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Advances in Global and Local Helioseismology: An Introductory Review

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The Pulsations of the Sun and the Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 832))

Abstract

Helioseismology studies the structure and dynamics of the Sun’s interior by observing oscillations on the surface. These studies provide information about the physical processes that control the evolution and magnetic activity of the Sun. In recent years, helioseismology has made substantial progress towards the understanding of the physics of solar oscillations and the physical processes inside the Sun, thanks to observational, theoretical and modeling efforts. In addition to global seismology of the Sun based on measurements of global oscillation modes, a new field of local helioseismology, which studies oscillation travel times and local frequency shifts, has been developed. It is capable of providing 3D images of subsurface structures and flows. The basic principles, recent advances and perspectives of global and local helioseismology are reviewed in this article.

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Acknowledgment

This work was supported by the CNRS, the International Space Science Institute (Bern), Nordita (Stockholm) and NASA.

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  1. W.W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA, 94305, USA

    Alexander G. Kosovichev

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  2. GEPI, bâtiment Copernic A, Observatoire de Meudon, place Jules Janssen 5, Meudon, Cedex, 92195, France

    Coralie Neiner

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Kosovichev, A.G. (2011). Advances in Global and Local Helioseismology: An Introductory Review. In: Rozelot, JP., Neiner, C. (eds) The Pulsations of the Sun and the Stars. Lecture Notes in Physics, vol 832. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-19928-8_1

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