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This article has been cited by the following article(s):
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Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures
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A New Broadening Technique of the Numerically Unresolved Solar Transition Region and Its Effect on the Spectroscopic Synthesis Using Coronal Approximation
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The Effect of Thermal Nonequilibrium on Helmet Streamers
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Corona and XUV emission modelling of the Sun and Sun-like stars
Static and dynamic solar coronal loops with cross-sectional area variations
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Reply to: Signatures of sunspot oscillations and the case for chromospheric resonances
Statistical Study of Chromospheric Evaporation in Impulsive Phase of Solar Flares
Viacheslav M Sadykov, Alexander G Kosovichev, Ivan N Sharykin and Graham S Kerr The Astrophysical Journal 871(1) 2 (2019) https://doi.org/10.3847/1538-4357/aaf6b0
The effects of numerical resolution, heating timescales and background heating on thermal non-equilibrium in coronal loops