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

	Date:		14 January 2005
	-----

 	Last revision:	18 January 2005 (Wu)
	--------------

	File Name: 	2005.01.16.a.log
	----------

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

	UVCS Activity:	North Coronal Hole LyA Observation for
	--------------	16 January 2005
			North Coronal Hole OVI Observation for 
			16 - 17 January 2005
			North Coronal Hole OVI Observation for 
			17 January 2005
			Load Streamer Study for 18 January 2005

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

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

	Command file:	05.01.14.15:00:00.cmd.log

	Activity:
	---------

	1) North Coronal Hole Observation 

	Sequence: 05.01_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=312 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: 2005.01.16.18:37
                    end: 2005.01.16.23:12

	ONUMs =	21988 (132 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 304.09, 305.27, 306.38 degrees (41362, 41576, 41779)
 
		- 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: 187470

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_188 in slot 6

	Fits Files:

q05.01.16.18:27:41.ovi.dat

	2) North Coronal Hole Observation 

	Sequence: 05.01_hole1OVI.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=312 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: 2005.01.16.23:13
                    end: 2005.01.17.08:39

	ONUMs =	21989 (105 exps)  
		21990 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 304.09, 305.27, 306.38 degrees (41362, 41576, 41779)

		- 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:

q05.01.16.23:12:14.ovi.dat
q05.01.17.02:51:08.ovi.dat

	3) North Coronal Hole Observation 

	Sequence: 05.01_holexOVI.tcl, n50min = 4

	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=312 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: 2005.01.16.08:41
                    end: 2005.01.16.12:53

	ONUMs =	21991 (14 exps)  
		21992 (108 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 304.09, 306.38 degrees (41362, 41779)
 
		- 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:

q05.01.17.08:39:29.ovi.dat
q05.01.17.09:09:37.ovi.dat