Solution Manual for Computer Vision A Modern Approach 2nd Edition by David A. Forsyth and Jean Ponce

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C H A P T E R 2: Light and Shading

PROBLEMS 2.1. We see a diffuse sphere centered at the origin, with radius one and albedop, in an orthographic camera, looking down the z-axis. This sphere is illuminated by a distant point light source whose source direction is (0, 0,1). There is no other illumination. Show that the shading field in the camera is 2 2 p\J 1 — x — y Solution: The surface is {x,y, \J\ — T2 — y1'). We get two tangent vectors by partial differentiation; they are (1,0, p) and (0,1, q) where p = —x/\/l — T2 — y1 and q = —y/\J\ — T2 — y1. You can verify that the unit normal is N = 1 + p2 + q2 and the shading must be p ((0, 0,1) • N , which yields

v7! + p12 + q2 2.2. What shapes can the shadow of a sphere take if it is cast on a plane and the source is a point source? Solution: These are conic sections with one important exception - you only get one half of the hyperbola. 2.3. We have a square area source and a square occluder, both parallel to a plane. The source is the same size as the occluder, and they are vertically above one another with their centers aligned. (a) What is the shape of the umbra? Solution: Square. This is rather a special case. You can construct the umbra by constructing all points on the plane that can see no part of the source. This is a square directly below the occluder. (b) What is the shape of the outside boundary of the penumbra?

1 Solution: This is quite a nasty question. Easiest way to construct the answer is to think about an arbitrary point on the occluder; construct a cone over the source, whose vertex is this point. Now intersect that cone with the plane — the resulting square region on the plane consists of all points such that this point on the occluder blocks some point on the source. Finally, take the union of all such regions (i.e. over all points on the occluder); that’s the penumbra. The envelope of the boundaries of these regions is the boundary of the penumbra. It’s a square. 2.4. We have a square area source and a square occluder, both parallel to a plane. The edge length of the source is now twice that of the occluder, and they are vertically above one another with their centers aligned. (a) What is the shape of the umbra?

Solution: Depending on the distances between area source, occluder and plane, either there isn’t one, or it’s square. (b) What is the shape of the outside boundary of the penumbra? Solution: same as in previous exercise; This is quite a nasty question. Easiest way to construct the answer is to think about an arbitrary point on the occluder; construct a cone over the source, whose vertex is this point. Now intersect that cone with the plane — the resulting square region on the plane consists of all points such that this point on the occluder blocks some point on the source. Finally, take the union of all such regions (i.e. over all points on the occluder); that’s the penumbra. The envelope of the boundaries of these regions is the boundary of the penumbra. It’s a square. 2.5. We have a square area source and a square occluder, both parallel to a plane. The edge length of the source is now half that of the occluder, and they are vertically above one another with their centers aligned. (a) What is the shape of the umbra? Solution: Square (b) What is the shape of the outside boundary of the penumbra? Solution: This is quite a nasty question. Easiest way to construct the answer is to think about an arbitrary point on the occluder; construct a cone over the source, whose vertex is this point. Now intersect that cone with the plane — the resulting square region on the plane consists of all points such that this point on the occluder blocks some point on the source. Finally, take the union of all such regions (i.e. over all points on the occluder); that’s the penumbra. The envelope of the boundaries of these regions is the boundary of the penumbra. It’s a square. 2.6. A small sphere casts a shadow on a larger sphere. Describe the possible shadow boundaries that occur. Solution:

2.7.

2.8.

(a)

(b)

2.9.

The question is slightly poorly posed, mea culpa, because it doesn’t say what the source is. Assume it’s a point source. There are two interesting cases: the point source is on the line connecting the two sphere centers; or it’s off. If it’s on, then the shadow must be a circle. If it’s off, it’s the intersection of a sphere and a right circular cone. Explain why it is difficult to use shadow boundaries to infer shape, particularly if the shadow is cast onto a curved surface. _______________________________________________ Solution: As the previous exercise suggested, quite simple geometries lead to very complex shadows; it becomes hard to tell whether the shadow is complex because it was a simple shadow cone intersected with a complex surface, or because it was a complex shadow cone intersected with a simple surface. As in Figure 2.18, a small patch views an infinite plane at unit distance. The patch is sufficiently small that it reflects a trivial quantity of light onto the plane. The plane has radiosity B(x,y) = 1 + sin ax. The patch and the plane are parallel to one another. We move the patch around parallel to the plane, and consider its radiosity at various points. Show that if one translates the patch, its radiosity varies periodically with its position in x. Solution: If you translate the patch by (2n/a) units, it’s in the same position with respect to the radiosity pattern as it was; and the plane is infinite. Fix the patch’s center at (0, 0); determine a closed form expression for the radiosity of the patch at this point as a function of a. You’ll need a table of integrals for this (if you don’t, you’re entitled to feel very pleased with yourself). Solution: This is worked out in detail in (Haddon and Forsyth 1997) If one looks across a large bay in the daytime, it is often hard to distinguish the mountains on the opposite side; near sunset, they are clearly visible. This phenomenon has to do with scattering of light by air—a large volume of air is actually a source. Explain what is happening. We have modeled air as a

