UVCS MISSION LOG ---------------- Date: 12 March 2002 ----- Last revision: 02 April 2002 (Ko) -------------- File Name: 2002.03.15.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start North Polar Coronal Hole Study for -------------- 15 - 16 March 2002 Load Long Synoptic for 16 March 2002 Load High Latitude Southern Coronal Hole Study for 16 - 17 March 2002 Load Long Synoptic for 17 March 2002 Load High Latitude Southern Coronal Hole Study for 17 - 18 March 2002 Load Long Synoptic for 18 March 2002 SOHO Activity: -------------- EOF Staff: M. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko: Planner Command file: 02.03.15.15:20:52.cmd.log Activity: --------- 1) Observation of the North Polar Coronal Hole Sequence: 01.06_hole1.tcl SCI_SPEC: Characterization of the north polar coronal hole. Goal is to measure the properties of the north 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 the high latitude coronal holes. Roll positions are VL-corrected for PA=5 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: 2002.03.15.18:03 end: 2002.03.16.04:13 ONUMs = 17228 (27 exps) 17229 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 347.1, 348.3, 349.4 Degrees (16412, 16626, 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_168MPM in slot 1 Fits Files: q02.03.15.17:50:04.lya.dat q02.03.15.17:50:04.ovi.dat q02.03.15.17:50:04.vld.dat q02.03.15.21:59:56.lya.dat q02.03.15.21:59:56.ovi.dat q02.03.15.21:59:56.vld.dat 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: 2002.03.16.04:23 end: 2002.03.16.17:36 ONUMs = 37940 (37 exps) 37941 (37 exps) 37942 (56 exps) 37943 (37 exps) 37944 (37 exps) 37945 (37 exps) 37946 (37 exps) 37947 (37 exps) Instrument configuration: - Pointing: Sun center - Roll: W: STR2B, NW: STR2B, N: STR1A, 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: 181000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_181 in slot 2 Fits Files: z02.03.16.04:22:45.lya.dat z02.03.16.04:22:45.ovi.dat z02.03.16.04:22:45.vld.dat z02.03.16.05:57:11.lya.dat z02.03.16.05:57:11.ovi.dat z02.03.16.05:57:11.vld.dat z02.03.16.07:32:05.lya.dat z02.03.16.07:32:05.ovi.dat z02.03.16.07:32:05.vld.dat z02.03.16.09:48:47.lya.dat z02.03.16.09:48:47.ovi.dat z02.03.16.09:48:47.vld.dat z02.03.16.11:23:09.lya.dat z02.03.16.11:23:09.ovi.dat z02.03.16.11:23:09.vld.dat z02.03.16.12:57:20.lya.dat z02.03.16.12:57:20.ovi.dat z02.03.16.12:57:20.vld.dat z02.03.16.14:31:47.lya.dat z02.03.16.14:31:47.ovi.dat z02.03.16.14:31:47.vld.dat z02.03.16.16:06:42.lya.dat z02.03.16.16:06:42.ovi.dat z02.03.16.16:06:42.vld.dat