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20.01.200506.00.

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:- 950-970 - 83. 31,6 8,5 - >1 ( 25, 5 .) - (1.0 3.0)0. ( - ) 135 , 435 - : 7 ; - 7 2007

Solar flare January, 20, 2005

UV (300- 400 nm) spectra of atmospheric emissions What is the role of energetic particles?

-, , 2005.UV flashes (~ msec) spatial distributionUp to 10 MJ!

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- 2

: (TLE Transient Light Events), , -

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2011 - 2014.

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AtmosphereThe Earth's surfaceTUS field of visionUV-collectorSatelliteSecondaryelectronsPrimary particle~10*19 - 10 *20 Fluorescent emissionCherenkov emissionNmax

Experimental facility TUS on-board LomonosovTotal mirror area 1,68 m2Altitude H=550kmCovered surface 5000 km2Active life period 5 years Lower energy limit - 5.1019 eV

Lomonosov 2. Studies of transient phenomena in the Earth's upper atmosphereScientific missionsTUS facility will be used for transients studies within UV-range

Lomonosov 3. Simultaneous studies of gamma-bursts by means of optic cameras and gamma-detectorsCentral engine ?Prompt radiationScientific missions

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TUS MissionMain goal is detection of Extreme Energy Cosmic Rays. For this goala large mirror-concentrator is needed. Pixels cover 4000 km2 of the atmosphere (orbit height 450 km). For detection of TLE a pinhole camera is incorporated.Satellite scientific payload:mass 60 kg, electric power 60 Wt, orientation to nadir 3mirror-concentrator area 2 m2

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BDRG + SHOKX-ray, Gamma measurements, Optical cameras for GRBs Trigger formation for GRB. measurementsParameters:Total mass: 305 kg;Power cons: up to 70 WTelemetry: up to 9 Gb/daySINP/ MSU, GAISh/MSU

UFFO Ultra Fast Flash Observatory UFFO Burst Alert & Trigger TelescopeGoals: -GRB observations in UV, Gamma & X-ray, trigger formation. EWHA Womans Univ. (Korea), Danmark; UCB,USA; Norway; Spain; SINP /MSUParameters:Dimensions: 600600200 mm; Power cons: 20 W; Mass: 203 ;Telemetry: 100 Mb/day

DEPRONGoals:- Charged particles fluxes measurements; - Radiation monitoring .SINP/MSUParameters:Dimensions: 22015070 mm;Mass: 45 kg; Power cons: 5 W;Telemetry: 10 Mb/day

ELFIN-L Goals: - Magnetic field measurements;- Charged particles fluxes measurementsUCLA, USA; SINP/MSU, RussiaParameters:Dimensions:200100720 mm. Mass: 31 kg;Telemetry: 10 Mb/day; Power cons: 5 W

BIInformation UnitBI tusks:- control of scientific payload power;- control of scientific payload instruments operation;- On-line data processing;- Formation of telemetric frame of scientific data;- GRB trigger generation and alert of event

Collaboration : MSUparameters:power: 303 W; mass: 102 kg;informativity: 40 b/day

1012 1015 Z =1 30; 165 ; 265 ; 120 ; 2011-2012 ; 5

500500270 : - 4 ( ); - 6 ( , ); - 6 - ( )

Nucleon experiment intended on study of very-high energy cosmic ray composition at the knee region ( < 1 PeV). Instrument is planned to be installed as the by-pass payload on the serial spacecraft.

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-1 (-2) NaI(Tl)/CsI(Tl)/ , : X- 0.01-2.0 M, 0.2-10.0 M ~200 c2 ~200 c2 (. ) ( ~800 cm2) 0.1 1.0 ~510-9 /2 ~10-1 ./c2

- < 7 ;

300(270(200 ;

-3 NaI(Tl)/CsI(Tl)/ , : 0.1-10.0 M,1.0-100.0 M. ~2 c2 ~2 c2 1.0 1.0 ~10 ./c2~10 ./c2

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250(250(250 ;

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T -T :

: 300-400 : 0.4o. : 7.5o. : 4000. : 64. : 100 . : 105.

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: -1 - 300-400 nm -2 () - 630-800 nm : 7.5o. : 100 . : 106.

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magnetic and electric field component meters

DOSTEL

Dosimetry unit

Technical parameters

Mass - < 1 kg;

sizes 100(80(70 mm;

power expenditure at 28 V no more 1 W.

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THE INTERHELIOSOND PROJECT (THE INTERSONG AND THE SKI-4 DEVICES) Studing neutral component of solar flare radiations (neutrons, x-ray and gammas) near to the Sun on a distances up to 25 solar radiiStuding fluxes of an electrons, protons and alpha - particles

The INTERSONG device allows to detect: neutrons ( 0.01 - 5 MeV, 20 - 100 MeV ) x-ray radiation ( 0.03 - 0.1 MeV ) gamma - quantums ( 0.1 - 20 MeV )

The SKI-4 device allows to detect:

protons ( 1.6 - 24 MeV, 80 - 200 MeV ) electrons ( 0,04 - 2,5 MeV ) alpha - particles ( 2.5 - 13 MeV / nucl )

Terms of realization of the project 2014 - 2015 years

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2005

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- 2004, 2005, 2006, 2007

5- , 20-25 2008.

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UNIVERSAT-2009University Satellites in Space EducationInternational ConferenceMay 25-31, 2009Moscow State University,Moscow, Russiacosmos.msu.ru/universat2009

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