UVCS MISSION LOG ---------------- Date: 25 February 2005 ----- Last revision: 01 November 2005 (Wu) -------------- File Name: 2005.02.28.a.log ---------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Coronal Jet Observations for 28 February 2005 -------------- Flush, Reload and Start Coronal Jet Observations for 28 February - 01 March 2005 Load Mini Synoptic for 01 March 2005 SOHO Activity: Received via email Tuesday, 01 March 2005 04:00:50 GMT: -------------- OBT DISTRIBUTED TO UVCS BY FOT EOF Staff: D. Dobrzycka: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo Command file: 05.02.25.16:44:00.cmd.log 05.02.28.16:54:13.cmd.log Activity: --------- 1) Coronal Jet Observations, JOP 155 Sequence: 05.02_jop155.tcl, nhour = 18.5 SCI_SPEC: Study of the dynamic jet structures originating in the polar coronal holes. The polar jets were originally observed at solar minimum when the polar holes were large, dominating structures in the corona. At the current declining phase of the solar cycle the polar holes appeared again as permanent structures. The purpose of the observations is to study counterparts of solar minimum polar coronal jets. OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Coverage SCI_OBJ: Coronal Structure...Fine Structure OBJ: Coronal Hole CMP_NAME: Polar Coronal Jets; UVCS; CDS; EIT; TRACE CMP_NUM: 7111 Duration: start: 2005.02.28.15:19 end: 2005.02.28.17:00 ONUMs = 22178 (49 exps) ; aborted 22179 (80 exps) ; not run 22180 (80 exps) ; not run 22181 (80 exps) ; not run 22182 (80 exps) ; not run 22183 (80 exps) ; not run 22184 (80 exps) ; not run 22185 (48 exps) ; not run Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 170 degrees (16942) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q05.02.28.15:19:10.ovi.dat 2) Coronal Jet Observations, JOP 155 Sequence: 05.02_jop155.tcl, nhour = 18.5 SCI_SPEC: Study of the dynamic jet structures originating in the polar coronal holes. The polar jets were originally observed at solar minimum when the polar holes were large, dominating structures in the corona. At the current declining phase of the solar cycle the polar holes appeared again as permanent structures. The purpose of the observations is to study counterparts of solar minimum polar coronal jets. OBS_PROG: Primary: Spectral Coverage Sub Obj: Temporal Coverage SCI_OBJ: Coronal Structure...Fine Structure OBJ: Coronal Hole CMP_NAME: Polar Coronal Jets; UVCS; CDS; EIT; TRACE CMP_NUM: 7111 Duration: start: 2005.02.28.17:12 end: 2005.03.01.11:39 ONUMs = 22179 (80 exps) 22180 (80 exps) 22181 (80 exps) 22182 (80 exps) 22183 (80 exps) 22184 (80 exps) 22185 (56 exps) Instrument configuration: - Pointing: Sun Center - Spacecraft Roll: 180 Degrees - Roll: 175 degrees (17852) - Mirror/Occulter: 1.7 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 164600 - OVI MCP Voltage: 200 - OVI mask: OVI_sp1_164 in slot 4 Fits Files: q05.02.28.17:11:50.ovi.dat q05.02.28.19:57:10.ovi.dat q05.02.28.22:42:30.ovi.dat q05.03.01.01:27:50.ovi.dat q05.03.01.04:13:09.ovi.dat q05.03.01.06:58:29.ovi.dat q05.03.01.09:43:49.ovi.dat 3) Mini-Synoptic Sequence Load and Start Sequence: SynopticD:Start SCI_SPEC: Synoptic studies. VLD & 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: 2005.03.01.11:49 end: 2005.03.01.17:18 ONUMs = 47400 (9 exps) 47401 (9 exps) 47402 (35 exps) 47403 (9 exps) 47404 (9 exps) 47405 (9 exps) 47406 (35 exps) 47407 (9 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: E: ms, SE: ms, S: mc, SW: ms, W: ms, NW: ms, N: mc, NE: ms - Mirror/Occulter: ls: 3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro lc: 2.10, 1.90, 1.75, 1.60 Ro os: 3.00, 2.10, 1.90, 1.75, 1.60 Ro oc: 1.90, 1.75, 1.60 Ro ms: 2.10, 1.75, 1.60 Ro mc: 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: 187260 (LyA Synoptic) 229000 (OVI, and Mini Synoptic) - OVI MCP Voltage: 200 - OVI mask: OVI_Syn_188 in slot 2 (LyA Synoptic) OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic) Fits Files: z05.03.01.11:48:40.ovi.dat z05.03.01.12:13:36.ovi.dat z05.03.01.12:38:32.ovi.dat z05.03.01.13:57:12.ovi.dat z05.03.01.14:22:08.ovi.dat z05.03.01.14:47:04.ovi.dat z05.03.01.15:39:22.ovi.dat z05.03.01.16:58:02.ovi.dat