UVCS MISSION LOG ---------------- Date: 12 April 2002 ----- Last revision: 15 April 2002 (Wu) -------------- File Name: 2002.04.13.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: High Latitude Southern Coronal Hole Study for -------------- 13 - 14 April 2002 Synoptic for 14 April 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 02.04.09.16:44:35.cmd.log Activity: --------- 1) Observation of the High Latitude Southern Coronal Hole Sequence: 01.06_hole1.tcl SCI_SPEC: Characterization of the high-latitude southern coronal hole. Goal is to measure the properties of these non-polar coronal holes. 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 the polar coronal holes. Roll positions are VL-corrected for PA=228 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: 2002.04.13.17:35 end: 2002.04.14.03:45 ONUMs = 17316 (27 exps) 17317 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 220.09, 221.27, 222.38 Degrees (58849, 59064, 59266) - 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_168MPM in slot 1 Fits Files: q02.04.13.17:33:04.lya.dat q02.04.13.17:33:04.ovi.dat q02.04.13.17:33:04.vld.dat q02.04.13.21:31:33.lya.dat q02.04.13.21:31:33.ovi.dat q02.04.13.21:31:33.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: 2002.04.14.03:48 end: 2002.04.14.17:01 ONUMs = 38260 (56 exps) 38261 (37 exps) 38262 (36 exps) 38263 (37 exps) 38264 (37 exps) 38265 (37 exps) 38266 (37 exps) 38267 (37 exps) Instrument configuration: - Pointing: Sun center - Roll: SW: STR1A, S: STR2B, SE: STR2B, 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: 181000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_181 in slot 2 Fits Files: z02.04.14.03:47:13.lya.dat z02.04.14.03:47:13.ovi.dat z02.04.14.03:47:13.vld.dat z02.04.14.06:04:30.lya.dat z02.04.14.06:04:30.ovi.dat z02.04.14.06:04:30.vld.dat z02.04.14.07:38:59.lya.dat z02.04.14.07:38:59.ovi.dat z02.04.14.07:38:59.vld.dat z02.04.14.09:13:36.lya.dat z02.04.14.09:13:36.ovi.dat z02.04.14.09:13:36.vld.dat z02.04.14.10:47:47.lya.dat z02.04.14.10:47:47.ovi.dat z02.04.14.10:47:47.vld.dat z02.04.14.12:22:28.lya.dat z02.04.14.12:22:28.ovi.dat z02.04.14.12:22:28.vld.dat z02.04.14.13:57:09.lya.dat z02.04.14.13:57:09.ovi.dat z02.04.14.13:57:09.vld.dat z02.04.14.15:31:35.lya.dat z02.04.14.15:31:35.ovi.dat z02.04.14.15:31:35.vld.dat