The M1 and E1 strength distributions in the energy range 3-12 MeV are calcu
lated in random-phase approximation for the deformed nuclei Sm-154, Er-168,
Hf-178 and U-238. It is found that the orbital motion, although providing
on the whole a modest contribution to the M1 strength, plays a significant
role in shaping the M1 spectra because of the destructive interference betw
een orbital and spin amplitudes. Strong E1 transitions also occur in the sa
me energy range. Their total strength in the energy range 3.6-7.6 MeV is ab
out four times larger than the M1 strength. Because of these highly intense
E1 transitions, the total dipole strength distribution computed as a sum o
f the M1 and E1 strengths is considerably different from the spectra of the
M1 transitions alone.