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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.

Describing Very Low Frequency Radio Waves

A hectometre (hm) is a unit of length equal to 100 metres, and it is used to describe very long wavelengths in the Very Low Frequency (VLF) and Low Frequency (LF) bands of the electromagnetic spectrum. Wavelengths in the hectometre range correspond to frequencies between approximately 3 kHz and 3 MHz. These long wavelengths are typically used for maritime navigation, military submarine communication, AM radio broadcasting, and time signal transmissions.

For example, a signal at 300 kHz has a wavelength of 1 kilometre, or 10 hectometres, and a signal at 1 MHz corresponds to 3 hectometres. These long wavelengths have the unique ability to travel long distances and penetrate water and the ground, which is why they are used in submarine communications and emergency broadcast systems.

Using hectometres to express wavelength offers a practical scale for understanding wave propagation over great distances. It also aids in antenna design, where very large antennas—often hundreds of metres long—are needed to efficiently transmit or receive these frequencies. Understanding wavelength in hectometres is important in geophysics, radio astronomy, and large-scale communications infrastructure.