Generation of radio emission in a pulsar magnetosphere

Details Generation of radio emission in a pulsar magnetosphere Generation of radio emission in a pulsar magnetosphere

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..224b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, March 1988, p. 224-232. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Neutron Stars, Pulsar Magnetospheres, Pulsars, Radio Emission, Relativistic Plasmas, Plasma-Electromagnetic Interaction, Wave Interaction

Scientific paper

It is shown that nonlinear interaction of the waves excited in a relativistic plasma flowing along curved field lines in the magnetosphere of a neutron star leads to an effective energy conversion into transverse oscillations capable of leaving the magnetosphere. The emissivity, spectrum, frequency band and the directivity pattern of generated radiation are determined. A good agreement between the theory and observational data is demonstrated.

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