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

	Date:		16 July 2008
	-----

 	Last revision:	22 July 2008 (Wu)
	--------------

	File Name: 	2008.07.17.a.log
	----------

	Compiled by:	M. Uzzo, R. Wu
	------------

	UVCS Activity:  North Polar Coronal Hole OVI Observation for 
	--------------	17 - 18 July 2008
			Flush and Abort North Polar Coronal Hole OVI 
			Observation for 17 - 18 July 2008
			Load and Start North Polar Coronal Hole OVI Observation 
			for 17 - 18 July 2008
			Load OVI Detector Diagnostic for 18 July 2008
			Load North Polar Coronal Hole OVI Observation for 
			18 - 19 July 2008
			Load North Polar Coronal Hole OVI Observation for 
			19 - 20 July 2008
			Load North Polar Coronal Hole OVI Observation for 
			20 - 21 July 2008
			Load North Polar Coronal Hole OVI Observation for 
			21 - 22 July 2008
			Load OVI Detector Diagnostic for 22 July 2008

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

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

	Command file:	08.07.16.15:40:01.cmd.log
			08.07.17.13:23:31.cmd.log

	Activity:
	---------

	1) 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: 2008.07.17.03:47
		    end: 2008.07.17.13:38

	ONUMs = 24607 (286 exps) ; aborted

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	354.38 Degrees (50528)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    75 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.07.17.03:46:55.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: 2008.07.17.13:44
		    end: 2008.07.18.12:44

	ONUMs = 24609 (320 exps)   
		24610 (348 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:

q08.07.17.13:44:00.ovi.dat
q08.07.18.00:45:20.ovi.dat