  The broad line profiles from a nonplanar (warped) accretion disk as a result
from reprocessing of central hard radiation are studied in this paper. The disk
is warped because of the Bardeen-Petterson effect. Obtained profiles depend
significantly on the line of sight - they are asymmetric as well as
frequency-shifted in most cases. Since such frequency shifted asymmetric
profiles are generally not observed in AGN, the most plausible interpretation
is that either the major part of the broad emission does not originate from the
disk or the disk is in general planar.
