We extend previous studies of the tidal truncation of coplanar disks in binary systems to the more general case of noncoplanar disks . As in the prograde coplanar case , Lindblad resonances play a key role in tidal truncation . We analyze the tidal torque acting on a misaligned nearly circular disk in a circular orbit binary system . We concentrate on the 2:1 inner Lindblad resonance associated with the m = 2 tidal forcing ( for azimuthal wavenumber m ) that plays a major role in the usual coplanar case . We determine the inclination dependence of this torque , which is approximately \cos ^ { 8 } { ( i / 2 ) } for misalignment angle i . Compared to the prograde coplanar case ( i = 0 ) , this torque decreases by a factor of about 2 for i = \pi / 6 and by a factor of about 20 for i = \pi / 2 . The Lindblad torque decreases to zero for a tilt angle of \pi ( counter-rotation ) , consistent with previous investigations . The effects of higher order resonances associated with m > 2 tidal forcing may contribute somewhat , but are much more limited than in the i = 0 case . These results suggest that misaligned disks in binary systems can be significantly extended compared to their coplanar counterparts . In cases where a disk is sufficiently inclined and viscous , it can overrun all Lindblad resonances and overflow the Roche lobe of the disk central object .