Three-dimensional MHD Modeling Of Waves In Active Regions: Comparison To Observations

Details Three-dimensional MHD Modeling Of Waves In Active Regions: Comparison To Observations Three-dimensional MHD Modeling Of Waves In Active Regions: Comparison To Observations

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640717s&link_type=abstract

American Astronomical Society, AAS Meeting #216, #407.17; Bulletin of the American Astronomical Society, Vol. 41, p.862

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the results of 3D MHD models of waves in active regions generated by a CME. We study the propagation and reflection of the waves in the solar corona and compare to recent STEREO observations. We also investigate the excitation of oscillations in individual coronal loops in realistic active region magnetic field initialized with extrapolated WSO magnetogram data. We compare the results of the model to EUV observations and demonstrate the development and application of coronal seismology.

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