Abstract
In this study, we aim to describe the first dynamic transitions of the MHD equations in a thin spherical shell. It is well known that the MHD equations admit a motionless steady state solution with constant vertically aligned magnetic field and linearly conducted temperature. This basic solution is stable for small Rayleigh numbers R and loses its stability at a critical threshold Rc. There are two possible sources for this instability. Either a set of real eigenvalues or a set of non-real eigenvalues cross the imaginary axis at Rc. We restrict ourselves to the study of the first case. In this case, by the center manifold reduction, we reduce the full PDE to a system of 2lc+1 ODE's where lc is a positive integer. We exhibit the most general reduction equation regardless of lc. Then, it is shown that for lc =1.2, the system either exhibits a continuous transition accompanied by an attractor homeomorphic to 2lc dimensional sphere which contains steady states of the system or a drastic transition accompanied by a repeller bifurcated on R<Rc. We show that there are parameter regimes where both types of transitions are realized. Besides, several identities involving the triple products of gradients of spherical harmonics are derived, which are useful for the study of related problems.
Original language | English |
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Pages (from-to) | 1531-1555 |
Number of pages | 25 |
Journal | Communications in Mathematical Sciences |
Volume | 17 |
Issue number | 6 |
DOIs | |
Publication status | Published - 2019 |
Bibliographical note
Publisher Copyright:© 2019 International Press.
Keywords
- Dynamical transition theory
- Linear stability
- Magnetohydrodynamics convection
- Principle of exchange of stabilities
- Spherical harmonics