UVCS MISSION LOG ---------------- Date: 24 January 2003 ----- Last revision: 27 January 2003 (Wu) -------------- File Name: 2003.01.24.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load North Coronal Hole Study for 24 - 25 January 2003 -------------- Load Synoptic for 25 January 2003 Load Low Latititude Coronal Hole Study for 25 - 26 January 2003 Load Low Latitude Coronal Hole Study for 26 January 2003 Load Mini-Synoptic for 26 January 2003 Load Low Latititude Coronal Hole Study for 26 - 27 January 2003 Load Low Latitude Coronal Hole Study for 27 January 2003 Load Low Latitude Coronal Hole Study for 27 January 2003 Load Mini-Synoptic for 27 January 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 03.01.24.15:07:35.cmd.log Activity: --------- 1) Observation of the North Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the north 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=342 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: 2003.01.24.17:20 end: 2003.01.25.03:30 ONUMs = 18479 (25 exps) 18480 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 334.09, 335.27, 336.38 Degrees (14046, 14259, 14462) - 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: q03.01.24.17:05:27.lya.dat q03.01.24.17:05:27.ovi.dat q03.01.24.17:05:27.vld.dat q03.01.24.21:16:36.lya.dat q03.01.24.21:16:36.ovi.dat q03.01.24.21:16:36.vld.dat GAP between 01/24/03|19:32:15( 890) and 01/24/03|19:45:53( 2194) 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: 2003.01.25.03:39 end: 2003.01.25.16:53 ONUMs = 41130 (37 exps) 41131 (56 exps) 41132 (37 exps) 41133 (37 exps) 41134 (37 exps) 41135 (37 exps) 41136 (37 exps) 41137 (37 exps) Instrument configuration: - Pointing: Sun center - 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: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z03.01.25.03:38:22.lya.dat z03.01.25.03:38:22.ovi.dat z03.01.25.03:38:22.vld.dat z03.01.25.05:13:04.lya.dat z03.01.25.05:13:04.ovi.dat z03.01.25.05:13:04.vld.dat z03.01.25.07:29:56.lya.dat z03.01.25.07:29:56.ovi.dat z03.01.25.07:29:56.vld.dat z03.01.25.09:04:07.lya.dat z03.01.25.09:04:07.ovi.dat z03.01.25.09:04:07.vld.dat z03.01.25.10:38:47.lya.dat z03.01.25.10:38:47.ovi.dat z03.01.25.10:38:47.vld.dat z03.01.25.12:13:16.lya.dat z03.01.25.12:13:16.ovi.dat z03.01.25.12:13:16.vld.dat z03.01.25.13:48:08.lya.dat z03.01.25.13:48:08.ovi.dat z03.01.25.13:48:08.vld.dat z03.01.25.15:22:36.lya.dat z03.01.25.15:22:36.ovi.dat z03.01.25.15:22:36.vld.dat