Fourier Series Properties & Parseval's Theorem
Linearity, time-shift, and the power equivalence between time and frequency domains
If a signal carries 17 watts of power in the time domain, how is that power distributed across its frequency components — and why must the two views always agree?
Properties That Simplify Analysis
Once you can compute a Fourier series, a handful of properties let you avoid recomputing it from scratch for related signals. Two of the most important are linearity and the time-shift property. These are analogous to properties you will encounter for the Fourier transform in the next lesson.
Linearity
The Fourier series is a linear operation. If x₁(t) has coefficients cₙ⁽¹⁾ and x₂(t) has coefficients cₙ⁽²⁾, then a·x₁(t)+b·x₂(t) has coefficients a·cₙ⁽¹⁾+b·cₙ⁽²⁾. This follows directly from the linearity of the integral that defines cₙ.
In practice, this means you can build up the spectrum of a composite signal from the spectra of its parts, without doing any new integrals.
Time-Shift Property
If you delay a signal by t₀ — forming x(t−t₀) — each exponential coefficient cₙ picks up a phase factor e−jnω₀t₀. The magnitude |cₙ| does not change; only the phase rotates. Shifting a signal in time does not change which frequencies are present or how much energy each carries — it only changes the relative alignment (phase) of the components.
The time-shift property tells you that the power spectrum |cₙ|² is time-shift invariant. This is why power calculations — like Parseval's theorem — don't depend on when you start your clock.
Parseval's Theorem for Periodic Signals
Parseval's theorem says: the average power of a periodic signal — computed by integrating |x(t)|² over one period — is exactly equal to the sum of the average powers in each harmonic component. The theorem is a direct consequence of the orthogonality of the Fourier basis functions: cross-terms between different harmonics integrate to zero, so the total power cleanly separates into a sum of individual harmonic powers.
In Module 8 you learned that the average power of a single sinusoid A cos(ωt) is A²/2. Parseval's theorem generalizes this: the total power is the DC power (a₀²) plus the power of each harmonic, where each cosine and sine term contributes (aₙ²+bₙ²)/2.
You can compute the average power of x(t) two ways: (1) directly in the time domain, P=(1/T₀)∫|x(t)|²dt, or (2) by summing the power in each frequency component using Parseval's formula. They must give the same result — a consequence of orthogonality. If the two methods disagree, you've made a computational error somewhere.
Connecting to the Single-Sinusoid Result
Recall from Module 8 that a single sinusoid A cos(ωt) has average power A²/2. In Parseval's formula, the n-th harmonic consists of aₙcos(nω₀t)+bₙsin(nω₀t): the cosine part contributes aₙ²/2 and the sine part contributes bₙ²/2, so the harmonic's total power is (aₙ²+bₙ²)/2. The DC term a₀ is a constant, so its power is simply a₀². Parseval's theorem is a direct extension of the single-sinusoid power result to an arbitrary sum of harmonics.
Why Parseval Matters in Practice
Parseval's theorem tells you that the Fourier coefficients cₙ (or aₙ, bₙ) carry complete information about the signal's power — no need to go back to the time domain. This is the basis for power spectral density analysis, filter design, and signal-to-noise ratio calculations you'll encounter later in the course and in communications systems. In the exponential form, Parseval's theorem becomes P=Σ|cₙ|², especially clean and reinforcing that each coefficient's squared magnitude represents the power at that frequency.
- Write Parseval's formula: P = a0² + (1/2)Σ(an²+bn²) for n = 1 to ∞.
- Only a0 and a1 are nonzero, so the sum reduces to a single term: P = a0² + (1/2)(a1²+b1²) = 3² + (1/2)(4²+0²).
- Compute: P = 9 + (1/2)(16) = 9 + 8 = 17.
- Apply Parseval's theorem: P = a0² + (1/2)(a1²+b1²).
- Substitute: P = 2² + (1/2)(6²+0²) = 4 + (1/2)(36).
- Compute: P = 4 + 18 = 22.
Check your understanding
- The linearity property states that the Fourier series of a weighted sum of signals is the weighted sum of their individual Fourier series.
- The time-shift property states that delaying x(t) by t0 multiplies each coefficient cn by e^(-jnω0t0), leaving the magnitude |cn| (and hence the power spectrum) unchanged.
- Parseval's theorem equates the average power of a periodic signal computed in the time domain to the sum of powers in each harmonic: P = a0² + (1/2)Σ(an²+bn²).
- Each harmonic's power (an²+bn²)/2 generalizes the single-sinusoid result P = A²/2 from Module 8, while the DC term contributes a0².