class of adaptive-optics problems is described in which phase distortions c
aused by atmospheric turbulence are corrected by adaptive wave-front recons
truction with a deformable mirror, i.e., the control loop that drives the m
irror adapts in real time to time-varying atmospheric conditions, as oppose
d to the linear time-invariant control loops used in conventional adaptive
optics. The basic problem is posed as an adaptive disturbance-rejection pro
blem with many channels. The solution given is an adaptive feedforward cont
rol loop built around a multichannel adaptive lattice filter. Simulation re
sults are presented for a l-m telescope with both one-layer and two-layer a
tmospheric turbulence profiles. These results demonstrate the significant i
mprovement in imaging resolution produced by the adaptive control loop comp
ared with a classical linear time-invariant control loop. (C) 2000 Optical
Society of America OCIS codes: 010.1080, 010.1290, 010.7060, 010.1330, 110.
6770.