Series, Real, Second-Order Sections
Converting the difference equation to a series bank of real first- and second-order sections is comparatively easy. In this case, we do not need a full blown partial fraction expansion. Instead, we need only factor the numerator and denominator of the transfer function into first- and/or second-order terms. Since a second-order section can accommodate up to two poles and two zeros, we must decide how to group pairs of poles with pairs of zeros. Furthermore, since the series sections can be implemented in any order, we must choose the section ordering. Both of these choices are normally driven in practice by numerical considerations. In fixed-point implementations, the poles and zeros are grouped such that dynamic range requirements are minimized. Similarly, the section order is chosen so that the intermediate signals are well scaled. For example, internal overflow is more likely if all of the large-gain sections appear before the low-gain sections. On the other hand, the signal-to-quantization-noise ratio will deteriorate if all of the low-gain sections are placed before the higher-gain sections. For further reading on numerical considerations for digital filter sections, see, e.g., [103].
Scaling:
The amplitude of the output is proportional to the amplitude of the input (the scaling property).
Superposition:
When two signals are added together and fed to the filter, the filter output is the same as if one had put each signal through the filter separately and then added the outputs (the superposition property).
While the implications of linearity are far-reaching, the mathematical definition is simple. Let us represent the general linear (but possibly time-varying) filter as a signal operator:
where is the entire input signal, is the output at time , and is the filter expressed as a real-valued function of a signal for each . Think of the subscript on as selecting the th output sample of the filter. In general, each output sample can be a function of several or even all input samples, and this is why we write as the filter input.
Definition. A filter
is said to be
linear
if for any pair of signals
and for all
constant gains , we have the following relation for each
sample time
:
where denotes the signal space (complex-valued sequences, in general). These two conditions are simply a mathematical restatement of the previous descriptive definition.
The scaling property of linear systems states that scaling the input of a linear system (multiplying it by a constant gain factor) scales the output by the same factor. The superposition property of linear systems states that the response of a linear system to a sum of signals is the sum of the responses to each individual input signal. Another view is that the individual signals which have been summed at the input are processed independently inside the filter--they superimpose and do not interact. (The addition of two signals, sample by sample, is like converting stereo to mono by mixing the two channels together equally.)
Another example of a linear signal medium is the earth's atmosphere. When two sounds are in the air at once, the air pressure fluctuations that convey them simply add (unless they are extremely loud). Since any finite continuous signal can be represented as a sum (i.e., superposition) of sinusoids, we can predict the filter response to any input signal just by knowing the response for all sinusoids. Without superposition, we have no such general description and it may be impossible to do any better than to catalog the filter output for each possible input.
Linear operators distribute over linear combinations, i.e.,
Real Linear Filtering of Complex Signals
When a filter is a linear filter (but not necessarily time-invariant), and its input is a complex signal , then, by linearity,
Appendix H presents a linear-algebraic view of linear filters that can be useful in certain applications.
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Why Dynamic Range Compression is Nonlinear
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Parallel Second-Order Signal Flow Graph