Nuclei with large neutron-to-proton ratios have neutron skins, which manife
st themselves in an excess of neutrons at distances greater than the radius
of the proton distribution. Ln addition, some drip-line nuclei develop ver
y extended halo structures. The neutron halo is a threshold effect; it appe
ars when the valence neutrons occupy weakly bound orbits. In this study, nu
clear skins and halos an analyzed within the self consistent Skyrme-Hartree
-Fock-Bogoliubov and relativistic Hartree-Bogoliubov theories for spherical
shapes. It is demonstrated that skins, halos, and surface thickness can be
analyzed in a model-independent way in terms of nucleonic density form fac
tors. Such an analysis allows for defining a quantitative measure of the ha
lo size. The systematic behavior of skins, halos, and surface thickness in
even-even nuclei is discussed.