ezfft |

Easy to use Power Spectrum

**ezfft**(T,U) plots the power spectrum of the signal U(T) , where T is a
'time' and U is a real signal (T can be considered as a space
coordinate as well). If T is a scalar, then it is interpreted as the
'sampling time' of the signal U. If T is a vector, then it is
interpreted as the 'time' itself. In this latter case, T must be
equally spaced (as obtained by LINSPACE for instance), and it must
have the same length as U. If T is not specified, then a 'sampling
time' of unity (1 second for instance) is taken. Windowing
(appodization) can be applied to reduce border effects (see below).
[W,E] = **ezfft**(T,U) returns the power spectrum E(W), where E is the
energy density and W the pulsation 'omega'. W is *NOT* the frequency:
the frequency is W/(2*pi). If T is considered as a space coordinate,
W is a wave number (usually noted K = 2*PI/LAMBDA, where LAMBDA is a
wavelength).
**ezfft**(..., 'Property1', 'Property2', ...) specifies the properties:
'hann' applies a Hann appodization window to the data (reduces
aliasing).
'disp' displays the spectrum (by default if no output argument)
'freq' the frequency f is displayed instead of the pulsation omega
(this applies for the display only: the output argument
remains the pulsation omega, not the frequency f).
'space' the time series is considered as a space series. This simply
renames the label 'omega' by 'k' (wave number) in the plot,
but has no influence on the computation itself.
'handle' returns a handle H instead of [W,E] - it works only if the
properties 'disp' is also specified. The handle H is useful
to change the line properties (color, thickness) of the
plot (see the example below).
The length of the vectors W and E is N/2, where N is the length of U
(this is because U is assumed to be a real signal.) If N is odd, the
last point of U and T are ignored. If U is not real, only its real part
is considered.
W(1) is always 0. E(1) is the energy density of the average of U
(when plotted in log coordinates, the first point is W(2), E(2)).
W(2) is the increment of pulsation, Delta W, given by 2*PI/Tmax
W(end), the highest measurable pulsation, is PI/DT, where DT is the
sampling time (Nyquist theorem).
Parseval Theorem (Energy conservation):
For every signal U, the 'energy' computed in the time domain and in the
frequency domain are equal,
MEAN(U.^2) == SUM(E)*W(2)
where W(2) is the pulsation increment Delta W.
Note that, depending on the situation considered, the physical 'energy'
is usually defined as 0.5*MEAN(U.^2). Energy conservation only applies
if no appodization of the signal (windowing) is used. Otherwise, some
energy is lost in the appodization, so the spectral energy is lower
than the actual one.

**Example**
simple display of a power spectrum
t = linspace(0,400,2000);
u = 0.2 + 0.7*sin(2*pi*t/47) + cos(2*pi*t/11);
**ezfft**(t,u);

**Example**
how to change the color of the plot
h = **ezfft**(t,u,'disp','handle');
set(h,'Color','red');

**Example**
how to use the output of **ezfft**
[w,e] = **ezfft**(t,u,'hann');
loglog(w,e,'b*');

**See Also**
FFT

Help file generated by makehtmldoc 1.22