007.10.01.12:34 ONUMs = 23719 (48 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 238.267 Degrees (62158) - Mirror/Occulter: 2.0 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: q07.10.01.10:54:23.ovi.dat 3) Equatorial Polar Coronal Hole LYA Observations Sequence: 06.08_hole.tcl, n = 0, m = 2, p = 1, r = 1, e = 0 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of an equatorial 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=245 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: 2007.10.01.12:36 end: 2007.10.01.14:36 ONUMs = 23720 (58 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 239.381 Degrees (62361) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp2_164 in slot 4 Fits Files: q07.10.01.12:35:53.ovi.dat 4) Equatorial Polar Coronal Hole OVI Observations Sequence: 06.08_hole.tcl, n = 0, m = 1, p = 1, r = 0, e = 0 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of an equatorial 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=245 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: 2007.10.01.14:38 end: 2007.10.01.15:40 ONUMs = 23721 (30 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 237.093 Degrees (61944) - 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: q07.10.01.14:38:09.ovi.dat 5) Equatorial Polar Coronal Hole OVI Observations Sequence: 06.08_hole.tcl, n = 1, m = 2, p = 0, r = 0, e = 0 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of an equatorial 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=245 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: 2007.10.01.15:42 end: 2007.10.01.19:49 ONUMs = 23722 (120 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 238.267 Degrees (62158) - Mirror/Occulter: 2.0 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: q07.10.01.15:42:02.ovi.dat 6) Equatorial Polar Coronal Hole OVI Observations Sequence: 06.08_hole.tcl, n = 8, m = 3, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of an equatorial 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=245 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: 2007.10.01.19:52 end: 2007.10.02.20:15 ONUMs = 23723 (320 exps) 23724 (388 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 239.381 Degrees (62361) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: q07.10.01.19:52:20.ovi.dat q07.10.02.06:53:40.ovi.dat