日冕 的英文怎麼說

中文拼音 [rìmiǎn]
日冕 英文
[天文學] （solar） corona日冕觀測鏡 coronascope; 日冕 （譜）線 coronal line; 日冕儀 coronagraph
  • 日 : Ⅰ名詞1 （太陽） sun 2 （白天） daytime; day 3 （一晝夜; 天） day 4 （泛指某一段時間） time 5 （日...
  • 冕 : 名詞1. （帝王的禮帽） crown 2. （姓氏） a surname
  1. Acoustic waves are a primary candidate for supplying the energy necessary to heat the solar chromosphere and corona.

    聲波是供給太陽色球和日冕加熱所需能量的主要候選能源。
  2. K. we still cannot completely explain why the temperature of the chromosphere and corona can be higher than the photosphere

    度。為甚麼日冕和色球層的溫度可以比光球層更高，仍是天文學上一個未解之謎。
  3. The continuum of the corona is essentially radially polarized.

    日冕連續區基本上是經向偏振。
  4. The corona gains and loses energy continuously.

    日冕總是不斷地獲得能量和損失能量。
  5. Looking at small details we find that the corona has a delicate structure.

    仔細研究細節后，我們發現日冕有精細結構。
  6. 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。
  7. Much of visible light reaching us from the solar corona also seems to be due to scattering by electrons.

    從日冕中射來的相當大一部分可見光看來也是由電子散射產生的。
  8. 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。
  9. 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。
  10. Trace, transition region and coronal trace

    太陽過渡區和日冕
  11. Coronal active region

    日冕活動區
  12. 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。
  13. " solarmax " is a heliograph production in association with museum of science and industry, chicago. the u. s. national science foundation provided funding to make " solar max " a reality

    由日冕儀製作公司與美國芝加哥科學及工業博物館聯合製作，並獲美國國家科學基金贊助拍攝。
  14. This halo could extend all the way to the milky way ' s nearest neighboring galaxies, the magellanic clouds, scientists said

    科學家說，該日冕可能一直延伸到銀河系最近的星系麥哲倫雲。
  15. Zheng, h. n., zhang, b. and wang, s., 1995, a mechanism for the formation of plasmoid - type cme in the solar corona, acta astron. sinica, 36, 341

    鄭惠南，張兵，王水， 1995 ，等離子體團型日冕物質拋射的形成機制，天文學報， 36 ， 341
  16. In chapter one, we make a review of particle acceleration theory and the use in solar corona. in chapter two, first we get the spectrum of synchrotron radiation then obtain the electron energy spectrum. in last chapter, we select the typical solar active region parameter to compare our result to the observation and discuss the acceleration mechanism

    本文第一章對粒子加速理論以及目前各種加速理論在太陽日冕中的應用作了介紹；第二章通過理論計算得到同步加速輻射譜以及電子能譜；第三章選取太陽日冕中典型參數，對同步加速輻射加速日冕快電子作了簡單討論。
  17. The movie frames were recorded from january 12 through jan 16 by a coronograph onboard the sun - staring soho spacecraft

    這部電影的定格是在1月12日到16日之間拍攝的，使用的設備是soho衛星上的日冕相機。
  18. The main research contents of the physical design include : presenting the domestic and international status of space weather and expanding on the need and the importance about the space weather forecast ; sorting the disastrous space weather and discussing their effects and adapted prediction methods ; analyzing the solar disturbing resources of space weather and the precursor or concomitant phenomena of solar eruption based on the newest observational results ; probing into the radiation principle of solar short - wave ray and presenting the computing methods about solar continuum and line spectrum radiation ; extrapolating physical methods of reconstructing the temperature and the emission measure of coronal plasma ; argumenting the effective observing spectrum for space weather empirical forecast and space weather numerical forecast

    物理設計的主要研究內容包括：分析目前國內國際空間天氣預報的發展現狀及開展空間天氣預報的必要性和重要性；分類討論了災害性空間天氣的種類、影響及目前國際上的預報方法：分析了空間天氣太陽擾動源及擾動源爆發的先兆現象或者伴生現象；討論了太陽短波輻射線譜和連續譜輻射強度的計算方法：推導了利用望遠鏡多波段的觀測結果反演日冕等離子體溫度、發射量等參數的物理方法：論證了開展空間天氣經驗預報和發展數值預報有效的成像譜段。
  19. In this thesis, we investigate the role of alfven wave in the coronal heating process. all the work consists of two main parts

    我們從兩個方面對這個問題進行了探討：第一個方面主要地研究了加熱日冕的alfven波源。
  20. Astronomers found the halo using nasa ' s far ultraviolet spectroscopic explorer ( fuse ) satellite to peer beyond the edges of our home galaxy

    天文學家是使用美國航空航天局的遠紫外線光譜探測儀（ fuse ）衛星，在我們所居住的星系邊緣外發現此日冕的。
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