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It consists of two mirrors in the light path with one ground to correct the aberration.
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Telescope mirrors are commonly made parabolic or hyperbolic in section to correct the aberrations of the image.
The lens elements may be cemented together or mounted at carefully calculated separations to correct the aberrations of the individual elements and obtain an image of acceptable sharpness (see also aberration).
In order to correct the aberrations well, under the guidance of the vector aberration theory, the modification of Czerny Turner system with inserted tilt lenses is proposed.
Both simulated and experimental results indicate that the method of wavefront pre-compensation can greatly correct the aberrations caused from thermal deformation, and the laboratory experiment is a feasible method to modeling the inner optical system with phase aberration.
In this paper, we propose a two-stage deconvolution method specifically designed to correct the aberrations induced by a slanted scan, but with general applicability to high-resolution bright-field microscopy.
The chromatic and spherical aberrations of the objective lens are corrected with an electrostatic electron mirror that provides independent control over the chromatic and spherical aberration coefficients Cc and C3, as well as the mirror focal length, to match and correct the aberrations of the objective lens.
To measure and correct the aberrations of the eye, a closed-loop AO system was used.
In the proposed corrector system, the micro-mirrors have to provide the exact negative spherical and chromatic aberrations for correcting the aberration of the objective lens.
The phase aberration caused by thermal deformations in a high power inner optical system is simulated and the wavefront pre-compensation for correcting the aberration is studied experimentally.
Au-Pd bimetallic particles deposited on a thin amorphous carbon film was used as a reference for correcting the aberration coefficients of the electronic optics system.
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