UVCS MISSION LOG ---------------- Date: 10 May 2002 ----- Last revision: 13 May 2002 (Wu) -------------- File Name: 2002.05.10.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start High Latitude Southern Coronal Hole -------------- Study for 10 - 11 May 2002 Load Synoptic for 11 May 2002 Load High Latitude Southern Coronal Hole Study for 11 - 12 May 2002 Load High Latitude Southern Coronal Hole Study for 12 May 2002 Load Mini Synoptic for 12 May 2002 Load High Latitude Southern Coronal Hole Study for 12 - 13 May 2002 Load High Latitude Southern Coronal Hole Study for 13 May 2002 Load Mini Synoptic for 13 May 2002 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 02.05.10.15:42:48.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=210 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: 2002.05.10.15:49 end: 2002.05.11.01:59 ONUMs = 17494 (27 exps) 17495 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 202.093, 203.267, 204.381 Degrees (55573, 55787, 55989) - 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: q02.05.10.15:44:58.lya.dat q02.05.10.15:44:58.ovi.dat q02.05.10.15:44:58.vld.dat q02.05.10.19:44:59.lya.dat q02.05.10.19:44:59.ovi.dat q02.05.10.19:44:59.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: 2002.05.11.02:03 end: 2002.05.11.15:17 ONUMs = 38560 (56 exps) 38561 (37 exps) 38562 (37 exps) 38563 (37 exps) 38564 (37 exps) 38565 (37 exps) 38566 (37 exps) 38567 (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: z02.05.11.02:02:19.lya.dat z02.05.11.02:02:19.ovi.dat z02.05.11.02:02:19.vld.dat z02.05.11.04:19:11.lya.dat z02.05.11.04:19:11.ovi.dat z02.05.11.04:19:11.vld.dat z02.05.11.05:53:40.lya.dat z02.05.11.05:53:40.ovi.dat z02.05.11.05:53:40.vld.dat z02.05.11.07:28:17.lya.dat z02.05.11.07:28:17.ovi.dat z02.05.11.07:28:17.vld.dat z02.05.11.09:02:58.lya.dat z02.05.11.09:02:58.ovi.dat z02.05.11.09:02:58.vld.dat z02.05.11.10:37:39.lya.dat z02.05.11.10:37:39.ovi.dat z02.05.11.10:37:39.vld.dat z02.05.11.12:12:20.lya.dat z02.05.11.12:12:20.ovi.dat z02.05.11.12:12:20.vld.dat z02.05.11.13:47:00.lya.dat z02.05.11.13:47:00.ovi.dat z02.05.11.13:47:00.vld.dat