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

	Date:		27 January 2006
	-----

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

	File Name:	2006.01.27.a.log
	----------

	Compiled by:	Y.-K. Ko, R. Wu
	------------

	UVCS Activity:	Load and Start OVI Detector Diagnostic for 
        --------------  27 January 2006
        		Load South Polar Coronal Hole OVI Observation for
			27 - 29 January 2006
                        Load and Start OVI Detector Diagnostic for 
                        29 January 2006
                        Load LyA Synoptic for 29 - 30 January 2006
                        Load OVI Synoptic for 30 January 2006

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

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

	Command file:	06.01.27.17:33:53.cmd.log

	Activity:
	---------

	1) OVI Detector Diagnostic

	Sequence: 06.01_OVI_164_chk.tcl

	SCI_SPEC: Instrument Diagnostics

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2006.01.27.22:27
                    end: 2006.01.27.23:28

	ONUMs =	22180 (12 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll: 354.38 degrees (17739)

		- Mirror/Occulter:  1.75 Ro
                                    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask: OVI_chk_1xfull in slot 1

	Fits Files:

q06.01.27.22:23:32.ovi.dat

	2) South Polar Coronal Hole Observation 

	Sequence: 06.02_holeOVI.tcl, r = 24, n6hr = 7, n3hr = 1

	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: 2006.01.27.23:29
		    end: 2006.01.29.20:26

	ONUMs = 22181 (153 exps)
		22182 (174 exps)
		22183 (174 exps)
		22184 (174 exps)
		22185 (174 exps)
		22186 (174 exps)
		22187 (174 exps)
		22188 (87 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 354.38 degrees (17739)

		- Mirror/Occulter:  2.4 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:

q06.01.27.23:29:10.ovi.dat

GAP between 01/28/06|04:33:44(11567) and 01/28/06|05:16:55(15716)

q06.01.28.05:28:46.ovi.dat
q06.01.28.11:28:22.ovi.dat
q06.01.28.17:27:58.ovi.dat
q06.01.28.23:27:34.ovi.dat
q06.01.29.05:27:10.ovi.dat
q06.01.29.11:26:46.ovi.dat
q06.01.29.17:26:22.ovi.dat