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

	Date:		28 March 1997	
	-----

 	Last revision:	31 March 1997 (Wu)
	-------------

	File Name: 	97.03.28.a.log
	-----------

	Compiled by:    R. O'Neal
	------------

	UVCS Activity:  Support of VLA observations of 0036+030
	-------------- 	Load and Start synoptic for March 29
			Load Turbulence in streamers sequence for March 29
			Load synoptic for March 30
			Load Turbulence in streamers sequence for March 30  
			Load synoptic for March 31
			Load CME watch sequence for March 31

      	SOHO Activity:  None
	-------------- 

	EOF Staff:      R. Kopp: Lead Scientist
	----------	R. O'Neal:Commander
 			A. Modigliani:Planner
			R. Wu
                        C. Benna 
 
       Command file:    97.03.28.14:47:49.cmd.log
			scint_ST.cmd.log

       Activity:

        1) Support of VLA observation

        Sequence: 97.03.28_scint_CH.tcl

 
        SCI_SPEC:  VLA observations of this double-lobed
                   radio source will give Faraday rotation
                   along 2 closely spaced lines of sight in
                   the corona from which to derive properties
                   of the fluctuating magnetic field.  UVCS
                   can provide density, flow speed and velocity
                   distributions along the same streamline but 
                   closer to the surface.
 
        OBS_PROG:  Sensitivity
                   Spectral Resolution
 
        SCI_OBJ:  Coronal Structure: Fine structure
                  Coronal Dynamics: Outflow Velocities
 
        OBJ:     Coronal Hole
 
        CMP_NO:  
 
        CMP_NAME:
 
        Duration: start: 97.03.28.17:42
                  end:   97.03.29.03:41
 
        ONUMs = 3976 (57 exposures)  
   
 
        Instrument configuration:
 
                - Pointing:  Sun Center
 
                - Roll: PA=135
 
                - Mirror/Occulter: 1.5 2.0 2.5 3.0 Ro
				   1.5mm overoccultation
 
                - LYA Slits:   50 um
                - OVI Slits:   300 um 
 
                - LYA GRTPOS:  140000
                - OVI GRTPOS:  226000

                - LYA mask: LYA_SYN_140 in slot 2
                - OVI mask: Cusp_OVI226 in slot 3

        Fits files:
 
q97.03.28.17:30:55.lya.dat
q97.03.28.17:30:55.ovi.dat
q97.03.28.17:30:55.vld.dat

        2) Synoptic Sequence Load and Start

	Sequence: Synoptic1:Start
	
        SCI_SPEC: Synoptic studies

	OBS_PROG: Synoptic 

	SCI_OBJ:  Synoptic 

	OBJ:      Entire Corona
                  

	Duration: start: 97.03.29.04:05
		  end:   97.03.29.17:49
		
	ONUMs = 3977 (57 exps) 
                3978 (24 exps)
    		3979 (36 exps)
		3980 (24 exps)
 		3981 (57 exps)
		3982 (24 exps)
		3983 (36 exps) 
		3984 (24 exps)

        Instrument configuration: 
 
                - Pointing:  Sun center 
 
                - Roll: W, NW, N, NE, E, SE, S, SW
 
                - Mirror/Occulter: 1.5, 1.75, 2.0, 2.25, 2.50 Ro (Polar scan)
 				   1.5, 1.75, 2.0, 2.25 Ro (MidLat scan)
                  		   1.5, 1.7, 1.9, 2.2, 2.6, 3 Ro (Equat. scan)
				   1.5 mm overocculting
					
                - LYA Slits:   50 um  
                - OVI Slits:  300 um 
 
                - LYA GRTPOS: 140000
                - OVI GRTPOS: 126000
 
                - LYA mask: LYA_Syn140 in slot 2
                - OVI mask: OVI_Syn13 in slot 2


	Fits Files:

q97.03.29.04:04:38.lya.dat
q97.03.29.04:04:38.ovi.dat
q97.03.29.04:04:38.vld.dat
q97.03.29.05:58:20.lya.dat
q97.03.29.05:58:20.ovi.dat
q97.03.29.05:58:20.vld.dat
q97.03.29.06:51:06.lya.dat
q97.03.29.06:51:06.ovi.dat
q97.03.29.06:51:06.vld.dat
q97.03.29.10:06:49.lya.dat
q97.03.29.10:06:49.ovi.dat
q97.03.29.10:06:49.vld.dat
q97.03.29.10:59:51.lya.dat
q97.03.29.10:59:51.ovi.dat
q97.03.29.10:59:51.vld.dat
q97.03.29.12:53:30.lya.dat
q97.03.29.12:53:30.ovi.dat
q97.03.29.12:53:30.vld.dat
q97.03.29.13:46:14.lya.dat
q97.03.29.13:46:14.ovi.dat
q97.03.29.13:46:14.vld.dat
q97.03.29.17:01:58.lya.dat
q97.03.29.17:01:58.ovi.dat
q97.03.29.17:01:58.vld.dat