Based on dense series of photoelectric observations and on our radial-
velocity measurements, we calculated the radii of 62 northern Cepheids
by Balona's method. We derived the following period-radius relation:
log R = 1.23(+/-0.03) + 0.62(+/-0.03) log P. Our detailed analysis sho
ws that the distance scale for Cepheids cannot be refined using their
radii by an independent method which is unrelated to the distances to
young open clusters because of the random and systematic errors of the
Baade-Wesselink technique.