KELVIN-HELMHOLTZ INSTABILITY IN SOLAR ATMOSPHERIC JETS
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.
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KELVIN-HELMHOLTZ INSTABILITY IN SOLAR ATMOSPHERIC JETS
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.
58.99 In Stock
KELVIN-HELMHOLTZ INSTABILITY IN SOLAR ATMOSPHERIC JETS

KELVIN-HELMHOLTZ INSTABILITY IN SOLAR ATMOSPHERIC JETS

KELVIN-HELMHOLTZ INSTABILITY IN SOLAR ATMOSPHERIC JETS

KELVIN-HELMHOLTZ INSTABILITY IN SOLAR ATMOSPHERIC JETS

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Overview

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.

Product Details

ISBN-13: 9789811223761
Publisher: World Scientific Publishing Company, Incorporated
Publication date: 11/17/2020
Sold by: Barnes & Noble
Format: eBook
Pages: 256
File size: 9 MB

Table of Contents

Preface; The Sun: General Introduction; Solar Jets: Origin, Classification and Basic Physical Parameters; Magnetohydrodynamic Waves and Instabilities; Normal Magnetohydrodynamic Modes in Solar Jets; Kelvin–Helmholtz Instability in Solar Spicules; Kelvin–Helmholtz Instability in Solar Photospheric Twisted Flux Tubes; Kelvin–Helmholtz Instability in Solar Surges and Dark Mottles; Kelvin–Helmholtz Instability in EUV Solar Jets; Kelvin–Helmholtz Instability in X-ray Solar Jets; Kelvin–Helmholtz Instability in Rotating Solar Jets; Kelvin–Helmholtz Instability in Coronal Mass Ejections; Summary and Outlook; Bibliography
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