Telecentric Lens Design
Magnification change Δm/m = −Δz/(s_EP + Δz) of an ordinary lens against a telecentric lens with a residual chief-ray slope, and the depth of field λ/NA² + e/(m·NA).
Results
With the sensor fixed, an image point lands where its chief ray does, so a lens whose entrance pupil sits s_EP from the object changes magnification as the object moves. Telecentricity puts the pupil at infinity; a residual slope θ_t at the field edge acts like a distant pupil. A negative slope is hypercentric.
Magnification change vs object displacement
Model and references
Textbook approximation. A standard approximation from the literature (for example paraxial, plane-wave or Gaussian-beam), valid within the range the page states. About the tiers
Paraxial chief ray with the sensor fixed: the blur centroid follows the chief ray. A residual telecentric slope is treated as a distant entrance pupil. The depth of field is Inoué's sum of a wave and a geometric term in air.
- Greivenkamp J. E. (2004). Field Guide to Geometrical Optics. SPIE Press. Telecentricity: the entrance pupil at infinity keeps the chief ray parallel to the axis, so magnification does not change with focus. doi:10.1117/3.547461
- Inoué S., Spring K. R. (1997). Microscope Image Formation. In: Video Microscopy, 2nd ed., ch. 2, pp. 13–117. Plenum. Total depth of field d = λ₀n/NA² + n·e/(M·NA). doi:10.1007/978-1-4615-5859-0_2