+Mission:			*.1
++Name:				GRANAT
++SatZond:			S
++GeoHelBoth:			B
++Launch:			89/12/01
--TrajectFile:			Y
++ShortDescription:		Russian orbital observatory for gamma-astronomy
++LongDescription:		Russian high-altitude satellite for 
				gamma-astronomy purposes.  Initial orbit 
				elements are: perigee - ~8000 km, apogee - 
				~200000 km, inclination - 51 degrees, period - 
				~4 days.  Evolution of the orbit changed its 
				elements so that in October 1994 they were: 
				perigee - ~65000 km, apogee - ~150000 km, 
				inclination - 87 degrees.  Then perigee 
				becomes its slow descending.  Main axis of 
				the spacecraft is sunward directed.


++Instrument:			*.1
+++Name:			KS-18-M
+++PI:				Dr. Eugene A. Chuchkov
+++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:			chuchkov@taspd.npi.msu.su
+++ShortDescription:		Measuring of charged particles and solar x-rays during the mission 
+++LongDescription:		KS-18-M was designed as a monitor of fluxes 
				of charged particles of medium energy in 
				the interplanetary space.  Solar x-rays may be 
				also registered.  There are two almost identical 
				sensor blocks: one is sunward directed (S) and 
				the other - anti-sunward (A).  Each block contains 
				the following sensors: two gas-discharge counters 
				(C1, C2); two stand-alone SSD of Si (D1, D2) of 
				130 micron and 1000 micron of thickness respectively; 
				a SSD system T1 of two Si-sensors of 70 and 
				1000 micron thickness plus a anti-coincident cup 
				of SSDs; and a combined system T2 of SSD 
				(50 micron Si) plus windowed gas-discharge 
				counter SBT-9 plus anti-coincident cup of SSDs.  
				View angle of each SSD sensor is as wide as 
				+-25 degrees.  Spacecraft memory is used for 
				data storing; 20 minute time resolution is 
				provided for all sensors; in addition, one channel 
				from D1 and two channels from D2 may work with 
				two minute time resolution if high intensity is 
				observed.  All sensors measure flux intensity 
				continuously.  All the data are broken up to six 
				groups according to their modes of timing.
+++Publication:			*.1
++++PublicationRef:		E.A.Chuchkov, S.I.Ermakov, V.B.Kadobnov, N.N.Kontor, 
				G.P.Lyubimov, T.I.Morozova, Yu.A.Rosental, T.I.Stepina, 
				V.V.Tochilina, V.I.Tulupov, and S.A.Filippychev, 
				"First results of measurement of charged particles 
				on the GRANAT spacecraft", Pisma v astronomicheskii 
				journal, 1991, v. 17, N 2, pp. 135-140
+++Publication:			*.2
++++PublicationRef:		E.A.Chuchkov, S.I.Ermakov, N.N.Kontor, G.P.Lyubimov, 
				N.N.Pavlov, V.I.Tulupov, and B.Ya.Scherbovsky, 
				"GRANAT mission: a solar cosmic ray event in march, 
				1991", Proc. 23rd Intern. Cosmic Ray Conf. Calgary, 
				Canada, 1993, v. 3, pp. 21-24
+++Publication:			*.3
++++PublicationRef:		N.N.Pavlov, L.V.Tverskaya, B.A.Tverskoy, and E.A.Chuchkov, 
				"Variations of radiation-belt energetic particles 
				during strong magnetic storm 24-26 March, 1991",
				Geomagnetism i aeronomia, 1994, v. 34, N 6, 
				pp. 41-46
+++Publication:			*.4
++++PublicationRef:		S.I.Ermakov, N.N.Kontor, L.E.Zosim, G.P.Lyubimov, 
				N.N.Pavlov, V.I.Tulupov, T.G.Khotilovskaya, 
				E.A.Chuchkov, and S.A.Filippychev, "Solar cosmic 
				rays in 22th solar cycle as for the data from GRANAT"
				Izvestiya Russian Academy of science, 1995, v. 59, 
				N 4, pp. 24-26
+++Publication:			*.5
++++PublicationRef:		E.A.Chuchkov, S.I.Ermakov, N.N.Kontor, G.P.Lyubimov, 
				N.N.Pavlov, V.I.Tulupov, and B.Ya.Scherbovsky, 
				"Interplanetary medium diagnostics during the large
				event in march 1991 based on GRANAT records", 
				Radiation Measurements, 1996, v. 26, N 3, pp. 437-442
+++AcknowledgingTo:		TASPD SINP MSU


+++DataSet:			*.1
++++ID:				G1
++++StartDate:			89/12/02
++++StopDate:			95/12/16
++++TimeResolution:		20 minutes
++++ApproxVolume:		15 MB
++++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:		Group1: Ep=1-3,>20MeV+others; 20-min time res.; Sun-antiSun directions
++++LongDescription:		Data channels of the 1st group: protons of 
				Ep=1.2-20 MeV plus alpha-particles of Ea>3.5 MeV 
				(Ea=3.5-400 MeV) in mix, from the SSD sensor 
				of 130 micron Si; protons of Ep>6 MeV and 
				alpha-particles of Ea>25 MeV + electrons of 
				Ee>0.1 MeV and solar x-rays of Ex>7 keV, 
				all presumably are solar-originated (SCR), 
				and protons of Ep>40 MeV and alpha-particles 
				of Ea>160 Mev and electrons of Ee>4 MeV, all 
				presumably are galactic originated (GCR) from 
				a windowed gas-discharge counter of SBT-9 series; 
				and also protons of Ep>20 MeV and electrons of 
				Ee>1.2 MeV and alpha-particles of Ea>80 MeV, all 
				in mix from gas-discharge counter of SBM-20 series.  
				Both Sun and antiSun directions are presented.	
				Time resolution is 20 minutes.  All sensors 
				measure flux intensity continuously.

++++Column:			*.1
+++++LongLegend:		Ep>20MeV from Sun
+++++ShortLegend:		p>20+
+++++InternalName:		C1S(11S)
+++++Units:			1/s
+++++MinValueApprox:		8.
+++++MaxValueApprox:		6138.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>20 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.2
++++++Name:			electron
++++++Energy:			>1.2 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.3
++++++Name:			proton
++++++Energy:			>500 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		54 cm2_sr
++++++ShortDescription:		>20 MeV protons from Sun + others
++++++LongDescription:		Gas-discharge counter (SBM-20) with minimum 
				shielding for particles arriving from the Sun 
				direction so that the energy thresholds are: 
				Ep=20 MeV and Ee=1.2 MeV.  For other directions 
				the threshold is Ep=500 MeV.  All species 
				are measured in mix, although the typically 
				higher presence of >20 MeV protons above others 
				makes the channel mostly recording the data on 
				this species (in the interplanetary space).  
				Overflow may occur for count rates higher 
				than ~5e3 1/s.

++++Column:			*.2
+++++LongLegend:		Ep>6MeV of SCR + X-rays from Sun + GCR
+++++ShortLegend:		p>6+
+++++InternalName:		T2S.1(07S)
+++++Units:			1/s
+++++MinValueApprox:		3.9
+++++MaxValueApprox:		5117.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>6 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			>25 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.3
++++++Name:			electron
++++++Energy:			>0.1 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.4
++++++Name:			x-ray
++++++Energy:			>7 keV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.5
++++++Name:			proton
++++++Energy:			>40 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.6
++++++Name:			alpha-particle
++++++Energy:			>160 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.7
++++++Name:			electron
++++++Energy:			>4 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
++++++ShortDescription:		>6 MeV protons + >7 keV x-rays + >0.1 MeV electrons from Sun + GCR 
++++++LongDescription:		A component of T2 system - windowed gas-discharge 
				counter of SBT-9 series for counting (all in mix) 
				through window (view angle is +-25 degrees) from 
				the Sun-direction: protons of Ep>6 MeV + 
				alpha-particles of Ea>25 MeV + electrons of 
				Ee>0.1 MeV + x-rays of Ex>7 keV (all the mentioned 
				are mostly solar cosmic rays - SCR) and through 
				the counter's body (i.e. from all directions 
				other than from the window): protons of 
				Ep>40 MeV + alpha-particles of Ea>160 MeV + 
				electrons of Ee>4 MeV (all the mentioned 
				are assumed as galactic cosmic rays - GCR).

++++Column:			*.3
+++++LongLegend:		Ep=1.2-20MeV + Ea=3.5-400MeV from Sun
+++++ShortLegend:		p1-20+
+++++InternalName:		D1S.1(01S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		6310.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-20 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-400.
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		1.2-20 MeV protons + 3.5-400 MeV alphas from Sun
++++++LongDescription:		Thin (130 microns) SSD (Si) sensor for counting 
				protons of Ep=1.2-20 MeV and alpha-particles 
				of Ea=3.5-400 MeV (in mix) arriving from 
				the direction of Sun.  View angle is 
				+-25 degrees.  May be contaminated by electrons 
				of Ee=700-800 keV energy with ~0.01% efficiency 
				and, due to coincided pulses, by electrons of 
				Ee=300-400 keV with ~0.0015% efficiency.  
				Coincided pulses play a significant role only 
				if intensity of the relevant electron flux 
				is higher than 5e4 1/cm2_cp_s.  Overflow may 
				occur for count rates higher than ~6e3 1/s.

++++Column:			*.4
+++++LongLegend:		Ep>20MeV from antiSun
+++++ShortLegend:		p>20-
+++++InternalName:		C1A(11A)
+++++Units:			1/s
+++++MinValueApprox:		7.2
+++++MaxValueApprox:		5754.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>20 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.2
++++++Name:			electron
++++++Energy:			>1.2 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.3
++++++Name:			proton
++++++Energy:			>500 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		54 cm2_sr
++++++ShortDescription:		>20 MeV protons from antiSun + others
++++++LongDescription:		Gas-discharge counter (SBM-20) with minimum 
				shielding for particles arriving from the antiSun 
				direction so that the energy thresholds are: 
				Ep=20 MeV and Ee=1.2 MeV.  For other directions 
				the threshold is Ep=500 MeV.  All species are measured 
				in mix, although the typically higher presence 
				of >20 MeV protons above others makes the channel 
				mostly recording the data on this species (in 
				the interplanetary space).  Overflow may occur for 
				count rates higher than ~5e3 1/s.

++++Column:			*.5
+++++LongLegend:		Ep>6MeV of SCR + X-rays from antiSun + GCR
+++++ShortLegend:		p>6-
+++++InternalName:		T2A.1(07A)
+++++Units:			1/s
+++++MinValueApprox:		3.4
+++++MaxValueApprox:		5000.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>6 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			>25 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.3
++++++Name:			electron
++++++Energy:			>0.1 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.4
++++++Name:			proton
++++++Energy:			>40 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.5
++++++Name:			alpha-particle
++++++Energy:			>160 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.6
++++++Name:			electron
++++++Energy:			>4 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
++++++ShortDescription:		>6 MeV protons + >0.1 MeV electrons from Sun + GCR 
++++++LongDescription:		A component of T2 system - windowed gas-discharge 
				counter of SBT-9 series for counting (all in mix) 
				through window (view angle is +-25 degrees) from 
				the antiSun-direction: protons of Ep>6 MeV + 
				alpha-particles of Ea>25 MeV + electrons of 
				Ee>0.1 MeV (all the mentioned are assumed 
				as solar cosmic rays - SCR) and through 
				the counter's body (i.e. from all directions 
				other than from the window): protons of 
				Ep>40 MeV + alpha-particles of Ea>160 MeV + 
				electrons of Ee>4 MeV (all the mentioned 
				are assumed as galactic cosmic rays - GCR).

++++Column:			*.6
+++++LongLegend:		Ep=1.2-20MeV + Ea=3.5-400MeV from antiSun
+++++ShortLegend:		p1-20-
+++++InternalName:		D1A.1(01A)
+++++Units:			1/s
+++++MinValueApprox:		0.027
+++++MaxValueApprox:		6310.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-20 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-400.
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		1.2-20 MeV protons + 3.5-400 MeV alphas from antiSun
++++++LongDescription:		Thin (130 microns) SSD (Si) sensor for counting 
				protons of Ep=1.2-20 MeV and alpha-particles 
				of Ea=3.5-400 MeV (in mix) arriving from 
				antiSun-direction.  View angle is +-25 degrees.  
				May be contaminated by electrons of 
				Ee=700-800 keV with ~0.01% efficiency and, 
				due to coincided pulses, by electrons of 
				Ee=300-400 keV with ~0.0015% efficiency.  
				Coincided pulses play a significant role only 
				if intensity of the relevant electron flux 
				is higher than 5e4 1/cm2_cp_s.  Overflow may 
				occur for count rates higher than ~6e3 1/s.


+++DataSet:			*.2
++++ID:				G2
++++StartDate:			89/12/01
++++StopDate:			95/12/16
++++TimeResolution:		2 minutes (min)
++++ApproxVolume:		30 MB
++++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:		Group2: Ep=2-6,5-20MeV; 2- or 20-min time res.; Sun-antiSun directions
++++LongDescription:		Data channels of the 2nd group: data from two 
				~130 micron and ~1000 micron Si	stand-alone SSD 
				sensors, directed towards Sun and antiSun; only 
				one median energy-channel from each: 
				1- protons of Ep=2-6 MeV + alphas of Ea=4-7 MeV 
				and Ea=35-120 (all in mix); 
				2 - protons of Ep=5-20 MeV + alphas of 
				Ea=6-20 MeV, in mix.  Time resolution is 2 or 
				20 minutes depending on flux intensity (high 
				intensity is measured with better time 
				resolution).  All sensors measure flux 
				intensity continuously.

++++Column:			*.1
+++++LongLegend:		Ep=2.3-5.8MeV + Ea=4.1-7.5MeV + Ea=28-110MeV from Sun
+++++ShortLegend:		p2-7+
+++++InternalName:		D1S.2(02S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		6026.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			2.3-5.8 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			4.1-7.5 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.3
++++++Name:			alpha-particle
++++++Energy:			28-110 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		2.3-5.8 MeV protons + 4.1-7.5 and 28-110 MeV alphas from Sun
++++++LongDescription:		The second channel of the thin (130 microns) SSD (Si) 
				sensor.  It counts protons of Ep=2.3-5.8 MeV and 
				alpha-particles of Ea=4.1-7.5 MeV and of Ea=28-110 MeV 
				(all in mix) arriving from Sun direction.  View 
				angle is +-25 degrees.  Overflow may occur for 
				count rates higher than ~6e3 1/s.

++++Column:			*.2
+++++LongLegend:		Ep=5.1-20MeV + Ea=6.3-20MeV from Sun
+++++ShortLegend:		p5-20+
+++++InternalName:		D2S.2(05S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		776.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			5.1-20 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			6.3-20 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		5.1-20 MeV protons + 6.3-20 MeV alphas from Sun
++++++LongDescription:		The second channel of the thick (1000 microns) SSD (Si) 
				sensor.  It counts protons of Ep=5.1-20 MeV and 
				alpha-particles of Ea=6.3-20 MeV (in mix) arriving 
				from Sun direction.  View angle is +-25 degrees.
				May be contaminated by electrons with energy 
				Ee>800 keV with ~35% efficiency due to 
				coincidence of their pulses if intensity of 
				the electron flux is higher than 5e4 1/cm2_cp_s.  
				Overflow may occur for count rates higher 
				than ~7e2 1/s.

