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

	Date:		12 May 2003
	-----

 	Last revision:	13 May 2003 (Wu)
	--------------

	File Name: 	2003.05.12.a.log
	-----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	Load and Start Coordinated Coronal UVCS/SPIRIT-CORONAS
	--------------	Observation for 12 - 13 May 2003
			Load Mini-Snynoptic for 13 May 2003
			Load Coordinated Coronal UVCS/SPIRIT-CORONAS 
			Observation for 13 May 2003

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

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

	Command file:	03.05.12.18:23:30.cmd.log
			03.05.13.12:14:01.cmd.log

	Activity:
	---------

  	1) Coordinated UVCS/SPIRIT-CORONAS Observation of the Solar Corona

        Sequence: 03.05_SF_SPIRIT.tcl

	SCI_SPEC: The SPIRIT-CORONAS has the capability of off-limb 
		  observations of EUV line emission: FeIX/X, 172 ang., 
		  and HeII, 304 ang. These line emissions  from streamers 
		  will observed by SPIRIT-CORONAS in coordination with 
		  UVCS-SOHO observation of Ly-alpha, OVI, and SiXII line 
		  emissions from the same coronal structures.

		  The scientific goal is the derivation of the absolute 
		  (i.e., relative to H) abundance of He in the extended 
		  corona. The morphologies of the coronal structures as 
		  observed in these different line emissions will also be
		  compared.
		  
		  Minor error in script caused dwell at each height to be 
		  3 hours rather than 18 minutes.

	OBS_PROG: Primary: Spatial Coverage
		  Sub Obj: Spectral Coverage

	SCI_OBJ:  Coronal Structure...Large-Scale Structure
		  Plasma Properties...Density
		  Abundances

	OBJ:      Streamer, Streamer Cusp, Streamer Boundary

	CMP_NAME: Observations with CORONAS, UVCS / CORONAS (S/C)

	CMP_NUM:  6941

	Duration: start: 2003.05.12.19:45
                    end: 2003.05.13.12:15

	ONUMs =	18901 (303 exps) ; aborted

	Instrument configuration:

		- Pointing:  Sun center
				
		- Roll: 315 Degrees (10570)
 
		- Mirror/Occulter:  1.6, 1.7, 1.8, 1.9 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 175604

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_SF_175  in slot 5

	Fits Files:

q03.05.12.19:44:43.lya.dat
q03.05.12.19:44:43.ovi.dat
q03.05.12.19:44:43.vld.dat

  	2) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 215,
		  LYA grating position now at 128000 "permanently".
		  
		  Reloaded after Flush and Abort of above observation.

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2003.05.13.12:27
		    end: 2003.05.13.15:54

	ONUMs = 42203 (9 exps) 
		42204 (9 exps) 
		42205 (9 exps) 
		42206 (9 exps) 
		42207 (9 exps) 
		42208 (9 exps) 
		42209 (9 exps) 
		42210 (9 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: W, NW, N, NE, E, SE, S, SW

		- Mirror/Occulter: 1.6, 1.75 Ro
 				   1.5 mm overocculting (1.6 Ro)
				   2.0 mm overocculting (1.75 Ro)

		- LYA Slits:   50 um
		- OVI Slits:  150 um

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 194372

		- LYA mask:   LYA_93_1sec    in slot 2
		- OVI mask:   OVI_Syn_194372 in slot 2

	Fits Files:

z03.05.13.12:26:09.lya.dat
z03.05.13.12:26:09.ovi.dat
z03.05.13.12:26:09.vld.dat
z03.05.13.12:52:35.lya.dat
z03.05.13.12:52:35.ovi.dat
z03.05.13.12:52:35.vld.dat
z03.05.13.13:19:04.lya.dat
z03.05.13.13:19:04.ovi.dat
z03.05.13.13:19:04.vld.dat
z03.05.13.13:45:33.lya.dat
z03.05.13.13:45:33.ovi.dat
z03.05.13.13:45:33.vld.dat
z03.05.13.14:12:16.lya.dat
z03.05.13.14:12:16.ovi.dat
z03.05.13.14:12:16.vld.dat
z03.05.13.14:38:45.lya.dat
z03.05.13.14:38:45.ovi.dat
z03.05.13.14:38:45.vld.dat
z03.05.13.15:05:14.lya.dat
z03.05.13.15:05:14.ovi.dat
z03.05.13.15:05:14.vld.dat
z03.05.13.15:31:41.lya.dat
z03.05.13.15:31:41.ovi.dat
z03.05.13.15:31:41.vld.dat