3D MHD models of waves in active regions: application to coronal seismology

Details 3D MHD models of waves in active regions: application to coronal seismology 3D MHD models of waves in active regions: application to coronal seismology

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh52a..06m&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH52A-06

Physics

7836 Mhd Waves And Instabilities (2149, 2752, 6050), 7839 Nonlinear Phenomena (4400, 6944)

Scientific paper

We present results from three-dimensional MHD simulations of the behavior of MHD waves in realistic models of coronal active regions. The models of the active regions are constructed by using the observed photospheric magnetic field and gravitationally stratified coronal density structure with individual loops. We compare the main features of the model with those seen recently by the SOHO and TRACE satellites, and investigate the application of the results to coronal seismology. We discuss the possible application of STEREO data to the improvement of our model.

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