A simplified expression for the bandwidth of an adaptive optics system is found to depend on a weighted path integral of the turbulence strength, where the weighting is transverse wind velocity to the 5/3 power. The wave-front corrector is conservatively assumed to match the phase perfectly, at least spatially, if not temporally. For the case of astronomical imaging from a mountaintop observatory, the necessary bandwidth is found to be less than 200 Hz.
© 1977 Optical Society of America
Darryl P. Greenwood, "Bandwidth specification for adaptive optics systems," J. Opt. Soc. Am. 67, 390-393 (1977)