Coherent Mechanisms of Pulsar Radio Emission

Details Coherent Mechanisms of Pulsar Radio Emission Coherent Mechanisms of Pulsar Radio Emission

1999-10-14

arxiv.org/abs/astro-ph/9910262v1

To be published in Proc. IAU Symp. 177, "Pulsar Astronomy - 2000 and Beyond", M. Kramer, N. Wex, and R. Wielebinski, eds.,ASP

Astronomy and Astrophysics

Astrophysics

4 pages, 2 Figures

Scientific paper

Relativistic plasma masers operating on the anomalous cyclotron-Cherenkov resonance and the Cherenkov-drift resonance are capable of explaining the main observational characteristics of pulsar radio emission. Both electromagnetic instabilities are due to the interaction of the fast particles from the primary beam and from the tail of the secondary pairs distribution with the normal modes of a strongly magnetized one-dimensional electron-positron plasma. In a typical pulsar both resonances occur in the outer parts of magnetosphere .

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