UVCS MISSION LOG ---------------- Date: 11 June 2003 ----- Last revision: 13 June 2003 (Wu) -------------- File Name: 2003.06.12.a.log ----------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start Southern Coronal Hole Observation for -------------- 12 - 13 June 2003 Load Southern Coronal Hole Observation for 13 June 2003 Load Mini-Synoptic for 13 June 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- M. Uzzo: Commander Y.-K. Ko: Planner R. Wu Command file: 03.06.12.12:48:54.cmd.log Activity: --------- 1) Observation of a Southern Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of a mid-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=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: 2003.06.12.19:54 end: 2003.06.13.06:04 ONUMs = 19948 (25 exps) 19949 (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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.06.12.19:52:03.lya.dat q03.06.12.19:52:03.ovi.dat q03.06.12.19:52:03.vld.dat GAP between 06/12/03|22:26:37( 9719) and 06/12/03|22:34:21(10465) GAP between 06/12/03|22:34:22(10468) and 06/12/03|22:39:00(10908) q03.06.12.23:50:44.lya.dat q03.06.12.23:50:44.ovi.dat q03.06.12.23:50:44.vld.dat 2) Observation of a Southern Coronal Hole Sequence: 02.12_hole5short.tcl SCI_SPEC: Characterization of a mid-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=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: 2003.06.13.06:07 end: 2003.06.13.12:53 ONUMs = 19946 (6 exps) ; loaded with wrong ONUMs 19947 (36 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: 170300 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_170300MPM in slot 5 Fits Files: q03.06.13.06:04:54.lya.dat q03.06.13.06:04:54.ovi.dat q03.06.13.06:04:54.vld.dat q03.06.13.06:39:25.lya.dat q03.06.13.06:39:25.ovi.dat q03.06.13.06:39:25.vld.dat 3) 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: 2003.06.13.13:25 end: 2003.06.13.16:52 ONUMs = 42500 (9 exps) 42501 (9 exps) 42502 (9 exps) 42503 (9 exps) 42504 (9 exps) 42505 (9 exps) 42506 (9 exps) 42507 (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: z03.06.13.13:24:31.lya.dat z03.06.13.13:24:31.ovi.dat z03.06.13.13:24:31.vld.dat z03.06.13.13:51:08.lya.dat z03.06.13.13:51:08.ovi.dat z03.06.13.13:51:08.vld.dat z03.06.13.14:17:33.lya.dat z03.06.13.14:17:33.ovi.dat z03.06.13.14:17:33.vld.dat z03.06.13.14:44:06.lya.dat z03.06.13.14:44:06.ovi.dat z03.06.13.14:44:06.vld.dat z03.06.13.15:10:50.lya.dat z03.06.13.15:10:50.ovi.dat z03.06.13.15:10:50.vld.dat z03.06.13.15:37:18.lya.dat z03.06.13.15:37:18.ovi.dat z03.06.13.15:37:18.vld.dat z03.06.13.16:03:47.lya.dat z03.06.13.16:03:47.ovi.dat z03.06.13.16:03:47.vld.dat z03.06.13.16:30:14.lya.dat z03.06.13.16:30:14.ovi.dat z03.06.13.16:30:14.vld.dat