3d Mhd Wave Behavior In Active Regions: Modeling Techniques

Details 3d Mhd Wave Behavior In Active Regions: Modeling Techniques 3d Mhd Wave Behavior In Active Regions: Modeling Techniques

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.0116m&link_type=abstract

American Astronomical Society, SPD meeting #37, #1.16; Bulletin of the American Astronomical Society, Vol. 38, p.218

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We have performed simulations of three-dimensional MHD wave propagation in models of coronal active regions. Here, we present descriptions of the methodology and techniques that are used in the construction of such simulations. These include:1) The MHD equations solved and the velocity perturbations used to simulate, for example, incoming EIT waves.2) The construction of the active region model using extrapolations of the observed photospheric magnetic field and gravitational stratification of the coronal density structure.3) The inclusion of the density structure of individual, realistic coronal loops using a new technique.We also discuss the application of the model to coronal seismology and the possibility of using STEREO data to the improvement of the simulations.

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