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

	Date:		02 April 2001
	-----

 	Last revision:	20 April 2001 (Wu)
	--------------

	File Name: 	2001.04.02.a.log
	-----------

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

	UVCS Activity:  Mid-latitude Coronal Hole Study for 
	--------------  02 April - 03 April 2001
			Mid-latitude Coronal Hole Study for 03 April 2001

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

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

	Command file:	01.04.02.15:21:50.cmd.log
			01.04.03.15:23:44.cmd.log

	Activity:
	---------

 	1) Observation of Low-Latitude Coronal Hole

	Sequence: 01.01_hole1a.tcl

	SCI_SPEC: Characterization of an Equatorial Coronal Hole.
                  Goal is to measure the properties of a mid-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.
 
	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: 2001.04.02.18:31
                    end: 2001.04.03.04:41

	ONUMs =	16051 (27 exps)
                16052 (36 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 223.053, 224.267, 225.381 Degrees (59396, 59610, 59812)
 
                - 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:

q01.04.02.18:29:17.lya.dat
q01.04.02.18:29:17.ovi.dat
q01.04.02.18:29:17.vld.dat
q01.04.02.22:27:13.lya.dat
q01.04.02.22:27:13.ovi.dat
q01.04.02.22:27:13.vld.dat

 	2) Observation of Low-Latitude Coronal Hole

	Sequence: 01.03_hole5.tcl

	SCI_SPEC: Characterization of an Equatorial Coronal Hole.
                  Goal is to measure the properties of a mid-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.
 
	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: 2001.04.03.04:43
                    end: 2001.04.03.14:53

	ONUMs =	16053 (9 exps)
                16054 (54 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 223.053, 225.381 Degrees (59396, 59812)
 
                - 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:

q01.04.03.04:41:36.lya.dat
q01.04.03.04:41:36.ovi.dat
q01.04.03.04:41:36.vld.dat
q01.04.03.05:32:38.lya.dat
q01.04.03.05:32:38.ovi.dat
q01.04.03.05:32:38.vld.dat

	3) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 205,
		  LYA grating position now at 128000 "permanently".

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2001.04.03.15:28
		    end: 2001.04.03.18:54

	ONUMs = 34780 (9 exps) 
		34781 (9 exps) 
		34782 (9 exps) 
		34783 (9 exps) 
		34784 (9 exps) 
		34785 (9 exps) 
		34786 (9 exps) 
		34787 (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: 168208

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_CME_168 in slot 4

	Fits Files:

z01.04.03.15:27:14.lya.dat
z01.04.03.15:27:14.ovi.dat
z01.04.03.15:27:14.vld.dat
z01.04.03.15:53:43.lya.dat
z01.04.03.15:53:43.ovi.dat
z01.04.03.15:53:43.vld.dat
z01.04.03.16:20:20.lya.dat
z01.04.03.16:20:20.ovi.dat
z01.04.03.16:20:20.vld.dat
z01.04.03.16:46:55.lya.dat
z01.04.03.16:46:55.ovi.dat
z01.04.03.16:46:55.vld.dat
z01.04.03.17:13:24.lya.dat
z01.04.03.17:13:24.ovi.dat
z01.04.03.17:13:24.vld.dat
z01.04.03.17:39:53.lya.dat
z01.04.03.17:39:53.ovi.dat
z01.04.03.17:39:53.vld.dat
z01.04.03.18:06:21.lya.dat
z01.04.03.18:06:21.ovi.dat
z01.04.03.18:06:21.vld.dat
z01.04.03.18:32:48.lya.dat
z01.04.03.18:32:48.ovi.dat
z01.04.03.18:32:48.vld.dat