UVCS MISSION LOG ---------------- Date: 04 March 2004 ----- Last revision: 08 March 2004 (Wu) -------------- File Name: 2004.03.05.a.log ---------- Compiled by: R. Wu ------------ UVCS Activity: Equatorial Coronal Hole LyA Observation for -------------- 05 March 2004 Equatorial Coronal Hole OVI Observation for 05 - 06 March 2004 Equatorial Coronal Hole OVI Observation for 06 March 2004 Mini-Synoptic for 06 March 2004 Load Equatorial Coronal Hole LyA Observation for 06 March 2004 Load Equatorial Coronal Hole OVI Observation for 06 - 07 March 2004 Load Equatorial Coronal Hole OVI Observation for 07 March 2004 Load Mini-Synoptic for 07 March 2004 Load Equatorial Coronal Hole LyA Observation for 07 - 08 March 2004 Load Equatorial Coronal Hole OVI Observation for 08 March 2004 Load Equatorial Coronal Hole OVI Observation for 08 March 2004 Load Mini-Synoptic for 08 March 2004 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- R. Wu: Commander Y.-K. Ko: Planner M. Uzzo Command file: 04.03.04.15:44:00.cmd.log Activity: --------- 1) Equatorial Coronal Hole Observation Sequence: 04.02_hole1LyA.tcl SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=285 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: 2004.03.05.15:43 end: 2004.03.05.20:41 ONUMs = 21052 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 277.09, 278.27, 279.38 degrees (36447, 36661, 36864) - 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: 188940 - OVI MCP Voltage: 200 - OVI mask: OVI_sp_188 in slot 6 Fits Files: q04.03.05.15:29:44.ovi.dat q04.03.05.15:29:44.vld.dat 2) Equatorial Coronal Hole Observation Sequence: 04.02_hole1OVI.tcl SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=285 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: 2004.03.05.20:43 end: 2004.03.06.06:47 ONUMs = 21053 (103 exps) 21054 (166 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 277.09, 278.27, 279.38 degrees (36447, 36661, 36864) - 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: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 4 Fits Files: q04.03.05.20:41:48.ovi.dat q04.03.05.20:41:48.vld.dat GAP between 03/05/04|23:03:04(10306) and 03/05/04|23:06:05(10599) GAP between 03/05/04|23:06:13(10602) and 03/05/04|23:07:15(10704) q04.03.06.00:36:30.ovi.dat q04.03.06.00:36:30.vld.dat 3) Equatorial Coronal Hole Observation Sequence: 04.02_holexOVI.tcl, n53min = 5 SCI_SPEC: Characterization of an equatorial coronal hole. Goal is to measure the properties of a non-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 polar coronal holes. Roll positions are VL-corrected for PA=285 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: 2004.03.06.06:49 end: 2004.03.06.12:12 ONUMs = 21055 (14 exps) 21056 (132 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 277.09, 279.38 degrees (36447, 36864) - 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: 230000 - OVI MCP Voltage: 200 - OVI mask: OVI_MPM_232 in slot 4 Fits Files: q04.03.06.06:47:38.ovi.dat q04.03.06.06:47:38.vld.dat q04.03.06.07:20:58.ovi.dat q04.03.06.07:20:58.vld.dat 4) Mini-Synoptic Sequence Load and Start Sequence: SynopticC:Start SCI_SPEC: Synoptic studies. LYA HV & Power off / OVI voltage at 200, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2004.03.06.12:32 end: 2004.03.06.17:52 ONUMs = 44650 (9 exps) 44651 (9 exps) 44652 (35 exps) 44653 (9 exps) 44654 (35 exps) 44655 (9 exps) 44656 (9 exps) 44657 (9 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: E: mini_str, SE: mini_str, S: mini_ch, SW: mini_str, W: mini_ch, NW: mini_str, N: mini_str, NE: mini_str - Mirror/Occulter: lya_str: 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro lya_ch: 2.10, 1.90, 1.75, 1.60 Ro ovi_str: 3.00, 2.10, 1.90, 1.75, 1.60 Ro ovi_ch: 1.90, 1.75, 1.60 Ro mini_str: 2.10, 1.75, 1.60 Ro mini_ch: 1.90, 1.75, 1.60 Ro 1.5 mm overocculting (1.60 Ro) 2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00 Ro) - LYA Slits: 50 um - OVI Slits: 150 um (LyA Synoptic) 200 um (OVI, and Mini Synoptic) - LYA GRTPOS: 128000 - OVI GRTPOS: 177596 (LyA Synoptic) 229000 (OVI, and Mini Synoptic) - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_178 in slot 2 (LyA Synoptic) OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic) Fits Files: z04.03.06.12:31:56.ovi.dat z04.03.06.12:31:56.vld.dat z04.03.06.12:59:02.ovi.dat z04.03.06.12:59:02.vld.dat z04.03.06.13:26:09.ovi.dat z04.03.06.13:26:09.vld.dat z04.03.06.14:47:22.ovi.dat z04.03.06.14:47:22.vld.dat z04.03.06.15:14:34.ovi.dat z04.03.06.15:14:34.vld.dat z04.03.06.16:35:52.ovi.dat z04.03.06.16:35:52.vld.dat z04.03.06.17:02:59.ovi.dat z04.03.06.17:02:59.vld.dat z04.03.06.17:30:10.ovi.dat z04.03.06.17:30:10.vld.dat