"evolution of noise" is a correct and usable phrase in written English.
It refers to the gradual development and changes in the concept and perception of noise over time. Example: The evolution of noise in modern society can be traced back to the invention of the steam engine and the subsequent industrialization, which brought about a shift from the natural sounds of the countryside to the constant hum of machines in urban areas.
The long term noise behavior in large and narrow lines has been studied and the possibility of using the evolution of noise during lifetime tests as a very sensitive precursory indicator of failure in lines and vias has been investigated.
This figure shows the evolution of noise levels given by INM under the flight path (INM curve) [16, 17] for standard trajectories in accordance with ICAO specifications [22, 40, 41, 42], and by the method described in this paper.
The present implementation facilitates a large number of computational tasks, including the definition, manipulation and parametrization of quantum states, the evaluation of quantum measures and quantum operations, the evolution of quantum noise in discrete models, quantum measurements and state estimation, and several others.
Fig. 13 Time evolutions of estimated noise level with error margins at tidal frequency bands of the six OBTMs.
Still, even some of those who have followed the long evolution of the new noise law say it will catch the city off guard.
Evolution of the obtained noise levels under the flight path, given by INM for standard trajectories in accordance with ICAO specifications, is compared with the optimized values behavior.
In this view, the potential deleterious effects of changes in dosage have been partly mitigated by the evolution of mechanisms for noise reduction and coordinated regulation.
Since the isogenic phenotypic fluctuation Vip increases with noise, this means that evolution of robustness is possible only when the amplitude of phenotypic noise is larger than some critical value as derived by Vip≥Vg, implying a positive role of noise to evolution.
We show that analysis of uncertainties may be useful for understanding the sensitivity of the model predictions to short-term evolution of magnetic field and noise in the synoptic magnetograms.
Very Large Array (VLA) observations at 20 and 91 cm wavelength are compared with data from the SOHO (EIT and MDI) and RHESSI solar missions to investigate the evolution of decimetric Type I noise storms and Type III bursts and related magnetic activity in the photosphere and corona.
