Hostname: page-component-848d4c4894-x24gv Total loading time: 0 Render date: 2024-05-14T05:14:08.023Z Has data issue: false hasContentIssue false

Resonant structures within incompressible ideal MHD

Published online by Cambridge University Press:  13 March 2009

C. Zorzan
Affiliation:
Department of Mathematics, Royal Melbourne Institute of Technology, Melbourne, Victoria 3000, Australia
P. S. Cally
Affiliation:
Department of Mathematics, Monash University, Clayton, Victoria 3168, Australia

Abstract

The resonant characteristics of an incompressible ideal MHD fluid are highly structured. To help expose this structure, an equivalent electrical analogue of the MHD system is developed. The model, in the form of a transmission line, makes it possible to identify a number of new and important concepts, one of which is the effective impedance. This in turn enables entire regions of MHD fluid to be replaced with equivalent impedances. When fully exploited, the model also provides a more consistent interpretation of the spectrum of ideal MHD. The discrete Alfvén modes are found to be highly degenerate, while the transition to a discontinuous profile is accompanied by a redistribution of an uncountably infinite number of ‘poles’ from the continuous spectrum and onto the Alfvén modes. In addition, the electrical analogue shows that within a continuously structured fluid the characteristic behaviour is not necessarily dominated by the ‘surface mode’ alone. This view is also supported by the results of a numerical simulation of the linear MHD equations. Depending on the initial conditions, the collective behaviour can have any frequency within the range spanned by the transition zone. The energy itself is monitored using a new pair of energy and flux expressions derived from a variational (Lagrangian) description of the MHD system. Again the electrical model is used to provide a physical interpretation of the individual terms within these expressions. In particular, it allows a partition of the total energy into separate kinetic- and potential-energy terms.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1992

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Adam, J. A. 1986 Phys. Rep. 142, 263.CrossRefGoogle Scholar
Barston, E. M. 1964 Ann. Phys. (NY) 29, 282.CrossRefGoogle Scholar
Briggs, R. J., Daugherty, J. D. & Levy, R. H. 1970 Phys. Fluids 13, 421.CrossRefGoogle Scholar
Cally, P. S. 1991 J. Plasma Phys. 45, 453.CrossRefGoogle Scholar
Crawford, J. D. & Hislop, P. D. 1989 Ann. Phys. (NY) 189, 265.CrossRefGoogle Scholar
Davila, J. M. 1987 Astrophys. J. 317, 514.CrossRefGoogle Scholar
Finlayson, B. A. 1972 The Method of Weighted Residuals and Variational Principles. Academic.Google Scholar
Hasegawa, A. & Chen, L. 1974 Phys. Rev. Lett. 32, 454.CrossRefGoogle Scholar
Hollweg, J. V. 1987 Astrophys. J. 312, 880.CrossRefGoogle Scholar
Ionson, J. A. 1978 Astrophys. J. 226, 650.CrossRefGoogle Scholar
Kappraff, J. M. & Tataronis, J. A. 1977 J. Plasma Phys. 18, 209.CrossRefGoogle Scholar
Kuo, F. F. 1966 Network Analysis and Synthesis. Wiley.Google Scholar
Lee, M. A. & Roberts, B. 1986 Astrophys. J. 301, 430.CrossRefGoogle Scholar
Leroy, B. 1980 Astron. Astrophys. 91, 136.Google Scholar
Leroy, B. 1981 Astron. Astrophys. 97, 245.Google Scholar
Leroy, B. 1985 Geophys. Aslrophys. Fluid Dyn. 32, 123.CrossRefGoogle Scholar
Leroy, B. & Bel, N. 1979 Astron. Astrophys. 78, 129.Google Scholar
Poedts, S., Kerner, W. & Goossens, M. 1989 J. Plasma Phys. 42, 27.CrossRefGoogle Scholar
Sedláček, Z. 1971 J. Plasma Phys. 5, 239.CrossRefGoogle Scholar
Sedláček, Z. & Roberts, B. 1989 J. Plasma Phys. 41, 97.CrossRefGoogle Scholar
Steinolfson, R. S. 1984 Phys. Fluids 27, 781.CrossRefGoogle Scholar
Steinolfson, R. S. 1985 Astrophys. J. 295, 213.CrossRefGoogle Scholar
Temes, G. C. & LaPatra, J. W. 1977 Introduction to Circuit Analysis. McGraw-Hill.Google Scholar
Vainberg, M. M. 1973 Variational Method and Method of Monotone Operators. Wiley.Google Scholar
Weitzner, H. 1963 Phys. Fluids 6, 1123.CrossRefGoogle Scholar
Weitzner, H. 1964 Phys. Fluids 7, 476.CrossRefGoogle Scholar
Weitzner, H. 1965 Commun. Pure Appl. Maths 18, 307.CrossRefGoogle Scholar
Wentzel, D. G. 1979 Astrophys. J. 233, 756.CrossRefGoogle Scholar