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

	Date:		16 December 2002
	-----

 	Last revision:	18 December 2002 (Wu)
	--------------

	File Name: 	2002.12.17.a.log
	-----------

	Compiled by:	Y.-K. Ko
	------------

	UVCS Activity:	Equatorial Coronal Hole Study for 17 - 18 December 2002
	--------------	Synoptic for 18 December 2002

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

	EOF Staff:	J. Kohl: Lead Scientist
	----------	Y.-K. Ko: Commander, Planner
                        M. Uzzo
                        R. Wu

	Command file:	02.12.16.14:40:06.cmd.log

	Activity:
	---------

	1) 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=105 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: 2002.12.17.18:31
                    end: 2002.12.18.04:41

	ONUMs =	18350 (27 exps)
		18351 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 97.09, 98.27, 99.38 Degrees (36447, 36661, 36864)
 
		- 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:

q02.12.17.18:17:19.lya.dat
q02.12.17.18:17:19.ovi.dat
q02.12.17.18:17:19.vld.dat
q02.12.17.22:27:19.lya.dat
q02.12.17.22:27:19.ovi.dat
q02.12.17.22:27:19.vld.dat

	2) Synoptic Sequence Load and Start

	Sequence: SynopticA:Start

	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: 2002.12.18.05:01
		    end: 2002.12.18.17:33

	ONUMs = 40740 (37 exps)
		40741 (37 exps)
		40742 (37 exps)
		40743 (37 exps)
		40744 (37 exps)
		40745 (37 exps)
		40746 (37 exps)
		40747 (37 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: W: STR2B, NW: STR2B, N: STR2B, NE: STR2B,
                        E: STR2B, SE: STR2B, S: STR2B, SW: STR2B

		- Mirror/Occulter:

			STR1A: 3.5, 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro
			STR2B: 3.0, 2.5. 2.1, 1.9, 1.75, 1.6 Ro
			STR3A: 3.5, 3.0 Ro
			STR4B: 4.0 Ro
			STR5A: 2.1, 1.9, 1.75, 1.6 Ro
			STR6B: 2.5 Ro
			STR7B: 3.0 Ro
			 CH1A: 1.9, 1.75, 1.6 Ro
			 CH2A: 2.1 Ro
			 CH2B: 2.1 Ro
			 CH3B: 2.5 Ro
			 CH4A: 1.75, 1.6 Ro
			 CH5B: 1.9 Ro

			1.5 mm overocculting (1.6 Ro)
			2.0 mm overocculting (1.75, 1.9, 2.1, 2.5, 3.0, 3.5,
					      4.0 Ro)

		- LYA Slits:   50 um
		- OVI Slits:  150 um (STR1A, STR2B, STR3A, STR4B, CH1A,
				      CH2A, CH2B, CH3B)
			      100 um (CH4A, CH5B)
			       75 um (STR5A, STR6B, STR7B)

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 194372

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

	Fits Files:

z02.12.18.05:00:49.lya.dat
z02.12.18.05:00:49.ovi.dat
z02.12.18.05:00:49.vld.dat
z02.12.18.06:35:16.lya.dat
z02.12.18.06:35:16.ovi.dat
z02.12.18.06:35:16.vld.dat
z02.12.18.08:10:10.lya.dat
z02.12.18.08:10:10.ovi.dat
z02.12.18.08:10:10.vld.dat
z02.12.18.09:44:38.lya.dat
z02.12.18.09:44:38.ovi.dat
z02.12.18.09:44:38.vld.dat
z02.12.18.11:19:31.lya.dat
z02.12.18.11:19:31.ovi.dat
z02.12.18.11:19:31.vld.dat
z02.12.18.12:54:00.lya.dat
z02.12.18.12:54:00.ovi.dat
z02.12.18.12:54:00.vld.dat
z02.12.18.14:28:37.lya.dat
z02.12.18.14:28:37.ovi.dat
z02.12.18.14:28:37.vld.dat
z02.12.18.16:03:16.lya.dat
z02.12.18.16:03:16.ovi.dat
z02.12.18.16:03:16.vld.dat