Phase mixing of a three dimensional magnetohydrodynamic pulse

Details Phase mixing of a three dimensional magnetohydrodynamic pulse Phase mixing of a three dimensional magnetohydrodynamic pulse

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506...67t&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Magnetohydrodynamics (Mhd), Waves, Sun: Activity, Sun: Wind, Sun: Corona

Scientific paper

Phase mixing of a three dimensional magnetohydrodynamic (MHD) pulse is studied in the compressive three-dimensional (without an ignorable coordinate) regime. It is shown that the coupling to the compressive modes dramatically enhances the efficiency of decay of an Alfvénic part of a compressible MHD pulse. However, the dynamics of weakly non-plane Alfvén waves can still be qualitatively understood in terms of the previous 2.5D models.

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