We describe the fundamental differences between weak (wave) turbulence in i
ncompressible and weakly compressible MHD at the level of three-wave intera
ctions. The main difference is in the structure of the resonant manifolds a
nd the mechanisms of redistribution of spectral densities along the applied
magnetic field B-0. Similar to pure acoustic waves, a three-wave resonance
between collinear wavevectors is observed but, in addition, we also have a
resonance through tilted planes and spheres. The properties of resonances
and their consequences for the asymptotics are also discussed.