Solar Radio Astronomy and Plasma Non-thermal Processes in Solar Atmosphere

Solar Radio Astronomy and Plasma Non-thermal Processes in Solar Atmosphere

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摘要 1。介绍太阳的射电天文学是太阳的物理的一个重要分支，它从太阳的空气处理收音机排放。在太阳的物理，最大的挑战之一是理解在太阳黑子并且它在暴发过程的突然的释放上面在热大气的血浆存储的精力，例如太阳耀斑，暴发细丝，和花冠团喷射 CME。内在地， 1. Introduction Solar radio astronomy is an important branch of solar physics, which deals with the radio emission from the solar atmosphere. In solar physics, one of the greatest challenges is to understand the energy storing in the hot atmospheric plasma above sunspots and its sudden releasing in eruptive processes, such as solar flares, eruptive filaments, and coronal mass ejections （CME）. Intrinsically,

作者 YAN Yihua TAN Baolin

机构地区 Key Laboratory of Solar Activity

出处《Bulletin of the Chinese Academy of Sciences》 2011年第3期202-207,共6页 中国科学院院刊（英文版）

关键词太阳物理学常压等离子体射电天文学大气层日冕物质抛射太阳大气太阳黑子太阳耀斑

分类号 P182 [天文地球—天文学] TG156.82 [金属学及工艺—热处理]

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Bulletin of the Chinese Academy of Sciences

2011年第3期

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Solar Radio Astronomy and Plasma Non-thermal Processes in Solar Atmosphere

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