UVCS MISSION LOG 
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	Date:		14 July 2009
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 	Last revision:	16 July 2009 (Wu)
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	File Name: 	2009.07.15.a.log
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	Compiled by:	M. Uzzo, R. Wu
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	UVCS Activity:	North Coronal Hole Study for 15 - 16 July 2009 
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	SOHO Activity:	
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	EOF Staff:	M. P. Miralles / J. Kohl: Lead Scientist
	----------	M. Uzzo: Commander, Planner
			R. Wu

	Command file:	09.07.14.14:40:50.cmd.log

	Activity:
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	1) North Polar Coronal Hole Study

	Sequence: 09.07_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: 2009.07.15.23:18
		    end: 2009.07.16.22:19

	ONUMs = 25626 (318 exps)   
		25627 (347 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 352.09 Degrees (50331)

		- Mirror/Occulter:  2.1 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    50 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 232100

		- OVI MCP Voltage: 205  

		- OVI mask:   OVI_Hole_237 in slot 2

	Fits Files:

q09.07.15.23:18:20.ovi.dat

GAP between 07/16/09|01:10:24(12361) and 07/16/09|01:11:26(12458)

q09.07.16.10:19:40.ovi.dat