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c++ - 图像处理 : luminance weighted 2

转载 作者:行者123 更新时间:2023-11-28 05:50:45 24 4
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我想权衡新图像的亮度值。我有一张 5 像素的图像 (5px.jpg),亮度为:50,100,150,200,250。

我有一个系数 vector 。

我创建了一个新的 Mat Z,它结合了 5px.jpg 的亮度和系数。

因此,我的第一个亮度值是 50 (lum[0]=50),我希望它应用于矩阵的第一个像素 5.1 (coef[0]=5.1)。为此,我需要用第一个和第二个亮度值对第 6 个像素进行加权。在我的例子中,我的第 6 个像素的亮度将为 95,因为 (0.1*50)+(0.9*100)=95

等等……

但我不知道为什么我的代码不起作用。

我已经针对 vector here 问过类似的问题现在,我正在尝试适应图像。

我输入的图片:

enter image description here

我的输出:

enter image description here

#define MPI 3.14159265358979323846264338327950288419716939937510
#define RAD2DEG (180./MPI)
#include "opencv2/core/core.hpp"
#include "opencv2/imgproc/imgproc.hpp"
#include "opencv2/imgcodecs.hpp"
#include "opencv2/highgui/highgui.hpp"
#include <opencv2/opencv.hpp>
#include <iostream>
#include <cmath>
#include <math.h>
#include <string.h>
using namespace cv;
using namespace std;

int main()
{

Mat image = imread("5px.jpg", 1);
if (image.empty())
{
cout << "Couldn't load " << image << endl;

}
else
{
cout << "Image upload, go" << endl;
}


namedWindow("ImageIn", CV_WINDOW_AUTOSIZE);
imshow("ImageIn", image);
Mat imgGrayScale;

cvtColor(image, imgGrayScale, CV_BGR2GRAY);


float *deltaP = new float[imgGrayScale.cols];
float *angle = new float[imgGrayScale.cols];
float *coeff = new float[imgGrayScale.cols];
int col;


for (col = 0; col < imgGrayScale.cols; ++col)
{
//cout << "position x = " << col << endl;
deltaP[col] = imgGrayScale.at<uchar>(0, col);
//cout << "luminance = " << deltaP[col] << endl;

angle[col] = acos(deltaP[col] / 255);
//cout << "angle =" << angle[col] << endl;

coeff[col] = (1 / cos(angle[col]));
cout << "coeff = " << coeff[col] << endl;
}

int width = imgGrayScale.size().width;
int height = imgGrayScale.size().height;

int width2 = width * 5;

int idx_coef = 0;
Mat Z = Mat::zeros(height, width2, CV_8UC1);


//for (int r = 0; r < imgGrayScale.rows; r++)
//{
//cout << "Saut de ligne " << endl << endl << endl;
for (int t = 0; t < imgGrayScale.cols; t++)
{
//cout << "Saut de colonne " << endl;
// Attribue le coeff à une variable
int c = int(coeff[idx_coef]);
//cout << "x" << t << endl;

for (int i = 0; i < c; ++i)
{
Z.at<uchar>(0, c) = imgGrayScale.at<uchar>(0, t);
}


float alpha = fmod(coeff[idx_coef], 1.f);
float beta = 1.f - alpha;

Z.at<uchar>(0, c + 1) = (alpha * imgGrayScale.at<uchar>(0, t) + beta * imgGrayScale.at<uchar>(0, t + 1));

idx_coef++;
coeff[idx_coef] = coeff[idx_coef] - beta;



if (idx_coef >= width - 1)
{

int cc = int(coeff[idx_coef]);
for (int i = 0; i < cc; ++i)
{
Z.at<uchar>(0, c) = imgGrayScale.at<uchar>(0, t);
}
idx_coef = 0;
break;

}

}
//}

namedWindow("m", CV_WINDOW_AUTOSIZE);
imshow("m", Z);
imwrite("lumianacetest.jpg", Z);
int t = waitKey();
if ((char)t == 27)

return 0;
}

最佳答案

  • 您在访问矩阵 Z 时弄乱了索引。您不应在 c 列访问 Z,但您需要访问 current 列(作为 vector::push_back会做)。所以你可以将当前索引列保存在一个变量中,这里是idx_z,每次访问Z
  • 时都会递增它
  • 这里你的 ZCV_8U,所以你失去了准确性,因为你的值是 float。您可以将Z创建为CV_32F,如果您需要以CV_8U格式存储值以保存图像,您可以转换为 CV_8U 后来,最终。
  • Z 的最后一列不会被设置为任何值(因此我将它们初始化为值 0)。如果您需要它们具有 imgGrayScale 中的最后一个值,只需对代码的相关部分进行反注释即可。

这里是代码:

#define MPI 3.14159265358979323846264338327950288419716939937510
#define RAD2DEG (180./MPI)

#include <opencv2\opencv.hpp>
#include <vector>
using namespace cv;
using namespace std;

int main()
{
Mat1b imgGrayScale = (Mat1b(2, 5) << 50, 100, 150, 200, 250,
50, 100, 150, 200, 250);

vector<float> deltaP(imgGrayScale.cols);
vector<float> angle(imgGrayScale.cols);
vector<float> coeff(imgGrayScale.cols);
int col;


for (col = 0; col < imgGrayScale.cols; ++col)
{
//cout << "position x = " << col << endl;
deltaP[col] = imgGrayScale.at<uchar>(0, col);
//cout << "luminance = " << deltaP[col] << endl;

angle[col] = acos(deltaP[col] / 255);
//cout << "angle =" << angle[col] << endl;

coeff[col] = (1 / cos(angle[col]));
cout << "coeff = " << coeff[col] << endl;
}

int width = imgGrayScale.size().width;
int height = imgGrayScale.size().height;

int width2 = width * 5;


Mat1f Z(height, width2, 0.f);


for (int r = 0; r < imgGrayScale.rows; r++)
{
int idx_lum = 0;
int idx_coef = 0;
int idx_z = 0;

vector<float> coef = coeff;

// Set all values in Z to the last value in imgGrayScale
Z.row(r) = imgGrayScale(r, imgGrayScale.cols-1);

while (true)
{
int c = int(coef[idx_coef]);

for (int i = 0; i < c; ++i)
{
Z(r, idx_z++) = imgGrayScale(r, idx_lum);
}


float alpha = fmod(coef[idx_coef], 1.f);
float beta = 1.f - alpha;

Z(r, idx_z++) = (alpha * imgGrayScale(r, idx_lum) + beta * imgGrayScale(r, idx_lum + 1));

idx_coef++;
idx_lum++;
coef[idx_coef] = coef[idx_coef] - beta;

if (idx_lum >= imgGrayScale.cols - 1 || idx_coef >= coef.size() - 1)
{

int cc = int(coef[idx_coef]);
for (int i = 0; i < cc; ++i)
{
Z(r, idx_z++) = imgGrayScale(r, idx_lum);
}
idx_coef = 0;
break;

}

}
}

Mat1b ZZ;
Z.convertTo(ZZ, CV_8U);

cout << "Float values:" << endl;
cout << Z << endl << endl;

cout << "Uchar values:" << endl;
cout << ZZ << endl << endl;

namedWindow("m", CV_WINDOW_AUTOSIZE);
imshow("m", Z);
imwrite("lumianacetest.png", ZZ);
waitKey();

return 0;
}

关于c++ - 图像处理 : luminance weighted 2,我们在Stack Overflow上找到一个类似的问题: https://stackoverflow.com/questions/35305206/

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