UVCS MISSION LOG 
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	Date:		09 October 2007
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 	Last revision:	12 October 2007 (MU)
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	File Name: 	2007.10.10.a.log
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	Compiled by:   	Y.-K. Ko
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	UVCS Activity:  North Coronal Hole OVI Observation for 
	--------------	10 - 11 October 2007

	SOHO Activity:	
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	EOF Staff:      S. Cranmer: Lead Scientist
	---------- 	M. Uzzo: Planner
			Y.-K. Ko: Commander, Planner

	Command file:	07.10.09.18:14:19.cmd.log
                        
	Activity:
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	1) North Polar Coronal Hole OVI 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: 2007.10.10.16:12
		    end: 2007.10.11.15:12

	ONUMs = 23745 (318 exps)   
		23746 (348 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	354.38 Degrees (17739)

		- 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:

q07.10.10.16:12:04.ovi.dat
q07.10.11.03:13:24.ovi.dat