UVCS MISSION LOG ---------------- Date: 31 July 2008 ----- Last revision: 07 August 2008 (Wu) -------------- File Name: 2008.08.04.a.log ---------- Compiled by: R. Wu, M. Uzzo ------------ UVCS Activity: OVI Detector Diagnostic for 04 August 2008 -------------- North Polar Coronal Hole OVI Observation for 04 - 05 August 2008 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander M. Uzzo: Planner Command file: 08.07.31.14:39:00.cmd.log Activity: --------- 1) OVI Detector Diagnostic Sequence: OVI_164_chk.tcl SCI_SPEC: Instrument Diagnostics Note: This observation lost to SOHO 26m keyhole. OBS_PROG: Spatial Resolution SCI_OBJ: Calibration OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.08.04.12: end: 2008.08.04.13: ONUMs = 24651 (0 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 0 Degrees (51551) - Mirror/Occulter: 1.75 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_chk_1xfull in slot 6 Fits Files: GAP between 08/04/08|09:45:40(10823) and 08/04/08|17:00:27( 3435) 2) North Polar Coronal Hole Observations Sequence: 08.01_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of a 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=0 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: 2008.08.04.16:58 end: 2008.08.05.12:42 ONUMs = 24652 (191 exps) 24653 (78 exps) ; aborted Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 354.38 Degrees (50528) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: GAP between 08/04/08|09:45:40(10823) and 08/04/08|17:00:27( 3435) q08.08.04.13:51:59.ovi.dat GAP between 08/04/08|19:29:24( 1362) and 08/04/08|19:30:25( 1465) GAP between 08/04/08|23:35:46( 8655) and 08/05/08|10:03:24( 3412) q08.08.05.00:53:19.ovi.dat