UVCS MISSION LOG ---------------- Date: 23 June 2005 ----- Last revision: 27 June 2005 (Wu) -------------- File Name: 2005.06.24.a.log ---------- Compiled by: M. Uzzo ------------ UVCS Activity: South Polar Coronal Hole LyA Observation for -------------- 24 June 2005 Load South Polar Coronal Hole OVI Observation for 24 - 25 June 2005 Load South Polar Coronal Hole OVI Observation for 25 June 2005 Load OVI Synoptic for 25 June 2005 Load South Polar Coronal Hole LyA Observation for 25 - 26 June 2005 Load South Polar Coronal Hole OVI Observation for 26 June 2005 Load South Polar Coronal Hole OVI Observation for 26 June 2005 Load OVI Synoptic for 26 - 27 June 2005 Load LyA Synoptic for 27 June 2005 Load South Polar Coronal Hole LyA Observation for 27 June 2005 Load South Polar Coronal Hole OVI Observation for 27 - 28 June 2005 Load South Polar Coronal Hole OVI Observation for 28 June 2005 Load Mini-Synoptic for 28 June 2005 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 05.06.23.13:42:02.cmd.log 05.06.24.13:17:19.cmd.log Activity: --------- 1) South Polar Coronal Hole Observation Sequence: 05.02_hole1LyA.tcl SCI_SPEC: Characterization of the South 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 HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=190 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: 2005.06.24.12:28 end: 2005.06.24.17:02 ONUMs = 21465 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 182.09, 183.27, 184.38 degrees (19142 19357 19559) - Mirror/Occulter: 1.7, 2.0, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q05.06.24.12:20:35.ovi.dat 2) South Polar Coronal Hole Observation Sequence: 05.02_hole1OVI.tcl SCI_SPEC: Characterization of the South 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 HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=190 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: 2005.06.24.17:03 end: 2005.06.25.02:29 ONUMs = 21466 (105 exps) 21467 (168 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 182.09, 183.27, 184.38 degrees (19142 19357 19559) - Mirror/Occulter: 1.7, 2.0, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.06.24.17:01:56.ovi.dat q05.06.24.20:40:54.ovi.dat 3) South Polar Coronal Hole Observation Sequence: 05.02_holexOVI.tcl, n50min = 5 SCI_SPEC: Characterization of the South 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 HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=190 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: 2005.06.25.02:30 end: 2005.06.25.07:33 ONUMs = 21468 (14 exps) 21469 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 182.09, 184.38 degrees (19142 19559) - Mirror/Occulter: 1.7, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 5 Fits Files: q05.06.25.02:28:55.ovi.dat q05.06.25.02:59:03.ovi.dat 4) OVI Synoptic Sequence Load and Start Sequence: SynopticD:Start SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage at 200, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2005.06.25.07:43 end: 2005.06.25.21:57 ONUMs = 48260 (49 exps) 48261 (49 exps) 48262 (47 exps) 48263 (49 exps) 48264 (49 exps) 48265 (49 exps) 48266 (47 exps) 48267 (49 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: E: os, SE: os, S: oc, SW: os, W: os, NW: os, N: oc, NE: os - Mirror/Occulter: ls: 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro lc: 2.10, 1.90, 1.75, 1.60 Ro os: 3.00, 2.10, 1.90, 1.75, 1.60 Ro oc: 1.90, 1.75, 1.60 Ro ms: 2.10, 1.75, 1.60 Ro mc: 1.90, 1.75, 1.60 Ro 1.5 mm overocculting (1.60 Ro) 2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (LyA Synoptic) 200 um (OVI, and Mini Synoptic) - LYA GRTPOS: 128000 - OVI GRTPOS: 187260 (LyA Synoptic) 229000 (OVI, and Mini Synoptic) - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_188 in slot 2 (LyA Synoptic) OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic) Fits Files: z05.06.25.07:42:28.ovi.dat z05.06.25.09:31:08.ovi.dat z05.06.25.11:19:48.ovi.dat z05.06.25.13:03:15.ovi.dat z05.06.25.14:51:55.ovi.dat z05.06.25.16:40:35.ovi.dat z05.06.25.18:29:15.ovi.dat z05.06.25.20:12:42.ovi.dat