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Understanding Infrared and Thermal Radiation

A micrometre (µm), also known as a micron, is equal to one millionth of a metre (1 µm = 10⁻⁶ m) and is commonly used to express wavelengths of electromagnetic radiation, particularly in the infrared (IR) region of the spectrum. Wavelengths in this range are crucial for understanding heat, thermal imaging, remote sensing, and optical communications. The infrared spectrum typically spans from 0.75 µm to about 1000 µm, with specific regions divided into near-IR (0.75–1.4 µm), mid-IR (1.4–8 µm), and far-IR (8–1000 µm).

Many natural processes, including thermal emission from objects, occur in the micrometre wavelength range. For example, the human body emits peak thermal radiation at around 9–10 µm. Materials scientists, astronomers, and engineers use these wavelengths to study heat flow, detect gases, and design sensors. Optical fibers used in telecommunications also operate efficiently in the near-IR range around 1.3 to 1.55 µm. Using micrometres to describe wavelength offers a practical and precise way to work with electromagnetic waves that are too long for nanometres but still far shorter than those measured in millimetres.

The Scale of Extremely Low Frequency and Astrophysical Waves

A gigametre (Gm) is equal to 1,000,000,000 metres (10⁹ m) and is used to describe extraordinarily long wavelengths found primarily in the extremely low frequency (ELF) band and in astrophysical phenomena. These wavelengths correspond to frequencies in the millihertz to microhertz range, far below typical human-made radio communications. Gigametre-scale wavelengths are associated with very slow oscillations in space plasmas, planetary magnetospheres, and cosmic radio waves.

For example, a frequency of 1 microhertz (10⁻⁶ Hz) corresponds to a wavelength of about 300 million kilometres (300 Gm), which is roughly twice the distance from the Earth to the Sun. Such enormous wavelengths are significant in studying solar-terrestrial interactions, long-period gravitational waves, and other phenomena in astrophysics and cosmology.

Although gigametre wavelengths are not practical for terrestrial communications, they help scientists understand the large-scale electromagnetic environment of the solar system and beyond. Using the gigametre unit allows researchers to quantify these immense scales and analyze signals and waves that influence planetary environments, space weather, and the interstellar medium.