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Conventional astrophysical observations have failed to provide stringentconstraints on physical processes operating in the interior of the stars.However, satellite missions now promise a solution to these problems byproviding long-term high-quality continuous data which will allow theapplication of seismic techniques. With this in mind, and using the Sun as ourastrophysical laboratory, our aim is to determine if Corot- and Kepler-likeasteroseismic data can constrain physical processes like microscopic diffusion.We test to what extent can the observed atmospheric abundances coupled withp-mode frequencies safely distinguish between stellar initial chemicalcomposition and diffusion of these elements. We present some preliminaryresults of our analysis.

Sensitivity of p modes for constraining velocities of microscopic diffusion of the elements