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Understanding Extremely Low Frequency Waves

A kilometre (km) is a unit of length equal to 1,000 metres, and in the context of electromagnetic waves, it is used to describe extremely long wavelengths, typically in the Very Low Frequency (VLF) and Extremely Low Frequency (ELF) ranges. These wavelengths correspond to very low frequencies, usually below 300 kHz, and are commonly used in long-distance radio communication, submarine communication, navigation systems, and geophysical research.

For instance, a frequency of 30 kHz has a wavelength of 10 km, while 3 kHz corresponds to a wavelength of 100 km. These long wavelengths can travel great distances, penetrate seawater, and diffuse around obstacles, making them ideal for communication with submerged submarines and in areas where traditional signals cannot reach. ELF waves, with wavelengths of hundreds to thousands of kilometres, are also used in Earth monitoring, such as detecting seismic or lightning activity.

Using kilometres to measure wavelength allows scientists and engineers to understand and design systems for global communication and natural signal monitoring. Although challenging to generate and detect, kilometre-scale wavelengths play a vital role in specialized but critical applications.

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.