Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer
The author argues that, after five decades of debate about the interactive of solar wind with the magnetosphere, it is time to get back to basics. Starting with Newton's law, this book also examines Maxwell's equations and subsidiary equations such as continuity, constitutive relations and the Lorentz transformation; Helmholtz' theorem, and Poynting's theorem, among other methods for understanding this interaction. - Includes chapters on prompt particle acceleration to high energies, plasma transfer event, and the low latitude boundary layer - More than 200 figures illustrate the text - Includes a color insert
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Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer
The author argues that, after five decades of debate about the interactive of solar wind with the magnetosphere, it is time to get back to basics. Starting with Newton's law, this book also examines Maxwell's equations and subsidiary equations such as continuity, constitutive relations and the Lorentz transformation; Helmholtz' theorem, and Poynting's theorem, among other methods for understanding this interaction. - Includes chapters on prompt particle acceleration to high energies, plasma transfer event, and the low latitude boundary layer - More than 200 figures illustrate the text - Includes a color insert
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Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer

Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer

by Walter Heikkila
Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer

Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer

by Walter Heikkila

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Overview

The author argues that, after five decades of debate about the interactive of solar wind with the magnetosphere, it is time to get back to basics. Starting with Newton's law, this book also examines Maxwell's equations and subsidiary equations such as continuity, constitutive relations and the Lorentz transformation; Helmholtz' theorem, and Poynting's theorem, among other methods for understanding this interaction. - Includes chapters on prompt particle acceleration to high energies, plasma transfer event, and the low latitude boundary layer - More than 200 figures illustrate the text - Includes a color insert

Product Details

ISBN-13: 9780080931654
Publisher: Elsevier Science
Publication date: 08/13/2011
Sold by: Barnes & Noble
Format: eBook
Pages: 536
File size: 13 MB
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About the Author

Walter Heikkila is Professor Emeritus in the Physics Department at the University of Texas at Dallas. His research interests include space physics and solar physics, specifically magnetospheric physics, solar wind, and auroral substorms. He received his PhD in Low Temperature Physics from the University of Toronto. He has since worked for the Defence Research Telecommunications Establishment, before becoming Associate Professor of Physics at the Southwest Center for Advanced Studies and subsequently Professor of Physics at University of Texas at Dallas. He is the author of the first edition of Earth's Magnetosphere and a leading expert on the Earth's magnetic field.
Walter Heikkila is Professor Emeritus in the Physics Department at the University of Texas at Dallas. His research interests include space physics and solar physics, specifically magnetospheric physics, solar wind, and auroral substorms. He received his PhD in Low Temperature Physics from the University of Toronto. He has since worked for the Defence Research Telecommunications Establishment, before becoming Associate Professor of Physics at the Southwest Center for Advanced Studies and subsequently Professor of Physics at University of Texas at Dallas. He is the author of the first edition of Earth’s Magnetosphere and a leading expert on the Earth’s magnetic field.

Table of Contents

Prologue 1. Historical Introduction 2. Approximate Methods 3. Helmholtz's Theorem 4. Poynting's Energy Conservation Theorem5. Magnetopause6. High Altitude Cusps7. Low-Latitude Boundary Layer 7. Driving The Plasma Sheet 9. Magnetospheric Substorms10. Epilogue

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From the Publisher

This book explores the interaction of solar wind with the magnetosphere starting with Newton's law and examining Maxwell's equations and subsidiary equations, Helmholtz's theorem and Poynting's theorem, and other methods.

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