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Bøker av Bruce (Max-Planck Institute for Plasma Physics Scott

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  • av Bruce (Max-Planck Institute for Plasma Physics Scott
    1 748,-

    Ever since the first observations of turbulent fluctuations in laboratory plasma experiments in the years around 1980, turbulence in magnetised plasmas has been a subject of vigorous interest in the field of plasma physics and magnetic confinement.The second of a two-volume set, this book begins with a review of the concepts behind magnetised plasma turbulence as covered in Volume One. After covering the effects of temperature dynamics, especially heat flux inertia, the rest of the first half reviews classical field theory in the necessary language, then builds the gyrokinetic and gyrofluid theory in a systematic and self-consistent manner, with special emphasis on energetic consistency. Gyrofluid turbulence in various flavours in a magnetised plasma is then covered, with control cases and energetic analysis. Familiar magnetohydrodynamic instabilities are reproduced in gyrofluid language, and then turbulence in a flow layer, current channel, pressure layer, or all three, is covered. A reprise of the theory in terms of a gauge transform with functional Lie-Poisson bracket structure closes the volume.Key FeaturesWritten by a world-leading expert in magnetised plasma turbulenceFills a long-standing gap in the plasma physics literatureFirst unified book on gyrokinetic and gyrofluid theory and turbulenceIncludes complete derivations of the fundamental concepts

  • - Fluid drift turbulence
    av Bruce (Max-Planck Institute for Plasma Physics Scott
    1 748,-

    Ever since the first observations of turbulent fluctuations in laboratory plasma experiments in the years around 1980, turbulence in magnetised plasmas has been a subject of vigorous interest in the field of plasma physics and magnetic confinement. This work fills a significant gap in the set of available references for research in the field, and serves as part of the wider literature helpful in related fields such as geophysical fluid dynamics or astrophysics, in which background rotation is mathematically similar to a background magnetic field in a plasma.The first of a two-volume set, this book begins with an overview of the essential nature of a plasma and a magnetised plasma, then turbulence and plasma turbulence are introduced conceptually and mathematically. There follows a theoretical interlude developing the concepts of fluid and plasma dynamics, emphasising the force balance and quasineutrality which shape its character. After this the three-dimensional situation takes over center stage. Concepts of energetic consistency and nonlinear instability and mode structure are emphasised. The effects of magnetic shear and curvature, and open and closed magnetic field line flux surfaces, and finally the interaction with both background and self-generated flows, are all covered in separate chapters. An interlude points to a second volume treating temperature gradients and fluctuations, gyrokinetic and gyrofluid theory, and the interplay with magnetohydrodynamic instabilities.Key FeaturesWritten by a world-leading expert in magnetised plasma turbulenceFills a long-standing gap in the plasma physics literatureFirst comprehensive books on two-fluid magnetised plasma turbulenceIncludes complete derivations of the fundamental concepts

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