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

	Date:		11 February 2005
	-----

 	Last revision:	14 February 2005 (Wu)
	--------------

	File Name:	2005.02.12.a.log
	----------

	Compiled by:	Y.-K. Ko
	------------

	UVCS Activity:	High Latitude Coronal Hole LyA Observation for
	--------------	12 - 13 February 2005
			High Latitude Coronal Hole OVI Observation for
			13  February 2005
			High Latitude Coronal Hole OVI Observation for
			13 February 2005

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

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

	Command file:	05.02.11.15:59:12.cmd.log

	Activity:
	---------

	1) High Latitude Coronal Hole Observation 

	Sequence: 05.02_hole1LyA.tcl

	SCI_SPEC: Characterization of a high latitude coronal hole.
		  Goal is to measure the properties of a non-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 polar coronal holes.

		  Roll positions are VL-corrected for PA=308 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: 2005.02.12.21:51
                    end: 2005.02.13.02:26

	ONUMs =	22104 (132 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 300.09, 301.27, 302.38 degrees (40634, 40848, 41051)
 
		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
			            1.5 mm overocculting

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

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_164 in slot 4

	Fits Files:

q05.02.12.21:39:56.ovi.dat

	2) High Latitude Coronal Hole Observation 

	Sequence: 05.02_hole1OVI.tcl

	SCI_SPEC: Characterization of a high latitude polar coronal hole.
		  Goal is to measure the properties of a non-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 polar coronal holes.

		  Roll positions are VL-corrected for PA=308 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: 2005.02.13.02:27
                    end: 2005.02.13.11:53

	ONUMs =	22105 (105 exps)  
		22106 (166 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 300.09, 301.27, 302.38 degrees (40634, 40848, 41051)

		- Mirror/Occulter:  1.7, 2.0, 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 5

	Fits Files:

q05.02.13.02:25:51.ovi.dat
q05.02.13.06:04:48.ovi.dat

	3) High Latitude Coronal Hole Observation 

	Sequence: 05.02_holexOVI.tcl, n50min = 7

	SCI_SPEC: Characterization of a high latitude polar coronal hole.
		  Goal is to measure the properties of a non-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 polar coronal holes.

		  Roll positions are VL-corrected for PA=308 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: 2005.02.13.11:54
                    end: 2005.02.13.18:36

	ONUMs =	22107 (14 exps)  
		22108 (130 exps) 
		22109 (48 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 300.09, 302.38 degrees (40634, 41051)

		- 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 5

	Fits Files:

q05.02.13.11:52:49.ovi.dat
q05.02.13.12:22:57.ovi.dat

GAP between 02/13/05|13:00:16(11242) and 02/13/05|13:03:15(11529)

q05.02.13.16:56:29.ovi.dat