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

	Date:		11 March 2010
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 	Last revision:	22 March 2010 (RR)
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	File Name: 	2010.03.11.a.log
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	Compiled by:	R. Rosati
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	UVCS Activity:	Load South Coronal Hole OVI Observations for
	--------------	09 Mar 2010 - 16 Mar 2010
			 
				
	SOHO Activity:	
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	EOF Staff:	J. Kohl: Lead Scientist
	----------	R. Rosati: Commander
		
			

	Command file:   10.03.09.16:40:13.cmd.log

	Activity:
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	1) South Coronal hole weekly observation
   
	Sequence: HoleOVIweek.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: 2010.03.11.12:45
		    end: 2010.03.12.03:30

	ONUMs = 26182 (217 exps)


	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll:	-90 Degrees (51551)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting
					
				    2.0 Ro
				    1.5 mm overocculting

				    2.4 Ro
				    1.5 mm overocculting



		- LYA Slit:   100 um
		- OVI Slit:    50, 75, 100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600, 232100


		- OVI MCP Voltage: 205

		- OVI mask:  OVI_sp2_164  in slot 4
			     OVI_Hole_237 in slot 2

	Fits Files:


q10.03.11.16:35:17.ovi.dat