Nonlinear development of MHD waves in coronal loops

Details Nonlinear development of MHD waves in coronal loops Nonlinear development of MHD waves in coronal loops

Publishing date

Jan 1997

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1891p&link_type=abstract

Journals

Advances in Space Research, vol. 19, p. 1891

Science

Physics

Additional info 3

Solar Corona, Magnetohydrodynamic Waves, Coronal Loops, Plasma Conductivity, Wave Propagation, Current Sheets, Nonlinear Equations, Digital Simulation, Plasma Resonance

Type

Scientific paper

Abstract

The numerical simulation of a solar corona by a low-beta resistive plasma slab that sustains MHD wave propagations presents the evolution of these waves and the formation of current sheets, leading to the observation of steep gradients at the slab edges that are indicative of resonance layers. As the plasma evolves, the edge heating-supplying current sheets undergo fragmentation into two current sheets at each edge; these in turn come closer when the twist is enlarged.

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