Nonlinear Magnetosonic Waves in a Turbulent Plasma
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概要
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Nonlinear magnetosonic waves in a turbulent plasma, characterized by an effective electrical conductivity σ_eff due to micro-instabilities, are governed by the Burgers type equation, which has a shock-like stationary solution. It is shown that initial magnetic pulses of gaussian and solitary wave forms first decay due to dissipation, and subsequently form a shock front whose steepness is determined by the opposing effects of nonlinearity and dissipation. This process is thought to be important in connection with shock formation in space plasmas.
- 核融合科学研究所の論文
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