UVCS MISSION LOG ---------------- Date: 10 October 2002 ----- Last revision: 15 October 2002 (Wu) -------------- File Name: 2002.10.13.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Southern Coronal Hole Study for 13 - 14 October 2002 -------------- Long Synoptic for 14 October 2002 Load Southern Coronal Hole Study for 14 - 15 October 2002 Load Southern Coronal Hole Study for 15 October 2002 Load Mini-Synoptic for 15 October 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 02.10.11.12:06:26.cmd.log 02.10.13.19:33:02.cmd.log Activity: --------- 1) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a high-latitude coronal hole. Goal is to measure the properties of a high-latitude 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=225 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: 2002.10.13.20:26 end: 2002.10.14.06:36 ONUMs = 18120 (27 exps) 18121 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 217.093, 218.267, 219.381 Degrees (58304, 58517, 58720) - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.10.13.20:23:57.lya.dat q02.10.13.20:23:57.ovi.dat q02.10.13.20:23:57.vld.dat q02.10.14.00:22:38.lya.dat q02.10.14.00:22:38.ovi.dat q02.10.14.00:22:38.vld.dat 2) Synoptic Sequence Load and Start Sequence: SynopticA:Start 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: 2002.10.14.06:39 end: 2002.10.14.19:52 ONUMs = 40080 (37 exps) 40081 (37 exps) 40082 (56 exps) 40083 (37 exps) 40084 (37 exps) 40085 (37 exps) 40086 (37 exps) 40087 (37 exps) Instrument configuration: - Pointing: Sun center - Roll: SW: STR2B, S: STR2B, SE: STR1A, E: STR2B, NE: STR2B, N: STR2B, NW: STR2B, W: STR2B - Mirror/Occulter: STR1A: 3.5, 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR2B: 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR3A: 3.5, 3.0 Ro STR4B: 4.0 Ro STR5A: 2.1, 1.9, 1.75, 1.6 Ro STR6B: 2.5 Ro STR7B: 3.0 Ro CH1A: 1.9, 1.75, 1.6 Ro CH2A: 2.1 Ro CH2B: 2.1 Ro CH3B: 2.5 Ro CH4A: 1.75, 1.6 Ro CH5B: 1.9 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75, 1.9, 2.1, 2.5, 3.0, 3.5, 4.0 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (STR1A, STR2B, STR3A, STR4B, CH1A, CH2A, CH2B, CH3B) 100 um (CH4A, CH5B) 75 um (STR5A, STR6B, STR7B) - LYA GRTPOS: 128000 - OVI GRTPOS: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.10.14.06:38:35.lya.dat z02.10.14.06:38:35.ovi.dat z02.10.14.06:38:35.vld.dat z02.10.14.08:13:22.lya.dat z02.10.14.08:13:22.ovi.dat z02.10.14.08:13:22.vld.dat z02.10.14.09:48:03.lya.dat z02.10.14.09:48:03.ovi.dat z02.10.14.09:48:03.vld.dat z02.10.14.12:04:56.lya.dat z02.10.14.12:04:56.ovi.dat z02.10.14.12:04:56.vld.dat z02.10.14.13:39:38.lya.dat z02.10.14.13:39:38.ovi.dat z02.10.14.13:39:38.vld.dat z02.10.14.15:14:17.lya.dat z02.10.14.15:14:17.ovi.dat z02.10.14.15:14:17.vld.dat z02.10.14.16:48:31.lya.dat z02.10.14.16:48:31.ovi.dat z02.10.14.16:48:31.vld.dat z02.10.14.18:23:08.lya.dat z02.10.14.18:23:08.ovi.dat z02.10.14.18:23:08.vld.dat