For a better understanding of the dynamic characteristics of GdDy/FeCo
magnetooptical (MO) disks, the magnetic properties of GdDy/FeCo films
with various thicknesses were investigated. The MO layer, whose thick
ness was varied from 200 Angstrom to 1500 Angstrom was sandwiched by d
ielectric SiN layers. Kerr rotation angle decreased as the MO layer wa
s made thinner, while the reflectivity showed little change. Tcomp shi
fted lower with decreasing thickness, while Tc was constant. This is a
ssumed to be caused by the effective composition shift of rare-earth i
n thinner layers. The CNR value saturated above 600 Angstrom thickness
, while noise level was less influenced with the thickness. Therefore,
the increase in CNR is mainly due to the carrier level and caused by
an increase of Kerr rotation angle. The degradation of CNR at lower ma
gnetic fields tends to be smaller as the thickness is made thinner, ow
ing to the lower noise level caused by decreasing demagnetization of t
he fields.