+Mission:			*.1
++Name:				ZOND-3
++SatZond:			Z
++GeoHelBoth:			H
++Launch:			65/07/18
--TrajectFile:			Y
++ShortDescription:		The 3rd Russian space probe of the ZOND series
++LongDescription:		Russian space zond for exploration of 
				the interplanetary space at the heliocentric 
				distances larger than 1 AU.  Main axis of 
				the spacecraft is sunward directed; spinning 
				period is about 9.6 minutes.


++Instrument:			*.1
+++Name:			KS-18
+++PI:				Dr. German P. Lyubimov
+++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:			lyubimov@taspd.npi.msu.su
+++ShortDescription:		Measuring of proton fluxes during the flight
+++LongDescription:		KS-18 has been designed as a monitor of charged 
				particles of medium energies travelling in 
				the interplanetary space.  There are two sensors: 
				a gas-discharge counter D1 of the STS-5 series and 
				a SSD (Si) detector D2 of 35 micron thickness.  
				Spacecraft memory is used for data storing; 
				time resolution is about four hours.  All sensors 
				measure flux intensity continuously.
+++Publication:			*.1
++++PublicationRef:		G.P.Lyubimov, "Measurement of cosmic irradiation 
				intensity on space probes ZOND-1, ZOND-2, ZOND-3, 
				LUNA-5, LUNA-6", (in Russian), Izvestiya Academy 
				of science USSR, 1966, v. 30, N. 11, Phys. ser., 
				pp. 1815-1817
+++Publication:			*.2
++++PublicationRef:		S.N.Vernov, A.E.Chudakov, P.V.Vakulov, Yu.I.Logachov, 
				G.P.Lyubimov, and N.V.Pereslegina, "Cosmic ray variations 
				as is from the data of ZOND-3 and VENERA-2 spacecraft", 
				(in Russian), Doklady Akademii Nauk USSR, 1966, v. 171, 
				N. 3, pp. 583-586
+++Publication:			*.3
++++PublicationRef:		S.N.Vernov, A.E.Chudakov, P.V.Vakulov, Yu.I.Logachov, 
				G.P.Lyubimov, A.G.Nikolaev, and N.V.Pereslegina,
				"Measurements of solar-born protons of 1-5 MeV energy 
				on VENERA-2, VENERA-3 and ZOND-3 spacecraft", 
				(in Russian),  Doklady Akademii Nauk USSR, 1966, v. 171, 
				N. 4, Geophysics, pp. 847-850
+++AcknowledgingTo:		TASPD SINP MSU


+++DataSet:			*.1
++++ID:				Z3
++++StartDate:			65/07/19
++++StopDate:			66/01/21
++++TimeResolution:		4 hours
++++ApproxVolume:		15 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=1-5,>30MeV; 4-hour time res.; Sun&SunPerp. directions
++++LongDescription:		Data on protons of Ep>30 MeV energy from Sun 
				(gas-discharge counter) and protons of Ep=1-5 MeV 
				energy arriving from the direction perpendicular 
				to the line Sun-spacecraft (stand-alone SSD sensor 
				of 35 micron Si).  Time resolution is 4 hours.  All 
				sensors measure flux intensity continuously.
++++Column:			*.1
+++++LongLegend:		Ep>30MeV from Sun
+++++ShortLegend:		p>30+
+++++InternalName:		D1
+++++Units:			1/s
+++++MinValueApprox:		24.5
+++++MaxValueApprox:		30.5
+++++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 Sun + others
++++++LongDescription:		Gas-discharge counter (STS-5) with minimum 
				shielding of ~1 g/cm2 Al for particles arriving 
				from the Sun direction so that 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.

++++Column:			*.2
+++++LongLegend:		Ep=1-5MeV from Sun-perp dir
+++++ShortLegend:		p1-5n
+++++InternalName:		D2
+++++Units:			1/s
+++++MinValueApprox:		0.055
+++++MaxValueApprox:		1.8
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1-5 MeV
++++++DirectionWhereFrom:	SunPerp
++++++GeomFactor:		0.2 cm2_sr
++++++ShortDescription:		1-5 MeV protons from Sun-perp dir
++++++LongDescription:		~35 microns of Si sensor for counting protons of 
				Ep=1-5 MeV arriving from the Sun perpendicular 
				direction with spacecraft spinnig velocity of 
				~6 rot/hour.  View angle is +-45 degrees.
********************************