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6 - Spectral theory

Published online by Cambridge University Press:  22 February 2010

J. P. Hans Goedbloed
Affiliation:
FOM-Instituut voor Plasmyafysica, Nieuwegein
Stefaan Poedts
Affiliation:
Centre for Plasma Astrophysics, KU Leuven
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Summary

Stability: intuitive approach

Two viewpoints

How does one know whether a dynamical system is stable or not? Consider the well-known example of a ball at rest at the bottom of a trough or on the top of a hill (Fig. 6.1). There is a position (indicated by the full circle) where the potential energy W due to gravity has an extremum W0. Displacing the ball slightly to a neighbouring position (at the open circle) results in either a higher or a lower potential energy W1. This corresponds to a stable system in the first case (W1 > W0) and an unstable system in the second case (W1 < W0).

Already at this stage some important observations can be made, viz.:

  1. (a) We have tacitly assumed that the constraining surface is curved, i.e. either convex or concave, so that there is a position of rest, which is called the equilibrium position. In this case, one may rescale the potential energy such that the equilibrium state corresponds to W0 = 0, and W1 becomes the potential energy of the displacement, which is called the perturbation.

  2. (b) If the constraining surface is flat and inclined, the system is not in equilibrium and the ball simply rolls along the plane. This lack of equilibrium, when W has no extremum, should be well distinguished from neutral or marginal stability, when W1 = W0. The latter situation occurs when the surface is horizontal, so that the value W = 0 may be assigned to both W0 and W1.

Type
Chapter
Information
Principles of Magnetohydrodynamics
With Applications to Laboratory and Astrophysical Plasmas
, pp. 230 - 299
Publisher: Cambridge University Press
Print publication year: 2004

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  • Spectral theory
  • J. P. Hans Goedbloed, FOM-Instituut voor Plasmyafysica, Nieuwegein, Stefaan Poedts, Centre for Plasma Astrophysics, KU Leuven
  • Book: Principles of Magnetohydrodynamics
  • Online publication: 22 February 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511616945.007
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  • Spectral theory
  • J. P. Hans Goedbloed, FOM-Instituut voor Plasmyafysica, Nieuwegein, Stefaan Poedts, Centre for Plasma Astrophysics, KU Leuven
  • Book: Principles of Magnetohydrodynamics
  • Online publication: 22 February 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511616945.007
Available formats
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Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Spectral theory
  • J. P. Hans Goedbloed, FOM-Instituut voor Plasmyafysica, Nieuwegein, Stefaan Poedts, Centre for Plasma Astrophysics, KU Leuven
  • Book: Principles of Magnetohydrodynamics
  • Online publication: 22 February 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511616945.007
Available formats
×