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Cited article:

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Properties of Turbulent Convection and Large-scale Flows in a Rotating F-type Star Revealed by 3D Realistic Radiative Hydrodynamic Simulations

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The Astrophysical Journal 991 (2) 187 (2025)
https://doi.org/10.3847/1538-4357/adfbe4

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Astronomy & Astrophysics 681 A81 (2024)
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Why Observations at Mid-infrared Wavelengths Partially Mitigate M Dwarf Star Host Stellar Activity Contamination in Exoplanet Transmission Spectroscopy

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Magnetic origin of the discrepancy between stellar limb-darkening models and observations

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Nature Astronomy 8 (7) 929 (2024)
https://doi.org/10.1038/s41550-024-02252-5

Spectral variability of photospheric radiation due to faculae – II. Facular contrasts for cool main-sequence stars

Charlotte M Norris, Yvonne C Unruh, Veronika Witzke, Sami K Solanki, Natalie A Krivova, Alexander I Shapiro, Kok Leng Yeo, Robert Cameron and Benjamin Beeck
Monthly Notices of the Royal Astronomical Society 524 (1) 1139 (2023)
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Small-Scale Dynamos: From Idealized Models to Solar and Stellar Applications

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The effect of stellar contamination on low-resolution transmission spectroscopy: needs identified by NASA’s Exoplanet Exploration Program Study Analysis Group 21

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On the influence of magnetic topology on the propagation of internal gravity waves in the solar atmosphere

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A Refined Model of Convectively Driven Flicker in Kepler Light Curves

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Forward modelling of Kepler-band variability due to faculae and spots

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The Umbral-penumbral Boundary in Sunspots in the Context of Magnetoconvection

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Internal Gravity Waves in the Magnetized Solar Atmosphere. II. Energy Transport

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