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

	Date:		09 October 2009
	-----

 	Last revision:	26 October 2009 (Wu)
	--------------

	File Name: 	2009.10.09.a.log
	----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	Load and Start Coronal Hole Intensity Study for 
	--------------	09 October 2009
			Load Coronal Hole Intensity Study for 
			09 - 10 October 2009
			Load Coronal Hole Intensity Study for 
			10 - 11 October 2009
			Load OVI Detector Dark Rate Diagnostic for
			11 October 2009
			Load Coronal Hole Intensity Study for 
			11 - 12 October 2009
			Load Coronal Hole Intensity Study for 
			12 - 13 October 2009
			Load Coronal Hole Intensity Study for 13 October 2009
			Load OVI Detector Dark Rate Diagnostic for
			13 October 2009

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

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

	Command file:   09.10.09.13:28:21.cmd.log

	Activity:
	---------

	1) Coronal Hole Intensity Study
   
	Sequence: 09.10_HoleIntOVI.tcl, n = 1, m = 3, p = 0, r = 0, e = 0 

	SCI_SPEC:  The purpose of this series of observations is to track the 
		   changes in polar coronal hole intensities that are occuring 
		   during the current prolonged solar minimum, and compare them 
		   to the intensities observed at the time of the previous 
		   minimum.

	OBS_PROG: Temporal Coverage

	SCI_OBJ:  Plasma Properties

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2009.10.09.20:08
		    end: 2009.10.10.00:57

	ONUMs =	25883 (140 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll:	352.1 Degrees (17322)

		- Mirror/Occulter:  1.70 Ro
				    1.5mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   300 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 232100

		- OVI MCP Voltage: 205

		- OVI mask:   OVI_Hole_237 in slot 2

	Fits Files:

q09.10.09.20:08:09.ovi.dat

	2) Coronal Hole Intensity Study
   
	Sequence: 09.10_HoleIntOVI.tcl, n = 5, m = 2, p = 0, r = 0, e = 0 

	SCI_SPEC:  The purpose of this series of observations is to track the 
		   changes in polar coronal hole intensities that are occuring 
		   during the current prolonged solar minimum, and compare them 
		   to the intensities observed at the time of the previous 
		   minimum.

	OBS_PROG: Temporal Coverage

	SCI_OBJ:  Plasma Properties

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2009.10.10.00:59
		    end: 2009.10.10.16:08

	ONUMs =	25884 (320 exps)
		25885 (120 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll:	353.3 Degrees (17537)

		- Mirror/Occulter:  2.00 Ro
				    1.5mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   300 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 232100

		- OVI MCP Voltage: 205

		- OVI mask:   OVI_Hole_237 in slot 2

	Fits Files:

q09.10.10.00:59:16.ovi.dat
q09.10.10.12:00:36.ovi.dat