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

Published online by Cambridge University Press:  07 August 2014

Khalil Daiffallah
Khalil Daiffallah*
Affiliation:
Observatory of Algiers, CRAAG, Route de l'Observatoire, BP 63, Bouzaréah 16340, Algiers, Algeria email: k.daiffallah@craag.dz
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Abstract

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Motivated by the problem of local solar subsurface magnetic structure, we have used numerical simulations to investigate the propagation of waves through monolithic magnetic flux tubes of different sizes. 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 are powerful tools to probe the structure and the dynamics of various solar features which are directly related to solar magnetic field activity.

Keywords

Magnetohydrodynamicswavesmagnetic fieldsunspotsplages
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 126 - 129
Copyright
Copyright © International Astronomical Union 2014 

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