Helioseismology

Details Helioseismology Helioseismology

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000npa..conf..488b&link_type=abstract

NEUTRINOS IN PHYSICS AND ASTROPHYSICS From 10-33 to 1028 cm (TASI 98). Held 1-26 June 1998 in Boulder, Colorado, USA. Edited by

Astronomy and Astrophysics

Astrophysics

Scientific paper

Helioseismology is the study of the Sun through properties of solar oscillations. Helioseismic techniques allow us to probe the interior of the Sun with very high precision, and in the process test the physical inputs to stellar models. This article gives a brief introduction to the theory of solar oscillations and helioseismic inversion techniques to determine solar structure.

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