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

	Date:		01 July 2009
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 	Last revision:	07 July 2009 (Wu)
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	File Name: 	2009.07.06.a.log
	----------

	Compiled by:	R. Wu
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	UVCS Activity:	OVI Detector Rate Diagnostic for 06 July 2009 
	--------------	North Coronal Hole Study for 06 - 07 July 2009
			Load North Coronal Hole Study for 07 - 08 July 2009
			Load OVI Detector Rate Diagnostic for 08 July 2009 
			Load North Coronal Hole Study for 08 - 09 July 2009
			Load North Coronal Hole Study for 09 - 10 July 2009
			Load OVI Detector Rate Diagnostic for 10 July 2009 
			Load North Coronal Hole Study for 10 - 11 July 2009
			Load North Coronal Hole Study for 11 - 12 July 2009
			Load OVI Detector Rate Diagnostic for 12 July 2009 
			Load North Coronal Hole Study for 12 - 13 July 2009

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

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

	Command file:	09.07.06.12:10:56.cmd.log

	Activity:
	---------

	1) OVI Detector Dark Rate Diagnostic

	Sequence: OVI_dark_chk.tcl

	SCI_SPEC: Determine Dark count rate for OVI detector. Instrument 
		  rolled to coronal hole, 5.0 Ro with 0.8 mm exposed mirror. 
		  Script engages OVI filter and then disengages it at end.

	OBS_PROG: Calibration

	SCI_OBJ:  Calibration

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2009.07.06.10:38
                    end: 2009.07.06.11:39

       	ONUMs =	25603 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  180 Degrees

		- Roll: 0 Degrees (51551)

		- Mirror/Occulter:  5.0 Ro
                                    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- OVI Filter Engaged

		- OVI MCP Voltage: 205 

		- OVI mask:   OVI_chk_1xfull in slot 6

	Fits Files:

q09.07.06.10:37:38.ovi.dat

	2) North Polar Coronal Hole Study

	Sequence: 09.07_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=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: 2009.07.06.11:41
		    end: 2009.07.07.10:41

	ONUMs = 25604 (319 exps)   
		25605 (348 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 352.09 Degrees (50331)

		- Mirror/Occulter:  2.1 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 232100

		- OVI MCP Voltage: 205  

		- OVI mask:   OVI_Hole_237 in slot 2

	Fits Files:

q09.07.06.11:40:52.ovi.dat
q09.07.06.22:42:12.ovi.dat