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

	Date:		02 March 2004
	-----

 	Last revision:	04 March 2004 (Wu)
	--------------

	File Name: 	2004.03.03.a.log
	----------

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

	UVCS Activity:	Load and Start Equatorial Coronal Hole OVI Observation 
	--------------  for 03 - 04 March 2004
			Load OVI Synoptic for 04 March 2004

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

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

	Command file:	04.03.03.15:24:00.cmd.log

	Activity:
	---------

	1) Equatorial Coronal Hole Observation 

	Sequence: 04.02_holexOVI.tcl, n53min = 6

	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=285 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: 2004.03.03.19:05
                    end: 2004.03.04.01:21

	ONUMs =	21046 (14 exps)  
		21047 (132 exps) 
                21048 (24 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: 277.09, 279.38 degrees (36447, 36864)
 
		- 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:

q04.03.03.18:55:16.ovi.dat
q04.03.03.18:55:16.vld.dat

GAP between 03/03/04|19:12:43( 6386) and 03/03/04|19:14:01( 6519)

q04.03.03.19:37:16.ovi.dat
q04.03.03.19:37:16.vld.dat
q04.03.04.00:28:09.ovi.dat
q04.03.04.00:28:09.vld.dat

	2) OVI Synoptic Sequence Load and Start

	Sequence: SynopticC: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: 2004.03.04.01:42
		    end: 2004.03.04.16:46

	ONUMs = 44630 (49 exps)
		44631 (49 exps) 
		44632 (47 exps)
		44633 (49 exps)
		44634 (49 exps)
		44635 (49 exps)
		44636 (47 exps)
		44637 (49 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	E: ovi_str, SE: ovi_str, S: ovi_ch, SW: ovi_str,
			W: ovi_str, NW: ovi_str, N: ovi_ch, NE: ovi_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:  150 um (LyA Synoptic)
			      200 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:

z04.03.04.01:41:33.ovi.dat
z04.03.04.01:41:33.vld.dat
z04.03.04.03:37:06.ovi.dat
z04.03.04.03:37:06.vld.dat
z04.03.04.05:32:46.ovi.dat
z04.03.04.05:32:46.vld.dat
z04.03.04.07:20:58.ovi.dat
z04.03.04.07:20:58.vld.dat
z04.03.04.09:16:36.ovi.dat
z04.03.04.09:16:36.vld.dat
z04.03.04.11:12:11.ovi.dat
z04.03.04.11:12:11.vld.dat
z04.03.04.13:07:40.ovi.dat
z04.03.04.13:07:40.vld.dat
z04.03.04.14:55:56.ovi.dat
z04.03.04.14:55:56.vld.dat