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

	Date:		14 March 2003
	-----

 	Last revision:	19 March 2003 (Wu)
	--------------

	File Name: 	2003.03.16.a.log
	-----------

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

	UVCS Activity:	Northern Coronal Hole Study for 16 - 17 March 2003
        -------------   Synoptic for 17 March 2003

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

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

	Command file:	03.03.14.15:50:05.cmd.log

	Activity:
	---------

	1) Observation of the Northern Coronal Hole

	Sequence: 02.12_hole1.tcl

	SCI_SPEC: Characterization of the northern coronal hole.
		  Goal is to measure the properties of a 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 non-polar coronal holes.

		  Roll positions are VL-corrected for PA=345 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: 2003.03.16.16:47
                    end: 2003.03.17.02:57

	ONUMs =	18675 (27 exps)
		18676 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 337.09, 338.27, 339.38 Degrees (14592, 14806, 15008)
 
		- 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:

q03.03.16.16:35:03.lya.dat
q03.03.16.16:35:03.ovi.dat
q03.03.16.16:35:03.vld.dat
q03.03.16.20:43:25.lya.dat
q03.03.16.20:43:25.ovi.dat
q03.03.16.20:43:25.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: 2003.03.17.03:06
		    end: 2003.03.17.15:37

	ONUMs = 41630 (37 exps)
		41631 (37 exps)
		41632 (37 exps)
		41633 (37 exps)
		41634 (37 exps)
		41635 (37 exps)
		41636 (37 exps)
		41637 (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:

z03.03.17.03:05:32.lya.dat
z03.03.17.03:05:32.ovi.dat
z03.03.17.03:05:32.vld.dat
z03.03.17.04:39:42.lya.dat
z03.03.17.04:39:42.ovi.dat
z03.03.17.04:39:42.vld.dat
z03.03.17.06:14:19.lya.dat
z03.03.17.06:14:19.ovi.dat
z03.03.17.06:14:19.vld.dat
z03.03.17.07:49:00.lya.dat
z03.03.17.07:49:00.ovi.dat
z03.03.17.07:49:00.vld.dat
z03.03.17.09:23:41.lya.dat
z03.03.17.09:23:41.ovi.dat
z03.03.17.09:23:41.vld.dat
z03.03.17.10:58:21.lya.dat
z03.03.17.10:58:21.ovi.dat
z03.03.17.10:58:21.vld.dat
z03.03.17.12:32:32.lya.dat
z03.03.17.12:32:32.ovi.dat
z03.03.17.12:32:32.vld.dat
z03.03.17.14:07:12.lya.dat
z03.03.17.14:07:12.ovi.dat
z03.03.17.14:07:12.vld.dat