Module: exposure  
skimage.exposure.adjust_gamma(image[, …]) Performs Gamma Correction on the input image.  
skimage.exposure.adjust_log(image[, gain, inv]) Performs Logarithmic correction on the input image.  
skimage.exposure.adjust_sigmoid(image[, …]) Performs Sigmoid Correction on the input image.  
skimage.exposure.cumulative_distribution(image) Return cumulative distribution function (cdf) for the given image.  
skimage.exposure.equalize_adapthist(image[, …]) Contrast Limited Adaptive Histogram Equalization (CLAHE).  
skimage.exposure.equalize_hist(image[, …]) Return image after histogram equalization.  
skimage.exposure.histogram(image[, nbins, …]) Return histogram of image.  
skimage.exposure.is_low_contrast(image[, …]) Determine if an image is low contrast.  
skimage.exposure.match_histograms(image, …) Adjust an image so that its cumulative histogram matches that of another.  
skimage.exposure.rescale_intensity(image[, …]) Return image after stretching or shrinking its intensity levels.   adjust_gamma  
skimage.exposure.adjust_gamma(image, gamma=1, gain=1) [source]
 
Performs Gamma Correction on the input image. Also known as Power Law Transform. This function transforms the input image pixelwise according to the equation O = I**gamma after scaling each pixel to the range 0 to 1.  Parameters 
 
imagendarray 

Input image.  
gammafloat, optional 

Non negative real number. Default value is 1.  
gainfloat, optional 

The constant multiplier. Default value is 1.    Returns 
 
outndarray 

Gamma corrected output image.      See also  
adjust_log

  Notes For gamma greater than 1, the histogram will shift towards left and the output image will be darker than the input image. For gamma less than 1, the histogram will shift towards right and the output image will be brighter than the input image. References  
1  
https://en.wikipedia.org/wiki/Gamma_correction   Examples >>> from skimage import data, exposure, img_as_float
>>> image = img_as_float(data.moon())
>>> gamma_corrected = exposure.adjust_gamma(image, 2)
>>> # Output is darker for gamma > 1
>>> image.mean() > gamma_corrected.mean()
True
 
 Examples using skimage.exposure.adjust_gamma
 
  Explore 3D images (of cells)   adjust_log  
skimage.exposure.adjust_log(image, gain=1, inv=False) [source]
 
Performs Logarithmic correction on the input image. This function transforms the input image pixelwise according to the equation O = gain*log(1 + I) after scaling each pixel to the range 0 to 1. For inverse logarithmic correction, the equation is O = gain*(2**I - 1).  Parameters 
 
imagendarray 

Input image.  
gainfloat, optional 

The constant multiplier. Default value is 1.  
invfloat, optional 

If True, it performs inverse logarithmic correction, else correction will be logarithmic. Defaults to False.    Returns 
 
outndarray 

Logarithm corrected output image.      See also  
adjust_gamma

  References  
1  
http://www.ece.ucsb.edu/Faculty/Manjunath/courses/ece178W03/EnhancePart1.pdf   
 adjust_sigmoid  
skimage.exposure.adjust_sigmoid(image, cutoff=0.5, gain=10, inv=False) [source]
 
Performs Sigmoid Correction on the input image. Also known as Contrast Adjustment. This function transforms the input image pixelwise according to the equation O = 1/(1 + exp*(gain*(cutoff - I))) after scaling each pixel to the range 0 to 1.  Parameters 
 
imagendarray 

Input image.  
cutofffloat, optional 

Cutoff of the sigmoid function that shifts the characteristic curve in horizontal direction. Default value is 0.5.  
gainfloat, optional 

The constant multiplier in exponential’s power of sigmoid function. Default value is 10.  
invbool, optional 

If True, returns the negative sigmoid correction. Defaults to False.    Returns 
 
outndarray 

Sigmoid corrected output image.      See also  
adjust_gamma

  References  
1  
Gustav J. Braun, “Image Lightness Rescaling Using Sigmoidal Contrast Enhancement Functions”, http://www.cis.rit.edu/fairchild/PDFs/PAP07.pdf   
 cumulative_distribution  
skimage.exposure.cumulative_distribution(image, nbins=256) [source]
 
