Contemporary high-energy data: which froissarton do they prefer?

Up-to-date data on pp and p-barp interactions are analyzed on the basis of two well-known representations which transmute the supercritical pomeron into a froissaron. Both approaches are found to be equivalent from the phenomenological point of view, and the impact amplitudes tend asymptotically in both cases to the values close to those values obtained in the scattering model on a black disk. The impact amplitudes are restored and the way in which the black spot is formed with the energy is studied