UVCS MISSION LOG ---------------- Date: 04 October 2002 ----- Last revision: 07 October 2002 (Wu) -------------- File Name: 2002.10.04.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Load and Start Northern Coronal Hole Study for -------------- 04 - 05 October 2002 Load Synoptic for 05 October 2002 Load Southern Coronal Hole Study for 05 - 06 October 2002 Load Southern Coronal Hole Study for 06 October 2002 Load Mini-Synoptic for 06 October 2002 Load Southern Coronal Hole Study for 06 - 07 October 2002 Load Synoptic for 07 October 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Y.-K. Ko Command file: 02.10.04.17:41:00.cmd.log Activity: --------- 1) Observation of a North Polar Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a northern 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=350 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: 2002.10.04.18:08 end: 2002.10.05.04:18 ONUMs = 18094 (27 exps) 18095 (35 exps) Instrument configuration: - Pointing: Sun center - Roll: 342.093, 343.267, 344.381 Degrees (15502, 15716, 15919) - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.10.04.17:54:53.lya.dat q02.10.04.17:54:53.ovi.dat q02.10.04.17:54:53.vld.dat q02.10.04.22:03:55.lya.dat q02.10.04.22:03:55.ovi.dat q02.10.04.22:03:55.vld.dat GAP between 10/05/02|00:50:22( 2964) and 10/05/02|00:52:02( 3121) 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: 2002.10.05.04:27 end: 2002.10.05.17:41 ONUMs = 39990 (37 exps) 39991 (37 exps) 39992 (37 exps) 39993 (37 exps) 39994 (56 exps) 39995 (37 exps) 39996 (37 exps) 39997 (35 exps) Instrument configuration: - Pointing: Sun center - Roll: W: STR2B, NW: STR2B, N: STR2B, NE: STR2B, E: STR1A, 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.10.05.04:26:27.lya.dat z02.10.05.04:26:27.ovi.dat z02.10.05.04:26:27.vld.dat z02.10.05.06:01:06.lya.dat z02.10.05.06:01:06.ovi.dat z02.10.05.06:01:06.vld.dat z02.10.05.07:35:35.lya.dat z02.10.05.07:35:35.ovi.dat z02.10.05.07:35:35.vld.dat z02.10.05.09:10:27.lya.dat z02.10.05.09:10:27.ovi.dat z02.10.05.09:10:27.vld.dat z02.10.05.10:44:56.lya.dat z02.10.05.10:44:56.ovi.dat z02.10.05.10:44:56.vld.dat z02.10.05.13:01:48.lya.dat z02.10.05.13:01:48.ovi.dat z02.10.05.13:01:48.vld.dat z02.10.05.14:36:12.lya.dat z02.10.05.14:36:12.ovi.dat z02.10.05.14:36:12.vld.dat z02.10.05.16:10:39.lya.dat z02.10.05.16:10:39.ovi.dat z02.10.05.16:10:39.vld.dat