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

	Date:		06 December 2002
	-----

 	Last revision:	09 December 2002 (Wu)
	--------------

	File Name: 	2002.12.06.a.log
	-----------

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

	UVCS Activity:  Load and Start Mini-Synoptic for 06 December 2002
	--------------	Load Equatorial Coronal Hole Study for 
			06 - 07 December 2002
			Load Synoptic for 07 December 2002
			Load Equatorial Coronal Hole Study for 
			07 - 08 December 2002
			Load Synoptic for 08 December 2002
			Load Equatorial Coronal Hole Study for 
			08 - 09 December 2002
			Load Equatorial Coronal Hole Study for 
			09 December 2002
			Load Mini-Synoptic for 09 December 2002

			Note: Science is a bit behind schedule due in part to
			unexpected safing of UVCS instrument

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

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

	Command file:	02.12.06.21:24:00.cmd.log

	Activity:
	---------

	1) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 210,
		  LYA grating position now at 128000 "permanently".

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2002.12.06.21:30
		    end: 2002.12.07.00:57

	ONUMs = 40620 (9 exps) 
		40621 (9 exps) 
		40622 (9 exps) 
		40623 (9 exps) 
		40624 (9 exps) 
		40625 (9 exps) 
		40626 (9 exps) 
		40627 (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:

z02.12.06.21:29:35.lya.dat
z02.12.06.21:29:35.ovi.dat
z02.12.06.21:29:35.vld.dat
z02.12.06.21:56:03.lya.dat
z02.12.06.21:56:03.ovi.dat
z02.12.06.21:56:03.vld.dat
z02.12.06.22:22:27.lya.dat
z02.12.06.22:22:27.ovi.dat
z02.12.06.22:22:27.vld.dat
z02.12.06.22:49:00.lya.dat
z02.12.06.22:49:00.ovi.dat
z02.12.06.22:49:00.vld.dat
z02.12.06.23:15:37.lya.dat
z02.12.06.23:15:37.ovi.dat
z02.12.06.23:15:37.vld.dat
z02.12.06.23:42:12.lya.dat
z02.12.06.23:42:12.ovi.dat
z02.12.06.23:42:12.vld.dat
z02.12.07.00:08:41.lya.dat
z02.12.07.00:08:41.ovi.dat
z02.12.07.00:08:41.vld.dat
z02.12.07.00:35:08.lya.dat
z02.12.07.00:35:08.ovi.dat
z02.12.07.00:35:08.vld.dat

        2) Observation of an Equatorial Coronal Hole

        Sequence: 02.12_hole1.tcl

	SCI_SPEC: Characterization of an equatorial coronal hole.
		  Goal is to measure the properties of a non-polar
		  coronal hole. In particular we are interested in the 
		  coronal conditions (intensities and line widths for 
		  HI Ly-alpha and OVI 1032/1037) as a function of height 
		  and latitude. We will compare these properties with 
		  the ones found in polar coronal holes.

		  Roll positions are VL-corrected for PA=270 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2002.12.07.01:30
                    end: 2002.12.07.11:40

	ONUMs =	18316 (27 exps)
		18317 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 262.093, 263.267, 264.381 Degrees (939, 1152, 1355)
 
		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:    50, 75 um 

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 170300

		- LYA mask:   LYA_93_1sec   in slot 2
		- OVI mask:   OVI_170300MPM in slot 5

	Fits Files:

q02.12.07.01:18:53.lya.dat
q02.12.07.01:18:53.ovi.dat
q02.12.07.01:18:53.vld.dat
q02.12.07.05:26:37.lya.dat
q02.12.07.05:26:37.ovi.dat
q02.12.07.05:26:37.vld.dat