Infrared radiation

Spectrum and approximate subbands

Infrared is commonly divided into overlapping bands rather than rigid borders. Typical, approximate categories are:

• Near infrared (NIR): just beyond visible red, roughly 0.7–1.4 µm (700–1,400 nm); used for short-range communications and many consumer sensors (example wavelengths).
• Short‑wave and mid‑infrared: extending from about 1.4 µm into a few micrometres; important for spectroscopy of molecules.
• Long‑wave or thermal infrared: roughly 8–15 µm, commonly used in thermal imaging because it matches room-temperature thermal emission (8–15 µm ranges).
• Far infrared: longer wavelengths that overlap with submillimetre radiation and approach radio bands.

Emission, absorption and atmospheric windows

All objects with temperatures above absolute zero emit infrared according to their temperature and emissivity. Molecular vibrations and rotations produce characteristic absorption and emission features in the IR, which makes infrared thermal and spectroscopic methods valuable for chemistry and materials analysis. The Earth's atmosphere absorbs IR strongly at many wavelengths; however, there are transmission "windows" where certain bands pass the atmosphere relatively well. These windows are exploited by ground‑based astronomy and remote sensing.

Detection technologies

Different detectors are optimized for different IR bands. Near‑IR uses semiconductor photodiodes and avalanche photodiodes; mid‑ and long‑wave IR often require thermal detectors such as bolometers, microbolometer arrays (commonly used in uncooled thermal cameras), pyroelectric sensors, or cooled semiconductor detectors for high sensitivity. Choice of detector depends on wavelength, required speed, sensitivity, and whether imaging or single‑point detection is needed.

Applications

• Consumer electronics: many remote controls and short‑range links use near‑IR LEDs and photodetectors (remote controls).
• Thermal imaging and building inspection: cameras create images from emitted thermal radiation to reveal heat loss, electrical faults, or people in low‑visibility conditions.
• Communications: optical fibers and some free‑space links use near‑IR wavelengths for efficient transmission over long distances.
• Scientific analysis: infrared spectroscopy identifies molecular bonds and monitors composition in laboratories and industry.
• Astronomy: IR telescopes detect cool objects, peer through dust clouds, and study star and planet formation.
• Defense and safety: heat‑seeking trackers and some guidance systems exploit IR contrast; certain guided weapons use infrared seekers to detect engine heat (missiles), while broader systems relate to air defence and tracking.

Biological and safety notes

People perceive infrared indirectly as warmth rather than as visible light. Some animals have specialized IR detection: for example, certain snakes sense thermal radiation to detect prey. Prolonged exposure to intense IR sources can cause thermal burns or eye damage, so appropriate protection is used in industrial and medical settings.

History and further reading

Infrared radiation was first identified in the early 19th century by experiments that detected heat beyond the red portion of the visible spectrum. Since then IR techniques have become central to fields ranging from climate science and remote sensing to medicine and telecommunications. For background on the physical principles and instrumentation, see basic treatments of the electromagnetic spectrum, wave propagation and detector physics (wave theory, electromagnetism), practical notes on visible versus infrared optics, and technical references on microwave and infrared engineering. Manufacturer guides and review articles provide detailed operational ranges such as near‑IR markers and thermal imaging bands like 8–15 µm.