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Cited article:

Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

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The Astrophysical Journal 962 (2) 118 (2024)
https://doi.org/10.3847/1538-4357/ad1834

Turbulent dynamo action and its effects on the mixing at the convective boundary of an idealized oxygen-burning shell

G. Leidi, R. Andrassy, J. Higl, P. V. F. Edelmann and F. K. Röpke
Astronomy & Astrophysics 679 A132 (2023)
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Methodology for estimating the magnetic Prandtl number and application to solar surface small-scale dynamo simulations

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Interaction of convective plasma and small-scale magnetic fields in the lower solar atmosphere

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https://doi.org/10.1007/s41614-022-00094-0

3D simulations of oxygen shell burning with and without magnetic fields

Vishnu Varma and Bernhard Müller
Monthly Notices of the Royal Astronomical Society 504 (1) 636 (2021)
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Small‐scale dynamos in simulations of stratified turbulent convection

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Astronomische Nachrichten 339 (2-3) 127 (2018)
https://doi.org/10.1002/asna.201813477

Varying the forcing scale in low Prandtl number dynamos

A Brandenburg, N E L Haugen, Xiang-Yu Li and K Subramanian
Monthly Notices of the Royal Astronomical Society 479 (2) 2827 (2018)
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Small-scale Dynamo Simulations: Magnetic Field Amplification in Exploding Granules and the Role of Deep and Shallow Recirculation

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The Astrophysical Journal 859 (2) 161 (2018)
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Numerical simulations of quiet Sun magnetic fields seeded by the Biermann battery

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The Life Cycle of Active Region Magnetic Fields

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Saturation of the magnetorotational instability in the unstratified shearing box with zero net flux: convergence in taller boxes

Ji-Ming Shi, James M. Stone and Chelsea X. Huang
Monthly Notices of the Royal Astronomical Society 456 (3) 2273 (2016)
https://doi.org/10.1093/mnras/stv2815