Relationship between Fourier coefficients and power spectral density

In summary, Parseval's Theorem relates the phase ##\phi(x,y)## to the power spectral density ##\Phi(f_{x_n},f_{y_m})## by equating the integral of the squared magnitude of the Fourier coefficients ##|c_{n,m}|^2## to the integral of the power spectral density. In the discrete case, this integral can be approximated as a sum over frequency bins, resulting in the equation ##|c_{n,m}|^2 \approx \Phi(f_{x_n}, f_{y_m})\sum_{f_{x_n}} \sum_{f_{y_m}}\Delta f_x \Delta f_y##. The ensemble average ##\langle|c_{
  • #1
Skaiserollz89
9
0
Homework Statement
Show that ##\langle|c_{n,m}|^2\rangle=\Phi(f_{x_n},f_{y_m})\Delta f_{x_n} \Delta f_{y_m}##, where
##\langle|c_{n,m}|^2\rangle## is the ensemble average of fourier coefficients of a phase screen given by ##\phi(x,y)=\sum\sum c_{n,m}e^{i2\pi(f_{x_n}x+f_{y_m})} ##, and ##\Phi(f_{x_n},f_{y_m})## is the phase power spectral density is the squared-magnitude of the fourier transform of ##\phi(x,y)##.
Relevant Equations
$$\langle|c_{n,m}|^2\rangle=\Phi(f_{x_n},f_{y_m})\Delta f_{x_n} \Delta f_{y_m}$$

$$\phi(x,y)=\sum\sum c_{n,m}e^{i2\pi(f_{x_n}x+f_{y_m}y)} $$

Parseval's Theorem:
$$\int\int_{-\infty}^{+\infty}|\phi(x,y)|^2 \,dx\,dy=\int\int_{-\infty}^{+\infty}\Phi(f_{x_n},f_{y_m}) \,df_x\,df_y.$$
Here, ##\Phi(f_{x_n},f_{y_m})=|\mathscr{F(\phi(x,y))}|^2 ## is the Power Spectral Density of ##\phi(x,y)## and ##\mathscr{F}## is the Fourier transform operator.

Parseval's Theorem relates the phase ##\phi(x,y)## to the power spectral density ##\Phi(f_{x_n},f_{y_m})## by

$$\int\int_{-\infty}^{+\infty}|\phi(x,y)|^2 \,dx\,dy=\int\int_{-\infty}^{+\infty}\Phi(f_{x_n},f_{y_m}) \,df_x\,df_y$$

Substitution of ##\phi(x,y)=\sum\sum c_{n,m}e^{i2\pi(f_{x_n}x+f_{y_m}y)} ## into the left side of Parsevals Theorem yields

$$|c_{n,m}|^2=\int\int_{-\infty}^{+\infty}\Phi(f_{x_n},f_{y_m}) \,df_x\,df_y$$.In ##\langle|c_{n,m}|^2\rangle=\Phi(f_{x_n},f_{y_m})\Delta f_{x_n} \Delta f_{y_m}##, ##\langle|c_{n,m}|^2\rangle## represents the ensemble average of ##|c_{n,m}|^2## and ##\Delta f_{x_n}## and ## \Delta f_{y_m}## represent the frequency bin widths, so we need to consider the discrete nature of the Fourier transform I think.

In the continuous case, the expression ##|c_{n,m}|^2## represents the contribution of the continuous frequency range within the integral to the squared magnitude of the Fourier coefficient ##c_{n,m}##. However, in the discrete case, we can approximate this integral as a sum over the frequency bins.

Thus, we can rewrite the equation as:

$$ |c_{n,m}|^2 \approx \sum_{f_{x_n}} \sum_{f_{y_m}} \Phi(f_{x_n}, f_{y_m}) \Delta f_x \Delta f_y$$where ##\Delta f_{x_n}## and ##\Delta f_{y_m}## represent the width of the frequency bins.

