The author argues that, after four 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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