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magnetosphere造句

"magnetosphere"是什么意思  
造句与例句手机版
  • 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?
  • 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。
  • It's difficult to see magnetosphere in a sentence. 用magnetosphere造句挺难的
  • 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。
  • The field forms a protective shell called magnetosphere that has a radius around 10 times that of the solid earth . but strong eruptions on the solar surface can seriously distort this shell , creating geomagnetic storms
    地球磁场形成一个大小约地球直径十倍称为磁层的保护壳,当太阳表面出现猛烈的爆发,便会严重扭曲这个保护壳,形成磁暴。
  • 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) 。
  • 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。
  • Recent study of the kilohertz quasi - periodic oscillations ( qpos ) in low mass x - ray binaries ( lmxbs ) indicates that the radiation force , other than the magnetosphere and disk interaction and the general relativity ( gr ) effect setting the inner disk edge , serves as the disk truncation mechanism on shorter time scales . some results and discussions are presented in this paper
    最近对低质量x射线双星中的千赫兹准周期振动的研究表明,是辐射压力,而不是盘和磁球的相互作用以及处于盘内边界的广义相对论效应在短时标的盘切断机制上起作用.本文给出了一些研究结果及讨论
  • On the basis of analyzing previous scientists ' work , aeromagnetic data from north china wee reprocessed with 3 - d magnetosphere inversion method and program quantitative buried depth of curie temperature interface was obtained ; seismogenesis and its re1atnhip with curie temperature interface were discussed in the light of results from deep seismic sounding and deep fluid
    摘要在前人工作的基础上,运用三维磁性层反演方法和程序,对华北地区航磁资料进行了再处理,得出了研究区内居里温度面的定量埋深,结合人工地震测深和深部流体对地震成因及其与居里面的关系进行了讨论。
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