++++Column:			*.3
+++++LongLegend:		Ep=2.1-7MeV + Ea=4-6.3MeV + Ea=40-130MeV from antiSun
+++++ShortLegend:		p2-7-
+++++InternalName:		D1A.2(02A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		6026.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			2.1-7 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			4-6.3 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.3
++++++Name:			alpha-particle
++++++Energy:			40-130 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		2.1-7 MeV protons + 4-6.3 and 40-130 MeV alphas from antiSun
++++++LongDescription:		The second channel of the thin (130 microns) SSD (Si) 
				sensor.  It counts protons of Ep=2.1-7 MeV and 
				alpha-particles of Ea=4-6.3 MeV and of Ea=40-130 MeV 
				(all in mix) arriving from antiSun direction.  View 
				angle is +-25 degrees.  Overflow may occur for 
				count rates higher than ~6e3 1/s.

++++Column:			*.4
+++++LongLegend:		Ep=5.1-20MeV + Ea=6.3-20MeV from antiSun
+++++ShortLegend:		p5-20-
+++++InternalName:		D2A.2(05A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		776.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			5.1-20 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			6.3-20 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		5.1-20 MeV protons + 6.3-20 MeV alphas from antiSun
++++++LongDescription:		The second channel of the thick (1000 microns) SSD (Si) 
				sensor.  It counts protons of Ep=5.1-20 MeV and 
				alpha-particles of Ea=6.3-20 MeV (in mix) arriving 
				from antiSun direction.  View angle is +-25 degrees.
				May be contaminated by electrons with energy 
				Ee>800 keV with ~35% efficiency due to 
				coincidence of their pulses if intensity of 
				the electron flux is higher than 5e4 1/cm2_cp_s.  
				Overflow may occur for count rates higher 
				than ~7e2 1/s.


+++DataSet:			*.3
++++ID:				G3
++++StartDate:			89/12/02
++++StopDate:			94/07/11
++++TimeResolution:		20 minutes
++++ApproxVolume:		2.5 MB
++++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:		Group3: Ea=12-15MeV; 20-min time res.; Sun-antiSun directions
++++LongDescription:		Data channels of the 3rd group: data of 12-15 MeV 
				alpha-particle channel of the T1 system of three 
				SSD (Si) with a defending cup.  Both Sun and antiSun 
				directions are presented.  Time resolution is 
				20 minutes.  View angle is +-25 degrees.  All 
				sensors measure flux intensity continuously.

++++Column:			*.1
+++++LongLegend:		Ea=12-15MeV from Sun
+++++ShortLegend:		a12-15+
+++++InternalName:		T1S.8(20S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		63.1
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			12-15 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		12-15 MeV alphas from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				alpha-particles of Ea=12-15 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.

++++Column:			*.2
+++++LongLegend:		Ea=12-18MeV from antiSun
+++++ShortLegend:		a12-18-
+++++InternalName:		T1A.8(20A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		91.2
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			12-18 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		12-18 MeV alphas from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				alpha-particles of Ea=12-18 MeV arriving from 
				antiSun direction.  View angle is +-25 degrees.


+++DataSet:			*.4
++++ID:				G4
++++StartDate:			89/12/01
++++StopDate:			95/12/16
++++TimeResolution:		2 minutes (min)
++++ApproxVolume:		34.5 MB
++++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:		Group4: Ep=1.2-2.1MeV + Ea=3.5-40MeV; 2- or 20-min time res.; Sun-antiSun directions
++++LongDescription:		Data channels of the 4th group: 1.2-2.1 MeV protons 
				and 3.5-40 MeV alpha-particles (in mix) from the 1st 
				channel of the ~1000 micron SSD (Si) sensor D2.  
				Both Sun and antiSun directions are presented.  
				Time resolution is 2 or 20 minutes depending on 
				flux intensity (high intensity is measured 
				with better time resolution).  View angle is 
				+-25 degrees.  All sensors measure flux intensity 
				continuously.

++++Column:			*.1
+++++LongLegend:		Ep=1.2-2.1MeV + Ea=3.5-4.0MeV from Sun
+++++ShortLegend:		p1-2+
+++++InternalName:		D2S.1(04S)
+++++Units:			1/s
+++++MinValueApprox:		0.13
+++++MaxValueApprox:		6310.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-2.1 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-4.0 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		1.2-2.1 MeV protons + 3.5-4.0 MeV alphas from Sun
++++++LongDescription:		The first channel of the thick (1000 microns) SSD (Si) 
				sensor.  It counts protons of Ep=1.2-2.1 MeV and 
				alpha-particles of Ea=3.5-4.0 MeV (in mix) arriving 
				from the Sun direction.  View angle is +-25 degrees.  
				May be contaminated by electrons of 
				Ee>600 keV with ~80% efficiency (for Ee=1MeV 
				the efficiency is ~30%) and, due to coincided 
				pulses, by electrons of Ee=300-600 keV with 
				~64% efficiency.  Coincided pulses play 
				a significant role only if intensity of 
				the relevant electron flux is higher than 
				5e4 1/cm2_cp_s.  Overflow may occur for count 
				rates higher than ~6e3 1/s.  The channel is 
				very noisy.

