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

	Date:		20 June 2006
	-----

 	Last revision:	11 July 2006 (Wu)
	--------------

	File Name: 	2006.06.26.a.log
	----------

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

	UVCS Activity:  North Polar Coronal Hole OVI Observation for
	--------------	26 June 2006
  			North Polar Coronal Hole OVI Observation for
			26 - 27 June 2006

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

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

	Command file:	06.06.23.12:26:16.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=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: 2006.06.26.00:37
		    end: 2006.06.26.23:37

	ONUMs = 22553 (320 exps)   
		22554 (348 exps)   

	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:

q06.06.26.00:36:46.ovi.dat
q06.06.26.11:38:06.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=0 degrees.

		  Note: Missing data recoverable from level 0 product.

	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: 2006.06.26.23:39
		    end: 2006.06.27.22:39

	ONUMs = 22555 (320 exps)   
		22556 (341 exps)   

	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:

q06.06.26.23:38:59.ovi.dat
q06.06.27.10:40:19.ovi.dat

GAP between 06/27/06|17:43:03(15552) and 06/27/06|17:44:33(15695)
GAP between 06/27/06|17:46:31(15882) and 06/27/06|17:49:29(16166)
GAP between 06/27/06|17:53:27(  164) and 06/27/06|17:54:50(  302)
GAP between 06/27/06|21:18:36( 3490) and 06/27/06|21:20:49( 3702)
GAP between 06/27/06|21:40:24( 5588) and 06/27/06|21:45:18( 6054)