• Collisionless shocks are the important physical phenomena in the space and cosmical plasmas.

    无碰撞激波是空间等离子体和宇宙等离子体中的重要物理现象。

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  • The results show that whistler waves can be directly excited by the collisionless current sheet.

    结果表明,哨声波能被无碰撞电流片直接激发。

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  • The collisionless magnetic reconnection is studied using two dimensional full particle simulation.

    采用二维全粒子模拟方法研究了无碰撞磁场重联。

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  • The process of magnetic reconnection in the collisionless plasma and distributions of particles in different positions are studied based on two-dimensional particle simulation.

    利用二维全粒子模拟方法研究了无碰撞等离子体中的磁场重联过程,得到了不同区域的离子和电子速度分布。

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  • The fluctuations of solar wind quantities at the magnetopause excite the compressed Alfven waves, which propagate through the collisionless plasma in the tail of magnetosphere.

    太阳风的涨落在磁层顶激发压缩阿尔文波,并在磁尾的无碰撞等离子体中传播。

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  • The fluctuations of solar wind quantities at the magnetopause excite the compressed Alfven waves, which propagate through the collisionless plasma in the tail of magnetosphere.

    太阳风的涨落在磁层顶激发压缩阿尔文波,并在磁尾的无碰撞等离子体中传播。

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