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 -