UVCS MISSION LOG ---------------- Date: 7 Apr 2011 ----- Last revision: 3 Aug 2011 (RR) -------------- File Name: 2011.04.07.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: 11.04.07.17:00:38.cmd.log Activity: --------- 1) 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 26938 51340 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: 2011.04.07. end: 2011.04.07. ONUMs = 26938 ( exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.9 Degrees (51340) - 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: 2) 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 26939 51340 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: 2011.04.07.23:52 end: 2011.04.08.04:50 ONUMs = 26939 (142 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.9 Degrees (51340) - 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: q11.04.08.03:31:20.ovi.dat 3) 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 26940 51318 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: 2011.04.08.09:10 end: 2011.04.08.11:38 ONUMs = 26940 (72 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.7 Degrees (51318) - 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: q11.04.08.09:36:46.ovi.dat 4) 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 26941 51318 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: 2011.04.08.11:42 end: 2011.04.08.17:46 ONUMs = 26941 (66 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.7 Degrees (51318) - 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: q11.04.08.15:42:12.ovi.dat 5) South Coronal Hole background observation. Sequence: Hole_BG 26942 51318 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: 2011.04.08.17:48 end: 2011.04.08.23:51 ONUMs = 26942 (129 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.7 Degrees (51318) - 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: q11.04.08.21:47:44.ovi.dat 6) 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 26943 51318 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: 2011.04.08.23:53 end: 2011.04.09.01:53 ONUMs = 26943 (58 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.7 Degrees (51318) - 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: q11.04.09.03:53:15.ovi.dat 7) 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 26944 51318 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: 2011.04.09.09:09 end: 2011.04.09.11:15 ONUMs = 26944 (60 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: -88.7 Degrees (51318) - 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: q11.04.09.09:58:41.ovi.dat