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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.

The Scale of Ultra-Low Frequency Waves

A megametre (Mm) equals 1,000,000 metres (10⁶ m) and is used to describe extraordinarily long wavelengths found in the ultra-low frequency (ULF) and extremely low frequency (ELF) bands of the electromagnetic spectrum. These wavelengths correspond to frequencies less than a few hertz, often in the range of millihertz to a few hertz. At this scale, wavelengths span hundreds to thousands of kilometres, extending into the megametre range.

Waves with megametre-scale wavelengths are critical for studying natural phenomena such as Earth’s magnetospheric oscillations, geomagnetic pulsations, and seismic electromagnetic signals. These frequencies and wavelengths are also important in geophysical research, allowing scientists to monitor changes in the Earth’s magnetic field and space weather effects. For example, a frequency of 0.1 Hz corresponds to a wavelength of about 3,000,000 metres, or 3 Mm.

Because of their immense scale, megametre wavelengths are not used for typical communication systems but are crucial in understanding planetary and space environments. Using the megametre unit helps researchers conceptualize and quantify these gigantic waves, linking electromagnetic theory with geophysical observations and space science.