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## Example 1: FFT of a Simple Sinusoid

Our first example is an FFT of the simple sinusoid

where we choose (frequency ) and (sampling rate set to 1). Since we’re using the FFT, the signal length must be a power of . Here is the Matlab code:echo on; hold off; diary off; % !/bin/rm -f examples.dia; diary examples.dia % For session log % !mkdirs eps % For figures% Example 1: FFT of a DFT sinusoid

% Parameters: N = 64; % Must be a power of two T = 1; % Set sampling rate to 1 f = 0.25; % Sinusoidal frequency in cycles per sample A = 1; % Sinusoidal amplitude phi = 0; % Sinusoidal phase n = [0:N-1]; x = cos(2*pi*n*f

T); % Signal to analyze X = fft(x); % SpectrumLet’s plot the time data and magnitude spectrum:

% Plot time data figure(1); subplot(3,1,1); plot(n,x,’’);

ni = [0:.1:N-1]; % Interpolated time axis hold on; plot(ni,cos(2*pi*ni*f*T),‘-’); title(‘Sinusoid Sampled at^{1}⁄_{4}the Sampling Rate’); xlabel(‘Time (samples)’); ylabel(‘Amplitude’); text(-8,1,‘a)’);% Plot spectral magnitude magX = abs(X); fn = [0:1.0/N:1-1.0/N]; % Normalized frequency axis subplot(3,1,2); stem(fn,magX) xlabel(‘Normalized Frequency (cycles per sample))’); ylabel(‘Magnitude (Linear)’); text(-.11,40,‘b)’);

% Same thing on a dB scale spec = 20*log10(magX); % Spectral magnitude in dB subplot(3,1,3); plot(fn,spec); axis([0 1 -350 50]); xlabel(‘Normalized Frequency (cycles per sample))’); ylabel(‘Magnitude (dB)’); text(-.11,50,‘c)’); print -deps eps/example1.eps; hold off;

The results are shown in Fig. 9.1. The time-domain signal is shown in Fig. 9.1a, both in pseudo-continuous and sampled form. In Fig. 9.1b, we see two peaks in the magnitude spectrum, each at magnitude on a linear scale, located at normalized frequencies and . Since the DFT length is , a spectral peak amplitude of is what we expect, since

when . This happens at bin numbers and for . However, recall that Matlab requires indexing from , so that these peaks will really show up at index and in themagXarray.The spectrum should be exactly zero at the other bin numbers. How accurately this happens can be seen by looking on a dB scale, as shown in Fig. 9.1c. We see that the spectral magnitude in the other bins is on the order of dB lower, which is close enough to zero for audio work.