++++Column:			*.2
+++++LongLegend:		Ep=1.2-2.1MeV + Ea=3.5-4.0MeV from antiSun
+++++ShortLegend:		p1-2-
+++++InternalName:		D2A.1(04A)
+++++Units:			1/s
+++++MinValueApprox:		0.25
+++++MaxValueApprox:		6310.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-2.1 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-4.0 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		1.2-2.1 MeV protons + 3.5-4.0 MeV alphas from antiSun
++++++LongDescription:		The first channel of the thick (1000 microns) SSD (Si) 
				sensor.  It counts protons of Ep=1.2-2.1 MeV and 
				alpha-particles of Ea=3.5-4.0 MeV (in mix) arriving 
				from antiSun direction.  View angle is +-25 degrees.  
				May be contaminated by electrons of 
				Ee>600 keV with ~80% efficiency (for Ee=1MeV 
				the efficiency is ~30%) and, due to coincided 
				pulses, by electrons of Ee=300-600 keV with 
				~64% efficiency.  Coincided pulses play 
				a significant role only if intensity of 
				the relevant electron flux is higher than 
				5e4 1/cm2_cp_s.  Overflow may occur for count 
				rates higher than ~6e3 1/s.  The data may be 
				noisy.


+++DataSet:			*.5
++++ID:				G5
++++StartDate:			89/12/02
++++StopDate:			95/11/30
++++TimeResolution:		20 minutes
++++ApproxVolume:		21 MB
++++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:		Group5: Ea=1-2-3-5-30-100MeV; 20-min time res.; Sun-antiSun directions
++++LongDescription:		Data channels of the 5th group: data of the T1 
				system of three SSD (Si) with a defending cup from 
				both Sun and antiSun directions.  The channels are:
				1 - 1-2 MeV protons + 3.5-4.0 alpha-particles;
				2 - 2-3 MeV protons + 4.0-6.5 alpha-particles;
				3 - 4-5 MeV protons;
				4 - 5-30 MeV protons;
				5 - 30-100 MeV protons;
				6 - 7-12 MeV alpha-particles;
				7 - >20 MeV nuclei heavier than alpha-particle.
				Time resolution is 20 minutes.  View angle is 
				+-25 degrees.  All sensors measure flux intensity 
				continuously.

++++Column:			*.1
+++++LongLegend:		Ep=1.3-2.5MeV + Ea=3.5-4MeV from Sun
+++++ShortLegend:		p1-2+
+++++InternalName:		T1S.1(13S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		6310.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.3-2.5 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-4 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		1-2 MeV protons + 3.5-4 MeV alphas from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=1.3-2.5 MeV in mix with 
				alpha-particles of Ea=3.5-4 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.  
				May be contaminated by electrons with energy 
				Ee>300 keV with ~0.06% efficiency due to 
				coincided pulses if intensity of the electron 
				flux is higher than 5e4 1/cm2_cp_s.  
				The channel may be noisy.

++++Column:			*.2
+++++LongLegend:		Ep=2.5-3.2MeV + Ea=4.0-6.5MeV from Sun
+++++ShortLegend:		p2-3+
+++++InternalName:		T1S.2(14S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		5888.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			2.5-3.2 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			4-6.5 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		2-3 MeV protons + 4-6.5 MeV alphas from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=2.5-3.2 MeV in mix with 
				alpha-particles of Ea=4-6.5 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.  
				Sometimes (seldom) shows periods of additional 
				rate (looks like normal count rate with offset).
				Overflow may occur for count rates higher 
				than ~5e3 1/s.

++++Column:			*.3
+++++LongLegend:		Ep=5.2-5.4MeV from Sun
+++++ShortLegend:		p5-6+
+++++InternalName:		T1S.3(15S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		549.5
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			5.2-5.4 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		5.2-5.4 MeV protons from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=5.2-5.4 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.
				Sometimes (seldom) shows periods of additional 
				rate (looks like normal count rate with offset).
				Overflow may occur for count rates higher 
				than ~7e2 1/s.

++++Column:			*.4
+++++LongLegend:		Ep=5.4-26MeV from Sun
+++++ShortLegend:		p6-30+
+++++InternalName:		T1S.4(16S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		758.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			5.4-26 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		5.4-26 MeV protons from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=5.4-26 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.
				May be contaminated by electrons with energy 
				Ee>1.5 MeV with ~0.3% efficiency due to 
				coincided pulses if intensity of the electron 
				flux is higher than 5e4 1/cm2_cp_s.  Overflow 
				may occur for count rates higher than ~7e2 1/s.

++++Column:			*.5
+++++LongLegend:		Ep=26-100MeV from Sun
+++++ShortLegend:		p30-100+
+++++InternalName:		T1S.5(17S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		758.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			26-100 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		26-100 MeV protons from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=26-100 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.  
				May be contaminated by electrons with energy 
				Ee>600 keV with ~70% efficiency due to 
				coincided pulses from electrons if their 
				intensity is higher than 5e4 1/cm2_cp_s.  
				Overflow may occur for count rates higher than 
				~7e2 1/s.  The channel may be noisy.

++++Column:			*.6
+++++LongLegend:		Ea=7.5-12MeV from Sun
+++++ShortLegend:		a7-12+
+++++InternalName:		T1S.6(18S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		204.2
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			7.5-12 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		7.5-12 MeV alphas from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				alpha-particles of Ea=7.5-12 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.

