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

	Date:		28 February 2003
	-----

 	Last revision:	03 March 2003 (Wu)
	--------------

	File Name: 	2003.03.02.a.log
	-----------

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

	UVCS Activity:	Low Latitude Coronal Hole Study for 02 - 03 March 2003
	-------------	Low Latitude Coronal Hole Study for 03 March 2003
			Mini-Synoptic for 03 March 2003

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

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

	Command file:	03.02.28.14:53:00.cmd.log
                        03.03.01.21:10:46.cmd.log

	Activity:
	---------

	1) Observation of the Low Latitude Coronal Hole

	Sequence: 02.12_hole1.tcl

	SCI_SPEC: Characterization of a low latitude 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=274 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: 2003.03.02.17:12
                    end: 2003.03.03.03:22

	ONUMs =	18617 (27 exps)
		18618 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 266.09, 267.27, 268.38 Degrees (1667, 1880, 2083)
 
		- 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:

q03.03.02.16:58:25.lya.dat
q03.03.02.16:58:25.ovi.dat
q03.03.02.16:58:25.vld.dat
q03.03.02.21:08:27.lya.dat
q03.03.02.21:08:27.ovi.dat
q03.03.02.21:08:27.vld.dat

	2) Observation of the Low Latitude Coronal Hole

	Sequence: 02.12_hole5.tcl
	
	SCI_SPEC: Characterization of a low latitude 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=274 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: 2003.03.03.03:24
                    end: 2003.03.03.13:17

	ONUMs =	18619 (6 exps)
		18620 (54 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 266.09, 268.38 Degrees (1667, 2083)
 
		- 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:

q03.03.03.03:22:30.lya.dat
q03.03.03.03:22:30.ovi.dat
q03.03.03.03:22:30.vld.dat
q03.03.03.03:56:53.lya.dat
q03.03.03.03:56:53.ovi.dat
q03.03.03.03:56:53.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: 2003.03.03.13:20
		    end: 2003.03.03.16:47

	ONUMs = 41490 (9 exps) 
		41491 (9 exps) 
		41492 (9 exps) 
		41493 (9 exps) 
		41494 (9 exps) 
		41495 (9 exps) 
		41496 (9 exps) 
		41497 (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: 194372

		- LYA mask:   LYA_93_1sec    in slot 2
		- OVI mask:   OVI_Syn_194372 in slot 2

	Fits Files:

z03.03.03.13:19:15.lya.dat
z03.03.03.13:19:15.ovi.dat
z03.03.03.13:19:15.vld.dat
z03.03.03.13:45:36.lya.dat
z03.03.03.13:45:36.ovi.dat
z03.03.03.13:45:36.vld.dat
z03.03.03.14:12:13.lya.dat
z03.03.03.14:12:13.ovi.dat
z03.03.03.14:12:13.vld.dat
z03.03.03.14:38:41.lya.dat
z03.03.03.14:38:41.ovi.dat
z03.03.03.14:38:41.vld.dat
z03.03.03.15:05:10.lya.dat
z03.03.03.15:05:10.ovi.dat
z03.03.03.15:05:10.vld.dat
z03.03.03.15:31:39.lya.dat
z03.03.03.15:31:39.ovi.dat
z03.03.03.15:31:39.vld.dat
z03.03.03.15:58:08.lya.dat
z03.03.03.15:58:08.ovi.dat
z03.03.03.15:58:08.vld.dat
z03.03.03.16:24:50.lya.dat
z03.03.03.16:24:50.ovi.dat
z03.03.03.16:24:50.vld.dat