UVCS MISSION LOG 
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	Date:		24 June 2009
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 	Last revision:	26 June 2009 (Wu)
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	File Name: 	2009.06.25.a.log
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	Compiled by:	M. Uzzo
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	UVCS Activity:	North Coronal Hole Study for 25 - 26 June 2009 
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	SOHO Activity:	
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	EOF Staff:	M. P. Miralles: Lead Scientist
	----------	R. Wu: Commander
			M. Uzzo: Planner

	Command file:	09.06.24.13:38:21.cmd.log
			09.06.26.12:41:51.cmd.log

	Activity:
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	1) North Polar Coronal Hole Study

	Sequence: 09.01_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: 2009.06.25.20:09
		    end: 2009.06.26.14:47

	ONUMs = 25576 (320 exps)   
		25577 (221 exps) ; aborted

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 354.381 Degrees (50528)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 235900

		- OVI MCP Voltage: 205  

		- OVI mask:   OVI_Hole_237 in slot 2

	Fits Files:

q09.06.25.20:09:06.ovi.dat
q09.06.26.07:10:26.ovi.dat