On the topology of the magnetic lines of solutions of the MHD equations

Fuente: arXiv
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Auteur principal: Ciampa, Gennaro
Format: Preprint
Publié: 2023
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author Ciampa, Gennaro
author_facet Ciampa, Gennaro
contents We construct examples of smooth periodic solutions to the Magnetohydrodynamic equations in dimension 2 with positive resistivity for which the topology of the magnetic lines changes under the flow. By Alfvén's theorem this is known to be impossible in the ideal case (resistivity = 0). In the resistive case the reconnection of the magnetic lines is known to occur and has deep physical implications, being responsible for many dynamic phenomena in astrophysics. The construction is a simplified proof of [3] and in addition we consider the case of the forced system.
format Preprint
id arxiv_https___arxiv_org_abs_2303_02999
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle On the topology of the magnetic lines of solutions of the MHD equations
Ciampa, Gennaro
Analysis of PDEs
We construct examples of smooth periodic solutions to the Magnetohydrodynamic equations in dimension 2 with positive resistivity for which the topology of the magnetic lines changes under the flow. By Alfvén's theorem this is known to be impossible in the ideal case (resistivity = 0). In the resistive case the reconnection of the magnetic lines is known to occur and has deep physical implications, being responsible for many dynamic phenomena in astrophysics. The construction is a simplified proof of [3] and in addition we consider the case of the forced system.
title On the topology of the magnetic lines of solutions of the MHD equations
topic Analysis of PDEs
url https://arxiv.org/abs/2303.02999