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Brownian noise
Brownian noise
from Wikipedia
Sample trace of Brownian noise

In science, Brownian noise, also known as Brown noise or red noise, is the type of signal noise produced by Brownian motion, hence its alternative name of random walk noise. The term "Brown noise" does not come from the color, but after Robert Brown, who documented the erratic motion for multiple types of inanimate particles in water. The term "red noise" comes from the "white noise"/"white light" analogy; red noise is strong in longer wavelengths, similar to the red end of the visible spectrum.

Explanation

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The graphic representation of the sound signal mimics a Brownian pattern. Its spectral density is inversely proportional to f 2, meaning it has higher intensity at lower frequencies, even more so than pink noise. It decreases in intensity by 6 dB per octave (20 dB per decade) and, when heard, has a "damped" or "soft" quality compared to white and pink noise. The sound is a low roar resembling a waterfall or heavy rainfall. See also violet noise, which is a 6 dB increase per octave.

Strictly, Brownian motion has a Gaussian probability distribution, but "red noise" could apply to any signal with the 1/f 2 frequency spectrum.

Power spectrum

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Spectrum of Brownian noise, with a slope of –20 dB per decade

A Brownian motion, also known as a Wiener process, is obtained as the integral of a white noise signal: meaning that Brownian motion is the integral of the white noise , whose power spectral density is flat:[1]

Note that here denotes the Fourier transform, and is a constant. An important property of this transform is that the derivative of any distribution transforms as[2] from which we can conclude that the power spectrum of Brownian noise is

An individual Brownian motion trajectory presents a spectrum , where the amplitude is a random variable, even in the limit of an infinitely long trajectory.[3]

Production

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A two-dimensional Brownian noise image, generated with a computer program (subscription required)[a]
A 3D Brownian noise signal, generated with a computer program (subscription required)[a], shown here as an animation, where each frame is a 2D slice of the 3D array

Brown noise can be produced by integrating white noise.[4][5] That is, whereas (digital) white noise can be produced by randomly choosing each sample independently, Brown noise can be produced by adding a random offset to each sample to obtain the next one. As Brownian noise contains infinite spectral power at low frequencies, the signal tends to drift away infinitely from the origin. A leaky integrator might be used in audio or electromagnetic applications to ensure the signal does not “wander off”, that is, exceed the limits of the system's dynamic range. This turns the Brownian noise into Ornstein–Uhlenbeck noise, which has a flat spectrum at lower frequencies, and only becomes “red” above the chosen cutoff frequency.

Brownian noise can also be computer-generated by first generating a white noise signal, Fourier-transforming it, then dividing the amplitudes of the different frequency components by the frequency (in one dimension), or by the frequency squared (in two dimensions) etc.[6] Matlab programs are available to generate Brownian and other power-law coloured noise in one[7] or any number[8] of dimensions.

Experimental evidence

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Evidence of Brownian noise, or more accurately, of Brownian processes has been found in different fields including chemistry,[9] electromagnetism,[10] fluid-dynamics,[11] economics,[12] and human neuromotor control.[13]

Human neuromotor control

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In human neuromotor control, Brownian processes were recognized as a biomarker of human natural drift in both postural tasks—such as quietly standing or holding an object in your hand—as well as dynamic tasks. The work by Tessari et al. highlighted how these Brownian processes in humans might provide the first behavioral support to the neuroscientific hypothesis that humans encode motion in terms of descending neural velocity commands.[13]

Notes

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Brownian noise, also known as brown noise or red noise, is a type of stochastic signal noise characterized by a power spectral density (PSD) that decreases inversely with the square of the frequency, following a 1/f² relationship. This distribution emphasizes low frequencies, with power dropping at a rate of -20 dB per decade, distinguishing it from (flat PSD) and (1/f PSD). It models the cumulative effect of random fluctuations, analogous to the position of a particle undergoing in physics. The concept originates from Brownian motion, the irregular movement of microscopic particles in a fluid due to collisions with surrounding molecules, first observed by Scottish botanist Robert Brown in 1827. Albert Einstein provided a theoretical foundation in 1905. In signal processing, Brownian noise is generated by integrating white noise, resulting in a non-stationary process where variance grows linearly with time. Brownian noise appears in various physical systems, such as thermal fluctuations in mechanical oscillators or financial time series modeling random walks, and its PSD properties make it valuable for simulating natural phenomena in engineering and scientific contexts. In acoustics and audio engineering, it produces a deep, rumbling sound often used for sound masking and relaxation.

