太阳日冕中的磁流体动力学波

IF 26.3 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
V. Nakariakov, D. Kolotkov
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引用次数: 70

摘要

太阳日冕是一个独特的环境,磁流体动力学(MHD)波是等离子体天体物理学的基本过程之一,可以直接研究它。有惊人的进展。。。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magnetohydrodynamic Waves in the Solar Corona
The corona of the Sun is a unique environment in which magnetohydrodynamic (MHD) waves, one of the fundamental processes of plasma astrophysics, are open to a direct study. There is striking progre...
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来源期刊
Annual Review of Astronomy and Astrophysics
Annual Review of Astronomy and Astrophysics 地学天文-天文与天体物理
CiteScore
54.80
自引率
0.60%
发文量
14
期刊介绍: The Annual Review of Astronomy and Astrophysics is covers significant developments in the field of astronomy and astrophysics including:The Sun,Solar system and extrasolar planets,Stars,Interstellar medium,Galaxy and galaxies,Active galactic nuclei,Cosmology,Instrumentation and techniques, History of the development of new areas of research.
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