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

	Date:		15 January 2002
	-----

 	Last revision:	16 January 2002 (Wu)
	--------------

	File Name: 	2002.01.15.a.log
	-----------

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

	UVCS Activity:  Recovery of UVCS from Soft Safe Configuration
	--------------  South Hemisphere Coronal Hole Study 
			for 15 - 16 January 2002

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

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

	Command file:	02.01.15.20:24:23.cmd.log

	Activity:
	---------

        1) Observation of High-Latitude South Hemisphere Coronal Hole

	Sequence: 01.06_hole1.tcl

	SCI_SPEC: Characterization of a high-latitude coronal hole.
                  Goal is to measure the properties of a high-latitude 
		  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=230 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: 2002.01.15.21:15
                    end: 2002.01.16.07:25

	ONUMs =	17050 (27 exps)
		17051 (36 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Roll: 222.09, 223.27, 224.38 Degrees (59214, 59428, 59630)
 
                - 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: 168208

                - LYA mask:   LYA_93_1sec in slot 2
                - OVI mask:   OVI_168MPM  in slot 1

	Fits Files:

q02.01.15.21:13:35.lya.dat
q02.01.15.21:13:35.ovi.dat
q02.01.15.21:13:35.vld.dat
q02.01.16.01:11:20.lya.dat
q02.01.16.01:11:20.ovi.dat
q02.01.16.01:11:20.vld.dat

        2) Observation of High-Latitude South Hemisphere Coronal Hole

	Sequence: 01.06_hole5.tcl

	SCI_SPEC: Characterization of a high-latitude coronal hole.
                  Goal is to measure the properties of a high-latitude 
		  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=230 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: 2002.01.16.07:27
                    end: 2002.01.16.17:20

	ONUMs =	17052 (6 exps)
		17053 (54 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Roll: 222.09, 224.38 Degrees (59214, 59630)

                - 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: 168208

                - LYA mask:   LYA_93_1sec in slot 2
                - OVI mask:   OVI_168MPM  in slot 1

	Fits Files:

q02.01.16.07:25:23.lya.dat
q02.01.16.07:25:23.ovi.dat
q02.01.16.07:25:23.vld.dat
q02.01.16.07:59:47.lya.dat
q02.01.16.07:59:47.ovi.dat
q02.01.16.07:59:47.vld.dat