UVCS MISSION LOG ---------------- Date: 21 January 2003 ----- Last revision: 23 January 2003 (Wu) -------------- File Name: 2003.01.22.a.log ----------- Compiled by: Y.-K. Ko, M. Uzzo, R. Wu ------------ UVCS Activity: North Coronal Hole Study for 22 - 23 January 2003 -------------- North Coronal Hole Study for 23 January 2003 Mini-Synoptic for 23 January 2003 Flush Loaded Observations and Reload with New Positions Load and Start North Coronal Hole Study for 22 - 23 January 2003 Load North Coronal Hole Study for 23 January 2003 Load Mini-Synoptic for 23 January 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo: Commander, Planner R. Wu: Commander Command file: 03.01.21.15:49:00.cmd.log 03.01.22.15:55:00.cmd.log Activity: --------- 1) Observation of the North Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the north 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=6 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: 2003.01.22.1 end: 2003.01.23.1 ONUMs = 18471 (27 exps) ; not run 18472 (36 exps) ; not run Instrument configuration: - Pointing: Sun center - Roll: 358.09, 359.27, 0.38 Degrees (18415, 18629, 18831) - 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: 2) Observation of the North Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of the north 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=6 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: 2003.01.23.0 end: 2003.01.23.1 ONUMs = 18473 (6 exps) ; not run 18474 (54 exps) ; not run Instrument configuration: - Pointing: Sun center - Roll: 358.09, 0.38 Degrees (18415, 18831) - 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: 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: 2003.01.23.1 end: 2003.01.23.1 ONUMs = 41110 (9 exps) ; not run 41111 (9 exps) ; not run 41112 (9 exps) ; not run 41113 (9 exps) ; not run 41114 (9 exps) ; not run 41115 (9 exps) ; not run 41116 (9 exps) ; not run 41117 (9 exps) ; not run 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: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: 4) Observation of the North Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the north 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=355 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: 2003.01.22.17:05 end: 2003.01.23.13:15 ONUMs = 18471 (27 exps) 18472 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 347.093, 348.267, 349.381 Degrees (16412, 16626, 16829) - 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: q03.01.22.16:51:01.lya.dat q03.01.22.16:51:01.ovi.dat q03.01.22.16:51:01.vld.dat q03.01.22.21:01:07.lya.dat q03.01.22.21:01:07.ovi.dat q03.01.22.21:01:07.vld.dat 5) Observation of the North Coronal Hole Sequence: 02.12_hole5.tcl SCI_SPEC: Characterization of the north 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=355 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: 2003.01.23.03:17 end: 2003.01.23.13:10 ONUMs = 18473 (6 exps) 18474 (54 exps) Instrument configuration: - Pointing: Sun center - Roll: 347.093, 349.381 Degrees (16412, 16829) - 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: q03.01.23.03:15:11.lya.dat q03.01.23.03:15:11.ovi.dat q03.01.23.03:15:11.vld.dat q03.01.23.03:49:48.lya.dat q03.01.23.03:49:48.ovi.dat q03.01.23.03:49:48.vld.dat 6) 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: 2003.01.23.13:20 end: 2003.01.23.16:47 ONUMs = 41110 (9 exps) 41111 (9 exps) 41112 (9 exps) 41113 (9 exps) 41114 (9 exps) 41115 (9 exps) 41116 (9 exps) 41117 (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: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_194372 in slot 2 Fits Files: z03.01.23.13:19:23.lya.dat z03.01.23.13:19:23.ovi.dat z03.01.23.13:19:23.vld.dat z03.01.23.13:46:09.lya.dat z03.01.23.13:46:09.ovi.dat z03.01.23.13:46:09.vld.dat z03.01.23.14:12:37.lya.dat z03.01.23.14:12:37.ovi.dat z03.01.23.14:12:37.vld.dat z03.01.23.14:39:06.lya.dat z03.01.23.14:39:06.ovi.dat z03.01.23.14:39:06.vld.dat z03.01.23.15:05:35.lya.dat z03.01.23.15:05:35.ovi.dat z03.01.23.15:05:35.vld.dat z03.01.23.15:32:19.lya.dat z03.01.23.15:32:19.ovi.dat z03.01.23.15:32:19.vld.dat z03.01.23.15:59:02.lya.dat z03.01.23.15:59:02.ovi.dat z03.01.23.15:59:02.vld.dat z03.01.23.16:25:29.lya.dat z03.01.23.16:25:29.ovi.dat z03.01.23.16:25:29.vld.dat