++++Column:			*.7
+++++LongLegend:		En>20MeV from Sun
+++++ShortLegend:		n>20+
+++++InternalName:		T1S.7(22S)
+++++Units:			1/s
+++++MinValueApprox:		0.0134
+++++MaxValueApprox:		0.0134
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			nucleon
++++++Energy:			>20 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		>20 MeV nuclei of Z>2 from Sun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It should 
				count nuclei with charge Z>2 and energy En>20 MeV 
				arriving from Sun direction.  View angle is 
				+-25 degrees.  Malfunctioned; almost does not 
				give meaningful data.

++++Column:			*.8
+++++LongLegend:		Ep=1.2-2.1MeV + Ea=3.5-4MeV from antiSun
+++++ShortLegend:		p1-2-
+++++InternalName:		T1A.1(13A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		6310.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-2.1 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-4 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		1-2 MeV protons + 3.5-4 MeV alphas from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=1.2-2.1 MeV in mix with 
				alpha-particles of Ea=6.5-12 MeV arriving from 
				antiSun direction.  View angle is +-25 degrees.
				May be contaminated by electrons with energy 
				Ee>300 keV with ~0.06% efficiency due to 
				coincided pulses if intensity of the electron 
				flux is higher than 5e4 1/cm2_cp_s.  

++++Column:			*.9
+++++LongLegend:		Ep=2.1-3.3MeV + Ea=4.0-6.5MeV from antiSun
+++++ShortLegend:		p2-3-
+++++InternalName:		T1A.2(14A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		6026.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			2.1-3.3 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			4.0-6.5 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		2-3 MeV protons + 4-6.5 MeV alphas from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=2.1-3.3 MeV in mix with 
				alpha-particles of Ea=4-6.5 MeV arriving from 
				antiSun direction.  View angle is +-25 degrees.
				Overflow may occur for count rates higher 
				than ~5e3 1/s.

++++Column:			*.10
+++++LongLegend:		Ep=4.6-5.7MeV from antiSun
+++++ShortLegend:		p5-6-
+++++InternalName:		T1A.3(15A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		758.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			4.6-5.7 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		4.6-5.7 MeV protons from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=4.6-5.7 MeV arriving from antiSun 
				direction.  View angle is +-25 degrees.
				Overflow may occur for count rates higher 
				than ~5e2 1/s.

++++Column:			*.11
+++++LongLegend:		Ep=5.7-30MeV from antiSun
+++++ShortLegend:		p6-30-
+++++InternalName:		T1A.4(16A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		758.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			5.7-30 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		5.7-30 MeV protons from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=5.7-30 MeV arriving from antiSun 
				direction.  View angle is +-25 degrees.  
				May be contaminated by electrons with energy 
				Ee>1.5 MeV with ~0.3% efficiency due to 
				coincided pulses if intensity of the electron 
				flux is higher than 5e4 1/cm2_cp_s.  Overflow 
				may occur for count rates higher than ~7e2 1/s.
				Overflow may occur for count rates higher 
				than ~7e2 1/s.

++++Column:			*.12
+++++LongLegend:		Ep=30-100MeV from antiSun
+++++ShortLegend:		p30-100-
+++++InternalName:		T1A.5(17A)
+++++Units:			1/s
+++++MinValueApprox:		0.054
+++++MaxValueApprox:		758.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			30-100 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		30-100 MeV protons from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				protons of Ep=30-100 MeV arriving from antiSun 
				direction.  View angle is +-25 degrees.  
				May be contaminated by electrons with energy 
				Ee>600 keV with ~70% efficiency due to 
				coincided pulses from electrons if their 
				intensity is higher than 5e4 1/cm2_cp_s.  
				Overflow may occur for count rates higher than 
				~7e2 1/s.  The channel may be noisy.

++++Column:			*.13
+++++LongLegend:		Ea=6.5-12MeV from antiSun
+++++ShortLegend:		a7-12-
+++++InternalName:		T1A.6(18A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		426.6
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			6.5-12 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		6.5-12 MeV alphas from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				alpha-particles of Ea=6.5-12 MeV arriving from 
				antiSun direction.  View angle is +-25 degrees.

++++Column:			*.14
+++++LongLegend:		En>20MeV from antiSun
+++++ShortLegend:		n>20-
+++++InternalName:		T1A.7(22A)
+++++Units:			1/s
+++++MinValueApprox:		0.0
+++++MaxValueApprox:		11.2
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			nucleon
++++++Energy:			>20 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		>20 MeV nuclei of Z>2 from antiSun
++++++LongDescription:		A channel of the T1 SSD (Si) system.  It counts 
				nuclei with charge Z>2 and energy En>20 MeV arriving 
				from antiSun direction.  View angle is +-25 degrees.


