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Table of contents
1.
Introduction
2.
Optical Flow 
2.1.
Lucas Kannade Method
3.
Implementation
4.
Applications
5.
FAQs
6.
Key Takeaways
Last Updated: Mar 27, 2024
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Optical Flow & Applications

Author Arun Nawani
0 upvote
Master Python: Predicting weather forecasts
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Ashwin Goyal
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Introduction

The primary difference between an image and a video is that a video is a collection of images sequenced in a very specific order. In more technical terms, videos have a temporal structure in addition to a spatial structure found in images. Information in a video is recorded not only spatially, i.e, objects or people in a video, but also sequentially. This extra piece of information is what makes classifying videos a bit more challenging. We require an algorithm that could classify videos keeping the motion of the video as a key feature.

Optical Flow 

Optical flow is the pattern of apparent motion of objects in the image between 2 consecutive frames caused by the displacement of the object or the camera. 

There are two major assumptions that optical flow assumes. 

  • It assumes that the brightness of every frame in the video is constant. 
  • Neighbouring pixels are in a similar motion. 

Optical flow is per pixel prediction, and it tries to estimate how the pixel brightness moves across the window over time. 

Consider a pixel at coordinates I(x, y, t), where t is time which is the third dimension. Now, consider the pixel moves by distance  dx, dy in time dt. 

So, since the pixel intensity remains unaltered. We can say that. 

I(x, y, t) = I(x + dx, y + dy, t + dt)

 

Here, the change in location is predicted by flow field. 

Suppose, there is an RGB pixel with values (255, 255, 255) at coordinates (11,15) at time t = 1 second. Optical flow assumes that the same RGB values,(255, 255, 255), will still be there on the screen at t=2 seconds. If there is a motion, the change of coordinates will give the displacement vector. Let’s say at t=2 seconds; the pixel is at (16, 23). The optical flow displacement vector for this pixel will be (5, 8). This means that if we take the pixel in the previous frame and apply the displacement vector to it, we should get the new image. 

Going back to the equation we derived earlier, 

I(x, y, t) = I(x + dx, y + dy, t + dt)

 

We simplify the equation using Taylor series, remove common terms and divide it by dt to get the final equation as - 

fxu + fyv + ft = 0   

 

Here,  fx , f are image gradients and fis the gradient of time. u  and v are unknown variables that can be solved using Lucas Kannade Method. 

Lucas Kannade Method

Remember, the second assumption of optical flow - Neighbouring pixel have similar motion. Lucas Kannade makes use of this assumption to take a 3x3 patch around a point and all the 9 points are assumed to have a similar motion. We can find fx,fy,f for these 9 points. So we now have 9 equations with 2 unknown variables in each to find. This is a computationally expensive task. A more convenient method would be the least square fit method. The equation for finding u,v is given by - 

Source - link

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Implementation

You can download the dataset from here. Video link can be found here.

import cv2
import numpy as np 
import math
import copy

def jacobian(x_shape, y_shape):
    # get jacobian of the template size.
    x = np.array(range(x_shape))
    y = np.array(range(y_shape))
    x, y = np.meshgrid(x, y) 
    ones = np.ones((y_shape, x_shape))
    zeros = np.zeros((y_shape, x_shape))

    row1 = np.stack((x, zeros, y, zeros, ones, zeros), axis=2)
    row2 = np.stack((zeros, x, zeros, y, zeros, ones), axis=2)
    jacob = np.stack((row1, row2), axis=2)

    return jacob

def get_template(image, roi, num_layers):
    template = cv2.cvtColor(image, cv2.COLOR_BGR2GRAY)
    template = cv2.GaussianBlur(template, (5, 5), 5) 
    template = resample_image(template, num_layers, resample=cv2.pyrDown)
    
    scale_down = 1/2**num_layers
    roi = (roi * scale_down).astype(int)
    
    #template = (template - np.mean(template)) / np.std(template)
    #return crop(template, roi)
    return template

def normalize_image(image, template):
    image = (image * (np.mean(template)/np.mean(image))).astype(float)
    return image

def resample_image(image, iteration, resample):
    for i in range(iteration):
        image = resample(image)
    return image

def crop(img, roi):
    return img[roi[0][1]:roi[1][1], roi[0][0]:roi[1][0]]

def gamma_correction(image, gamma=1.0):
# build a lookup table mapping the pixel values [0, 255] to
# their adjusted gamma values
invGamma = 1.0 / gamma
table = np.array([((i / 255.0) ** invGamma) * 255
for i in np.arange(0, 256)]).astype("uint8")
# apply gamma correction using the lookup table
return cv2.LUT(image, table)

def equalize_light(image, limit=12.0, grid=(2,2), gray=False):
    if (len(image.shape) == 2):
        image = cv2.cvtColor(image, cv2.COLOR_GRAY2BGR)
        gray = True
    
