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

	Date:		16 February 2004
	-----

 	Last revision:	18 February 2004 (Wu)
	--------------

	File Name: 	2004.02.16.a.log
	----------

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

	UVCS Activity:	Equatorial Coronal Hole OVI Observation for
	--------------	16 - 17 February 2004
			Mini-Synoptic for 17 February 2004

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

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

	Command file:	04.02.13.16:11:00.cmd.log

	Activity:
	---------

	1) Equatorial Coronal Hole Observation 

	Sequence: 04.02_holexOVI.tcl, n53min = 8

	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=280 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: 2004.02.16.19:39
                    end: 2004.02.17.03:41

	ONUMs =	20977 (14 exps)  
		20978 (132 exps) 
		20979 (72 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: 272.09, 274.38 degrees (34437, 35954)
 
		- Mirror/Occulter:  1.7, 2.4 Ro
			            1.5 mm overocculting

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

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 4

	Fits Files:

q04.02.16.19:38:05.ovi.dat
q04.02.16.19:38:05.vld.dat
q04.02.16.20:11:28.ovi.dat
q04.02.16.20:11:28.vld.dat
q04.02.17.01:02:28.ovi.dat
q04.02.17.01:02:28.vld.dat

	2) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticB:Start

	SCI_SPEC: Synoptic studies.  LYA HV & Power off / OVI voltage at 200,
		  LYA grating position now at 128000 "permanently".

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2004.02.17.03:56
		    end: 2004.02.17.09:12

	ONUMs = 44460 (10 exps)
		44461 (24 exps) 
		44462 (10 exps)
		44463 (24 exps)
		44464 (10 exps)
		44465 (24 exps)
		44466 (10 exps)
		44467 (10 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

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

		- Mirror/Occulter:

			lya_str:  3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro
			lya_ch:   2.10, 1.90, 1.75, 1.60 Ro
			ovi_str:  3.00, 2.10, 1.90, 1.75, 1.60 Ro
			ovi_ch:   1.90, 1.75, 1.60 Ro
			mini_str: 2.10, 1.75, 1.60 Ro
			mini_ch:  1.90, 1.75, 1.60 Ro

			1.5 mm overocculting (1.60 Ro)
			2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00 Ro)

		- LYA Slits:   50 um
		- OVI Slits:  100 um (LyA Synoptic)
			      150 um (OVI, and Mini Synoptic)

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 177596 (LyA Synoptic)
			      229000 (OVI, and Mini Synoptic)

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Syn_178 in slot 2 (LyA Synoptic)
			      OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic)

	Fits Files:

z04.02.17.03:55:39.ovi.dat
z04.02.17.03:55:39.vld.dat
z04.02.17.04:24:50.ovi.dat
z04.02.17.04:24:50.vld.dat
z04.02.17.05:23:03.ovi.dat
z04.02.17.05:23:03.vld.dat
z04.02.17.05:52:16.ovi.dat
z04.02.17.05:52:16.vld.dat
z04.02.17.06:50:31.ovi.dat
z04.02.17.06:50:31.vld.dat
z04.02.17.07:19:42.ovi.dat
z04.02.17.07:19:42.vld.dat
z04.02.17.08:17:54.ovi.dat
z04.02.17.08:17:54.vld.dat
z04.02.17.08:47:17.ovi.dat
z04.02.17.08:47:17.vld.dat