磁层顶 meaning in Chinese

magnetopause

The region of solar - wind plasma between the bow shock and the magnetopause is known as the magnetosheath
在弓形震波和磁层顶之间充满太阳风电浆的区域，称为磁鞘。
In addition , the study shows that the cmes " traveling direction is also an important factor , which influence the intensity of the geomagnetic storms . we also analyzed gcrs data from beijing super - neutron - monitor ( snm ) by using fft and power spectrum method
我们对cme运动方向与磁暴强弱的关系进行了初步的研究，研究表明，同样条件下，正对磁层顶的cme形成的磁暴更强，即cme的运动方向是影响磁暴强弱的一个重要因素。
Just as the passage of a supersonic jet through the atmosphere produces a shock wave , the encounter of the solar wind with the magnetosphere forms a shock wave ? known as the bow shock ? some 13 , 000 kilometers upstream ( that is , closer to the sun ) from the dayside magnetopause
就像超音速喷射机在大气层飞行时会产生震波，当太阳风碰上地球磁层，也一样会产生震波，我们称之为弓形震波，产生位置约在昼侧的磁层顶外13000公里处。