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

	Date:		30 December 2005
	-----

	Last revision:	02 January 2006 (Wu)
	--------------

	File Name:	2005.12.29.a.log
	----------

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

	UVCS Activity:	Load and Start North Coronal Hole MgX Observation for
	--------------	29 - 30 December 2005
			Load Mini-Synoptic for 30 December 2005

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

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

	Command file:	05.12.29.22:35:00.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole Observation 

	Sequence: 05.12_hole1MgX.tcl, n = 6, p = 10

	SCI_SPEC: Characterization of a 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.

		  This observation specifically observes MgX 625 line 
		  intensities.

		  Roll positions are VL-corrected for PA=0 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: 2005.12.29.23:06
                    end: 2005.12.30.19:05

	ONUMs =	22064 (240 exps)
		22065 (240 exps)
		22066 (100 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 352.093 degrees (50112)

		- Mirror/Occulter:  1.7 Ro
			            1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS:  67500

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_164 in slot 4

	Fits Files:

q05.12.29.23:06:09.ovi.dat
q05.12.30.07:22:09.ovi.dat
q05.12.30.15:38:09.ovi.dat

	2) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticD:Start

	SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage 
		  at 200.

		  Detector gain test that follows this aborted Mini-Synoptic
		  uses the same ONUM (49261).

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2005.12.30.19:13
		    end: 2005.12.30.20:29

	ONUMs = 49260 (9 exps)
		49261 (12 exps) ; aborted
		49262 ( exps) ; not run
		49263 ( exps) ; not run
		49264 ( exps) ; not run
		49265 ( exps) ; not run
		49266 ( exps) ; not run
		49267 ( exps) ; not run

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll: 180 Degrees

		- Roll:	NE: ms, N: mc, NW: ms, W: ms,  
			SW: ms, S: mc, SE: ms, E: ms

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 187260 (LyA Synoptic)
			      229000 (OVI, and Mini Synoptic)

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Syn_188 in slot 2 (LyA Synoptic)
			      OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic)

	Fits Files:

z05.12.30.19:12:01.ovi.dat
z05.12.30.19:36:57.ovi.dat