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Self-consistent 3D radiative magnetohydrodynamic simulations of coronal rain formation and evolution

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Modelling the solar transition region using an adaptive conduction method

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Coronal Rain in Randomly Heated Arcades

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Revisiting the formation mechanism for coronal rain from previous studies

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Research in Astronomy and Astrophysics 21 (10) 255 (2021)
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A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)

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On-disk Solar Coronal Condensations Facilitated by Magnetic Reconnection between Open and Closed Magnetic Structures

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Magnetic field inference in active region coronal loops using coronal rain clumps

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Effect of optically thin cooling curves on condensation formation: Case study using thermal instability

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Transverse kink oscillations of inhomogeneous prominence threads: Numerical analysis and Hα forward modelling

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The role of asymmetries in coronal rain formation during thermal non-equilibrium cycles

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Transition region adaptive conduction (TRAC) in multidimensional magnetohydrodynamic simulations

Yu-Hao Zhou, Wen-Zhi Ruan, Chun Xia and Rony Keppens
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