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

	Date:		13 February 2007
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 	Last revision:	21 February 2007 (Wu)
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	File Name:	2007.02.17.a.log
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	Compiled by:	M. Uzzo
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	UVCS Activity:  Calibration Observation Using Star 38 Aquarius for 
	--------------	17 February 2007
 			Load and Start South Polar Coronal Hole LyA 
			Observation for 17 - 18 February 2007
 			Load South Polar Coronal Hole OVI Observation for 
			18 - 19 February 2007
			Load South Polar Coronal Hole OVI Observation for 
			19 February 2007
			OVI Detector Diagnostic for 19 February 2007

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

	EOF Staff:	L. Gardner / M. P. Miralles: Lead Scientist
	---------	M. Uzzo: Commander, Planner
			Y.-K. Ko
			R. Wu

	Command file:	07.02.17.11:31:06.cmd.log
	
	Activity:
	---------

	1) Calibration Using 38 Aquarius

	Sequence: Manual, TakeOVIexps.tcl

	SCI_SPEC: Star Observations to determine mirror degradation through 
		  comparison of stellar intensity at various occulter settings
		  from this study and a similar study of the same star in 1996.

	OBS_PROG: Calibration

	SCI_OBJ:  Calibration

	OBJ:      Star...38 Aqr

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2006.02.17.11:59
		    end: 2006.02.17.16:05

	ONUMs = 23155 (110 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll:  degrees (3470, 3561, 3652)
 
		- Mirror/Occulter: 8.43 - 7.85 Ro
				   Occulter @ 11 mm, 49 mm
 
		- LYA Slits:  100 um
		- OVI Slits:  150 um
 
		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- OVI MCP Voltage: 200 
 
		- OVI mask:   OVI_303_8x2 in slot 3
 
	Fits Files:

q07.02.17.11:47:01.ovi.dat

	2) South Coronal Hole Observations

	Sequence: 06.08_hole.tcl, n = , m = , p = , r = , e = 

	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.

	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: 2007.02.17.16:15
		    end: 2007.02.18.04:49

	ONUMs = 23157 (58 exps)   
		23158 (102 exps)
		23159 (203 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	172.09, 173.27, 174.38 Degrees (17322, 17537, 17739)

		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    50 um, 75 um (2.4 Ro)

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q07.02.17.16:15:19.ovi.dat
q07.02.17.18:16:58.ovi.dat
q07.02.17.21:49:47.ovi.dat