By approximating ##\Phi(f_{x_n}, f_{y_m})## as constant within each sum, it can be moved out in front of the double sum. However, it's important to note that this is an approximation and assumes that ##\Phi(f_{x_n}, f_{y_m})## doesn't vary significantly within each sum.

$$ |c_{n,m}|^2 \approx \Phi(f_{x_n}, f_{y_m})\sum_{f_{x_n}} \sum_{f_{y_m}}\Delta f_x \Delta f_y$$From here, I am not really sure what additional simplifications I can make to get to the result that

$$ \langle|c_{n,m}|^2\rangle=\Phi(f_{x_n},f_{y_m})\Delta f_{x_n} \Delta f_{y_m} $$

but it seems as though the ensemble average has something to do with collapsing the summation.
Any additional help here, or suggestions would be much appreciated.
 
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  • #2


One way to approach this problem is by considering the concept of ergodicity. In signal processing, ergodicity refers to the idea that the statistical properties of a signal can be determined by a single realization of the signal, as long as the signal is stationary (its statistical properties do not change over time).

In this case, we can consider our signal to be the function ##\phi(x,y)## and its Fourier transform ##\mathscr{F}[\phi(x,y)]##. By assuming ergodicity, we can say that the ensemble average of ##|c_{n,m}|^2## is equivalent to the time average of the squared magnitude of the Fourier transform at a specific point in space.

Using this idea, we can rewrite the ensemble average as:

$$\langle|c_{n,m}|^2\rangle = \frac{1}{T} \int_0^T |\mathscr{F}[\phi(x,y)]|^2 dt$$

where T represents the total time duration of the signal.

We can then apply Parseval's Theorem to this time average, which gives us:

$$\frac{1}{T} \int_0^T |\mathscr{F}[\phi(x,y)]|^2 dt = \frac{1}{T} \int_0^T \int\int_{-\infty}^{+\infty} \Phi(f_{x_n},f_{y_m}) df_x df_y dt$$

Since ##\Phi(f_{x_n},f_{y_m})## is constant with respect to time, we can move it out of the time integral, giving us:

$$\frac{1}{T} \int_0^T \int\int_{-\infty}^{+\infty} \Phi(f_{x_n},f_{y_m}) df_x df_y dt = \int\int_{-\infty}^{+\infty} \Phi(f_{x_n},f_{y_m}) df_x df_y$$

Now, we can equate this result with the previous expression for the ensemble average, giving us:

$$\int\int_{-\infty}^{+\infty} \Phi(f_{x_n},f_{y_m}) df_x df_y = \langle|c_{n,m}|^2\rangle$$

Comparing this with the previous equation we derived, we can see
 

1. What is the relationship between Fourier coefficients and power spectral density?

The Fourier coefficients and power spectral density are two mathematical concepts used to analyze signals in the frequency domain. The Fourier coefficients represent the amplitudes of the different sinusoidal components that make up a signal, while the power spectral density represents the distribution of power across different frequencies in the signal. In other words, the Fourier coefficients are used to calculate the power spectral density.

2. How are Fourier coefficients calculated?

Fourier coefficients are calculated using the Fourier transform, which is a mathematical operation that converts a signal from the time domain to the frequency domain. This involves decomposing the signal into its individual sinusoidal components and determining their amplitudes and frequencies. The resulting values are the Fourier coefficients.

3. What does the power spectral density tell us about a signal?

The power spectral density provides information about the distribution of power in a signal across different frequencies. This can help identify dominant frequencies and their amplitudes, as well as any underlying patterns or trends in the signal. It is often used in signal processing and analysis to understand the frequency characteristics of a signal.

4. How is the power spectral density related to signal power?

The power spectral density is directly related to signal power, as it represents the power of a signal at different frequencies. The total power of a signal can be calculated by integrating the power spectral density over all frequencies. In other words, the power spectral density is a measure of how much power is contained within each frequency component of a signal.

5. Can the Fourier coefficients and power spectral density be used for any type of signal?

Yes, the Fourier coefficients and power spectral density can be used for any type of signal, as long as it can be represented as a combination of sinusoidal components. This includes both continuous and discrete signals, and can be applied to various fields such as audio and image processing, communication systems, and physics.

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