UVCS MISSION LOG ---------------- Date: 13 Apr 2011 ----- Last revision: 4 Aug 2011 (RR) -------------- File Name: 2011.04.13.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: 11.04.13.22:52:48.cmd.log Activity: --------- 1) South Coronal Hole background observation. Sequence: Hole_BG 26962 51207 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: 2011.04.13.19:37 end: 2011.04.13.20:49 ONUMs = 26962 (35 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.1 Degrees (51207) - 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: q11.04.13.23:37:08.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 26963 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: 2011.04.14.02:07 end: 2011.04.14.05:07 ONUMs = 26963 (85 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: q11.04.14.05:42:39.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 26964 51185 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: 2011.04.14.09:38 end: 2011.04.14.12:44 ONUMs = 26964 (88 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.0 Degrees (51185) - 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: q11.04.14.11:48:05.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 26965 51185 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: 2011.04.14.17:49 end: 2011.04.14.19:57 ONUMs = 26965 (62 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.0 Degrees (51185) - 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: q11.04.14.17:53:31.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 26966 51185 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: 2011.04.14.19:59 end: 2011.04.15.20:11 ONUMs = 26966 (6 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.0 Degrees (51185) - 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: q11.04.14.23:58:57.ovi.dat 6) South Coronal Hole background observation. Sequence: Hole_BG 26967 51185 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: 2011.04.15.02:40 end: 2011.04.15.08:08 ONUMs = 26967 (159 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.0 Degrees (51185) - 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: q11.04.15.06:04:29.ovi.dat 7) 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 26968 51163 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: 2011.04.15.08:10 end: 2011.04.15.09:12 ONUMs = 26968 (22 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -87.9 Degrees (51163) - 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: q11.04.15.12:10:00.ovi.dat 8) 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 26969 51163 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: 2011.04.15.17:30 end: 2011.04.15.20:19 ONUMs = 26969 (82 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -87.9 Degrees (51163) - 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: q11.04.15.18:15:26.ovi.dat