The natural wave modes in a pulsar magnetosphere

Details The natural wave modes in a pulsar magnetosphere The natural wave modes in a pulsar magnetosphere

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasau...3..120m&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 11th, Clayton, Victoria, Australia, May 30-June 1, 1977.) Astronomic

Astronomy and Astrophysics

Astronomy

36

Polarization Characteristics, Propagation Modes, Pulsar Magnetospheres, Pulsars, Radio Emission, High Energy Electrons, Positrons, Relativistic Particles, Stellar Atmospheres

Scientific paper

The response tensor for a relativistically streaming electron-positron
gas is used to evaluate natural wave modes propagated through it, with
attention to polarization characteristics of pulsar radio emission.
Equations are presented for both linear and nonlinear propagation modes.

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