UVCS MISSION LOG ---------------- Date: 12 Apr 2011 ----- Last revision: 4 Aug 2011 (RR) -------------- File Name: 2011.04.12.a.log ---------- Compiled by: R. Rosati ------------ UVCS Activity: Joint UVCS - Hinode/EIS Observations of South Polar -------------- Coronal Hole SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Rosati: Commander Command file: 11.04.12.16:18:31.cmd.log Activity: --------- 1) South Coronal Hole background observation. Sequence: Hole_BG 26957 51229 2 0 0 2 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2011.04.12.18:18 end: 2011.04.12.19:13 ONUMs = 26957 (27 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.2 Degrees (51229) - Mirror/Occulter: 5.0 Ro 1.5 mm exposed mirror - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 83040 - OVI GRTPOS: 98000 - OVI Filter Engaged - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q11.04.12.17:09:47.ovi.dat 2) South Coronal Hole observation coordinated with Hinode/EIS. OVI grating positioned so 1032 OVI line is placed on well-behaved region of OVI detector. Sequence: HoleOVI 26958 51229 17 0 2 0 0 2 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2011.04.12.19:15 end: 2011.04.13.01:19 ONUMs = 26958 (89 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.2 Degrees (51229) - Mirror/Occulter: 1.8 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 83040 - OVI GRTPOS: 98000 - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q11.04.12.23:15:18.ovi.dat 3) South Coronal Hole observation coordinated with Hinode/EIS. OVI grating positioned so 1037 OVI line is placed on same well-behaved region of OVI detector as the 1032 line. Sequence: HoleOVI 26959 51229 17 1 2 0 0 2 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2011.04.13.01:21 end: 2011.04.13.07:24 ONUMs = 26959 (11 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.2 Degrees (51229) - Mirror/Occulter: 1.8 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 83040 - OVI GRTPOS: 82900 - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q11.04.13.05:20:44.ovi.dat 4) South Coronal Hole observation coordinated with Hinode/EIS. OVI grating positioned so 1032 OVI line is placed on well-behaved region of OVI detector. Sequence: HoleOVI 26960 51207 17 0 2 0 0 2 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2011.04.13.07:26 end: 2011.04.13.09:01 ONUMs = 26960 (46 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.1 Degrees (51207) - Mirror/Occulter: 1.8 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 83040 - OVI GRTPOS: 98000 - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q11.04.13.11:26:10.ovi.dat 5) South Coronal Hole observation coordinated with Hinode/EIS. OVI grating positioned so 1037 OVI line is placed on same well-behaved region of OVI detector as the 1032 line. Sequence: HoleOVI 26961 51207 17 1 2 0 0 2 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 OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. 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: 2011.04.13.17:23 end: 2011.04.13.19:35 ONUMs = 26961 (64 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.1 Degrees (51207) - Mirror/Occulter: 1.8 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 83040 - OVI GRTPOS: 82900 - OVI MCP Voltage: 215 - OVI mask: OVI_Hole_237 in slot 2 Fits Files: q11.04.13.17:31:36.ovi.dat