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

	Date:		24 March 2006
	-----

 	Last revision:	27 March 2006 (Wu)
	--------------

	File Name:	2006.03.24.a.log
	----------

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

	UVCS Activity:  Load OVI Detector Masks 
	--------------		OVI_Eclipse06_215 into OVI slot 1
				OVI_EclipSyn_215  into OVI slot 2
				OVI_sp2_164       into OVI slot 4
				OVI_JOP175new     into OVI slot 5	
			Load and Start OVI Detector Diagnostic for 
			March 24 2006
                        Load and Start JOP175 Extended Filaments at 
                        the Limb for
                        Observation for 24 - 25 March 2006
                       	Load JOP175 Extended Filaments at the Limb 
                       	Observation for 26 - 27 March 2006
			Load OVI Detector Diagnostic for March 27 2006
			Load JOP158 Coordinated with Natural Solar 
			Eclipse Observation for 27 - 28 March 2006

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

	EOF Staff:	L. Gardner / J. Raymond: Lead Scientist
	---------	M. Uzzo: Commander, Planner
			Y.-K. Ko: Planner
			R. Wu

	Command file:	06.03.24.13:59:21.cmd.log
	
	Activity:
	---------

	1) OVI Detector Diagnostic

	Sequence: 06.02_OVI_164_chk.tcl

	SCI_SPEC: Instrument Diagnostics

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2006.03.24.18:54
                    end: 2006.03.24.19:55

	ONUMs =	22315 (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:

q06.03.24.18:52:32.ovi.dat

	2) JOP175 Extended Filaments at the Limb

	Sequence: 06.03.24_JOP175.tcl

	SCI_SPEC: JOP 175 is designed to study prominences above the limb.
                  The UVCS observations will constrain the abundances and
                  other coronal parameters in the streamer above the 
                  prominence to look for correlations between prominence 
                  and streamer properties. 

                  Target Angle = 136 deg

	OBS_PROG: Spectral Coverage

	SCI_OBJ:  Abundances

	OBJ:      Prominence

	CMP_NAME: JOP175 Extended Filaments at the Limb, 
		  LASCO; EIT; UVCS; TRACE(S/C); Mauna Loa (GBO)

	CMP_NUM:  7135

	Duration: start: 2006.03.24.20:11
		    end: 2006.03.25.23:15

	ONUMs = 22316 (511 exps) 
		22317 (264 exps) 

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	155 degrees (47000)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slits:  100 um
		- OVI Slits:  150 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 232100, 164600, 86600, 67500

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_JOP175new in slot 5

	Fits Files:

q06.03.24.20:10:01.ovi.dat

GAP between 03/25/06|00:30:38( 2455) and 03/25/06|00:44:43( 3812)
GAP between 03/25/06|00:55:05( 4801) and 03/25/06|00:59:25( 5225)

q06.03.25.14:05:47.ovi.dat