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

	Date:		12 October 2004
	-----

 	Last revision:	21 October 2004 (Wu)
	--------------

	File Name: 	2004.10.12.a.log
	----------

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

	UVCS Activity:	Load and Start South Coronal Hole OVI Observation for
	-------------	12 - 13 October 2004
                        Load OVI Synoptic for 13 October 2004

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

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

	Command file:	04.10.12.15:04:08.cmd.log

	Activity:
	---------

	1) South Coronal Hole Observation 

	Sequence: 04.08_hole1OVI.tcl

	SCI_SPEC: Characterization of a south polar 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=185 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: 2004.10.12.15:20
                    end: 2004.10.13.00:46

	ONUMs =	21682 (104 exps)  
		21683 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 177.09, 178.27, 179.38 degrees (51021, 51236, 51438)

		- 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: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 4

	Fits Files:

q04.10.12.15:06:09.ovi.dat

GAP between 10/12/04|17:53:13( 9706) and 10/12/04|17:55:39( 9937)

q04.10.12.18:58:05.ovi.dat

	2) OVI Synoptic Sequence Load and Start

	Sequence: SynopticD:Start

	SCI_SPEC: Synoptic studies.  VLD & 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: 2004.10.13.00:52
		    end: 2004.10.13.15:05

	ONUMs = 46400 (49 exps)
		46401 (47 exps) 
		46402 (49 exps)
		46403 (49 exps)
		46404 (49 exps)
		46405 (47 exps)
		46406 (49 exps)
		46407 (48 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

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

		- Mirror/Occulter:

			ls:	3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro
			lc:	2.10, 1.90, 1.75, 1.60 Ro
			os:	3.00, 2.10, 1.90, 1.75, 1.60 Ro
			oc:	1.90, 1.75, 1.60 Ro
			ms:	2.10, 1.75, 1.60 Ro
			mc:	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:

z04.10.13.00:51:15.ovi.dat
z04.10.13.02:39:55.ovi.dat
z04.10.13.04:23:23.ovi.dat
z04.10.13.06:12:03.ovi.dat
z04.10.13.08:00:43.ovi.dat
z04.10.13.09:49:23.ovi.dat
z04.10.13.11:32:51.ovi.dat
z04.10.13.13:21:31.ovi.dat

GAP between 10/13/04|14:54:46(16223) and 10/13/04|14:57:01(   55)