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Formation of a Coronal Hole by a Quiet-Sun Filament Eruption
Stefan J. Hofmeister, Eleanna Asvestari, Karin Dissauer, Michael Hahn, Stephan G. Heinemann, Veronika Jercic, Alexandros Koukras, Kilian Krikova, Jonas Saqri, Daniel W. Savin, Manuela Temmer and Astrid Veronig The Astrophysical Journal 994(2) 190 (2025) https://doi.org/10.3847/1538-4357/ae11b0
Representation learning for time-domain high-energy astrophysics: Discovery of extragalactic fast X-ray transient XRT 200515
Steven Dillmann, Juan Rafael Martínez-Galarza, Roberto Soria, Rosanne Di Stefano and Vinay L Kashyap Monthly Notices of the Royal Astronomical Society 537(2) 931 (2025) https://doi.org/10.1093/mnras/stae2808
Time-dependent heating problem of the solar corona in fractal dimensions: A plausible solution
Numerical simulations of macrospicule jets under energy imbalance conditions in the solar atmosphere
J J González-Avilés, K Murawski, A K Srivastava, T V Zaqarashvili and J A González-Esparza Monthly Notices of the Royal Astronomical Society 505(1) 50 (2021) https://doi.org/10.1093/mnras/stab1261
The Direct Relation between the Duration of Magnetic Reconnection and the Evolution of GOES Light Curves in Solar Flares
F. Reale, S. Orlando, M. Guarrasi, A. Mignone, G. Peres, A. W. Hood and E. R. Priest The Astrophysical Journal 830(1) 21 (2016) https://doi.org/10.3847/0004-637X/830/1/21
PLASMA SLOSHING IN PULSE-HEATED SOLAR AND STELLAR CORONAL LOOPS
OBSERVING THE FORMATION OF FLARE-DRIVEN CORONAL RAIN
E. Scullion, L. Rouppe van der Voort, P. Antolin, S. Wedemeyer, G. Vissers, E. P. Kontar and P. T. Gallagher The Astrophysical Journal 833(2) 184 (2016) https://doi.org/10.3847/1538-4357/833/2/184
Modelling nanoflares in active regions and implications for coronal heating mechanisms
P. J. Cargill, H. P. Warren and S. J. Bradshaw Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 373(2042) 20140260 (2015) https://doi.org/10.1098/rsta.2014.0260
Numerical simulations of transverse oscillations in radiatively cooling coronal loops