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Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT
H. P. Wang, S. Poedts, A. Lani, L. Linan, T. Baratashvili, F. Zhang, D. Sorokina, H.-J. Jeong, Y. C. Li, M. Najafi-Ziyazi and B. Schmieder Astronomy & Astrophysics 702 A37 (2025) https://doi.org/10.1051/0004-6361/202555760
High-frequency Alfvén waves and energy transfer within accretion disks of neutron star merger remnants
SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections
H. P. Wang, J. H. Guo, L. P. Yang, S. Poedts, F. Zhang, A. Lani, T. Baratashvili, L. Linan, R. Lin and Y. Guo Astronomy & Astrophysics 693 A257 (2025) https://doi.org/10.1051/0004-6361/202450771
Modeling the propagation of coronal mass ejections with COCONUT: Implementation of the regularized Biot-Savart law flux rope model
J. H. Guo, L. Linan, S. Poedts, Y. Guo, A. Lani, B. Schmieder, M. Brchnelova, B. Perri, T. Baratashvili, Y. W. Ni and P. F. Chen Astronomy & Astrophysics 683 A54 (2024) https://doi.org/10.1051/0004-6361/202347634
COCONUT-MF: Two-fluid ion-neutral global coronal modelling