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

	Date:		06 October 2008
	-----

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

	File Name: 	2008.10.04.a.log
	----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:  Coordinated Prominence Observation with Hinode 
	--------------	and SUMER for 04 - 05 October 2008
			Coordinated Prominence Observation with Hinode 
			and SUMER for 05 October 2008 

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

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

	Command file:	08.10.03.14:59:30.cmd.log

	Activity:
	---------

	1) Prominence Observations

	Sequence: 08.09_Prom.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 @ 42 Degrees

        OBS_PROG: Primary: Spectral Coverage
                  Sub Obj: Temporal Resolution

        SCI_OBJ:  Primary: Abundances
                  Sub Obj: Density

	OBJ:      Prominence

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

        CMP_NUM:  7287

	Duration: start: 2008.10.04.15:54
		    end: 2008.10.05.13:57

	ONUMs = 24797 (240 exps)
		24798 (240 exps)
		24799 (180 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	63 Degrees (29877)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 232100

		- OVI MCP Voltage: 200

		- OVI mask:   OVI_303_8x2 in slot 3

	Fits Files:

q08.10.04.15:54:08.ovi.dat
q08.10.05.00:10:08.ovi.dat
q08.10.05.08:26:08.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 @ 42 Degrees

        OBS_PROG: Primary: Spectral Coverage
                  Sub Obj: Temporal Resolution

        SCI_OBJ:  Primary: Abundances
                  Sub Obj: Density

	OBJ:      Prominence

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

        CMP_NUM:  7287

	Duration: start: 2008.10.05.13:59
		    end: 2008.10.05.14:57

	ONUMs = 24800 (28 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	63 Degrees (33518)

		- 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:

q08.10.05.13:58:47.ovi.dat