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

	Date:		01 October 2007
	-----

 	Last revision:	09 October 2007 (MU)
	--------------

	File Name: 	2007.10.04.a.log
	----------

	Compiled by:   	M. Uzzo, R. Wu
	------------

	UVCS Activity:  North Coronal Hole LYA Observation for 
	--------------	04 October 2007
			North Coronal Hole OVI Observation for 
			04 - 05 October 2007

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

	EOF Staff:      S. Cranmer: Lead Scientist
	---------- 	M. Uzzo: Planner
			Y.-K. Ko: Commander

	Command file:	07.10.01.13:05:36.cmd.log
                        07.10.02.15:18:12.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole LYA Observations

	Sequence: 06.08_hole.tcl, n = 2, m = 2, p = 0, r = 0, e = 3

	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=0 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: 2007.10.04.13:53
		    end: 2007.10.04.20:53

	ONUMs = 23731 (203 exps)   
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	354.381 Degrees (17739)

		- Mirror/Occulter:  2.4 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    75 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q07.10.04.13:53:32.ovi.dat

	2) North Polar 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=0 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: 2007.10.04.20:54
		    end: 2007.10.05.19:55

	ONUMs = 23732 (319 exps)   
		23733 (348 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	354.381 Degrees (17739)

		- 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:

q07.10.04.20:54:51.ovi.dat
GAP between 10/05/07|05:41:02( 3608) and 10/05/07|05:44:00( 3890)
q07.10.05.07:56:11.ovi.dat