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

	Date:		22 September 2008
	-----

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

	File Name: 	2008.09.24.a.log
	----------

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

	UVCS Activity:  Flush and Abort Coordinated Prominence Observation with 
	--------------	Hinode and SUMER for 24 - 25 September 2008 
			Reload and Start Coordinated Prominence Observation 
			with Hinode and SUMER for 24 - 25 September 2008

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

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

	Command file:	08.09.23.12:48:31.cmd.log
			08.09.24.15:26:31.cmd.log

	Activity:
	---------

	1) Prominence Observations

	Sequence: 08.09_Prom.tcl, n = 8, m = 3, 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: 2008.09.24.14:39
		    end: 2008.09.25.20:17

	ONUMs = 24750 (164 exps) ; aborted
		24751 (0 exps) ; flushed
		24752 (0 exps) ; flushed

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	336 Degrees (14393) 

		- 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:

q08.09.24.14:38:36.ovi.dat

	2) Prominence Observations

	Sequence: 08.09_Prom.tcl, n = 7, 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 @ 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: 2008.09.24.20:47
		    end: 2008.09.25.16:04

	ONUMs = 24752 (240 exps) 
		24753 (240 exps) 
		24754 (80 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	246 Degrees (63566) 

		- 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:

q08.09.24.20:47:00.ovi.dat
q08.09.25.05:03:00.ovi.dat
q08.09.25.13:19:00.ovi.dat