| 1. | A continuous stream of charged particles, called the solar wind, impinges on the earth's magnetosphere .
称作太阳风的连续带电子流撞击在地球的磁层上。 |
| 2. | The second - order resonance between superluminous r - x mode wave and magnetospheric electrons
模电磁波与磁层电子的二阶共振作用 |
| 3. | The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere
从太阳风传来的磁场能量，彻底改变了磁层形状。 |
| 4. | This animation shows a conceptual sketch of mercury ' s magnetosphere at the time of the messenger flyby
这个动画是信使号探测船探测水星磁层时的模拟图。 |
| 5. | 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。 |
| 6. | But in the magnetosphere , weather results from the interaction between the earth ' s magnetic field and the solar wind
但在磁层里，太空天气却是由地球磁场和太阳风的交互作用所造成。 |
| 7. | The variation curve of the giant - magnetoresistance with the change of the thickness of the ferromagnetic layer , a , usually shows a maximum
巨磁电阻随铁磁层厚度a的变化曲线通常显示一个最大值。 |
| 8. | The field that space environment contain is high - layer atmosphere , ionosphere , magnetic layer , interplanetary space and even sun
涵盖的区域包括地球高层大气、电离层、磁层、行星际空间直至太阳。 |
| 9. | In other words , how can the wind overcome the barrier of the geomagnetic field and drive the motions of the plasma inside the magnetosphere
换言之，即太阳风是如何克服地球磁场的阻碍，进而驱动磁层里的电浆运动？ |
| 10. | The tunneling current is obstructed when the two ferromagnetic layers have opposite orientations and is allowed when their orientations are the same
若两侧的铁磁层磁性方向相反，穿隧电流就被挡住，反之则可通过。 |
