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

	Date:		24 March 2008
	-----

 	Last revision:	24 March 2008 (Wu)
	--------------

	File Name: 	2008.03.21.a.log
	----------

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

	UVCS Activity:  JOP 201: Linking the Corona to the Solar Wind at 
	-------------	Ulysses for 21 March 2008
			JOP 201: Linking the Corona to the Solar Wind at 
			Ulysses for 21 - 22 March 2008
			JOP 201: Linking the Corona to the Solar Wind at 
			Ulysses for 22 March 2008
			JOP 201: Linking the Corona to the Solar Wind at 
			Ulysses for 22 March 2008
			Flush Batch Queue
			Load JOP 201: Linking the Corona to the Solar 
			Wind at Ulysses for 23 March 2008
			Load JOP 201: Linking the Corona to the Solar 
			Wind at Ulysses for 23 - 24 March 2008
			Load JOP 201: Linking the Corona to the Solar 
			Wind at Ulysses for 24 March 2008
			Load JOP 201: Linking the Corona to the Solar 
			Wind at Ulysses for 24 March 2008

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

	EOF Staff:	G. Poletto: Lead Scientist
	----------	R. Wu: Commander
			M. Uzzo: Planner

	Command file:	08.03.20.20:00:00.cmd.log
			08.03.21.15:35:00.cmd.log

	Activity:
	---------

	1) Linking the Corona to the Solar Wind at Ulysses

	Sequence: 08.03_Poletto_WHI.tcl, sw = 17

	SCI_SPEC: Plume vs. interplume observations with the aim of 1) 
		  defining plume properties, with the help of other 
		  coordinated observations from TRACE, STEREO, possibly 
		  HINODE, 2) check whether wind originates preferentially 
		  from plume or interplume regions.

	OBS_PROG: Primary: Spatial Resolution
		  Sub Obj: Temporal Coverage

	SCI_OBJ:  Primary: Coronal Dynamics...Outflow Velocities
		  Sub Obj: Coronal Structure...Fine Structure

	OBJ:      Polar Plume

	CMP_NAME: JOP201, Fast wind from its source to Ulysses, 

	CMP_NUM:  7265

	Duration: start: 2008.03.21.21:15
		    end: 2008.03.21.23:19

	ONUMs = 24173 (60 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	194 Degrees (54100)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 um
		- OVI Slit:   100 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- LYA MCP Voltage: 195 

		- LYA mask:   LYA_VEX_4x1 in slot 2

	Fits Files:

q08.03.21.21:15:21.lya.dat

	2) Linking the Corona to the Solar Wind at Ulysses

	Sequence: 08.03_Poletto_WHI.tcl, sw = 20

	SCI_SPEC: Plume vs. interplume observations with the aim of 1) 
		  defining plume properties, with the help of other 
		  coordinated observations from TRACE, STEREO, possibly 
		  HINODE, 2) check whether wind originates preferentially 
		  from plume or interplume regions.

	OBS_PROG: Primary: Spatial Resolution
		  Sub Obj: Temporal Coverage

	SCI_OBJ:  Primary: Coronal Dynamics...Outflow Velocities
		  Sub Obj: Coronal Structure...Fine Structure

	OBJ:      Polar Plume

	CMP_NAME: JOP201, Fast wind from its source to Ulysses, 

	CMP_NUM:  7265

	Duration: start: 2008.03.21.23:20
		    end: 2008.03.22.02:06

	ONUMs = 24174 (80 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	192 Degrees (53736)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 um
		- OVI Slit:   100 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- LYA MCP Voltage: 195 

		- LYA mask:   LYA_VEX_4x1 in slot 2

	Fits Files:

q08.03.21.23:20:15.lya.dat

	3) Linking the Corona to the Solar Wind at Ulysses

	Sequence: 08.03_Poletto_WHI.tcl, sw = 24

	SCI_SPEC: Plume vs. interplume observations with the aim of 1) 
		  defining plume properties, with the help of other 
		  coordinated observations from TRACE, STEREO, possibly 
		  HINODE, 2) check whether wind originates preferentially 
		  from plume or interplume regions.

	OBS_PROG: Primary: Spatial Resolution
		  Sub Obj: Temporal Coverage

	SCI_OBJ:  Primary: Coronal Dynamics...Outflow Velocities
		  Sub Obj: Coronal Structure...Fine Structure

	OBJ:      Polar Plume

	CMP_NAME: JOP201, Fast wind from its source to Ulysses, 

	CMP_NUM:  7265

	Duration: start: 2008.03.22.02:06
		    end: 2008.03.22.08:02

	ONUMs = 24175 (171 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	190 Degrees (53371)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 um
		- OVI Slit:   100 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- LYA MCP Voltage: 195 

		- LYA mask:   LYA_VEX_4x1 in slot 2

	Fits Files:

q08.03.22.02:06:29.lya.dat

GAP between 03/22/08|05:12:20( 1713) and 03/22/08|05:13:44( 1842)

	4) Linking the Corona to the Solar Wind at Ulysses

	Sequence: 08.03_Poletto_WHI.tcl, sw = 30

	SCI_SPEC: Plume vs. interplume observations with the aim of 1) 
		  defining plume properties, with the help of other 
		  coordinated observations from TRACE, STEREO, possibly 
		  HINODE, 2) check whether wind originates preferentially 
		  from plume or interplume regions.

	OBS_PROG: Primary: Spatial Resolution
		  Sub Obj: Temporal Coverage

	SCI_OBJ:  Primary: Coronal Dynamics...Outflow Velocities
		  Sub Obj: Coronal Structure...Fine Structure

	OBJ:      Polar Plume

	CMP_NAME: JOP201, Fast wind from its source to Ulysses, 

	CMP_NUM:  7265

	Duration: start: 2008.03.22.08:03
		    end: 2008.03.22.21:08

	ONUMs = 24176 (380 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	 188 Degrees (53007)

		- Mirror/Occulter:  3.0 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 um
		- OVI Slit:   100 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- LYA MCP Voltage: 195 

		- LYA mask:   LYA_VEX_4x1 in slot 2

	Fits Files:

q08.03.22.08:02:51.lya.dat