Numerical Simulation of Wave Energy Transport in Auroral Flux Tubes

Details Numerical Simulation of Wave Energy Transport in Auroral Flux Tubes Numerical Simulation of Wave Energy Transport in Auroral Flux Tubes

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsm43c..08w&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SM43C-08

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Applications

2407 Auroral Ionosphere (2704), 2431 Ionosphere/Magnetosphere Interactions (2736), 7839 Nonlinear Phenomena, 7843 Numerical Simulation Studies, 7868 Wave/Wave Interactions

Scientific paper

A pseudospectral method is used to solve the three-dimensional, nonlinear reduced magnetohydrodynamic equations. The model is applied to auroral flux tubes and we investigate the development of fine scale structure through nonlinear wave coupling. Further refinements and applications, such as the inclusion of compressibility and the study of density cavity formation, are discussed.

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