CORONAL RAIN IN MAGNETIC ARCADES: REBOUND SHOCKS, LIMIT CYCLES, AND SHEAR FLOWS

ABSTRACT We extend our earlier multidimensional, magnetohydrodynamic simulations of coronal rain occurring in magnetic arcades with higher resolution, grid-adaptive computations covering a much longer (>6 hr) time span. We quantify how blob-like condensations forming in situ grow along and across...

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Veröffentlicht in:	The Astrophysical journal 2015-07, Vol.807 (2), p.1-15
Hauptverfasser:	Fang, X., Xia, C., Keppens, R., Doorsselaere, T. Van
Format:	Artikel
Sprache:	eng
Schlagworte:	Arcades ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CALCULATION METHODS Computer simulation COMPUTERIZED SIMULATION Condensing CORRELATIONS DENSITY Dynamics FILAMENTS KINETIC ENERGY LIMIT CYCLE MAGNETOHYDRODYNAMICS magnetohydrodynamics(MHD) Rain RESOLUTION SHEAR Shear flow Siphons SOLAR CORONA SOLAR PROMINENCES SUN Sun: corona Sun: filaments, prominences THERMODYNAMICS VELOCITY
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