TY - GEN T1 - Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: do flux pile-up models work? T2 - arXiv PY - 2018/09/03 AU - Shelyag S AU - Litvinenko YE AU - Fedun V AU - Verth G AU - Gonz谩lez-Avil茅s JJ AU - Guzm谩n FS ED - Y2 - 2025/01/07 ER -