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

	Date:		07 November 2008
	-----

 	Last revision:	01 December 2008 (Wu)
	--------------

	File Name:	2008.11.25.a.log
	----------

	Compiled by:	M. Uzzo
	------------

	UVCS Activity:	Load and Run Radiometric Calibration using Star
	--------------	Delta Scorpionis for 25 - 26 November 2008
			Load South Polar Coronal Hole LYA Observation for
			26 November 2008
			Load South Polar Coronal Hole LYA Observation for
			26 November 2008
	SOHO Activity:	
	--------------

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

	Command file:	08.11.25.17:25:09.cmd.log

	Activity:
	---------
	
	1) Spectral Studies Using Delta Scorpionis 

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

	SCI_SPEC: Star Observations
                 
	OBS_PROG: Primary: Calibration
		  Sub Obj: Spectral Coverage

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

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2008.11.26.02:32
		    end: 2008.11.26.04:39

	ONUMs = 24933 (48 exps) 

	Instrument configuration:

                - Pointing:  Sun center

		- Spacecraft Roll:  180 Degrees

		- Roll:  -  Degrees ( - )

		- Mirror/Occulter:  -  Ro
				   Occulter widths:  
				  

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 235000, 180500

		- OVI mask:   OVI_303_8x2 in slot 3

        Fits Files:

q08.11.26.00:38:44.ovi.dat

	2) South Polar Coronal Hole Observations

	Sequence: 08.11_hole.tcl, n = 1, m = 1, 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: 2008.11.26.0
		    end: 2008.11.26.0

	ONUMs = 24935 ( 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: 164600

		- OVI MCP Voltage: 205 (Nominal + 5) 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q08.11.26.04:44:25.ovi.dat

	3) South Polar Coronal Hole Observations

	Sequence: 08.11_hole.tcl, n = 1, m = 2, p = 1, 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: 2008.11.26.08:12
		    end: 2008.11.26.12:41

	ONUMs = 24936 (130 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: 164600

		- OVI MCP Voltage: 205 (Nominal + 5) 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q08.11.26.08:12:52.ovi.dat