UVCS MISSION LOG ---------------- Date: 05 September 2003 ----- Last revision: 08 September 2003 (Wu) -------------- File Name: 2003.09.05.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Load and Start South Coronal Hole Observation -------------- for 05 - 06 September 2003 Load Synoptic for 06 September 2003 Load South Coronal Hole Observation for 06 - 07 September 2003 Load South Coronal Hole Observation for 07 September 2003 Load Mini Synoptic for 07 September 2003 Load South Coronal Hole Observation for 07 - 08 September 2003 Load Synoptic for 08 September 2003 Load Global Dynamic Studies of the Extended Corona for 08 - 09 September 2003 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner R. Wu Command file: 03.09.05.14:54:36.cmd.log Activity: --------- 1) Observation of the South Coronal Hole Sequence: 02.12_hole1.tcl SCI_SPEC: Characterization of the south 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=188 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: 2003.09.05.18:54 end: 2003.09.06.05:04 ONUMs = 20284 (27 exps) 20285 (36 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 180.09, 181.27, 182.38 Degrees (18779, 18993, 19195) - 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: q03.09.05.18:41:27.lya.dat q03.09.05.18:41:27.ovi.dat q03.09.05.18:41:27.vld.dat q03.09.05.22:50:09.lya.dat q03.09.05.22:50:09.ovi.dat q03.09.05.22:50:09.vld.dat 2) Synoptic Sequence Load and Start Sequence: SynopticA:Start 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: 2003.09.06.05:15 end: 2003.09.06.17:45 ONUMs = 43110 (37 exps) 43111 (37 exps) 43112 (37 exps) 43113 (37 exps) 43114 (37 exps) 43115 (37 exps) 43116 (37 exps) 43117 (37 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: E: STR2B, SE: STR2B, S: STR2B, SW: STR2B, W: STR2B, NW: STR2B, N: STR2B, NE: 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: 192000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn_192 in slot 2 Fits Files: z03.09.06.05:14:12.lya.dat z03.09.06.05:14:12.ovi.dat z03.09.06.05:14:12.vld.dat z03.09.06.06:48:38.lya.dat z03.09.06.06:48:38.ovi.dat z03.09.06.06:48:38.vld.dat z03.09.06.08:23:19.lya.dat z03.09.06.08:23:19.ovi.dat z03.09.06.08:23:19.vld.dat z03.09.06.09:58:00.lya.dat z03.09.06.09:58:00.ovi.dat z03.09.06.09:58:00.vld.dat z03.09.06.11:32:26.lya.dat z03.09.06.11:32:26.ovi.dat z03.09.06.11:32:26.vld.dat z03.09.06.13:07:20.lya.dat z03.09.06.13:07:20.ovi.dat z03.09.06.13:07:20.vld.dat z03.09.06.14:41:35.lya.dat z03.09.06.14:41:35.ovi.dat z03.09.06.14:41:35.vld.dat z03.09.06.16:15:56.lya.dat z03.09.06.16:15:56.ovi.dat z03.09.06.16:15:56.vld.dat