The present invention relates in general to image processing and in particular to a method and system for determining optical flow.
Optical flow is a concept which approximates the motion of objects within a visual representation. Optical flow is the velocity field which warps one image into another (usually very similar) image. Optical flow techniques are based on the idea that the same physical point on an object in the scene is captured by the camera in corresponding points in the two images preserving certain image properties such as brightness, the gradient vector, etc.
Optical flow computations are central to many image processing applications that deal with groups of similar images. For example, image sequence compression algorithms commonly use optical flow parameters to represent images compactly in terms of changes relative to preceding or succeeding images in the sequence. Optical flow parameters are also used in three-dimensional reconstruction by stereo matching of pixels in a group of images taken of an object from different angles, or by tracking the motion of rigid objects in a scene, as well as in image resolution enhancement. In addition, variations in optical flow over the area of an image may be used in image segmentation and in tracking the motion of an object across a sequence of images.
Despite much research effort invested in addressing optical flow computation it remains a challenging task in the field of computer vision. It is a necessary step in various applications like stereo matching, video compression, object tracking, depth reconstruction and motion based segmentation. Hence, many approaches have been proposed for optical flow computation. Most methods assume brightness constancy and introduce additional assumptions on the optical flow in order to deal with the inherent aperture problem. Lucas and Kanade (1981) tackled the aperture problem by solving for the parameters of a constant motion model over image patches. Subsequently, Irani et al. (1993, 1997) used motion models in a region in conjunction with Lucas-Kanade in order to recover the camera ego-motion. Spline based motion models were suggested by Szeliski and Coughlan (1997).
Horn and Schunck (1981) sought to recover smooth flow fields and were the first to use functional minimization for solving optical flow problems employing mathematical tools from calculus of variations. Their pioneering work put forth the basic idea for solving dense optical flow fields over the whole image by introducing a quality functional with two terms: a data term penalizing for deviations from the brightness constancy equation, and a smoothness term penalizing for variations in the flow field. Several important improvements have been proposed following their work. Nagel (1990, 1986) proposed an oriented smoothness term that penalizes anisotropically for variations in the flow field according to the direction of the intensity gradients. Ari and Sochen (2006) recently used a functional with two alignment terms composed of the flow and image gradients. Replacing quadratic penalty terms by robust statistics integral measures was proposed in (Black and Anandan 1996; Deriche et al. 1995) in order to allow sharp discontinuities in the optical flow solution along motion boundaries. Extensions to multi-frame formulations of the initial two-frames formulation allowed the consideration of spatiotemporal smoothness to replace the original spatial smoothness term (Black and Anandan 1991; Farnebäck 2001; Nagel 1990; Weickert and Schnörr 2001). Brox et al. (2004, 2006) demonstrated the importance of using the exact brightness constancy equation instead of its linearized version and added a gradient constancy to the data term which may be important if the scene illumination changes in time. Cremers and Soatto (2005) proposed a motion competition algorithm for variational motion segmentation and parametric motion estimation. Amiaz and Kiryati (2005) followed by Brox et al. (2006) introduced a variational approach for joint optical flow computation and motion segmentation. In Farneback (2000, 2001), a constant and affine motion model is employed. The motion model is assumed to act on a region, and optic flow based segmentation is performed by a region growing algorithm. In a classical contribution to structure from motion Adiv (1985) used optical flow in order to determine motion and structure of several rigid objects moving in the scene. Sekkati and Mitiche (2006) used joint segmentation and optical flow estimation in conjunction with a single rigid motion in each segmented region. Vázquez et al. (2006) used joint multi-region segmentation with high order DCT basis functions representing the optical flow in each segmented region.
