A measure of the short-term frequency stability of a signal, expressed in dBc/Hz at a given offset.Phase noise is a measure of the short-term frequency stability of a signal, expressed in dBc/Hz at a given offset from the carrier frequency. It describes how much a signal's phase (and therefore its frequency) fluctuates over very short timescales. In any real oscillator, the output is not a perfect single frequency; it has a 'skirt' of noise around the carrier, and phase noise quantifies the power in that skirt relative to the carrier power, in a 1 Hz bandwidth, at a specific frequency offset.
The concept was formalized in the mid-20th century with the development of radar and microwave communications, where frequency stability became critical. Key contributions came from researchers like W. A. Edson and later D. B. Leeson, whose model (1966) remains a standard for understanding oscillator phase noise.
Phase noise arises from random fluctuations in the phase of an oscillator's output, caused by thermal noise, shot noise, and other stochastic processes in the active and passive components. These fluctuations spread the signal's power from the ideal single line into a continuous spectrum. The measurement involves comparing the signal to a reference or using a phase detector to isolate the phase fluctuations, then analyzing their spectral density.
Phase noise is critical in radar systems, high-speed digital communications, and precision timekeeping. Low phase noise oscillators are essential for accurate GPS, satellite communication, and the synchronization of large arrays like the Event Horizon Telescope.
The 'ringing' of a radio signal from space, as described in the article 'Радиосигнал из космоса зазвучал как колокол', is essentially a manifestation of phase noise in the signal's source, revealing the internal dynamics of a neutron star or pulsar.





