Lens (optical) distortion is an aberration that causes straight lines to curve near the edges of images. It can be troublesome for architectural photography and photogrammetry (measurements derived from images). The simplest approximation is the 3rd order equation, ru = rd + krd3 where ru is the undistorted and rd is the distorted radius. Depending on the sign of k, it can be either “barrel” (shown on the right) or “pincushion.” A mixture known as “mustache” distortion may occur for complex lenses when the coefficients of the 5th order approximation (ru = rd + h1rd3+ h2rd3) have opposite signs.
Lens distortion and coefficients for correcting it are calculated in the Distortion module, which contains 3rd order, 5th order and tangent/arctangent distortion models, and in Dot Pattern, which performs a CPIQ-compliant distortion measurement. SFRplus and Checkerboard measure distortion in nearly as much detail as the Distortion module, along with sharpness and several other factors. SFRplus distortion results are in the Image, Geometry, Distortion, FoV and Radial distortion plots. eSFR ISO measures distortion with slightly less precision than SFRplus.
Distortion is worst in wide angle, telephoto, and zoom lenses. It often worse for close-up images than for images at a distance. It can be easily corrected in software. Picture Window Pro and PTLens have tools for removing it.