Source code for medpy.filter.image

# Copyright (C) 2013 Oskar Maier
# 
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# 
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
# GNU General Public License for more details.
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# You should have received a copy of the GNU General Public License
# along with this program.  If not, see <http://www.gnu.org/licenses/>.
#
# author Oskar Maier
# version r0.3.0
# since 2013-11-29
# status Release

# build-in modules
import itertools
import numbers
import math

# third-party modules
import numpy
from scipy.ndimage.filters import convolve, gaussian_filter, minimum_filter
from scipy.ndimage._ni_support import _get_output
from scipy.ndimage.interpolation import zoom

# own modules
from .utilities import pad, __make_footprint
from ..io import header

# code
[docs]def sls(minuend, subtrahend, metric = "ssd", noise = "global", signed = True, sn_size = None, sn_footprint = None, sn_mode = "reflect", sn_cval = 0.0, pn_size = None, pn_footprint = None, pn_mode = "reflect", pn_cval = 0.0): r""" Computes the signed local similarity between two images. Compares a patch around each voxel of the minuend array to a number of patches centered at the points of a search neighbourhood in the subtrahend. Thus, creates a multi-dimensional measure of patch similarity between the minuend and a corresponding search area in the subtrahend. This filter can also be used to compute local self-similarity, obtaining a descriptor similar to the one described in [1]_. Parameters ---------- minuend : array_like Input array from which to subtract the subtrahend. subtrahend : array_like Input array to subtract from the minuend. metric : {'ssd', 'mi', 'nmi', 'ncc'}, optional The `metric` parameter determines the metric used to compute the filter output. Default is 'ssd'. noise : {'global', 'local'}, optional The `noise` parameter determines how the noise is handled. If set to 'global', the variance determining the noise is a scalar, if set to 'local', it is a Gaussian smoothed field of estimated local noise. Default is 'global'. signed : bool, optional Whether the filter output should be signed or not. If set to 'False', only the absolute values will be returned. Default is 'True'. sn_size : scalar or tuple, optional See sn_footprint, below sn_footprint : array, optional The search neighbourhood. Either `sn_size` or `sn_footprint` must be defined. `sn_size` gives the shape that is taken from the input array, at every element position, to define the input to the filter function. `sn_footprint` is a boolean array that specifies (implicitly) a shape, but also which of the elements within this shape will get passed to the filter function. Thus ``sn_size=(n,m)`` is equivalent to ``sn_footprint=np.ones((n,m))``. We adjust `sn_size` to the number of dimensions of the input array, so that, if the input array is shape (10,10,10), and `sn_size` is 2, then the actual size used is (2,2,2). sn_mode : {'reflect', 'constant', 'nearest', 'mirror', 'wrap'}, optional The `sn_mode` parameter determines how the array borders are handled, where `sn_cval` is the value when mode is equal to 'constant'. Default is 'reflect' sn_cval : scalar, optional Value to fill past edges of input if `sn_mode` is 'constant'. Default is 0.0 pn_size : scalar or tuple, optional See pn_footprint, below pn_footprint : array, optional The patch over which the distance measure is applied. Either `pn_size` or `pn_footprint` must be defined. `pn_size` gives the shape that is taken from the input array, at every element position, to define the input to the filter function. `pn_footprint` is a boolean array that specifies (implicitly) a shape, but also which of the elements within this shape will get passed to the filter function. Thus ``pn_size=(n,m)`` is equivalent of dimensions of the input array, so that, if the input array is shape (10,10,10), and `pn_size` is 2, then the actual size used is (2,2,2). pn_mode : {'reflect', 'constant', 'nearest', 'mirror', 'wrap'}, optional The `pn_mode` parameter determines how the array borders are handled, where `pn_cval` is the value when mode is equal to 'constant'. Default is 