OpenCV: Discrete Fourier Transform

| OpenCV 3.4.2 Open Source Computer Vision

Discrete Fourier Transform

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## Goal

We'll seek answers for the following questions:

- What is a Fourier transform and why use it?
- How to do it in OpenCV?
- Usage of functions such as: copyMakeBorder() , merge() , dft() , getOptimalDFTSize() , log() and normalize() .

## Source code

C++

You can download this from here or find it in the `samples/cpp/tutorial_code/core/discrete_fourier_transform/discrete_fourier_transform.cpp` of the OpenCV source code library.

Java

You can download this from here or find it in the `samples/java/tutorial_code/core/discrete_fourier_transform/DiscreteFourierTransform.java` of the OpenCV source code library.

Python

You can download this from here or find it in the `samples/python/tutorial_code/core/discrete_fourier_transform/discrete_fourier_transform.py` of the OpenCV source code library.

Here's a sample usage of dft() :

C++
#include "opencv2/core.hpp"
#include "opencv2/imgproc.hpp"
#include "opencv2/imgcodecs.hpp"
#include "opencv2/highgui.hpp"
#include <iostream>
using namespace cv;
using namespace std;
static void help(void)
{
cout << endl
<< "This program demonstrated the use of the discrete Fourier transform (DFT). " << endl
<< "The dft of an image is taken and it's power spectrum is displayed." << endl
<< "Usage:" << endl
<< "./discrete_fourier_transform [image_name -- default ../data/lena.jpg]" << endl;
}
int main(int argc, char ** argv)
{
help();
const char* filename = argc >=2 ? argv[1] : "../data/lena.jpg";
Mat I = imread(filename, IMREAD_GRAYSCALE);
if( I.empty()){
cout << "Error opening image" << endl;
return -1;
}
Mat padded; //expand input image to optimal size
int m = getOptimalDFTSize( I.rows );
int n = getOptimalDFTSize( I.cols ); // on the border add zero values
copyMakeBorder(I, padded, 0, m - I.rows, 0, n - I.cols, BORDER_CONSTANT, Scalar::all(0));
Mat planes[] = {Mat_<float>(padded), Mat::zeros(padded.size(), CV_32F)};
Mat complexI;
merge(planes, 2, complexI); // Add to the expanded another plane with zeros
dft(complexI, complexI); // this way the result may fit in the source matrix
// compute the magnitude and switch to logarithmic scale
// => log(1 + sqrt(Re(DFT(I))^2 + Im(DFT(I))^2))
split(complexI, planes); // planes[0] = Re(DFT(I), planes[1] = Im(DFT(I))
magnitude(planes[0], planes[1], planes[0]);// planes[0] = magnitude
Mat magI = planes[0];
magI += Scalar::all(1); // switch to logarithmic scale
log(magI, magI);
// crop the spectrum, if it has an odd number of rows or columns
magI = magI(Rect(0, 0, magI.cols & -2, magI.rows & -2));
// rearrange the quadrants of Fourier image so that the origin is at the image center
int cx = magI.cols/2;
int cy = magI.rows/2;
Mat q0(magI, Rect(0, 0, cx, cy)); // Top-Left - Create a ROI per quadrant
Mat q1(magI, Rect(cx, 0, cx, cy)); // Top-Right
Mat q2(magI, Rect(0, cy, cx, cy)); // Bottom-Left
Mat q3(magI, Rect(cx, cy, cx, cy)); // Bottom-Right
Mat tmp; // swap quadrants (Top-Left with Bottom-Right)
q0.copyTo(tmp);
q3.copyTo(q0);
tmp.copyTo(q3);
q1.copyTo(tmp); // swap quadrant (Top-Right with Bottom-Left)
q2.copyTo(q1);
tmp.copyTo(q2);
normalize(magI, magI, 0, 1, NORM_MINMAX); // Transform the matrix with float values into a
// viewable image form (float between values 0 and 1).
imshow("Input Image" , I ); // Show the result
imshow("spectrum magnitude", magI);
waitKey();
return 0;
}
Java
import org.opencv.core.*;
import org.opencv.highgui.HighGui;
import org.opencv.imgcodecs.Imgcodecs;
import java.util.List;
import java.util.*;
class DiscreteFourierTransformRun{
private void help() {
System.out.println("" +
"This program demonstrated the use of the discrete Fourier transform (DFT). \n" +
"The dft of an image is taken and it's power spectrum is displayed.\n" +
"Usage:\n" +
"./DiscreteFourierTransform [image_name -- default ../data/lena.jpg]");
}
public void run(String[] args){
help();
String filename = ((args.length > 0) ? args[0] : "../data/lena.jpg");
Mat I = Imgcodecs.imread(filename, Imgcodecs.IMREAD_GRAYSCALE);
if( I.empty() ) {
System.out.println("Error opening image");
System.exit(-1);
}
Mat padded = new Mat(); //expand input image to optimal size
int m = Core.getOptimalDFTSize( I.rows() );