It is an object of the present invention to represent the optical flow vector at each pixel by different coefficients of the same motion model in a variational framework. Such a grossly over-parameterized representation has the advantage that the smoothness term may now penalize deviations from the motion model instead of directly penalizing the change of the flow. For example, in an affine motion model, if the flow in a region can be accurately represented by an affine model, then in this region there will be no flow regularization penalty, while in the usual setting there is a cost resulting from the changes in the flow induced by the affine model. This over-parameterized model thereby offers a richer means for optical flow representation. For segmentation purposes, the over-parameterization has the benefit of making segmentation decisions in a more appropriate space (e.g. the parameters of the affine flow) rather than in a simple constant motion model space. The work of Ju et al. (1996) is related to our methodology, they used local affine models to describe the motion in image regions imposing spatial smoothness on the affine parameters between neighboring patches. The key and conceptually very important difference is that, in our approach, the model is represented at the pixel level which makes the problem over-parameterized while the patch size chosen in (Ju et al. 1996) makes it under-parameterized and requires the choice of a neighborhood size.
In one aspect, the present invention relates to a method of determining the optical flow vector of a plurality of image pixels between two consecutive images in a group of images, the method comprising the steps of:
(i) creating multiple sets of the group of images wherein each set contains a decreasing number of pixels per image;
(ii) defining an optical flow motion model applicable to the group of images in terms of a set of basis functions;
(iii) representing the optical flow vector of each pixel image by different coefficients of the same motion model;
(iv) starting with the set of group of images with the lowest number of pixels per image, determining respective over-parameterized optical flow vectors at the pixels responsively to motion between the images in the group by computing respective regularized coefficients of the basis functions at each of the pixels;
(v) interpolating the results to the next higher resolution set of group of images and refining the estimation using the over-parameterized optical flow representation; and
(vi) repeating step (v) until the highest resolution set of group of images is reached.
The present invention introduces a novel over-parameterized variational framework for accurately solving the optical flow problem. The flow field is represented by a general space-time model. The proposed approach is useful and highly flexible in the fact that each pixel has the freedom to choose its own set of model parameters. Subsequently, the decision on the discontinuity locations of the model parameters is resolved within the variational framework for each sequence. In most scenarios, the optical flow would be better represented by a piecewise constant affine model or a rigid motion model rather than a piecewise constant flow. Therefore, compared to existing variational techniques, the smoothness penalty term modeled by the proposed overparameterization models yields better optic flow recovery performance as demonstrated by our experiments. Our experiments focused on spatial basis functions, though the same principles apply for spatio-temporal basis functions. Incorporating learning of the basis functions (dictionaries) for specific scenes is of great interest and useful for video compression. According to the invention, motion segmentation based on optical flow should generally be replaced by segmentation in the higher dimensional parameter space as suggested by our initial results presented herein for the synthetic sequence. Although the models suggested were all over-parameterized, an under-parameterized model might also be used in this framework, for example, in case one has prior knowledge regarding constraints between the u and v components (as in stereo matching or when we know the optic flow to be radial).
In the following detailed description of various embodiments, reference is made to the accompanying drawings that form a part thereof, and in which are shown by way of illustration specific embodiments in which the invention may be practiced. It is understood that other embodiments may be utilized and structural changes may be made without departing from the scope of the present invention.
We propose to represent the optical flow (u(x, y, t), v(x, y, t)) by the general over-parameterized space-time model
