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

	Date:		07 March 2008
	-----

 	Last revision:	10 March 2008 (Wu)
	--------------

	File Name: 	2008.03.08.a.log
	----------

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

	UVCS Activity:	Streamer Study OVI Observations for 08 March 2008
	--------------	Streamer Study OVI Observations for 08 March 2008
			Streamer Study OVI Observations for 08 March 2008
			Streamer Study OVI Observations for 08 - 09 March 2008

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

	EOF Staff:      L. Strachan: Lead Scientist
	----------	R. Wu: Commander
			M. Uzzo: Planner

	Command file:	08.03.07.16:11:00.cmd.log

	Activity:
	---------

 	1) Streamer Study OVI Observations

	Sequence: 08.01_StrObsOVI.tcl, sw = 21

        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: 2008.03.08.00:36
		    end: 2008.03.08.05:18

	ONUMs = 24102 (16 exps)   
		24103 (120 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	85 Degrees (34246)

		- Mirror/Occulter:  2.5 Ro
				    1.5 mm overocculting

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

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

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Str_Prof in slot 5

	Fits Files:

q08.03.08.00:34:51.ovi.dat
q08.03.08.01:08:54.ovi.dat

	2) Streamer Study OVI Observations

	Sequence: 08.02_StrObsOVI.tcl, sw = 4

        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: 2008.03.08.05:20
		    end: 2008.03.08.12:31

	ONUMs = 24104 (20 exps)   
		24105 (188 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	85 Degrees (34246)

		- Mirror/Occulter:  2.5 Ro
				    1.5 mm overocculting

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

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

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Str_Prof in slot 5

	Fits Files:

q08.03.08.05:19:02.ovi.dat
q08.03.08.06:01:28.ovi.dat

	3) Streamer Study OVI Observations

	Sequence: 08.02_StrObsOVI.tcl, sw = 4

        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: 2008.03.08.12:33
		    end: 2008.03.08.19:44

	ONUMs = 24106 (20 exps)   
		24107 (188 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	85 Degrees (34246)

		- Mirror/Occulter:  2.5 Ro
				    1.5 mm overocculting

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

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

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Str_Prof in slot 5

	Fits Files:

q08.03.08.12:31:37.ovi.dat
q08.03.08.13:14:02.ovi.dat

 	4) Streamer Study OVI Observations

	Sequence: 08.01_StrObsOVI.tcl, sw = 21

        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: 2008.03.08.19:46
		    end: 2008.03.09.00:28

	ONUMs = 24108 (16 exps)   
		24109 (120 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	85 Degrees (34246)

		- Mirror/Occulter:  2.5 Ro
				    1.5 mm overocculting

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

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

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Str_Prof in slot 5

	Fits Files:

q08.03.08.19:44:42.ovi.dat
q08.03.08.20:18:52.ovi.dat