Optical window

  In astronomy, the optical window is the optical portion of the electromagnetic spectrum that passes through the atmosphere all the way to the ground. Most EM wavelengths are blocked by the atmosphere, so this is like a window that lets only a narrow selection of what is out there, though the Sun is particularly active in the passed wavelengths. It is called "optical" because the wavelengths we can see are all in this range. The window runs from around 300 nanometers (ultraviolet-C) at the short end up into the range the eye can use, roughly 400-700 nm and continues up through the visual infrared to around 1100 nm, which is thermal infrared.

Additional recommended knowledge

Daily Sensitivity Test

Essential Laboratory Skills Guide

Safe Weighing Range Ensures Accurate Results

There are also infrared and "radio windows" that transmit some infrared and radio waves. The radio window runs from about one centimeter to about eleven-meter waves.

In medical physics, the optical window is the portion of the visible and infrared spectrum where living tissue absorbs relatively little light. This window runs approximately from 650 nm to 1200 nm. At shorter wavelengths light is strongly absorbed by hemoglobin in blood, while at longer wavelengths water strongly absorbs infrared light.

Optical window can also mean a (usually flat, sometimes optical flat) piece of transparent optical material that allows light into an optical instrument.

See also

• Radio window
• Atmospheric window
• Astronomical window