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Cited article:

Effect of numerical resolution on synthetic observables of simulated coronal loops

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Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops

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Astronomy & Astrophysics 693 A312 (2025)
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Coronal heating driven by random foot point motions: the effects of magnetic field topology

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Periodic Coronal Rain Driven by Self-consistent Heating Process in a Radiative Magnetohydrodynamic Simulation

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The Astrophysical Journal Letters 973 (1) L1 (2024)
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AWSoM Magnetohydrodynamic Simulation of a Solar Active Region. II. Statistical Analysis of Alfvén Wave Dissipation and Reflection, Scaling Laws, and Energy Budget on Coronal Loops

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Non-thermal broadening of coronal lines in a 3D MHD loop model

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MUSE observations of small-scale heating events

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Damping of coronal oscillations in self-consistent 3D radiative magnetohydrodynamics simulations of the solar atmosphere

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Quantifying Poynting Flux in the Quiet Sun Photosphere

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The Astrophysical Journal 956 (2) 83 (2023)
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Magnetic Tornado Properties: A Substantial Contribution to the Solar Coronal Heating via Efficient Energy Transfer

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The Astrophysical Journal 949 (1) 8 (2023)
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How numerical treatments of the transition region modify energy flux into the solar corona

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Deciphering Solar Coronal Heating: Energizing Small-scale Loops through Surface Convection

D. Nóbrega-Siverio, F. Moreno-Insertis, K. Galsgaard, K. Krikova, L. Rouppe van der Voort, R. Joshi and M. S. Madjarska
The Astrophysical Journal Letters 958 (2) L38 (2023)
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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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