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Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions
Lucas A. Tarr, N. Dylan Kee, Mark G. Linton, Peter W. Schuck and James E. Leake The Astrophysical Journal Supplement Series 270(2) 30 (2024) https://doi.org/10.3847/1538-4365/ad0e0c
A Near-half-century Simulation of the Solar Corona
Valentin Aslanyan, Karen A. Meyer, Roger B. Scott and Anthony R. Yeates The Astrophysical Journal Letters 961(1) L3 (2024) https://doi.org/10.3847/2041-8213/ad1934
Photospheric Pore Rotation Associated with a C-class Flare from Spectropolarimetric Observations with DKIST
Rahul Yadav, Maria D. Kazachenko, Andrey N. Afanasyev, Gianna Cauzzi and Kevin Reardon The Astrophysical Journal Letters 973(1) L10 (2024) https://doi.org/10.3847/2041-8213/ad758d
Energy and helicity evolution in a flux emergence simulation
Thermodynamic and Magnetic Topology Evolution of the X1.0 Flare on 2021 October 28 Simulated by a Data-driven Radiative Magnetohydrodynamic Model
J. H. Guo, Y. W. Ni, Z. Zhong, Y. Guo, C. Xia, H. T. Li, S. Poedts, B. Schmieder and P. F. Chen The Astrophysical Journal Supplement Series 266(1) 3 (2023) https://doi.org/10.3847/1538-4365/acc797
Effects of optimisation parameters on data-driven magnetofrictional modelling of active regions
Self-consistent propagation of flux ropes in realistic coronal simulations
L. Linan, F. Regnault, B. Perri, M. Brchnelova, B. Kuzma, A. Lani, S. Poedts and B. Schmieder Astronomy & Astrophysics 675 A101 (2023) https://doi.org/10.1051/0004-6361/202346235
Investigating the associations between solar flares and magnetic complexity of active regions