UVCS MISSION LOG ---------------- Date: 05 September 2002 ----- Last revision: 06 September 2002 (Wu) -------------- File Name: 2002.09.05.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Northern Coronal Hole Study for 05 - 06 September 2002 -------------- Synoptic for 06 September 2002 Load Coronal Jets Study for 06 - 07 September 2002 Load Mini Synoptic for 07 September 2002 Load Coronal Jets Study for 07 September 2002 SOHO Activity: -------------- EOF Staff: S. Cranmer: Lead Scientist ---------- Y.-K. Ko: Commander M. Uzzo: Planner R. Wu Command file: 02.09.04.17:45:55.cmd.log Activity: --------- 1) Observation of Northern Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a north 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=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: 2002.09.05.18:10 end: 2002.09.06.04:20 ONUMs = 17972 (27 exps) 17973 (35 exps) Instrument configuration: - Pointing: Sun center - Roll: 347.09, 348.27, 349.38 Degrees (16412, 16627, 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.09.05.17:58:38.lya.dat q02.09.05.17:58:38.ovi.dat q02.09.05.17:58:38.vld.dat q02.09.05.22:06:03.lya.dat q02.09.05.22:06:03.ovi.dat q02.09.05.22:06:03.vld.dat GAP between 09/05/02|22:48:14( 9595) and 09/05/02|22:49:16( 9694) 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: 2002.09.06.04:30 end: 2002.09.06.17:01 ONUMs = 39700 (37 exps) 39701 (37 exps) 39702 (37 exps) 39703 (37 exps) 39704 (37 exps) 39705 (37 exps) 39706 (37 exps) 39707 (37 exps) Instrument configuration: - Pointing: Sun center - Roll: W: STR2B, NW: STR2B, 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.09.06.04:29:02.lya.dat z02.09.06.04:29:02.ovi.dat z02.09.06.04:29:02.vld.dat z02.09.06.06:03:45.lya.dat z02.09.06.06:03:45.ovi.dat z02.09.06.06:03:45.vld.dat z02.09.06.07:38:12.lya.dat z02.09.06.07:38:12.ovi.dat z02.09.06.07:38:12.vld.dat z02.09.06.09:13:05.lya.dat z02.09.06.09:13:05.ovi.dat z02.09.06.09:13:05.vld.dat z02.09.06.10:47:32.lya.dat z02.09.06.10:47:32.ovi.dat z02.09.06.10:47:32.vld.dat z02.09.06.12:22:11.lya.dat z02.09.06.12:22:11.ovi.dat z02.09.06.12:22:11.vld.dat z02.09.06.13:56:22.lya.dat z02.09.06.13:56:22.ovi.dat z02.09.06.13:56:22.vld.dat z02.09.06.15:31:01.lya.dat z02.09.06.15:31:01.ovi.dat z02.09.06.15:31:01.vld.dat