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

	Date:		02 January 2004
	-----

 	Last revision:	07 January 2004 (Wu)
	--------------

	File Name: 	2004.01.03.a.log
	----------

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

	UVCS Activity:	North Coronal Hole Observation for 03 January 2004 
	--------------	North Coronal Hole Observation for 03 January 2004 

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

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

	Command file:	UVC40102.BCK

	Activity:
	---------

	1) Observation of the North Coronal Hole

	Sequence: 03.12_hole5short2.tcl, n53min=2

	SCI_SPEC: Characterization of a 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=335 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: 2004.01.03.08:51
                    end: 2004.01.03.11:24

	ONUMs =	20713 (26 exps)
		20714 (42 exps)
		
	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 328.27, 327.09, 328.277 degrees (45775, 45560, 45775)
 
		- Mirror/Occulter:  2.0, 1.7, 2.0 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:    50 um 

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 170300

		- LYA mask:   LYA_93_1sec   in slot 2
		- OVI mask:   OVI_170300MPM in slot 5

	Fits Files:

q04.01.03.08:49:32.lya.dat
q04.01.03.08:49:32.ovi.dat
q04.01.03.08:49:32.vld.dat

GAP between 01/03/04|09:00:27( 2512) and 01/03/04|09:01:48( 2651)

q04.01.03.09:50:07.lya.dat
q04.01.03.09:50:07.ovi.dat
q04.01.03.09:50:07.vld.dat

	2) Observation of the North Coronal Hole

	Sequence: 03.12_hole5short2.tcl, n53min=1

	SCI_SPEC: Characterization of a 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=335 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: 2004.01.03.19:20
                    end: 2004.01.03.20:43

	ONUMs =	20715 (26 exps)
		20716 (10 exps)
		
	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 328.27, 327.09, 328.277 degrees (45775, 45560, 45775)
 
		- Mirror/Occulter:  2.0, 1.7, 2.0 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:    50 um 

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 170300

		- LYA mask:   LYA_93_1sec   in slot 2
		- OVI mask:   OVI_170300MPM in slot 5

	Fits Files:

q04.01.03.19:19:32.lya.dat
q04.01.03.19:19:32.ovi.dat
q04.01.03.19:19:32.vld.dat
q04.01.03.20:19:52.lya.dat
q04.01.03.20:19:52.ovi.dat
q04.01.03.20:19:52.vld.dat