    clahe = cv2.createCLAHE(clipLimit=limit, tileGridSize=grid)
    lab = cv2.cvtColor(image, cv2.COLOR_BGR2LAB)
    l, a, b = cv2.split(lab)

    cl = clahe.apply(l)
    #cl = cv2.equalizeHist(l)
    limg = cv2.merge((cl,a,b))

    image = cv2.cvtColor(limg, cv2.COLOR_LAB2BGR)
    if gray: 
        image = cv2.cvtColor(image, cv2.COLOR_BGR2GRAY)

    return np.uint8(image)

def update_roi_bolt(frame, roi):
    roi_map = {
        50: np.array([[221, 73], [278, 173]]),
        110: np.array([[206, 53], [269, 174]]),
        150: np.array([[272, 70], [319, 166]]),
        190: np.array([[327, 66], [381, 162]]),
        220: np.array([[327, 89], [382, 172]]),
        250: np.array([[351, 98], [420, 173]]),
        280: np.array([[351, 85], [410, 176]]), 
    }
    return roi_map.get(frame, roi)

def update_roi_car(frame, roi):
    roi_map = {
        50: np.array([[64, 52], [167, 133]]),
        100: np.array([[81, 58], [163, 127]]),
        130: np.array([[82, 64], [176, 138]]),
        160: np.array([[100, 55], [199, 134]]),
        180: np.array([[116, 59], [198, 128]]),
        210: np.array([[135, 60], [227, 130]]),
        240: np.array([[160, 58], [248, 126]]),
        280: np.array([[191, 59], [261, 119]]),
        320: np.array([[200, 65], [278, 122]]),
        400: np.array([[221, 74], [295, 128]])
    }
    return roi_map.get(frame, roi)

def update_roi_baby(frame, roi):
    roi_map = {
        14: np.array([[133, 78], [207, 141]]),
        44: np.array([[21, 44], [135, 105]]),
        55: np.array([[193, 81], [259, 132]]),
        80: np.array([[94, 133], [209, 252]]),
        90: np.array([[166, 63], [253, 160]])
    }
    return roi_map.get(frame, roi)

def affineLKtracker(img, template, rect, p, threshold, check_brightness, max_iter=100):
        d_p_norm = np.inf
        
        template = crop(template, rect)
        rows, cols = template.shape
        
        #img = (img-np.mean(img))/np.std(img)
        p_prev = p
        iter = 0
        while (d_p_norm >= threshold) and iter <= max_iter:
            warp_mat = np.array([[1+p_prev[0], p_prev[2], p_prev[4]], [p_prev[1], 1+p_prev[3], p_prev[5]]])
          
            
            warp_img = crop(cv2.warpAffine(img, warp_mat, (img.shape[1],img.shape[0]),flags=cv2.INTER_CUBIC), rect)
            if check_brightness and np.linalg.norm(warp_img) < np.linalg.norm(template):
                #warp_img  = gamma_correction(warp_img.astype(int), gamma=1.5)
                print('inside')
                warp_img = equalize_light(warp_img.astype(int))
                
            diff = template.astype(int) - warp_img.astype(int)
        
            # Calculate warp gradient of image
            grad_x = cv2.Sobel(img, cv2.CV_64F, 1, 0, ksize=5)
            grad_y = cv2.Sobel(img, cv2.CV_64F, 0, 1, ksize=5)
            
            #warp the gradient
            grad_x_warp = crop(cv2.warpAffine(grad_x, warp_mat, (img.shape[1],img.shape[0]),flags=cv2.INTER_CUBIC+cv2.WARP_INVERSE_MAP), rect)
            grad_y_warp = crop(cv2.warpAffine(grad_y, warp_mat, (img.shape[1],img.shape[0]),flags=cv2.INTER_CUBIC+cv2.WARP_INVERSE_MAP), rect)
            
            # Calculate Jacobian for the 
            jacob = jacobian(cols, rows)
            
            grad = np.stack((grad_x_warp, grad_y_warp), axis=2)
            grad = np.expand_dims((grad), axis=2)
            
            #calculate steepest descent
            steepest_descents = np.matmul(grad, jacob)
            steepest_descents_trans = np.transpose(steepest_descents, (0, 1, 3, 2))
            
            # Compute Hessian matrix
            hessian_matrix = np.matmul(steepest_descents_trans, steepest_descents).sum((0,1))
        
            # Compute steepest-gradient-descent update
            diff = diff.reshape((rows, cols, 1, 1))
            update = (steepest_descents_trans * diff).sum((0,1))
            
