The results of a study are presented of the linear stability of a magnetohy
drodynamic planar free-shear flow subject to system rotation and a uniform
magnetic field which are both parallel or antiparallel to the shear flow vo
rticity vector. The results show that, with anticyclonic rotation, the effe
ct of the uniform magnetic field is to enlarge the unstable region of the r
otating shear flow, while the growth rate of the most unstable disturbance
is left unchanged. With cyclonic rotation, on the other hand, the effect of
the magnetic field is to strongly stabilize the flow. The spatial structur
e of the anticyclonic magnetic shear/Coriolis instability mode is investiga
ted. Considering the Rossby number at which the spatial extent of the most
unstable disturbance becomes minimum, it is found that this Rossby number d
ecreases as the uniform magnetic field is intensified. (C) 2001 American In
stitute of Physics.