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

	Date:		01 October 2008
	-----

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

	File Name: 	2008.10.01.a.log
	----------

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

	UVCS Activity:  Load and Start OVI Detector Diagnostic for 
	--------------	01 October 2008
			Load Coordinated Prominence Observation with Hinode 
			and SUMER for 01 October 2008
			Load Coordinated Prominence Observation with Hinode 
			and SUMER for 01 - 02 October 2008 
			Load Coordinated Prominence Observation with Hinode 
			and SUMER for 02 October 2008
			Load OVI Detector Diagnostic for 02 October 2008

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

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

	Command file:	08.10.01.14:39:00.cmd.log

	Activity:
	---------

	1) OVI Detector Diagnostic

	Sequence: OVI_164_chk.tcl

	SCI_SPEC: Instrument Diagnostics

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  Calibration

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2008.10.01.20:59
                    end: 2008.10.01.22:00

	ONUMs =	24782 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll: 0 Degrees (18762)

		- 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:

q08.10.01.20:49:07.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 @ 40 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: 2008.10.01.22:08
		    end: 2008.10.01.23:06

	ONUMs = 24783 (28 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	61 Degrees (29877)

		- 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:

q08.10.01.22:07:46.ovi.dat

	3) Prominence Observations

	Sequence: 08.09_Prom.tcl, n = 5, 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 @ 40 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: 2008.10.01.23:08
		    end: 2008.10.02.12:54

	ONUMs = 24784 (240 exps)
		24785 (160 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	61 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:

q08.10.01.23:07:38.ovi.dat
q08.10.02.07:23:38.ovi.dat

	4) 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 @ 40 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: 2008.10.02.12:56
		    end: 2008.10.02.13:54

	ONUMs = 24786 (28 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	61 Degrees (29877)

		- 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:

q08.10.02.12:56:18.ovi.dat