Windows for spectral analysis.
These are generally double-precision, because they are mostly calculated during setup/reconfiguring, not real-time code.
Files | |
file | windows.h |
Classes | |
class | signalsmith::windows::Kaiser |
The Kaiser window (almost) maximises the energy in the main-lobe compared to the side-lobes. More... | |
class | signalsmith::windows::ApproximateConfinedGaussian |
The Approximate Confined Gaussian window is (almost) optimal. More... | |
Functions | |
template<typename Data > | |
void | signalsmith::windows::forcePerfectReconstruction (Data &&data, int windowLength, int interval) |
Forces STFT perfect-reconstruction (WOLA) on an existing window, for a given STFT interval. More... | |
void signalsmith::windows::forcePerfectReconstruction | ( | Data && | data, |
int | windowLength, | ||
int | interval | ||
) |
Forces STFT perfect-reconstruction (WOLA) on an existing window, for a given STFT interval.
For example, here are perfect-reconstruction versions of the approximately-optimal Kaiser windows: