We investigate the role of the coronal mass ejections (CMEs) (by using
soft X ray solar emission as proxy data) in producing the nonrecurren
t geomagnetic storms in the period 1969-1974. The linkage between thes
e phenomena is confirmed: however, it turns out that CMEs associated w
ith chromospheric flares, accompanied by type 4 radio emission, are th
e most effective in perturbing the geomagnetic field.