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8 - MHD stability – general considerations

Published online by Cambridge University Press:  05 July 2014

Jeffrey P. Freidberg
Affiliation:
Massachusetts Institute of Technology
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Summary

Introduction

In the remainder of the book, it is assumed that an MHD equilibrium has been calculated, either analytically or numerically. The next basic question to ask is whether or not the equilibrium is MHD stable. Qualitatively, the question of stability can be stated as follows. The existence of an MHD equilibrium implies a plasma state in which the sum of all forces acting on the plasma is zero. Assume now that the plasma is perturbed from this state producing a set of corresponding perturbed forces. If the direction of these forces is such as to restore the plasma to its original equilibrium position then the plasma is stable. If, on the other hand, the direction of the forces tends to enhance the initial perturbation then the plasma is unstable.

The question of ideal MHD stability is a crucial one, since plasmas, in general, suffer serious degradation in performance, ranging from enhanced transport to catastrophic termination, as a consequence of such instabilities. Not surprisingly, there is consensus in the international fusion community that a plasma must be MHD stable to be viable in a fusion reactor. Indeed, it is fair to say that MHD stability considerations are a primary driver in the design of virtually all the magnetic geometries that have been proposed as fusion reactors.

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Chapter
Information
Ideal MHD , pp. 327 - 380
Publisher: Cambridge University Press
Print publication year: 2014

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References

Bernstein, I. B., Frieman, E. A., Kruskal, M. D., and Kulsrud, R. M. (1958). Proc. R. Soc. London, Ser. A 244, 17.CrossRef
Chandraseker, S. (1961). Hydrodynamic and Hydromagnetic Stability. Oxford: Clarendon.Google Scholar
Furth, H. P., Killeen, J., Rosenbluth, M. N., and Coppi, B. (1965). In Plasma Physics and Controlled Nuclear Fusion Research 1964. Vienna: International Atomic Energy Agency, Vol. I, p. 103.Google Scholar
Goedbloed, J. P. (1975). Phys. Fluids 18, 1258.CrossRef
Goedbloed, H. and Poedts, S. (2004). Principles of Magnetohydrodynamics. Cambridge: Cambridge University Press.CrossRefGoogle Scholar
Grad, H. (1973). Proc. Natl. Acad. Sci. USA 70, 3277.CrossRef
Greene, J. M. and Johnson, J. L. (1968). Plasma Phys. 10, 729.CrossRef
Laval, G., Mercier, C., and Pellat, R. M. (1965). Nucl Fusion 5, 156.CrossRef

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