Tutorial : miscellaneous - power of an optical system

Focal lengths are necessary parameters for calculating the paraxial image of a given object.

The front effective focal length f is the algebric distance NF from the front nodal point ( or primary principal point ) N to the front focal point F or from the primary principal plane H to the front focal plane P_f.
The back effective focal length f_i is the algebric distance N_iF_i from the back nodal point ( or secondary principal point ) N_i to the back focal point F_i or from the secondary principal plane H_i to the back focal plane P_fi.

The optical system is said positive (or converging) in the case where the effective back focal length is positive with respect to the direction of the emerging rays. It its said negative (or diverging) otherwise. Sometimes (particulary in ophtalmic optic), focal lengths are replaced by their inverse value which is commonly called the power.

As principal planes are generally not coinciding with a surface of the system, it is also useful to calculate the front and back focal lengths f_t and f_b.

f_t is the algebric distance from the vertex of the first optical surface to the front focal point F.
f_b is the algebric distance from the vertex of the last optical surface to the back focal point F_i.

The front and back focal lengths (not to be confused with front and back effective focal lengths) are not used for optical calculations but for positionning the focal planes regarding a mechanical reference.

Note that the definitions of the front and back focal lengths given above are not standard. For instance, some manufacturers selling mounted lenses may define the front and back focal lengths referred to the mount.

Some other characteristic lengths may be necessary to locate the principal planes referred to mechanical references. They are listed below :

l - distance from the vertex of the first optical surface to the primary principal point N ;
l_i - distance from the vertex of the last optical surface to the secondary principal point N_i ;
d - distance from the primary principal plane H to the secondary principal plane H_i .