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

	Date:		30 November 2009
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 	Last revision:	03 December 2009 (MU)
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	File Name: 	2009.12.01.a.log
	----------

	Compiled by:	M. Uzzo
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	UVCS Activity:	Coronal Hole Weekly Study for 01-07 December 2009
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	SOHO Activity:	
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	EOF Staff:	J. Kohl: Lead Scientist
	----------	M. Uzzo:  Commander, Planner
			

	Command file:   09.11.30.13:02:13.cmd.log

	Activity:
	---------
	
	1) North Coronal Hole Weekly Study (1.7 Ro)
	
	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.

	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: 2009.12.01.04:31
		    end: 2009.12.01.18:19

	ONUMs = 26009 (80 exps)   
		26010 (320 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 0 Degrees (51551)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    50 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:
	
q09.12.01.04:31:20.ovi.dat
q09.12.01.07:17:56.ovi.dat

	2) North Coronal Hole Weekly Study (2.0 Ro)
	
	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.

	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: 2009.12.01.18:20
		    end: 2009.12.03.00:40

	ONUMs = 26011 (80 exps)   
		26012 (400 exps)
		26013 (399 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 0 Degrees (51551)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

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

q09.12.01.18:20:33.ovi.dat
q09.12.01.21:07:10.ovi.dat
q09.12.02.10:53:50.ovi.dat