What have we learned about the solar interior from solar oscillations?

Physics

Scientific paper

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Solar Oscillations, Convection, Solar Neutrinos, Solar Interior, Sun, Diffusivity, Frequencies, Helium, Rotation, Settling

Scientific paper

After a brief review of the discovery and properties of solar oscillations, I summarize the significant advances in our knowledge of the Sun's interior structure achieved by using solar oscillation frequency data. I discuss the surprising solar interior rotation profile; the precise determination of the convection zone depth; the convection zone helium abundance; evidence for diffusive settling of helium during the Sun's 4.5 billion year lifetime; and the Sun's central structure and implications for the solar neutrino problem.

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