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Measuring Light and Electromagnetic Waves

A nanometre (nm) is a unit of length equal to one billionth of a metre (1 nm = 10⁻⁹ m) and is commonly used to express wavelengths of light and other electromagnetic waves. In this context, nanometres provide a convenient scale for describing phenomena that occur at the atomic and molecular level. Visible light, for example, spans wavelengths from about 380 nm (violet) to 750 nm (red). Ultraviolet (UV) light has shorter wavelengths, typically between 10 nm and 400 nm, while infrared (IR) light has longer wavelengths, from about 750 nm to 1,000,000 nm.

Wavelengths in nanometres are critical in fields like optics, photonics, spectroscopy, and nanotechnology. They determine the energy and color of light, how it interacts with matter, and how it can be manipulated in devices like lasers, fiber optics, and solar cells. Shorter wavelengths (in the UV or X-ray range) carry more energy and are used in applications such as medical imaging and semiconductor fabrication. Understanding and working with wavelengths in nanometres allows scientists and engineers to explore and control the behavior of light at extremely small scales—down to the size of atoms and molecules.

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.