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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 Interstellar and Cosmological Waves

A petametre (Pm) equals 1,000 terametres (10¹⁵ metres), representing unimaginably vast distances that describe the longest electromagnetic wavelengths in the universe. These wavelengths correspond to frequencies in the attohertz (10⁻¹⁸ Hz) and lower ranges, which are mostly relevant in cosmology, astrophysics, and the study of gravitational waves and large-scale cosmic phenomena.

For context, a frequency of 1 attohertz (10⁻¹⁸ Hz) corresponds to a wavelength of approximately 300 petametres. This scale is far beyond any human-made signals and reflects waves that stretch across entire galaxies or even clusters of galaxies. Such waves help scientists study the cosmic microwave background (CMB) fluctuations, the large-scale structure of the universe, and primordial gravitational waves created shortly after the Big Bang.

Using petametres to measure wavelength allows researchers to grasp the vastness of these cosmic oscillations and the slowest processes influencing the universe’s evolution. These extreme wavelengths provide crucial insight into the origins, expansion, and ultimate fate of the cosmos.