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

	Date:		30 March 2001
	-----

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

	File Name: 	2001.03.31.a.log
	-----------

	Compiled by:	S. Mancuso
	------------

	UVCS Activity:  Start mid-latitude coronal hole for 
	--------------  03/31/01-04/01/01
  			Start mini-Synoptic for 04/01/01

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

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

	Command file:	01.03.30.16:33:22.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: 2001.03.31.17:44
                    end: 2001.04.01.03:53

	ONUMs =	16043 (27 exps)
                16044 (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:

q01.03.31.17:42:00.lya.dat
q01.03.31.17:42:00.ovi.dat
q01.03.31.17:42:00.vld.dat
q01.03.31.21:39:58.lya.dat
q01.03.31.21:39:58.ovi.dat
q01.03.31.21:39:58.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: 2001.04.01.03:55
                    end: 2001.04.01.14:05

	ONUMs =	16045 (9 exps)
                16046 (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:

q01.04.01.03:53:49.lya.dat
q01.04.01.03:53:49.ovi.dat
q01.04.01.03:53:49.vld.dat
q01.04.01.04:44:55.lya.dat
q01.04.01.04:44:55.ovi.dat
q01.04.01.04:44:55.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: 2001.04.01.14:37
		    end: 2001.04.01.18:04

	ONUMs = 34764 (9 exps) 
		34765 (9 exps) 
		34766 (9 exps) 
		34767 (9 exps) 
		34768 (9 exps) 
		34769 (9 exps) 
		34770 (9 exps) 
		34771 (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:

z01.04.01.14:36:55.lya.dat
z01.04.01.14:36:55.ovi.dat
z01.04.01.14:36:55.vld.dat
z01.04.01.15:03:30.lya.dat
z01.04.01.15:03:30.ovi.dat
z01.04.01.15:03:30.vld.dat
z01.04.01.15:29:55.lya.dat
z01.04.01.15:29:55.ovi.dat
z01.04.01.15:29:55.vld.dat
z01.04.01.15:56:43.lya.dat
z01.04.01.15:56:43.ovi.dat
z01.04.01.15:56:43.vld.dat
z01.04.01.16:23:11.lya.dat
z01.04.01.16:23:11.ovi.dat
z01.04.01.16:23:11.vld.dat
z01.04.01.16:49:40.lya.dat
z01.04.01.16:49:40.ovi.dat
z01.04.01.16:49:40.vld.dat
z01.04.01.17:16:03.lya.dat
z01.04.01.17:16:03.ovi.dat
z01.04.01.17:16:03.vld.dat
z01.04.01.17:42:36.lya.dat
z01.04.01.17:42:36.ovi.dat
z01.04.01.17:42:36.vld.dat