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

	Date:		28 March 2003
	-----

 	Last revision:	24 April 2003 (Ko)
	--------------

	File Name: 	2003.03.28.a.log
	-----------

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

	UVCS Activity:	Load and Start Equatorial Coronal Hole Observation for 
	--------------	28 - 29 March 2003
			Load Equatorial Coronal Hole Observation for
			29 March 2003
			Load Equatorial Coronal Hole Observation for
			29 - 30 March 2003
			Load Equatorial Coronal Hole Observation for
			30 March 2003
			Load Mini-Synoptic for 30 March 2003
			Load Equatorial Coronal Hole Observation for
			30 - 31 March 2003
			Load Synoptic for 31 March 2003

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

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

	Command file:	03.03.28.16:13:00.cmd.log

	Activity:
	---------

	1) Observation of an Equatorial Coronal Hole

	Sequence: 02.12_hole1.tcl

	SCI_SPEC: 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=275 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: 2003.03.28.17:43
                    end: 2003.03.29.03:53

	ONUMs =	18722 (27 exps)
		18723 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 267.09, 268.27, 269.38 Degrees (1849, 2063, 2265)
 
		- 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: 170300

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

	Fits Files:

q03.03.28.17:40:56.lya.dat
q03.03.28.17:40:56.ovi.dat
q03.03.28.17:40:56.vld.dat
q03.03.28.21:39:09.lya.dat
q03.03.28.21:39:09.ovi.dat
q03.03.28.21:39:09.vld.dat

GAP between 03/29/03|01:59:44( 4989) and 03/29/03|02:00:57( 5102)

	2) Observation of an Equatorial Coronal Hole

	Sequence: 02.12_hole5.tcl

	SCI_SPEC: 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=275 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: 2003.03.29.03:55
                    end: 2003.03.29.13:48
            
	ONUMs =	18724 (6 exps)
		18725 (54 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 267.09, 269.38 Degrees (1849, 2265)
 
		- 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: 170300

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

	Fits Files:

q03.03.29.03:53:15.lya.dat
q03.03.29.03:53:15.ovi.dat
q03.03.29.03:53:15.vld.dat
q03.03.29.04:27:50.lya.dat
q03.03.29.04:27:50.ovi.dat
q03.03.29.04:27:50.vld.dat