UVCS MISSION LOG ---------------- Date: 15 October 2002 ----- Last revision: 17 October 2002 (Wu) -------------- File Name: 2002.10.15.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load and Start Southern Coronal Hole Study for -------------- 15 - 16 October 2002 Load Southern Coronal Hole Study for 16 October 2002 Load Mini-Synoptic for 16 October 2002 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 02.10.15.14:47:38.cmd.log Activity: --------- 1) Observation of Southern Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a high-latitude southern coronal hole. Goal is to measure the properties of a high-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=225 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: 2002.10.15.20:32 end: 2002.10.16.06:42 ONUMs = 18126 (27 exps) 18127 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 217.093, 218.267, 219.381 Degrees (58304, 58517, 58720)) - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.10.15.20:29:25.lya.dat q02.10.15.20:29:25.ovi.dat q02.10.15.20:29:25.vld.dat q02.10.16.00:27:55.lya.dat q02.10.16.00:27:55.ovi.dat q02.10.16.00:27:55.vld.dat 2) Observation of Southern Coronal Hole Sequence: 02.06_hole5.tcl SCI_SPEC: Characterization of a high-latitude southern coronal hole. Goal is to measure the properties of a high-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=225 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: 2002.10.16.06:44 end: 2002.10.16.16:37 ONUMs = 18128 (6 exps) 18129 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 217.093, 219.381 Degrees (58304, 58720) - 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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_173MPM in slot 1 Fits Files: q02.10.16.06:41:59.lya.dat q02.10.16.06:41:59.ovi.dat q02.10.16.06:41:59.vld.dat q02.10.16.07:16:36.lya.dat q02.10.16.07:16:36.ovi.dat q02.10.16.07:16:36.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: 2002.10.16.17:09 end: 2002.10.16.20:35 ONUMs = 40100 (9 exps) 40101 (9 exps) 40102 (9 exps) 40103 (9 exps) 40104 (9 exps) 40105 (9 exps) 40106 (9 exps) 40107 (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: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.10.16.17:08:01.lya.dat z02.10.16.17:08:01.ovi.dat z02.10.16.17:08:01.vld.dat z02.10.16.17:34:26.lya.dat z02.10.16.17:34:26.ovi.dat z02.10.16.17:34:26.vld.dat z02.10.16.18:00:48.lya.dat z02.10.16.18:00:48.ovi.dat z02.10.16.18:00:48.vld.dat z02.10.16.18:27:23.lya.dat z02.10.16.18:27:23.ovi.dat z02.10.16.18:27:23.vld.dat z02.10.16.18:53:52.lya.dat z02.10.16.18:53:52.ovi.dat z02.10.16.18:53:52.vld.dat z02.10.16.19:20:21.lya.dat z02.10.16.19:20:21.ovi.dat z02.10.16.19:20:21.vld.dat z02.10.16.19:46:43.lya.dat z02.10.16.19:46:43.ovi.dat z02.10.16.19:46:43.vld.dat z02.10.16.20:13:16.lya.dat z02.10.16.20:13:16.ovi.dat z02.10.16.20:13:16.vld.dat