Hydromagnetic Wave Propagation near Ion Cyclotron Resonance

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Wave dispersion near cyclotron resonance in pulsar plasmas.

In a standard pulsar model, the radio emission is produced in the relativistic, strongly magnetized electron-positron plasma in the polar-cap region of the magnetosphere. Waves are generated well below the cyclotron frequency and must propagate through the cyclotron resonance region where they are affected by the resonance. Wave dispersion near the cyclotron resonance is discussed in the formal...

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ژورنال

عنوان ژورنال: Physics of Fluids

سال: 1963

ISSN: 0031-9171

DOI: 10.1063/1.1706848