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

	Date:		24 November 2004
	-----

 	Last revision:	29 November 2004 (Wu)
	--------------

	File Name:	2004.11.24.a.log
	----------

	Compiled by:	M. Uzzo, R. Wu
	------------

	UVCS Activity:	Flush Flat Field Calibration using Star Delta 
	--------------  Scorpionis for 24 November 2004
			Adjust mirror height & Reload Flat Field Calibration
			using Star Delta Scorpionis for 24 November 2004
			Load OVI Detector Mask OVI_303_2x6 into OVI slot 4
					       OVI_sp2_188 into OVI slot 5
			Load South Coronal Hole OVI Observation for
			24 - 25 November 2004
			Load South Coronal Hole OVI Observation for
			25 November 2004
			Load South Coronal Hole OVI Observation for
			25 November 2004
			Load South Coronal Hole OVI Observation for
			25 - 26 November 2004
			Load South Coronal Hole OVI Observation for
			26 November 2004	
			Load Ulysses-SOHO Quadrature for 26 - 27 November 2004
			Load South Coronal Hole LyA Observation for
			27 November 2004
			Load West Scan of Mini-Synoptic for 27 November 2004
			Load Ulysses-SOHO Quadrature for 27-28 November 2004
			Load OVI Synoptic for 28 November 2004
			Load Ulysses-SOHO Quadrature for 29 November 2004
			Load LyA Synoptic for 29 November 2004

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

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

	Command file:	04.11.24.12:38:13.cmd.log

	Activity:
	---------

	1) South Coronal Hole Observation 

	Sequence: 04.08_holexOVI.tcl, n50min = 5

	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 degree.

	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: 2004.11.24.19:12
                    end: 2004.11.25.00:14

	ONUMs =	21825 (14 exps)
		21826 (108 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

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

		- 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 3

	Fits Files:

q04.11.24.19:10:39.ovi.dat
q04.11.24.19:41:00.ovi.dat