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Neutron stars might have multipole magnetic fields as implied by recentobservations of pulsars. The presence of the quadrupole field might have aneffect on the interaction between the disc and the neutron star depending onthe location of the inner radius of the disc and the strength of the quadrupolefield. For a quadrudipole stellar field, we calculate the toroidal fieldgenerated within the disc, the magnetospheric radius and the torque exertedonto the star. Also, we deduce the effect of the rotation of the star on themagnetospheric radius which is relevant even for pure dipole magnetic fields.

Magnetically Threaded Thin Disks in the Presence of the Quadrupole Magnetic Field