Comparison of the thin flux tube approximation with 3D MHD simulations
Context: The structure and dynamics of small vertical photospheric magnetic flux concentrations has been often treated in the framework of an approximation based upon a low-order truncation of the Taylor expansions of all quantities in the horizontal direction, together with the assumption of instantaneous total pressure balance at the boundary to
Yelles Chaouche, L. et al.
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9
2009