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

	Date:		13 December 2007
	-----

 	Last revision:	20 December 2007 (Wu)
	--------------

	File Name:	2007.12.17.a.log
 	----------

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

	UVCS Activity:	Flush and Abort Solar Minimum Watching with Italian 
	--------------	SINERGIES Observations for 16 - 17 December 2007
			Ramp Down and Turn off LYA Detector HV
			Power off LYA Detector
			Turn on OVI Detector
			Conduct OVI Stimulus Pulse Test
			Load Mask OVI_FF_RED_4x1 in OVI slot 5
			Turn on and Ramp Up OVI Detector HV 
			Load and Start OVI Detector Diagnostic for 
			17 December 2007
			Load Ulysses-SOHO Quadrature Observations for 
			17 - 18 December 2007
			Load Ulysses-SOHO Quadrature Observations for 
			18 - 19 December 2007
			Load Ulysses-SOHO Quadrature Observations for 
			19 - 20 December 2007
			Load OVI Detector Diagnostic for 20 December 2007
			Load Ulysses-SOHO Quadrature Observations for 
			20 - 21 December 2007
			Load Ulysses-SOHO Quadrature Observations for 
			21 - 22 December 2007

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

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

	Command file:	07.12.17.14:34:49.cmd.log

	Activity:
	---------

	1) OVI Stimulus Pulse Test

	Sequence: TakeUV_TxN.tcl

	SCI_SPEC: 

	OBS_PROG: 

	SCI_OBJ:  

	OBJ:

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2007.12.17.18:41
		    end: 2007.12.17.18:45

	ONUMs = 23906 (2 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:  103.6 Degrees (4854)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

                - LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- LYA MCP Voltage: 0 
		- OVI MCP Voltage: 0 

		- OVI mask:   OVI_303_8x2 in slot 3

	Fits Files:

q07.12.17.18:37:35.ovi.dat

	2) 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: 2007.12.17.19:32
                    end: 2007.12.17.20:33

	ONUMs =	23907 (12 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll:  180 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:

q07.12.17.19:22:04.ovi.dat

	3) 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: 2007.12.17.20:37
		    end: 2007.12.18.20:36

	ONUMs =	23908 (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:

q07.12.17.20:37:27.ovi.dat

GAP between 12/18/07|10:05:57(10436) and 12/18/07|10:06:59(10533)