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

	Date:		11 April 2003
	-----

 	Last revision:	15 April 2003 (Wu)
	--------------

	File Name: 	2003.04.13.a.log
	-----------

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

	UVCS Activity:	Equatorial Coronal Hole Observation for 
	--------------	13 - 14 April 2003
			Synoptic for 14 April 2003

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

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

	Command file:	03.04.11.18:40:01.cmd.log

	Activity:
	---------

	1) Observation of a High Latitude Southern Coronal Hole

	Sequence: 02.12_hole1.tcl

	SCI_SPEC: Characterization of a high latitude 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=257 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: 2003.04.13.15:57
                    end: 2003.04.14.02:07

	ONUMs =	18782 (26 exps)
		18783 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 249.09, 250.27, 251.38 Degrees (64129, 64343, 64546)
 
		- 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:

q03.04.13.15:53:34.lya.dat
q03.04.13.15:53:34.ovi.dat
q03.04.13.15:53:34.vld.dat
q03.04.13.19:53:41.lya.dat
q03.04.13.19:53:41.ovi.dat
q03.04.13.19:53:41.vld.dat

	2) Synoptic Sequence Load and Start

	Sequence: SynopticA:Start

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 215,
		  LYA grating position now at 128000 "permanently".
                  
	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2003.04.14.02:12
		    end: 2003.04.14.15:25

	ONUMs = 41900 (56 exps)
		41901 (37 exps)
		41902 (37 exps)
		41903 (37 exps)
		41904 (37 exps)
		41905 (37 exps)
		41906 (37 exps)
		41907 (37 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: SW: STR1A, S: STR2B, SE: STR2B, E: STR2B, 
                        NE: STR2B, N: STR2B, NW: STR2B, W: 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:

z03.04.14.02:11:32.lya.dat
z03.04.14.02:11:32.ovi.dat
z03.04.14.02:11:32.vld.dat
z03.04.14.04:28:24.lya.dat
z03.04.14.04:28:24.ovi.dat
z03.04.14.04:28:24.vld.dat
z03.04.14.06:03:05.lya.dat
z03.04.14.06:03:05.ovi.dat
z03.04.14.06:03:05.vld.dat
z03.04.14.07:37:44.lya.dat
z03.04.14.07:37:44.ovi.dat
z03.04.14.07:37:44.vld.dat
z03.04.14.09:11:56.lya.dat
z03.04.14.09:11:56.ovi.dat
z03.04.14.09:11:56.vld.dat
z03.04.14.10:46:51.lya.dat
z03.04.14.10:46:51.ovi.dat
z03.04.14.10:46:51.vld.dat
z03.04.14.12:21:29.lya.dat
z03.04.14.12:21:29.ovi.dat
z03.04.14.12:21:29.vld.dat
z03.04.14.13:56:11.lya.dat
z03.04.14.13:56:11.ovi.dat
z03.04.14.13:56:11.vld.dat