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

	Date:		21 July 2006
	-----

 	Last revision:	31 July 2006 (Wu)
	--------------

	File Name:	2006.07.28.a.log
	----------

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

	UVCS Activity:	North Polar Coronal Hole LYA Observation for
	--------------	28 July 2006
			North Polar Coronal Hole OVI Observation for
			28 - 29 July 2006

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

	EOF Staff:	M. P. Miralles: Lead Scientist
	---------	M. Uzzo: Commander, Planner
 			Y.-K. Ko
			R. Wu
		
	Command file:	06.07.25.18:25:20.cmd.log

	Activity:
	---------

	1) North Coronal Hole Observations

	Sequence: 06.06_hole.tcl

	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: 2006.07.28.15:17
		    end: 2006.07.28.18:48

	ONUMs = 22642 (102 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	174.38 Degrees (17739)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 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:

q06.07.28.15:16:46.ovi.dat

	2) North Coronal Hole Observations

	Sequence: 06.06_hole.tcl

	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: 2006.07.28.18:49
		    end: 2006.07.29.17:50

	ONUMs = 22643 (320 exps)   
		22644 (348 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	174.38 Degrees (17739)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 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:

q06.07.28.18:49:21.ovi.dat
q06.07.29.05:50:41.ovi.dat