Author:
FOURNIER J.-D.,GALTIER S.
Abstract
The one-dimensional MHD system first introduced by J.H. Thomas [Phys.
Fluids 11, 1245 (1968)] as a model of the dynamo effect is thoroughly studied in
the limit of large magnetic Prandtl number. The focus is on two types of localized solutions involving shocks (antishocks) and hollow (bump) waves. Numerical
simulations suggest phenomenological rules concerning their generation, stability
and basin of attraction. Their topology, amplitude and thickness are compared
favourably with those of the meromorphic travelling waves, which are obtained
exactly, and respectively those of asymptotic descriptions involving rational
or degenerate elliptic functions. The meromorphy bars the existence of certain
configurations, while others are explained by assuming imaginary residues. These
explanations are tested using the numerical amplitude and phase of the Fourier transforms
as probes of the analyticity properties. Theoretically, the proof of the partial integrability
backs up the role ascribed to meromorphy. Practically, predictions are
derived for MHD plasmas.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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1. Turbulence in space plasmas and beyond;Journal of Physics A: Mathematical and Theoretical;2018-06-12