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

	Date:		13 January 2004
	-----

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

	File Name: 	2004.01.13.a.log
	----------

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

	UVCS Activity:	Load New Embedded routines found in OVIExposure.tcl,
	--------------	and OVIPolExp.tcl for observations without LyA 
			detector exposures. Embedded routines for
			04.01_hole1OVI.tcl, 04.01_hole1LyA.tcl,
			SynopticOVI (Mini, str1a, str2b, str4b)
			Load Masks: 	OVI_Syn_230 in slot 1
					OVI_Syn_188 in slot 2
					OVI_MPM_232 in slot 4
			Load and Start Coronal Hole Observation/Engineering 
			Study with MCP voltage @ 200 for 13 - 14 January 2004
			Load Coronal Hole Observation/Engineering Study 
			with MCP voltage @ 200 for 14 January 2004

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

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

	Command file:	04.01.13.13:35:03.cmd.log

	Activity:
	---------

	1) Coronal Hole Observation / Engineering Study with MCP voltage @ 200

	Sequence: 04.01_hole1LyA.tcl

	SCI_SPEC: Examining the possibility of running this observation
		  at grating position 188,940 with MCP voltage at 200. 

		  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=295 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: 2004.01.13.22:28
                    end: 2004.01.14.01:03

	ONUMs =	20770 (66 exps)  

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: 287.09, 288.27, 289.38 degrees (38268, 38481, 38684)
 
		- 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: 188940

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_Syn_184 in slot 2

	Fits Files:

q04.01.13.22:26:36.ovi.dat
q04.01.13.22:26:36.vld.dat

	2) Coronal Hole Observation / Engineering Study with MCP voltage @ 200

	Sequence: 04.01_hole1OVI.tcl

	SCI_SPEC: Examining the possibility of running this observation
		  at grating position 230,000 with MCP voltage at 200. 

		  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=295 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: 2004.01.14.01:05
                    end: 2004.01.14.11:09

	ONUMs =	20772 (105 exps)  
		20773 (168 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: 287.09, 288.27, 289.38 degrees (38268, 38481, 38684)
 
		- 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:

q04.01.14.01:04:02.ovi.dat
q04.01.14.01:04:02.vld.dat
q04.01.14.04:58:36.ovi.dat
q04.01.14.04:58:36.vld.dat