New Code for Simulation of Auroral Alfven Waves

Details New Code for Simulation of Auroral Alfven Waves New Code for Simulation of Auroral Alfven Waves

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsm41c1200d&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SM41C-1200

Physics

2407 Auroral Ionosphere (2704), 2487 Wave Propagation (0689, 3285, 4275, 4455, 6934), 2704 Auroral Phenomena (2407), 2752 Mhd Waves And Instabilities (2149, 6050, 7836), 2753 Numerical Modeling

Scientific paper

A new simulation code is being developed for the simulation of auroral Alfven waves. This code uses energy conserving reduced MHD equations which couple the Alfven and slow mode waves. The effects of the ponderomotive force, curvature, and anisotropic pressure, are included. The code is written in generalized curvilinear coordinates, and the equations will be solved in a meridional plane with dipole-like geometry. Results to date will be presented.

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