Slightly Oblique Shock Waves in a Collisionless Magnetized Plasma
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概要
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Numerical computations for collisionless shock waves are carried out by using a simple model which retains the primitive but essential features of hot plasma. It is supposed that the direction of propagation of the wave is parallel or slightly oblique to the magnetic field ahead of the wave. For the case of low temperature and exactly parallel propagation, a train of solitary waves exists, and each of the solitary waves has a shape essentially identical with that of the solitary wave described by Saffman. The train of solitary waves, however, abruptly changes into a shock wave, when the direction of propagation becomes slightly oblique to the magnetic field. When the temperature is relatively high, only shock waves are found to exist for the case of exactly parallel as well as slightly oblique propagation.
- 社団法人日本物理学会の論文
- 1972-09-05
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関連論文
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