英语释义

• the magnetic field of a planet; the volume around the planet in which charged particles are subject more to the planet's magnetic field than to the solar magnetic field

片语

Saturnian magnetosphere土星磁层

pulsar magnetosphere脉沖星磁层

magnetosphere coupling磁层耦合

asymmetric magnetosphere不对称磁层

induced magnetosphere[天]

planetary magnetosphere行星磁层

magnetosphere physics磁层物理

Jovian magnetosphere木星磁层

magnetosphere shape磁层形状

英汉例句

• the rate at which the solar wind transfers energy to the magnetosphere can vary widely, but what determines the rate of energy transfer is unclear.

  太阳风将能量转化至磁气圈的速率变化很大。但是目前为止，我们仍不清楚到底是什么在决定着这种传送速率。

• besides directing compasses, the earth「s magnetic field reaches out into space to direct the flow of the solar wind around the planet—forming a structure called the magnetosphere (depicted above).

  地球的磁场效应不仅能够指引指南针，还能够将其效应延伸至宇宙空间来指引地球四周的太阳风的流向，这样就形成了一种称为「磁气圈」的结构（如上图所示）。

• the magnetosphere is a bubble of magnetism that surrounds earth and protects us from solar wind.

  磁气圈是一个包裹着地球的磁性泡泡，保护着我们免受太阳风的吹袭。

• the movie almost gets this one right—earth’s magnetosphere does protect us from blasts of subatomic particles from the sun.

  影片在这点上倒是说对了，地球的磁气圈确实保护我们免受太阳风中亚原子颗粒的直击。

• it will defend the earth」s magnetosphere by deflecting meteorites and comets, it will lessen the effects of gamma rays into the earth「s atmosphere.

  它会通过使陨石和彗星偏离而保护地磁圈，这会有效地减少进入地球的伽马射线。

• but understanding how the magnetosphere works now should help to deal with the consequences if and when it vanishes.

  但是，不论地球磁场是否消失或何时消失，深刻地理解磁气圈的工作原理都会有助于人们去解决磁场消失后所出现的一切。

• 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。

• convection in the magnetosphere and ionosphere can be strongly driven by these fluctuations, independent of the direction of the interplanetary magnetic field.

  磁气圈和电离层之间的能量传递可以靠磁场的变化产生的强大的推动力，而不一定要依赖于行星际磁场方向。

• the magnetosphere was discovered in 1957.

  1957年，人们发现了磁气圈的存在。

• aurora on may 29 were likely triggered by the interaction of the magnetosphere with a coronal mass ejection erupting from the sun on may 24.

  5月29日的极光可能是由5月4日太阳日冕物质抛射影响磁层而触发。

• the energy of the particles and the fields in the magnetosphere can vary by large amounts.

  带电粒子的能量大小与磁气圈中的磁场的大小变化极大。

• unlike the symmetrical pattern of the iron filings and magnet, the magnetosphere is pushed in on the side facing the sun and stretched out in the earth」s wake.

  与铁屑和磁棒对称整齐的磁场模式不同，地球磁层面向太阳的一面被向内推，在相反的方向上延伸出磁场的轨迹。

• when the charged electrical particles approach the earth, they carve out a highly magnetized region —the magnetosphere —which surrounds and protects the earth.

  当这些带电粒子接近地球时，便形成一个很强的磁场区--磁气圈--包围着地球并对地球起一定的保护作用。

• now, it is storms in the magnetosphere that are recorded.

  现在，磁力计中所记录下的都与暴风雨有关。

• the compass will be no help in this matter for perhaps months as the earth「s magnetosphere will take some time to re-establish.

  在这种情况下指南针将在大约几个月之内没有一点用处，因为地球的磁气圈需要时间来重建。

• the dust cloud reacts to the earth」s magnetosphere by swinging first to one side, then the other, as the earth wobbles.

  由于地球的抖动，尘埃云通过先是摇摆向一边，再向另一边来对地球的磁气圈做出反应。