The continuum of the corona is essentially radially polarized.

日冕连续区基本上是经向偏振.

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The corona gains and loses energy continuously.

日冕总是不断地获得能量和损失能量.

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Looking at small details we find that the corona has a delicate structure.

仔细研究细节后,我们发现日冕有精细结构.

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These results may interpret the formation of plasmoid type CME.

这些结果可用于解释等离子体团型日冕物质抛射的形成.

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Using model of coronal and non - coronal radiation, ionization rate equation has been solved respectively.

在日冕和 非 日冕两种模型下,分别求解了电离速率方程.

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The difference and relationship between CME and plasma cloud in flares are shown by space observations.

日冕物质抛射和耀斑等离子体云的空间观测揭示出它们之间的区别和联系,认识到耀斑的热区和冷区.

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