Plasma Masers in Radio Pulsars

Details Plasma Masers in Radio Pulsars Plasma Masers in Radio Pulsars

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ptep.proc..376l&link_type=abstract

Plasma Turbulence and Energetic Particles in Astrophysics, Proceedings of the International Conference, Cracow (Poland), 5-10 Se

Astronomy and Astrophysics

Astrophysics

Scientific paper

Relativistic plasma masers operating on the anomalous cyclotron-Cherenkov resonance ω-kparallel vparallel + ωB/γres=0 and the Cherenkov-drift resonance ω-kparallel vparallel-kx ud =0, are capable of explaining the main observational characteristics of pulsar radio emission. Both electromagnetic instabilities are due to the interaction of the fast particles of the primary beam and from the tail of the 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 at rres ~109 cm.

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