FresnelEquations.R_p
— FunctionR_p(n₁, n₂, θᵢ)
R_p(n₁, n₂, θᵢ, θₜ)
Calculate the reflectance for p-polarized light, i.e. the fraction of incident light energy that is reflected.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations.R_s
— FunctionR_s(n₁, n₂, θᵢ)
R_s(n₁, n₂, θᵢ, θₜ)
Calculate the reflectance for s-polarized light, i.e. the fraction of incident light energy that is reflected.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations.T_p
— FunctionT_p(n₁, n₂, θᵢ)
T_p(n₁, n₂, θᵢ, θₜ)
Calculate the transmittance for p-polarized light, i.e. the fraction of incident light energy that is transmitted.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations.T_s
— FunctionT_s(n₁, n₂, θᵢ)
T_s(n₁, n₂, θᵢ, θₜ)
Calculate the transmittance for s-polarized light, i.e. the fraction of incident light energy that is transmitted.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations._check_angles
— MethodAn internal function to check if the inputs make physical sense.
FresnelEquations._θₜ
— MethodTransmitted angle as function of n₁, n₂ and θᵢ. By Snell's law, intended for internal use as default argument value for θₜ.
FresnelEquations.r_p
— Functionr_p(n₁, n₂, θᵢ)
r_p(n₁, n₂, θᵢ, θₜ)
Calculate the reflection coefficient for p-polarized light, i.e. the factor gained by the E-field amplitude by the reflection.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations.r_s
— Functionr_s(n₁, n₂, θᵢ)
r_s(n₁, n₂, θᵢ, θₜ)
Calculate the reflection coefficient for s-polarized light, i.e. the factor gained by the E-field amplitude by the reflection.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations.t_p
— Functiont_p(n₁, n₂, θᵢ)
t_p(n₁, n₂, θᵢ, θₜ)
Calculate the transmission coefficient for p-polarized light, i.e. the factor gained by the E-field amplitude by the transmission.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal
FresnelEquations.t_s
— Functiont_s(n₁, n₂, θᵢ)
t_s(n₁, n₂, θᵢ, θₜ)
Calculate the transmission coefficient for s-polarized light, i.e. the factor gained by the E-field amplitude by the transmission.
The transmitted angle θₜ defaults to asin(n₁ / n₂ * sin(θᵢ))
, which Snell's law states.
Arguments:
n₁: The refractive index of the original medium n₂: The refractive index of the medium transmitted into θᵢ: The incident angle in radians, meansured from the surface normal θₜ: The transmitted angle in radians, measured from the surface normal