Shell-models of Rmhd Turbulence and the Heating of Solar Coronal Loops

  • E. B UCHLIN
  • Published 2007

Abstract

A simplified non-linear numerical model for the development of incompressible magnetohydrodynamics (MHD) in the presence of a strong magnetic field ~ B‖ and stratification, nicknamed SHELL-ATM, is presented. In planes orthogonal to the mean field, the non-linear incompressible dynamics is replaced by 2D shell-models for the complex variables u and b… (More)

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