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Generation of Magnetic Fields in Accreting Systems as a Basis of Nonthermal Mode of Energy Release

Published online by Cambridge University Press:  19 July 2016

L.A. Pustil'Nik  and
N.R. Ikhsanov
L.A. Pustil'Nik
Affiliation:
Special Astrophysical Observatory Russian Acad. of Sci. Niznij Arhyz, Stavropol Territory, 357147, Russia
N.R. Ikhsanov
Affiliation:
Special Astrophysical Observatory Russian Acad. of Sci. Niznij Arhyz, Stavropol Territory, 357147, Russia

Abstract

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Generation of the magnetic field during procces of disc accretion onto black hole or magnetize neutrin star may form current structures in a polar region. The instability and disruption of this currents must lead to effective acceleration of the particles to ultra high energy as it observe by GRO and UHE-astronomy experiments.

Keywords

accretiondynamoinstabilityaccelerationgamma astronomy
Type
5. Magnetic Field Generation in Accretion Disks
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 197 - 201
Copyright
Copyright © Kluwer 1993 

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