'reflect' pn_cval : scalar, optional Value to fill past edges of input if `pn_mode` is 'constant'. Default is 0.0 Returns ------- sls : ndarray The signed local similarity image between subtrahend and minuend. References ---------- .. [1] Mattias P. Heinrich, Mark Jenkinson, Manav Bhushan, Tahreema Matin, Fergus V. Gleeson, Sir Michael Brady, Julia A. Schnabel MIND: Modality independent neighbourhood descriptor for multi-modal deformable registration Medical Image Analysis, Volume 16, Issue 7, October 2012, Pages 1423-1435, ISSN 1361-8415 http://dx.doi.org/10.1016/j.media.2012.05.008 """ minuend = numpy.asarray(minuend) subtrahend = numpy.asarray(subtrahend) if numpy.iscomplexobj(minuend): raise TypeError('complex type not supported') if numpy.iscomplexobj(subtrahend): raise TypeError('complex type not supported') mshape = [ii for ii in minuend.shape if ii > 0] sshape = [ii for ii in subtrahend.shape if ii > 0] if not len(mshape) == len(sshape): raise RuntimeError("minuend and subtrahend must be of same shape") if not numpy.all([sm == ss for sm, ss in zip(mshape, sshape)]): raise RuntimeError("minuend and subtrahend must be of same shape") sn_footprint = __make_footprint(minuend, sn_size, sn_footprint) sn_fshape = [ii for ii in sn_footprint.shape if ii > 0] if len(sn_fshape) != minuend.ndim: raise RuntimeError('search neighbourhood footprint array has incorrect shape.') #!TODO: Is this required? if not sn_footprint.flags.contiguous: sn_footprint = sn_footprint.copy() # created a padded copy of the subtrahend, whereas the padding mode is always 'reflect' subtrahend = pad(subtrahend, footprint=sn_footprint, mode=sn_mode, cval=sn_cval) # compute slicers for position where the search neighbourhood sn_footprint is TRUE slicers = [[slice(x, (x + 1) - d if 0 != (x + 1) - d else None) for x in range(d)] for d in sn_fshape] slicers = [sl for sl, tv in zip(itertools.product(*slicers), sn_footprint.flat) if tv] # compute difference images and sign images for search neighbourhood elements ssds = [ssd(minuend, subtrahend[slicer], normalized=True, signed=signed, size=pn_size, footprint=pn_footprint, mode=pn_mode, cval=pn_cval) for slicer in slicers] distance = [x[0] for x in ssds] distance_sign = [x[1] for x in ssds] # compute local variance, which constitutes an approximation of local noise, out of patch-distances over the neighbourhood structure variance = numpy.average(distance, 0) variance = gaussian_filter(variance, sigma=3) #!TODO: Figure out if a fixed sigma is desirable here... I think that yes if 'global' == noise: variance = variance.sum() / float(numpy.product(variance.shape)) # variance[variance < variance_global / 10.] = variance_global / 10. #!TODO: Should I keep this i.e. regularizing the variance to be at least 10% of the global one? # compute sls sls = [dist_sign * numpy.exp(-1 * (dist / variance)) for dist_sign, dist in zip(distance_sign, distance)] # convert into sls image, swapping dimensions to have varying patches in the last dimension return numpy.rollaxis(numpy.asarray(sls), 0, minuend.ndim + 1)
[docs]def ssd(minuend, subtrahend, normalized=True, signed=False, size=None, footprint=None, mode="reflect", cval=0.0, origin=0): r""" Computes the sum of squared difference (SSD) between patches of minuend and subtrahend. Parameters ---------- minuend : array_like Input array from which to subtract the subtrahend. subtrahend : array_like Input array to subtract from the minuend. normalized : bool, optional Whether the SSD of each patch should be divided through the filter size for normalization. Default is 'True'. signed : bool, optional Whether the accumulative sign of each patch should be returned as well. If 'True', the second return value is a numpy.sign array, otherwise the scalar '1'. Default is 'False'. size : scalar or tuple, optional See footprint, below footprint : array, optional The patch over which to compute the SSD. Either `size` or `footprint` must be defined. `size` gives the shape that is taken from the input array, at every element position, to define the input to the filter function. `footprint` is a boolean array that specifies (implicitly) a shape, but also which of the elements within this shape will get passed to the