Return cumulative distribution function (cdf) for the given image.  Parameters 
 
imagearray 

Image array.  
nbinsint, optional 

Number of bins for image histogram.    Returns 
 
img_cdfarray 

Values of cumulative distribution function.  
bin_centersarray 

Centers of bins.      See also  
histogram

  References  
1  
https://en.wikipedia.org/wiki/Cumulative_distribution_function   Examples >>> from skimage import data, exposure, img_as_float
>>> image = img_as_float(data.camera())
>>> hi = exposure.histogram(image)
>>> cdf = exposure.cumulative_distribution(image)
>>> np.alltrue(cdf[0] == np.cumsum(hi[0])/float(image.size))
True
 
 Examples using skimage.exposure.cumulative_distribution
 
  Local Histogram Equalization  

  Explore 3D images (of cells)   equalize_adapthist  
skimage.exposure.equalize_adapthist(image, kernel_size=None, clip_limit=0.01, nbins=256) [source]
 
Contrast Limited Adaptive Histogram Equalization (CLAHE). An algorithm for local contrast enhancement, that uses histograms computed over different tile regions of the image. Local details can therefore be enhanced even in regions that are darker or lighter than most of the image.  Parameters 
 
image(N1, …,NN[, C]) ndarray 

Input image.  kernel_size: int or array_like, optional

Defines the shape of contextual regions used in the algorithm. If iterable is passed, it must have the same number of elements as image.ndim (without color channel). If integer, it is broadcasted to each image dimension. By default, kernel_size is 1/8 of image height by 1/8 of its width.  
clip_limitfloat, optional 

Clipping limit, normalized between 0 and 1 (higher values give more contrast).  
nbinsint, optional 

Number of gray bins for histogram (“data range”).    Returns 
 
out(N1, …,NN[, C]) ndarray 

Equalized image with float64 dtype.      See also  
equalize_hist, rescale_intensity

  Notes  
 For color images, the following steps are performed:

 The image is converted to HSV color space The CLAHE algorithm is run on the V (Value) channel The image is converted back to RGB space and returned     For RGBA images, the original alpha channel is removed.   Changed in version 0.17: The values returned by this function are slightly shifted upwards because of an internal change in rounding behavior.  References  
1  
http://tog.acm.org/resources/GraphicsGems/  
2  
https://en.wikipedia.org/wiki/CLAHE#CLAHE   
 Examples using skimage.exposure.equalize_adapthist
 
  3D adaptive histogram equalization   equalize_hist  
skimage.exposure.equalize_hist(image, nbins=256, mask=None) [source]
 
Return image after histogram equalization.  Parameters 
 
imagearray 

Image array.  
nbinsint, optional 

Number of bins for image histogram. Note: this argument is ignored for integer images, for which each integer is its own bin.  mask: ndarray of bools or 0s and 1s, optional

Array of same shape as image. Only points at which mask == True are used for the equalization, which is applied to the whole image.    Returns 
 
outfloat array 

Image array after histogram equalization.     Notes This function is adapted from [1] with the author’s permission. References  
1  
http://www.janeriksolem.net/histogram-equalization-with-python-and.html  
2  
https://en.wikipedia.org/wiki/Histogram_equalization   
 Examples using skimage.exposure.equalize_hist
 
  Local Histogram Equalization  

  3D adaptive histogram equalization  

  Explore 3D images (of cells)  

  Rank filters   histogram  
skimage.exposure.histogram(image, nbins=256, source_range='image', normalize=False) [source]
 
Return histogram of image. Unlike numpy.histogram, this function returns the centers of bins and does not rebin integer arrays. For integer arrays, each integer value has its own bin, which improves speed and intensity-resolution. The histogram is computed on the flattened image: for color images, the function should be used separately on each channel to obtain a histogram for each color channel.  Parameters 
 
imagearray 

Input image.  
nbinsint, optional 

Number of bins used to calculate histogram. This value is ignored for integer arrays.  
source_rangestring, optional 

‘image’ (default) determines the range from the input image. ‘dtype’ determines the range from the expected range of the images of that data type.  
normalizebool, optional 

If True, normalize the histogram by the sum of its values.    Returns 
 
histarray 

The values of the histogram.  
bin_centersarray 

The values at the center of the bins.      See also  
cumulative_distribution

  Examples >>> from skimage import data, exposure, img_as_float
>>> image = img_as_float(data.camera())
>>> np.histogram(image, bins=2)
(array([ 93585, 168559]), array([0. , 0.5, 1. ]))
>>> exposure.histogram(image, nbins=2)
(array([ 93585, 168559]), array([0.25, 0.75]))
 
 Examples using skimage.exposure.histogram
 
  Rank filters   is_low_contrast  
skimage.exposure.is_low_contrast(image, fraction_threshold=0.05, lower_percentile=1, upper_percentile=99, method='linear') [source]
 
