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solar corona 日冕。

solar cycle

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。

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

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。