Solar Flux Emergence Simulations

We simulate the rise through the upper convection zone and emergence through the solar surface of initially uniform, untwisted, horizontal magnetic flux, with the same entropy as the nonmagnetic plasma, that is advected into a domain 48 Mm wide by 20 Mm deep. The magnetic field is advected upward by...

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Veröffentlicht in:	Solar physics 2011-02, Vol.268 (2), p.271-282
Hauptverfasser:	Stein, R. F., Lagerfjärd, A., Nordlund, Å., Georgobiani, D.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics and Astroparticles Atmospheric Sciences Buoyancy Entropy Helioseismology Magnetic fields Physics Physics and Astronomy Plasma Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Sun
Online-Zugang:	Volltext
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