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

	Date:		12 January 2006
	-----

 	Last revision:	17 February 2006 (Wu)
	--------------

	File Name:	2006.01.13.a.log
	----------

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

	UVCS Activity:	Flush South Polar Coronal Hole OVI Observation
        --------------  for 12 - 14 January 2006
			Load and Start South Polar Coronal Hole OVI 
			Observation for 13 - 15 January 2006
			Load South Polar Coronal Hole LyA Observation for
			15 January 2006
			Load South Polar Coronal Hole OVI Observation for 
			15 - 17 January 2006

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

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

	Command file:	06.01.12.20:49:00.cmd.log
			06.01.13.19:56:00.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole Observation 

	Sequence: 06.01_holeOVI.tcl, r = 17, n6hr = 8

	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=180 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: 2006.01.12.22:08
                    end: 2006.01.13.21:38

	ONUMs =	22109 (174 exps)
		22110 (174 exps)
		22111 (174 exps)
		22112 (160 exps) ; flushed
		22113 (174 exps) ; not run
		22114 (174 exps) ; not run
		22115 (174 exps) ; not run
		22116 (174 exps) ; not run

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 352.09 degrees (17323)

		- Mirror/Occulter:  1.7 Ro
			            1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    75 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 5

	Fits Files:

q06.01.12.22:08:07.ovi.dat
q06.01.13.04:07:43.ovi.dat
q06.01.13.10:07:19.ovi.dat
q06.01.13.16:06:55.ovi.dat

	2) South Polar Coronal Hole Observation 

	Sequence: 06.01_holeOVI.tcl, r = 17, n6hr = 8

	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=180 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: 2006.01.13.21:38
                    end: 2006.01.15.21:35

	ONUMs =	22113 (174 exps)
		22114 (174 exps)
		22115 (174 exps)
		22116 (174 exps)
		22117 (174 exps)
		22118 (174 exps)
		22119 (174 exps)
		22120 (174 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 352.09 degrees (17323)

		- Mirror/Occulter:  1.7 Ro
			            1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:    75 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 5

	Fits Files:

q06.01.13.21:38:23.ovi.dat
q06.01.14.03:37:59.ovi.dat
q06.01.14.09:37:35.ovi.dat
q06.01.14.15:37:11.ovi.dat
q06.01.14.21:36:47.ovi.dat
q06.01.15.03:36:23.ovi.dat
q06.01.15.09:35:59.ovi.dat
q06.01.15.15:35:35.ovi.dat