FresnelEquations.R_pFunction
R_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_sFunction
R_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_pFunction
T_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_sFunction
T_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.r_pFunction
r_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_sFunction
r_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_pFunction
t_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_sFunction
t_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