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The Energy Emission of Sheets in the The Pulsar Magnetosphere

Published online by Cambridge University Press:  27 September 2017

Tong Yi  and
Li Zhong Yuan
Tong Yi
Affiliation:
Beijing Normal University
Li Zhong Yuan
Affiliation:
University of Science and Technology of China

Abstract

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We present a possible emission mechanism based on the idea of current sheets in magnetohydrodynamice. The current sheets are formed close to the light cylinder due to a relativistic effect involving partly frozen-in particles. We estimate that the energy emitted by the current sheets fits the observations fairly well.

Type
Part III Magnetospheric models
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 114 - 116
Copyright
Copyright © United States Naval Observatory 1992