UVCS MISSION LOG ---------------- Date: 29 August 2003 ----- Last revision: 03 September 2003 (Wu) -------------- File Name: 2003.08.30.a.log ----------- Compiled by: M. Uzzo, R. Wu, Y.-K. Ko ------------ UVCS Activity: Load and Start South Polar Coronal Hole Observation -------------- for 30 - 31 August 2003 Load Synoptic for 31 August 2003 Load South Polar Coronal Hole Observation for 31 August 2003 - 01 September 2003 Load South Polar Coronal Hole Observation for 01 September 2003 Load Mini-Synoptic for 01 September 2003 Load South Polar Coronal Hole Observation for 01 - 02 September 2003 Load Long Synoptic for 02 September 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Command file: 03.08.30.20:29:35.cmd.log Activity: --------- 1) Observation of the South Polar Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the south polar coronal hole. Goal is to measure the properties of a 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 non-polar coronal holes. Roll positions are VL-corrected for PA=230 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: 2003.08.30.20:40 end: 2003.08.31.06:50 ONUMs = 20262 (26 exps) 20263 (36 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 222.09, 223.27, 224.38 Degrees (26424, 26639, 26841) - 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: q03.08.30.20:31:34.lya.dat q03.08.30.20:31:34.ovi.dat q03.08.30.20:31:34.vld.dat q03.08.31.00:36:21.lya.dat q03.08.31.00:36:21.ovi.dat q03.08.31.00:36:21.vld.dat 2) Synoptic Sequence Load and Start Sequence: SynopticA:Start SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 215, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2003.08.31.07:05 end: 2003.08.31.19:36 ONUMs = 43050 (37 exps) 43051 (37 exps) 43052 (37 exps) 43053 (37 exps) 43054 (37 exps) 43055 (37 exps) 43056 (37 exps) 43057 (37 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: E: STR2B, SE: STR2B, S: STR2B, SW: STR2B, W: STR2B, NW: STR2B, N: STR2B, NE: 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: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z03.08.31.07:04:42.lya.dat z03.08.31.07:04:42.ovi.dat z03.08.31.07:04:42.vld.dat z03.08.31.08:39:33.lya.dat z03.08.31.08:39:33.ovi.dat z03.08.31.08:39:33.vld.dat z03.08.31.10:13:58.lya.dat z03.08.31.10:13:58.ovi.dat z03.08.31.10:13:58.vld.dat z03.08.31.11:48:38.lya.dat z03.08.31.11:48:38.ovi.dat z03.08.31.11:48:38.vld.dat z03.08.31.13:22:50.lya.dat z03.08.31.13:22:50.ovi.dat z03.08.31.13:22:50.vld.dat z03.08.31.14:57:14.lya.dat z03.08.31.14:57:14.ovi.dat z03.08.31.14:57:14.vld.dat z03.08.31.16:31:40.lya.dat z03.08.31.16:31:40.ovi.dat z03.08.31.16:31:40.vld.dat z03.08.31.18:06:22.lya.dat z03.08.31.18:06:22.ovi.dat z03.08.31.18:06:22.vld.dat