UVCS MISSION LOG ---------------- Date: 14 March 2003 ----- Last revision: 17 March 2003 (Wu) -------------- File Name: 2003.03.14.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load and Start Southern Coronal Hole Study for ------------- 14 - 15 March 2003 Load Southern Coronal Hole Study for 15 March 2003 Load Mini-Synoptic for 15 March 2003 Load Northern Coronal Hole Study for 15 - 16 March 2003 Load Northern Coronal Hole Study for 16 March 2003 Load Mini-Synoptic for 16 March 2003 Load Northern Coronal Hole Study for 16 - 17 March 2003 Load Synoptic for 17 March 2003 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- Y.-K. Ko: Commander, Planner D. H. Phillips: Planner R. Wu Command file: 03.03.14.15:50:05.cmd.log Activity: --------- 1) Observation of the Southern Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of a mid-latitude southern 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=154 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: 2003.03.14.16:17 end: 2003.03.15.02:27 ONUMs = 18667 (27 exps) 18668 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 146.09, 147.27, 148.38 Degrees (45378, 45592, 45795) - 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: q03.03.14.16:05:27.lya.dat q03.03.14.16:05:27.ovi.dat q03.03.14.16:05:27.vld.dat q03.03.14.20:13:44.lya.dat q03.03.14.20:13:44.ovi.dat q03.03.14.20:13:44.vld.dat 2) Observation of the Southern Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of a mid-latitude southern 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=154 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: 2003.03.15.02:29 end: 2003.03.15.12:23 ONUMs = 18669 (6 exps) 18670 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 146.09, 148.38 Degrees (45378, 45795) - 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: q03.03.15.02:27:48.lya.dat q03.03.15.02:27:48.ovi.dat q03.03.15.02:27:48.vld.dat q03.03.15.03:02:25.lya.dat q03.03.15.03:02:25.ovi.dat q03.03.15.03:02:25.vld.dat GAP between 03/15/03|03:36:08(10686) and 03/15/03|03:37:51(10852) 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: 2003.03.15.12:48 end: 2003.03.15.16:14 ONUMs = 41610 (9 exps) 41611 (9 exps) 41612 (9 exps) 41613 (9 exps) 41614 (9 exps) 41615 (9 exps) 41616 (9 exps) 41617 (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: z03.03.15.12:47:01.lya.dat z03.03.15.12:47:01.ovi.dat z03.03.15.12:47:01.vld.dat z03.03.15.13:13:26.lya.dat z03.03.15.13:13:26.ovi.dat z03.03.15.13:13:26.vld.dat z03.03.15.13:40:14.lya.dat z03.03.15.13:40:14.ovi.dat z03.03.15.13:40:14.vld.dat z03.03.15.14:06:42.lya.dat z03.03.15.14:06:42.ovi.dat z03.03.15.14:06:42.vld.dat z03.03.15.14:33:11.lya.dat z03.03.15.14:33:11.ovi.dat z03.03.15.14:33:11.vld.dat z03.03.15.14:59:40.lya.dat z03.03.15.14:59:40.ovi.dat z03.03.15.14:59:40.vld.dat z03.03.15.15:26:09.lya.dat z03.03.15.15:26:09.ovi.dat z03.03.15.15:26:09.vld.dat z03.03.15.15:52:29.lya.dat z03.03.15.15:52:29.ovi.dat z03.03.15.15:52:29.vld.dat