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

	Date:		28 May 2009
	-----

 	Last revision:	04 June 2009 (Wu)
	--------------

	File Name: 	2009.06.01.a.log
	----------

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

	UVCS Activity:  Load and Start North Coronal Hole and Calibration Study
	--------------	(LyA Redundant) for 01 June 2009
			Increase OVI HV to 215
			Load and Start North Coronal Hole and Calibration Study
			(OVI Doublet) @ HV=215 for 01 - 02 June 2009
			Load North Coronal Hole and Calibration Study (LyA 
			Redundant) @ HV=215 for 02 June 2009

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

	EOF Staff:	M. Miralles & L. Gardner: Lead Scientist
	----------	R. Wu: Commander
			M. Uzzo: Planner

	Command file:	09.06.01.11:47:09.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole and Calibration Study

	Sequence: 09.01_hole.tcl, n = 0, m = 2, p = 1, 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.

		  Calibrations: Compare coronal hole intensity and 
		  line width at OVI HV 205 and 215.

		  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: 2009.06.01.12:14
		    end: 2009.06.01.14:13

	ONUMs = 25488 (60 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 352.09 Degrees (50111)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 205  

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q09.06.01.12:13:35.ovi.dat

	2) North Polar Coronal Hole and Calibration Study

	Sequence: 09.01_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.

		  Calibrations: Compare coronal hole intensity and 
		  line width at OVI HV 205 and 215.

		  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: 2009.06.01.14:22
		    end: 2009.06.01.13:23

	ONUMs = 25489 (320 exps)   
		25490 (347 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 352.09 Degrees (50111)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 235900

		- OVI MCP Voltage: 215 (Nominal + 10)

		- OVI mask:   OVI_Hole_237 in slot 2

	Fits Files:

q09.06.01.14:22:26.ovi.dat
q09.06.02.01:23:46.ovi.dat