Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-11T03:55:32.667Z Has data issue: false hasContentIssue false
  • English
  • Français

Propagation of Electromagnetic Waves in Pulsar Magnetospheres

Published online by Cambridge University Press:  12 April 2016

Ya. Istomin
Ya. Istomin*
Affiliation:
Lebedev Physical Institute, Leninsky Prosp. 53, Moscow, 117924, Russia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have developed a numerical code for the propagation of different electromagnetic modes in a pulsar magnetosphere filled by a relativistic, streaming electron-positron plasma in a strong, curved magnetic field. We determine the trajectories, limiting polarization and damping of the waves leaving the magnetosphere.

Type
Chapter Two Pulsars: Their Scattering and Intrinsic Properties
Information
International Astronomical Union Colloquium , Volume 182: Sources and Scintillations: Refraction and Scattering in Radio Astronomy , 2001 , pp. 77 - 80
Copyright
Copyright © Kluwer 2001

References

Beskin, V.S., Gurevich, A.V. and Istomin, Ya.N.: 1993, Physics of the Pulsar Magnetosphere, Cambridge University Press.Google Scholar
Hardee, P.E. and Rose, W.K.: 1976, A mechanism for the production of pulsar radio emission, Astrophys. J. 210, 533–538.Google Scholar
Lyne, A.G. and Smith, F.G.: 1990, Pulsar Astronomy, Cambridge University Press.Google Scholar
Smirnov, A.P. and Harvey, R.W.: 1995, Calculation of the current drive in DIII-D with GENRAY ray tracing code, Bulletin of the American physical Society 40, 1837–1842.Google Scholar
Taylor, J.H. and Stinebring, D.R.: 1986, Recent progress in the understanding of pulsars, Annu. Rev. Astron. Astrophys. 24, 285–328.Google Scholar