+++DataSet:			*.6
++++ID:				G6
++++StartDate:			89/12/02
++++StopDate:			95/12/16
++++TimeResolution:		20 minutes
++++ApproxVolume:		20.5 MB
++++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:		Group6: Ep=1-6,>20MeV+others; 20-min time res.; Sun-antiSun directions
++++LongDescription:		Data channels of the 6th group: protons of 
				Ep>20 MeV and others from the gas-discharge 
				counter C2 (SBM-20 series); alpha-particles of 
				Ea=6.3-40 MeV and Ea=20-90 from the third channels 
				of the stand-alone SSD sensors D1 and D2 of 
				130 micron and 1000 micron thickness respectively; 
				1.2-6 MeV plus alpha-particles of Ea>3.5 MeV 
				(Ea=3.5-100 MeV) in mix, from T2 combined sensor 
				system; and protons of Ep>2.4 MeV in mix with 
				alpha-particles of Ea>10 MeV and electrons of 
				Ee>0.1 MeV and solar x-rays of Ex>7 keV, all 
				presumably are the solar-originated (SCR), and protons 
				of Ep>40 MeV and alpha-particles of Ea>160 Mev and 
				electrons of Ee>4 MeV, all presumably are the galactic 
				originated (GCR) from a T2 combined sensor system 
				(based on a windowed gas-discharge counter of SBT-9 
				series).  Both Sun and antiSun directions are 
				presented.  Time resolution is 20 minutes.  All 
				sensors measure flux intensity continuously.

++++Column:			*.1
+++++LongLegend:		Ep>20MeV from Sun
+++++ShortLegend:		p>20+
+++++InternalName:		C2S(12S)
+++++Units:			1/s
+++++MinValueApprox:		7.1
+++++MaxValueApprox:		6039.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>20 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.2
++++++Name:			electron
++++++Energy:			>1.2 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.3
++++++Name:			proton
++++++Energy:			>500 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		54 cm2_sr
++++++ShortDescription:		>20 MeV protons from Sun + others
++++++LongDescription:		Gas-discharge counter (SBM-20) with minimum 
				shielding for particles arriving from the Sun 
				direction so that the energy thresholds are: 
				Ep=20 MeV and Ee=1.2 MeV.  For other directions 
				the energy threshold is Ep=500 MeV.  All species 
				are measured in mix, although the typically higher 
				presence of >20 MeV protons above others makes 
				the channel mostly recording the data on this 
				species (in the interplanetary space).  Overflow 
				may occur for count rates higher than ~5e3 1/s.

++++Column:			*.2
+++++LongLegend:		Ep>2.4MeV of SCR + X-rays from Sun + GCR
+++++ShortLegend:		p>2.4+
+++++InternalName:		T2S.3(09S)
+++++Units:			1/s
+++++MinValueApprox:		4.0
+++++MaxValueApprox:		5117.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>2.4 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			>10 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.3
++++++Name:			electron
++++++Energy:			>0.1 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.4
++++++Name:			x-ray
++++++Energy:			>7 keV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.5
++++++Name:			proton
++++++Energy:			>40 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.6
++++++Name:			alpha-particle
++++++Energy:			>160 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.7
++++++Name:			electron
++++++Energy:			>4 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
++++++ShortDescription:		>2.4 MeV protons + >7 keV x-rays + >0.1 MeV electrons from Sun + GCR 
++++++LongDescription:		A channel of the combined T2 system; it counts 
				(all in mix) on the basis of the sensor window 
				(view angle is +-25 degrees) from 
				the Sun-direction: protons of Ep>2.4 MeV + 
				alpha-particles of Ea>10 MeV + electrons of 
				Ee>0.1 MeV + x-rays of Ex>7 keV (all the mentioned 
				are assumed as solar cosmic rays - SCR) and on 
				the basis of the counter's body (i.e. from all 
				directions): protons of Ep>40 MeV + alpha-particles 
				of Ea>160 MeV + electrons of Ee>4 MeV (all 
				the mentioned are assumed as galactic cosmic 
				rays - GCR).  Overflow may occur for count 
				rates higher than ~5e3 1/s.

++++Column:			*.3
+++++LongLegend:		Ep=1.2-6MeV + Ea=3.5-100MeV from Sun
+++++ShortLegend:		p1-6+
+++++InternalName:		T2S.2(08S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		644.2
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-6 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-100 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.005 cm2_sr
++++++ShortDescription:		1.2-6 MeV protons + 3.5-100 MeV alphas from Sun
++++++LongDescription:		A channel of the T2 combined sensor system.  
				It counts protons of Ep=1.2-6 MeV in mix with 
				alpha-particles of Ea=3.5-100 MeV arriving from 
				Sun direction.  View angle is +-25 degrees.  
				Due to its very noisy behaviour, the data from 
				the channel has been decided unreliable and 
				almost completely excluded from the collection.

++++Column:			*.4
+++++LongLegend:		Ea=7.5-28MeV from Sun
+++++ShortLegend:		a7-28+
+++++InternalName:		D1S.3(03S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		407.4
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			7.5-28 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		7.5-28 MeV alphas from Sun
++++++LongDescription:		The 3rd channel of the 130 micron SSD (Si) sensor.  
				It counts alpha-particles of Ea=7.5-28 MeV arriving 
				from Sun direction.  View angle is +-25 degrees.

++++Column:			*.5
+++++LongLegend:		Ea=20-90MeV from Sun
+++++ShortLegend:		a20-90+
+++++InternalName:		D2S.3(06S)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		213.8
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			20-90 MeV
++++++DirectionWhereFrom:	Sun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		20-90 MeV alphas from Sun
++++++LongDescription:		The 3rd channel of the 1000 micron SSD (Si) sensor.  
				It counts alpha-particles of Ea=20-90 MeV arriving 
				from Sun direction.  View angle is +-25 degrees.

