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

	Date:		27 September 2006
	-----

 	Last revision:	02 November 2006 (Ko)
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	File Name: 	2006.09.27.a.log
	----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	Load and Start OVI Detector Diagnostic for 
	--------------	27 September 2006
			Load North Polar Coronal Hole OVI Observation for
			27 - 28 September 2006
			Load North Polar Coronal Hole OVI Observation for
			28 - 29 September 2006
			Load North Polar Coronal Hole OVI Observation for
			29 - 30 September 2006
			Load North Polar Coronal Hole LyA Observation for
			30 September 2006
			OVI Detector Diagnostic for 30 September 2006
			Load North Polar Coronal Hole OVI Observation for
			30 September - 01 October 2006
			Load North Polar Coronal Hole OVI Observation for
			01 - 02 October 2006
			Load North Polar Coronal Hole OVI Observation for
			02 - 03 October 2006

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

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

	Command file:	06.09.27.15:08:00.cmd.log

	Activity:
	---------

	1) OVI Detector Diagnostic

	Sequence: 06.02_OVI_164_chk.tcl

	SCI_SPEC: Instrument Diagnostics

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2006.09.27.18:58
                    end: 2006.09.27.19:59

	ONUMs =	22743 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 0 Degrees

		- Roll: 0 degrees (18762)

		- Mirror/Occulter:  1.75 Ro
                                    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask: LYA_chk_1xfull in slot 6

	Fits Files:

q06.09.27.18:56:27.ovi.dat

	2) North Coronal Hole Observations

	Sequence: 06.08_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: 2006.09.27.20:02
		    end: 2006.09.28.19:03

	ONUMs = 22744 (320 exps)   
		22745 (347 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	354.38 Degrees (17739)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

		- LYA Slit:    75 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:

q06.09.27.20:02:03.ovi.dat
q06.09.28.07:03:23.ovi.dat