Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: Do flux pile-up models work?

S. Shelyag, Y. E. Litvinenko, V. Fedun, G. Verth, J. J. González-Avilés, F. S. Guzmán

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

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