filter function. Thus ``size=(n,m)`` is equivalent to ``footprint=np.ones((n,m))``. We adjust `size` to the number of dimensions of the input array, so that, if the input array is shape (10,10,10), and `size` is 2, then the actual size used is (2,2,2). mode : {'reflect', 'constant', 'nearest', 'mirror', 'wrap'}, optional The `mode` parameter determines how the array borders are handled, where `cval` is the value when mode is equal to 'constant'. Default is 'reflect' cval : scalar, optional Value to fill past edges of input if `mode` is 'constant'. Default is 0.0 Returns ------- ssd : ndarray The patchwise sum of squared differences between minuend and subtrahend. """ convolution_filter = average_filter if normalized else sum_filter output = numpy.float if normalized else minuend.dtype if signed: difference = minuend - subtrahend difference_squared = numpy.square(difference) distance_sign = numpy.sign(convolution_filter(numpy.sign(difference) * difference_squared, size=size, footprint=footprint, mode=mode, cval=cval, origin=origin, output=output)) distance = convolution_filter(difference_squared, size=size, footprint=footprint, mode=mode, cval=cval, output=output) else: distance = convolution_filter(numpy.square(minuend - subtrahend), size=size, footprint=footprint, mode=mode, cval=cval, origin=origin, output=output) distance_sign = 1 return distance, distance_sign
[docs]def average_filter(input, size=None, footprint=None, output=None, mode="reflect", cval=0.0, origin=0): r""" Calculates a multi-dimensional average filter. Parameters ---------- input : array-like input array to filter size : scalar or tuple, optional See footprint, below footprint : array, optional Either `size` or `footprint` must be defined. `size` gives the shape that is taken from the input array, at every element position, to define the input to the filter function. `footprint` is a boolean array that specifies (implicitly) a shape, but also which of the elements within this shape will get passed to the filter function. Thus ``size=(n,m)`` is equivalent to ``footprint=np.ones((n,m))``. We adjust `size` to the number of dimensions of the input array, so that, if the input array is shape (10,10,10), and `size` is 2, then the actual size used is (2,2,2). output : array, optional The ``output`` parameter passes an array in which to store the filter output. mode : {'reflect','constant','nearest','mirror', 'wrap'}, optional The ``mode`` parameter determines how the array borders are handled, where ``cval`` is the value when mode is equal to 'constant'. Default is 'reflect' cval : scalar, optional Value to fill past edges of input if ``mode`` is 'constant'. Default is 0.0 origin : scalar, optional The ``origin`` parameter controls the placement of the filter. Default 0 Returns ------- average_filter : ndarray Returned array of same shape as `input`. Notes ----- Convenience implementation employing convolve. See Also -------- scipy.ndimage.filters.convolve : Convolve an image with a kernel. """ footprint = __make_footprint(input, size, footprint) filter_size = footprint.sum() output = _get_output(output, input) sum_filter(input, footprint=footprint, output=output, mode=mode, cval=cval, origin=origin) output /= filter_size return output
[docs]def sum_filter(input, size=None, footprint=None, output=None, mode="reflect", cval=0.0, origin=0): r""" Calculates a multi-dimensional sum filter. Parameters ---------- input : array-like input array to filter size : scalar or tuple, optional See footprint, below footprint : array, optional Either `size` or `footprint` must be defined. `size` gives the shape that is taken from the input array, at every element position, to define the input to the filter function. `footprint` is a boolean array that specifies (implicitly) a shape, but also which of the elements within this shape will get passed to the filter function. Thus ``size=(n,m)`` is equivalent to ``footprint=np.ones((n,m))``. We adjust `size` to the number of dimensions of the input array, so that, if the input array is shape (10,10,10), and `size` is 2, then the actual size used is (2,2,2). output : array, optional The ``output`` parameter passes an array in which to store the