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

	Date:		01 July 2005
	-----

 	Last revision:	05 July 2005 (Wu)
	--------------

	File Name:	2005.07.01.a.log
	----------

	Compiled by:	M. Uzzo, R. Wu
	------------

	UVCS Activity:	Load and Start North Polar Coronal Hole LyA Observation 
        --------------  for 01 - 02 July 2005
        		Load North Polar Coronal Hole OVI Observation for 
        		02 July 2005
	       	        Load North Polar Coronal Hole OVI Observation for 
	       	        02 July 2005
			Load OVI Synoptic for 02 - 03 July 2005
			Load LyA Synoptic for 03 July 2005
			Load Low Latitude Coronal Hole LyA Observation 
			for 03 July 2005
        		Load Low Latitude Coronal Hole OVI Observation for 
        		03 - 04 July 2005
	       	        Load Low Latitude Coronal Hole OVI Observation for 
	       	        04 July 2005
			Load Mini-Synoptic for 04 July 2005
			Load Low Latitude Coronal Hole OVI Observation 
			for 04 - 05 July 2005
        		Load OVI Synoptic for 05 July 2005

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

	EOF Staff:      M. P. Miralles: Lead Scientist
	---------- 	M. Uzzo: Commander, Planner

	Command file:	05.07.01.12:17:20.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole Observation 

	Sequence: 05.02_hole1LyA.tcl

	SCI_SPEC: Characterization of the North 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=5 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: 2005.07.01.23:18
                    end: 2005.07.02.03:52

	ONUMs =	21492 (132 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 357.09, 358.27, 359.38 degrees (51021, 51236, 51438)

		- 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:

q05.07.01.23:06:11.ovi.dat

	2) North Polar Coronal Hole Observation 

	Sequence: 05.02_hole1OVI.tcl

	SCI_SPEC: Characterization of the North 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=5 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: 2005.07.02.03:53
                    end: 2005.07.02.13:19

	ONUMs =	21493 (105 exps)  
		21494 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 357.09, 358.27, 359.38 degrees (51021, 51236, 51438)

		- 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:

q05.07.02.03:52:17.ovi.dat
q05.07.02.07:31:14.ovi.dat

	3) North Polar Coronal Hole Observation 

	Sequence: 05.02_holexOVI.tcl, n50min = 7

	SCI_SPEC: Characterization of the North 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=5 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: 2005.07.02.13:20
                    end: 2005.07.02.20:02

	ONUMs =	21495 (14 exps)  
		21496 (132 exps)
		21497 (48 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 357.09, 359.38 degrees (51021, 51438)

		- 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:

q05.07.02.13:19:15.ovi.dat
q05.07.02.13:49:23.ovi.dat
q05.07.02.18:22:55.ovi.dat