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

	Date:		23 December 2008
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 	Last revision:	29 December 2008 (Wu)
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	File Name: 	2008.12.26.a.log
	----------

	Compiled by:	R. Wu
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	UVCS Activity:	South Polar Coronal Hole OVI Observation for 
	--------------	26 - 27 December 2008

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

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

	Command file:	08.12.23.15:11:00.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole Observations

	Sequence: 08.11_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.

		  Note: New Nominal OVI MCP Voltage = 205

	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: 2008.11.26.15:25
		    end: 2008.11.27.14:26

	ONUMs = 25024 (320 exps)   
		25025 (345 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 172.09 Degrees (17322)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    50 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 223500

		- OVI MCP Voltage: 205 (Nominal) 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.12.26.15:25:04.ovi.dat
q08.12.27.02:26:24.ovi.dat

GAP between 12/27/08|04:15:40( 1959) and 12/27/08|04:16:51( 2067)
GAP between 12/27/08|06:40:46(15898) and 12/27/08|06:43:25(16148)