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Some Peculiaritiers of the Relativistic Electron-Positron Plasma Dynamics in the Pulsar Magnetosphere

Published online by Cambridge University Press:  12 April 2016

Irakli S. Nanobashvili
Irakli S. Nanobashvili*
Affiliation:
Abastumani Astrophysical Observatory, Georgian Academy of Sciences, A. Kazbegi Ave.2a, GE-380060 Tbilisi, Georgia

Abstract

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Some aspects of relativistic electron-positron plasma dynamics in the pulsar magnetosphere are discussed. Namely it is shown that if we take into account the influence of centrifugal force, this gives rise to the new dynamical effect of plasma particle radial braking in the pulsar magnetosphere. Also the possibility of aperiodic instability development in the pulsar magnetosphere is demonstrated. The mechanism for the toroidal magnetic field generation is proposed. Besides, the possible changes of the pulsar magnetosphere structure caused by above mentioned processes is considered.

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 465 - 468
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Chedia, O.V., Kahniashvili, T.A., Machabeli, G.Z. & Nanobashvili, I.S. 1996, Ap&SS, 239, 57.Google Scholar
Nanobashvili, I.S. 1997, Czech. J. Phys., 47, 217.Google Scholar
Kahniashvili, T.A., Machabeli, G.Z., & Nanobashvili, I.S. 1997, Phys. Plas., 4, 1132.CrossRefGoogle Scholar