filter output. mode : {'reflect','constant','nearest','mirror', 'wrap'}, optional The ``mode`` parameter determines how the array borders are handled, where ``cval`` is the value when mode is equal to 'constant'. Default is 'reflect' cval : scalar, optional Value to fill past edges of input if ``mode`` is 'constant'. Default is 0.0 origin : scalar, optional The ``origin`` parameter controls the placement of the filter. Default 0 Returns ------- sum_filter : ndarray Returned array of same shape as `input`. Notes ----- Convenience implementation employing convolve. See Also -------- scipy.ndimage.filters.convolve : Convolve an image with a kernel. """ footprint = __make_footprint(input, size, footprint) slicer = [slice(None, None, -1)] * footprint.ndim return convolve(input, footprint[slicer], output, mode, cval, origin)
[docs]def otsu (img, bins=64): r""" Otsu's method to find the optimal threshold separating an image into fore- and background. This rather expensive method iterates over a number of thresholds to separate the images histogram into two parts with a minimal intra-class variance. An increase in the number of bins increases the algorithms specificity at the cost of slowing it down. Parameters ---------- img : array_like The image for which to determine the threshold. bins : integer The number of histogram bins. Returns ------- otsu : float The otsu threshold to separate the input image into fore- and background. """ # cast bins parameter to int bins = int(bins) # cast img parameter to scipy arrax img = numpy.asarray(img) # check supplied parameters if bins <= 1: raise AttributeError('At least a number two bins have to be provided.') # determine initial threshold and threshold step-length steplength = (img.max() - img.min()) / float(bins) initial_threshold = img.min() + steplength # initialize best value variables best_bcv = 0 best_threshold = initial_threshold # iterate over the thresholds and find highest between class variance for threshold in numpy.arange(initial_threshold, img.max(), steplength): mask_fg = (img >= threshold) mask_bg = (img < threshold) wfg = numpy.count_nonzero(mask_fg) wbg = numpy.count_nonzero(mask_bg) if 0 == wfg or 0 == wbg: continue mfg = img[mask_fg].mean() mbg = img[mask_bg].mean() bcv = wfg * wbg * math.pow(mbg - mfg, 2) if bcv > best_bcv: best_bcv = bcv best_threshold = threshold return best_threshold
[docs]def local_minima(img, min_distance = 4): r""" Returns all local minima from an image. Parameters ---------- img : array_like The image. min_distance : integer The minimal distance between the minimas in voxels. If it is less, only the lower minima is returned. Returns ------- indices : sequence List of all minima indices. values : sequence List of all minima values. """ # @TODO: Write a unittest for this. fits = numpy.asarray(img) minfits = minimum_filter(fits, size=min_distance) # default mode is reflect minima_mask = fits == minfits good_indices = numpy.transpose(minima_mask.nonzero()) good_fits = fits[minima_mask] order = good_fits.argsort() return good_indices[order], good_fits[order]
[docs]def resample(img, hdr, target_spacing, bspline_order=3, mode='constant'): """ Re-sample an image to a new voxel-spacing. Parameters ---------- img : array_like The image. hdr : object The image header. target_spacing : number or sequence of numbers The target voxel spacing to achieve. If a single number, isotropic spacing is assumed. bspline_order : int The bspline order used for interpolation. mode : str Points outside the boundaries of the input are filled according to the given mode ('constant', 'nearest', 'reflect' or 'wrap'). Default is 'constant'. Warning ------- Voxel-spacing of input header will be modified in-place! Returns ------- img : ndarray The re-sampled image. hdr : object The image header with the new voxel spacing. """ if isinstance(target_spacing, numbers.Number): target_spacing = [target_spacing] * img.ndim # compute zoom values zoom_factors = [old / float(new) for new, old in zip(target_spacing, header.get_pixel_spacing(hdr))] # zoom image img = zoom(img, zoom_factors, order=bspline_order, mode=mode) # set new voxel spacing header.set_pixel_spacing(hdr, target_spacing) return img, hdr