where, Φi(x, y, t) and ηi(x, y, t), i=1, . . . , n are n basis functions of the flow model, while the Ai are space and time varying coefficients of the model. This is an obviously heavily over-parameterized model since for more than two basis functions, there are typically many ways to express the same flow at any specific location. This redundancy however will be adequately resolved by a regularization assumption applied to the coefficients of the model. The coefficients and basis functions may be general functions of space-time, however, they play different roles in the functional minimization process: The basis functions are fixed and selected a priori. The coefficients are the unknown functions we solve for in the optical flow estimation process. In our model, appropriate basis functions are such that the true flow could be described by approximately piecewise constant coefficients, so that most of the local spatio-temporal changes of the flow are induced by changes in the basis functions and not by variations of the coefficients. This way, regularization applied to the coefficients (as will be described later on) becomes meaningful since major parts in the optic flow variations can be described without changes of the coefficients. For example, rigid body motion has a specific optical flow structure which can explain the flow using only six parameters at locations with approximately constant depth. Let us start from conventional optical flow functionals that include a data term ED (u, v), that measures the deviation from the brightness constancy assumption, and a regularization (or smoothness) term ES (u, v) that quantifies the smoothness of the flow field. The solution is the minimizer of the sum of the data and smoothness terms
E(u,v)=ED(u,v)+αES(u,v). (2)
The main difference between the diverse variational methods is in the choice of data and smoothness terms, and in the numerical methods used for solving for the minimizing flow field (u(x, y, t), v(x, y, t)). For the data term we shall use the functional)
ED(u,v)=∫Ψ((I(x+w)−I(x))2)dx, (3)
where, x=(x, y, t)T and w=(u, v, 1)T. This is the integral measure used for example in (Brox et al. 2004) (omitting the gradient constancy term). The function Ψ(s2)=√{square root over (s2+ε2)} that is by now widely used, induces an approximate L1 metric of the data term for a small ε. The smoothness term used in (Brox et al. 2004) is given by
ES(u,v)=∫Ψ(∥{tilde over (∇)}u∥2+∥{tilde over (∇)}v∥2)dx (4)
Where {tilde over (∇)}f≡(fx, fy, ωtft)T denotes the weighted spatiotemporal gradient. ωt indicates the weight of the temporal axis relative to the spatial axes in the context of the smoothness term (ωt=1 is used in (Brox et al. 2004)). Inserting the over-parameterized model into the data term, we have
Our proposed smoothness term replaces (4) with a penalty for spatio-temporal changes in the coefficient functions,
Notice that in (6), constant parameters of the model can describe changes of the flow field according to the chosen model as described in (1) (e.g. Euclidean, affine, etc.) without smoothness penalty, whereas in (4), any change in the flow field is penalized by the smoothness term. For the sake of simplicity of the resulting Euler-Lagrange equations, we have omitted writing explicit relative weights to the different coefficients in the smoothness term, the weighting is alternatively achieved by scaling the basis functions by appropriate factors as will be shown in the description of the motion models. Scaling a basis function by a small factor would mean that in order to achieve the same overall influence on the optical flow, the corresponding coefficient would have to make larger changes (proportional to the inverse of the factor). These larger changes would be suppressed by the regularization term. On the other hand, scaling a basis function by a large factor would scale down the changes required from the corresponding coefficient in order to achieve the same overall change and therefore would result in less regularization for this specific term.
2.1 Euler-Lagrange Equations
For an over-parameterization model with n coefficients, there are n Euler-Lagrange equations, one for each coefficient. The Euler-Lagrange equation for Aq (q=1, . . . , n) is given by
where {circumflex over (∇)}f≡(fx, fy, ωt2ft)T, and
2.2 The Affine Over-Parameterization Model
The affine model is a good approximation of the flow in large regions in many real world scenarios. We therefore first start with the affine model for our method. Note that we do not force the affine model over image patches as in previously considered image registration techniques, and here each pixel has “its own” independent affine model parameters. The affine model has n=6 parameters,
and x0 and y0 are half image width and height respectively. ρ is a constant that has no meaning in an unconstrained optimization such as the Lucas-Kanade method. In our variational formulation, ρ is a parameter which weighs the penalty of the x and y coefficients relative to the coefficient of the constant term in the regularization. An equivalent alternative is to add a different weight for each coefficient in (6).