Definition and Fundamentals

Core Definition

Brownian noise, also referred to as brown noise or red noise—a term deriving from the analogy to light spectra, where red noise emphasizes lower frequencies similar to the longer wavelengths at the red end of the visible spectrum, akin to white noise's flat spectrum resembling white light—is a in which the signal's undergoes a , characterized by continuous sample paths that are nowhere differentiable . This results in a signal that accumulates random deviations over time without any inherent directionality or bounded variance in short intervals. Brownian noise represents the integral of , with each increment adding to the previous state in a cumulative manner. This integration leads to a power that decays as 1/f², emphasizing low-frequency components over the flat spectrum of . Brownian noise is distinguished from other noise types by its power spectral density. White noise exhibits a flat spectrum across all frequencies, pink noise has a spectrum decaying as 1/f, whereas Brownian noise decays as 1/f², resulting in a greater emphasis on lower frequencies. Unlike deterministic signals, which evolve according to fixed equations and exhibit repeatable patterns, Brownian noise is inherently random and unpredictable, with independent increments that preclude any long-term forecasting or periodic structure.

Historical Context

The concept of Brownian noise traces its origins to the observation of erratic particle motion by Scottish botanist Robert Brown in 1827, who noted the irregular jiggling of pollen grains suspended in water under a microscope, a phenomenon that persisted regardless of the particle type or environmental conditions. This discovery, initially puzzling and attributed to various causes like capillary action, remained unexplained until Albert Einstein provided a theoretical framework in 1905, interpreting the motion as the result of incessant bombardment by surrounding fluid molecules, thereby linking it to the kinetic theory of matter and offering indirect evidence for the existence of atoms. Einstein's explanation was experimentally validated by French physicist Jean Perrin starting in 1908, through meticulous measurements of particle displacements that matched the predicted diffusion behavior, confirming the molecular basis of the motion and quantifying atomic properties like Avogadro's number. Perrin's work, detailed in his 1909 publications and later expanded in his 1913 book Les Atomes, resolved longstanding debates about atomic reality and earned him the 1926 Nobel Prize in Physics for demonstrating the discontinuous structure of matter. The evolution from physical observation to formal noise theory began in the 1920s with American mathematician , who rigorously defined as a continuous Gaussian in his seminal 1923 paper "Differential Space," providing the mathematical foundation for modeling random fluctuations in physical systems. The term "brown noise" derives from this connection to observed by Robert Brown.

Mathematical Properties

Power Spectral Density

The power spectral density (PSD) of Brownian noise, which characterizes the random walk-like fluctuations in the position of a particle undergoing , is given by S(f)=Cf2S(f) = \frac{C}{f^2} for frequencies f>0f > 0, where CC is a positive constant and ff denotes the in Hz. This single-sided PSD formulation applies to positive frequencies. The constant CC is directly related to the variance of the underlying driving the process, ensuring the PSD units are consistent with power (e.g., variance) per unit frequency, such as m2/Hz\mathrm{m}^2 / \mathrm{Hz} for displacement noise. This 1/f21/f^2 form derives from the fact that Brownian noise represents the time integral of white noise, a stationary process with constant (flat) PSD Sξ(f)=σ2S_\xi(f) = \sigma^2, where σ2\sigma^2 is the noise variance. In the frequency domain, integration corresponds to multiplication by 1/(j2πf)1/(j 2\pi f), so the transfer function magnitude squared yields 1/(2πf)21/(2\pi f)^2. Thus, the PSD of the integrated process becomes S(f)=σ2/(2πf)2S(f) = \sigma^2 / (2\pi f)^2, establishing the 1/f21/f^2 scaling after normalizing the constant. This relationship highlights Brownian noise as a non-stationary process with stationary increments, allowing a well-defined PSD via the Wiener-Khinchin theorem applied to its covariance structure. A key property of this PSD is the divergence as f0f \to 0, resulting in theoretically infinite total energy unless the signal is band-limited.

