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20212026
most citedSmall-scale dynamos: From idealized models to solar and stellar applications

36 citations · 150 across the 18 of their papers we have counts for

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astro-ph.SR2026

High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates II. Stellar Winds

Yue-Hong Chen, Julián D. Alvarado-Gómez, Xin Cheng +6

Observations suggest a connection between steady-wind mass loss and coronal X-ray activity in low-mass main-sequence stars. Interpreting this connection is challenging because the…

astro-ph.SR2025

High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates I. X-ray Coronae

Yue-Hong Chen, Julián D. Alvarado-Gómez, Xin Cheng +8

Stellar coronae are believed to be the main birthplace of various stellar magnetic activities. However, the structures and properties of stellar coronae remain poorly understood. U…

astro-ph.SR2024★ 4 cited

Small-scale and large-scale dynamos in global convection simulations of solar-like stars

Jörn Warnecke, Maarit J. Korpi-Lagg, Matthias Rheinhard +2

It has been recently shown numerically that a small-scale dynamo (SSD) instability could be possible in solar-like low magnetic Prandtl number plasmas. It has been proposed that th…

astro-ph.SR2023★ 24 cited

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

Jörn Warnecke, Maarit J. Korpi-Lagg, Frederick A. Gent +1

Magnetic fields on small scales are ubiquitous in the universe. Though they can often be observed in detail, their generation mechanisms are not fully understood. One possibility i…

astro-ph.SR2023

From convective stellar dynamo simulations to Zeeman-Doppler images

Thomas Hackman, Oleg Kochukhov, Mariangela Viviani +3

Zeeman-Doppler imaging (ZDI) is used to reconstruct the surface magnetic field of late-type stars from high resolution spectropolarimetric observations. The results are usually des…

astro-ph.SR2023★ 36 cited

Small-scale dynamos: From idealized models to solar and stellar applications

Matthias Rempel, Tanayveer Bhatia, Luis Bellot Rubio +1

In this article we review small-scale dynamo processes that are responsible for magnetic field generation on scales comparable to and smaller than the energy carrying scales of tur…

astro-ph.SR2022

Solar-Cycle Variation of quiet-Sun Magnetism and Surface Gravity Oscillation Mode

Maarit J. Korpi-Lagg, Andreas Korpi-Lagg, Nigul Olspert +1

The origin of the quiet Sun magnetism is under debate. Investigating the solar cycle variation observationally in more detail can give us clues about how to resolve the controversi…

astro-ph.SR2022★ 4 cited

V889 Her: abrupt changes in the magnetic field or differential rotation?

Teemu Willamo, Thomas Hackman, Jyri J. Lehtinen +2

We have applied Zeeman-Doppler imaging (ZDI) to an extensive spectropolarimetric HARPSpol data set of the magnetically active young solar analogue V889 Her, covering 35 spectra obt…