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Cited article:

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Data-driven Simulations of Magnetic Field Evolution in Active Region 11429: Magneto-frictional Method Using PENCIL CODE

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Research in Astronomy and Astrophysics 24 (2) 025007 (2024)
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Effects of Magnetic Perturbation on Reconnection and Heating in the Solar Corona

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Magnetic Helicity Reversal in the Corona at Small Plasma Beta

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Observationally quantified reconnection providing a viable mechanism for active region coronal heating

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On the Importance of Spatial and Velocity Resolution in the Hybrid-Vlasov Modeling of Collisionless Shocks

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Frontiers in Physics 6 (2018)
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Plasma Beta Stratification in the Solar Atmosphere: A Possible Explanation for the Penumbra Formation

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The Astrophysical Journal Letters 850 (2) L29 (2017)
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GIANT CORONAL LOOPS DOMINATE THE QUIESCENT X-RAY EMISSION IN RAPIDLY ROTATING M STARS

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The Plasma Parameters and Geometry of Cool and Warm Active Region Loops

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EXPLAINING INVERTED-TEMPERATURE LOOPS IN THE QUIET SOLAR CORONA WITH MAGNETOHYDRODYNAMIC WAVE-MODE CONVERSION

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The Astrophysical Journal 831 (1) 10 (2016)
https://doi.org/10.3847/0004-637X/831/1/10