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Cited article:

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Effect of numerical resolution on synthetic observables of simulated coronal loops

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Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC. II. Optimization and Application in 3D Models

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Filament Mass Losses Forced by Magnetic Reconnection in the Solar Corona

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The evolution of the coronal loop structure due to the phase mixing of high and low-frequency Alfvén waves

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Monthly Notices of the Royal Astronomical Society 535 (2) 1640 (2024)
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Improving Coronal Hole Detections and Open Flux Estimates

Ronald M. Caplan, Emily I. Mason, Cooper Downs and Jon A. Linker
The Astrophysical Journal 958 (1) 43 (2023)
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How numerical treatments of the transition region modify energy flux into the solar corona

T A Howson and C Breu
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Multi-Scale Variability of Coronal Loops Set by Thermal Non-Equilibrium and Instability as a Probe for Coronal Heating

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Frontiers in Astronomy and Space Sciences 9 (2022)
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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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