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

	Date:		16 July 2007
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 	Last revision:	19 July 2007 (Wu)
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	File Name: 	2007.07.18.a.log
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	Compiled by:	Y.-K. Ko
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	UVCS Activity:	South Polar Coronal Hole OVI Observation for
	--------------	18 July 2007

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

	EOF Staff:	M. P. Miralles: Lead Scientist
	----------	Y.-K. Ko: Commander, Planner
			M. Uzzo
			R. Wu

	Command file:	07.07.16.15:23:40.cmd.log

	Activity:
	---------
 
	1) South Polar Coronal Hole OVI Observations

	Sequence: 06.08_hole.tcl, n = 6, m = 3, p = 1, r = 0, 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=180 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: 2007.07.18.05:01
		    end: 2007.07.18.23:58

	ONUMs = 23504 (320 exps)   
                23505 (230 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	173.27 Degrees (17537)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q07.07.18.05:01:08.ovi.dat
q07.07.18.16:02:28.ovi.dat