Dynamics of nonlinear resonant slow MHD waves in twisted flux tubes
Nonlinear resonant magnetohydrodynamic (MHD) waves are studied in weakly dissipative isotropic plasmas in cylindrical geometry. This geometry is suitable and is needed when one intends to study resonant MHD waves in magnetic flux tubes (e.g. for sunspots, coronal loops, solar plumes, solar wind,...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2002-01-01
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Series: | Nonlinear Processes in Geophysics |
Online Access: | http://www.nonlin-processes-geophys.net/9/79/2002/npg-9-79-2002.pdf |