UVCS MISSION LOG ---------------- Date: 26 October 2003 ----- Last revision: 31 October 2003 (Wu) -------------- File Name: 2003.10.24.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Flush Remaining Positions of Mini-Synoptic for -------------- 24 October 2003 from Batch Queue, and Reload Individually into Interactive Queue Load and Start South Coronal Hole Observation for 24 - 25 October 2003 Load Synoptic for 25 October 2003 Load South Coronal Hole Observation for 25 - 26 October 2003 Load South Coronal Hole Observation for 26 October 2003 Load Mini-Synoptic for 26 October 2003 Load South Coronal Hole Observation for 26 - 27 October 2003 Load Synoptic for 27 October 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 03.10.24.14:50:01.cmd.log Activity: --------- 1) Observation of a Southern Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of a mid-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=252 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: 2003.10.24.16:28 end: 2003.10.25.02:38 ONUMs = 20436 (27 exps) 20437 (36 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: 244.093, 245.267, 246.381 Degrees (63219, 63433, 63536) - 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: q03.10.24.16:25:12.lya.dat q03.10.24.16:25:12.ovi.dat q03.10.24.16:25:12.vld.dat q03.10.24.20:24:51.lya.dat q03.10.24.20:24:51.ovi.dat q03.10.24.20:24:51.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: 2003.10.25.03:14 end: 2003.10.25.16:26 ONUMs = 43590 (37 exps) 43591 (56 exps) 43592 (37 exps) 43593 (37 exps) 43594 (37 exps) 43595 (37 exps) 43596 (37 exps) 43597 (37 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 0 Degrees - Roll: W: STR2B, NW: STR1A, N: STR2B, NE: STR2B, E: STR2B, SE: STR2B, S: STR2B, SW: 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: z03.10.25.03:13:21.lya.dat z03.10.25.03:13:21.ovi.dat z03.10.25.03:13:21.vld.dat z03.10.25.04:47:35.lya.dat z03.10.25.04:47:35.ovi.dat z03.10.25.04:47:35.vld.dat z03.10.25.07:04:27.lya.dat z03.10.25.07:04:27.ovi.dat z03.10.25.07:04:27.vld.dat z03.10.25.08:38:55.lya.dat z03.10.25.08:38:55.ovi.dat z03.10.25.08:38:55.vld.dat z03.10.25.10:13:33.lya.dat z03.10.25.10:13:33.ovi.dat z03.10.25.10:13:33.vld.dat z03.10.25.11:47:47.lya.dat z03.10.25.11:47:47.ovi.dat z03.10.25.11:47:47.vld.dat z03.10.25.13:22:24.lya.dat z03.10.25.13:22:24.ovi.dat z03.10.25.13:22:24.vld.dat z03.10.25.14:56:33.lya.dat z03.10.25.14:56:33.ovi.dat z03.10.25.14:56:33.vld.dat