发现有一个博主写得比较详细了,参考着看即可。
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实验大致流程:
#!/usr/bin/env python
# -*- coding:utf-8 -*-
import cv2
import numpy as np
def zmMinFilterGray(src, r=7):
'''最小值滤波,r是滤波器半径'''
'''if r <= 0:
return src
h, w = src.shape[:2]
I = src
res = np.minimum(I , I[[0]+range(h-1) , :])
res = np.minimum(res, I[range(1,h)+[h-1], :])
I = res
res = np.minimum(I , I[:, [0]+range(w-1)])
res = np.minimum(res, I[:, range(1,w)+[w-1]])
return zmMinFilterGray(res, r-1)'''
return cv2.erode(src, np.ones((2 * r + 1, 2 * r + 1))) # 使用opencv的erode函数更高效
def guidedfilter(I, p, r, eps):
'''引导滤波,直接参考网上的matlab代码'''
height, width = I.shape
m_I = cv2.boxFilter(I, -1, (r, r))
m_p = cv2.boxFilter(p, -1, (r, r))
m_Ip = cv2.boxFilter(I * p, -1, (r, r))
cov_Ip = m_Ip - m_I * m_p
m_II = cv2.boxFilter(I * I, -1, (r, r))
var_I = m_II - m_I * m_I
a = cov_Ip / (var_I + eps)
b = m_p - a * m_I
m_a = cv2.boxFilter(a, -1, (r, r))
m_b = cv2.boxFilter(b, -1, (r, r))
return m_a * I + m_b
def getV1(m, r, eps, w, maxV1): # 输入rgb图像,值范围[0,1]
'''计算大气遮罩图像V1和光照值A, V1 = (1-t)A'''
V1 = np.min(m, 2) # 得到暗通道图像
V1 = guidedfilter(V1, zmMinFilterGray(V1, 7), r, eps) # 使用引导滤波优化
bins = 2000
ht = np.histogram(V1, bins) # 计算大气光照A
d = np.cumsum(ht[0]) / float(V1.size)
for lmax in range(bins - 1, 0, -1):
if d[lmax] <= 0.999:
break
A = np.mean(m, 2)[V1 >= ht[1][lmax]].max()
V1 = np.minimum(V1 * w, maxV1) # 对值范围进行限制
return V1, A
def deHaze(m, r=81, eps=0.001, w=0.95, maxV1=0.80, bGamma=False):
Y = np.zeros(m.shape)
V1, A = getV1(m, r, eps, w, maxV1) # 得到遮罩图像和大气光照
for k in range(3):
Y[:, :, k] = (m[:, :, k] - V1) / (1 - V1 / A) # 颜色校正
Y = np.clip(Y, 0, 1)
if bGamma:
Y = Y ** (np.log(0.5) / np.log(Y.mean())) # gamma校正,默认不进行该操作
return Y
if __name__ == '__main__':
m = deHaze(cv2.imread('land.jpg') / 255.0) * 255
cv2.imwrite('defog.jpg', m)