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

	Date:		16 July 2007
	-----

 	Last revision:	17 July 2007 (Wu)
	--------------

	File Name: 	2007.07.16.a.log
	----------

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

	UVCS Activity:	South Coronal Hole OVI Observation for 
	--------------	16 July 2007
			Load and Start South Polar Coronal Hole OVI Observation 
			for 17 July 2007
			Load OVI Detector Diagnostic for July 17 2007
			Load Equatorial Coronal Hole LyA Observations for
			17 July 2007
			Load Equatorial Coronal Hole LyA Observations for
			17 July 2007
			Load Equatorial Coronal Hole LyA Observations for
			17 July 2007
			Load Equatorial Coronal Hole OVI Observations for
			17 July 2007
			Load Equatorial Coronal Hole OVI Observations for
			17 July 2007
			Load Equatorial Coronal Hole OVI Observations for
			17 - 18 July 2007
			Load South Polar Coronal Hole OVI Observation for
                        18 July 2007

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

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

	Command file:	07.07.12.11:35:19.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:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2007.07.16.00:55
		    end: 2007.07.16.23:56

	ONUMs = 23493 (320 exps)   
		23494 (348 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	173.27 Degrees (17537)

		- 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:

q07.07.16.00:55:24.ovi.dat
q07.07.16.11:56:44.ovi.dat

	2) South Polar Coronal Hole OVI Observations

	Sequence: 06.08_hole.tcl, n = 1, m = 1, p = 1, 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: 2007.07.16.23:58
		    end: 2007.07.17.03:49

	ONUMs = 23495 (112 exps)   

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	173.27 Degrees (17537)

		- 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:

q07.07.16.23:57:37.ovi.dat