Spectral Density

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The Spectral Density Sy(f) of the real random process y(t) is defined as


S_y(f) = \begin{matrix}\textrm{lim}\\T\rightarrow\infty\end{matrix} \frac{2}{T}\left|\int^{+T/2}_{-T/2} \left[y(t)-\bar{y}\right] e^{2 \pi i f t} dt\right|^2

where \bar{y} is the time average of y(t) (note that the above definition of Sy(f) assumes that the process is ergodic.) The factor of 2 found in the definition of Sy(f) accounts for the fact that the spectral density is defined over only positive frequencies: for a real process y(t), Sy(f) = Sy( − f), so that negative frequencies contain no new information. The factor of 2 essentially fold the negative frequencies onto the positive ones.


Given the spectral density, the variance of y(t) may be easily computed by using the relation

\sigma_y^2 = \int_{0}^{\infty}S_y(f) df
.

For any random process y(t), the Spectral Density, Sy(f) is related to the Correlation Function, Cy(τ), through the Wiener-Khintchine Theorem:


C_y(\tau) = \int_0^\infty S_y(f) \cos{(2\pi f \tau)} df
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