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Pulsar Electrodynamics

Published online by Cambridge University Press:  14 August 2015

Houshang Ardavan
Houshang Ardavan*
Affiliation:
University of Northern Iran, Babolsar, Iran Institute of Astronomy, Cambridge, England

Extract

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This paper briefly discusses the salient features of quasi-steady electrodynamics; that is to say it considers certain general properties of Maxwell's equations and their solutions when these equations are subjected to the constraint where ω is a constant angular frequency, ⊘ and t are the azimuthal angle and time, and the operators are applied only to quantities which are scalars or the cylindrical components of a vector (Mestel 1971).

Type
I. Electrodynamics of the Pulsar Magnetosphere and Wave Zone
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 31 - 33
Copyright
Copyright © Reidel 1981 

References

Ardavan, H.: 1980a, Astrophys. J., submitted.Google Scholar
Ardavan, H.: 1980b, Nature, submitted.Google Scholar
Mestel, L.: 1971, Nature Phys. Sci. 223, p. 149.Google Scholar