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

	Date:		28 December 2006
	-----

 	Last revision:	03 January 2007 (Wu)
	--------------

	File Name: 	2006.12.31.a.log
	----------

	Compiled by:	R. Wu
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	UVCS Activity:	North Polar Coronal Hole OVI Observation for
	--------------	31 December 2006 - 01 January 2007

	SOHO Activity:	Received via email Friday, 01 January 2007, 
	--------------	05:00:48 GMT: OBT DISTRIBUTED TO UVCS BY FOT

	EOF Staff:	J. Kohl: Lead Scientist
	----------	R. Wu: Commander
			M. Uzzo: Planner

	Command file:	06.12.28.20:52:00.cmd.log

	Activity:
	---------

	1) North Coronal Hole Observations

	Sequence: 06.08_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0

	SCI_SPEC: Characterization of a polar coronal hole.
		  Goal is to measure the properties of a polar
		  coronal hole. In particular we are interested in the 
		  coronal conditions (intensities and line widths for 
		  HI Ly-alpha and OVI 1032/1037) as a function of height 
		  and latitude. We will compare these properties with 
		  the ones found in non-polar coronal holes.

		  Roll positions are VL-corrected for PA=0 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2006.12.31.01:35
		    end: 2007.01.01.00:36

	ONUMs = 22987 (320 exps)   
		22988 (348 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	354.38 Degrees (50528)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q06.12.31.01:35:11.ovi.dat
q06.12.31.12:36:31.ovi.dat