2.3 The Rigid Motion Model
The optic flow of an object moving in rigid motion or of a static scene with a moving camera is described by
u=−θ1+θ3{circumflex over (x)}+Ω1{circumflex over (x)}ŷ−Ω2(1+{circumflex over (x)}2)+Ω3ŷ,
v=−θ2+θ3ŷ+Ω1(1+ŷ2)−Ω2{circumflex over (x)}ŷ−Ω3{circumflex over (x)}, (11)
where (θ1, θ2, θ3)T is the translation vector divided by the depth and (Ω1,Ω2,Ω3)T is the rotation vector. Here too, the number of coefficients is n=6. The coefficients Ai represent the translation and rotation variables, A1=θ1; A2=θ2; A3=θ3; A4=Ω1; A5=Ω2; A6=Ω3, and the basis functions are φ1−1; Φ2=0; φ3={circumflex over (x)}; φ4={circumflex over (x)}ŷ; φ5=−(1+{circumflex over (x)}2); φ6=ŷ and ηn1=0; η2−1η3=ŷ; η4=1+ŷ2; η5=−{circumflex over (x)}ŷ; and η6=−{circumflex over (x)}. Similar constraints on optical flow of rigid motion were first introduced by Adiv in (Adiv 1985). However, there the optical flow is a preprocessing step to be followed by structure and motion estimation, while our formulation uses the rigid motion model in the optimality criterion of the optical flow estimation process. Using the rigid motion model directly in the optimality criterion was previously suggested by Sekkati and Mitiche (2003) where the functional is explicitly written in terms of the model parameters. However, since the data term in (Sekkati and Mitiche 2003) is quadratic and uses the linearized brightness constancy assumption, it is expected to be more sensitive to outliers and prone to errors for motion fields of large magnitudes. Since the optical flow induced by camera rotation is independent of the depth it has a more global nature and therefore one may wish to penalize more severely for changes in rotation when considering the smoothness term. This can be done by scaling the basis functions multiplying the rotation coefficients by a factor between 0 and 1. Such a factor would require larger changes in the coefficients in order to achieve the same overall influence of the rotation on the optical flow. Such larger changes in the corresponding coefficients would be suppressed by the regularization term and therefore achieve a more global effect of the rotation. Note, that assuming rigid motion one could also extract the depth profile (up to scaling) from the above coefficients.
2.4 Pure Translation Motion Model
A special case of the rigid motion scenario can be thought of when we limit the motion to simple translation. In this case we have,
u=−θ1+θ3{circumflex over (x)},
v=−θ1+θ3ŷ, (12)
The Euler-Lagrange equations of the rigid motion still applies in this case when considering only the first n=3 coefficients and corresponding basis functions.
2.5 Constant Motion Model
The constant motion model includes only n=2 coefficients, with
φ1=1; φ2=0
η1=0; η2=1, (13)
as basis functions. For this model there are two coefficients to solve for A1 and A2 which are the optic flow components u and v, respectively. In this case we obtain the familiar variational formulation where we solve for the u and v components. This fact can also be seen by substitution of (13) into (7), that yields the Euler-Lagrange equations used, for example, in (Brox et al. 2004) (without the gradient constancy term).
In our numerical scheme we use a multi-resolution solver, by down sampling the image data with a standard factor of 0.5 along the x and y axes between the different resolutions. The solution is interpolated from coarse to fine resolution. Similar techniques to overcome the intrinsic non-convex nature of the resulting optimization problem were used, for example, in (Brox et al. 2004), we compare our model and results to (Brox et al. 2004) since, to the best of our knowledge, that paper reports the most accurate flow field results for the Yosemite without clouds sequence. At the lowest resolution, we start with the initial guess of Ai=0, i=1, . . . , n. From this guess, the solution is iteratively refined and the coefficients are interpolated to become the initial guess at the next higher resolution and the process is repeated until the solution at the finest resolution is reached. At each resolution, three loops of iterations are applied. At the outer loop with iteration variable k, we freeze the brightness constancy linear approximation in the Euler-Lagrange equations
Inserting the first terms of the Taylor expansion
where Aik+1=Aik+dAik. The second inner loop—fixed point iteration—deals with the nonlinearity of Ψ with iteration variable l, it uses the expressions of Ψ′ from the previous iteration in both the data and smoothness terms, while the rest of the equation is written with respect to the l+1 iteration
At this point, we have for each pixel n linear equations with n unknowns, the increments of the coefficients of the model parameters. The linear system of equations is solved on the sequence volume using Gauss-Seidel iterations. Each Gauss-Seidel iteration involves the solution of n linear equations for each pixel as described by (16). The discretization uses two point central difference for the flow components and four point central difference for the image derivatives as suggested in (Barron et al. 1994).
In this section we compare our optical flow computation results to the best published results. For test sequences with ground truth, we use the standard measures of Average Angular Error (AAE) and Standard Deviation (STD). Our results are measured over all the pixels (100% dense). The angle is defined as:
where u and v are the estimated optical flow components, and ug and vg represent the ground truth optical flow. The AAE is the average and STD is the standard deviation of θ over the image domain.
