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The Pulsar Magnetosphere – A Stationary Self-Consistent Solution

Published online by Cambridge University Press:  12 April 2016

Bernhard Hofmann ,
Heinz Herold  and
Hanns Ruder
Bernhard Hofmann
Affiliation:
Institut für Astronomie und Astrophysik, Abteilung Theoretische Astrophysik, Universität Tübingen
Heinz Herold
Affiliation:
Institut für Astronomie und Astrophysik, Abteilung Theoretische Astrophysik, Universität Tübingen
Hanns Ruder
Affiliation:
Institut für Astronomie und Astrophysik, Abteilung Theoretische Astrophysik, Universität Tübingen

Abstract

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Using fundamental equations of physics we determine with a simple model a globally self-consistent state of a pulsar magnetosphere.

Type
Part 6 Winds and the ISM
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 429 - 430
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Finkbeiner, B. et al. 1989, A&A, 225, 479 Google Scholar
Goldreich, P., Julian, W.H. 1969, ApJ, 157, 869 CrossRefGoogle Scholar
Herold, H. et al. 1993, In: Isolated Pulsars, Proc. Los Alamos Workshop, Taos NM, Cambridge University Press, 208 Google Scholar