Method for designing freeform surfaces off-axial imaging system with a real exit pupil
US-2016232258-A1 · Aug 11, 2016 · US
US12085445B2 · US · B2
| Field | Value |
|---|---|
| Publication number | US-12085445-B2 |
| Application number | US-202017603487-A |
| Country | US |
| Kind code | B2 |
| Filing date | Apr 3, 2020 |
| Priority date | Apr 16, 2019 |
| Publication date | Sep 10, 2024 |
| Grant date | Sep 10, 2024 |
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A detector system for Fourier spectroscopy such as a spectral domain optical coherence tomography instrument includes a diffractive optic for diffracting the interfering light into angularly dispersed wavenumbers, a prism for reduces a nonlinear angular dispersion among the wavenumbers, and a focusing optic for converting the angularly dispersed wavenumbers from the prism into spatially distributed wavenumbers along a detector having an array of pixels. A field lens between the focusing optic and the detector has a freeform surface for more evenly distributing the wavenumbers along the array of pixels.
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The invention claimed is: 1. An absolute linear-in-K spectrometer comprising: a diffractive optic for diffracting collimated light from an entrance aperture into angularly dispersed wavenumbers; a prism for reducing a nonlinear angular dispersion among the wavenumbers; a focusing optic for converting the angularly dispersed wavenumbers from the prism into spatially distributed wavenumbers along a detector; and a field lens between the focusing optic and the detector having a freeform surface with a surface geometry that reduces field dependent aberrations introduced by the prism and more linearly distributes the wavenumbers along the detector; wherein a sag of the freeform surface is defined by a plurality of polynomial terms in which coefficients of the polynomial terms are constrained so that chief rays of evenly spaced wavenumbers are distributed along the detector in a form that is maximized toward an even spacing of the chief rays along the detector, such that a residual nonlinearity RN of the wavenumbers distributed along the detector is less than 10 −4 percent, where the residual nonlinearity RN as a percent is determined in accordance with the following expression: R N [ % ] = ( ∫ k min k max [ f ( k ) - g ( k ) ] 2 dk ) / ( k max - k min ) f ( k max ) - f ( k min ) × 1 0 0 where k max and k min are respective maximum and minimum wavenumbers distributed along the detector, f(k) is a function of calibration relating wavenumbers to pixels of the detector, and g(k) is the linear approximation of f(k) with the least root mean square error. 2. The spectrometer of claim 1 in which the freeform surface has a sag z defined in accordance with the following expression: z = c r 2 1 + 1 - ( 1 + k c ) c 2 r 2 + ∑ j C j Z j ( ρ , φ ) , where r is a radial coordinate of the surface, cis a curvature of a base sphere, k c is a conic constant, ρ and φ are normalized radial and azimuthal components in an aperture, and C j is a weight factor of a j th Zernike term, Z j , where the weight factor C j is determined in a way that chief rays of evenly spaced wavenumbers are distributed along the detector in a form that is maximized toward an even spacing of the chief rays along the detector. 3. The spectrometer of claim 2 in which the expression for the sag z includes 16 Zernike terms Zj. 4. The spectrometer of claim 1 in which the prism is a Brewster-angled prism that is oriented and spaced between the diffractive optic and the focusing optic for reducing the nonlinear angular dispersion among the wavenumbers. 5. The spectrometer of claim 4 in which the field lens has front surface facing the fo
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