UVCS MISSION LOG ---------------- Date: 14 December 2001 ----- Last revision: 17 December 2001 (Wu) -------------- File Name: 2001.12.14.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start High-latitude South Hemisphere Coronal -------------- Hole Study for 14 - 15 December 2001 Load Long Synoptic for 15 December 2001 Load High-latitude South Hemisphere Coronal for 15 - 16 December 2001 Load Long Synoptic for 16 December 2001 Load High-latitude South Hemisphere Coronal for 16 - 17 December 2001 Load Long Synoptic for 17 December 2001 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner R. Hauck Command file: 01.12.14.19:01:14.cmd.log Activity: --------- 1) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 01.06_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=355 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: 2001.12.14.19:25 end: 2001.12.15.05:35 ONUMs = 16970 (27 exps) 16971 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 347.093, 348.267, 349.381 Degrees (16412, 16626, 16829) - 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: q01.12.14.19:21:57.lya.dat q01.12.14.19:21:57.ovi.dat q01.12.14.19:21:57.vld.dat q01.12.14.23:20:55.lya.dat q01.12.14.23:20:55.ovi.dat q01.12.14.23:20:55.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: 2001.12.15:05:45 end: 2001.12.15.18:58 ONUMs = 37180 (37 exps) 37181 (37 exps) 37182 (37 exps) 37183 (37 exps) 37184 (37 exps) 37185 (37 exps) 37186 (37 exps) 37187 (55 exps) Instrument configuration: - Pointing: Sun center - Roll: W: STR2B, NW: STR2B, N: STR2B, NE: STR2B, E: STR2B, SE: STR2B, S: STR2B, SW: STR1A - 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: 184200 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_184 in slot 2 Fits Files: z01.12.15.05:44:48.lya.dat z01.12.15.05:44:48.ovi.dat z01.12.15.05:44:48.vld.dat z01.12.15.07:19:23.lya.dat z01.12.15.07:19:23.ovi.dat z01.12.15.07:19:23.vld.dat z01.12.15.08:53:34.lya.dat z01.12.15.08:53:34.ovi.dat z01.12.15.08:53:34.vld.dat z01.12.15.10:28:14.lya.dat z01.12.15.10:28:14.ovi.dat z01.12.15.10:28:14.vld.dat z01.12.15.12:02:43.lya.dat z01.12.15.12:02:43.ovi.dat z01.12.15.12:02:43.vld.dat z01.12.15.13:37:35.lya.dat z01.12.15.13:37:35.ovi.dat z01.12.15.13:37:35.vld.dat z01.12.15.15:12:02.lya.dat z01.12.15.15:12:02.ovi.dat z01.12.15.15:12:02.vld.dat z01.12.15.16:46:41.lya.dat z01.12.15.16:46:41.ovi.dat z01.12.15.16:46:41.vld.dat GAP between 12/15/01|18:20:50( 6747) and 12/15/01|18:21:52( 6850)