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

	Date:		30 January 2007
	-----

 	Last revision:	06 February 2007 (Ko)
	--------------

	File Name:	2007.01.29.a.log
	----------

	Compiled by:	M. Uzzo, R .Wu
	------------

	UVCS Activity:	Observations of Polar Coronal Holes 
	--------------	for 29 - 30 January 2007
			Observations of Polar Coronal Holes 
			for 30 January 2007
			Load Observations of Polar Coronal Holes 
			for 30 - 31 January 2007
			Load Observations of Polar Coronal Holes 
			for 31 - 01 February 2007
			Load Observations of Polar Coronal Holes 
			for 01 - 02 February 2007

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

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

	Command file:	07.01.28.14:42:13.cmd.log
			07.01.29.16:46:00.cmd.log

	Activity:
	---------

 	1) Observations of Polar Coronal Holes

	Sequence: 07.01_Daniele.tcl  n = 8, m = 3, r = 0

	SCI_SPEC: Main scientific objective is to make some comparisons
		  between coronal hole and streamer observations in
		  order to study plasma properties varying with time.

	OBS_PROG: Primary: Temporal Coverage
	          Sub Obj: Temporal Resolution

	SCI_OBJ:  Primary: Plasma Properties
	          Sub Obj: Ion Temperatures

	OBJ:      Entire Corona

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2007.01.29.06:23
                    end: 2007.01.30.06:29

	ONUMs =	23067 (240 exps)
		23068 (240 exps)
		23069 (160 exps)
		23070 (60 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll:  180 Degrees (18762)

		- Mirror/Occulter:  1.7 Ro
                                    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q07.01.29.06:22:51.ovi.dat
q07.01.29.14:38:51.ovi.dat
q07.01.29.22:54:51.ovi.dat
q07.01.30.04:25:31.ovi.dat

 	2) Observations of Polar Coronal Holes

	Sequence: 07.01_Daniele.tcl  n = 4, m = 0, r = 0

	SCI_SPEC: Main scientific objective is to make some comparisons
		  between coronal hole and streamer observations in
		  order to study plasma properties varying with time.

	OBS_PROG: Primary: Temporal Coverage
	          Sub Obj: Temporal Resolution

	SCI_OBJ:  Primary: Plasma Properties
	          Sub Obj: Ion Temperatures

	OBJ:      Entire Corona

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2007.01.30.06:31
                    end: 2007.01.30.17:32

	ONUMs =	23071 (237 exps)
		23072 (80 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll:  180 Degrees (18762)

		- Mirror/Occulter:  1.7 Ro
                                    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q07.01.30.06:31:07.ovi.dat
q07.01.30.14:47:07.ovi.dat