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

	Date:		07 November 2008
	-----

 	Last revision:	26 November 2008 (Wu)
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	File Name:	2008.11.24.a.log
	----------

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

	UVCS Activity:	Flush and Abort OVI Detector Dark Rate Diagnostic for 
	--------------	24 November 2008
			Load and Start Flat Field Calibration using Star Delta  
			Scorpionis for 24 - 25 November 2008
			Load South Polar Coronal Hole OVI Observation for
			25 November 2008
	
	SOHO Activity:	
	--------------

	EOF Staff:	L. Gardner: Lead Scientist
	----------	M. Uzzo: Commander, Planner
			R. Wu

	Command file:	08.11.24.09:08:17.cmd.log

	Activity:
	---------

	1) Flat Field Calibration Using Delta Scorpionis 

	Sequence: Manual, Star_Can.tcl (120 sec.)

	SCI_SPEC: Spatial Flat Field Calibration. 

	OBS_PROG: Primary: Calibration
         	  Sub Obj: Spatial Coverage

	SCI_OBJ:  Primary: Calibration...Radiometric Calibration
		  Sub Obj: Celetial Targets...Star (Delta Sco)

	OBJ:      Star

	CMP_NAME: 

	CMP_NUM:  

        Duration: start: 2008.11.24.10:44
		    end: 2008.11.25.06:01

        ONUMs = 24926 (240 exps)
		24927 (240 exps)
		24928 (80 exps)
		
        Instrument configuration:

                - Pointing:  Sun center
				
                - Spacecraft Roll: 180 Degrees

                - Roll: 172.96 Degrees (50268)

		- Mirror/Occulter: 7.24 Ro (36300)
                                    1.5 mm overocculting

                - LYA Slits:  100 um
                - OVI Slits:  200 um

                - LYA GRTPOS: 100000
                - OVI GRTPOS:  59800

		- OVI mask:   StarFF_4x4 in slot 5

        Fits Files:

q08.11.24.10:43:49.ovi.dat
q08.11.24.18:59:49.ovi.dat
q08.11.25.03:15:49.ovi.dat

	2) South Polar Coronal Hole Observations

	Sequence: 08.11_hole.tcl, n = 6, m = 2, 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=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: 2008.11.25.06:04
		    end: 2008.11.25.23:58

	ONUMs = 24930 (320 exps)   
		24931 (200 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll: 172.09 Degrees (17322)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 223500

		- OVI MCP Voltage: 205 (Nominal + 5) 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q08.11.25.06:04:16.ovi.dat
q08.11.25.17:05:36.ovi.dat