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

	Date:		21 March 2007
	-----

 	Last revision:	26 March 2007 (Wu)
	--------------

	File Name:	2007.03.23.a.log
	----------

	Compiled by:	Y.-K. Ko
	------------

	UVCS Activity:	South Coronal Hole LyA Observations for
	--------------	23 - 24 March 2007
			South Coronal Hole OVI Observations for 
			24 March 2007
			Load South Coronal Hole OVI Observations for 
			24 - 25 March 2007
			Load South Coronal Hole OVI Observations for 
			25 - 26 March 2007
                        Load and Start OVI Detector Diagnostic for
                        26 March 2007
                        Load South Coronal Hole LyA Observations for
                        26 - 27 March 2007
                        Load South Coronal Hole OVI Observations for
                        27 - 28 March 2007

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

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

	Command file:	07.03.21.13:21:39.cmd.log

	Activity:
	---------

	1) South Coronal Hole LyA Observations

	Sequence: 06.08_hole.tcl, n = 1, m = 1, p = 0, r = 0, e = 2

	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: 2007.03.23.20:39
		    end: 2007.03.24.00:10

	ONUMs = 23195 (102 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	173.27 Degrees (50326)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 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:

q07.03.23.20:39:16.ovi.dat

	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:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2007.03.24.00:12
		    end: 2007.03.24.23:12

	ONUMs = 23196 (320 exps)   
		23197 (348 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	173.27 Degrees (50326)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 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:

q07.03.24.00:11:51.ovi.dat
q07.03.24.11:13:11.ovi.dat