            # calculate dp and update it
            d_p = np.matmul(np.linalg.pinv(hessian_matrix), update).reshape((-1))
                
            p_prev += d_p
            
            d_p_norm = np.linalg.norm(d_p)
            iter += 1
            
        return p_prev



def pyr_LK_Tracker(image, template, roi, num_layers, threshold, check_brightness):
    image_copy = copy.deepcopy(image)
    template_copy = copy.deepcopy(template)
    
    scale_down = 1/2**num_layers
    scale_up = 2**num_layers
    roi_down = (roi*scale_down).astype(int)
    
    image = resample_image(image, num_layers, resample=cv2.pyrDown)
    p = np.zeros(6)
    roi_pyr = roi_down
    
    #num_layers = 0  # to be removed
    for i in range(num_layers+1):
        p = affineLKtracker(image, template_copy, roi_pyr, p, threshold, check_brightness)
        
        image = resample_image(image, iteration=1, resample=cv2.pyrUp)
        template_copy = resample_image(template_copy, iteration=1, resample=cv2.pyrUp)
        roi_pyr = (roi_pyr * 2).astype(int)
        
    return p

if __name__ == "__main__":
    frame = 1
    frame_str = str(frame).zfill(4) 
    folder_path = 'DragonBaby/img/'
    img_file = folder_path + frame_str + '.jpg'
    template = cv2.imread(img_file)
    height, width, _ = template.shape
    #template = cv2.cvtColor(template, cv2.COLOR_BGR2GRAY)

    roi = np.array([[149, 63], [223, 154]])  # baby
    
    rect_tl_pt = np.array([roi[0][0], roi[0][1], 1])
    rect_br_pt = np.array([roi[1][0], roi[1][1], 1])
    frame = 2

    fourcc = cv2.VideoWriter_fourcc(*'XVID')
    out = cv2.VideoWriter("track_baby3.avi", fourcc, 10.0, (width,height))

    num_layers = 1
    template_copy = copy.deepcopy(template)
    template = get_template(template, roi, num_layers)
    threshold = 0.001

    while True:
        img_file = folder_path + frame_str + '.jpg'
        image = cv2.imread(img_file)
        
        if image is None or cv2.waitKey(1) == 27:
            print('No Image found')
            break
            
        image_copy = copy.deepcopy(image)
        image = cv2.cvtColor(image, cv2.COLOR_BGR2GRAY)
        image = cv2.GaussianBlur(image, (5, 5), 5)
        image = normalize_image(image, template)
        
        p = np.zeros(6)
        p_prev = p
        
        p = pyr_LK_Tracker(image, template, roi, num_layers, threshold, False)
        warp_mat = np.array([[1 + p[0], p[2], p[4]], [p[1], 1 + p[3], p[5]]])
    
        rect_tl_pt_new = (warp_mat @ rect_tl_pt).astype(int)
        rect_br_pt_new = (warp_mat @ rect_br_pt).astype(int)
  
        cv2.rectangle(image_copy, tuple(rect_tl_pt_new), tuple(rect_br_pt_new), (255, 255, 0), 1)
        cv2.imshow('Tracked Image', image_copy)
        
        frame += 1
        frame_str = str(frame).zfill(4)
        p_prev = p
        
        
        roi = update_roi_baby(frame, roi)
        rect_tl_pt = np.array([roi[0][0], roi[0][1], 1])
        rect_br_pt = np.array([roi[1][0], roi[1][1], 1])
        
        
        #print('frame----------------', frame)
        
        out.write(image_copy)
        
        
    out.release()    
    cv2.destroyAllWindows()

 

Output:

Applications

Optical flow finds various uses in the domain of deep learning as well as outside of it. Some examples of Optical flow uses outside of deep learning are:

  • 3D shape generation from motion
  • Global motion compensation used in video compression, and stabilisation. 
  • Used in autonomous vehicle navigation. 
  • Used in film industry for intense VFX shots. 

 

Examples of Optical flow applications in the domain of deep learning include:

  • Used in smoothening of generative adversarial networks so that outputs can be temporally coherent. This would be a tough task if we were to use only GANs which are unable to encode a temporal coherent. 
  • Video recognition using the two-stream architecture where the first stream takes the raw image and the second stream takes a series of optical flow images. 
    Also read, Sampling and Quantization

FAQs

  1. What are the 2 main assumptions of optical flow?
    Optical flow assumes that the pixel intensity remains constant across all the frames in a video. The second assumption in optical flow is that the neighbouring pixels are in a similar motion. 
     
  2. Mention one limitation of optical flow in digital video processing. 
    The main problem with the optical flow is that the smoothness of the motion doesn’t allow for discontinuities of motion across object boundaries in a given scene. 

Key Takeaways

The blog gives a brief introduction to optical flow and discusses its various applications in deep learning. The blog also gives an implementation of sparse optical flow using Lucas Kannade method. Readers are strongly advised to go through the blog at least a few couple times. If you wish to take a stride forward in your machine learning career, you may want to check out our industry-oriented machine learning courses. 

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