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

	Date:		11 July 2008
	-----

 	Last revision:	15 July 2008 (Wu)
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	File Name: 	2008.07.13.a.log
	----------

	Compiled by:	M. Uzzo
	------------

	UVCS Activity:  North Polar Coronal Hole LYA Observation for 
	--------------	13 July 2008
			North Polar Coronal Hole OVI Observation for 
			13 - 14 July 2008

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

	EOF Staff:	M. P. Miralles: Lead Scientist
	----------	M. Uzzo: Commander, Planner
			R. Wu

	Command file:	08.07.11.15:10:30.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole Observations

	Sequence: 08.01_hole.tcl, n = 1, m = 1, p = 0, r = 2, 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: 2008.07.13.18:32
		    end: 2008.07.13.22:32

	ONUMs = 24597 (116 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	353.27 Degrees (50326)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q08.07.13.18:32:21.ovi.dat

	2) North Polar Coronal Hole Observations

	Sequence: 08.01_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: 2008.07.13.22:34
		    end: 2008.07.14.21:34

	ONUMs = 24598 (320 exps)   
		24599 (347 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	353.27 Degrees (50326)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.07.13.22:33:52.ovi.dat
q08.07.14.09:35:12.ovi.dat