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

	Date:		08 January 2004
	-----

 	Last revision:	15 January 2004 (Ko)
	--------------

	File Name: 	2004.01.08.a.log
	----------

	Compiled by:	M. Uzzo
	------------

	UVCS Activity:	Abort UVCS Instrument Study for 07 - 08 January 
	--------------	2004 with MCP voltage @ 205
			Load OVI Detector Mask OVI_CH_230 into OVI Slot 4
			Load and Start Coronal Hole Observation/Engineering 
			Study with MCP voltage @ 205 for 08 - 09 January 2004
			Load Coronal Hole Observation/Engineering Study
			with MCP voltage @ 205 for 09 January 2004

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

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

	Command file:	04.01.08.20:13:48.cmd.log

	Activity:
	---------

	1) Coronal Hole Observation/Engineering Study with MCP voltage @ 205

	Sequence: 04.01_hole1_230.tcl

	SCI_SPEC: Examining the possibility of running this observation
		  at grating position 230,000 with MCP voltage at 205. 

		  Characterization of an equatorial 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=270 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: 2004.01.08.23:46
                    end: 2004.01.09.09:54

	ONUMs =	20735 (104 exps)
		20736 (168 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: 262.09, 263.27, 264.38 degrees (33717, 33930, 34133)
 
		- 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

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_CH_230  in slot 4

	Fits Files:

q04.01.08.23:39:48.lya.dat
q04.01.08.23:39:48.ovi.dat
q04.01.08.23:39:48.vld.dat
q04.01.09.03:40:50.lya.dat
q04.01.09.03:40:50.ovi.dat
q04.01.09.03:40:50.vld.dat

	2) Coronal Hole Observation/Engineering Study with MCP voltage @ 205

	Sequence: 04.01_hole1_230.tcl

	SCI_SPEC: Examining the possibility of running this observation
		  at grating position 230,000 with MCP voltage at 205. 

		  Characterization of an equatorial 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=270 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: 2004.01.09.09:55
                    end: 2004.01.09.16:18

	ONUMs =	20737 (105 exps)
		20738 (66 exps) ; aborted

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: 262.09, 263.27, 264.38 degrees (33717, 33930, 34133)
 
		- 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

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_CH_230  in slot 4

	Fits Files:

q04.01.09.09:54:06.lya.dat
q04.01.09.09:54:06.ovi.dat
q04.01.09.09:54:06.vld.dat
q04.01.09.13:50:54.lya.dat
q04.01.09.13:50:54.ovi.dat
q04.01.09.13:50:54.vld.dat