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

	Date:		13 January 2006
	-----

 	Last revision:	17 February 2006 (Wu)
	--------------

	File Name:	2006.01.16.a.log
	----------

	Compiled by:	R. Wu
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	UVCS Activity:	South Polar Coronal Hole OVI Observation for 
        --------------  15 - 17 January 2006

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

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

	Command file:	06.01.13.19:56:00.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole Observation 

	Sequence: 06.01_holeOVI.tcl, r = 24, n6hr = 8

	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: 2006.01.15.23:17
                    end: 2006.01.17.23:14

	ONUMs = 22122 (174 exps)
		22123 (174 exps)
		22124 (174 exps)
		22125 (174 exps)
		22126 (174 exps)
		22127 (174 exps)
		22128 (174 exps)
		22129 (174 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 354.38 degrees (17739)

		- Mirror/Occulter:  2.4 Ro
			            1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 5

	Fits Files:

q06.01.15.23:16:58.ovi.dat
q06.01.16.05:16:34.ovi.dat
q06.01.16.11:16:10.ovi.dat
q06.01.16.17:15:46.ovi.dat
q06.01.16.23:15:22.ovi.dat
q06.01.17.05:14:58.ovi.dat
q06.01.17.11:14:34.ovi.dat
q06.01.17.17:14:10.ovi.dat