Electron beam formation and stability

Details Electron beam formation and stability Electron beam formation and stability

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130..201m&link_type=abstract

(Committee of European Radio Astronomers, SNSF, URSI, et al., Workshop on Particle Beams in the Solar Atmosphere, Braunwald, Swi

Physics

37

Electron Beams, Interplanetary Medium, Plasma-Particle Interactions, Solar Radio Emission, Background Radiation, Electron Distribution, Electrostatic Waves, Magnetohydrodynamic Turbulence, Wave Interaction, Wave Propagation

Scientific paper

The dynamics of fast electrons streaming from the sun through the interplanetary plasma is reviewed from the kinetic viewpoint. How can a bump appear on the tail of the electron distribution function? How can the beam survive the beam-plasma instability and propagate up to 1 AU as observed? These two questions are discussed in light of the recent data acquired in situ on electron distributions, Langmuir waves, ion acoustic waves, and background density fluctuations.

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