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Shock Drift Acceleration and Type II Solar Radio Bursts

  • Arthur G. Street (a1), Lewis Ball (a1) and D. B. Melrose (a1)

Abstract

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 shock 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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References

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Publications of the Astronomical Society of Australia
  • ISSN: 1323-3580
  • EISSN: 1448-6083
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