UVCS MISSION LOG ---------------- Date: 22 September 2008 ----- Last revision: 06 October 2008 (Wu) -------------- File Name: 2008.09.25.a.log ---------- Compiled by: M. Uzzo, R. Wu ------------ UVCS Activity: Load and Start Prominence Coordinated Observation -------------- with Hinode and SUMER for 25 September 2008 Load and Start Prominence Coordinated Observation with Hinode and SUMER for 25 - 26 September 2008 Load Prominence Coordinated Observation with Hinode and SUMER for 26 September 2008 SOHO Activity: -------------- EOF Staff: J. Raymond: Lead Scientist ---------- M. Uzzo: Commander, Planner R. Wu Command file: 08.09.25.14:30:32.cmd.log Activity: --------- 1) Prominence Observations Sequence: 08.09_Prom_LYA.tcl SCI_SPEC: We wish to observe the plasma above a prominence in conjunction with SUMER observations (JOP207, S. Parenti). The Lyman lines and He II 1085 A are the primary lines of interest, but O VI will also be needed for density estimates. HiRes Centered @ 225 Degrees OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Resolution SCI_OBJ: Primary: Abundances Sub Obj: Density OBJ: Prominence CMP_NAME: JOP 207 / HOP 082, Quiescent and Eruptive Prominences, SUMER; UVCS; Hinode-EIS (S/C) CMP_NUM: 7287 Duration: start: 2008.09.25.16:06 end: 2008.09.25.17:04 ONUMs = 24755 (28 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 246 Degrees (63566) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_Str_Prof in slot 5 Fits Files: q08.09.25.16:06:02.ovi.dat 2) Prominence Observations Sequence: 08.09_Prom.tcl, n = 8, m = 0, r = 0, e = 0 SCI_SPEC: We wish to observe the plasma above a prominence in conjunction with SUMER observations (JOP207, S. Parenti). The Lyman lines and He II 1085 A are the primary lines of interest, but O VI will also be needed for density estimates. HiRes Centered @ 225 Degrees OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Resolution SCI_OBJ: Primary: Abundances Sub Obj: Density OBJ: Prominence CMP_NAME: JOP 207 / HOP 082, Quiescent and Eruptive Prominences, SUMER; UVCS; Hinode-EIS (S/C) CMP_NUM: 7287 Duration: start: 2008.09.25.17:06 end: 2008.09.26.15:08 ONUMs = 24756 (240 exps) 24757 (238 exps) 24758 (154 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 246 Degrees (63566) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 100 um - LYA GRTPOS: 100000 - OVI GRTPOS: 232100 - OVI MCP Voltage: 200 - OVI mask: OVI_303_8x2 in slot 3 Fits Files: q08.09.25.17:05:36.ovi.dat q08.09.26.01:21:36.ovi.dat GAP between 09/26/08|03:46:56( 1541) and 09/26/08|03:50:24( 1873) GAP between 09/26/08|05:30:11(11463) and 09/26/08|05:31:18(11560) GAP between 09/26/08|09:39:21( 2628) and 09/26/08|09:52:28( 3892) q08.09.26.09:37:36.ovi.dat 3) Prominence Observations Sequence: 08.09_Prom_LYA.tcl SCI_SPEC: We wish to observed the plasma above a prominence in conjunction with SUMER observations (JOP207, S. Parenti). The Lyman lines and He II 1085 A are the primary lines of interest, but O VI will also be needed for density estimates. HiRes Centered @ 225 Degrees OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Resolution SCI_OBJ: Primary: Abundances Sub Obj: Density OBJ: Prominence CMP_NAME: JOP 207 / HOP 082, Quiescent and Eruptive Prominences, SUMER; UVCS; Hinode-EIS (S/C) CMP_NUM: 7287 Duration: start: 2008.09.26.15:10 end: 2008.09.26.16:08 ONUMs = 24759 (28 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 0 Degrees - Roll: 246 Degrees (63566) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 50 um - LYA GRTPOS: 100000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_Str_Prof in slot 5 Fits Files: q08.09.26.15:09:59.ovi.dat