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- W145327900 abstract "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." @default.
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- W145327900 title "Shock Drift Acceleration and Type II Solar Radio Bursts" @default.
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- W145327900 doi "https://doi.org/10.1017/s1323358000019603" @default.
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