vacuum and asserted that no energy is lost along a straight line in a vacuum. Use your explanation to give an estimate of the kind of scales over which that model is acceptable. Solution: During the day, the sun illuminates the air, so the air between the viewer and the far side of the bay glows (from the light scattered into the viewing direction). This reduces the contrast of the stuff on the other side of the bay — the viewer sees a bright light superimposed on so can’t distinguish the edges of objects, etc. In the evening, the air does not glow, and so you can see the far side of the bay. Generally, you can think of air as a vacuum on scales up to kilometers; if you’re very lucky and the air is very clear, perhaps 100 km. 2.10. Read the book Colour and Light in Nature, by Lynch and Livingstone, published by Cambridge University Press, 1995. PROGRAMMING EXERCISES 2.11. An area source can be approximated as a grid of point sources. The weakness of this approximation is that the penumbra contains quantization errors, which can be quite offensive to the eye. (a) Explain. Solution: As you move along the penumbra, you see an integer number of point sources; at various points, one comes in or out and so there is a visible jump in the intensity. (b) Render this effect for a square source and a single occluder casting a shadow onto an infinite plane. For a fixed geometry, you should find that as the number of point sources goes up, the quantization error goes down. (c) This approximation has the unpleasant property that it is possible to produce arbitrarily large quantization errors with any finite grid by changing the geometry. This is because there are configurations of source and occluder that produce large penumbrae. Use a square source and a single occluder, casting a shadow onto an infinite plane, to explain this effect. Solution:

2.12.

2.13.

2.14.

2.15. (a)

(b)

(c)

The trick to this is to have the plane at an angle, so that the penumbra is stretched out. Make a world of black objects and another of white objects (paper, glue, and spraypaint are useful here) and observe the effects of interreflections. Can you come up with a criterion that reliably tells, from an image, which is which? (If you can, publish it; the problem looks easy, but isn’t.) Solution: Can’t help you here; I’ve been looking for a good criterion for absolute lightness for years, as the exercise suggests. (This exercise requires some knowledge of numerical analysis.) Do the numerical integrals required to reproduce Figure 2.18. These integrals aren’t particularly easy: if one uses coordinates on the infinite plane, the size of the domain is a nuisance; if one converts to coordinates on the view hemisphere of the patch, the frequency of the radiance becomes infinite at the boundary of the hemisphere. The best way to estimate these integrals is using a Monte Carlo method on the hemisphere. You should use importance sampling because the boundary contributes rather less to the integral than the top does. Solution: It could help to look at (Haddon and Forsyth 1997) Set up and solve the linear equations for an interreflection solution for the interior of a cube with a small square source in the center of the ceiling. Implement a photometric stereo system. How accurate are its measurements (i.e., how well do they compare with known shape information)? Do interreflections affect the accuracy? How repeatable are its measurements (i.e., if you obtain another set of images, perhaps under different illuminants, and recover shape from those, how does the new shape compare with the old)? Compare the minimization approach to reconstruction with the integration approach; which is more accurate or more repeatable and why? Does this difference appear in experiment?

(d)

One possible way to improve the integration approach is to obtain depths by integrating over many different paths and then average these depths (you need to be a little careful about constants here). Does this improve the accuracy or repeatability of the method?

