Photonics Research, Volume. 11, Issue 6, 1015(2023)

Direct observation of longitudinal aberrated wavefields

J. P. Trevino1,2, V. Coello3、*, A. Jaimes-Nájera1, C. E. Garcia-Ortiz1, S. Chávez-Cerda4, and J. E. Gómez-Correa4
Author Affiliations
  • 1Tecnológico de Monterrey, School of Engineering and Sciences, Monterrey NL 64849, Mexico
  • 2Universidad Politécnica de Puebla, Cuanalá Puebla 72640, Mexico
  • 3Centro de Investigación Científica y de Educación Superior de Ensenada, Unidad Monterrey, Apodaca NL 66629, Mexico
  • 4Instituto Nacional de Astrofísica, Óptica y Electrónica, Coordinación de Óptica, Tonantzintla Puebla 72840, Mexico
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    Figures & Tables(8)
    3D representation of a beam propagation. The beam is aberrated with coma; the main planes where the analyses take place are indicated with blue squares parallel to each plane.
    Each one of the Seidel terms for wave aberrations is plotted. The piston aberration is just a wave delay, while the tilt has a linear variation. The slope is proportional to the tilt angle of the incident beam. Defocus is a quadratic function and coma is cubic.
    How to adjust the system. The exit pupil plane is in yellow. The position of the sample relative to the Gaussian beam: (a) with the initial alignment to get an unaberrated field and with a displacement to get a defocused field and (b) with a tilt and a displacement to get tilted and comatic aberrations. This figure illustrates how there are regions of the wavefront arriving at the sample ahead of others, thus producing the desired Seidel aberrations. (c) Moving the beam is equivalent to moving the sample since the wavefront is incident on the plane with the same phase shifts.
    Image of an LRM system. The angle α and the distance from the beam waist to the golden ridge are the parameters that determine the Seidel aberration. A waist shift will produce a defocus because the beam will arrive at the ridge at a point where the front is converging, while changing an angle α produces a tilt if the beam waist is at the ridge; otherwise, a coma is produced.
    Aberration-free beam. (a) Incident Gaussian light beam focused with the 10× objective. (b) LRM image of the intensity distribution of SPP propagating from left to right. (c) and (d) Corresponding numerical simulations of the 3D beam propagation.
    Tilting the incident beam. (a) Incident light beam focused with the 40× objective. (b) LRM image of the intensity distribution of SPP propagating from left to right. (c) and (d) Corresponding numerical simulations of the 3D beam propagation.
    Defocused beam. (a) Incident light beam defocused with the 40× objective. (b) LRM image of the intensity distribution of SPP propagating from left to right. (c) and (d) Corresponding numerical simulations of the 3D beam propagation.
    Coma-like beam. (a) Incident light beam defocused with the 40× objective. (b) LRM image of the intensity distribution of SPP propagating from left to right. (c) and (d) Corresponding numerical simulations of the 3D beam propagation.
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    J. P. Trevino, V. Coello, A. Jaimes-Nájera, C. E. Garcia-Ortiz, S. Chávez-Cerda, J. E. Gómez-Correa, "Direct observation of longitudinal aberrated wavefields," Photonics Res. 11, 1015 (2023)

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    Paper Information

    Category: Imaging Systems, Microscopy, and Displays

    Received: Dec. 1, 2022

    Accepted: Mar. 17, 2023

    Published Online: May. 29, 2023

    The Author Email: V. Coello (vcoello@cicese.mx)

    DOI:10.1364/PRJ.482323

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