  We propose a phenomenological theory of strong incompressible
magnetohydrodynamic turbulence in the presence of a strong large-scale external
magnetic field. We argue that in the inertial range of scales, magnetic-field
and velocity-field fluctuations tend to align the directions of their
polarizations. However, the perfect alignment cannot be reached, it is
precluded by the presence of a constant energy flux over scales. As a
consequence, the directions of fluid and magnetic-field fluctuations at each
scale $\lambda$ become effectively aligned within the angle
$\phi_{\lambda}\propto \lambda^{1/4}$, which leads to scale-dependent depletion
of nonlinear interaction and to the field-perpendicular energy spectrum
$E(k_{\perp})\propto k_{\perp}^{-3/2}$. Our results may be universal, i.e.,
independent of the external magnetic field, since small-scale fluctuations
locally experience a strong field produced by large-scale eddies.
