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

	Date:		16 March 2001
	-----

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

	File Name: 	2001.03.16.a.log
	-----------

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

	UVCS Activity:  Mini-Synoptic 03/16/01
	--------------  Load high-latitude coronal hole study 03/16/01
                        Load long synoptic 03/17/01
                        Load high-latitude coronal hole study 03/17/01
                        Load mini-synoptic 03/18/01
                        Load high-latitude coronal hole study 03/18/01
			
	SOHO Activity:  
	--------------  

	EOF Staff:	L. Strachan: Lead Scientist
	----------	Y.-K. Ko: Commander, Planner
			D. Phillips: Planner
                        M. Uzzo
      			R. Wu

	Command file:	01.03.15.15:30:31.cmd.log
                        01.03.16.16:51:38.cmd.log

	Activity:
	---------

	1) 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: 2001.03.16.15:36
		    end: 2001.03.16.19:03

	ONUMs = 34630 (9 exps) 
		34631 (9 exps) 
		34632 (9 exps) 
		34633 (9 exps) 
		34634 (9 exps) 
		34635 (9 exps) 
		34636 (9 exps) 
		34637 (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:

z01.03.16.15:35:53.lya.dat
z01.03.16.15:35:53.ovi.dat
z01.03.16.15:35:53.vld.dat
z01.03.16.16:02:28.lya.dat
z01.03.16.16:02:28.ovi.dat
z01.03.16.16:02:28.vld.dat
z01.03.16.16:28:57.lya.dat
z01.03.16.16:28:57.ovi.dat
z01.03.16.16:28:57.vld.dat
z01.03.16.16:55:26.lya.dat
z01.03.16.16:55:26.ovi.dat
z01.03.16.16:55:26.vld.dat
z01.03.16.17:22:03.lya.dat
z01.03.16.17:22:03.ovi.dat
z01.03.16.17:22:03.vld.dat
z01.03.16.17:48:38.lya.dat
z01.03.16.17:48:38.ovi.dat
z01.03.16.17:48:38.vld.dat
z01.03.16.18:15:07.lya.dat
z01.03.16.18:15:07.ovi.dat
z01.03.16.18:15:07.vld.dat
z01.03.16.18:41:34.lya.dat
z01.03.16.18:41:34.ovi.dat
z01.03.16.18:41:34.vld.dat

 	2) Observation of High-Latitude Coronal Hole

	Sequence: 01.01_hole4.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.
 
	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: 2001.03.16.19:29
                    end: 2001.03.17.05:20

	ONUMs =	15973 (57 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 341.141 degrees (15329)
 
                - Mirror/Occulter:  3.5 Ro
                                    1.5 mm overocculting

                - LYA Slit:    50 um
                - OVI Slit:    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:

q01.03.16.19:17:22.lya.dat
q01.03.16.19:17:22.ovi.dat
q01.03.16.19:17:22.vld.dat

 	3) Observation of High-Latitude Coronal Hole

	Sequence: 01.01_hole4.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.
 
	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: 2001.03.17.05:21
                    end: 2001.03.17.15:12

	ONUMs =	15974 (57 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

		- Roll: 341.141 degrees (15329)
 
                - Mirror/Occulter:  3.5 Ro
                                    1.5 mm overocculting

                - LYA Slit:    50 um
                - OVI Slit:    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:
	
q01.03.17.05:19:45.lya.dat
q01.03.17.05:19:45.ovi.dat
q01.03.17.05:19:45.vld.dat