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Cited article:

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Extreme-ultraviolet (EUV) observables of simulated plasmoid-mediated reconnection in the solar corona

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Oscillatory Reconnection of a 2D X-point in a Hot Coronal Plasma

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The Independence of Oscillatory Reconnection Periodicity from the Initial Pulse

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The Formation and Dissipation of Current Sheets and Shocks due to Compressive Waves in a Stratified Atmosphere Containing a Magnetic Null

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Fast-to-Alfvén Mode Conversion Mediated by Hall Current. II. Application to the Solar Atmosphere

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Generation Mechanisms of Quasi-parallel and Quasi-circular Flare Ribbons in a Confined Flare

Aaron Hernandez-Perez, Julia K. Thalmann, Astrid M. Veronig, Yang Su, Peter Gömöry and Ewan C. Dickson
The Astrophysical Journal 847 (2) 124 (2017)
https://doi.org/10.3847/1538-4357/aa8814