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

	Date:		24 February 2006
	-----

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

	File Name:	2006.02.26.a.log
	----------

	Compiled by:	Y.-K. Ko
	------------

	UVCS Activity:  JOP175 Extended Filaments at the Limb Observation
	--------------	for 26 February 2006
                        JOP175 Extended Filaments at the Limb Observation
                        for 26 - 27 February 2006
                        OVI Detector Diagnostic for 27 February 2006						
	SOHO Activity:	
	--------------	

	EOF Staff:	J. Raymond: Lead Scientist
	---------	Y.-K. Ko: Commander, Planner
			M. Uzzo

	Command file:	06.02.24.19:52:24.cmd.log
	
	Activity:
	---------

	1) JOP175 Extended Filaments at the Limb

	Sequence: 06.02_JOP175long.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.

	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: 2006.02.26.00:44
		    end: 2006.02.26.20:22

	ONUMs = 22279 (368 exps)
		22280 (200 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll: 180 Degrees

		- Roll:	65 degrees (63383)

		- 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_JOP175 in slot 5

	Fits Files:

q06.02.26.00:43:18.ovi.dat
q06.02.26.13:24:55.ovi.dat

	2) JOP175 Extended Filaments at the Limb

	Sequence: 06.02_JOP175long.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.

	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: 2006.02.26.20:25
		    end: 2006.02.27.16:03

	ONUMs = 22281 (368 exps)
		22282 (200 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll: 180 Degrees

		- Roll:	65 degrees (63383)

		- 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_JOP175 in slot 5

	Fits Files:

q06.02.26.20:24:00.ovi.dat
q06.02.27.09:05:37.ovi.dat

	3) 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: 2006.02.27.16:12
                    end: 2006.02.27.17:13

	ONUMs =	22283 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll: 0 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:

q06.02.27.16:04:41.ovi.dat