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

	Date:		11 April 2008
	-----

 	Last revision:	18 April 2008 (Wu)
	--------------

	File Name: 	2008.04.15.a.log
	----------

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

	UVCS Activity:  JOP 206 / 203: Low-Latitude Coronal Holes and Hole 
	--------------	Boundary for 15 - 16 April 2008
			Load OVI Detector Diagnostic for 17 April 2008
			Load JOP 206 / 203: Low-Latitude Coronal Holes and 
			Hole Boundary for 17 - 18 April 2008
			Load JOP 206 / 203: Low-Latitude Coronal Holes and 
			Hole Boundary for 18 April 2008
			Flush Batch Queue
			Reload Remainder of JOP 206 / 203: Low-Latitude Coronal 
			Holes and Hole Boundary for 15 - 16 April 2008 into 
			Interactive Queue
			Reload JOP 206 / 203: Low-Latitude Coronal Holes and 
			Hole Boundary for 16 - 17 April 2008
			Reload OVI Detector Diagnostic for 17 April 2008
			Reload JOP 206 / 203: Low-Latitude Coronal Holes and 
			Hole Boundary for 17 - 18 April 2008
			Reload JOP 206 / 203: Low-Latitude Coronal Holes and 
			Hole Boundary for 18 April 2008

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

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

	Command file:	08.04.11.14:23:01.cmd.log
			08.04.15.13:07:00.cmd.log

	Activity:
	---------

	1) Low-Latitude Coronal Holes and Coronal Hole Boundary

	Sequence: 08.04_WHI_CH.tcl, 08.04_WHI_CH_Roll.tcl

	SCI_SPEC: To understand the origin of the solar wind from 
                  low-latitude coronal holes, including coronal hole 
                  boundaries by characterizing the physical properties 
                  of the coronal plasma (temperature, density, abundance,
                  outflow velocity) with coordinated multi-spacecraft and
                  ground-based observations in order to investigate the 
                  physical processes that lead to the origin of the solar 
                  wind. UVCS will position the slit to cover the coronal 
                  hole and boundary regions, at the limb, with three roll 
                  angles and run observations in H I Ly-alpha and 
                  OVI 1032/1037 at a height of 1.7 Ro.

                  NOTE: ONUM 24341 flushed, and remaining sqstrt commands 
                  reloaded.  The following (final) 4 ONUMS reloaded using 
                  script 08.04_WHI_CH_Roll.tcl.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      Coronal Hole

	CMP_NAME: JOP 206 / 203, Low-Latitude Coronal Holes

	CMP_NUM:  7270, 7267

	Duration: start: 2008.04.15.06:25
		    end: 2008.04.16.06:58

	ONUMs = 24340 (50 exps)   
                24341 (186 exps) ; flushed
		24342 (50 exps)   
                24343 (186 exps)
		24344 (50 exps)   
                24345 (186 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	263, 279, 295 Degrees (1104, 4016, 6929)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600, 217000

		- OVI MCP Voltage: 200 

		- OVI mask:     OVI_sp2_164	 in slot 4
				OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.04.15.06:24:57.ovi.dat
q08.04.15.08:09:11.ovi.dat
q08.04.15.14:38:10.ovi.dat
q08.04.15.16:22:24.ovi.dat
q08.04.15.22:49:42.ovi.dat
q08.04.16.00:33:56.ovi.dat