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Towards a Pulsar Magnetosphere Model — Physical Principles
Published online by Cambridge University Press: 25 April 2016
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I shall outline the physical principles on which I believe pulsar magnetosphere models should be based. The principles follow from the equations of continuity and motion for each species and the two sourceless members of Maxwell’s set of equations, together with the steady-rotation constraint and boundary conditions at the stellar surface.
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- Copyright © Astronomical Society of Australia 1981