+Mission:			*.1
++Name:				PHOBOS-2
++SatZond:			Z
++GeoHelBoth:			H
++Launch:			88/07/12
--TrajectFile:			N
++ShortDescription:		Russian expedition to Mars-Phobos
++LongDescription:		Russian space zond for exploration of Phobos, 
				a natural satellite of Mars.  A couple of zonds, 
				PHOBOS-1 and PHOBOS-2 have been launched in a 5-day 
				interval.  Main axis of the spacecraft is sunward 
				directed with precision of ~10 degrees.


++Instrument:			*.1
+++Name:			VFS-F
+++PI:				Dr. Vladimir I. Tulupov
+++ResearchGroup:		Heliosphere Physics Laboratory
+++Lab:				Theoretical and Applied Space Physics Division
+++Institution:			Skobeltsyn Institute of Nuclear Physics, 
				Moscow State University
+++Address:			Vorobyovy Gory, Moscow, 119899, Russia
+++Fax:				+7-095-939-2488 (fax/voice)
+++Phone:			+7-095-939-5097
+++E-mail:			tulupov@taspd.npi.msu.su
+++ShortDescription:		Measuring of >30 MeV proton flux during the mission
+++LongDescription:		VFS-F has been designed as a very simple monitor 
				of charged particles in the interplanetary space.  
				There are three closely placed and mutually 
				perpendicularly oriented gas-discharge counters 
				of the SBM-20 series.  Spacecraft memory is used for 
				data storing; time resolution is about one hour.  
				All sensors measure flux intensity continuously.  
				Since all counters demonstrate very similar results 
				only the data from one detector is presented.
+++Publication:			
+++AcknowledgingTo:		TASPD SINP MSU


+++DataSet:			*.1
++++ID:				F1
++++StartDate:			88/07/13
++++StopDate:			89/03/23
++++TimeResolution:		1 hour
++++ApproxVolume:		90 kB
++++DataSupportContact:		Dr. Nickolay N. Pavlov
++++Institution:		Skobeltsyn Institute of Nuclear Physics, 
				Moscow State University
++++Address:			Vorobyovy Gory, Moscow, 119899, Russia
++++Fax:			+7-095-939-2488 (fax/voice)
++++Phone:			+7-095-939-5928
++++E-mail:			nnpavlov@taspd.npi.msu.su
++++ShortDescription:		Ep>30MeV; 1-hour time res.; normal to Sun direction
++++LongDescription:		Data on protons of Ep>30 MeV energy (gas-discharge 
				counter) from the direction perpendicular to the line 
				Sun-spacecraft.  Time resolution is 20 minutes.  
				All sensors measure flux intensity continuously.
++++Column:			*.1
+++++LongLegend:		Ep>30MeV from normal-to-Sun direction
+++++ShortLegend:		p>30n
+++++InternalName:		D1
+++++Units:			1/s
+++++MinValueApprox:		15.1
+++++MaxValueApprox:		134.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>30 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.2
++++++Name:			electron
++++++Energy:			>2 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.3
++++++Name:			proton
++++++Energy:			>500 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		54 cm2_sr
++++++ShortDescription:		>30 MeV protons from normal-to-Sun + others
++++++LongDescription:		Gas-discharge counter (SBM-20) with minimum 
				shielding of ~1 g/cm2 Al for particles arriving 
				from the direction perpendicular to the line 
				Sun-spacecraft; the thresholds are: Ep=30 MeV 
				and Ee=2 MeV.  For other directions the threshold 
				is Ep=500 MeV.  All species are measured in mix, 
				although the typically higher presence of >30 MeV 
				protons above others makes the channel mostly 
				recording the data on this species.  Spacecraft 
				is spinned with a period of 0.2-1 hour.
********************************