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

	Date:		06 March 2002
	-----

 	Last revision:	11 March 2002 (MU)
	--------------

	File Name: 	2002.03.06.a.log
	-----------

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

	UVCS Activity:  Load and Start High Latitude Streamer Study
	--------------	for 06 March - 07 March 2002
			Load Mini Synoptic for 07 March 2002
			Load High Latitude Streamer Study for 07 March 2002

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

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

	Command file:	02.03.06.16:33:54.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=183 degrees.

	OBS_PROG: Primary: Spectral Resolution
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Coronal Dynamics...Outflow Velocities

	OBJ:	  Streamer

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2002.03.06.17:25
                    end: 2002.03.07.03:04

	ONUMs =	17191 (6 exps)
		17192 (6 exps)
		17193 (9 exps)
		17194 (15 exps)
		17195 (15 exps)
		17196 (21 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Roll:  174.8, 175.7, 176.4, 177.5, 178.4, 179.0 Degrees 
                	(50611, 50769, 50896, 51089, 51257, 51377)

                - 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:

q02.03.06.17:18:38.lya.dat
q02.03.06.17:18:38.ovi.dat
q02.03.06.17:18:38.vld.dat
q02.03.06.17:57:47.lya.dat
q02.03.06.17:57:47.ovi.dat
q02.03.06.17:57:47.vld.dat
q02.03.06.18:31:29.lya.dat
q02.03.06.18:31:29.ovi.dat
q02.03.06.18:31:29.vld.dat
q02.03.06.19:21:42.lya.dat
q02.03.06.19:21:42.ovi.dat
q02.03.06.19:21:42.vld.dat
q02.03.06.20:44:53.lya.dat
q02.03.06.20:44:53.ovi.dat
q02.03.06.20:44:53.vld.dat
q02.03.06.23:23:02.lya.dat
q02.03.06.23:23:02.ovi.dat
q02.03.06.23:23:02.vld.dat

	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: 2002.03.07.03:32
		    end: 2002.03.07.06:59

	ONUMs = 37842 (9 exps) 
		37843 (9 exps) 
		37844 (9 exps) 
		37845 (9 exps) 
		37846 (9 exps) 
		37847 (9 exps) 
		37848 (9 exps) 
		37849 (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:

z02.03.07.03:31:16.lya.dat
z02.03.07.03:31:16.ovi.dat
z02.03.07.03:31:16.vld.dat
z02.03.07.03:57:47.lya.dat
z02.03.07.03:57:47.ovi.dat
z02.03.07.03:57:47.vld.dat
z02.03.07.04:24:18.lya.dat
z02.03.07.04:24:18.ovi.dat
z02.03.07.04:24:18.vld.dat
z02.03.07.04:50:51.lya.dat
z02.03.07.04:50:51.ovi.dat
z02.03.07.04:50:51.vld.dat
z02.03.07.05:17:35.lya.dat
z02.03.07.05:17:35.ovi.dat
z02.03.07.05:17:35.vld.dat
z02.03.07.05:43:57.lya.dat
z02.03.07.05:43:57.ovi.dat
z02.03.07.05:43:57.vld.dat
z02.03.07.06:10:32.lya.dat
z02.03.07.06:10:32.ovi.dat
z02.03.07.06:10:32.vld.dat
z02.03.07.06:36:59.lya.dat
z02.03.07.06:36:59.ovi.dat
z02.03.07.06:36:59.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=204 degrees.

	OBS_PROG: Primary: Spectral Resolution
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Coronal Dynamics...Outflow Velocities

	OBJ:	  Streamer

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2002.03.07.07:04
                    end: 2002.03.07.16:43

	ONUMs =	17197 (6 exps)
		17198 (6 exps)
		17199 (9 exps)
		17200 (15 exps)
		17201 (15 exps)
		17202 (21 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Roll:  195.8, 196.7, 197.4, 198.5, 199.4, 200.0 Degrees 
                	(54434, 54592, 54719, 54912, 55080, 55200)

                - 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:

q02.03.07.07:00:15.lya.dat
q02.03.07.07:00:15.ovi.dat
q02.03.07.07:00:15.vld.dat
q02.03.07.07:36:37.lya.dat
q02.03.07.07:36:37.ovi.dat
q02.03.07.07:36:37.vld.dat
q02.03.07.08:10:22.lya.dat
q02.03.07.08:10:22.ovi.dat
q02.03.07.08:10:22.vld.dat
q02.03.07.09:00:33.lya.dat
q02.03.07.09:00:33.ovi.dat
q02.03.07.09:00:33.vld.dat
q02.03.07.10:23:44.lya.dat
q02.03.07.10:23:44.ovi.dat
q02.03.07.10:23:44.vld.dat
q02.03.07.13:01:52.lya.dat
q02.03.07.13:01:52.ovi.dat
q02.03.07.13:01:52.vld.dat