3 CHAPTER Color PROBLEMS 3.1. Sit down with a friend and a packet of colored papers, and compare the color names that you use. You need a large packet of papers—one can very often get collections of colored swatches for paint, or for the Pantone color system very cheaply. The best names to try are basic color names—the terms red, pink, orange, yellow, green, blue, purple, brown, white, gray and black, which (with a small number of other terms) have remarkable canonical properties that apply widely across different languages (the papers in Hardin and Maffi (1997) give a good summary of current thought on this issue). You will find it surprisingly easy to disagree on which colors should be called blue and which green, for example. Solution: This one is really worth doing. In my experience, quite substantial disagreements appear, and you won’t get a sense of this without trying it. 3.2. Derive the equations for transforming from RGB to CIE XYZ and back. This is a linear transformation. It is sufficient to write out the expressions for the elements of the linear transformation—you don’t have to look up the actual numerical values of the color matching functions. Solution: Write R(A) for the R primary, G(A) for the green primary, B(A) for the B primary. A color E(A) has RGB coordinates r,g,b if it matches rR(A) + gG(A) + bB(A). Write 0x(A) for the colormatching function for the X primary, (A) for the colormatching function for the Y primary, and (A) for the colormatching function for the Z primary. Then rR(A) + gG(A) + bB(A) will have X coordinate J(rR(A) + gG(A) + bB(A))0 x(A)dA. By this reasoning, x f R(A)0x(A)dA f G(A)0x(A)dA f B(A)0x(A)dA r \ y = f R(A)0y(A)dA f G(A)0y(A)dA f B(A)0y(A)dA g z R(A)0z(A)dA / G(A)0z(A)dA / B(A)0z(A)dA b )

and this works the other way round if one swaps R(A) for X(A), etc. and 0x(A) for 0r(A). 3.3. Linear color spaces are obtained by choosing primaries and then constructing color matching functions for those primaries. Show that there is a linear transformation that takes the coordinates of a color in one linear color space to those in another; the easiest way to do this is to write out the transformation in terms of the color matching functions. Solution: Take the result of the previous exercise; now use the primaries of the first color space and the color matching functions of the second. 6 3.4. Exercise 3 means that, in setting up a linear color space, it is possible to choose primaries arbitrarily, but there are constraints on the choice of color matching functions. Why? What are these constraints? Solution: When you choose colormatching functions, the new ones must be a linear combination of the colormatching functions for any other linear color space. For example, think of RGB and XYZ. The r coordinate of a color matching some E(A) is obtained by forming J 0 r(A)E(A)dA; it can also be obtained as a linear combination of the X, Y, and Z coordinates (as above). This is true for any E(A), and so means that 0 r(A) is a linear combination of (A), (A), and (A). 3.5. Two surfaces that have the same color under one light and different colors under another are often referred to as metamers. An optimal color is a spectral reflectance or radiance that has value 0 at some wavelengths and 1 at others. Although optimal colors donâ€™t occur in practice, they are a useful device (due to Ostwald) for explaining various effects. (a) Use optimal colors to explain how metamerism occurs. Solution: For example, mixing red and green light gets yellow. So if we have one surface albedo that is zero everywhere except in the yellow range, and

(b)

(c)

(d)

3.6.

another that is zero except in green and red, the two surfaces will look the same (yellow) in white light. But now if we obtain a light that is zero in the red range, one surface will look yellow and the other will look green. Given a particular spectral albedo, show that there are an infinite number of metameric spectral albedoes. Solution: Assume we have illumination that is uniform over albedo (white). Now this spectral albedo reflects some color of light. Choose three distinct wavelengths (say, the RGB primaries) as primaries, and determine the weights for these primaries to match the reflected light. You can then build an albedo that matches by setting the albedo to these weights at the chosen wavelengths, and zero elsewhere. There is clearly an infinite number, even though for some triples the construction will fail because subtractive matching applies. Use optimal colors to construct an example of surfaces that look different under one light (say, red and green) and the same under another. Solution: See the solution to the question before the last. Use optimal colors to construct an example of surfaces that swop apparent color when the light is changed (i.e., surface one looks red and surface two looks green under light one, and surface one looks green and surface two looks red under light two). Solution: Apply the strategy of the solution to the question before the last. You have to map the gamut for a printer to that of a monitor. There are colors in each gamut that do not appear in the other. Given a monitor color that canâ€™t be reproduced exactly, you could choose the printer color that is closest. Why is this a bad idea for reproducing images? Would it work for reproducing â€œbusiness graphicsâ€? (bar charts, pie charts, and the like, which all consist of many differernt large blocks of a single color)? Solution: The closest color might be saturated, so would produce very unpleasant effects on smooth

3.7.

