#ifndef WIENER_OP_H #define WIENER_OP_H #include #include namespace icl { /// Class for Wiener Filter \ingroup UNARY \ingroup NBH /** Wiener filters are commonly used in image processing applications to remove additive noise from degraded images, to restore a blurred image. The following operation is performed on each pixel: \f[ R(x,y,c) = \mu_m(x,y,c) + \frac{\sigma_m^2(x,y,c)-\nu^2}{\sigma^2} * (S(x,y,c) - \mu_m(x,y,c)) \f] where: - \f$R(x,y,c)\f$ is the result image at position (x,y) and channel c - \f$\mu_m(x,y,c)\f$ is the mean of the image in region m (mask) centered at (x,y), channel c - \f$\sigma^2_m(x,y,c)\f$ is the variance of the image in region m (mask) centered at (x,y), channel c - \f$\sigma^2 \f$ is the image variance - \f$S(x,y,c)\f$ is the source image at position (x,y) and channel c */ class WienerOp : public NeighborhoodOp { public: /// Constructor that creates a wiener filter object, with specified mask size /** @param maskSize of odd width and height Even width or height is increased to next higher odd value. @param noise nois factor **/ WienerOp (const Size &maskSize, icl32f noise=0): NeighborhoodOp(maskSize),m_fNoise(noise){} /// Filters an image using the Wiener algorithm. /** @param poSrc Source image @param ppoDst Destination image **/ void apply (const ImgBase *poSrc, ImgBase **ppoDst); /// Import unaryOps apply function without destination image NeighborhoodOp::apply; /// returns the current noise factor /** @return current noise factor **/ icl32f getNoise() const { return m_fNoise; } /// sets up a new noise factor /** @ param noise new noise factor **/ void setNoise(icl32f noise) { m_fNoise = noise; } private: /// internal buffer for applying the wiener operation std::vector m_vecBuffer; /// internal storage for the current noise factor icl32f m_fNoise; }; } // namespace icl #endif // WIENER_H