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Maser Theory of Pulsar Radiation

Published online by Cambridge University Press:  07 February 2017

Hong-Yee Chiu
Hong-Yee Chiu*
Affiliation:
Institute for Space Studies, Goddard Space Flight Center, NASA, New York, N.Y., U.S.A.

Abstract

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In this paper we present an account of a theory of pulsar radio emission. The emission mechanism is via a maser amplification process. This theory avoids the difficulty of coherent plasma emission, that the bandwidth of radiation must be less than 1/2 λ. The high brightness radio temperature and the insensitivity of pulsar radio flux to pulsar periods can be easily accounted for.

Type
Session 7
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 414 - 428
Copyright
Copyright © Reidel 1971 

References

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