• The magnetopause exerts a tremendous influence on magnetic field within the magnetosphere.

    太阳风与地磁场相互作用形成的磁层顶对磁层内磁场有重要影响。

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  • The analysis shows that this method may be used to identify several types of the discontinuities which may occur at the magnetopause.

    分析表明,这种方法可以用来识别磁层顶上可能出现的若干种间断。

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  • The location and intensity of the CF-current on the magnetopause are almost same as the results from the model of the ideal discontinuous surface.

    实际磁层顶电流片的位置和强度与我们假设的理想磁层顶间断面计算结果基本吻合。

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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 first constellations will most likely observe the inner magnetosphere and the dayside magnetopause with each cake-size craft recording the basic characteristics of the plasmas and magnetic fields.

    第一个大卫星群可能用来监测磁层内层及昼侧的磁层顶,每个蛋糕般大小的小卫星都将记录各别区域内,电浆与磁场的基本数据。

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  • The first constellations will most likely observe the inner magnetosphere and the dayside magnetopause with each cake-size craft recording the basic characteristics of the plasmas and magnetic fields.

    第一个大卫星群可能用来监测磁层内层及昼侧的磁层顶,每个蛋糕般大小的小卫星都将记录各别区域内,电浆与磁场的基本数据。

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