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Understanding Low-Frequency Oscillations

The millihertz (mHz) is a unit of frequency equal to 10⁻³ hertz, meaning one cycle occurs every 1,000 seconds or roughly 16.7 minutes. This low-frequency range is important in fields such as seismology, astrophysics, and geophysics, where it describes slow, periodic events that unfold over minutes to hours.

In astrophysics, millihertz frequencies are commonly observed in solar oscillations and stellar pulsations, providing key information about the internal structure and dynamics of stars. These oscillations help scientists understand energy transport, magnetic activity, and the life cycles of stars.

In geophysics, millihertz frequencies correspond to long-period seismic waves generated by earthquakes or volcanic activity. These waves travel long distances through the Earth’s interior and can reveal valuable data about its composition and structure.

Additionally, millihertz frequencies are relevant in oceanography and atmospheric science for studying tides, slow atmospheric waves, and other natural cycles that influence climate and weather patterns.

Because millihertz oscillations have relatively long periods and wavelengths, they allow researchers to probe processes that develop over extended timeframes and large spatial scales, bridging the gap between faster waves and ultra-low-frequency phenomena.

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.