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

	Date:		28 September 2007
	-----

 	Last revision:	01 October 2007 (Wu)
	--------------

	File Name: 	2007.09.30.a.log
	----------

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

	UVCS Activity:  North Polar Coronal Hole OVI Observationfor 
	--------------	30 September 2007
			North Polar Coronal Hole OVI Observation for 
			30 September - October 01 2007
			OVI Detector Diagnostic for 01 October 2007

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

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

	Command file:	07.09.29.13:30:00.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole OVI Observations

	Sequence: 06.08_hole.tcl, n = 8, m = 0, p = 0, r = 0, 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: 2007.09.30.00:15
		    end: 2007.09.30.22:18

	ONUMs = 23714 (319 exps)   
		23715 (320 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	353.267 Degrees (17536)

		- 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:

q07.09.30.00:15:03.ovi.dat
q07.09.30.11:16:23.ovi.dat

	2) North Polar Coronal Hole OVI Observations

	Sequence: 06.08_hole.tcl, n = 3, m = 2, 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=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: 2007.09.30.22:19
		    end: 2007.10.01.08:23

	ONUMs = 23716 (292 exps)   
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	353.267 Degrees (17536)

		- 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:

q07.09.30.22:19:24.ovi.dat

	3) OVI Detector Diagnostic

	Sequence: OVI_164_chk.tcl

	SCI_SPEC: 

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2007.10.01.08:25
                    end: 2007.10.01.09:26

	ONUMs =	23717 (12 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll:  0 Degrees (18762)

		- Mirror/Occulter:  1.75 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_chk_1xfull in slot 6

	Fits Files:

q07.10.01.08:22:52.ovi.dat