Illumination and Shading


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1 Illumination and Shading Computer Graphics COMP 770 (236) Spring 2007 Instructor: Brandon Lloyd 2/14/07 1
2 From last time Texture mapping overview notation wrapping Perspectivecorrect interpolation Texture filtering Bilinear interpolation MIP maps Summedarea tables 2/14/07 2
3 Topics for today Light Sources Empirical Illumination Shading Local vs Global Illumination 2/14/07 3
4 Illumination Models Computer Graphics Jargon: Illumination  the transport luminous flux from light sources between surfaces via direct and indirect paths Lighting  the process of computing the luminous intensity reflected from a specified 3D point Shading  the process of assigning a colors to a pixels Illumination Models: Empirical  simple formulations that approximate observed phenomenon Physicallybased  models based on the actual physics of light's interactions with matter 2/14/07 4
5 Two components of illumination Light Sources: Emittance spectrum (color) Geometry (position and direction) Directional attenuation Surface Properties: Reflectance spectrum (color) Geometry (position, orientation, and microstructure) Absorption Simplifications used by most computer graphics systems: Compute only direct illumination from the emitters to the reflectors of the scene Ignore the geometry of light emitters, and consider only the geometry of reflectors 2/14/07 5
6 Ambient light source Ambient light sources are a simple hack for indirect illumination Incoming ambient illumination (I i,a ) is constant for all surfaces in the scene Reflected ambient illumination (I r,a ) depends only on the surface s ambient reflection coefficient (k a ) and not its position or orientation I r,a = k I a i,a These quantities typically specified as (R, G, B) triples 2/14/07 6
7 Point light sources Point light sources emit rays from a single point a fair approximation to a local light source such as a light bulb The direction to the light changes across the surface p l ˆL = p p p p l l ˆL p 2/14/07 7
8 Directional light sources Light rays are parallel and have no origin Can be considered as a point light at infinity A good approximation for sunlight The direction to the light source is constant over the surface ˆL 2/14/07 8
9 Lights in OpenGL Light positions are specified in homogeneous coordinates They are transformed by the current modelview matrix Directional light sources have w=0 # define a directional light lightdirection = [1, 1, 1, 0] gllightfv(gl_light0, GL_POSITION, lightdirection) glenable(gl_light0) # define a point light lightpoint = [100, 100, 100, 1] gllightfv(gl_light1, GL_POSITION, lightpoint) glenable(gl_light1) # set up light s color gllightfv(gl_light0, GL_AMBIENT, ambientintensity) gllightfv(gl_light0, GL_DIFFUSE, diffuseintensity) gllightfv(gl_light0, GL_SPECULAR, specularintensity) 2/14/07 9
10 Other light sources Spotlights point source whose intensity falls off away from a given direction Area Light Sources occupies a 2D area (e.g. a polygon or a disk) generates soft shadows Extended Light Sources occupies a 3D area (e.g. a sphere) generates soft shadows Area and extended often used interchangeably 2/14/07 10
11 Ideal diffuse reflection Ideal diffuse reflectors very rough at the microscopic level microscopic variations in the surface make any direction over the hemisphere equally likely to be the reflected direction of an incoming light ray reflection is viewindependent follow Lambert s cosine law Chalk is a good approximation to an ideal diffuse surface 2/14/07 11
12 Lambert s cosine law Lambert s cosine law : the reflected energy from a small surface area from illumination arriving from direction ˆL is proportional to the cosine of the angle between ˆL and the surface normal ˆN Ir Iicosθ θ ˆL I(Nˆ L) ˆ i 2/14/07 12
13 Computing diffuse reflection Constant of proportionality depends on surface properties I = k I(Nˆ L) ˆ r,d The constant k d specifies how much of the incident light I i is diffusely reflected When (Nˆ L) ˆ < 0 the incident light is blocked by the surface itself and the diffuse reflection is 0 d i diffuse reflection for varying light 2/14/07 13
14 Specular reflection Specular reflectors have a bright, view dependent highlight examples polished metal, glossy car finish, a mirror at the microscopic level a specular reflecting surface is very smooth Specular reflection obeys Snell s law: The incoming ray, the surface normal, and the reflected ray all lie in a common plane. The relationship between the angles of the incoming and reflected rays with the normal is given by: nsinθ = n sinθ i i o o ˆL θ i ˆN θ o ˆR n i and n o are the indices of refraction for the incoming and outgoing ray, respectively Reflection is a special case where n i = n o so θ o = θ i 2/14/07 14
15 Computing the reflection vector The vector R can be computed from the incoming light direction and the surface normal as shown below. Rˆ = (2(Nˆ Lˆ))Nˆ Lˆ The diagram below illustrates this relationship. ˆL ˆN ˆR 2(Nˆ L)N ˆ ˆ 2/14/07 15 ˆL
