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Transition of Magnetohydrodynamical Waves in the Solar Atmosphere

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Advances in Turbulence
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Abstract

Transition to irregular behaviour of Magnetohydrodynamical (MHD) waves is investigated using a simple four-mode dynamical system worked out from the basic MHD equations by means of a Fourier and a multiple-scale analysis. In the initial stage of the transition, when most of the energy in concentrated in the low-wave-number Fourier component, the system behaves like a van dr Pol oscillator, exhibiting saddlenode bifurcations. Hopf bifurcations are found numerically when the low- and high-wavenumber components have comparable magnitude. Two Hopf bifurcations leading to a two-D torus are followed by bifurcation to a nonperiodic attractor.

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References

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© 1987 Springer-Verlag Berlin Heidelberg

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Nocera, L. (1987). Transition of Magnetohydrodynamical Waves in the Solar Atmosphere. In: Comte-Bellot, G., Mathieu, J. (eds) Advances in Turbulence. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-83045-7_33

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  • DOI: https://doi.org/10.1007/978-3-642-83045-7_33

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-83047-1

  • Online ISBN: 978-3-642-83045-7

  • eBook Packages: Springer Book Archive

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