UVCS MISSION LOG ---------------- Date: 16 September 2003 ----- Last revision: 16 September 2003 (Wu) -------------- File Name: 2003.09.16.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load and Start North Polar Coronal Hole Observation -------------- for 16 - 17 September 2003 Flush and Abort North Polar Coronal Hole Observation for 16 - 17 September 2003 Reload and Start North Polar Coronal Hole Observation for 16 - 17 September 2003 Load North Polar Coronal Hole Observation for 17 September 2003 Load Mini-Synoptic for 17 September 2003 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 03.09.16.13:15:58.cmd.log Activity: --------- 1) Observation of the North Polar Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the north 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=350 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: 2003.09.16.14:39 end: 2003.09.16.15:06 ONUMs = 20301 (5 exps) ; Flushed, not completed 20302 (36 exps) ; Flushed, not run Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 342.09, 343.27, 344.38 Degrees (48291, 48505, 48708) - 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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.09.16.14:25:51.lya.dat q03.09.16.14:25:51.ovi.dat q03.09.16.14:25:51.vld.dat 2) Observation of the North Polar Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the north 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=350 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: 2003.09.16.15:12 end: 2003.09.17.01:22 ONUMs = 20302 (27 exps) 20303 (36 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 342.09, 343.27, 344.38 Degrees (48291, 48505, 48708) - 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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.09.16.15:10:35.lya.dat q03.09.16.15:10:35.ovi.dat q03.09.16.15:10:35.vld.dat q03.09.16.19:08:29.lya.dat q03.09.16.19:08:29.ovi.dat q03.09.16.19:08:29.vld.dat 3) Observation of the North Polar Coronal Hole Sequence: 03.02_hole5short.tcl, nhour=6 SCI_SPEC: Characterization of the north 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=350 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: 2003.09.17.01:24 end: 2003.09.17.06:06 ONUMs = 20304 (6 exps) 20305 (24 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 342.09, 344.38 Degrees (48291, 48708) - 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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.09.17.01:22:32.lya.dat q03.09.17.01:22:32.ovi.dat q03.09.17.01:22:32.vld.dat q03.09.17.01:56:55.lya.dat q03.09.17.01:56:55.ovi.dat q03.09.17.01:56:55.vld.dat 4) 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". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2003.09.17.06:33 end: 2003.09.17.09:59 ONUMs = 43220 (9 exps) 43221 (9 exps) 43222 (9 exps) 43223 (9 exps) 43224 (9 exps) 43225 (9 exps) 43226 (9 exps) 43227 (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: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z03.09.17.06:32:03.lya.dat z03.09.17.06:32:03.ovi.dat z03.09.17.06:32:03.vld.dat z03.09.17.06:58:44.lya.dat z03.09.17.06:58:44.ovi.dat z03.09.17.06:58:44.vld.dat z03.09.17.07:25:28.lya.dat z03.09.17.07:25:28.ovi.dat z03.09.17.07:25:28.vld.dat z03.09.17.07:51:57.lya.dat z03.09.17.07:51:57.ovi.dat z03.09.17.07:51:57.vld.dat z03.09.17.08:18:26.lya.dat z03.09.17.08:18:26.ovi.dat z03.09.17.08:18:26.vld.dat z03.09.17.08:44:54.lya.dat z03.09.17.08:44:54.ovi.dat z03.09.17.08:44:54.vld.dat z03.09.17.09:11:23.lya.dat z03.09.17.09:11:23.ovi.dat z03.09.17.09:11:23.vld.dat z03.09.17.09:37:50.lya.dat z03.09.17.09:37:50.ovi.dat z03.09.17.09:37:50.vld.dat