Radiative or two-stream instability as a source for pulsar radio emission

• 1 March 1983
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 266, 201-214
• https://doi.org/10.1086/160770

Abstract

Keywords

• MAGNETOHYDRODYNAMIC FLOW
• PARTICLE ACCELERATION
• PULSARS
• RADIO STARS
• RELATIVISTIC PARTICLES
• ELECTROMAGNETIC RADIATION
• MAGNETOHYDRODYNAMIC STABILITY
• MAGNETOSPHERES
• POLAR CAPS
• RADIO EMISSION
• STELLAR MODELS