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Radiation Damping and the Two Mode Behavior in Pulsars

Published online by Cambridge University Press:  27 September 2017

C. -I. Björnsson
C. -I. Björnsson*
Affiliation:
Stockholm Observatory

Abstract

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It is argued that both observations and theory indicate that radiation damping plays an important rôle in pulsar emission. The two-mode behavior as well as the observed value of the brightness temperature can both be understood as a result of radiation damping. In this context, a possible cause for the enhanced depolarization in the wings of pulsar profiles is discussed.

Type
Part IX Polarization phenomena
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 391 - 393
Copyright
Copyright © United States Naval Observatory 1992