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Cited article:

Coronal heating driven by random foot point motions: the effects of magnetic field topology

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G. Cozzo, P. Pagano, F. Reale, P. Testa, A. Petralia, J. Martinez-Sykora, V. Hansteen and B. De Pontieu
Astronomy & Astrophysics 695 A40 (2025)
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Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops

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Transverse MHD Waves as Signatures of Braiding-induced Magnetic Reconnection in Coronal Loops

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The Astrophysical Journal Letters 961 (1) L17 (2024)
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Coronal energy release by MHD avalanches

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The thermodynamic response of heating at coronal null points

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How numerical treatments of the transition region modify energy flux into 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
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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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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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Linking computational models to follow the evolution of heated coronal plasma

J Reid, P J Cargill, C D Johnston and A W Hood
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Coronal Mini-jets in an Activated Solar Tornado-like Prominence

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The Astrophysical Journal 899 (1) 19 (2020)
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Nanoflare Diagnostics from Magnetohydrodynamic Heating Profiles

K. J. Knizhnik, W. T. Barnes, J. W. Reep and V. M. Uritsky
The Astrophysical Journal 899 (2) 156 (2020)
https://doi.org/10.3847/1538-4357/aba959