#cython: cdivision=True #cython: boundscheck=False #cython: nonecheck=False #cython: wraparound=False cimport numpy as cnp import numpy as np from libc.math cimport exp, fabs, sqrt from libc.float cimport DBL_MAX from .._shared.interpolation cimport get_pixel3d from ..util import img_as_float cdef inline double _gaussian_weight(double sigma, double value): return exp(-0.5 * (value / sigma)**2) cdef double[:] _compute_color_lut(Py_ssize_t bins, double sigma, double max_value): cdef: double[:] color_lut = np.empty(bins, dtype=np.double) Py_ssize_t b for b in range(bins): color_lut[b] = _gaussian_weight(sigma, b * max_value / bins) return color_lut cdef double[:] _compute_range_lut(Py_ssize_t win_size, double sigma): cdef: double[:] range_lut = np.empty(win_size**2, dtype=np.double) Py_ssize_t kr, kc Py_ssize_t window_ext = (win_size - 1) / 2 double dist for kr in range(win_size): for kc in range(win_size): dist = sqrt((kr - window_ext)**2 + (kc - window_ext)**2) range_lut[kr * win_size + kc] = _gaussian_weight(sigma, dist) return range_lut cdef inline Py_ssize_t Py_ssize_t_min(Py_ssize_t value1, Py_ssize_t value2): if value1 < value2: return value1 else: return value2 def _denoise_bilateral(image, Py_ssize_t win_size, sigma_range, double sigma_spatial, Py_ssize_t bins, mode, double cval): image = np.atleast_3d(img_as_float(image)) # if image.max() is 0, then dist_scale can have an unverified value # and color_lut[(dist * dist_scale)] may cause a segmentation fault # so we verify we have a positive image and that the max is not 0.0. if image.min() < 0.0: raise ValueError("Image must contain only positive values") cdef: Py_ssize_t rows = image.shape[0] Py_ssize_t cols = image.shape[1] Py_ssize_t dims = image.shape[2] Py_ssize_t window_ext = (win_size - 1) / 2 Py_ssize_t max_color_lut_bin = bins - 1 double max_value double[:, :, ::1] cimage double[:, :, ::1] out double[:] color_lut double[:] range_lut Py_ssize_t r, c, d, wr, wc, kr, kc, rr, cc, pixel_addr, color_lut_bin double value, weight, dist, total_weight, csigma_range, color_weight, \ range_weight double dist_scale double[:] values double[:] centres double[:] total_values if sigma_range is None: csigma_range = image.std() else: csigma_range = sigma_range max_value = image.max() if max_value == 0.0: raise ValueError("The maximum value found in the image was 0.") if mode not in ('constant', 'wrap', 'symmetric', 'reflect', 'edge'): raise ValueError("Invalid mode specified. Please use `constant`, " "`edge`, `wrap`, `symmetric` or `reflect`.") cdef char cmode = ord(mode[0].upper()) cimage = np.ascontiguousarray(image) out = np.zeros((rows, cols, dims), dtype=np.double) color_lut = _compute_color_lut(bins, csigma_range, max_value) range_lut = _compute_range_lut(win_size, sigma_spatial) dist_scale = bins / dims / max_value values = np.empty(dims, dtype=np.double) centres = np.empty(dims, dtype=np.double) total_values = np.empty(dims, dtype=np.double) for r in range(rows): for c in range(cols): total_weight = 0 for d in range(dims): total_values[d] = 0 centres[d] = cimage[r, c, d] for wr in range(-window_ext, window_ext + 1): rr = wr + r kr = wr + window_ext for wc in range(-window_ext, window_ext + 1): cc = wc + c kc = wc + window_ext # save pixel values for all dims and compute euclidian # distance between centre stack and current position dist = 0 for d in range(dims): value = get_pixel3d(&cimage[0, 0, 0], rows, cols, dims, rr, cc, d, cmode, cval) values[d] = value dist += (centres[d] - value)**2 dist = sqrt(dist) range_weight = range_lut[kr * win_size + kc] color_lut_bin = Py_ssize_t_min( (dist * dist_scale), max_color_lut_bin) color_weight = color_lut[color_lut_bin] weight = range_weight * color_weight for d in range(dims): total_values[d] += values[d] * weight total_weight += weight for d in range(dims): out[r, c, d] = total_values[d] / total_weight return np.squeeze(np.asarray(out)) def _denoise_tv_bregman(image, double weight, int max_iter, double eps, char isotropic): image = np.atleast_3d(img_as_float(image)) cdef: Py_ssize_t rows = image.shape[0] Py_ssize_t cols = image.shape[1] Py_ssize_t dims = image.shape[2] Py_ssize_t rows2 = rows + 2 Py_ssize_t cols2 = cols + 2 Py_ssize_t r, c, k Py_ssize_t total = rows * cols * dims shape_ext = (rows2, cols2, dims) u = np.zeros(shape_ext, dtype=np.double) cdef: double[:, :, ::1] cimage = np.ascontiguousarray(image) double[:, :, ::1] cu = u double[:, :, ::1] dx = np.zeros(shape_ext, dtype=np.double) double[:, :, ::1] dy = np.zeros(shape_ext, dtype=np.double) double[:, :, ::1] bx = np.zeros(shape_ext, dtype=np.double) double[:, :, ::1] by = np.zeros(shape_ext, dtype=np.double) double ux, uy, uprev, unew, bxx, byy, dxx, dyy, s int i = 0 double lam = 2 * weight double rmse = DBL_MAX double norm = (weight + 4 * lam) u[1:-1, 1:-1] = image # reflect image u[0, 1:-1] = image[1, :] u[1:-1, 0] = image[:, 1] u[-1, 1:-1] = image[-2, :] u[1:-1, -1] = image[:, -2] while i < max_iter and rmse > eps: rmse = 0 for k in range(dims): for r in range(1, rows + 1): for c in range(1, cols + 1): uprev = cu[r, c, k] # forward derivatives ux = cu[r, c + 1, k] - uprev uy = cu[r + 1, c, k] - uprev # Gauss-Seidel method unew = ( lam * ( + cu[r + 1, c, k] + cu[r - 1, c, k] + cu[r, c + 1, k] + cu[r, c - 1, k] + dx[r, c - 1, k] - dx[r, c, k] + dy[r - 1, c, k] - dy[r, c, k] - bx[r, c - 1, k] + bx[r, c, k] - by[r - 1, c, k] + by[r, c, k] ) + weight * cimage[r - 1, c - 1, k] ) / norm cu[r, c, k] = unew # update root mean square error rmse += (unew - uprev)**2 bxx = bx[r, c, k] byy = by[r, c, k] # d_subproblem after reference [4] if isotropic: s = sqrt((ux + bxx)**2 + (uy + byy)**2) dxx = s * lam * (ux + bxx) / (s * lam + 1) dyy = s * lam * (uy + byy) / (s * lam + 1) else: s = ux + bxx if s > 1 / lam: dxx = s - 1/lam elif s < -1 / lam: dxx = s + 1 / lam else: dxx = 0 s = uy + byy if s > 1 / lam: dyy = s - 1 / lam elif s < -1 / lam: dyy = s + 1 / lam else: dyy = 0 dx[r, c, k] = dxx dy[r, c, k] = dyy bx[r, c, k] += ux - dxx by[r, c, k] += uy - dyy rmse = sqrt(rmse / total) i += 1 return np.squeeze(np.asarray(u[1:-1, 1:-1]))