4.1 Parameter Settings
The parameters were set experimentally by an optimization process which numerically minimizes the weighted sum of AAE and STD measured on the Yosemite sequence. Such a parameter optimization or training process is usual in many other papers, for example (Roth and Black 2005). Brox et al. (2004), Papenberg et al. (2006) also seem to have an optimal parameter setting since in their parameter sensitivity analysis, each parameter change in any direction results in an increase of the AAE measure for the Yosemite sequence.
We have found slightly different parameter settings for the 2D and 3D smoothness cases as shown in Table 1, where 2D refers to smoothness term with only spatial derivatives, while 3D refers to spatio-temporal smoothness term that couples the solution of the optic flow field at different frames (also known as the “two frames” versus “multi-frame” formulation). Here a denotes the standard deviation of the 2D Gaussian pre-filter used for pre-processing the image sequence. We used 60 iterations of the outer loop in the 3D method and 80 iterations in the 2D method, 5 inner loop iterations and 10 Gauss-Seidel iterations.
4.2 Yosemite Sequence
We applied our method to the Yosemite sequence without clouds (available at http://www.cs.brown.edu/people/black/images.html), with four resolution levels.
Table 2 shows our results relative to the best published ones. As seen in the table, our method achieves a better reconstructed solution compared to all other reported results for this sequence, both for the 2D and 3D cases. In fact, our result for the 2D case is good even compared to 3D results from the literature.
Table 3 summarizes the noise sensitivity results of our method. We also coupled the affine over-parameterized model with our previous work on joint optic flow computation and denoising presented in (Nir et al. 2005) by iterating between optical flow computation on the denoised sequence and denoising with the current optical flow. A related concept was first introduced by Borzi et al. (2002). This coupling provides a model with robust behavior under noise, that obtains better AAE measure under all noise levels compared to the best published results.
Our improvement relative to (Brox et al. 2004) results mostly from the over-parameterization and not by the additional smoothness weight parameter ωt. Table 4 shows the results obtained with equal spatio-temporal smoothness weights (ωt=1) as used in Brox et al. (2004). The AAE measure changes by approximately 1 percent for the pure translation model and 2 percent for the affine model, where, the ωt parameter was changed by approximately 21 and 45 percent for the pure translation and affine models respectively.
4.3 Synthetic Piecewise Constant Affine Flow Example
For illustration purposes we also considered the piecewise affine flow over an image of size 100×100 having the ground truth shown in
For x<40,
u=−0.8−1.6(x−50)/50+0.8(y−50)/50,
v=1.0+0.65(x−50)/50−0.35(y−50)/50.
For x≧40,
u=0.48−0.36(x−50)/50−0.6(y−50)/50,
v=0.3−0.75(x−50)/50−0.75(y−50)/50.
The two images used for this test were obtained by sampling a grid of size 100×100 from frame 8 of the Yosemite sequence (denoted Iyosemite). The second image I2(x, y)=Iyosemite(x+Δx, y+Δy) and the first image is sampled at warped locations I1(x, y)=Iyosemite(x+Δx+y, y+Δy+v) using bilinear interpolation. The constant shift values are: Δx=79 and Δy=69. The two images obtained are displayed in
The results exhibited in Table 5 show that our method with the affine over-parameterization outperforms the method of (Brox et al. 2004). This is to be expected since the true flow is not piecewise constant and the smoothness term in (Brox et al. 2004) penalizes for changes from the constant flow model, whereas, the affine over-parameterization model solves the optimization problem in the (correct) affine space in which it accurately finds the piecewise constant affine parameters solution of the problem, as shown in
4.4 Flower Garden Sequence
We also applied our method to the real image sequence “flower garden”. The results obtained by the 2D affine model are shown in
4.5 Road Sequence
The two frames of this real sequence courtesy of the authors of (Vázquez et al. 2006) are shown in
Although the invention has been described in detail, nevertheless changes and modifications, which do not depart from the teachings of the present invention, will be evident to those skilled in the art. Such changes and modifications are deemed to come within the purview of the present invention and the appended claims.
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/IL2008/000194 | 2/14/2008 | WO | 00 | 7/8/2010 |
Publishing Document | Publishing Date | Country | Kind |
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WO2008/099399 | 8/21/2008 | WO | A |
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