3.8.

3.9.

(b)

(c)

color gradients. Business graphics use saturated colors anyhow, and don’t use color gradients. Volume color is a phenomenon associated with translucent materials that are colored—the most attractive example is a glass of wine. The coloring comes from different absorption coefficients at different wavelengths. Explain (a) why a small glass of sufficiently deeply colored red wine (a good Cahors or Gigondas) looks black (b) why a big glass of lightly colored red wine also looks black. Experimental work is optional. Solution: (a) it absorbs all the light; absorption is exponential in distance. (b) Again, absorption is exponential in distance, so if the distance is long enough, all light will be absorbed. Read the book Colour: Art and Science, by Lamb and Bourriau, Cambridge University Press, 1995. In section 3.5.3, we described the gamut as a possible cue to illuminant color. Write G for the convex hull of the gamut of the given image, W for the convex hull of the gamut of an image of many different surfaces under white light, and Me for the map that takes an image seen under illuminant e to an image seen under white light. (a) Show the only illuminants we need to consider are those such that Me(G) £ W. ______________________________________________________________ ___________________ Solution: Because any other map produces a color we would not see under white light. Show that, for the case of finite dimensional linear models, Me depends linearly on e. Solution: This is a typographic error. In fact, the map from white light to the image under e depends linearly on e. Show that, for the case of finite dimensional linear models, the set of M e such that Me(G) £ W is convex.

Solution: Write S for the set of Me such that Me(G) £ W. The maps are linear and the image is convex; so if M £ S and N £ S, (tM + (1 — t)N) £ S for 0 < t < 1. This means S is convex. (d) How would you represent this set? Solution: There are a variety of ways to do this. The usual thing is to note that the maps are diagonal, so the convex set is three dimensional, and then use an octtree to get an approximate representation. Other methods are described in (Forsyth 1990). PROGRAMMING EXERCISES 3.10. Spectra for illuminants and for surfaces are available on the web (try http: //www. it. lut. fi/ip/research/color/database/database .html). Fit a finite-dimensional linear model to a set of illuminants and surface reflectances using principal components analysis, render the resulting models, and compare your rendering with an exact rendering. Where do you get the most significant errors? Why? Solution: The most significant errors tend to be under fluourescent light sources, which are hard to model well with finite dimensional linear models. 3.11. Print a colored image on a color inkjet printer using different papers and compare the result. It is particularly informative to (a) ensure that the driver knows what paper the printer will be printing on, and compare the variations in colors (which are ideally imperceptible), and (b) deceive the driver about what paper it is printing on (i.e., print on plain paper and tell the driver it is printing on photographic paper). Can you explain the variations you see? Why is photographic paper glossy? Solution: It’s glossy because that means it reflects more light in the view direction if you hold it right; in turn, as long as it isn’t too specular, it looks like a bright diffuse surface, and you get better contrast in prints.

3.12. Fitting a finite-dimensional linear model to illuminants and reflectances separately is somewhat ill-advised because there is no guarantee that the interactions will be represented well (theyâ€™re not accounted for in the fitting error). It turns out that one can obtain g^ by a fitting process that sidesteps the use of basis functions. Implement this procedure (which is described in detail in Marimont and Wandell (1992)), and compare the results with those obtained from the previous assignment. 3.13. Build a color constancy algorithm that uses the assumption that the spatial average of reflectance is constant. Use finite-dimensional linear models. You can get values of gj from your solution to the previous exercise. 3.14. We ignore color interreflections in our surface color model. Do an experiment to get some idea of the size of color shifts possible from color interreflections (which are astonishingly big). Humans seldom interpret color interreflections as surface color. Speculate as to why this might be the case, using the discussion of the lightness algorithm as a guide. 3.15. Build a specularity finder along the lines described in Section 3.5.1. 3.16. Build a shadow remover along the lines described in Section 3.5.2 (this is much easier than it sounds, and the results are usually rather good).

link full download https://bit.ly/2IsFW8n Language: English ISBN-10: 013608592X ISBN-13: 978-0136085928 ISBN-13: 9780136085928 People Also...

Published on Apr 16, 2019

link full download https://bit.ly/2IsFW8n Language: English ISBN-10: 013608592X ISBN-13: 978-0136085928 ISBN-13: 9780136085928 People Also...

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