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

	Date:		09 December 2002
	-----

 	Last revision:	12 December 2002 (Wu)
	--------------

	File Name: 	2002.12.10.a.log
	-----------

	Compiled by:	M. Uzzo
	------------

	UVCS Activity:	Equatorial Coronal Hole Study for 10 - 11 December 2002 
	--------------	Equatorial Coronal Hole Study for 11 December 2002 

			Note: Science is a bit behind schedule due in part to
			unexpected safing of UVCS instrument

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

	EOF Staff:	J. Kohl: Lead Scientist
	----------	M. Uzzo: Commander, Planner 
			R. Wu

	Command file:	02.12.09.14:14:48.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=257 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: 2002.12.10.23:52
                    end: 2002.12.11.10:02

	ONUMs =	18328 (26 exps)
		18329 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 249.093 250.267 251.381 Degrees (64129 64343 64546)
 
		- 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:

q02.12.10.23:47:59.lya.dat
q02.12.10.23:47:59.ovi.dat
q02.12.10.23:47:59.vld.dat
q02.12.11.03:48:09.lya.dat
q02.12.11.03:48:09.ovi.dat
q02.12.11.03:48:09.vld.dat

	3) 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=257 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: 2002.12.11.10:04
                    end: 2002.12.11.19:57

	ONUMs =	18330 (6 exps)
		18332 (53 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 249.093 251.381 Degrees (64129 64546)
 
		- 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:

q02.12.11.10:02:07.lya.dat
q02.12.11.10:02:07.ovi.dat
q02.12.11.10:02:07.vld.dat
q02.12.11.10:36:37.lya.dat
q02.12.11.10:36:37.ovi.dat
q02.12.11.10:36:37.vld.dat