Kelvin-Helmholtz Instability in Solar Atmospheric Jets

太阳大气喷流中的KELVIN-HELMHOLTZ不稳定性

天体物理学

原   价:
1066.00
售   价:
799.00
发货周期:预计3-5周发货
出  版 社
出版时间
2020年11月20日
装      帧
精装
ISBN
9789811223747
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页      码
256 pp
语      种
英文
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图书简介
The book provides a comprehensive overview of the eruptive and wave phenomena in the solar atmosphere. One of the ongoing problems in solar physics is the heating of the solar corona. Currently there is a competition between two mechanisms in explaining the heating, i.e., dissipation of energy by waves and small scale frequent coronal magnetic reconnection. However, some studies indicate this may be a joint effect of these two possible mechanisms. Kelvin–Helmholtz Instability (KHI) of propagating magnetohydrodynamic modes in solar flowing structures plays an important role in the solar atmosphere. It can trigger the onset of wave turbulence leading to effective plasma heating and particle acceleration. KHI is a multifaceted phenomenon and the purpose of this book is to illuminate its (instability) manifestation in various solar jets like spicules, dark mottles, surges, macrospicules, Extreme Ultraviolet (EUV) and X-ray jets, as well as rotating, tornado-like, jets, solar wind, and coronal mass ejections. The modeling of KHI is performed in the framework of ideal magnetohydrodynamics. The book consists of 12 chapters and is intended primarily for advanced undergraduate and postgraduate students, as well as early career researchers. Key Feature: o Clear treatment of major topics, well-illustrated material, and the good agreement between theory and observations
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