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In the theory of Taylor series we investigate the approximation of general functions by polynomials. Now we want to consider the approximation of general 2*pi-periodic functions by functions A of the form
By analogy with the Taylor approximation theory, these functions are called trigonometric polynomials.
In this part we concentrate on the trigonometric polynomials themselves. Suppose we "know" the polynomial -- in the sense that we have a list of values for the polynomial for a range of values of t. How can we find the coefficients a0, a1, b1, ... ? Our approach will be to calculate (numerically) various integrals involving the function. In Part 3 of this module you established the following:
for any integer n, | ||
for n a nonzero integer, | ||
for all integers m and n, | ||
for all integers m and n with m not equal to n, | ||
for all nonzero integers m and n. |
So suppose we know that a trigonometric polynomial A is of the form
For simplicity, we will start by assuming that A has period 2*pi, that is w = 1. We will also assume that A can be written as a combination of just the first two harmonics, that is,
You will need the following information about C:
Once you have determined the coefficients, use them to define a trigonometric polynomial and compare its graph to that of C.
3. Write general formulas for finding the values of a0, and ak and bk for k greater than or equal to 1.
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modules at math.duke.edu | Copyright CCP and the author(s), 1998 |