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

	Date:		28 March 2003
	-----

 	Last revision:	24 April 2003 (Ko)
	--------------

	File Name: 	2003.03.29.a.log
	-----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	Equatorial Coronal Hole Observation for 
	--------------	29 - 30 March 2003
			Equatorial Coronal Hole Observation for
			30 March 2003
			Mini-Synoptic for 30 March 2003

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

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

	Command file:	03.03.28.16:13:00.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=275 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: 2003.03.28.13:50
                    end: 2003.03.29.00:00

	ONUMs =	18726 (27 exps)
		18727 (36 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 267.09, 268.27, 269.38 Degrees (1849, 2063, 2265)
 
		- 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:

q03.03.29.13:48:33.lya.dat
q03.03.29.13:48:33.ovi.dat
q03.03.29.13:48:33.vld.dat
q03.03.29.17:46:40.lya.dat
q03.03.29.17:46:40.ovi.dat
q03.03.29.17:46:40.vld.dat

	2) 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=275 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: 2003.03.29.00:02
                    end: 2003.03.29.09:55
            
	ONUMs =	18728 (6 exps)
		18729 (54 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 267.09, 269.38 Degrees (1849, 2265)
 
		- 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:

q03.03.30.00:00:38.lya.dat
q03.03.30.00:00:38.ovi.dat
q03.03.30.00:00:38.vld.dat
q03.03.30.00:35:08.lya.dat
q03.03.30.00:35:08.ovi.dat
q03.03.30.00:35:08.vld.dat

	3) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 215,
		  LYA grating position now at 128000 "permanently".

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2003.03.30.09:58
		    end: 2003.03.30.13:25

	ONUMs = 41750 (9 exps) 
		41751 (9 exps) 
		41752 (9 exps) 
		41753 (9 exps) 
		41754 (9 exps) 
		41755 (9 exps) 
		41756 (9 exps) 
		41757 (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:

z03.03.30.09:57:27.lya.dat
z03.03.30.09:57:27.ovi.dat
z03.03.30.09:57:27.vld.dat
z03.03.30.10:24:00.lya.dat
z03.03.30.10:24:00.ovi.dat
z03.03.30.10:24:00.vld.dat
z03.03.30.10:50:28.lya.dat
z03.03.30.10:50:28.ovi.dat
z03.03.30.10:50:28.vld.dat
z03.03.30.11:16:57.lya.dat
z03.03.30.11:16:57.ovi.dat
z03.03.30.11:16:57.vld.dat
z03.03.30.11:43:26.lya.dat
z03.03.30.11:43:26.ovi.dat
z03.03.30.11:43:26.vld.dat
z03.03.30.12:10:02.lya.dat
z03.03.30.12:10:02.ovi.dat
z03.03.30.12:10:02.vld.dat
z03.03.30.12:36:38.lya.dat
z03.03.30.12:36:38.ovi.dat
z03.03.30.12:36:38.vld.dat
z03.03.30.13:03:05.lya.dat
z03.03.30.13:03:05.ovi.dat
z03.03.30.13:03:05.vld.dat