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Cited article:

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Evolution of solar and stellar coronal abundances owing to magnetic activity

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Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 384 (2323) (2026)
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3D MHD Simulations of Coronal Loops Heated via Magnetic Braiding. II. Automatic Detection of Reconnection Outflows and Statistical Analysis of Their Properties

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3D MHD Simulations of Coronal Loops Heated via Magnetic Braiding. I. Continuous Driving

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Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures

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On the Connection of Coronal Loop Plasma with the Ambient Magnetic Field

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Avalanches in magnetohydrodynamical simulations

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Effect of numerical resolution on synthetic observables of simulated coronal loops

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Systematic Nonthermal Velocity Increase Preceding Soft X-Ray Flare Onset: A Large-scale Hinode/EIS Study

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Turbulence and particle energization in twisted flux ropes under solar-wind conditions

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