High performance Nd2Fe14B-based permanent magnets are produced with di
fferent composition and various processing techniques. The composition
and the processing route influence the complex, multiphase microstruc
ture of the magnets, such as grain size, alignment, and distribution o
f phases. Grain sizes in the range between 10 and 500 nm are obtained
by melt spinning, mechanical alloying, and the HDDR process. Sintered
and hot worked magnets exhibit grain sizes above 1 mu m. The coercive
field is determined by the high uniaxial magnetocrystalline anisotropy
as well as the magnetostatic and exchange interactions between neighb
oring hard magnetic grains. The dipolar interactions between misaligne
d gains are more pronounced in large-grained magnets, whereas exchange
coupling reduces the coercive field in small grained magnets. Transmi
ssion electron microscopy has been used to study the influence of subs
tituent and dopant elements on microstructure, coercivity, and corrosi
on resistance of advanced (Nd,S1)-(Fe,S2)-B:(M1,M2) magnets. The repla
cement of the Nd-rich intergranular phase by secondary phases formed a
fter doping by M1 and M2 type elements improves the corrosion resistan
ce, especially in large-grained magnets. Secondary, nonmagnetic phases
reduce the remanence and the energy product. In addition to the chara
cterization of the microstructure, special attention has been paid to
the computer modeling of the interaction between microstructure and co
ercivity. The simulation of the magnetization reversal process based o
n the real microstructure reveals a good agreement with experimental v
alues. It is shown that the coercive field depends on grain size, dist
ribution, and misorientation of grains. A strong exchange coupling bet
ween hard magnetic grains is desired in nanostructured magnets in orde
r to improve the remanence. This effect is further increased by second
ary, soft magnetic phases. Nanocrystalline, composite Nd-Fe-B based ma
gnets show a remanence enhancement, both in experiments and in model c
alculations. (C) 1996 American Institute of Physics.