Note
Click here to download the full example code or to run this example in your browser via Binder
Explore 3D images (of cells)¶
This tutorial is an introduction to threedimensional image processing. Images
are represented as numpy
arrays. A singlechannel, or grayscale, image is a
2D matrix of pixel intensities of shape (n_row, n_col)
, where n_row
(resp. n_col
) denotes the number of rows (resp. columns). We can
construct a 3D volume as a series of 2D planes, giving 3D images the shape
(n_plane, n_row, n_col)
, where n_plane
is the number of planes.
A multichannel, or RGB(A), image has an additional
channel dimension in the final position containing color information.
These conventions are summarized in the table below:
Image type 
Coordinates 

2D grayscale 

2D multichannel 

3D grayscale 

3D multichannel 

Some 3D images are constructed with equal resolution in each dimension (e.g.,
synchrotron tomography or computergenerated rendering of a sphere).
But most experimental data are captured
with a lower resolution in one of the three dimensions, e.g., photographing
thin slices to approximate a 3D structure as a stack of 2D images.
The distance between pixels in each dimension, called spacing, is encoded as a
tuple and is accepted as a parameter by some skimage
functions and can be
used to adjust contributions to filters.
The data used in this tutorial were provided by the Allen Institute for Cell Science. They were downsampled by a factor of 4 in the row and column dimensions to reduce their size and, hence, computational time. The spacing information was reported by the microscope used to image the cells.
import matplotlib.pyplot as plt
from mpl_toolkits.mplot3d.art3d import Poly3DCollection
import numpy as np
from skimage import exposure, io, util
from skimage.data import cells3d
Load and display 3D images¶
data = util.img_as_float(cells3d()[:, 1, :, :]) # grab just the nuclei
print("shape: {}".format(data.shape))
print("dtype: {}".format(data.dtype))
print("range: ({}, {})".format(data.min(), data.max()))
# Report spacing from microscope
original_spacing = np.array([0.2900000, 0.0650000, 0.0650000])
# Account for downsampling of slices by 4
rescaled_spacing = original_spacing * [1, 4, 4]
# Normalize spacing so that pixels are a distance of 1 apart
spacing = rescaled_spacing / rescaled_spacing[2]
print("microscope spacing: {}\n".format(original_spacing))
print("rescaled spacing: {} (after downsampling)\n".format(rescaled_spacing))
print("normalized spacing: {}\n".format(spacing))
Out:
shape: (60, 256, 256)
dtype: float64
range: (0.0, 1.0)
microscope spacing: [0.29 0.065 0.065]
rescaled spacing: [0.29 0.26 0.26] (after downsampling)
normalized spacing: [1.11538462 1. 1. ]
Let us try and visualize the (3D) image with io.imshow.
Out:
Invalid shape (60, 256, 256) for image data
The io.imshow function can only display grayscale and RGB(A) 2D images. We can thus use it to visualize 2D planes. By fixing one axis, we can observe three different views of the image.
def show_plane(ax, plane, cmap="gray", title=None):
ax.imshow(plane, cmap=cmap)
ax.axis("off")
if title:
ax.set_title(title)
(n_plane, n_row, n_col) = data.shape
_, (a, b, c) = plt.subplots(ncols=3, figsize=(15, 5))
show_plane(a, data[n_plane // 2], title=f'Plane = {n_plane // 2}')
show_plane(b, data[:, n_row // 2, :], title=f'Row = {n_row // 2}')
show_plane(c, data[:, :, n_col // 2], title=f'Column = {n_col // 2}')
As hinted before, a threedimensional image can be viewed as a series of twodimensional planes. Let us write a helper function, display, to display 30 planes of our data. By default, every other plane is displayed.
def display(im3d, cmap="gray", step=2):
_, axes = plt.subplots(nrows=5, ncols=6, figsize=(16, 14))
vmin = im3d.min()
vmax = im3d.max()
for ax, image in zip(axes.flatten(), im3d[::step]):
ax.imshow(image, cmap=cmap, vmin=vmin, vmax=vmax)
ax.set_xticks([])
ax.set_yticks([])
display(data)
Alternatively, we can explore these planes (slices) interactively using Jupyter widgets. Let the user select which slice to display and show the position of this slice in the 3D dataset. Note that you cannot see the Jupyter widget at work in a static HTML page, as is the case in the scikitimage gallery. For the following piece of code to work, you need a Jupyter kernel running either locally or in the cloud: see the bottom of this page to either download the Jupyter notebook and run it on your computer, or open it directly in Binder.
def slice_in_3D(ax, i):
# From https://stackoverflow.com/questions/44881885/pythondraw3dcube
Z = np.array([[0, 0, 0],
[1, 0, 0],
[1, 1, 0],
[0, 1, 0],
[0, 0, 1],
