Formation of fast electron tails in type II solar bursts

Details Formation of fast electron tails in type II solar bursts Formation of fast electron tails in type II solar bursts

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...212..886l&link_type=abstract

Astrophysical Journal, Part 1, vol. 212, Mar. 15, 1977, p. 886-890. Research supported by the U.S. Defense Nuclear Agency.

Astronomy and Astrophysics

Astrophysics

24

Shock Fronts, Solar Corona, Solar Electrons, Solar Flares, Type 2 Bursts, Astronomical Models, Current Density, Electron Diffusion, Fourier Transformation, Ionic Diffusion, Stochastic Processes

Scientific paper

It is shown that low-frequency turbulence, due to the modified
two-stream instability excited in the front of a collisionless shock,
can accelerate electrons to very large energies in the shock wake. This
mechanism can produce nonthermal tails of the sort required to explain
type II solar bursts, contrary to previous conclusions.

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