NUMERICAL EXPERIMENTS ON THE TWO-STEP EMERGENCE OF TWISTED MAGNETIC FLUX TUBES IN THE SUN

We present the new results of the two-dimensional numerical experiments on the cross-sectional evolution of a twisted magnetic flux tube rising from the deeper solar convection zone (--20,000 km) to the corona through the surface. The initial depth is 10 times deeper than most of the previous calcul...

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Veröffentlicht in:	The Astrophysical journal Jg. 735; H. 2; S. 126 - jQuery1323906737520='48'
Hauptverfasser:	Toriumi, S., Yokoyama, T.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Bristol IOP 10.07.2011
Schlagworte:	ACCELERATION Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ATMOSPHERES CHROMOSPHERE CONVECTION Earth, ocean, space ENERGY TRANSFER EVOLUTION Exact sciences and technology FLUID MECHANICS HEAT TRANSFER HYDRODYNAMICS MAGNETIC FIELDS MAGNETIC FLUX MAGNETOHYDRODYNAMICS MAIN SEQUENCE STARS MASS TRANSFER MECHANICS PARAMETRIC ANALYSIS PHOTOSPHERE PRESSURE GRADIENTS SOLAR ATMOSPHERE SOLAR CORONA STARS STELLAR ATMOSPHERES STELLAR CORONAE SUN TWO-DIMENSIONAL CALCULATIONS Solar corona Magnetic flux Plasma Magnetohydrodynamics Sun: interior Deceleration Flux tubes Sun: corona Digital simulation Numerical method Sun: photosphere Vortex pair methods: numerical Sun Convection Sun: chromosphere Pressure gradients Dynamics Instability Magnetic fields Solar interior magnetohydrodynamics (MHD) Twisted flux tube
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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