Amplitude spectral density 2026-10-18
An amplitude spectral density is the square root of a power spectral density. For an electric potential difference expressed in volts and frequency in hertz, its units are .
Electrical noise reduction starts by identifying what is unwanted in the measured signal and where it enters. Increasing gain amplifies both signal and input noise; it does not by itself improve the input signal-to-noise ratio. Separate intrinsic component fluctuations, amplifier noise and external pickup before choosing a remedy.
Physical sources. A resistor at temperature has classical one-sided open-circuit thermal electrical noise density per hertz. In a flat measurement bandwidth , its rms voltage is . Lowering an appropriate resistance, reducing temperature or narrowing the useful bandwidth can reduce this noise, with loading and signal-gain tradeoffs considered. These are power spectral densities; an amplitude spectral density is their square root.
Discrete independent charge transfers give shot noise, with one-sided current density in the simple Poisson process model. Reducing leakage or unwanted bias current can help, but reducing a photocurrent may also reduce the desired signal. Charge correlations can change the simple shot-noise law. At low frequency, flicker noise and drift often dominate and are not described by a white spectrum.
Amplifier and impedance choice. An operational amplifier has equivalent input voltage and current noise. In a simplified uncorrelated model, a resistive source contributes the input-referred voltage densityHere are the voltage and current amplitude spectral densities and is the source electrical impedance; feedback components add further terms in a full circuit. Low current noise matters particularly for a high-impedance source, while voltage noise can dominate for a low-impedance source. Minimize needless source impedance, leakage and long sensitive connections without sacrificing the required transduction gain or bandwidth. Bias-current offsets and thermal drift also require calibration; they are not removed simply by quoting a random-noise density.
Pickup and bandwidth. Shield sensitive circuits against electric-field coupling, minimize loop area to reduce changing magnetic-flux pickup, and use twisted signal/return pairs or suitable coaxial connections. Differential readout rejects common-mode interference when impedances and amplifier responses are adequately matched. Plan the signal returns to avoid unwanted circulating ground currents, and decouple supply rails locally so supply fluctuations do not enter the signal path. Mechanical vibration, cable motion and temperature changes may be converted into electrical noise as well.
A low-pass filter removes out-of-band noise before digitization; an anti-aliasing filter is needed because digital filtering cannot undo already aliased content. Avoid a narrower passband than the physical signal requires. For a known periodic signal, modulation and a lock-in amplifier select a narrow frequency interval, often moving the measurement above a strong flicker noise region. A notch can reject a narrow interference line if that does not remove essential signal information.
Independent noise contributions add in variance, not directly in rms amplitude. Averaging independent equal-variance readings reduces the standard error by , but slow correlated drift and systematic errors need separate controls. Good noise reduction preserves the information-bearing signal while reducing unwanted coupling, intrinsic fluctuations or the admitted noise bandwidth.
Shot noise spectral convention 2026-10-18
Write an ideal point-transfer model using the Dirac delta function:For this arrival stream with independent increments, distinct arrivals contribute the product of the means, which cancels when centering. The same-arrival term leaves the autocovarianceIts Fourier transform gives the two-sided power spectral density, while folding negative frequencies onto positive ones gives the one-sided convention:These spectra describe , excluding the spectral line from the mean direct current. The amplitude spectral density is in ; it is not a root mean square electric current until a measurement signal bandwidth is specified. Approximate white noise requires frequencies low enough that the single-transfer pulse shape and any correlations can be neglected. Neither the ideal impulses nor a flat spectrum extending to infinity describe a real detector at every timescale.
All spectra above are per hertz, with in cycles per second. One possible angular frequency convention defines a density integrated using alone. Since , it hasAnother common convention keeps the numerical density but integrates it with . State the integration measure as well as whether a spectrum is one-sided: a change of variable and a folding of signs are separate operations.
Thermal noise spectral convention 2026-10-18
Model an ideal resistor of constant electrical resistance at uniform absolute temperature by its Thévenin equivalent: a zero-mean random voltage source in series with a noiseless . In the classical range its one-sided, open-circuit voltage power spectral density, per hertz, iswhere is the Boltzmann constant. Thus a positive-frequency interval of width contributes to the mean square voltage. This is approximately white noise only where the electrical resistance is effectively constant and , with the Planck constant. The ideal constant spectrum cannot describe arbitrarily high frequencies.[ref]
For a real voltage, an equivalent two-sided power spectral density is over signed frequencies. With a real linear time-invariant system of frequency response , the same output mean square isAngle brackets denote an expected value; for this zero-mean noise the mean square is its variance. Do not integrate over both signs of frequency: that counts the same fluctuations twice. All integrals here use frequency in hertz, not angular frequency . The amplitude spectral density is in , whereas the root mean square voltage requires a specified measurement signal bandwidth.