上述物理过程可能对解释磁鞘至磁层的能量及动量异常输运现象有所帮助。
The physical processes described above may be useful in understanding the anomalous transport phenomena of energy and momentum from the magnetosheath to the magnetosphere.
用流体方法数值模拟了电子离子磁鞘和电负性磁鞘的结构，分析了鞘层的特性和磁场的影响。
The structure of electrostatic plasma magnetic sheath and electronegative plasma magnetic sheath are numerical simulated by fluid method.
磁鞘区和地球弓激波前兆区是影响和改变太阳风波动特性，将太阳风能量传输到地球磁层的关键区域。
The magnetosheath and foreshock are the key regions which somewhat modify and then transmit the solar wind variations to the Earth's magnetosphere.
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