耀斑物理 的英文怎麼說

中文拼音 [yàobānwùlǐ]
耀斑物理 英文
flare physics
  • 耀 : Ⅰ動詞1. （光線強烈地照射） shine; illuminate; dazzle 2. （誇耀） boast of; laud Ⅱ名詞（光榮） honour; credit
  • 斑 : Ⅰ名詞（斑點; 斑紋; 污點; 瑕疵） spot; speck; speckle; stripe; stain Ⅱ形容詞（有斑點或斑紋的） spo...
  • 物 : 名詞1 （東西） thing; matter; object 2 （指自己以外的人或與己相對的環境） other people; the outsi...
  • 理 : Ⅰ名詞1 （物質組織的條紋） texture; grain （in wood skin etc ） 2 （道理;事理） reason; logic; tru...
  • 耀斑 : [天文學] chromospheric eruption; solar flare
  • 物理 : 1. （事物的內在規律） innate laws of things2. （物理學） physics
  1. Theoretical researches on solar activity, solar flare and cme were involved in many fields of foundational physics such as plasma astrophysics, magnetohydrodynamics ( mhd ) and so on. the forecast of solar activity, a main branch of space weather, was becoming more and more significant for preventing space disaster and for many aspects of space science

    探索太陽活動的規律、太陽耀斑及其伴隨cme的先兆、觸發過程及能量傳播機制等等，從理論上推動了等離子體天體物理、磁流體力學等諸多基礎理論的發展，有著重要的理論意義；而對太陽活動的預報，是國際前沿科學?空間天氣學的重要組成部分，對避免空間災害、為航空航天科學提供服務等方面，具有重大的實際應用價值。
  2. With x - ray " s erupting generated by solar proton flare, x - ray transmit toward earth with light speed and isn " t effected by magnetic field of earth. it arrive in earth earlier several decades minutes to hours than proton liquid. make use of the difference of time they spend on space spread, we make alarm for solar proton event by physical character of solar x - ray, which is a very valid means

    伴隨太陽質子耀斑產生的x射線爆發，它以光速向地球傳播而且不受地磁場的影響，它比質子流超前幾十分鐘甚至幾十小時到達地球，利用二者在空間傳播的時間差，以太陽x射線某些物理特徵警報太陽質子事件是一種十分有效的手段。
  3. The bastille - day flare of 14 july 2000, a great solar flare with x - ray / ha importance of x5. 7 / b3, was observed around 10 : 24 ut in the noaa 9077 ar at position n22w07. in this flare, very rich interesting radio bursts and fine radio spectral structures were detected, not only in metric wave band, but also in decimetric and microwave band ( 1. 0 - 7. 6 ghz by national astronomical observatories of chinese academy of sciences - naoc )

    2000年7月14日的太陽耀斑爆發? bastille事件，備受國際太陽物理學家關注，著名的sci刊物「 solarphysics 」特出版專輯研討該事件，從光球、色球、日冕、直至日地空間的廣闊空間尺度范圍內，對該事件的觀測資料進行了分析和理論研究。
  4. Though the analysis of the distributions, we found that there are two separated loops in the post flare loop, one is almost upright to line - of - sight, the other is nearly parallel to the line - of - sight

    通過分析這些物理量場，我們發現在該耀斑后環當中可能存在兩個獨立的環系。位於北面的環幾乎與觀測者的視線垂直，而南面的環則幾乎與觀測者視線平行。
  5. Furthermore the " microflare theory " tried to discuss and find the elementary flares in small space and time scale which might form and trigger the whole solar flare. the detection of radio fine structures showed many observational evidences of " microflare ". the observations and theoretical researches on radio fine structure have been developed fast recently and played an important role in solar radio astrophysics

    著名的「微耀斑理論」 ，試圖從較小的時間、空間尺度范圍探究太陽耀斑形成和觸發的基本單元，而射電精細結構是微耀斑理論的重要觀測基礎，對射電精細結構的觀測和理論研究已成為太陽射電天文學中快速發展的領域，對揭示太陽活動源區的物理本質具有重要的意義。
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