UVCS MISSION LOG ---------------- Date: 06 January 2004 ----- Last revision: 09 January 2004 (Wu) -------------- File Name: 2004.01.06.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Set Mirror/Occulter Heater to 0% (255 EU) -------------- Load and Start Synoptic for 06 - 07 January 2004 Load Coronal Hole Observation for 07 January 2004 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander, Planner Y.-K. Ko R. Wu Command file: 04.01.06.16:30:24.cmd.log Activity: --------- 1) 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: 2004.01.06.19:53 end: 2004.01.07.09:48 ONUMs = 44210 (37 exps) 44211 (37 exps) 44212 (37 exps) 44213 (37 exps) 44214 (56 exps) 44215 (36 exps) 44216 (56 exps) 44217 (37 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: NE: STR2B, N: STR2B, NW: STR2B, W: STR2B, SW: STR1A, S: STR2B, SE: STR1A, E: 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: 184200 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_184 in slot 2 Fits Files: z04.01.06.19:52:10.lya.dat z04.01.06.19:52:10.ovi.dat z04.01.06.19:52:10.vld.dat z04.01.06.21:27:05.lya.dat z04.01.06.21:27:05.ovi.dat z04.01.06.21:27:05.vld.dat z04.01.06.23:01:17.lya.dat z04.01.06.23:01:17.ovi.dat z04.01.06.23:01:17.vld.dat z04.01.07.00:35:58.lya.dat z04.01.07.00:35:58.ovi.dat z04.01.07.00:35:58.vld.dat z04.01.07.02:10:22.lya.dat z04.01.07.02:10:22.ovi.dat z04.01.07.02:10:22.vld.dat z04.01.07.04:27:01.lya.dat z04.01.07.04:27:01.ovi.dat z04.01.07.04:27:01.vld.dat z04.01.07.06:01:41.lya.dat z04.01.07.06:01:41.ovi.dat z04.01.07.06:01:41.vld.dat z04.01.07.08:18:07.lya.dat z04.01.07.08:18:07.ovi.dat z04.01.07.08:18:07.vld.dat GAP between 01/07/04|09:12:45( 37) and 01/07/04|09:14:13( 177) 2) Observation of the North Coronal Hole Sequence: 03.10_hole1.tcl SCI_SPEC: Characterization of a 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=0 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: 2004.01.07.10:15 end: 2004.01.07.19:41 ONUMs = 20727 (105 exps) 20728 (149 exps) ; aborted Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 352.09, 353.27, 354.38 degrees (50111, 50326, 50528) - 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: q04.01.07.10:09:01.lya.dat q04.01.07.10:09:01.ovi.dat q04.01.07.10:09:01.vld.dat q04.01.07.14:10:38.lya.dat q04.01.07.14:10:38.ovi.dat q04.01.07.14:10:38.vld.dat