UVCS MISSION LOG ---------------- Date: 02 January 2004 ----- Last revision: 07 January 2004 (Wu) -------------- File Name: 2004.01.02.a.log ---------- Compiled by: R. Wu, M. Uzzo ------------ UVCS Activity: Coronal North Hole Observation for 02 January 2004 -------------- Coronal North Hole Observation for 02 January 2004 Load North Coronal Hole Observation for 03 January 2004 using Batch Queue Time Tagged Commands via the Background Queue Load North Coronal Hole Observation for 03 January 2004 using Batch Queue Time Tagged Commands via the Background Queue Load Mini-Synoptic for 04 January 2004 using Batch Queue Time Tagged Commands via the Background Queue Load North Coronal Hole Observation for 04 January 2004 using Batch Queue Time Tagged Commands via the Background Queue Load North Coronal Hole Observation for 05 January 2004 using Batch Queue Time Tagged Commands via the Background Queue Submit North Coronal Hole Observation for 05 January 2004 using Batch Queue Time Tagged Commands via the Background Queue (Separate File Uplinked 04 January 2004) Submit North Coronal Hole Observation for 06 January 2004 using Batch Queue Time Tagged Commands via the Background Queue (Separate File Uplinked 04 January 2004) SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: UVC31231.BCK UVC40102.BCK Activity: --------- 1) Observation of the North Coronal Hole Sequence: 03.12_hole5short3.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: 2004.01.02.08:10 end: 2004.01.02.10:46 ONUMs = 20709 (23 exps) 20710 (43 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 329.38, 327.09, 329.38 degrees (45977, 45560, 45977) - Mirror/Occulter: 2.4, 1.7, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 75, 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: q04.01.02.08:09:31.lya.dat q04.01.02.08:09:31.ovi.dat q04.01.02.08:09:31.vld.dat GAP between 01/02/04|08:15:24( 7293) and 01/02/04|08:18:39( 7607) q04.01.02.09:10:01.lya.dat q04.01.02.09:10:01.ovi.dat q04.01.02.09:10:01.vld.dat 2) Observation of the North Coronal Hole Sequence: 03.12_hole5short3.tcl, n53min=5 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: 2004.01.02.16:20 end: 2004.01.02.21:18 ONUMs = 20711 (23 exps) 20712 (107 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 329.38, 327.09, 329.38 degrees (45977, 45560, 45977) - Mirror/Occulter: 2.4, 1.7, 2.4 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 75, 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: q04.01.02.16:19:31.lya.dat q04.01.02.16:19:31.ovi.dat q04.01.02.16:19:31.vld.dat GAP between 01/02/04|16:30:20( 5700) and 01/02/04|16:36:45( 6311) q04.01.02.17:20:08.lya.dat q04.01.02.17:20:08.ovi.dat q04.01.02.17:20:08.vld.dat