Lab: Edge Detection

CSC 295 - Computer Vision - Weinman

Summary:

We calculate image gradients to find edges at multiple scales, strengths, and orientations.

Due:

2/17

Deliverables

• The Matlab script used to make your comparisons and generate all figures
• (10 points) Horizontal and vertical partial derivatives (A.5, A.7)
  Note: You may wish to place the side-by-side in the same figure with one caption.
• (10 points) Observations of the horizontal and vertical partial derivatives (A.6, A.8)
• (10 points) Gradient magnitude image and observations (B.2)
• (10 points) Gradient orientation image and observations (C.4, 5)
• (10 points) Multi-scale gradient magnitude and orientation images (E.2)
  Note: Using the same figure with a single caption, you may wish to place these images together in two rows, with the scale varying horizontally across the page.
• (10 points) Observations of multi-scale gradient magnitudes (F.1)
• (10 points) Observations of multi-scale gradient orientations (F.2)
• (10 points) Multi-scale edge images (E.4)
  Note: You may wish to arrange these images into a grid, with scale changing along the vertical axis and the threshold changing along the horizontal. Regardles of how they are arranged, be sure your captions are clear.
• (10 points) Multi-scale edge observations (F.3)
• (10 points) Professionalism of write-up

Preparation

/home/weinman/courses/CSC295/images/bug.png

Exercises

A. Gradient Components

1. Create a 1-D Gaussian kernel with variance 4 using gkern.

   gauss = gkern(4);
2. We can also create a 1-D derivative of Gaussian kernel with variance 4 by giving another argument to gkern that specifies how many times we want to take the derivative:

   dgauss = gkern(4,1);

   (For completeness, you could have given the argument 0 in the previous exercise to indicate taking the derivative zero times.)
3. Recall that conv2 accepts two separable kernels for filtering: one to operate along rows and the other to operate along columns. Use your two Gaussian kernels to calculate the partial derivative of the bug image along the rows (that is, the horizontal partial derivative). Have it return an answer only for the valid portions of the convolution (the last parameter should be 'valid' rather than 'same').
4. Display your result as an image, remembering that the partial derivative may be positive or negative. Thus, you will need to tell imshow to relax its displaying conventions.
5. Save your image using a combination of imwrite and imadj (a custom procedure that linearly remaps low (high, resp.) values to 0 (1, resp.)). For example,

   imwrite(imadj(X),'mypic.png');
6. Interpret your result. Where is it bright? Where is it dark? Where is it gray? In all three cases: why?
7. Calculate the partial derivative of the image along the columns in a similar fashion. Display and save your result.
8. Inspect your result, making similar observations as in A.6.

B. Gradient Magnitude

1. Create an image representing the magnitude of the gradient at each pixel location. (Recall that the magnitude of a vector is the root of the sum of the squares of its components.)
2. Display, save, and inspect your image. Where are the strongest responses? How do they correspond to the values of the partial derivatives?
3. It is typical to place a threshold on the gradient magnitude so that the edge detection result is binary. Use a vectorized "greater than" operation on the gradient magnitude and display your thresholded image.
   You may wish to start with a threshold of 0.02 and adjust it to find what you think is a good threshold for a nice edge image.

C. Gradient Orientation

1. As we discussed in class, use atan2 to create an image representing the orientation/direction of the gradient at each pixel location.
2. Recall that the gradient orientation may be in the range [-pi,pi]. We can tell imshow to treat these as its bounds for display (black to white) explicitly, i.e.,

   imshow(X,[-pi pi]);

   Display your orientation image in this fashion.
3. Black and white values are not very intuitive for interpreting orientation. Fortunately, Matlab has a built-in way of changing the way actual image values are mapped to display values. Much like you've done before manually, you can explicitly change the map using the command colormap. This requires an argument. The procedure hsv creates a circular color map that is useful for such visualizations. Apply this to your figure:

   colormap(hsv); % Change the map of the 

                  % current figure to "hsv"

   colorbar;      % Add a color bar to the figure 

                  % to aid interpretation
4. Use print to save your orientation image. (Recall that afterward you may wish to use

   $ convert -trim in.png out.png

   to tighten up the boundaries.)
5. Spend some time analyzing the orientations. Where do the colors indicate the gradient points horizontally? "Diagonally?" Vertically? Be sure to distinguish direction (i.e., left versus right.) Do these make sense with respect to the image contents?

D. Gradient Orientation Revisited

Hue:

the pure chroma

Saturation:

the amount of color present

Value:

the perceived brightness

1. To represent the hue, rescale your previous orientation image so that instead of the range [-pi,pi] it has the range [0,1].
   Hint: To rescale a quantity x from [a,b] to [0,1], something you will do quite often, you can use the transform
   

   xrescale=(x-a)/(b-a).
2. To represent the saturation, create a rescaled version of the gradient magnitude image so that the maximum value in the rescaled version is 1. Hint: Here we can simply divide by the largest value.
3. To represent the value, create an image of all ones the same size as your other images.
4. To create the final HSV image, concatenate these M×N matrices along the third dimension into one M×N×3 image using the cat procedure, i.e.,

   W = cat(3,X,Y,Z);
5. Convert your new HSV image to an RGB image using hsv2rgb, i.e.,

   B = hsv2rgb(A);

E. Edge Detection and Scale

1. Place your commands for creating the gaussian kernels, partial derivatives, gradient magnitude, and weighted orientation (the RGB version from D.5) inside a for loop that calculates these for the following Gaussian variances: 1, 2, 4, 16, and 32.
2. Inside your loop, add commands to save your rescaled magnitude image (from D.2) and color orientation image as PNG files.
   Hint: To automatically create appropriate file names, you can use num2str to convert from numbers to strings as done in the image formation lab.
3. We also need to threshold our edges so that we have binary detections. Inside your loop, add another for loop over several gradient magnitude thresholds: [2/256], [4/256], [8/256], [12/256].
   Hint: For an easier to read file name, you may wish to loop over the numerators and use the denominator when calculating the threshold.
4. The command subplot(m,n,p) breaks a figure window into an m×n array of axes and set the pth axis as the current. For instance, The following table shows the values of p where m is 2 and n is 3.

   1	2	3
   4	5	6

   
   
   Inside your inner loop (over thresholds), add commands to
   • activate an appropriate subplot in a 1×4 array of axes
   • display the (binary) thresholded image
   After your inner loop, use the print to save the figure's array of (binary) thresholded images as a PNG file.

F. Analysis

1. How do the magnitude images change as the scale increases?
2. How do the orientation images change as the scale increases?
3. How do the detection images change with scale and threshold? Note: these are not independent; consider them together. What happens as each changes? (For example consider the four extrema along both axes.)