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arXiv · 1310.7398

Probing the structure of local magnetic field of solar features with helioseismology

Khalil Daiffallah
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Abstract

Motivated by the problem of local solar subsurface magnetic structure, we have used numerical simulation to investigate the propagation of waves through monolithic magnetic flux tubes of different size. A cluster model can be a good approximation to simulate sunspots as well as solar plage regions which are composed of an ensemble of compactly packed thin flux tubes. Simulations of this type is a powerful tool to probe the structure and the dynamic of various solar features which are related directly to solar magnetic field activity.

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Khalil Daiffallah. 2013-10-28. Probing the structure of local magnetic field of solar features with helioseismology. https://doi.org/10.1017/s1743921314001860

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