magnetosphere造句
例句与造句
- 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。 - 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。 - 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。 - 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。 - 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？ - It's difficult to find magnetosphere in a sentence. 用magnetosphere造句挺难的
- Yet the actual long - term survival of active organisms , spores or complex organic molecules beyond earth ' s magnetosphere has never been tested
活性有机体、孢子或复杂的有机分子，在地球磁层之外能否长期幸存，则从未实地验证过。 - The three st5 satellites , each no bigger than an average tv set , will help scientists to study magnetic fields in earth ' s magnetosphere
三个空间技术5号卫星(每个尺寸都不大于一台普通的电视机)将帮助科学家研究地球磁气圈的磁场。 - Thus , this research could not say much about the effects of interplanetary charged particles , which cannot penetrate earth ' s magnetosphere
因此，对游走于行星之间，但是无法穿透地球磁层的带电粒子所产生的效应，这项研究所透露的讯息不多。 - The finding is evidence of the complex interaction between saturn ' s moons , rings and magnetosphere . studying this interaction is one of cassini ' s objectives
这个发现是土星的月亮，环状物和磁气圈之间复杂交互感应的证明。这种交互感应的研究是卡西尼的主要目标之一。 - They move under the influence of the dynamo currents in the earth ' s core , as well as electric currents flowing in the ionosphere , the radiation belts and the earth ' s magnetosphere
它们在地核内发电机流以及流动在电离层、辐射带和地球磁气圈内电流的影响下产生移动。 - Under these circumstances , reconnection takes place along a wide equatorial belt , opening up nearly the entire outer boundary of the magnetosphere to the solar wind
在这种情况下，磁力线重连会在赤道面上宽广的带状区域内发生，几乎把整个磁层外围边界都打开，放太阳风进来。 - Reconnection is most efficient when the imf has a component that is directed southward ? that is , opposite to the northward direction of the earth ' s magnetic field at the dayside of the magnetosphere
在磁层昼侧，若imf有南向分量，也就是和北向的地球磁场方向相反，则磁力线重连的效率最高。 - The latter measurements provide definitive evidence that mercury ' s magnetosphere ? despite its small size ? is not a vacuum but hosts significant densities of heated solar wind plasma
后者测量提供确切的证据表明，水星的磁层-尽管它体积小-是不是一个真空，但东道主密度显著激烈的太阳风等离子体。 - For other orientations of the imf , reconnection still happens , but it may be more localized in the higher latitudes , where the released energy mainly flows around the magnetosphere rather than into it
假如imf指向别的方向，磁力线重连仍能发生，但会比较局限在高纬度，释放出的能量则主要流经磁层外围，而非流入磁层内部。 - These results show the expected increases in solar wind plasma density downstream of the bow - shock boundary , as well as significant solar wind plasma densities within mercury ' s magnetosphere close to the planet
这些调查结果表明，预计增幅在太阳风等离子体密度下游弓激波边界，以及大量的太阳风等离子体密度与水星的磁层接近地球。
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