int n = Core.getOptimalDFTSize( I.cols() ); // on the border add zero values
Core.copyMakeBorder(I, padded, 0, m - I.rows(), 0, n - I.cols(), Core.BORDER_CONSTANT, Scalar.all(0));
List<Mat> planes = new ArrayList<Mat>();
padded.convertTo(padded, CvType.CV_32F);
planes.add(padded);
planes.add(Mat.zeros(padded.size(), CvType.CV_32F));
Mat complexI = new Mat();
Core.merge(planes, complexI); // Add to the expanded another plane with zeros
Core.dft(complexI, complexI); // this way the result may fit in the source matrix
// compute the magnitude and switch to logarithmic scale
// => log(1 + sqrt(Re(DFT(I))^2 + Im(DFT(I))^2))
Core.split(complexI, planes); // planes.get(0) = Re(DFT(I)
// planes.get(1) = Im(DFT(I))
Core.magnitude(planes.get(0), planes.get(1), planes.get(0));// planes.get(0) = magnitude
Mat magI = planes.get(0);
Mat matOfOnes = Mat.ones(magI.size(), magI.type());
Core.add(matOfOnes, magI, magI); // switch to logarithmic scale
Core.log(magI, magI);
// crop the spectrum, if it has an odd number of rows or columns
magI = magI.submat(new Rect(0, 0, magI.cols() & -2, magI.rows() & -2));
// rearrange the quadrants of Fourier image so that the origin is at the image center
int cx = magI.cols()/2;
int cy = magI.rows()/2;
Mat q0 = new Mat(magI, new Rect(0, 0, cx, cy)); // Top-Left - Create a ROI per quadrant
Mat q1 = new Mat(magI, new Rect(cx, 0, cx, cy)); // Top-Right
Mat q2 = new Mat(magI, new Rect(0, cy, cx, cy)); // Bottom-Left
Mat q3 = new Mat(magI, new Rect(cx, cy, cx, cy)); // Bottom-Right
Mat tmp = new Mat(); // swap quadrants (Top-Left with Bottom-Right)
q0.copyTo(tmp);
q3.copyTo(q0);
tmp.copyTo(q3);
q1.copyTo(tmp); // swap quadrant (Top-Right with Bottom-Left)
q2.copyTo(q1);
tmp.copyTo(q2);
magI.convertTo(magI, CvType.CV_8UC1);
Core.normalize(magI, magI, 0, 255, Core.NORM_MINMAX, CvType.CV_8UC1); // Transform the matrix with float values
// into a viewable image form (float between
// values 0 and 255).
HighGui.imshow("Input Image" , I ); // Show the result
HighGui.imshow("Spectrum Magnitude", magI);
HighGui.waitKey();
System.exit(0);
}
}
public class DiscreteFourierTransform {
public static void main(String[] args) {
// Load the native library.
System.loadLibrary(Core.NATIVE_LIBRARY_NAME);
new DiscreteFourierTransformRun().run(args);
}
}
Python
from __future__ import print_function
import sys
import cv2 as cv
import numpy as np
def print_help():
print('''
This program demonstrated the use of the discrete Fourier transform (DFT).
The dft of an image is taken and it's power spectrum is displayed.
Usage:
discrete_fourier_transform.py [image_name -- default ../../../../data/lena.jpg]''')
def main(argv):
print_help()
filename = argv[0] if len(argv) > 0 else "../../../../data/lena.jpg"
I = cv.imread(filename, cv.IMREAD_GRAYSCALE)
if I is None:
print('Error opening image')
return -1
rows, cols = I.shape
m = cv.getOptimalDFTSize( rows )
n = cv.getOptimalDFTSize( cols )
padded = cv.copyMakeBorder(I, 0, m - rows, 0, n - cols, cv.BORDER_CONSTANT, value=[0, 0, 0])
planes = [np.float32(padded), np.zeros(padded.shape, np.float32)]
complexI = cv.merge(planes) # Add to the expanded another plane with zeros
cv.dft(complexI, complexI) # this way the result may fit in the source matrix
cv.split(complexI, planes) # planes[0] = Re(DFT(I), planes[1] = Im(DFT(I))
cv.magnitude(planes[0], planes[1], planes[0])# planes[0] = magnitude
magI = planes[0]
matOfOnes = np.ones(magI.shape, dtype=magI.dtype)
cv.add(matOfOnes, magI, magI) # switch to logarithmic scale
cv.log(magI, magI)
magI_rows, magI_cols = magI.shape
# crop the spectrum, if it has an odd number of rows or columns
magI = magI[0:(magI_rows & -2), 0:(magI_cols & -2)]
cx = int(magI_rows/2)
cy = int(magI_cols/2)
q0 = magI[0:cx, 0:cy] # Top-Left - Create a ROI per quadrant
q1 = magI[cx:cx+cx, 0:cy] # Top-Right
q2 = magI[0:cx, cy:cy+cy] # Bottom-Left
q3 = magI[cx:cx+cx, cy:cy+cy] # Bottom-Right
tmp = np.copy(q0) # swap quadrants (Top-Left with Bottom-Right)
magI[0:cx, 0:cy] = q3
magI[cx:cx + cx, cy:cy + cy] = tmp
tmp = np.copy(q1) # swap quadrant (Top-Right with Bottom-Left)
magI[cx:cx + cx, 0:cy] = q2
magI[0:cx, cy:cy + cy] = tmp
cv.normalize(magI, magI, 0, 1, cv.NORM_MINMAX) # Transform the matrix with float values into a
cv.imshow("Input Image" , I ) # Show the result
cv.imshow("spectrum magnitude", magI)
cv.waitKey()
if __name__ == "__main__":
main(sys.argv[1:])

