Adaptive optical systems are used to ensure maximum angular resolution of telescopes in observing remote objects through a turbulent atmosphere, and also for focusing radiation onto remote objects in a nonlinear and turbulent medium. The potential of additive systems is largely determined by the type of corrector used and its parameters: the band of working frequencies and the sensitivity. The parameters of correcting mirrors are expediently measured by interferometric methods.
Faculty of Physics, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
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