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

	Date:		24 October 2005
	-----

 	Last revision:	25 October 2005 (Wu)
	--------------

	File Name:	2005.10.24.a.log
	----------

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

	UVCS Activity:	Load and Start Polar Coronal Hole LyA Observation for 
	--------------	24 - 25 October 2005
                      	Load and Start Polar Coronal Hole OVI Observation for 
                      	25 October 2005
                      	Load LyA Synoptic for 25 October 2005
                      	Load OVI Synoptic for 25 - 26 October 2005

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

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

	Command file:	05.10.24.12:07:00.cmd.log

	Activity:
	---------

	1) Polar Coronal Hole Observation 

	Sequence: 05.09_hole1LyA.tcl

	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.

		  Roll positions are VL-corrected for PA=8 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: 2005.10.25.00:01
                    end: 2005.10.25.04:35

	ONUMs =	21867 (107 exps)  

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 0.093, 1.267, 2.381 degrees (18779, 18993, 19195)

		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
			            1.5 mm overocculting (1.7, 2.0 Ro)
			            2.0 mm overocculting (2.4 Ro)

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_164 in slot 4

	Fits Files:

q05.10.24.23:49:49.ovi.dat

	2) Polar Coronal Hole Observation 

	Sequence: 05.09_hole1OVI.tcl

	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.

		  Roll positions are VL-corrected for PA=8 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: 2005.10.25.04:37
                    end: 2005.10.25.14:03

	ONUMs =	21868 (105 exps)  
		21869 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 0.093, 1.267, 2.381 degrees (18779, 18993, 19195)

		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
			            1.5 mm overocculting (1.7, 2.0 Ro)
			            2.0 mm overocculting (2.4 Ro)

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 5

	Fits Files:

q05.10.25.04:35:51.ovi.dat
q05.10.25.08:14:48.ovi.dat

GAP between 10/25/05|13:48:20(12600) and 10/25/05|13:50:20(12792)