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  - González-Avilés JJ

AU  - Guzmán FS

ED  - 

Y2  - 2024/09/20

ER  -