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Cited article:

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

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Effects of Magnetic Perturbation on Reconnection and Heating in the Solar Corona

Mostafa M. Hammoud, Ghassan Y. Antar, Maher A. Dayeh, Marwan S. Darwish and Mounib F. El Eid
The Astrophysical Journal 903 (2) 95 (2020)
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Magnetic Helicity Reversal in the Corona at Small Plasma Beta

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

Yann Pfau-Kempf, Markus Battarbee, Urs Ganse, et al.
Frontiers in Physics 6 (2018)
https://doi.org/10.3389/fphy.2018.00044

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

Haixia Xie, Maria S. Madjarska, Bo Li, Zhenghua Huang, Lidong Xia, Thomas Wiegelmann, Hui Fu and Chaozhou Mou
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GIANT CORONAL LOOPS DOMINATE THE QUIESCENT X-RAY EMISSION IN RAPIDLY ROTATING M STARS

O. Cohen, R. Yadav, C. Garraffo, S. H. Saar, S. J. Wolk, V. L. Kashyap, J. J. Drake and I. Pillitteri
The Astrophysical Journal 834 (1) 14 (2017)
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Plasma Beta Stratification in the Solar Atmosphere: A Possible Explanation for the Penumbra Formation

Ph.-A. Bourdin
The Astrophysical Journal Letters 850 (2) L29 (2017)
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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