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

	Date:		29 March 2007
	-----

 	Last revision:	04 April 2007 (Wu)
	--------------

	File Name:	2007.04.02.a.log
	----------

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

	UVCS Activity:	South Coronal Hole OVI Observations for 02 April 2007
	--------------	South Coronal Hole OVI Observations for 
			02 - 03 April 2007

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

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

	Command file:	07.03.29.15:46:00.cmd.log
                        
	Activity:
	---------

	1) South Coronal Hole OVI Observations

	Sequence: 06.08_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=180 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      

	CMP_NAME: 

	CMP_NUM:  7201

	Duration: start: 2007.04.02.00:41
		    end: 2007.04.02.23:42

	ONUMs = 23217 (320 exps)   
		23218 (347 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	174.38 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:

q07.04.02.00:41:28.ovi.dat
q07.04.02.11:42:48.ovi.dat

GAP between 04/02/07|20:33:01(13909) and 04/02/07|20:34:35(14063)

	2) South Coronal Hole OVI Observations

	Sequence: 06.08_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=180 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      

	CMP_NAME: 

	CMP_NUM:  7201

	Duration: start: 2007.04.02.23:44
		    end: 2007.04.03.22:44

	ONUMs = 23219 (320 exps)   
		23220 (348 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	174.38 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:

q07.04.02.23:43:41.ovi.dat
q07.04.03.10:45:01.ovi.dat

GAP between 04/03/07|13:17:55(12148) and 04/03/07|13:20:25(12384)