1/f = 1/o + 1/i
Here, f is the focal length of a thin lens, and o and i are the object and image distances, respectively.
However, what if we used the inverses of the quantities (f, o, and i) involved?
Then the equation takes the (arguably) simpler form of:
F = O + I
where:
F = 1/f
O = 1/o
I = 1/i
Now, if we know two of the quantities involved, we can find the third by a simple addition or subtraction.
Since f, o, and i are lengths (distances), the quantities F, O, and I have units of 1/length.
If lengths are measured in meters (m), then F, O, and I have units of:
1/meter (1/m)
The unit 1/m is called a diopter, usually denoted by the symbol D.
F is called the lens power, and O and I are the object and image vergences.
Working with lens power has the aesthetically pleasing result that a stronger lens (i.e., the light is bent more) has a higher lens power.
Also, if the air spaces between lenses are small enough to be ignored, the total power of multiple thin lenses is just the sum of the individual component powers.
Diopter units are most commonly found in ophthalmic optics.
After an eye examination, the prescription you are given for corrective spectacles or contact lenses is simply the power of the required corrective lens, in diopters.
While diopters are often associated with vision correction, the concept of lens power and vergence is fundamental across optical system design.
Understanding how powers add—and how systems behave when lenses are combined—becomes especially important in: