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Cited article:

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Coriolis darkening in late-type stars

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Magnetohydrodynamic simulations of A-type stars: Long-term evolution of core dynamo cycles

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Small-Scale Dynamos: From Idealized Models to Solar and Stellar Applications

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Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers

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Causality in heliophysics: Magnetic fields as a bridge between the Sun’s interior and the Earth’s space environment

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Simulations of Solar and Stellar Dynamos and Their Theoretical Interpretation

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Space Science Reviews 219 (7) (2023)
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Simulations of dynamo action in slowly rotating M dwarfs: Dependence on dimensionless parameters

C. A. Ortiz-Rodríguez, P. J. Käpylä, F. H. Navarrete, D. R. G. Schleicher, R. E. Mennickent, J. P. Hidalgo and B. Toro-Velásquez
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Mean-field Analysis on Large-scale Magnetic Fields at High Reynolds Numbers

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The Astrophysical Journal 935 (1) 55 (2022)
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Solar evolution and extrema: current state of understanding of long-term solar variability and its planetary impacts

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A Knee Point in the Rotation–Activity Scaling of Late-type Stars with a Connection to Dynamo Transitions

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Sensitivity to luminosity, centrifugal force, and boundary conditions in spherical shell convection

P. J. Käpylä, F. A. Gent, N. Olspert, M. J. Käpylä and A. Brandenburg
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Rotational dependence of turbulent transport coefficients in global convective dynamo simulations of solar-like stars

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https://doi.org/10.1051/0004-6361/201936922

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Stellar Dynamos in the Transition Regime: Multiple Dynamo Modes and Antisolar Differential Rotation

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The Astrophysical Journal 886 (1) 21 (2019)
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Effects of a subadiabatic layer on convection and dynamos in spherical wedge simulations

P. J. Käpylä, M. Viviani, M. J. Käpylä, A. Brandenburg and F. Spada
Geophysical & Astrophysical Fluid Dynamics 113 (1-2) 149 (2019)
https://doi.org/10.1080/03091929.2019.1571584

Small‐scale dynamos in simulations of stratified turbulent convection

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Astronomische Nachrichten 339 (2-3) 127 (2018)
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Turbulent transport coefficients in spherical wedge dynamo simulations of solar-like stars

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Astronomy & Astrophysics 609 A51 (2018)
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Consequences of high effective Prandtl number on solar differential rotation and convective velocity

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Transition from axi- to nonaxisymmetric dynamo modes in spherical convection models of solar-like stars

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Convective Velocity Suppression via the Enhancement of the Subadiabatic Layer: Role of the Effective Prandtl Number

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The Astrophysical Journal 851 (2) 74 (2017)
https://doi.org/10.3847/1538-4357/aa9b7f

Long‐term variations of turbulent transport coefficients in a solarlike convective dynamo simulation

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Astronomische Nachrichten 338 (8) 885 (2017)
https://doi.org/10.1002/asna.201713406

Influence of a coronal envelope as a free boundary to global convective dynamo simulations

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Astronomy & Astrophysics 596 A115 (2016)
https://doi.org/10.1051/0004-6361/201526131