  We report the first attempt to mode decomposition of the velocity field using
wavelet transforms in the application to the magnetized turbulence analysis. We
compare results of the separation with respect to the global and local mean
magnetic field for models with a strong and weak external magnetic field. We
show, that for models with a strong external magnetic field our results are
relatively consistent for both methods. However, for superAlfv\'{e}nic
turbulence with spatially variable direction of the local mean magnetic field
the differences are substantial.
