We present in this paper a new model for internal wave generation by d
isturbances at the bottom of the convective region in the frame of the
convective penetration model by Zahn (1991). Several morphologies are
proposed for these per turbations. Fourier analysis and the results f
rom Press (1981) for sinusoidal perturbation, provide us with analytic
al expression for the velocity field in the stellar radiative interior
. A diffusion coefficient is obtained using the definition of macrosco
pic diffusion coefficient given by Schatzman (1991) following Press' s
uggestion of irreversibility of the process in the radiative interior.
The comparison between observations and Li depletion provided by this
diffusive process in the Sun, shows that it is possible to justify wi
th this process a Li depletion factor of 10(2) if we assume the distur
bance described by a plume, and with a velocity of the downdraft in th
e convective zone four times that one given by the mixing length theor
y. Furthermore, the results are compatible with the pre-main-sequence
(PMS) lithium burning.