## Explanation

The Fourier Transform will decompose an image into its sinus and cosines components. In other words, it will transform an image from its spatial domain to its frequency domain. The idea is that any function may be approximated exactly with the sum of infinite sinus and cosines functions. The Fourier Transform is a way how to do this. Mathematically a two dimensional images Fourier transform is:

\[F(k,l) = \displaystyle\sum\limits_{i=0}^{N-1}\sum\limits_{j=0}^{N-1} f(i,j)e^{-i2\pi(\frac{ki}{N}+\frac{lj}{N})}\]

\[e^{ix} = \cos{x} + i\sin {x}\]

Here f is the image value in its spatial domain and F in its frequency domain. The result of the transformation is complex numbers. Displaying this is possible either via a real image and a complex image or via a magnitude and a phase image. However, throughout the image processing algorithms only the magnitude image is interesting as this contains all the information we need about the images geometric structure. Nevertheless, if you intend to make some modifications of the image in these forms and then you need to retransform it you'll need to preserve both of these.

In this sample I'll show how to calculate and show the magnitude image of a Fourier Transform. In case of digital images are discrete. This means they may take up a value from a given domain value. For example in a basic gray scale image values usually are between zero and 255. Therefore the Fourier Transform too needs to be of a discrete type resulting in a Discrete Fourier Transform (DFT). You'll want to use this whenever you need to determine the structure of an image from a geometrical point of view. Here are the steps to follow (in case of a gray scale input image I):

#### Expand the image to an optimal size

The performance of a DFT is dependent of the image size. It tends to be the fastest for image sizes that are multiple of the numbers two, three and five. Therefore, to achieve maximal performance it is generally a good idea to pad border values to the image to get a size with such traits. The getOptimalDFTSize() returns this optimal size and we can use the copyMakeBorder() function to expand the borders of an image (the appended pixels are initialized with zero):