Statistical Characteristics

Brownian noise is mathematically modeled as a standard W(t)W(t), a continuous-time with zero , E[W(t)]=0\mathbb{E}[W(t)] = 0, and variance that increases linearly with time, Var(W(t))=σ2t\mathrm{Var}(W(t)) = \sigma^2 t. The process features independent increments, where for 0s<t0 \leq s < t, the increment W(t)W(s)W(t) - W(s) is normally distributed as N(0,σ2(ts))\mathcal{N}(0, \sigma^2 (t - s)) and independent of the history up to time ss. These increments are Gaussian, which implies that the finite-dimensional distributions of the process are multivariate Gaussian, resulting in Gaussian marginal distributions at each fixed time tt. The autocorrelation function (or covariance function, since the mean is zero) for the non-stationary Wiener process is E[W(t)W(s)]=σ2min(t,s)\mathbb{E}[W(t) W(s)] = \sigma^2 \min(t, s), capturing the cumulative dependence from shared initial segments of the path. For the stationary approximation applied to increments, the process ΔW(t)=W(t+Δt)W(t)\Delta W(t) = W(t + \Delta t) - W(t) over fixed small intervals Δt\Delta t exhibits white noise characteristics with zero autocorrelation for non-overlapping intervals. Unlike white noise, which is stationary with constant variance, the Wiener process is inherently non-stationary due to its time-dependent variance, leading to unbounded growth in spread over long times and rendering the process non-ergodic.

Generation Methods

Brownian noise can be produced or approximated through synthetic and natural methods, with a focus on replicating its characteristic 1/f² power spectral density via principles such as integration of white noise or thermal fluctuations.

Synthetic Production

Synthetic production of Brownian noise involves algorithmic and hardware-based methods to replicate its characteristic 1/f² power spectral density. The most straightforward algorithmic approach is to compute the cumulative sum of independent Gaussian noise samples, yielding a discrete-time realization of . Specifically, the sequence is generated via the recurrence X{{grok:render&&&type=render_inline_citation&&&citation_id=0&&&citation_type=wikipedia}} = 0 and X=X[n1]+WX = X[n-1] + W for n=1,2,,Nn = 1, 2, \dots, N, where WW are i.i.d. Gaussian random variables with mean zero and variance σ2\sigma^2. This method ensures the increments are Gaussian while the process exhibits the integrated behavior central to Brownian noise. In digital implementations, this cumulative summation is efficiently realized using built-in functions in scientific computing libraries. For instance, in Python with , the code np.cumsum(np.random.randn(N)) produces a sequence of length NN scaled to unit variance increments, which can be adjusted by multiplying by σ\sigma. Similarly, MATLAB's cumsum(randn(N,1)) achieves the same result. These software methods are computationally inexpensive and allow for high-fidelity generation over arbitrary lengths, provided the sampling rate is sufficiently high to capture the desired frequency range. Analog synthesis mimics the integration of thermal noise using circuits, where white noise from a or zener breakdown is passed through an or multiple low-pass stages to approximate the 1/f² roll-off. A practical circuit employs a reverse-biased or for generation, followed by an op-amp with feedback to produce the cumulative effect, ensuring stability through component selection like a 1 kΩ and 1 μF . Alternatively, frequency-domain filtering applies a 1/f² weighting to the of white noise before inverse transformation; this involves generating complex , multiplying magnitudes by 1/f21/|f|^2 (with phase preservation), and performing the inverse FFT. Practical considerations include band-limiting to mitigate low-frequency divergence, as the unbounded variance growth (Var(X)=σ2t\text{Var}(X) = \sigma^2 t) can lead to numerical instability; a at 20 Hz or windowing techniques confines the spectrum to relevant bands. Scaling for target variance involves multiplying the increments by σΔt\sigma \sqrt{\Delta t}
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