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

Aims. We study the process of magnetic field annihilation and reconnection in simulations of magnetised solar photosphere and chromosphere with magnetic fields of opposite polarities and constant numerical resistivity. Methods. Exact analytical solutions for reconnective annihilations were used to i...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2018-12, Vol.620, p.A159
Hauptverfasser:	Shelyag, S., Litvinenko, Y. E., Fedun, V., Verth, G., González-Avilés, J. J., Guzmán, F. S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmosphere Atmospheric models Chromosphere Computational fluid dynamics Computer simulation Convection Fluctuations Magnetic field reconnection Magnetic fields Magnetic flux Magnetism Magnetohydrodynamic simulation Numerical methods Photosphere Simulation Solar atmosphere Solar magnetic field Sun: atmosphere Sun: chromosphere Sun: magnetic fields Sun: photosphere
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