Magnetic topology in fluids
Amir Jafari, Ethan Vishniac

TL;DR
This paper explores magnetic topology in turbulent fluids using topological and dynamical systems theory, revealing that topology is well-defined in phase space and that reconnection relates to entropy increase and time irreversibility.
Contribution
It introduces a phase space perspective for magnetic topology, challenging the literal interpretation of magnetic field lines and linking reconnection to thermodynamic entropy.
Findings
Magnetic topology is well-defined in phase space, not in real space.
Time reversal invariance holds for ideal, continuous fields, but not when resistivity causes entropy increase.
Reconnection is driven by entropy increase and stochastic disturbances at small scales.
Abstract
We study the evolution of turbulent magnetic fields from a topological point of view, invoking commonplace mathematical tools from general topology and dynamical systems theory which connect magnetic field evolution to time reversal invariance, entropy increase and the second law of thermodynamics. We show that in fact magnetic topology is well-defined only in the phase space corresponding to a dynamical system governed by the induction equation. Hence the field's topology and stochasticity can be studied in terms of the corresponding phase space trajectories rather than the field lines in real Euclidean space. In fact, our results suggest that magnetic field lines should not be taken too literally because their existence and uniqueness and more importantly continuity in time require strong mathematical conditions, hardly satisfied in astrophysical systems. As for magnetic topology…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Solar and Space Plasma Dynamics · Complex Systems and Time Series Analysis
