UVCS MISSION LOG ---------------- Date: 06 March 2001 ----- Last revision: 06 March 2001 (MU) -------------- File Name: 2001.03.07.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Run Star calibration with Feige 110 -------------- Load Mid-latitude coronal hole for 03/08/01 Load Mini-Synoptic 03/08/01 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Commander, Planner D. Phillips: Planner S. Mancuso: Planner Y.-K. Ko Command file: 01.03.06.17:07:57.cmd.log 01.03.07.16:13:24.cmd.log Activity: --------- 1) Star Calibration of Feige 110 Sequence: Manual and TakeOVI_TxN SCI_SPEC: Star Observations to determine mirror degradation through comparison of stellar intensity at various occulter settings from this study and a similar study of the same star in 1996. OBS_PROG: Calibration SCI_OBJ: Calibration... OBJ: Star / Feige 110 CMP_NAME: CMP_NUM: Duration: start: 2001.03.07.16:53 end: 2001.03.08.01:56 ONUMs = 15935 (196 exps) Instrument configuration: - Pointing: Sun center - Roll: 115 degrees (39707) - Mirror/Occulter: From 7.47 to Ro Occulter 40.35mm - LYA Slits: 50 um - OVI Slits: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 235000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: Star_5x2 in slot 6 Fits Files: q01.03.07.16:52:24.ovi.dat 2) Observation of Low-Latitude Coronal Hole Sequence: 01.01_hole1a.tcl SCI_SPEC: Characterization of an Equatorial Coronal Hole. Goal is to measure the properties of a mid-latitude 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 polar coronal holes. 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: 2001.03.08.02:08 end: 2001.03.08.12:19 ONUMs = 15931 (27 exps) 15932 (35 exps) Instrument configuration: - Pointing: Sun center - Roll: 220.1, 221.3, 222.4 Degrees (58850, 59063, 59266) - 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: q01.03.08.02:03:15.lya.dat q01.03.08.02:03:15.ovi.dat q01.03.08.02:03:15.vld.dat q01.03.08.06:05:08.lya.dat q01.03.08.06:05:08.ovi.dat q01.03.08.06:05:08.vld.dat GAP between 03/08/01|08:50:15(15753) and 03/08/01|09:01:44( 472) 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 205, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2001.03.08.12:52 end: 2001.03.08.16:19 ONUMs = 34540 (9 exps) 34541 (9 exps) 34542 (9 exps) 34543 (9 exps) 34544 (9 exps) 34545 (9 exps) 34546 (9 exps) 34547 (9 exps) Instrument configuration: - Pointing: Sun center - Roll: W, NW, N, NE, E, SE, S, SW - 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: 168208 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_CME_168 in slot 4 Fits Files: z01.03.08.12:51:43.lya.dat z01.03.08.12:51:43.ovi.dat z01.03.08.12:51:43.vld.dat z01.03.08.13:18:21.lya.dat z01.03.08.13:18:21.ovi.dat z01.03.08.13:18:21.vld.dat z01.03.08.13:44:50.lya.dat z01.03.08.13:44:50.ovi.dat z01.03.08.13:44:50.vld.dat z01.03.08.14:11:11.lya.dat z01.03.08.14:11:11.ovi.dat z01.03.08.14:11:11.vld.dat z01.03.08.14:37:48.lya.dat z01.03.08.14:37:48.ovi.dat z01.03.08.14:37:48.vld.dat z01.03.08.15:04:16.lya.dat z01.03.08.15:04:16.ovi.dat z01.03.08.15:04:16.vld.dat z01.03.08.15:30:45.lya.dat z01.03.08.15:30:45.ovi.dat z01.03.08.15:30:45.vld.dat z01.03.08.15:57:06.lya.dat z01.03.08.15:57:06.ovi.dat z01.03.08.15:57:06.vld.dat