Magnetohydrodynamic processes in solar plasmas /

This book, edited by Abhishek Kumar Srivastava and others, explores dynamic processes in solar plasmas, focusing on the physics of astrophysical fluids and the Sun. It covers topics such as solar interior plasma processes, solar magnetism, MHD waves, and magnetic reconnection. The text aims to provi...

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Altri autori: Srivastava, Abhishek Kumar (Redattore), Goossens, Marcel (Redattore), Arregui, Iñigo (Redattore)
Natura: Elettronico eBook
Lingua:inglese
Pubblicazione: Amsterdam : Elsevier, 2024.
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Accesso online:ScienceDirect
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245 0 0 |a Magnetohydrodynamic processes in solar plasmas /  |c edited by Abhishek Kumar Srivastava, Marcel Goossens, Iñigo Arregui. 
264 1 |a Amsterdam :  |b Elsevier,  |c 2024. 
300 |a 1 online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
588 0 |a Online resource; title from PDF title page (ScienceDirect, viewed June 4, 2024). 
504 |a Includes bibliographical references and index. 
505 0 |a Front Cover -- Magnetohydrodynamic Processes in Solar Plasmas -- Copyright -- Contents -- Contributors -- Preface -- 1 Dynamical processes in the solar plasma -- 1.1 Introduction -- 1.2 The solar interior and its plasma processes -- 1.3 The solar magnetism and its cycle -- 1.4 Dynamical processes in the solar plasma -- 1.4.1 Wave processes in the solar atmosphere -- 1.4.1.1 Waves and oscillations in the stratified lower solar atmosphere -- 1.4.1.2 The waves in the homogeneous coronal plasma -- 1.4.1.3 Waves in the inhomogeneous magnetic structures 
505 8 |a 1.4.2 Physical manifestations of shocks in the solar atmosphere -- 1.4.3 Evolution of plasma instabilities and turbulence in the solar atmosphere -- 1.4.4 Magnetic reconnection process -- 1.4.5 Heating of the solar atmosphere -- 1.5 Outline and scope of the book -- References -- 2 Helioseismology -- 2.1 Introduction -- 2.2 The standard solar model -- 2.3 Observation of solar oscillations -- 2.4 Properties of solar oscillations -- 2.5 Seismic inferences of the solar structure -- 2.5.1 Inverse techniques -- 2.5.2 Inferences from structure inversions -- 2.5.3 Constraints on heavy element abundances 
505 8 |a 2.6 Rotation rate in the solar interior -- 2.6.1 Inversion for rotation rate -- 2.6.2 Inversion results -- 2.6.3 The tachocline -- 2.6.4 Magnetic field and other asphericities in the solar interior -- 2.6.5 The meridional flow -- 2.7 Temporal variations in the solar interior -- 2.7.1 Temporal variations in the solar radius -- 2.7.2 Temporal variations in the solar rotation -- 2.8 Summary -- Acknowledgments -- References -- 3 The Sun's magnetic cycle: observations and modeling -- 3.1 Magnetic field observations on the solar surface -- 3.2 Solar flows and helioseismology 
505 8 |a 3.3 Magnetohydrodynamics and mean field models -- 3.4 Saturation of dynamo generated magnetic field -- 3.5 Kinematic flux transport dynamo models -- 3.6 Summary -- References -- 4 MHD waves in homogeneous and continuously stratified atmospheres -- 4.1 Introduction -- 4.1.1 Magneto-acoustic-gravity (MAG) waves in the combined photosphere/chromosphere -- 4.1.2 Overview -- 4.2 MHD equations -- 4.2.1 Conventional form -- 4.2.2 Conservation form -- 4.3 MHD equilibria -- 4.3.1 Lorentz force and equilibrium -- 4.3.2 Energy, variational principles and stability -- 4.4 What are MHD waves? 
505 8 |a 4.4.1 Basic equations -- 4.4.2 Dispersion relation -- 4.4.3 Phase and group velocities -- 4.4.4 Wave polarizations -- 4.5 Waves in stratified atmospheres -- 4.5.1 Acoustic-gravity waves and the WKBJ method -- 4.5.2 MAG waves -- 4.5.3 Exact 2D MHD solutions and their mixed properties -- 4.5.4 Decoupled Alfvén waves -- 4.5.5 Horizontal magnetic field, critical levels, resonant absorption and phase mixing -- 4.5.6 Exact 3D MHD solutions -- 4.6 Eikonal method and ray theory -- 4.6.1 Ray theory basics -- 4.6.2 Application to MHD waves -- 4.6.2.1 Dispersion relation 
520 |a This book, edited by Abhishek Kumar Srivastava and others, explores dynamic processes in solar plasmas, focusing on the physics of astrophysical fluids and the Sun. It covers topics such as solar interior plasma processes, solar magnetism, MHD waves, and magnetic reconnection. The text aims to provide a comprehensive understanding of plasma behavior in the solar environment, drawing on observations and theoretical models. It targets researchers and students in astrophysics and related fields, offering insights into plasma dynamics and solar phenomena.  |7 Generated by AI 
650 0 |a Solar wind. 
650 0 |a Magnetohydrodynamics. 
650 6 |a Vents solaires.  |0 (CaQQLa)201-0018749 
650 6 |a Magnétohydrodynamique.  |0 (CaQQLa)201-0008599 
650 7 |a Magnetohydrodynamics  |2 fast  |0 (OCoLC)fst01005872 
650 7 |a Solar wind  |2 fast  |0 (OCoLC)fst01125214 
700 1 |a Srivastava, Abhishek Kumar,  |e editor. 
700 1 |a Goossens, Marcel,  |e editor.  |1 https://id.oclc.org/worldcat/entity/E39PCjD7xBrWxhCjXPXJTFPmh3 
700 1 |a Arregui, Iñigo,  |e editor.  |1 https://id.oclc.org/worldcat/entity/E39PCjJ74Mb8jFQ4WXCkQxCvpP 
776 0 8 |i Print version:  |z 0323956645  |z 9780323956642  |w (OCoLC)1385449503 
856 4 0 |3 ScienceDirect  |u https://www.sciencedirect.com/science/book/9780323956642