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

	Date:		22 September 2008
	-----

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

	File Name: 	2008.09.26.a.log
	----------

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

	UVCS Activity:  Load and Start OVI Detector Diagnostic for 
	--------------	26 September 2008
			Load Coordinated Prominence Observation with Hinode 
			and SUMER for 26 - 27 September 2008 
			Load Coordinated Prominence Observation with 
			Hinode and SUMER for 27 September 2008 
			Load Coordinated Prominence Observation with Hinode
			and SUMER for 27 - 28 September 2008 
			Load Coordinated Prominence Observation with Hinode
			and SUMER for 28 September 2008
			Load OVI Detector Diagnostic for 28 September 2008
			Load Coordinated Prominence Observation with Hinode
			and SUMER for 28 - 29 September 2008 
			Load Coordinated Prominence Observation with Hinode
			and SUMER for 29 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) 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: 2008.09.26.16:16
                    end: 2008.09.26.17:16

	ONUMs =	24760 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 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:

q08.09.26.16:08:05.ovi.dat

	2) 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 @ 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: 2008.09.26.17:39
		    end: 2008.09.27.15:42

	ONUMs = 24761 (240 exps)
		24762 (239 exps)
		24763 (160 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: 232100

		- OVI MCP Voltage: 200

		- OVI mask:   OVI_303_8x2 in slot 3

	Fits Files:

q08.09.26.17:39:03.ovi.dat
q08.09.27.01:55:03.ovi.dat

GAP between 09/27/08|03:46:34( 8778) and 09/27/08|03:48:21( 8951)

q08.09.27.10:11:03.ovi.dat

	3) 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: 2008.09.27.15:43
		    end: 2008.09.27.16:41

	ONUMs = 24764 (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:

q08.09.27.15:43:25.ovi.dat