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

	Date:		01 March 2002
	-----

 	Last revision:	03 March 2002 (Wu)
	--------------

	File Name: 	2002.03.02.a.log
	-----------

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

	UVCS Activity:  High Latitude Streamer Study for 02 - 03 March 2002
	--------------	Mini Synoptic for 03 March 2002
			High Latitude Streamer Study for 03 March 2002

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

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

	Command file:	02.03.01.14:57:57.cmd.log

	Activity:
	---------

        1) High Latitude Streamer Study

	Sequence: 01.03_streamer1.tcl

	SCI_SPEC: Measurement of radial and latitudinal properties of high
                  latitude streamers.  These properties will be compared with
                  those of solar minimum equatorial streamers.
                
                  Roll positions are VL-corrected for PA=190 degrees.

	OBS_PROG: Primary: Spectral Resolution
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Coronal Dynamics...Outflow Velocities

	OBJ:	  Streamer

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2002.03.02.16:18
                    end: 2002.03.03.01:56

	ONUMs =	17171 (6 exps)
		17172 (6 exps)
		17173 (9 exps)
		17174 (15 exps)
		17175 (15 exps)
		17176 (21 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Roll:  182.0, 183.0, 183.5, 184.5, 185.5, 186.0 Degrees 
                	(51912, 52064, 52187, 52375, 52540, 52658)
 
                - Mirror/Occulter:  1.7, 1.9, 2.1, 2.5, 3.0, 3.5 Ro
                                    1.5 mm overocculting

                - LYA Slit:    50 um
                - OVI Slit:    75 um 

                - LYA GRTPOS: 128000
                - OVI GRTPOS: 184200

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_Syn_184 in slot 2

	Fits Files:

q02.03.02.16:02:43.lya.dat
q02.03.02.16:02:43.ovi.dat
q02.03.02.16:02:43.vld.dat
q02.03.02.16:50:04.lya.dat
q02.03.02.16:50:04.ovi.dat
q02.03.02.16:50:04.vld.dat
q02.03.02.17:23:49.lya.dat
q02.03.02.17:23:49.ovi.dat
q02.03.02.17:23:49.vld.dat
q02.03.02.18:14:00.lya.dat
q02.03.02.18:14:00.ovi.dat
q02.03.02.18:14:00.vld.dat
q02.03.02.19:37:11.lya.dat
q02.03.02.19:37:11.ovi.dat
q02.03.02.19:37:11.vld.dat

GAP between 03/02/02|20:17:26(10737) and 03/02/02|20:18:31(10846)

q02.03.02.22:15:19.lya.dat
q02.03.02.22:15:19.ovi.dat
q02.03.02.22:15:19.vld.dat

GAP between 03/03/02|01:18:16( 6871) and 03/03/02|01:24:01( 7427)

	2) 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: 2002.03.03.02:28
		    end: 2002.03.03.05:52

	ONUMs = 37800 (8 exps) 
		37801 (9 exps) 
		37802 (9 exps) 
		37803 (9 exps) 
		37804 (9 exps) 
		37805 (9 exps) 
		37806 (9 exps) 
		37807 (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: 184200

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_Syn_184 in slot 2

	Fits Files:

z02.03.03.02:24:43.lya.dat
z02.03.03.02:24:43.ovi.dat
z02.03.03.02:24:43.vld.dat
z02.03.03.02:51:12.lya.dat
z02.03.03.02:51:12.ovi.dat
z02.03.03.02:51:12.vld.dat
z02.03.03.03:17:34.lya.dat
z02.03.03.03:17:34.ovi.dat
z02.03.03.03:17:34.vld.dat
z02.03.03.03:44:09.lya.dat
z02.03.03.03:44:09.ovi.dat
z02.03.03.03:44:09.vld.dat
z02.03.03.04:10:38.lya.dat
z02.03.03.04:10:38.ovi.dat
z02.03.03.04:10:38.vld.dat
z02.03.03.04:37:07.lya.dat
z02.03.03.04:37:07.ovi.dat
z02.03.03.04:37:07.vld.dat
z02.03.03.05:03:50.lya.dat
z02.03.03.05:03:50.ovi.dat
z02.03.03.05:03:50.vld.dat
z02.03.03.05:30:17.lya.dat
z02.03.03.05:30:17.ovi.dat
z02.03.03.05:30:17.vld.dat

        3) High Latitude Streamer Study

	Sequence: 01.03_streamer1.tcl

	SCI_SPEC: Measurement of radial and latitudinal properties of high
                  latitude streamers.  These properties will be compared with
                  those of solar minimum equatorial streamers.
                
                  Roll positions are VL-corrected for PA=175 degrees.

	OBS_PROG: Primary: Spectral Resolution
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Coronal Dynamics...Outflow Velocities

	OBJ:	  Streamer

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2002.03.03.06:00
                    end: 2002.03.03.15:39

	ONUMs =	17177 (6 exps)
		17178 (6 exps)
		17179 (9 exps)
		17180 (15 exps)
		17181 (15 exps)
		17182 (21 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Roll:  167.0, 168.0, 168.5, 169.5, 170.5, 171.0 Degrees 
                	(49181, 49333, 49457, 49644, 49809, 49927)
 
                - Mirror/Occulter:  1.7, 1.9, 2.1, 2.5, 3.0, 3.5 Ro
                                    1.5 mm overocculting

                - LYA Slit:    50 um
                - OVI Slit:    75 um 

                - LYA GRTPOS: 128000
                - OVI GRTPOS: 184200

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_Syn_184 in slot 2

	Fits Files:

q02.03.03.05:53:38.lya.dat
q02.03.03.05:53:38.ovi.dat
q02.03.03.05:53:38.vld.dat
q02.03.03.06:32:40.lya.dat
q02.03.03.06:32:40.ovi.dat
q02.03.03.06:32:40.vld.dat
q02.03.03.07:06:24.lya.dat
q02.03.03.07:06:24.ovi.dat
q02.03.03.07:06:24.vld.dat
q02.03.03.07:56:38.lya.dat
q02.03.03.07:56:38.ovi.dat
q02.03.03.07:56:38.vld.dat
q02.03.03.09:19:49.lya.dat
q02.03.03.09:19:49.ovi.dat
q02.03.03.09:19:49.vld.dat
q02.03.03.11:57:55.lya.dat
q02.03.03.11:57:55.ovi.dat
q02.03.03.11:57:55.vld.dat