C++
Mat padded; //expand input image to optimal size
int m = getOptimalDFTSize( I.rows );
int n = getOptimalDFTSize( I.cols ); // on the border add zero values
copyMakeBorder(I, padded, 0, m - I.rows, 0, n - I.cols, BORDER_CONSTANT, Scalar::all(0));
Java
Mat padded = new Mat(); //expand input image to optimal size
int m = Core.getOptimalDFTSize( I.rows() );
int n = Core.getOptimalDFTSize( I.cols() ); // on the border add zero values
Core.copyMakeBorder(I, padded, 0, m - I.rows(), 0, n - I.cols(), Core.BORDER_CONSTANT, Scalar.all(0));
Python
rows, cols = I.shape
m = cv.getOptimalDFTSize( rows )
n = cv.getOptimalDFTSize( cols )
padded = cv.copyMakeBorder(I, 0, m - rows, 0, n - cols, cv.BORDER_CONSTANT, value=[0, 0, 0])

#### Make place for both the complex and the real values

The result of a Fourier Transform is complex. This implies that for each image value the result is two image values (one per component). Moreover, the frequency domains range is much larger than its spatial counterpart. Therefore, we store these usually at least in a float format. Therefore we'll convert our input image to this type and expand it with another channel to hold the complex values:

C++
Mat planes[] = {Mat_<float>(padded), Mat::zeros(padded.size(), CV_32F)};
Mat complexI;
merge(planes, 2, complexI); // Add to the expanded another plane with zeros
Java
List<Mat> planes = new ArrayList<Mat>();
padded.convertTo(padded, CvType.CV_32F);
planes.add(padded);
planes.add(Mat.zeros(padded.size(), CvType.CV_32F));
Mat complexI = new Mat();
Core.merge(planes, complexI); // Add to the expanded another plane with zeros
Python
planes = [np.float32(padded), np.zeros(padded.shape, np.float32)]
complexI = cv.merge(planes) # Add to the expanded another plane with zeros

#### Make the Discrete Fourier Transform

It's possible an in-place calculation (same input as output):

C++
dft(complexI, complexI); // this way the result may fit in the source matrix
Java
Core.dft(complexI, complexI); // this way the result may fit in the source matrix
Python
cv.dft(complexI, complexI) # this way the result may fit in the source matrix

#### Transform the real and complex values to magnitude

A complex number has a real (Re) and a complex (imaginary - Im) part. The results of a DFT are complex numbers. The magnitude of a DFT is:

\[M = \sqrt[2]{ {Re(DFT(I))}^2 + {Im(DFT(I))}^2}\]

Translated to OpenCV code:

C++
split(complexI, planes); // planes[0] = Re(DFT(I), planes[1] = Im(DFT(I))
magnitude(planes[0], planes[1], planes[0]);// planes[0] = magnitude
Mat magI = planes[0];
Java
Core.split(complexI, planes); // planes.get(0) = Re(DFT(I)
// planes.get(1) = Im(DFT(I))
Core.magnitude(planes.get(0), planes.get(1), planes.get(0));// planes.get(0) = magnitude
Mat magI = planes.get(0);
Python
cv.split(complexI, planes) # planes[0] = Re(DFT(I), planes[1] = Im(DFT(I))
cv.magnitude(planes[0], planes[1], planes[0])# planes[0] = magnitude
magI = planes[0]

#### Switch to a logarithmic scale

It turns out that the dynamic range of the Fourier coefficients is too large to be displayed on the screen. We have some small and some high changing values that we can't observe like this. Therefore the high values will all turn out as white points, while the small ones as black. To use the gray scale values to for visualization we can transform our linear scale to a logarithmic one:

\[M_1 = \log{(1 + M)}\]

Translated to OpenCV code:

C++
magI += Scalar::all(1); // switch to logarithmic scale
log(magI, magI);
Java
Mat matOfOnes = Mat.ones(magI.size(), magI.type());
Core.add(matOfOnes, magI, magI); // switch to logarithmic scale
Core.log(magI, magI);
Python
matOfOnes = np.ones(magI.shape, dtype=magI.dtype)
cv.add(matOfOnes, magI, magI) # switch to logarithmic scale
cv.log(magI, magI)

#### Crop and rearrange

Remember, that at the first step, we expanded the image? Well, it's time to throw away the newly introduced values. For visualization purposes we may also rearrange the quadrants of the result, so that the origin (zero, zero) corresponds with the image center.

