磁星 的英文怎麼說

中文拼音 [cíxīng]
磁星 英文
magnetar
  • 磁 : 名詞1. [物理學] （磁性; 能吸引鐵、鎳等的性質） magnetism 2. （瓷） porcelain; china
  • 星 : 名詞1 （夜晚天空中閃爍發光的天體） star 2 [天文學] （宇宙間能發射光或反射光的天體） heavenly body...
  1. Simulations of magnetic fields generated by the antarctic circumpolar current at satellite altitude : can geomagnetic measurements be used to monitor the flow

    在衛星高度南極周圍電流所產生磁場的模擬：地磁測量能用監視器流的嗎？
  2. Cu-fe-ni sulfides are disseminated both in the core of titaniferous iron ore and in some other rocks.

    Cu-Fe-Ni硫化物星散分佈於鈦磁鐵礦核心部分以及其他幾種巖石中。
  3. Number of stars ; electromagnetic spectrum limit

    恆星數、電磁波譜極限
  4. In the absence of an appreciable magnetic field, the ensemble of nebular electrons interacts with ions to emit weak continuous radiation by free-free and free-bound transitions.

    在不存在可觀的磁場時，星雲中的電子系綜與離子相互作用可通過自由-自由和自由-束縛躍遷而發射弱連續輻射。
  5. The plasma affects the magnetic field, contributes to the “ space weathering ” of the planet ' s surface, and sputters material from the surface to populate the exosphere

    等離子體影響磁場，有助於將"太空風化"的這個星球的表面上，並屢有起伏，從材料的表面，以填充exosphere 。
  6. The characteristics of the field - aligned currents facs measured by isee 1 and 2 satellites during substorms are studied. these characteristics include the variations of facs with the interplanetary magnetic field, local time,

    分析了由isee - 1和isee - 2飛船在亞暴期間觀測到的場向電流的特性，包括場向電流所伴隨的行星際磁場地方時與
  7. Electromagnetic compatibility and radio spectrum matters - electromagnetic compatibility standard for radio equipment and services - part 12 : specific conditions for very small aperture terminal, satellite interactive earth stations operated in the frequency ranges between 4 ghz and 30 ghz in the fixed satellite service v1. 2. 1

    電磁兼容性和無線電頻譜情況.無線電設備和服務的電磁兼容性標準.第12部分:固定衛星服務中工作在4 ghz到30 ghz頻帶的衛星地面站微小孔徑端的具體條件
  8. 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。
  9. Among other incidents, the geomagnetic storm caused a japanese communications satellite to shut down temporarily

    在紜紜受影響的事件中，地磁暴使日本的一枚通訊衛星短暫停止運作。
  10. We now call this kind of super - strong magnetic field neutron stars magnetar, a term coined a few years ago by two theoretical astrophysicists duncan and thompson

    天體物理學家鄧肯和湯遜在多年前已把這類具有超級強力磁場的中子星稱為磁星。
  11. Many of us are trying to predict their properties at this moment

    至今，天文學家還在摸索著磁星的特質。
  12. With such a high magnetic field, magnetar slows down very rapidly

    由於磁星的磁場非常強，它的減速率很高。
  13. This is where a magnetic field changes shape and bumps into itself

    這就是磁星的磁場改變了形狀然後向本身內部撞擊。
  14. Concept image of a magnetar which is the object with the strongest magnetic field

    構想的磁星是擁有最強磁場的天體。
  15. Magnetars, soft gamma repeaters very strong magnetic fields, robert c. duncan

    磁星繼發軟伽瑪射線源及極強磁場，鄧肯
  16. In this respect, we are very lucky to find one and still the only one at this moment - sgr1806 - 20 - in the sky

    然而sgr1806 - 20卻被僥幸找到，亦是迄今唯一被發現的磁星。
  17. Owing to its super - strong magnetic field, calculating various properties of magnetars are hard problems for astronomers

    磁星的磁場非常強，對天文學家來說，找出它們的特性絕非容易。
  18. Therefore soon after their supernova birth, their rotational speed will become so low that they stop to emit electromagnetic pulses

    因此，超新星爆發后不久，磁星的自轉速度會變得非常緩慢，因而停止發放電磁脈沖。
  19. In other words, astronomers can only detect those extremely young energetic magnetars before they stop emittng electromagnetic pulses. consequently, it is extremely hard for us to find them in the sky

    換句話說，天文學家只能向那些仍未停止發放電磁脈沖的年青有活力的磁星埋手，故此要在天空中尋找磁星非常困難。
  20. Consequently, heat conduction along the magnetic field lines on the surface of a magnetar is far more efficient than the heat conduction perpendicular to the magnetic field lines. this may lead to a profound effect on the thermal evolution as well as the shape of the x - ray pulse of a magnetar

    結果，沿著磁星表面磁線的傳熱作用較與磁線垂直的傳熱作用為佳，這現象對磁星的熱演化和x射線脈沖的形狀有著很大的作用。
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