UVCS MISSION LOG ---------------- Date: 10 February 2003 ----- Last revision: 11 February 2003 (Wu) -------------- File Name: 2003.02.10.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Flush Southern Coronal Hole Study for ------------- 09 - 10 February 2003 Load and Start Mini-Synoptic for 10 February 2003 Load Southern Coronal Hole Study for 10 - 11 February 2003 Load Southern Coronal Hole Study for 11 February 2003 Load Mini-Synoptic for 11 February 2003 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 03.02.10.17:02:00.cmd.log Activity: --------- 1) Observation of a Low Latitude Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of a low latitude coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=160 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: 2003.02.10.21:05 end: 2003.02.11.07:15 ONUMs = 18558 (27 exps) 18559 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 152.093, 153.267, 154.381 Degrees (46471, 46684, 46887) - 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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.02.10.20:57:04.lya.dat q03.02.10.20:57:04.ovi.dat q03.02.10.20:57:04.vld.dat q03.02.11.01:01:47.lya.dat q03.02.11.01:01:47.ovi.dat q03.02.11.01:01:47.vld.dat 2) Observation of a Low Latitude Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of a low latitude coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=160 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: 2003.02.11.07:17 end: 2003.02.11.17:11 ONUMs = 18560 (6 exps) 18561 (53 exps) Instrument configuration: - Pointing: Sun center - Roll: 152.093, 154.381 Degrees (46471, 46887) - 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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.02.11.07:15:53.lya.dat q03.02.11.07:15:53.ovi.dat q03.02.11.07:15:53.vld.dat q03.02.11.07:50:28.lya.dat q03.02.11.07:50:28.ovi.dat q03.02.11.07:50:28.vld.dat 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 210, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2003.02.11.17:36 end: 2003.02.11.21:03 ONUMs = 41300 (9 exps) 41301 (9 exps) 41302 (9 exps) 41303 (9 exps) 41304 (9 exps) 41305 (9 exps) 41306 (9 exps) 41307 (9 exps) Instrument configuration: - Pointing: Sun center - Roll: W, NW, N, NE, E, SE, S, SW - Mirror/Occulter: 1.6, 1.75 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75 Ro) - LYA Slits: 50 um - OVI Slits: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z03.02.11.17:35:43.lya.dat z03.02.11.17:35:43.ovi.dat z03.02.11.17:35:43.vld.dat z03.02.11.18:02:18.lya.dat z03.02.11.18:02:18.ovi.dat z03.02.11.18:02:18.vld.dat z03.02.11.18:28:47.lya.dat z03.02.11.18:28:47.ovi.dat z03.02.11.18:28:47.vld.dat z03.02.11.18:55:31.lya.dat z03.02.11.18:55:31.ovi.dat z03.02.11.18:55:31.vld.dat z03.02.11.19:21:59.lya.dat z03.02.11.19:21:59.ovi.dat z03.02.11.19:21:59.vld.dat z03.02.11.19:48:28.lya.dat z03.02.11.19:48:28.ovi.dat z03.02.11.19:48:28.vld.dat z03.02.11.20:14:57.lya.dat z03.02.11.20:14:57.ovi.dat z03.02.11.20:14:57.vld.dat z03.02.11.20:41:32.lya.dat z03.02.11.20:41:32.ovi.dat z03.02.11.20:41:32.vld.dat