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

	Date:		13 December 2007
	-----

 	Last revision:	26 December 2007 (Wu)
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	File Name:	2007.12.23.a.log
 	----------

	Compiled by:	M. Uzzo, R. Wu, Y.-K. Ko
	------------

	UVCS Activity:	Ulysses-SOHO Quadrature Observations for 
	--------------	23 - 24 December 2007

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

	EOF Staff:      G. Poletto / A. Bemporad: Lead Scientist
	----------	Y.-K. Ko: Commander
			M. Uzzo: Planner
			R. Wu

	Command file:	07.12.21.14:31:55.cmd.log

	Activity:
	---------

	1) Ulysses-SOHO Quadrature Observations

	Sequence: 07.12_Poletto.tcl, n = 14, r = 1

	SCI_SPEC: The goal of these observations will be to study the 
                  power spectrum of the OVI intensity fluctuations at 
		  very low frequencies. In particular we are interested 
		  in latitude dependences and in the comparison of OVI
		  spectra with Lyman-alpha spectra we get from previous
                  observations. Moreover SOHO/UVCS remote sensing spectra 
		  will be compared with Ulysses/SWOOPS spectra detected 
 		  in situ, in order to study possible radial dependences
		  during the propagation of the solar wind.

	OBS_PROG: Primary: Temporal Coverage
		  Sub Obj: Spatial Resolution

	SCI_OBJ:  Primary: Coronal Structure...Fine Structure
           	  Sub Obj: Coronal Dynamics...Turbulance Plasmoids
                
	OBJ:      Coronal Hole

	CMP_NAME: Ulysses-SOHO Quadrature Observations

	CMP_NUM:  7261

        Duration: start: 2007.12.23.21:47
		    end: 2007.12.24.14:41

	ONUMs =	23915 (284 exps) 

        Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  180 Degrees

		- Roll: 27 Degrees (56466)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   200 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Plume_217 in slot 1

	Fits Files:

q07.12.23.21:47:26.ovi.dat