UVCS MISSION LOG ---------------- Date: 17 February 2004 ----- Last revision: 19 February 2004 (Wu) -------------- File Name: 2004.02.18.a.log ---------- Compiled by: Y.-K. Ko ------------ UVCS Activity: North Coronal Hole OVI Observation for -------------- 18 - 19 February 2004 Mini-Synoptic for 19 February 2004 Load Star Calibration using 38 Aquarius for 19 February 2004 using Batch Queue time-tagged commands via NRT Load Star Calibration using 38 Aquarius for 19 February 2004 using Batch Queue time-tagged commands via NRT Load North Coronal Observations for 19 - 20 February 2004 Load Mini-Synoptic for 20 February 2004 Load Star Calibration using 38 Aquarius for 20 February 2004 using Batch Queue time-tagged commands via NRT Load Star Calibration using 38 Aquarius for 20 February 2004 using Batch Queue time-tagged commands via NRT SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo: Planner R. Wu Command file: 04.02.17.10:39:19.cmd.log 04.02.18.22:55:32.cmd.log Activity: --------- 1) North Coronal Hole Observation Sequence: 04.02_holexOVI.tcl, n53min = 11 SCI_SPEC: Characterization of the 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=354 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: 2004.02.18.16:47 end: 2004.02.19.03:27 ONUMs = 20982 (14 exps) 20983 (132 exps) 20984 (144 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 346.09, 348.38 degrees (49019, 49436) - Mirror/Occulter: 1.7, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50, 75 um - LYA GRTPOS: 128000 - OVI GRTPOS: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 4 Fits Files: q04.02.18.16:40:54.ovi.dat q04.02.18.16:40:54.vld.dat q04.02.18.17:19:36.ovi.dat q04.02.18.17:19:36.vld.dat q04.02.18.22:10:31.ovi.dat q04.02.18.22:10:31.vld.dat 2) Mini-Synoptic Sequence Load and Start Sequence: SynopticB:Start SCI_SPEC: Synoptic studies. LYA HV & Power off / OVI voltage at 200, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2004.02.19.03:35 end: 2004.02.19.08:22 ONUMs = 44480 (10 exps) 44481 (24 exps) 44482 (10 exps) 44483 (10 exps) 44484 (10 exps) 44485 (24 exps) 44486 (10 exps) 44487 (10 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: NE: mini_str, N: mini_ch, NW: mini_str, W: mini_str, SW: mini_str, S: mini_ch, SE: mini_str, E: mini_str, - Mirror/Occulter: lya_str: 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro lya_ch: 2.10, 1.90, 1.75, 1.60 Ro ovi_str: 3.00, 2.10, 1.90, 1.75, 1.60 Ro ovi_ch: 1.90, 1.75, 1.60 Ro mini_str: 2.10, 1.75, 1.60 Ro mini_ch: 1.90, 1.75, 1.60 Ro 1.5 mm overocculting (1.60 Ro) 2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00 Ro) - LYA Slits: 50 um - OVI Slits: 100 um (LyA Synoptic) 150 um (OVI, and Mini Synoptic) - LYA GRTPOS: 128000 - OVI GRTPOS: 177596 (LyA Synoptic) 229000 (OVI, and Mini Synoptic) - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_178 in slot 2 (LyA Synoptic) OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic) Fits Files: z04.02.19.03:34:33.ovi.dat z04.02.19.03:34:33.vld.dat z04.02.19.04:03:51.ovi.dat z04.02.19.04:03:51.vld.dat z04.02.19.05:02:14.ovi.dat z04.02.19.05:02:14.vld.dat z04.02.19.05:31:36.ovi.dat z04.02.19.05:31:36.vld.dat z04.02.19.06:01:00.ovi.dat z04.02.19.06:01:00.vld.dat z04.02.19.06:30:14.ovi.dat z04.02.19.06:30:14.vld.dat z04.02.19.07:28:27.ovi.dat z04.02.19.07:28:27.vld.dat z04.02.19.07:57:40.ovi.dat z04.02.19.07:57:40.vld.dat