UVCS MISSION LOG ---------------- Date: 26 September 2002 ----- Last revision: 30 September 2002 (Wu) -------------- File Name: 2002.09.27.a.log ----------- Compiled by: R. Wu ------------ UVCS Activity: Southern Coronal Hole Study for 27 - 28 September 2002 -------------- Load Southern Coronal Hole Study for 28 September 2002 Load Southern Coronal Hole Study for 28 September 2002 Load Synoptic for 28 September 2002 Load Southern Coronal Hole Study for 28 - 29 September 2002 Load Southern Coronal Hole Study for 29 September 200 Load Mini-Synoptic for 29 September 2002 Load Southern Coronal Hole Study for 29 - 30 September 2002 Load Southern Coronal Hole Study for 30 September 200 Load Mini-Synoptic for 30 September 2002 SOHO Activity: -------------- EOF Staff: J. Kohl: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 02.09.27.12:59:59.cmd.log Activity: --------- 1) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 02.06_hole1.tcl SCI_SPEC: Characterization of a high-latitude 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=130 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: 2002.09.27.13:39 end: 2002.09.27.23:49 ONUMs = 18070 (27 exps) 18071 (36 exps) Instrument configuration: - Pointing: Sun center - Roll: 122.093, 123.267, 124.381 Degrees (40998, 41212, 41415) - 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: q02.09.27.13:27:58.lya.dat q02.09.27.13:27:58.ovi.dat q02.09.27.13:27:58.vld.dat q02.09.27.17:35:27.lya.dat q02.09.27.17:35:27.ovi.dat q02.09.27.17:35:27.vld.dat 2) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 02.06_hole6.tcl SCI_SPEC: Characterization of a high-latitude 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=130 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: 2002.09.27.23:51 end: 2002.09.28.01:29 ONUMs = 18072 (18 exps) Instrument configuration: - Pointing: Sun center - Roll: 124.381 Degrees (41415) - Mirror/Occulter: 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: q02.09.27.23:49:07.lya.dat q02.09.27.23:49:07.ovi.dat q02.09.27.23:49:07.vld.dat 3) Observation of High-Latitude South Hemisphere Coronal Hole Sequence: 02.06_hole6.tcl SCI_SPEC: Characterization of a high-latitude 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=130 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: 2002.09.28.01:31 end: 2002.09.28.03:09 ONUMs = 18073 (18 exps) Instrument configuration: - Pointing: Sun center - Roll: 124.381 Degrees (41415) - Mirror/Occulter: 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: q02.09.28.01:29:05.lya.dat q02.09.28.01:29:05.ovi.dat q02.09.28.01:29:05.vld.dat 4) Synoptic Sequence Load and Start Sequence: SynopticA:Start 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: 2002.09.28.03:32 end: 2002.09.28.16:46 ONUMs = 39920 (36 exps) 39921 (37 exps) 39922 (36 exps) 39923 (37 exps) 39924 (37 exps) 39925 (56 exps) 39926 (37 exps) 39927 (37 exps) Instrument configuration: - Pointing: Sun center - Roll: W: STR2B, NW: STR2B, N: STR2B, NE: STR2B, E: STR2B, SE: STR1A, S: STR2B, SW: STR2B - Mirror/Occulter: STR1A: 3.5, 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR2B: 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro STR3A: 3.5, 3.0 Ro STR4B: 4.0 Ro STR5A: 2.1, 1.9, 1.75, 1.6 Ro STR6B: 2.5 Ro STR7B: 3.0 Ro CH1A: 1.9, 1.75, 1.6 Ro CH2A: 2.1 Ro CH2B: 2.1 Ro CH3B: 2.5 Ro CH4A: 1.75, 1.6 Ro CH5B: 1.9 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75, 1.9, 2.1, 2.5, 3.0, 3.5, 4.0 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (STR1A, STR2B, STR3A, STR4B, CH1A, CH2A, CH2B, CH3B) 100 um (CH4A, CH5B) 75 um (STR5A, STR6B, STR7B) - LYA GRTPOS: 128000 - OVI GRTPOS: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.09.28.03:31:31.lya.dat z02.09.28.03:31:31.ovi.dat z02.09.28.03:31:31.vld.dat z02.09.28.05:06:16.lya.dat z02.09.28.05:06:16.ovi.dat z02.09.28.05:06:16.vld.dat z02.09.28.06:40:56.lya.dat z02.09.28.06:40:56.ovi.dat z02.09.28.06:40:56.vld.dat z02.09.28.08:15:23.lya.dat z02.09.28.08:15:23.ovi.dat z02.09.28.08:15:23.vld.dat z02.09.28.09:50:02.lya.dat z02.09.28.09:50:02.ovi.dat z02.09.28.09:50:02.vld.dat z02.09.28.11:24:32.lya.dat z02.09.28.11:24:32.ovi.dat z02.09.28.11:24:32.vld.dat z02.09.28.13:41:22.lya.dat z02.09.28.13:41:22.ovi.dat z02.09.28.13:41:22.vld.dat z02.09.28.15:16:00.lya.dat z02.09.28.15:16:00.ovi.dat z02.09.28.15:16:00.vld.dat