| Description |
1 online resource. |
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text txt rdacontent |
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computer c rdamedia |
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online resource cr rdacarrier |
| Note |
Online resource; title from PDF title page (ScienceDirect, viewed June 4, 2024). |
| Bibliography |
Includes bibliographical references and index. |
| Contents |
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 |
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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 |
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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 |
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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? |
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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 |
| Subject |
Solar wind.
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Magnetohydrodynamics.
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Vents solaires.
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Magnétohydrodynamique.
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| Added Author |
Srivastava, Abhishek Kumar, editor.
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Goossens, Marcel, editor.
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Arregui, Iñigo, editor.
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| Other Form: |
Print version: 0323956645 9780323956642 (OCoLC)1385449503 |
| ISBN |
9780323956642 |
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9780323956659 electronic book |
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0323956653 electronic book |
|
0323956645 |
| Standard No. |
AU@ 000076674172 |
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