UVCS MISSION LOG
				----------------

	Date:		14 August 2003
	-----

 	Last revision:	19 August 2003 (Wu)
	--------------

	File Name: 	2003.08.16.a.log
	-----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	UVCS / VLA Coordinated Observation for 
	--------------	16 - 17 August 2003
			Mini-Synoptic for 17 August 2003

	SOHO Activity: 
	--------------

	EOF Staff:	S. Cranmer: Lead Scientist
	----------	R. Wu: Commander
			M. Uzzo: Planner

	Command file:	03.08.13.15:08:00.cmd.log


	Activity:
	---------

	1) UVCS with VLA Faraday rotation observations using radio source 3C228

	Sequence: 03.08_UVCS_VLA_str.tcl

	SCI_SPEC: Steve Spangler will obtain VLA observations of the radio
		  source 3C228 to search for Faraday rotation fluctuations
		  due to waves in the solar corona.  We expect the source
		  to pass behind a streamer in the later part of his
		  observation at about 7 solar radii and the north coronal 
		  hole at about 4 solar radii.  UVCS will observe O VI and 
		  Lyman lines to determine kinetic temperatures, average 
		  densities and outflow speeds.

		  Roll positions are VL-corrected for PA=348 degrees.

	OBS_PROG: Primary: Spatial Coverage
		  Sub Obj: Sensitivity

	SCI_OBJ:  Plasma Properties...Ion Temperatures
		  Plasma Properties...Density

	OBJ:      Streamer

	CMP_NAME: Observations of the Radio Source 3C228, UVCS; VLA (GBO)

	CMP_NUM:  6975

	Duration: start: 2003.08.15.16:33
                    end: 2003.08.16.12:17

	ONUMs =	20190 (160 exps)
		20191 (144 exps)
		20192 (176 exps)
		20193 (56 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  180 Degrees

		- Roll: 50 Degrees (60653)
 
		- Mirror/Occulter:  7.00, 4.50, 3.50, 3.00, 2.50, 2.10, 1.90, 
				    1.75, 1.60  Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:    50, 75 um 

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 175604

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_str_175 in slot 6

	Fits Files:

q03.08.16.16:33:18.lya.dat
q03.08.16.16:33:18.ovi.dat
q03.08.16.16:33:18.vld.dat
q03.08.16.22:20:38.lya.dat
q03.08.16.22:20:38.ovi.dat
q03.08.16.22:20:38.vld.dat
q03.08.17.03:34:00.lya.dat
q03.08.17.03:34:00.ovi.dat
q03.08.17.03:34:00.vld.dat
q03.08.17.10:05:05.lya.dat
q03.08.17.10:05:05.ovi.dat
q03.08.17.10:05:05.vld.dat

	2) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	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: 2003.08.17.12:51
		    end: 2003.08.17.16:17

	ONUMs = 42930 (9 exps) 
		42931 (9 exps) 
		42932 (9 exps) 
		42933 (9 exps) 
		42934 (9 exps) 
		42935 (9 exps) 
		42936 (9 exps) 
		42937 (9 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  180 Degrees

		- Roll: E, SE, S, SW, W, NW, N, NE

		- Mirror/Occulter: 1.6, 1.75 Ro
 				   1.5 mm overocculting (1.6 Ro)
				   2.0 mm overocculting (1.75 Ro)

		- LYA Slits:   50 um
		- OVI Slits:  150 um

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 192000

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_Syn_192 in slot 2
	
	Fits Files:

z03.08.17.12:50:09.lya.dat
z03.08.17.12:50:09.ovi.dat
z03.08.17.12:50:09.vld.dat
z03.08.17.13:16:27.lya.dat
z03.08.17.13:16:27.ovi.dat
z03.08.17.13:16:27.vld.dat
z03.08.17.13:42:56.lya.dat
z03.08.17.13:42:56.ovi.dat
z03.08.17.13:42:56.vld.dat
z03.08.17.14:09:32.lya.dat
z03.08.17.14:09:32.ovi.dat
z03.08.17.14:09:32.vld.dat
z03.08.17.14:36:01.lya.dat
z03.08.17.14:36:01.ovi.dat
z03.08.17.14:36:01.vld.dat
z03.08.17.15:02:30.lya.dat
z03.08.17.15:02:30.ovi.dat
z03.08.17.15:02:30.vld.dat
z03.08.17.15:28:59.lya.dat
z03.08.17.15:28:59.ovi.dat
z03.08.17.15:28:59.vld.dat
z03.08.17.15:55:42.lya.dat
z03.08.17.15:55:42.ovi.dat
z03.08.17.15:55:42.vld.dat