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这种方法本身与磁层顶的法线方向无关。This method itself is independent of the normal directions on the magnetopause.

磁层顶边界层可以看作是受到非均匀太阳风动压冲击的边界层。Magnetopause boundary layer is always impacted by the solar wind from the bow shock.

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

受卫星观测数据的限制，高纬磁层顶位形模型比较少。There are few models for the high-latitude magnetopause because of the limit of the satellite observations data.

基于上述理由，一般并不认为磁层顶上的波动是太阳风影响磁层的主要机制。For these reasons, magnetopause waves are not considered the primary means by which the solar wind affects the magnetosphere.

太阳风的动量涨落将通过磁层边界在磁尾激发磁流体力学波。The magnetohydrodynamic waves can be excited in the magnetotail by the momentum fluctuation of solar wind through 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。The analysis shows that this method may be used to identify several types of the discontinuities which may occur at the magnetopause.

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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。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.

该椭球面的平均大小、形状和方位的观测值与理论预计值是非常一致的。Observations of the average values of the size, shape and orientation of the dayside magnetopause agree quite well with the theoretical prediction.

本文应用三层模式和ISEE卫星观测资料，讨论了磁层顶旋转间断的稳定性。In this paper, by using a three-layer model and the observations from Satellite ISEE, the stabilities of rotational discontinuity for magnetopause are discussed.

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。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.

本文用二维可压缩MHD模型，模拟研究了向阳面磁顶区的涡旋诱发重联过程。By using a two-dimensional compressible MHD model, the local reconnection processes at the dayside magnetopause region are simulated based on the theory of vortex-induced reconnection.

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事实上，研究人员的确曾经观测到地球磁层顶上的波动，只是以它们的强度，似乎不足以驱动磁层里的大规模循环运动，或造成经常性的剧烈扰动。Waves are in fact observed along the magnetopause. But they do not seem capable of driving the large-scale circulation of the magnetosphere or the great disturbances that often occur there.

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。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.