磁層 的英文怎麼說

中文拼音 [cícéng]
磁層 英文
（在太陽風作用下地球磁場被局限的范圍） magnetic layer; magnetic coating; magnetosphere
  • 磁 : 名詞1. [物理學] （磁性; 能吸引鐵、鎳等的性質） magnetism 2. （瓷） porcelain; china
  • 層 : i 量詞1 （用於重疊、積累的東西 如樓層、階層、地層） storey; tier; stratum 2 （用於可以分項分步的...
  1. This animation shows a conceptual sketch of mercury ' s magnetosphere at the time of the messenger flyby

    這個動畫是信使號探測船探測水星磁層時的模擬圖。
  2. The direction of the easy axis of the soft layer has little influence on the magnetic hysteresis and magnetostriction of the ecmm when the magnetic anisotropy of the magnetostrictive layer is much larger than that of the soft layer

    雖然軟磁層的磁各向異性角對多層膜的磁學及力學性質幾乎沒有影響，但磁各向異性常數卻會顯著影響多層膜的性質。
  3. A continuous stream of charged particles, called the solar wind, impinges on the earth's magnetosphere.

    稱作太陽風的連續帶電子流撞擊在地球的磁層上。
  4. The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere

    從太陽風傳來的磁場能量，徹底改變了磁層形狀。
  5. But in the magnetosphere, weather results from the interaction between the earth ' s magnetic field and the solar wind

    但在磁層里，太空天氣卻是由地球磁場和太陽風的交互作用所造成。
  6. In other words, how can the wind overcome the barrier of the geomagnetic field and drive the motions of the plasma inside the magnetosphere

    換言之，即太陽風是如何克服地球磁場的阻礙，進而驅動磁層里的電漿運動？
  7. Yet the actual long - term survival of active organisms, spores or complex organic molecules beyond earth ' s magnetosphere has never been tested

    活性有機體、孢子或復雜的有機分子，在地球磁層之外能否長期倖存，則從未實地驗證過。
  8. Thus, this research could not say much about the effects of interplanetary charged particles, which cannot penetrate earth ' s magnetosphere

    因此，對遊走於行星之間，但是無法穿透地球磁層的帶電粒子所產生的效應，這項研究所透露的訊息不多。
  9. When reconnection is initiated on the dayside magnetopause, the interconnected imf and geomagnetic field lines are swept back by the solar wind over the earth ' s poles, pouring energy into the northern and southern lobes of the long magnetotail on the nightside

    當磁力線重連在晝側的磁層頂上開始發生，連在一起的imf和地球磁場磁力線便被太陽風往後吹，掃過地球南北極，把能量灌入長磁尾的南北兩葉。
  10. 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

    地球磁場形成一個大小約地球直徑十倍稱為磁層的保護殼，當太陽表面出現猛烈的爆發，便會嚴重扭曲這個保護殼，形成磁暴。
  11. 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

    在這種情況下，磁力線重連會在赤道面上寬廣的帶狀區域內發生，幾乎把整個磁層外圍邊界都打開，放太陽風進來。
  12. The second - order resonance between superluminous r - x mode wave and magnetospheric electrons

    模電磁波與磁層電子的二階共振作用
  13. The region of solar - wind plasma between the bow shock and the magnetopause is known as the magnetosheath

    在弓形震波和磁層頂之間充滿太陽風電漿的區域，稱為磁鞘。
  14. The variation curve of the giant - magnetoresistance with the change of the thickness of the ferromagnetic layer, a, usually shows a maximum

    巨磁電阻隨鐵磁層厚度a的變化曲線通常顯示一個最大值。
  15. The field that space environment contain is high - layer atmosphere, ionosphere, magnetic layer, interplanetary space and even sun

    涵蓋的區域包括地球高層大氣、電離層、磁層、行星際空間直至太陽。
  16. The tunneling current is obstructed when the two ferromagnetic layers have opposite orientations and is allowed when their orientations are the same

    若兩側的鐵磁層磁性方向相反，穿隧電流就被擋住，反之則可通過。
  17. 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

    這些調查結果表明，預計增幅在太陽風等離子體密度下游弓激波邊界，以及大量的太陽風等離子體密度與水星的磁層接近地球。
  18. 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

    後者測量提供確切的證據表明，水星的磁層-盡管它體積小-是不是一個真空，但東道主密度顯著激烈的太陽風等離子體。
  19. 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

    我們對cme運動方向與磁暴強弱的關系進行了初步的研究，研究表明，同樣條件下，正對磁層頂的cme形成的磁暴更強，即cme的運動方向是影響磁暴強弱的一個重要因素。
  20. 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

    就像超音速噴射機在大氣層飛行時會產生震波，當太陽風碰上地球磁層，也一樣會產生震波，我們稱之為弓形震波，產生位置約在晝側的磁層頂外13000公里處。
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