Determine if an image is low contrast.  Parameters 
 
imagearray-like 

The image under test.  
fraction_thresholdfloat, optional 

The low contrast fraction threshold. An image is considered low- contrast when its range of brightness spans less than this fraction of its data type’s full range. [1]  
lower_percentilefloat, optional 

Disregard values below this percentile when computing image contrast.  
upper_percentilefloat, optional 

Disregard values above this percentile when computing image contrast.  
methodstr, optional 

The contrast determination method. Right now the only available option is “linear”.    Returns 
 
outbool 

True when the image is determined to be low contrast.     References  
1  
https://scikit-image.org/docs/dev/user_guide/data_types.html   Examples >>> image = np.linspace(0, 0.04, 100)
>>> is_low_contrast(image)
True
>>> image[-1] = 1
>>> is_low_contrast(image)
True
>>> is_low_contrast(image, upper_percentile=100)
False
 
 match_histograms  
skimage.exposure.match_histograms(image, reference, *, multichannel=False) [source]
 
Adjust an image so that its cumulative histogram matches that of another. The adjustment is applied separately for each channel.  Parameters 
 
imagendarray 

Input image. Can be gray-scale or in color.  
referencendarray 

Image to match histogram of. Must have the same number of channels as image.  
multichannelbool, optional 

Apply the matching separately for each channel.    Returns 
 
matchedndarray 

Transformed input image.    Raises 
 ValueError

Thrown when the number of channels in the input image and the reference differ.     References  
1  
http://paulbourke.net/miscellaneous/equalisation/   
 rescale_intensity  
skimage.exposure.rescale_intensity(image, in_range='image', out_range='dtype') [source]
 
Return image after stretching or shrinking its intensity levels. The desired intensity range of the input and output, in_range and out_range respectively, are used to stretch or shrink the intensity range of the input image. See examples below.  Parameters 
 
imagearray 

Image array.  
in_range, out_rangestr or 2-tuple, optional 

Min and max intensity values of input and output image. The possible values for this parameter are enumerated below.  ‘image’

Use image min/max as the intensity range.  ‘dtype’

Use min/max of the image’s dtype as the intensity range.  dtype-name

Use intensity range based on desired dtype. Must be valid key in DTYPE_RANGE.  2-tuple

Use range_values as explicit min/max intensities.      Returns 
 
outarray 

Image array after rescaling its intensity. This image is the same dtype as the input image.      See also  
equalize_hist

  Notes  Changed in version 0.17: The dtype of the output array has changed to match the output dtype, or float if the output range is specified by a pair of floats.  Examples By default, the min/max intensities of the input image are stretched to the limits allowed by the image’s dtype, since in_range defaults to ‘image’ and out_range defaults to ‘dtype’: >>> image = np.array([51, 102, 153], dtype=np.uint8)
>>> rescale_intensity(image)
array([  0, 127, 255], dtype=uint8)
 It’s easy to accidentally convert an image dtype from uint8 to float: >>> 1.0 * image
array([ 51., 102., 153.])
 Use rescale_intensity to rescale to the proper range for float dtypes: >>> image_float = 1.0 * image
>>> rescale_intensity(image_float)
array([0. , 0.5, 1. ])
 To maintain the low contrast of the original, use the in_range parameter: >>> rescale_intensity(image_float, in_range=(0, 255))
array([0.2, 0.4, 0.6])
 If the min/max value of in_range is more/less than the min/max image intensity, then the intensity levels are clipped: >>> rescale_intensity(image_float, in_range=(0, 102))
array([0.5, 1. , 1. ])
 If you have an image with signed integers but want to rescale the image to just the positive range, use the out_range parameter. In that case, the output dtype will be float: >>> image = np.array([-10, 0, 10], dtype=np.int8)
>>> rescale_intensity(image, out_range=(0, 127))
array([  0. ,  63.5, 127. ])
 To get the desired range with a specific dtype, use .astype(): >>> rescale_intensity(image, out_range=(0, 127)).astype(np.int8)
array([  0,  63, 127], dtype=int8)
 If the input image is constant, the output will be clipped directly to the output range: >>> image = np.array([130, 130, 130], dtype=np.int32) >>> rescale_intensity(image, out_range=(0, 127)).astype(np.int32) array([127, 127, 127], dtype=int32) 
 Examples using skimage.exposure.rescale_intensity
 
  Phase Unwrapping  

  Explore 3D images (of cells)  

  Rank filters