
The passage of electromagnetic radiation through a medium.Transmission is the process by which electromagnetic radiation (or other waves) passes through a medium without being absorbed or reflected. It is a fundamental concept in optics, atmospheric science, and astrophysics, determining how much light reaches our eyes from distant objects. The degree of transmission depends on the material's properties, the wavelength of the radiation, and the path length through the medium.
The quantitative study of transmission began with Pierre Bouguer in 1729 and was extended by Johann Heinrich Lambert in 1760 and August Beer in 1852, leading to the Beer-Lambert law.
When light encounters a medium, its electric field interacts with the atoms or molecules. If the light's frequency does not match an absorption transition, the medium's electrons are forced to oscillate and re-emit the light, effectively passing it along. This re-emission can be slightly delayed, causing a change in the speed of light (refraction). Transmission is reduced by absorption (where energy is converted to heat) and scattering (where light is redirected). The Beer-Lambert law quantifies this: transmitted intensity decreases exponentially with path length and absorption coefficient.
Transmission is exploited in fiber-optic communications, where light pulses travel through glass fibers; in atmospheric remote sensing, where satellite signals pass through the air; and in medical imaging, such as X-ray radiography, where tissue transmission reveals internal structures.
The Earth's atmosphere is almost perfectly transparent to visible light but strongly absorbs infrared and ultraviolet radiation, which is why we can see the sun but get sunburned.





