UVCS MISSION LOG ---------------- Date: 02 October 2003 ----- Last revision: 14 October 2003 (Wu) -------------- File Name: 2003.10.03.a.log ---------- Compiled by: Y.-K. Ko ------------ UVCS Activity: South Coronal Hole Observation for 03 - 04 October 2003 -------------- South Coronal Hole Observation for 04 October 2003 Mini Synoptic for 04 October 2003 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- Y.-K. Ko: Commander M. Uzzo: Planner R. Wu Command file: 03.10.02.14:12:22.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=180 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: South Coronal Hole Observations CMP_NUM: 6988 Duration: start: 2003.10.03.15:30 end: 2003.10.04.01:40 ONUMs = 20367 (27 exps) 20368 (36 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 172.09, 173.27, 174.38 Degrees (17322, 17537, 17739) - 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: q03.10.03.15:16:44.lya.dat q03.10.03.15:16:44.ovi.dat q03.10.03.15:16:44.vld.dat q03.10.03.19:26:18.lya.dat q03.10.03.19:26:18.ovi.dat q03.10.03.19:26:18.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=180 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: 2003.10.04.01:42 end: 2003.10.04.11:35 ONUMs = 20369 (6 exps) 20370 (54 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 172.09, 174.38 Degrees (17322, 17739) - 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: q03.10.04.01:40:09.lya.dat q03.10.04.01:40:09.ovi.dat q03.10.04.01:40:09.vld.dat q03.10.04.02:14:32.lya.dat q03.10.04.02:14:32.ovi.dat q03.10.04.02:14:32.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: 2003.10.04.11:45 end: 2003.10.04.15:12 ONUMs = 43380 (9 exps) 43381 (9 exps) 43382 (9 exps) 43383 (9 exps) 43384 (9 exps) 43385 (9 exps) 43386 (9 exps) 43387 (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: z03.10.04.11:44:36.lya.dat z03.10.04.11:44:36.ovi.dat z03.10.04.11:44:36.vld.dat z03.10.04.12:11:06.lya.dat z03.10.04.12:11:06.ovi.dat z03.10.04.12:11:06.vld.dat z03.10.04.12:37:35.lya.dat z03.10.04.12:37:35.ovi.dat z03.10.04.12:37:35.vld.dat z03.10.04.13:04:04.lya.dat z03.10.04.13:04:04.ovi.dat z03.10.04.13:04:04.vld.dat z03.10.04.13:30:33.lya.dat z03.10.04.13:30:33.ovi.dat z03.10.04.13:30:33.vld.dat z03.10.04.13:57:10.lya.dat z03.10.04.13:57:10.ovi.dat z03.10.04.13:57:10.vld.dat z03.10.04.14:23:45.lya.dat z03.10.04.14:23:45.ovi.dat z03.10.04.14:23:45.vld.dat z03.10.04.14:50:12.lya.dat z03.10.04.14:50:12.ovi.dat z03.10.04.14:50:12.vld.dat