16 Nonideal reflectors Snell s law applies only to ideal specular reflectors Real materials have microscopic surface variations that cause some of the light to be reflected in directions slightly offset from the the ideal reflected ray Causes highlight to spread out according to roughness Empirical models try to simulate the appearance of this effect, without trying to capture the physics of it ˆL ˆN ˆR 2/14/07 16
17 Phong illumination The Phong model is an empirical model one of the most commonly used illumination models in computer graphics has no physical basis I = k I(cos φ) r,s s i = ki(vˆ R) ˆ si n s n s ˆL ˆN ˆV φ ˆR (V) ˆ is the direction to the viewer (Vˆ R) ˆ is clamped to [0,1] The specular exponent n s controls how quickly the highlight falls off 2/14/07 17
18 Effect of specular exponent How the shape of the highlight changes with varying n s 2/14/07 18
19 Phong examples varying light direction varying specular exponent 2/14/07 19
20 Blinn & Torrance variation Jim Blinn introduced another approach for computing Phonglike illumination based on the work of Ken Torrance: I = k I(Nˆ H) ˆ r,s s i Lˆ Ĥ = Lˆ + Vˆ + Vˆ n s ˆL ˆN Ĥ ˆV Ĥis the halfway vector that bisects the light and viewer directions 2/14/07 20
21 Putting it all together numlights ( ˆ ˆ ˆ ˆ n ) I = k I + I k (N L ) + k (V R ) r a a i,j d j s j j= 1 s 2/14/07 21
22 OpenGL surface properties glmaterialfv(gl_front, GL_AMBIENT, ambientcolor) glmaterialfv(gl_front, GL_DIFFUSE, diffusecolor) glmaterialfv(gl_front, GL_SPECULAR, specularcolor) glmaterialfv(gl_front, GL_SHININESS, nshininess) 2/14/07 22
23 Where do we Illuminate? Illumination can be expensive requires computation and normalizing of vectors for multiple light sources Compute illumination for faces Use face normal If the light is directional then the diffuse contribution is constant across the facet If the eye is infinitely far away and the light is directional then the specular contribution is constant across the facet Compute illumination for vertices Use vertex normals. interpolate illumination across face Compute illumination at each pixel most accurate and expensive interpolate normal across face 2/14/07 23
24 Flat shading The simplest shading method applies only one illumination calculation per face called constant or flat shading Issues: For point light sources the light direction varies over the face For specular reflections the viewer direction varies over the facet Illumination usually computed at the centroid of the face: n 1 centroid = p n i = 1 i 2/14/07 24
25 Need for vertex normals Even when the illumination equation is applied at each pixel, the polygonal nature of the model is still apparent. To overcome this limitation normals are introduced at each vertex. Usually different than the polygon normal Used only for shading (not backface culling or other geometric computations) Better approximates the "real" surface 2/14/07 25
26 Vertex normals If vertex normals are not provided they can often be approximated by averaging the normals of the facets which share the vertex. n v This only works if the polygons reasonably approximate the underlying surface. k = n i= 1 face,i A better approximation can be found using a clustering analysis of the normals on the unit sphere. 2/14/07 26
27 Gouraud shading Gouraud shading applies the illumination model on a subset of surface points and interpolates the intensity of the remaining points on the surface. For a polygonal mesh the illumination model is usually applied at each vertex and linearly interpolated over the polygons Notice that facet artifacts are still visible. 2/14/07 27
28 Phong shading Phong shading (not to be confused with Phong s illumination model), the surface normal is linearly interpolated across polygonal facets, and the Illumination model is applied at every point. Phong shading will usually result in a very smooth appearance, however, evidence of the polygonal model can usually be seen along silhouettes. 2/14/07 28
29 Local illumination Local illumination models compute the colors of points on surfaces by considering only local properties the position of the point the surface properties the properties of any light sources that affect it No other objects in the scene are considered neither as light blockers nor as reflectors Typical of immediatemode renders, such as OpenGL 2/14/07 29
30 Global Illumination In the real world, light takes indirect paths Light reflects off of other materials (possibly multiple objects) Light is blocked by other objects Light can be scattered Light can be focused Light can bend Harder to model At each point we must consider not only every light source, but and other point that might have reflected light toward it 2/14/07 30
31 Next time Illumination and shading physicallybased models 2/14/07 31
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