IIR1 -- Realtime C++ filter library

An infinite impulse response (IIR) filter library for Linux, Mac OSX and Windows which implements Butterworth, RBJ, Chebychev filters and can easily import coefficients generated by Python (scipy).

The filter processes the data sample by sample for realtime processing.

It uses templates to allocate the required memory so that it can run without any malloc / new commands. Memory is allocated at compile time so that there is never the risk of memory leaks.

Add the following include statement to your code:

#include "Iir.h"

The general coding approach is that first the filter is instantiated specifying its order, then the parameters are set with the function setup and then it's ready to be used for sample by sample realtime filtering.

All filters are available as lowpass, highpass, bandpass and bandstop/notch filters. Butterworth / Chebyshev offer also low/high/band-shelves with specified passband gain and 0dB gain in the stopband.

See the header files in \iir or the documentation for the arguments of the setup commands.

The examples below are for lowpass filters:

1. Butterworth -- Butterworth.h Standard filter suitable for most applications. Monotonic response.

const int order = 4; // 4th order (=2 biquads)
Iir::Butterworth::LowPass<order> f;
const float samplingrate = 1000; // Hz
const float cutoff_frequency = 5; // Hz
f.setup (samplingrate, cutoff_frequency);

2. Chebyshev Type I -- ChebyshevI.h With permissible passband ripple in dB.

Iir::ChebyshevI::LowPass<order> f;
const float passband_ripple_in_db = 5;
f.setup (samplingrate,
         cutoff_frequency,
         passband_ripple_in_dB);

3. Chebyshev Type II -- ChebyshevII.h With worst permissible stopband rejection in dB.

Iir::ChebyshevII::LowPass<order> f;
double stopband_ripple_in_dB = 20;
f.setup (samplingrate,
         cutoff_frequency,
         stopband_ripple_in_dB);

4. RBJ -- RBJ.h 2nd order filters with cutoff and Q factor.

Iir::RBJ::LowPass f;
const float cutoff_frequency = 100;
const float Q_factor = 5;
f.setup (samplingrate, cutoff_frequency, Q_factor);

5. Designing filters with Python's scipy.signal -- Custom.h

########
# Python
# See "elliptic_design.py" for the complete code.
from scipy import signal
order = 4
sos = signal.ellip(order, 5, 40, 0.2, 'low', output='sos')
print(sos) # copy/paste the coefficients over & replace [] with {}

///////
// C++
// part of "iirdemo.cpp"
Iir::Custom::SOSCascade<2> cust;
const double coeff[][6] = {
		{1.665623674062209972e-02,
		 -3.924801366970616552e-03,
		 1.665623674062210319e-02,
		 1.000000000000000000e+00,
		 -1.715403014004022175e+00,
		 8.100474793174089472e-01},
		{1.000000000000000000e+00,
		 -1.369778997100624895e+00,
		 1.000000000000000222e+00,
		 1.000000000000000000e+00,
		 -1.605878925999785656e+00,
		 9.538657786383895054e-01}
	};
cust.setup(coeff);

Samples are processed one by one. In the example below a sample x is processed with the filter command and then saved in y. The types of x and y can either be float or double (integer is also allowed but is still processed internally as floating point):

y = f.filter(x);

This is then repeated for every incoming sample in a loop or event handler.

Invalid values provided to setup() will throw an exception. Parameters provided to setup() which result in coefficients being NAN will also throw an exception.

If you use cmake as your build system then just add to your CMakeLists.txt the following lines for the dynamic library:

find_package(iir)
target_link_libraries(... iir::iir)

or for the static one:

find_package(iir)
target_link_libraries(... iir::iir_static)

Link it against the dynamic library (Unix/Mac: -liir, Windows: iir.lib) or the static library (Unix/Mac: libiir_static.a, Windows: libiir_static.lib).

If you have Ubuntu xenial or bionic then install it as a pre-compiled package:

sudo add-apt-repository ppa:berndporr/usbdux

It's available for 32,64 bit PC and 32,64 bit ARM (Raspberry PI etc). The documentation and the example programs are in:

/usr/share/doc/iir1-dev/

The build tool is cmake which generates the make- or project files for the different platforms. cmake is available for Linux, Windows and Mac. It also compiles directly on a Raspberry PI.

Run

cmake .

which generates the Makefile. Then run:

make
sudo make install

which installs it under /usr/local/lib and /usr/local/include.

Both gcc and clang have been tested.

cmake -G "Visual Studio 15 2017 Win64" .

See cmake for the different build-options. Above is for a 64 bit build. Then start Visual C++ and open the solution. This will create the DLL and the LIB files. Under Windows it's highly recommended to use the static library and link it into the application program.

Run unit tests by typing make test or just ctest. These test if after a delta pulse all filters relax to zero and that their outputs never become NaN.

For an overview of the class structure and general concepts have a look at Documentation.txt.

The easiest way to learn is from the examples which are in the demo directory. A delta pulse as a test signal is sent into the different filters and saved in a file. With the Python script plot_impulse_fresponse.py you can then plot the frequency responses.

Also the directory containing the unit tests provides examples for every filter type.

A PDF of all classes, methods and in particular setup functions is in the doc/pdf directory.

Run doxygen to generate the HTML documentation.

These responses have been generated by iirdemo.cpp in the /demo/ directory and then plotted with plot_impulse_fresponse.py.

This library has been adapted from Vinnie Falco's original work which can be found here:

https://github.com/vinniefalco/DSPFilters

While his original library processes audio arrays this library has been adapted to do realtime processing sample by sample. Also, in contrast to the original library the setup command won't require the filter order and instead remembers it from the template argument.

Enjoy!

Bernd Porr -- http://www.berndporr.me.uk