Doppler ground-based search for solar-like oscillations with CORALIE and HARPS

Observations of solar-like oscillation frequencies allow to constrain theory of structure and evolution of stars with an outer convective zone. Recent improvements in radial velocity measurements have led to p-mode detections on some bright target stars. We briefly review some Doppler ground-based programs of asteroseismology of solar-like stars in operation and present results obtained on alpha Cen A with the spectrograph CORALIE. Photon noise study shows that the future spectrograph HARPS, which will be installed on the 3.6 m ESO La Silla telescope, will be able to conduct a program of asteroseismology from the ground on several tens of solar-like stars. Such an astero-seismological program is far from the expected accuracy of the future photometric space missions but is useful to conduct a preliminary and complementary study on solar-like stars.