Book contents
- Frontmatter
- Dedication
- Contents
- Preface
- Acknowledgements
- 1 Introduction
- 2 The ideal MHD model
- 3 General properties of ideal MHD
- 4 MHD equilibrium: general considerations
- 5 Equilibrium: one-dimensional configurations
- 6 Equilibrium: two-dimensional configurations
- 7 Equilibrium: three-dimensional configurations
- 8 MHD stability – general considerations
- 9 Alternate MHD models
- 10 MHD stability comparison theorems
- 11 Stability: one-dimensional configurations
- 12 Stability: multi-dimensional configurations
- Appendix A Heuristic derivation of the kinetic equation
- Appendix B The Braginskii transport coefficients
- Appendix C Time derivatives in moving plasmas
- Appendix D The curvature vector
- Appendix E Overlap limit of the high β and Greene–Johnson stellarator models
- Appendix F General form for q(ψ)
- Appendix G Natural boundary conditions
- Appendix H Upper and lower bounds on δQKIN
- Index
- References
8 - MHD stability – general considerations
Published online by Cambridge University Press: 05 July 2014
- Frontmatter
- Dedication
- Contents
- Preface
- Acknowledgements
- 1 Introduction
- 2 The ideal MHD model
- 3 General properties of ideal MHD
- 4 MHD equilibrium: general considerations
- 5 Equilibrium: one-dimensional configurations
- 6 Equilibrium: two-dimensional configurations
- 7 Equilibrium: three-dimensional configurations
- 8 MHD stability – general considerations
- 9 Alternate MHD models
- 10 MHD stability comparison theorems
- 11 Stability: one-dimensional configurations
- 12 Stability: multi-dimensional configurations
- Appendix A Heuristic derivation of the kinetic equation
- Appendix B The Braginskii transport coefficients
- Appendix C Time derivatives in moving plasmas
- Appendix D The curvature vector
- Appendix E Overlap limit of the high β and Greene–Johnson stellarator models
- Appendix F General form for q(ψ)
- Appendix G Natural boundary conditions
- Appendix H Upper and lower bounds on δQKIN
- Index
- References
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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- Ideal MHD , pp. 327 - 380Publisher: Cambridge University PressPrint publication year: 2014