Adjusting optical systems on the basis of the line scattering function

Mathematics

Scientific paper

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Aberration, Adjusting, Optical Equipment, Optimization, Scattering Functions, Degrees Of Freedom, High Resolution, Mathematical Models, Mirrors, Telescopes

Scientific paper

This paper discusses a method for calculating the adjusting motions of the elements of an optical system from the line scattering function (LSF), in order to compensate aberrations that arise when the air gaps and decentering are disturbed. The method is based on the reconstruction of the fourth-order aberrations of a perturbed optical system by means of nonlinear approximation of the LSF and uses global and local optimization elements. A model example is presented of the reconstruction of the aberrations that arise in a telescope when the secondary mirror is displayed along three degress of freedom.

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