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Tutorial : source and screen conjugated by an optical system - lambertian source at infinity - aperture defined with F number

Radiometry and optical systems




Etendue conservation

Let consider a small light source of area dSo conjugated by a perfect optical system in Gauss conditions.

radiometry photometry The etendue in the object space is :

radiometry-photometry formula.

no is the refraction index in the object space, dΩo is the solid angle defined by the aperture angle io in the object space.

radiometry-photometry formula.

The etendue in the image space is :

radiometry-photometry formula.

no is the refraction index in the image space, dΩi is the solid angle defined by the aperture angle ii in the image space and dSi is the area of the source conjucgated.

radiometry-photometry formula.

The paraxial formulas give the following relations :

radiometry-photometry formula and radiometry-photometry formula.

m is the magnification of the optical system. Therfore :

radiometry-photometry formula.

The etendue is thus conserved through the optical system.

Considering the transmission T of the optical system and the flux in the object space d2Fo, the flux in the image space is :

radiometry-photometry formula.

Therefore, as radiometry-photometry formula, the radiance of the secondary source (conjugated of the initial source by the optical system) is :

radiometry-photometry formula.

If the initial and final media have the same refractive index, the ratio between the radiance of the conjugated source and the radiance of the initial source is equal to the transmission.



Irradiance produced by a source and an optical system

The irradiance on a screen can be anaytically calculated in some cases where light go through a perfect optical system ( in Gauss conditions).

radiometry photometry In the case where a punctual isotropic light source ( intensity I ) is in the focal plane of a system ( focal length fi ), the irradiance on a screen, whatever its position, is :

radiometry-photometry formula.

D is the aperture diameter and T is the system transmission.

radiometry photometry In the case of a small Lambertian source ( area S and radiance L ) located in the front focal plane of the slightly opened system, the beam is slightly diverging after being transmitted trough the optical system. Therefore, the irradiance depends on the position zi of the screen. Indeed, the flux after the system is :

radiometry-photometry formula.

Considering the beam area Si on the screen : radiometry-photometry formula.

Therefore, the irradiance E on the screen is :

radiometry-photometry formula.

radiometry photometry In the case where the screen is conjugated with a small Lambertian source ( area So and radiance L ) and considering that the system has a small aperture, the flux on the screen is :

radiometry-photometry formula.

xo is the algebric distance of the source.

radiometry-photometry formula where xi is the algebric distance of the source conjugate.

The magnification is given by :

radiometry-photometry formula.

If Si is the area on the screen and m is the magnification :

radiometry-photometry formula.

Then, the irradiance on the screen is :

radiometry-photometry formula.

In the case where the light source is at infinity and the screen is located in the back focal plane of the system :

radiometry-photometry formula.

radiometry photometry In this case, when defining the aperture with the aperture numbre N, the ratio between the irradiance on the screen with and without the optical system is ( the angular size α of the source is supposed to be small ) :

radiometry-photometry formula.