National Science Library of Georgia

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Physics of the pulsar magnetosphere / V.S. Beskin, A.V. Gurevich & Ya. N. Istomin ; translated from Russian by M.V. Tsaplina.

By: Contributor(s): Material type: TextTextLanguage: English Original language: Russian Publisher: Cambridge : Cambridge University Press, 1993Description: 1 online resource (xxiii, 408 pages) : digital, PDF file(s)Content type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 9780511564673 (ebook)
Subject(s): Additional physical formats: Print version: : No titleDDC classification:
  • 523.8/874 20
LOC classification:
  • QB843.P8 B47 1993
Online resources: Summary: This book presents the theory of the electrodynamic phenomena which occur in the magnetosphere of a pulsar. It also provides a clear picture of the formation and evolution of neutron stars. The authors address the basic physical processes of electron-positron plasma production, the generation of electric fields and currents, and the emission of radio waves and gamma rays. The book also reviews observational data, and devotes a complete chapter to a detailed comparison of this data with accepted theory and with some recent theoretical predictions. Tables containing the values of the physical parameters of all observed radio pulsars are also provided. The book is illustrated throughout and is fully referenced. Graduate students and researchers in astrophysics and plasma physics working in the field of radio pulsars will find this book of great value.
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Title from publisher's bibliographic system (viewed on 05 Oct 2015).

This book presents the theory of the electrodynamic phenomena which occur in the magnetosphere of a pulsar. It also provides a clear picture of the formation and evolution of neutron stars. The authors address the basic physical processes of electron-positron plasma production, the generation of electric fields and currents, and the emission of radio waves and gamma rays. The book also reviews observational data, and devotes a complete chapter to a detailed comparison of this data with accepted theory and with some recent theoretical predictions. Tables containing the values of the physical parameters of all observed radio pulsars are also provided. The book is illustrated throughout and is fully referenced. Graduate students and researchers in astrophysics and plasma physics working in the field of radio pulsars will find this book of great value.

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