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

	Date:		07 April 2006
	-----

 	Last revision:	14 April 2006 (Wu)
	--------------

	File Name:	2006.04.09.a.log
	----------

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

	UVCS Activity:	South Coronal Hole Observations in LyA for 
	--------------	09 April 2006
			South Coronal Hole Observations in OVI for
			09 - 10 April 2006

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

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

	Command file:	06.04.07.20:37:59.cmd.log

	Activity:
	---------

	1) South Coronal Hole Observations

	Sequence: 06.04_holeLyA24.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=180 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      Coronal Hole

	CMP_NAME: South Coronal Hole Study, UVCS; LASCO

	CMP_NUM:  7180

	Duration: start: 2006.04.09.18:34
		    end: 2006.04.09.22:01

	ONUMs = 22374 (100 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 Slits:  100 um
		- OVI Slits:   75 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q06.04.09.18:31:02.ovi.dat

	2) South Coronal Hole Observations

	Sequence: 06.04_holeOVI24.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=180 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      Coronal Hole

	CMP_NAME: South Coronal Hole Study, UVCS; LASCO

	CMP_NUM:  7180

	Duration: start: 2006.04.09.22:02
		    end: 2006.04.10.21:03

	ONUMs = 22375 (333 exps) 
		22376 (334 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 Slits:  100 um
		- OVI Slits:   75 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q06.04.09.22:02:03.ovi.dat

GAP between 04/10/06|03:19:29( 4025) and 04/10/06|03:20:59( 4166)

q06.04.10.09:32:19.ovi.dat