1999
DOI: 10.1016/s0030-4018(99)00084-x
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Fresnel coefficients for weak reflection, and the scattering potential for three-dimensional imaging

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Cited by 11 publications
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“…Here, r and z denote the lateral and axial spatial coordinates, respectively; ν i and η(ν i ) = λ −2 − |ν i | 2 are the illumination's lateral and axial spatial frequencies, respectively; the amplitude A = S(ν i )P (−ν i ); S is the incoherent primary source function; and P is the pupil function. To calculate the reflected field, we use the average TE and TM wave Fresnel coefficients R(ν i ) = 1 2 [|R TE (ν i )| + |R TM (ν i )|] to model the reflection amplitude of the unpolarized illumination from the boundary [65].…”
Section: Theorymentioning
confidence: 99%
“…Here, r and z denote the lateral and axial spatial coordinates, respectively; ν i and η(ν i ) = λ −2 − |ν i | 2 are the illumination's lateral and axial spatial frequencies, respectively; the amplitude A = S(ν i )P (−ν i ); S is the incoherent primary source function; and P is the pupil function. To calculate the reflected field, we use the average TE and TM wave Fresnel coefficients R(ν i ) = 1 2 [|R TE (ν i )| + |R TM (ν i )|] to model the reflection amplitude of the unpolarized illumination from the boundary [65].…”
Section: Theorymentioning
confidence: 99%