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

	Date:		31 July 2008
	-----

 	Last revision:	05 August 2008 (Wu)
	--------------

	File Name: 	2008.07.31.a.log
	----------

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

	UVCS Activity:	Load and Start OVI Detector Diagnostic for 31 July 2008
	--------------	Load North Polar Coronal Hole OVI Observation for 
			31 July - 01 August 2008
			Load North Polar Coronal Hole OVI Observation for 
			01 - 02 August 2008
			Load North Polar Coronal Hole OVI Observation for 
			02 - 03 August 2008
			Load North Polar Coronal Hole OVI Observation for 
			03 - 04 August 2008
			Load OVI Detector Diagnostic for 04 August 2008
			Load North Polar Coronal Hole OVI Observation for 
			04 - 05 August 2008

	SOHO Activity:	Received via email Friday, 01 August 2008,  
	--------------	01:59:58 GMT: OBT DISTRIBUTED TO UVCS BY FOT

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

	Command file:	08.07.31.14:39:00.cmd.log

	Activity:
	---------

	1) OVI Detector Diagnostic

	Sequence: OVI_164_chk.tcl

	SCI_SPEC: Instrument Diagnostics

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  Calibration

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2008.07.31.15:34
                    end: 2008.07.31.16:35

	ONUMs =	24642 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  180 Degrees

		- Roll: 0 Degrees (51551)

		- Mirror/Occulter:  1.75 Ro
                                    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_chk_1xfull in slot 6

	Fits Files:

q08.07.31.15:32:22.ovi.dat

	2) North Polar Coronal Hole Observations

	Sequence: 08.01_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: 2008.07.31.16:39
		    end: 2008.08.01.15:39

	ONUMs = 24643 (320 exps)   
		24644 (346 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	353.27 Degrees (50326)

		- Mirror/Occulter:  2.0 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.07.31.16:38:35.ovi.dat
q08.08.01.03:39:55.ovi.dat