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

	Date:		24 February 1997	
	-----

 	Last revision:	25 February 1997 (Wu)
	-------------

	File Name: 	97.02.24.a.log
	-----------

	Compiled by:    M. Romoli
	------------

	UVCS Activity:  Solitary waves detection above S pole
	--------------	Load and start synoptic for February 25
                        
      	SOHO Activity:  
	-------------- 

	EOF Staff:      M. Romoli: Lead Scientist
	---------       A. Modigliani
			A. Ciaravella
			S. Fineschi
			R. O'Neal
			R. Wu
                 
       Command files:   97.02.24.15:29:19.cmd.log

       Activity:

        1) Solitary waves detection above S pole
 
	Sequence:  97.02.24_marco
		   97.02.24_marco1

        SCI_SPEC:  Detection of solitary waves in coronal hole plume
        	   and interplume region, by monitoring of density
                   fluctuations using visible polarized brightness.
                   UV measurements of line intensity and profile of
                   Lya and OVI provide averaged plasma parameters of
                   the studied region.

        OBS_PROG:       Temporal Resolution
 
        SCI_OBJ:        Coronal Dynamics... Waves
        	        Plasma Properties...Density
 
        OBJ:            Coronal Hole

	CMP_NO:	  

	CMP_NAME: 

        Duration: start: 97.02.24.16:18
                  end:   97.02.25.01:14

        ONUMs = 3578 (72 exposures) 
		3579 (3 Exposures; UV only, pointing test)
		3580 (149 exposures)

        Instrument configuration:
 
                - Pointing:  Sun center
 
                - Roll: PA= 180 (3578,3579), 184 (3580)
 
                - Mirror/Occulter:  2.45 (3578), 1.9 (3580) Ro
                                    1.5 mm occulting

 
                - LYA Slits:   50 um
                - OVI Slits:   300 um (3578,3579), 100 um (3580)
 
                - LYA GRTPOS: 120000
                - OVI GRTPOS: 126000
 
                - LYA mask: SOL_LYA_120 in slot 5
                - OVI mask: SOL_OVI_126 in slot 5
 
 
        Fits files:

q97.02.24.16:16:42.lya.dat
q97.02.24.16:16:42.ovi.dat
q97.02.24.16:16:42.vld.dat
q97.02.24.20:29:47.lya.dat
q97.02.24.20:29:47.ovi.dat
q97.02.24.21:27:58.lya.dat
q97.02.24.21:27:58.ovi.dat
q97.02.24.21:27:58.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: 97.02.25.01:43
		  end:   97.02.25.15:27
		
	ONUMs = 3581 (57 exps) 
                3582 (24 exps)
    		3583 (36 exps)
		3584 (24 exps)
 		3585 (57 exps)
		3586 (24 exps)
		3587 (36 exps) 
		3588 (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: 120000
                - OVI GRTPOS: 126000
 
                - LYA mask: LYA_Syn10 in slot 2
                - OVI mask: OVI_Syn13 in slot 2

	Fits Files:

q97.02.25.01:41:42.lya.dat
q97.02.25.01:41:42.ovi.dat
q97.02.25.01:41:42.vld.dat
q97.02.25.03:35:22.lya.dat
q97.02.25.03:35:22.ovi.dat
q97.02.25.03:35:22.vld.dat
q97.02.25.04:28:16.lya.dat
q97.02.25.04:28:16.ovi.dat
q97.02.25.04:28:16.vld.dat
q97.02.25.07:44:07.lya.dat
q97.02.25.07:44:07.ovi.dat
q97.02.25.07:44:07.vld.dat
q97.02.25.08:37:04.lya.dat
q97.02.25.08:37:04.ovi.dat
q97.02.25.08:37:04.vld.dat
q97.02.25.10:30:30.lya.dat
q97.02.25.10:30:30.ovi.dat
q97.02.25.10:30:30.vld.dat
q97.02.25.11:23:16.lya.dat
q97.02.25.11:23:16.ovi.dat
q97.02.25.11:23:16.vld.dat
q97.02.25.14:38:56.lya.dat
q97.02.25.14:38:56.ovi.dat
q97.02.25.14:38:56.vld.dat