++++Column:			*.6
+++++LongLegend:		Ep>20MeV from antiSun
+++++ShortLegend:		p>20-
+++++InternalName:		C2A(12A)
+++++Units:			1/s
+++++MinValueApprox:		7.3
+++++MaxValueApprox:		5129.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>20 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.2
++++++Name:			electron
++++++Energy:			>1.2 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		13 cm2_sr
+++++Species:			*.3
++++++Name:			proton
++++++Energy:			>500 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		54 cm2_sr
++++++ShortDescription:		>20 MeV protons from antiSun + others
++++++LongDescription:		Gas-discharge counter (SBM-20) with minimum 
				shielding for particles arriving from the antiSun 
				direction so that the energy thresholds are: 
				Ep=20 MeV and Ee=1.2 MeV.  For other directions 
				the energy threshold is Ep=500 MeV.  All species 
				are measured in mix, although the typically higher 
				presence of >20 MeV protons above others makes 
				the channel mostly recording the data on this 
				species (in the interplanetary space).  Overflow 
				may occur for count rates higher than ~5e3 1/s.

++++Column:			*.7
+++++LongLegend:		Ep>2.4MeV of SCR + X-rays from antiSun + GCR
+++++ShortLegend:		p>2.4-
+++++InternalName:		T2A.3(09A)
+++++Units:			1/s
+++++MinValueApprox:		3.4
+++++MaxValueApprox:		5000.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			>2.4 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			>10 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.3
++++++Name:			electron
++++++Energy:			>0.1 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.4
++++++Name:			proton
++++++Energy:			>40 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.5
++++++Name:			alpha-particle
++++++Energy:			>160 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
+++++Species:			*.6
++++++Name:			electron
++++++Energy:			>4 MeV
++++++DirectionWhereFrom:	omni
++++++GeomFactor:		30 cm2_sr
++++++ShortDescription:		>2.4 MeV protons + >0.1 MeV electrons from Sun + GCR 
++++++LongDescription:		A channel of the combined T2 system; it counts 
				(all in mix) on the basis of the sensor window 
				(view angle is +-25 degrees) from 
				the Sun-direction: protons of Ep>2.4 MeV + 
				alpha-particles of Ea>10 MeV + electrons of 
				Ee>0.1 MeV (all the mentioned are assumed as 
				solar cosmic rays - SCR) and on the basis of 
				the counter's body (i.e. from all directions): 
				protons of Ep>40 MeV + alpha-particles of 
				Ea>160 MeV + electrons of Ee>4 MeV (all 
				the mentioned are assumed as galactic cosmic 
				rays - GCR).  Overflow may occur for count rates 
				higher than ~5e3 1/s.

++++Column:			*.8
+++++LongLegend:		Ep=1.2-6MeV + Ea=3.5-100MeV from antiSun
+++++ShortLegend:		p1-6-
+++++InternalName:		T2A.2(08A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		5875.
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			proton
++++++Energy:			1.2-6 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
+++++Species:			*.2
++++++Name:			alpha-particle
++++++Energy:			3.5-100 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.005 cm2_sr
++++++ShortDescription:		1.2-6 MeV protons + 3.5-100 MeV alphas from antiSun
++++++LongDescription:		A channel of the T2 combined sensor system.  It 
				counts protons of Ep=1.2-6 MeV in mix with 
				alpha-particles of Ea=3.5-100 MeV arriving from 
				antiSun direction.  View angle is +-25 degrees.  
				May be contaminated by electrons with energy 
				Ee>300 keV with ~0.04% efficiency due to 
				coincided pulses from electrons if their 
				intensity is higher than 5e4 1/cm2_cp_s.  
				Data from the channel may be noisy.  
				In 1993-1994 the channel is unreliable.

++++Column:			*.9
+++++LongLegend:		Ea=6.3-40MeV from antiSun
+++++ShortLegend:		a6-40-
+++++InternalName:		D1A.3(03A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		676.1
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			6.3-40 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		6.3-40 MeV alphas from antiSun
++++++LongDescription:		The 3rd channel of the 130 micron SSD (Si) sensor.  
				It counts alpha-particles of Ea=6.3-40 MeV arriving 
				from antiSun direction.  View angle is +-25 degrees.

++++Column:			*.10
+++++LongLegend:		Ea=20-90MeV from antiSun
+++++ShortLegend:		a20-90-
+++++InternalName:		D2A.3(06A)
+++++Units:			1/s
+++++MinValueApprox:		0.013
+++++MaxValueApprox:		186.2
+++++FillerNODATA:		-9.999E+99
+++++Species:			*.1
++++++Name:			alpha-particle
++++++Energy:			20-90 MeV
++++++DirectionWhereFrom:	antiSun
++++++GeomFactor:		0.1 cm2_sr
++++++ShortDescription:		20-90 MeV alphas from antiSun
++++++LongDescription:		The 3rd channel of  the 1000 micron SSD (Si) sensor.  
				It counts alpha-particles of Ea=20-90 MeV arriving 
				from antiSun direction.  View angle is +-25 degrees.
********************************