Shock drift acceleration and type II solar radio bursts

Details Shock drift acceleration and type II solar radio bursts Shock drift acceleration and type II solar radio bursts

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasau..11...21s&link_type=abstract

Astronomical Society of Australia, Proceedings, vol. 11, no. 1, p. 21-24

Astronomy and Astrophysics

Astronomy

4

Electric Fields, Electron Acceleration, Plasma Drift, Shock Waves, Solar Magnetic Field, Solar Radio Bursts, Particle Acceleration, Radio Astronomy, Radio Emission, Shock Fronts, Wave Propagation

Scientific paper

Shock drift acceleration of the electrons which produce herringbone structure in type II bursts is considered. A non-coplanar component of the magnetic field within the schock front and an electric field across the shock are taken into account. A quantitative difficulty with shock drift acceleration is identified, and possible ways of overcoming the difficulty are outlined.

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