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Turbulence and particle energization in twisted flux ropes under solar-wind conditions
O. Pezzi, D. Trotta, S. Benella, L. Sorriso-Valvo, F. Malara, F. Pucci, C. Meringolo, W. H. Matthaeus and S. Servidio Astronomy & Astrophysics 686 A116 (2024) https://doi.org/10.1051/0004-6361/202348700
The Lorentz Force at Work: Multiphase Magnetohydrodynamics throughout a Flare Lifespan
From kink instability to magnetic reconnection to oscillations in solar flares
Philippa K. Browning, Mykola Gordovskyy, Luiz A.C.A. Schiavo and James Stewart Fundamental Plasma Physics 10 100049 (2024) https://doi.org/10.1016/j.fpp.2024.100049
Magnetohydrodynamic Turbulence Formation in Solar Flares: 3D Simulation and Synthetic Observations
The Triple-layered Leading Edge of Solar Coronal Mass Ejections
Z. X. Mei, R. Keppens, Q. W. Cai, J. Ye, Y. Li, X. Y. Xie and J. Lin The Astrophysical Journal Letters 898(1) L21 (2020) https://doi.org/10.3847/2041-8213/aba2ce
Phase-modulated X-Ray Emission from Cepheids due to Pulsation-driven Shocks
Sofia-Paraskevi Moschou, Nektarios Vlahakis, Jeremy J. Drake, Nancy Remage Evans, Hilding R. Neilson, Joyce Ann Guzik and John ZuHone The Astrophysical Journal 900(2) 157 (2020) https://doi.org/10.3847/1538-4357/aba8fa
Combining MHD and kinetic modelling of solar flares
Localized Microwave and EUV Bright Structures in an Eruptive Prominence
Jing Huang, Baolin Tan, Satoshi Masuda, Xin Cheng, Susanta Kumar Bisoi and Victor Melnikov The Astrophysical Journal 874(2) 176 (2019) https://doi.org/10.3847/1538-4357/ab0e80
Forward Modeling of SDO/AIA and X-Ray Emission from a Simulated Flux Rope Ejection
Xiaozhou 小舟 Zhao 赵, Chun Xia, Tom Van Doorsselaere, Rony Keppens and Weiqun Gan The Astrophysical Journal 872(2) 190 (2019) https://doi.org/10.3847/1538-4357/ab0284
Solar flares and Kelvin-Helmholtz instabilities: A parameter survey
Observational Signatures of a Kink-unstable Coronal Flux Rope Using Hinode/EIS
B. Snow, G. J. J. Botha, S. Régnier, R. J. Morton, E. Verwichte and P. R. Young The Astrophysical Journal 842(1) 16 (2017) https://doi.org/10.3847/1538-4357/aa6d0e
THE ROLE OF KELVIN–HELMHOLTZ INSTABILITY FOR PRODUCING LOOP-TOP HARD X-RAY SOURCES IN SOLAR FLARES