  We derive an analytical solution for the flavor evolution of a neutrino
through a turbulent density profile which is found to accurately predict the
amplitude and transition wavelength of numerical solutions on a case-by-case
basis. The evolution is seen to strongly depend upon those Fourier modes in the
turbulence which are approximately the same as the splitting between neutrino
eigenvalues. Transitions are strongly enhanced by those Fourier modes in the
turbulence which are approximately the same as the splitting between neutrino
eigenvalues. We also find a suppression of transitions due to the long
wavelength modes when the ratio of their amplitude and the wavenumber is of
order, or greater than, the first root of the Bessel function $J_0$.
