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Let us look at a basic continuous-time convolution example to help express some of the important ideas. We will convolve together two square pulses, and , as shown in
Now we will take one of the functions and reflect it around
the y-axis. Then we must shift the function, such that theorigin, the point of the function that was originally on the
origin, is labeled as point
. This
step is shown in
,
.
We start out with the convolution integral, . The value of the function at time is given by the amount of overlap(to be precise the integral of theoverlapping region) between and .
Next, we want to look at the functions and divide the span
of the functions into different limits of integration.These different regions can be understood by thinking about
how we slide
over
, see
.
Finally we are ready for a little math. Using the convolution integral, let us integrate the product of . For our first and fourth region this will be trivial as it will always be . The second region, , will require the following math:
Note that the value of at all time is given by the integral of the overlapping functions. In this example for a given equals the gray area in the plots in .
Thus, we have the following results for our four regions:
By looking at we can obtain the system output, , by "common" sense.For there is no overlap, so is 0. As goes from 0 to 1 the overlap will linearly increase with a maximum for , the maximum corresponds to the peak value in the triangular pulse.As goes from 1 to 2 the overlap will linearly decrease. For there will be no overlap and hence no output.
We see readily from the "common" sense approach that the output function is the same as obtained above with calculations. When convolving to squarepulses the result will always be a triangular pulse. Its origin, peak value and strech will, of course, vary.
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