On the location of the excitation of solar p-modes

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Solar Oscillations

Scientific paper

We give the general expression for the power spectrum of oscillations nonlinearly excited by convection and we show how it simplifies for p-modes. The source term is described by a correlation function of well chosen variables which contains 7 free parameters. If observations of line powers and asymmetries were available for p-modes of various degrees it would be possible to find, among other things, the location of the source and its width as well as their variation with frequency and degree. This would provide an excellent test of the theory of modes excitation by convection.

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