色球爆發 的英文怎麼說
中文拼音 [shǎiqiúbàofā]
色球爆發
英文
chromosphere eruption-
The recent researches on observations of h line profile asymmetry in chromospheric flare are reviewed. spectral properties, the corresponding mechanisms of asymmetry, and reproduction of observational spectrum by using semi - empirical atmosphere model are dicussed in detail. at last, the main problems to be solved and further researches are put forward
綜述了近年來太陽色球耀斑爆發時h譜線不對稱性的研究進展，著重討論了光譜特徵和與其對應的不對稱性產生機制，以及利用大氣半經驗模型再生觀測譜線輪廓不對稱性等方面，並提出尚待解決的主要問題和進一步的研究方向。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。Here is what they now generally expect from an event the scale of those that struck long valley and yellowstone : instead of a slow leak of red - hot lava as is seen creeping down the sides of kilauea volcano in hawaii, these eruptions feature supersonic blasts of superheated, foamlike gas and ash that rise buoyantly all the way into the earth ' s stratosphere, 50 kilometers high
對于造成長谷與黃石公園的那些爆發，或是相同等級的現象，目前他們普遍的看法是：這些爆發不像夏威夷奇勞亞火山緩慢滲出的紅熱巖漿、沿著火山側蜿蜒流出；它們的特色是以超音速的沖擊波，噴出極熱、泡沫般的氣體與火山灰，這些物質極易進入地球大氣的平流層，上升到50公里的高處。
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