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

	Date:		17 January 2006
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 	Last revision:	17 February 2006 (Wu)
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	File Name:	2006.01.18.a.log
	----------

	Compiled by:	M. Uzzo
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	UVCS Activity:	South Polar Coronal Hole OVI Observation for
	--------------	18 - 19 January 2006

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

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

	Command file:	06.01.17.15:47:23.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole Observation 

	Sequence: 06.01_holeOVI.tcl, r = 24, n6hr = 7

	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: 2006.01.18.00:17
		    end: 2006.01.19.18:15

	ONUMs = 22131 (174 exps)
		22132 (174 exps)
		22133 (174 exps)
		22134 (143 exps)
		22135 (174 exps)
		22136 (174 exps)
		22137 (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:

q06.01.18.00:17:29.ovi.dat
q06.01.18.06:17:05.ovi.dat
q06.01.18.12:16:41.ovi.dat
q06.01.18.18:16:17.ovi.dat

GAP between 01/18/06|21:41:16( 4762) and 01/18/06|22:44:56(10874)

q06.01.19.00:15:53.ovi.dat
q06.01.19.06:15:29.ovi.dat
q06.01.19.12:15:05.ovi.dat