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

	Date:		22 September 2008
	-----

 	Last revision:	06 October 2008 (Wu)
	--------------

	File Name: 	2008.09.27.a.log
	----------

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

	UVCS Activity:  Prominence Coordinated Observation with Hinode and 
	--------------	SUMER for 27 - 28 September 2008 
			Prominence Coordinated Observation with Hinode and 
			SUMER for 28 September 2008 

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

	EOF Staff:	J. Raymond: Lead Scientist
	----------	M. Uzzo: Commander, Planner
			R. Wu

	Command file:	08.09.26.12:56:07.cmd.log

	Activity:
	---------

	1) Prominence Observations

	Sequence: 08.09_HeII.tcl, n = 8, m = 0, r = 0, e = 0

        SCI_SPEC: We wish to observe the plasma above a prominence in
		  conjunction with SUMER observations (JOP207, S. Parenti).  
  		  The Lyman lines and He II 1085 A are the primary lines of
		  interest, but O VI will also be needed for density estimates.

		  HiRes Centered @ 315 Degrees

        OBS_PROG: Primary: Spectral Coverage
                  Sub Obj: Temporal Resolution

        SCI_OBJ:  Primary: Abundances
                  Sub Obj: Density

        OBJ:      Prominence

	CMP_NAME: JOP 207 / HOP 082, Quiescent and Eruptive Prominences, 
        	  SUMER; UVCS; Hinode-EIS (S/C)

        CMP_NUM:  7287

	Duration: start: 2008.09.27.16:43
		    end: 2008.09.28.14:46

	ONUMs = 24765 (240 exps)
		24766 (240 exps)
		24767 (159 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	321 Degrees (11662)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS:  74000

		- OVI MCP Voltage: 200

		- OVI mask:   OVI_303_8x2 in slot 3

	Fits Files:

q08.09.27.16:43:32.ovi.dat
q08.09.28.00:59:32.ovi.dat
q08.09.28.09:15:32.ovi.dat

	2) Prominence Observations

	Sequence: 08.09_Prom_LYA.tcl

        SCI_SPEC: We wish to observe the plasma above a prominence in
		  conjunction with SUMER observations (JOP207, S. Parenti).  
  		  The Lyman lines and He II 1085 A are the primary lines of
		  interest, but O VI will also be needed for density estimates.

		  HiRes Centered @ 225 Degrees

        OBS_PROG: Primary: Spectral Coverage
                  Sub Obj: Temporal Resolution

        SCI_OBJ:  Primary: Abundances
                  Sub Obj: Density

        OBJ:      Prominence

	CMP_NAME: JOP 207 / HOP 082, Quiescent and Eruptive Prominences, 
        	  SUMER; UVCS; Hinode-EIS (S/C)

        CMP_NUM:  7287

	Duration: start: 2008.09.27.14:48
		    end: 2008.09.27.15:46

	ONUMs = 24768 (28 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	321 Degrees (11662)

		- 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: 200

		- OVI mask:   OVI_Str_Prof in slot 5

	Fits Files:

q08.09.28.14:48:27.ovi.dat