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

	Date:		04 October 2005
	-----

 	Last revision:	04 October 2005 (Wu)
	--------------

	File Name:	2005.10.03.a.log
	----------

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

	UVCS Activity:	Load and Start Streamer Study for 03 - 04 October 2005
	--------------	Load Streamer Study for 04 October 2005
			Load Streamer Study for 04 - 05 October 2005

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

	EOF Staff:      M. Uzzo: Lead Scientist
	---------- 	R. Wu: Commander
			M. Uzzo: Planner
			Y.-K. Ko

	Command file:	05.10.03.20:09:00.cmd.log

	Activity:
	---------

	1) Streamer Properties Over the Solar Cycle

	Sequence: 05.09_StrObs.tcl, sw = 41

	SCI_SPEC: A comprehensive study of several streamer properties 
		  including the outflow velocities, abundances, electron
		  densities and temperatures. The spatial distribution
		  of these physical properties are analyzed at multiple 
	          heights within several streamers examined over the 
		  course of the solar cycle.  

	OBS_PROG: Primary: Spectral Resolution
		  Sub Obj: Spatial Resolution

	SCI_OBJ:  Primary: Coronal Dynamics...Outflow Velocities
		  Sub Obj: Abundances

	OBJ:      Streamer

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2005.10.03.21:06
                    end: 2005.10.04.04:33

	ONUMs =	21773 (24 exps)
		21774 (191 exps)
	
	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 0 Degrees

		- Roll: 280 Degrees (4198)

		- Mirror/Occulter:  4.00 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600, 223500

		- OVI MCP Voltage: 200 

		- OVI mask:   msk_000303_OVI  in slot 3
			      OVI_str_164_225 in slot 6

	Fits Files:

q05.10.03.21:04:56.ovi.dat
q05.10.03.21:55:39.ovi.dat

	2) Streamer Properties Over the Solar Cycle

	Sequence: 05.09_StrObs.tcl, sw = 41

	SCI_SPEC: A comprehensive study of several streamer properties 
		  including the outflow velocities, abundances, electron
		  densities and temperatures. The spatial distribution
		  of these physical properties are analyzed at multiple 
	          heights within several streamers examined over the 
		  course of the solar cycle.  

	OBS_PROG: Primary: Spectral Resolution
		  Sub Obj: Spatial Resolution

	SCI_OBJ:  Primary: Coronal Dynamics...Outflow Velocities
		  Sub Obj: Abundances

	OBJ:      Streamer

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2005.10.04.04:35
                    end: 2005.10.04.12:03

	ONUMs =	21775 (24 exps)
		21776 (192 exps)
	
	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 0 Degrees

		- Roll: 280 Degrees (4198)

		- Mirror/Occulter:  4.00 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600, 223500

		- OVI MCP Voltage: 200 

		- OVI mask:   msk_000303_OVI  in slot 3
			      OVI_str_164_225 in slot 6

	Fits Files:

q05.10.04.04:34:04.ovi.dat
q05.10.04.05:24:45.ovi.dat