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Cited article:

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Observational Signatures of Coronal Heating in Magnetohydrodynamic Simulations without Radiation or a Lower Atmosphere

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The Astrophysical Journal 942 (1) 10 (2023)
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Parallel Plasma Loops and the Energization of the Solar Corona

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Self-consistent nanoflare heating in model active regions: MHD avalanches

J Reid, J Threlfall and A W Hood
Monthly Notices of the Royal Astronomical Society 518 (1) 1584 (2022)
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Linking computational models to follow the evolution of heated coronal plasma

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Example of exponentially enhanced magnetic reconnection driven by a spatially bounded and laminar ideal flow

Allen H. Boozer and Todd Elder
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A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method

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Astronomy & Astrophysics 654 A2 (2021)
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Multi-Stranded Coronal Loops: Quantifying Strand Number and Heating Frequency from Simulated Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) Observations

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Solar Physics 296 (6) (2021)
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Investigating coronal wave energy estimates using synthetic non-thermal line widths

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Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points

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Magnetic Field Line Twisting by Photospheric Vortices: Energy Storage and Release

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