contrast-image 0.1.6

🌈 Library to work with contrast

Contrast-image

Base on multiple papers about contrast, I create this library to contrast images with opencv.

Installation

pip install contrast-image

Usage

from contrast_image import contrast_image
import cv2 as cv

input = cv.imread('input.jpg')

ci = CI(input, 'HSV')
output = ci.GHE()

API

CI

Store all functions to contrast image

from contrast_image import contrast_image

ci = CI(image, color_space = 'HSV')

GHE (Global Histogram Equalization)

This function is similar to equalizeHist(image) in opencv.

ci.GHE()

• Return: image after equalization

BBHE (Brightness Preserving Histogram Equalization)

This function separate the histogram by the mean of the image, then equalize histogram of each part.

This method tries to preserve brightness of output image by assume PDF is symmetrical distribution.

ci.BBHE()

• Return: image after equalization

DSIHE (Dualistic Sub-Image Histogram Equalization)

This function is similar to BBHE except using median instead of mean.

Unlike BBHE, DSIHE tries to preserve brightness of output image by maximum entropy after separate.

ci.DSIHE()

• Return: image after equalization

MMBEBHE (Minimum Mean Brightness Error Histogram Equalization)

This function is similar to BBHE except using minimum mean brightness error instead of mean.

Theortically, mean of output image (by GHE) is middle gray level. Therefore, MMBEBHE believe by separate histogram such that mean of output image near mean of input image must preserve brightness.

ci.MMBEBHE()

• Return: image after equalization

BPHEME (Brightness Preserving Histogram Equalization with Maximum Entropy)

This function finds matching function such that make output image maximum entropy, then using histogram specification to match input's histogram and matching function.

Based on idea of DSIHE, BPHEME tries to generalize by using histogram specification and solve optimize problem by Lagrange interpolation.

ci.BPHEME()

• Return: image after equalization

RLBHE (Range Limited Bi-Histogram Equalization)

This function is similar to BBHE except using otsu's method instead of mean. Moreover, this limit range of gray level such that output image has minimum mean brightness error.

This method tries to equalize histogram for foreground and background separately by Otsu's method.

ci.RLBHE()

• Return: image after equalization

RMSHE (Recursively Mean-Separate Histogram Equalization)

This function recursively separate histogram by mean. Therefore, recursive = 2 will create 4 sub-histograms, then equalize each sub-histograms.

Same idea as BBHE but recursively separate to preserve more brightness.

ci.RMSHE(recursive = 2)

• Parameter recurive: number of recursive time
• Return: image after equalization

RSIHE (Recursive Sub-Image Histogram Equalization)

This function is similar to RMSHE except using median instead of mean.

Same idea as DSIHE but recursively separate to preserve more brightness.

ci.RSIHE(recursive = 2)

• Parameter recurive: number of recursive time
• Return: image after equalization

RSWHE (Recursive Separated and Weighted Histogram Equalization)

This function recursively separate histogram by mean or median, then weighting each sub-histogram before equalize them.

This method similar to RMSHE and RSIHE except weighting sub-histogram to avoid local extreme value in histogram.

ci.RSWHE(type = 'mean', beta = 0, recursive = 2)

• Parameter type: 'mean' or 'median'
• Parameter beta: increasing more brightness in output image
• Parameter recurive: number of recursive time
• Return: image after equalization

FHSABP (Flattest Histogram Specification with Accurate Brightness Preservation)

This function finds matching function such that make the flattest output's histogram, then using histogram specification to match input's histogram and matching function.

Because of discrete, histogram equalization does not often the flattest histogram. FHSABP tries to solve optimization function to find the flattest output's histogram.

ci.FHSABP()

• Return: image after equalization

WTHE (Weighted Thresholded Histogram Equalization)

This function weight histogram before equalize it.

ci.WTHE(root, value, lower = 0)

• Return: image after equalization

AGCWD (Adaptive Gamma Correction with Weighting Distribution)

This function automatic correct gamma using weighting distribution

ci.AGCWD(alpha)

• Parameter alpha: adjustment
• Return: image after equalization

AGCCPF (Adaptive Gamma Correction Color Preserving Framework)

This similar to AGCWD except smooth pdf

ci.AGCCPF(alpha)

• Parameter alpha: adjustment
• Return: image after equalization

Quantitation

Store all functions to quantity output image

from contrast_image import quantitation

quantitation = Quantitation()

AMBE (Absolute Mean Brightness Error)

ci.AMBE(input_image, output_image)

PSNR (Peak Signal to Noise Ratio)

ci.PSNR(input_image, output_image)

Entropy

ci.Entropy(image)

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

Please make sure to update tests as appropriate.

License

MIT