[en] The weak turbulence of the magnetohydrodynamic waves in the strongly magnetized plasma, when the plasma pressure is low as compared to the magnetic field pressure, is studied. The resonance scattering of the magnetoacoustic and Alfven waves on the slow magnetoacoustic waves is the basic nonlinear mechanism in this situation. The given motion integral in the weak turbulence mode generates the Kolmogorov spectrum with the constant flux of the HF waves numbers into the long-wave area. The Kolmogorov spectrum with the constant energy flow is realized in the short-wave area. The exact angular dependence of the turbulent spectra for the propagation angles, close to the average magnetic field, is established