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

	Date:		26 April 2006
	-----

 	Last revision:	01 May 2006 (Wu)
	--------------

	File Name:	2006.04.27.a.log
	----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	North Coronal Hole Observations in OVI for
        -------------- 	27 - 28 April 2006 

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

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

	Command file:	06.04.26.14:28:00.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: 2006.04.27.11:31
		    end: 2006.04.28.10:32

	ONUMs = 22425 (334 exps)   
		22426 (330 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:

q06.04.27.11:31:09.ovi.dat
q06.04.27.23:01:25.ovi.dat