Adaptive optics system (AOS) performance is a function of the system d
esign, seeing conditions, and light level of the wave-front beacon. It
is desirable to optimize the controllable parameters in an AOS to max
imize some measure of performance. For this optimization to be useful,
it is necessary that a set of image-quality metrics be developed that
vary monotonically with the AOS performance under a wide variety of i
maging environments. Accordingly, as conditions change, one can be con
fident that the computed metrics dictate appropriate system settings t
hat will optimize performance. Three such candidate metrics are presen
ted. The first is the Strehl ratio; the second is a novel metric that
modifies the Strehl ratio by integration of the modulus of the average
system optical transfer function to a noise-effective cutoff frequenc
y at which some specified image spectrum signal-to-noise ratio level i
s attained; and the third is simply the cutoff frequency just mentione
d. It is shown that all three metrics are correlated with the rms erro
r (RMSE) between the measured image and the associated diffraction-lim
ited image. Of these, the Strehl ratio and the modified Strehl ratio e
xhibit consistently high correlations with the RMSE across a broad ran
ge of conditions and system settings. Furthermore, under conditions th
at yield a constant average system optical transfer function, the modi
fied Strehl ratio can still be used to delineate image quality, wherea
s the Strehl ratio cannot.