Formation of fast electron tails in type 2 solar bursts

Details Formation of fast electron tails in type 2 solar bursts Formation of fast electron tails in type 2 solar bursts

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976nrl..reptu....l&link_type=abstract

Interim Report Naval Research Lab., Washington, DC. Plasma Physics Div.

Physics

Plasma Physics

Electrons, Solar Flares, Solar Radio Emission, Chromosphere, Magnetic Fields, Mathematical Models, Shock Waves, Turbulence

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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