UVCS MISSION LOG 
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	Date:		11 April 2006
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 	Last revision:	14 April 2006 (Wu)
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	File Name:	2006.04.11.a.log
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	Compiled by:	R. Wu
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	UVCS Activity:	Load and Start South Coronal Hole Observations in OVI 
	--------------	for 11 - 12 April 2006
			Load OVI Detector Diagnostic for 12 April 2006
			Load South Coronal Hole Observations in OVI for 
			12 - 13 April 2006

	SOHO Activity:	
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	EOF Staff:	J. Kohl: Lead Scientist
	---------	R. Wu Commander
			Y.-K. Ko: Planner
			M. Uzzo

	Command file:	06.04.11.12:24:00.cmd.log

	Activity:
	---------

	1) South Coronal Hole Observations

	Sequence: 06.04_holeOVI24.tcl

	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: South Coronal Hole Study, UVCS; LASCO

	CMP_NUM:  7180

	Duration: start: 2006.04.11.20:05
		    end: 2006.04.12.19:05

	ONUMs = 22379 (334 exps) 
		22380 (334 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	174.38 Degrees (50528)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

		- LYA Slits:  100 um
		- OVI Slits:   75 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q06.04.11.20:04:43.ovi.dat
q06.04.12.07:34:59.ovi.dat