When we talk about light pollution, most people imagine glowing cityscapes that obscure the stars. In infrared (IR) imaging and sensing, however, the term takes on a different meaning: stray light.
This blog explores the theoretical background of optical waveguides and demonstrates how to simulate them using Ansys Lumerical MODE and Finite-Difference Time-Domain (FDTD) solvers.
Diffraction is a fundamental optical phenomenon that occurs when light interacts with an obstacle or aperture, bending and spreading rather than traveling in a straight line.