Turbulent transport coefficients in galactic dynamo simulations using singular value decomposition
Abhijit B. Bendre, Kandaswamy Subramanian, Detlef Elstner, Oliver, Gressel

TL;DR
This paper applies singular value decomposition to directly measure turbulent transport coefficients in galactic dynamo simulations, enabling better understanding of magnetic field generation in galaxies.
Contribution
The study introduces the use of SVD to accurately determine turbulent transport coefficients from simulation data, offering an effective alternative to existing methods.
Findings
SVD-derived EMF profiles match simulation data well
SVD coefficients successfully reproduce mean magnetic field evolution
Results show qualitative agreement with test-field method
Abstract
Coherent magnetic fields in disc galaxies are thought to be generated by a large-scale (or mean-field) dynamo operating in their interstellar medium. A key driver of mean magnetic field growth is the turbulent electromotive force (EMF), which represents the influence of correlated small-scale (or fluctuating) velocity and magnetic fields on the mean field. The EMF is usually expressed as a linear expansion in the mean magnetic field and its derivatives, with the dynamo tensors as expansion coefficients. Here, we adopt the singular value decomposition (SVD) method to directly measure these turbulent transport coefficients in a simulation of the turbulent interstellar medium that realizes a large-scale dynamo. Specifically, the SVD is used to least-square fit the time series data of the EMF with that of the mean field and its derivatives, to determine these coefficients. We demonstrate…
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