[1, 0, 1],
[1, 1, 1],
[0, 1, 1]])
Z = Z * data.shape
r = [1, 1]
X, Y = np.meshgrid(r, r)
# Plot vertices
ax.scatter3D(Z[:, 0], Z[:, 1], Z[:, 2])
# List sides' polygons of figure
verts = [[Z[0], Z[1], Z[2], Z[3]],
[Z[4], Z[5], Z[6], Z[7]],
[Z[0], Z[1], Z[5], Z[4]],
[Z[2], Z[3], Z[7], Z[6]],
[Z[1], Z[2], Z[6], Z[5]],
[Z[4], Z[7], Z[3], Z[0]],
[Z[2], Z[3], Z[7], Z[6]]]
# Plot sides
ax.add_collection3d(
Poly3DCollection(
verts,
facecolors=(0, 1, 1, 0.25),
linewidths=1,
edgecolors="darkblue"
)
)
verts = np.array([[[0, 0, 0],
[0, 0, 1],
[0, 1, 1],
[0, 1, 0]]])
verts = verts * (60, 256, 256)
verts += [i, 0, 0]
ax.add_collection3d(
Poly3DCollection(
verts,
facecolors="magenta",
linewidths=1,
edgecolors="black"
)
)
ax.set_xlabel("plane")
ax.set_xlim(0, 100)
ax.set_ylabel("row")
ax.set_zlabel("col")
# Autoscale plot axes
scaling = np.array([getattr(ax,
f'get_{dim}lim')() for dim in "xyz"])
ax.auto_scale_xyz(* [[np.min(scaling), np.max(scaling)]] * 3)
def explore_slices(data, cmap="gray"):
from ipywidgets import interact
N = len(data)
@interact(plane=(0, N  1))
def display_slice(plane=34):
fig, ax = plt.subplots(figsize=(20, 5))
ax_3D = fig.add_subplot(133, projection="3d")
show_plane(ax, data[plane], title="Plane {}".format(plane), cmap=cmap)
slice_in_3D(ax_3D, plane)
plt.show()
return display_slice
explore_slices(data);
Out:
[2K
[2K
interactive(children=(IntSlider(value=34, description='plane', max=59), Output()), _dom_classes=('widgetinteract',))
<function explore_slices.<locals>.display_slice at 0x7ff6677d1ee0>
Adjust exposure¶
Scikitimage’s exposure module contains a number of functions for adjusting image contrast. These functions operate on pixel values. Generally, image dimensionality or pixel spacing doesn’t need to be considered. In local exposure correction, though, one might want to adjust the window size to ensure equal size in real coordinates along each axis.
Gamma correction brightens or darkens an image. A powerlaw transform, where gamma denotes the powerlaw exponent, is applied to each pixel in the image: gamma < 1 will brighten an image, while gamma > 1 will darken an image.
def plot_hist(ax, data, title=None):
# Helper function for plotting histograms
ax.hist(data.ravel(), bins=256)
ax.ticklabel_format(axis="y", style="scientific", scilimits=(0, 0))
if title:
ax.set_title(title)
gamma_low_val = 0.5
gamma_low = exposure.adjust_gamma(data, gamma=gamma_low_val)
gamma_high_val = 1.5
gamma_high = exposure.adjust_gamma(data, gamma=gamma_high_val)
_, ((a, b, c), (d, e, f)) = plt.subplots(nrows=2, ncols=3, figsize=(12, 8))
show_plane(a, data[32], title='Original')
show_plane(b, gamma_low[32], title=f'Gamma = {gamma_low_val}')
show_plane(c, gamma_high[32], title=f'Gamma = {gamma_high_val}')
plot_hist(d, data)
plot_hist(e, gamma_low)
plot_hist(f, gamma_high)
Histogram equalization improves contrast in an image by redistributing pixel intensities. The most common pixel intensities get spread out, increasing contrast in lowcontrast areas. One downside of this approach is that it may enhance background noise.
equalized_data = exposure.equalize_hist(data)
display(equalized_data)
As before, if we have a Jupyter kernel running, we can explore the above slices interactively.
explore_slices(equalized_data);
Out:
[2K
[2K
interactive(children=(IntSlider(value=34, description='plane', max=59), Output()), _dom_classes=('widgetinteract',))
<function explore_slices.<locals>.display_slice at 0x7ff665faa040>
Let us now plot the image histogram before and after histogram equalization. Below, we plot the respective cumulative distribution functions (CDF).
_, ((a, b), (c, d)) = plt.subplots(nrows=2, ncols=2, figsize=(16, 8))
plot_hist(a, data, title="Original histogram")
plot_hist(b, equalized_data, title="Equalized histogram")
cdf, bins = exposure.cumulative_distribution(data.ravel())
c.plot(bins, cdf, "r")
c.set_title("Original CDF")
cdf, bins = exposure.cumulative_distribution(equalized_data.ravel())
d.plot(bins, cdf, "r")
d.set_title("Histogram equalization CDF")
Out:
Text(0.5, 1.0, 'Histogram equalization CDF')
Most experimental images are affected by salt and pepper noise. A few bright artifacts can decrease the relative intensity of the pixels of interest. A simple way to improve contrast is to clip the pixel values on the lowest and highest extremes. Clipping the darkest and brightest 0.5% of pixels will increase the overall contrast of the image.
vmin, vmax = np.percentile(data, q=(0.5, 99.5))
clipped_data = exposure.rescale_intensity(
data,
in_range=(vmin, vmax),
out_range=np.float32
)
display(clipped_data)
Total running time of the script: ( 0 minutes 10.603 seconds)