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Helioseismology and the solar interior dynamics
Journal of Astrophysics and Astronomy, 2000AbstractThe inversion of helioseismic modes leads to the sound velocity inside the Sun with a precision of about 0.1 per cent. Comparisons of solar models with the “seismic sun” represent powerful tools to test the physics: depth of the convection zone, equation of state, opacities, element diffusion processes and mixing inside the radiative zone.
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Local helioseismology in the SDO HMI/AIA data analysis pipeline
Astronomische Nachrichten, 2007R S Bogart
exaly

