UVCS MISSION LOG ---------------- Date: 05 September 2003 ----- Last revision: 08 September 2003 (Wu) -------------- File Name: 2003.09.06.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: South Coronal Hole Observation -------------- for 06 - 07 September 2003 South Coronal Hole Observation for 07 September 2003 Mini-Synoptic for 07 September 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner R. Wu Command file: 03.09.05.14:54:36.cmd.log Activity: --------- 1) Observation of the South Coronal Hole Sequence: 02.12_hole1.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=188 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: 2003.09.06.18:10 end: 2003.09.07.04:20 ONUMs = 20286 (27 exps) 20287 (36 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180.09, 181.27, 182.38 Degrees (18779, 18993, 19195) - 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: q03.09.06.17:57:12.lya.dat q03.09.06.17:57:12.ovi.dat q03.09.06.17:57:12.vld.dat q03.09.06.22:06:06.lya.dat q03.09.06.22:06:06.ovi.dat q03.09.06.22:06:06.vld.dat 2) Observation of the South Coronal Hole Sequence: 02.12_hole5.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=188 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: 2003.09.07.04:22 end: 2003.09.07.14:15 ONUMs = 20288 (6 exps) 20289 (54 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180.09, 182.38 Degrees (18779, 19195) - 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: q03.09.07.04:20:09.lya.dat q03.09.07.04:20:09.ovi.dat q03.09.07.04:20:09.vld.dat q03.09.07.04:54:32.lya.dat q03.09.07.04:54:32.ovi.dat q03.09.07.04:54:32.vld.dat 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 215, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2003.09.07.14:26 end: 2003.09.07.17:53 ONUMs = 43120 (9 exps) 43121 (9 exps) 43122 (9 exps) 43123 (9 exps) 43124 (9 exps) 43125 (9 exps) 43126 (9 exps) 43127 (9 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: E, SE, S, SW, W, NW, N, NE - 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: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z03.09.07.14:25:24.lya.dat z03.09.07.14:25:24.ovi.dat z03.09.07.14:25:24.vld.dat z03.09.07.14:51:53.lya.dat z03.09.07.14:51:53.ovi.dat z03.09.07.14:51:53.vld.dat z03.09.07.15:18:37.lya.dat z03.09.07.15:18:37.ovi.dat z03.09.07.15:18:37.vld.dat z03.09.07.15:45:12.lya.dat z03.09.07.15:45:12.ovi.dat z03.09.07.15:45:12.vld.dat z03.09.07.16:11:49.lya.dat z03.09.07.16:11:49.ovi.dat z03.09.07.16:11:49.vld.dat z03.09.07.16:38:18.lya.dat z03.09.07.16:38:18.ovi.dat z03.09.07.16:38:18.vld.dat z03.09.07.17:04:54.lya.dat z03.09.07.17:04:54.ovi.dat z03.09.07.17:04:54.vld.dat z03.09.07.17:31:30.lya.dat z03.09.07.17:31:30.ovi.dat z03.09.07.17:31:30.vld.dat