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

	Date:		17 February 2009
	-----

 	Last revision:	24 February 2009 (Wu)
	--------------

	File Name: 	2009.02.24.a.log
 	----------

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

	UVCS Activity:	Recover UVCS from Soft Safe Configuration 
	--------------	Load and Start OVI Detector Dark Rate Diagnostic 
			for 24 February 2009
			Load Equatorial Coronal Observation for 
			24 - 25 February 2009

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

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

	Command file:	09.02.24.12:31:09.cmd.log

	Activity:
	---------

	1) UVCS Recovery from Soft Safe Configuration

	Sequence: Manual

	SCI_SPEC: Completion of recovery of UVCS from soft safe configuration.
		  OVI Detector High Voltage is powered on and ramped up at this 
		  time. 

		  Note: Recovery times (below) are approximate.

	OBS_PROG: 

	SCI_OBJ:  

	OBJ:      

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2009.02.19.12:35
                    end: 2009.02.24.12:55

	ONUMs =	25156

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 0 Degrees

		- Roll: 90 Degrees (35156)
 
		- Mirror/Occulter:  1.5 Ro
                                    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- OVI MCP Voltage: 205

		- OVI mask:   OVI_303_8x2 in slot 3

	Fits Files:


	2) OVI Detector Dark Rate Diagnostic

	Sequence: OVI_dark_chk.tcl

	SCI_SPEC: Determine Dark count rate for OVI detector. Instrument 
		  rolled to coronal hole, 5.0 Ro with 0.8 mm exposed mirror. 
		  Script engages OVI filter and then disengages it at end.

	OBS_PROG: Calibration

	SCI_OBJ:  Calibration

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2009.02.24.12:55
                    end: 2009.02.24.13:56

       	ONUMs =	25157 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll: 0 Degrees (18762)

		- Mirror/Occulter:  5.0 Ro
                                    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 210000

		- OVI Filter Engaged

		- OVI MCP Voltage: 205 

		- OVI mask:   OVI_chk_1xfull in slot 6

	Fits Files:

q09.02.24.12:54:59.ovi.dat

	3) Equatorial Coronal Observation

	Sequence: 09.01_StrProfOVI.tcl, sw = 40, n11 = 2

        SCI_SPEC: A comprehensive study of several streamer properties
                  including the outflow velocities, abundances, electron
                  densities and temperatures. The spatial distribution
                  of these physical properties are analyzed at multiple
                  heights within several streamers examined over the
                  course of the solar cycle.

        OBS_PROG: Primary: Spectral Resolution
                  Sub Obj: Spatial Resolution

        SCI_OBJ:  Primary: Coronal Dynamics...Nonthermal Velocities
                  Sub Obj: Plasma Properties...Proton Temperature

        OBJ:      Streamer

        CMP_NAME:

        CMP_NUM:

	Duration: start: 2009.02.24.14:06
		    end: 2009.02.25.13:57

	ONUMs = 25158 (20 exps)   
		25159 (335 exps)
		25160 (336 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	95 Degrees (36066)

		- Mirror/Occulter:  4.0 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   100 um

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600, 235900

		- OVI MCP Voltage: 205

		- OVI mask:   OVI_str_Prof09 in slot 5

	Fits Files:

q09.02.24.14:05:58.ovi.dat
q09.02.24.14:48:25.ovi.dat
q09.02.25.02:22:49.ovi.dat