UVCS MISSION LOG ---------------- Date: 14 July 2001 ----- Last revision: 16 July 2001 (Wu) -------------- File Name: 2001.07.14.a.log ----------- Compiled by: M. Uzzo ------------ UVCS Activity: Global Coronal Dynamics Study for -------------- 14 - 15 July 2001 Mid-latitude Coronal Hole Study for 15 July 2001 Mini-Synoptic for 15 July 2001 SOHO Activity: -------------- EOF Staff: C. Benna: Lead Scientist ---------- M. P. Miralles: Lead Scientist M. Uzzo: Commander, Planner Y.-K. Ko: Planner Command file: 01.07.12.18:00:32.cmd.log Activity: --------- 1) Global Coronal Dynamics Study Sequence: 01.07_benna_low.tcl SCI_SPEC: Solar maximum coronal dynamics studies -- gravitational settling studies. OBS_PROG: Primary: Spatial Coverage Sub Obj: Spectral Coverage SCI_OBJ: Coronal Dynamics...Outflow Velocities Abundances OBJ: Streamer CMP_NAME: CMP_NUM: Duration: start: 2001.07.14.16:12 end: 2001.07.15.02:09 ONUMs = 16435 (168 exps) Instrument configuration: - Pointing: Sun center - Roll: 6019 (290 deg) - Mirror/Occulter: 1.50, 1.55, 1.60, 1.65, 1.70, 1.75, 1.80, 1.85, 1.90, 1.95, 2.00, 2.05, 2.10, 2.15, 2.20, 2.25, 2.30, 2.35, 2.40, 2.45, 2.50 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 50 um - LYA GRTPOS: 128000 - OVI GRTPOS: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_GSS_192 in slot 6 Fits Files: q01.07.14.15:56:01.lya.dat q01.07.14.15:56:01.ovi.dat q01.07.14.15:56:01.vld.dat 2) Observation of High-Latitude Coronal Hole Sequence: 01.06_hole1.tcl SCI_SPEC: Characterization of a mid-latitude 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. Roll positions are VL-corrected for PA=340 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: 2001.07.15.02:15 end: 2001.07.15.12:25 ONUMs = 16436 (27 exps) 16437 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 13681, 13896, 14098 (332.09, 333.27, 334.38 deg) - 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: q01.07.15.02:09:08.lya.dat q01.07.15.02:09:08.ovi.dat q01.07.15.02:09:08.vld.dat q01.07.15.06:10:53.lya.dat q01.07.15.06:10:53.ovi.dat q01.07.15.06:10:53.vld.dat 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 210, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2001.07.15.12:33 end: 2001.07.15.16:00 ONUMs = 35750 (9 exps) 35751 (9 exps) 35752 (9 exps) 35753 (9 exps) 35754 (9 exps) 35755 (9 exps) 35756 (9 exps) 35757 (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: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z01.07.15.12:32:28.lya.dat z01.07.15.12:32:28.ovi.dat z01.07.15.12:32:28.vld.dat z01.07.15.12:58:47.lya.dat z01.07.15.12:58:47.ovi.dat z01.07.15.12:58:47.vld.dat z01.07.15.13:25:14.lya.dat z01.07.15.13:25:14.ovi.dat z01.07.15.13:25:14.vld.dat z01.07.15.13:51:50.lya.dat z01.07.15.13:51:50.ovi.dat z01.07.15.13:51:50.vld.dat z01.07.15.14:18:20.lya.dat z01.07.15.14:18:20.ovi.dat z01.07.15.14:18:20.vld.dat z01.07.15.14:44:48.lya.dat z01.07.15.14:44:48.ovi.dat z01.07.15.14:44:48.vld.dat z01.07.15.15:11:24.lya.dat z01.07.15.15:11:24.ovi.dat z01.07.15.15:11:24.vld.dat z01.07.15.15:37:52.lya.dat z01.07.15.15:37:52.ovi.dat z01.07.15.15:37:52.vld.dat