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

	Date:		02 January 2008
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 	Last revision:	15 January 2008 (Wu)
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	File Name: 	2008.01.09.a.log
	----------

	Compiled by:	R. Wu, Y.-K. Ko
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	UVCS Activity:  South Coronal Hole OVI Observation for 
	--------------	09 - 10 January 2008
                        Load South Coronal Hole OVI Observation for
                        10 January 2008
                        Load OVI Detector Diagnostic for 10 January 2008

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

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

	Command file:	08.01.02.15:13:00.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole OVI Observations

	Sequence: 08.01_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=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: 2008.01.09.03:08
		    end: 2008.01.10.02:08

	ONUMs = 23955 (319 exps)   
                23956 (348 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	174.38 Degrees (17739)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    75 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.01.09.03:07:41.ovi.dat
q08.01.09.14:09:01.ovi.dat

GAP between 01/09/08|18:20:34( 5036) and 01/09/08|18:22:06( 5181)