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

	Date:		28 April 2006
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 	Last revision:	03 May 2006 (Wu)
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	File Name:	2006.04.30.a.log
	----------

	Compiled by:	R. Wu
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	UVCS Activity:	North Coronal Hole Observations in OVI for
        -------------- 	30 April - 01 May 2006

	SOHO Activity:	Received via email Monday, 01 May 2006, 04:01:13 GMT: 
	--------------	OBT DISTRIBUTED TO UVCS BY FOT

	EOF Staff:	M. P. Miralles: Lead Scientist
	---------	R. Wu: Commander
                        D. H. Phillips: Planner
                        M. Uzzo: Co-Planner
                        Y.-K. Ko

	Command file:	06.04.28.15:00:00.cmd.log

	Activity:
	---------

	1) North 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=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: 2006.04.30.09:40
		    end: 2006.05.01.08:40

	ONUMs = 22432 (334 exps)   
		22433 (332 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 Slits:   75 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:

q06.04.30.09:39:50.ovi.dat
q06.04.30.21:10:06.ovi.dat

GAP between 05/01/06|03:46:36(11970) and 05/01/06|03:48:38(12169)