UVCS MISSION LOG ---------------- Date: 02 January 2004 ----- Last revision: 07 January 2004 (Wu) -------------- File Name: 2004.01.04.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Mini-Synoptic for 04 January 2004 -------------- North Coronal Hole Observation for 04 January 2004 Load North Coronal Hole Observation for 05 January 2004 using Batch Queue Time Tagged Commands via Background Queue (Background Queue File Submitted 02 January 2004) Load North Coronal Hole Observation for 06 January 2004 using Batch Queue Time Tagged Commands via Background Queue (Background Queue File Submitted 02 January 2004) SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: UVC40102.BCK Activity: --------- 1) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 215, LYA grating position now at 128000 "permanently". NB: Data missing from last position recovered. Part of VIRGO record time on SSR. OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2004.01.04.08:52 end: 2004.01.04.12:18 ONUMs = 44200 (9 exps) 44201 (9 exps) 44202 (9 exps) 44203 (9 exps) 44204 (9 exps) 44205 (9 exps) 44206 (9 exps) 44207 (9 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: E, SE, S, SW, W, NW, N, NE - Mirror/Occulter: 1.6, 1.75 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75 Ro) - LYA Slits: 50 um - OVI Slits: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 184200 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_184 in slot 2 Fits Files: GAP between 01/04/04|08:50:24( 8828) and 01/04/04|08:51:41( 8953) z04.01.04.08:51:01.lya.dat z04.01.04.08:51:01.ovi.dat z04.01.04.08:51:01.vld.dat z04.01.04.09:17:25.lya.dat z04.01.04.09:17:25.ovi.dat z04.01.04.09:17:25.vld.dat z04.01.04.09:44:08.lya.dat z04.01.04.09:44:08.ovi.dat z04.01.04.09:44:08.vld.dat z04.01.04.10:10:37.lya.dat z04.01.04.10:10:37.ovi.dat z04.01.04.10:10:37.vld.dat z04.01.04.10:37:06.lya.dat z04.01.04.10:37:06.ovi.dat z04.01.04.10:37:06.vld.dat z04.01.04.11:03:35.lya.dat z04.01.04.11:03:35.ovi.dat z04.01.04.11:03:35.vld.dat z04.01.04.11:30:12.lya.dat z04.01.04.11:30:12.ovi.dat z04.01.04.11:30:12.vld.dat z04.01.04.11:56:45.lya.dat z04.01.04.11:56:45.ovi.dat z04.01.04.11:56:45.vld.dat 2) Observation of the North Coronal Hole Sequence: 03.12_hole5short2.tcl, n53min=2 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=335 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: 2004.01.04.15:55 end: 2004.01.04.18:13 ONUMs = 20717 (26 exps) 20718 (35 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 328.27, 327.09, 328.277 degrees (45775, 45560, 45775) - Mirror/Occulter: 2.0, 1.7, 2.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 128000 - OVI GRTPOS: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q04.01.04.15:54:32.lya.dat q04.01.04.15:54:32.ovi.dat q04.01.04.15:54:32.vld.dat q04.01.04.16:54:54.lya.dat q04.01.04.16:54:54.ovi.dat q04.01.04.16:54:54.vld.dat