solar wind 中文意思是什麼

solar wind 解釋
太陽風,日射微粒流。

  • solar : adj 太陽的,根據太陽運行測量的;因太陽作用產生的。n = solarium the solar system 太陽系。 a solar...
  • wind : n 1 風;大風,暴風;氣流;【機械工程】壓縮空氣。2 【航海】上風;風向;〈古語〉〈pl 〉方向。3 氣息...
  1. The final speed of the solar wind depends mainly on the maximum temperature in the solar corona.

    太陽風的最終速度主要取決于日冕中的最高溫度。
  2. The gas pressure eventually overcomes the force of solar gravity and the corona inevitably expands into space as the solar wind.

    這里的氣體壓強最終會超過太陽的引力作用,使日冕終于只好以太陽風的形式向空間膨脹。
  3. One other interesting aspect of the relation of coronal holes to the solar wind follows from the appearance of coronal holes at the poles.

    日冕洞與太陽風的關系的另一個有趣的方面是日冕洞在兩極的形狀。
  4. The excess energy goes into creating and accelerating a high-speed solar wind that emanates primarily from the regions of the holes.

    多餘的能量用來產生並加速高速的太陽風,而太陽風主要發端于日冕洞區域。
  5. 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。
  6. 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。
  7. 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。
  8. 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。
  9. Astronomers have another reason for studying the solar wind besides wanting to understand its influence on the earth.

    天文學家研究太陽風,除了希望了解太陽風對地球的影響外,還有一些別的動機。
  10. The high-speed streams in the solar wind seem to affect the world's weather-particularly the strength of storms in our atmosphere.

    太陽風中的高速射流似乎還影響到我們地球上的天氣,特別是影響到大氣中風暴的強度。
  11. Fig. 11 a solar wind powered automatic weather station

    圖十一利用太陽能和風力供應能源的一個自動氣象站
  12. The mass - loss includes the light radiation and solar wind

    太陽質量損失包括光子輻射和太陽風造成的質量損失。
  13. Their shells, which apart from hydrogen, helium, and carbon also contain portions of the heavy elements formed in the stellar core, are inherently unstable, and their pulsing creates a withering stellar wind a billion times stronger than the solar wind we know today

    它的殼層除了氫層、氦曾和碳層外還有包含一部分產生自恆星核心的重元素,天生的不穩定,它們的脈動產生了一種毀滅性的星風,比我們現在知道的太陽風要強數百萬倍。
  14. Despite umpteen bumps during the race, " solar wind " successfully completed the whole course without a single failure, as reliable as hko staff

    比賽中,被其它車輛多次碰撞,太陽風完全未出現過故障,順利跑畢全程。
  15. While the magnetic field on the earth which traps charged particles encircling the earth into radiation belts called the van allen belts normally protects our planet from the solar wind, it may be deformed in the event of violent solar wind, resulting in a geomagnetic storm on earth

    雖然地球上的磁場能將環繞地球的帶電荷粒子困於其輻射帶van allen belts ,一般能有效阻擋太陽風,但在猛烈太陽風情況下它可能受影響而變形,導致地磁暴的出現。
  16. While the magnetic field on the earth ( which traps charged particles encircling the earth into radiation belts called the van allen belts ) normally protects our planet from the solar wind, it may be deformed in the event of violent solar wind, resulting in a geomagnetic storm on earth

    雖然地球上的磁場能將環繞地球的帶電荷粒子困於其輻射帶( vanallenbelts ) ,一般能有效阻擋太陽風,但在猛烈太陽風情況下它可能受影響而變形,導致地磁暴的出現。
  17. Caption : : the dramatical phenomenon, is characterised by having a dashing luminance in the upper layer of the atmosphere, created by the collisions of energetic particles of solar wind with the atoms and molecules in the polar areas

    當太陽風被地球磁場引領至兩極地區,與地球大氣層的粒子發生碰撞時,便會形成極光,宛如一張色彩斑瀾的輕妙掃過夜空,絢麗奪目。
  18. 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。
  19. Earth ' s magnetic field repels most of this onslaught, but some occasionally leaks through as a result of a sudden, explosive release of these particles from the solar wind

    地磁場阻止了其大部分的沖擊,但是偶爾太陽風中會有一些粒子突然爆發而泄漏出來。
  20. Earth ' s magnetic field repel s most of this onslaught, but some occasionally leaks through as a result of a sudden, explosive release of these particles from the solar wind

    地球的磁場能阻擋這股沖擊的大部分能量,但是,有時也會因為太陽風中的突然性的粒子的爆炸釋放而未能阻擋成功。
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