Physics of pulsar magnetospheres

V.S. Beskin, A.V. Gurevich, Ya.N. Istomin
Lebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation

A self-consistent model of the magnetosphere of a pulsar is constructed. This model is based on a successive solution of the equations describing global properties of the magnetosphere and on a comparison of the basic predictions of the developed theory and observational data.

PACS: 97.60.Gb, 97.10.Ex, 97.10.Ld, 95.30.Qd, 98.70.Dk (all)
DOI: 10.1070/PU1986v029n10ABEH003528
URL: https://ufn.ru/en/articles/1986/10/c/
Citation: Beskin V S, Gurevich A V, Istomin Ya N "Physics of pulsar magnetospheres" Sov. Phys. Usp. 29 946–970 (1986)

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Оригинал: Бескин В С, Гуревич А В, Истомин Я Н «Физика магнитосферы пульсара» УФН 150 257–298 (1986); DOI: 10.3367/UFNr.0150.198610c.0257

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