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

	Date:		10 October 2002
	-----

 	Last revision:	15 October 2002 (Wu)
	--------------

	File Name: 	2002.10.14.a.log
	-----------

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

	UVCS Activity:  Southern Coronal Hole Study for 14 - 15 October 2002
	--------------	Southern Coronal Hole Study for 15 October 2002
			Mini-Synoptic for 15 October 2002 

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

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

	Command file:	02.10.13.19:33:02.cmd.log

	Activity:
	---------

        1) Observation of High-Latitude South Hemisphere Coronal Hole

        Sequence: 02.06_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=225 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: 2002.10.14.20:24
                    end: 2002.10.15.06:35

	ONUMs =	18122 (27 exps)
		18123 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 217.093, 218.267, 219.381 Degrees (58304, 58517, 58720))
 
		- 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:

q02.10.14.20:13:19.lya.dat
q02.10.14.20:13:19.ovi.dat
q02.10.14.20:13:19.vld.dat
q02.10.15.00:20:48.lya.dat
q02.10.15.00:20:48.ovi.dat
q02.10.15.00:20:48.vld.dat

        2) Observation of High-Latitude South Hemisphere Coronal Hole

        Sequence: 02.06_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=225 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: 2002.10.15.06:37
                    end: 2002.10.15.16:30

	ONUMs =	18124 (6 exps)
		18125 (54 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 217.093, 219.381 Degrees (58304, 58720)
 
		- 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:

q02.10.15.06:34:54.lya.dat
q02.10.15.06:34:54.ovi.dat
q02.10.15.06:34:54.vld.dat
q02.10.15.07:09:30.lya.dat
q02.10.15.07:09:30.ovi.dat
q02.10.15.07:09:30.vld.dat

	3) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 210,
		  LYA grating position now at 128000 "permanently".

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2002.10.15.17:02
		    end: 2002.10.15.20:28

	ONUMs = 40090 (9 exps) 
		40091 (9 exps) 
		40092 (9 exps) 
		40093 (9 exps) 
		40094 (9 exps) 
		40095 (9 exps) 
		40096 (9 exps) 
		40097 (9 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: W, NW, N, NE, E, SE, S, SW

		- Mirror/Occulter: 1.6, 1.75 Ro
 				   1.5 mm overocculting (1.6 Ro)
				   2.0 mm overocculting (1.75 Ro)

		- LYA Slits:   50 um
		- OVI Slits:  150 um

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 173000

		- LYA mask:   LYA_93_1sec  in slot 2
		- OVI mask:   OVI_Syn3_173 in slot 2

	Fits Files:

z02.10.15.17:01:07.lya.dat
z02.10.15.17:01:07.ovi.dat
z02.10.15.17:01:07.vld.dat
z02.10.15.17:27:33.lya.dat
z02.10.15.17:27:33.ovi.dat
z02.10.15.17:27:33.vld.dat
z02.10.15.17:54:02.lya.dat
z02.10.15.17:54:02.ovi.dat
z02.10.15.17:54:02.vld.dat
z02.10.15.18:20:31.lya.dat
z02.10.15.18:20:31.ovi.dat
z02.10.15.18:20:31.vld.dat
z02.10.15.18:47:00.lya.dat
z02.10.15.18:47:00.ovi.dat
z02.10.15.18:47:00.vld.dat
z02.10.15.19:13:36.lya.dat
z02.10.15.19:13:36.ovi.dat
z02.10.15.19:13:36.vld.dat
z02.10.15.19:40:12.lya.dat
z02.10.15.19:40:12.ovi.dat
z02.10.15.19:40:12.vld.dat
z02.10.15.20:06:39.lya.dat
z02.10.15.20:06:39.ovi.dat
z02.10.15.20:06:39.vld.dat