C++
// crop the spectrum, if it has an odd number of rows or columns
magI = magI(Rect(0, 0, magI.cols & -2, magI.rows & -2));
// rearrange the quadrants of Fourier image so that the origin is at the image center
int cx = magI.cols/2;
int cy = magI.rows/2;
Mat q0(magI, Rect(0, 0, cx, cy)); // Top-Left - Create a ROI per quadrant
Mat q1(magI, Rect(cx, 0, cx, cy)); // Top-Right
Mat q2(magI, Rect(0, cy, cx, cy)); // Bottom-Left
Mat q3(magI, Rect(cx, cy, cx, cy)); // Bottom-Right
Mat tmp; // swap quadrants (Top-Left with Bottom-Right)
q0.copyTo(tmp);
q3.copyTo(q0);
tmp.copyTo(q3);
q1.copyTo(tmp); // swap quadrant (Top-Right with Bottom-Left)
q2.copyTo(q1);
tmp.copyTo(q2);
Java
// crop the spectrum, if it has an odd number of rows or columns
magI = magI.submat(new Rect(0, 0, magI.cols() & -2, magI.rows() & -2));
// rearrange the quadrants of Fourier image so that the origin is at the image center
int cx = magI.cols()/2;
int cy = magI.rows()/2;
Mat q0 = new Mat(magI, new Rect(0, 0, cx, cy)); // Top-Left - Create a ROI per quadrant
Mat q1 = new Mat(magI, new Rect(cx, 0, cx, cy)); // Top-Right
Mat q2 = new Mat(magI, new Rect(0, cy, cx, cy)); // Bottom-Left
Mat q3 = new Mat(magI, new Rect(cx, cy, cx, cy)); // Bottom-Right
Mat tmp = new Mat(); // swap quadrants (Top-Left with Bottom-Right)
q0.copyTo(tmp);
q3.copyTo(q0);
tmp.copyTo(q3);
q1.copyTo(tmp); // swap quadrant (Top-Right with Bottom-Left)
q2.copyTo(q1);
tmp.copyTo(q2);
Python
magI_rows, magI_cols = magI.shape
# crop the spectrum, if it has an odd number of rows or columns
magI = magI[0:(magI_rows & -2), 0:(magI_cols & -2)]
cx = int(magI_rows/2)
cy = int(magI_cols/2)
q0 = magI[0:cx, 0:cy] # Top-Left - Create a ROI per quadrant
q1 = magI[cx:cx+cx, 0:cy] # Top-Right
q2 = magI[0:cx, cy:cy+cy] # Bottom-Left
q3 = magI[cx:cx+cx, cy:cy+cy] # Bottom-Right
tmp = np.copy(q0) # swap quadrants (Top-Left with Bottom-Right)
magI[0:cx, 0:cy] = q3
magI[cx:cx + cx, cy:cy + cy] = tmp
tmp = np.copy(q1) # swap quadrant (Top-Right with Bottom-Left)
magI[cx:cx + cx, 0:cy] = q2
magI[0:cx, cy:cy + cy] = tmp

#### Normalize

This is done again for visualization purposes. We now have the magnitudes, however this are still out of our image display range of zero to one. We normalize our values to this range using the cv::normalize() function.

C++
normalize(magI, magI, 0, 1, NORM_MINMAX); // Transform the matrix with float values into a
// viewable image form (float between values 0 and 1).
Java
Core.normalize(magI, magI, 0, 255, Core.NORM_MINMAX, CvType.CV_8UC1); // Transform the matrix with float values
// into a viewable image form (float between
// values 0 and 255).
Python
cv.normalize(magI, magI, 0, 1, cv.NORM_MINMAX) # Transform the matrix with float values into a

## Result

An application idea would be to determine the geometrical orientation present in the image. For example, let us find out if a text is horizontal or not? Looking at some text you'll notice that the text lines sort of form also horizontal lines and the letters form sort of vertical lines. These two main components of a text snippet may be also seen in case of the Fourier transform. Let us use this horizontal and this rotated image about a text.

In case of the horizontal text:

In case of a rotated text:

You can see that the most influential components of the frequency domain (brightest dots on the magnitude image) follow the geometric rotation of objects on the image. From this we may calculate the offset and perform an image rotation to correct eventual miss alignments.