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

	Date:		13 June 2002
	-----

 	Last revision:	14 June 2002 (Wu)
	--------------

	File Name: 	2002.06.13.a.log
	-----------

	Compiled by:	Y.-K. Ko
	------------

	UVCS Activity:  Load and Start North Polar Coronal Hole Study for 
	--------------	13 - 14 June 2002
			Load North Polar Coronal Hole Study for
			14 June 2002
			Load short North Polar Coronal Hole Study for
			14 June 2002
		
	SOHO Activity:  
	--------------  

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

	Command file:	02.06.13.14:41:18.cmd.log

	Activity:
	---------

        1) Observation of the North Polar Coronal Hole

	Sequence: 02.06_hole1.tcl

        SCI_SPEC: Characterization of the north polar coronal 
                  hole.

                  Goal is to measure the properties of the north 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 the non-polar coronal holes.
                
		  Roll positions are VL-corrected for PA=337 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: 2002.06.13.16:37
                    end: 2002.06.14.02:47

	ONUMs =	17621 (27 exps)
		17622 (36 exps)
	
	Instrument configuration:

		- Pointing:  Sun center

                - Roll: 329.09, 330.27, 331.38 Degrees (13136, 13349, 13552)
 
                - 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: 173000

                - LYA mask:   LYA_93_1sec in slot 2
                - OVI mask:   OVI_173MPM  in slot 1

	Fits Files:

q02.06.13.16:24:36.lya.dat
q02.06.13.16:24:36.ovi.dat
q02.06.13.16:24:36.vld.dat

GAP between 06/13/02|20:21:17( 6884) and 06/13/02|20:25:32( 7293)

q02.06.13.20:33:39.lya.dat
q02.06.13.20:33:39.ovi.dat
q02.06.13.20:33:39.vld.dat

	2) Observation of the North Polar Coronal Hole

	Sequence: 02.06_hole5.tcl

        SCI_SPEC: Characterization of the north polar coronal 
                  hole.

                  Goal is to measure the properties of the north 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 the non-polar coronal holes.
                
		  Roll positions are VL-corrected for PA=337 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: 2002.06.14.02:49
                    end: 2002.06.14.12:42

	ONUMs =	17623 (6 exps)
		17624 (54 exps)
	
	Instrument configuration:

		- Pointing:  Sun center

                - Roll: 329.09, 331.38 Degrees (13136, 13552)
 
                - 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: 173000

                - LYA mask:   LYA_93_1sec in slot 2
                - OVI mask:   OVI_173MPM  in slot 1

	Fits Files:

q02.06.14.02:47:33.lya.dat
q02.06.14.02:47:33.ovi.dat
q02.06.14.02:47:33.vld.dat
q02.06.14.03:22:07.lya.dat
q02.06.14.03:22:07.ovi.dat
q02.06.14.03:22:07.vld.dat

	3) Observation of the North Polar Coronal Hole

	Sequence: 02.06_hole6.tcl

        SCI_SPEC: Characterization of the north polar coronal 
                  hole.

                  Goal is to measure the properties of the north 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 the non-polar coronal holes.
                
		  Roll positions are VL-corrected for PA=337 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: 2002.06.14.12:44
                    end: 2002.06.14.14:22

	ONUMs =	17625 (18 exps)
	
	Instrument configuration:

		- Pointing:  Sun center

                - Roll: 331.38 Degrees (13552)
 
                - Mirror/Occulter:  2.4 Ro
                                    1.5 mm overocculting

                - LYA Slit:    50 um
                - OVI Slit:    75 um 

                - LYA GRTPOS: 128000
                - OVI GRTPOS: 173000

                - LYA mask:   LYA_93_1sec in slot 2
                - OVI mask:   OVI_173MPM  in slot 1

	Fits Files:

q02.06.14.12:42:39.lya.dat
q02.06.14.12:42:39.ovi.dat
q02.06.14.12:42:39.vld.dat