Bifurcation phenomena of the magnetofluid equations
We report on bifurcation studies for the incompressible magnetohydrodynamic equations in three space dimensions with periodic boundary conditions and a temporally constant external forcing. Fourier reprsentations of velocity, pressure and magnetic field have been used to transform the original parti...
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Universität Potsdam
1995
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ndltd-Potsdam-oai-kobv.de-opus-ubp-13582013-01-08T00:56:16Z Bifurcation phenomena of the magnetofluid equations Feudel Fred Seehafer, Norbert Schmidtmann, Olaf Physics We report on bifurcation studies for the incompressible magnetohydrodynamic equations in three space dimensions with periodic boundary conditions and a temporally constant external forcing. Fourier reprsentations of velocity, pressure and magnetic field have been used to transform the original partial differential equations into systems of ordinary differential equations (ODE), to which then special numerical methods for the qualitative analysis of systems of ODE have been applied, supplemented by the simulative calculation of solutions for selected initial conditions. In a part of the calculations, in order to reduce the number of modes to be retained, the concept of approximate inertial manifolds has been applied. For varying (incereasing from zero) strength of the imposed forcing, or varying Reynolds number, respectively, time-asymptotic states, notably stable stationary solutions, have been traced. A primary non-magnetic steady state loses, in a Hopf bifurcation, stability to a periodic state with a non-vanishing magnetic field, showing the appearance of a generic dynamo effect. From now on the magnetic field is present for all values of the forcing. The Hopf bifurcation is followed by furhter, symmetry-breaking, bifurcations, leading finally to chaos. We pay particular attention to kinetic and magnetic helicities. The dynamo effect is observed only if the forcing is chosen such that a mean kinetic helicity is generated; otherwise the magnetic field diffuses away, and the time-asymptotic states are non-magnetic, in accordance with traditional kinematic dynamo theory. Universität Potsdam Mathematisch-Naturwissenschaftliche Fakultät. Institut für Physik und Astronomie Wissenschaftliche Einrichtungen. Interdisziplinäres Zentrum Dynamik komplexer Systeme 1995 Preprint application/pdf urn:nbn:de:kobv:517-opus-13585 http://opus.kobv.de/ubp/volltexte/2007/1358/ eng http://opus.kobv.de/ubp/doku/urheberrecht.php |
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Physics |
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Physics Feudel Fred Seehafer, Norbert Schmidtmann, Olaf Bifurcation phenomena of the magnetofluid equations |
description |
We report on bifurcation studies for the incompressible magnetohydrodynamic equations in three space dimensions with periodic boundary conditions and a temporally constant external forcing. Fourier reprsentations of velocity, pressure and magnetic field have been used to transform the original partial differential equations into systems of ordinary differential equations (ODE), to which then special numerical methods for the qualitative analysis of systems of ODE have been applied, supplemented by the simulative calculation of solutions for selected initial conditions. In a part of the calculations, in order to reduce the number of modes to be retained, the concept of approximate inertial manifolds has been applied. For varying (incereasing from zero) strength of the imposed forcing, or varying Reynolds number, respectively, time-asymptotic states, notably stable stationary solutions, have been traced. A primary non-magnetic steady state loses, in a Hopf bifurcation, stability to a periodic state with a non-vanishing magnetic field, showing the appearance of a generic dynamo effect. From now on the magnetic field is present for all values of the forcing. The Hopf bifurcation is followed by furhter, symmetry-breaking, bifurcations, leading finally to chaos. We pay particular attention to kinetic and magnetic helicities. The dynamo effect is observed only if the forcing is chosen such that a mean kinetic helicity is generated; otherwise the magnetic field diffuses away, and the time-asymptotic states are non-magnetic, in accordance with traditional kinematic dynamo theory. |
author |
Feudel Fred Seehafer, Norbert Schmidtmann, Olaf |
author_facet |
Feudel Fred Seehafer, Norbert Schmidtmann, Olaf |
author_sort |
Feudel |
title |
Bifurcation phenomena of the magnetofluid equations |
title_short |
Bifurcation phenomena of the magnetofluid equations |
title_full |
Bifurcation phenomena of the magnetofluid equations |
title_fullStr |
Bifurcation phenomena of the magnetofluid equations |
title_full_unstemmed |
Bifurcation phenomena of the magnetofluid equations |
title_sort |
bifurcation phenomena of the magnetofluid equations |
publisher |
Universität Potsdam |
publishDate |
1995 |
url |
http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-13585 http://opus.kobv.de/ubp/volltexte/2007/1358/ |
work_keys_str_mv |
AT feudel bifurcationphenomenaofthemagnetofluidequations AT fred bifurcationphenomenaofthemagnetofluidequations AT seehafernorbert bifurcationphenomenaofthemagnetofluidequations AT schmidtmannolaf bifurcationphenomenaofthemagnetofluidequations |
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1716502016755236864 |