1. Rendering theory & practice

2. Introduction  We’ve looked at modelling, surfacing and animating.  The final stage is rendering.  This can be the most time consuming part of the process depending on the complexity of you scene.  Many people underestimate the time needed But you won’t of course!

3. Some basic things to remember  Render to frame files rather than movie files  Use file formats that use no compression or loss-less compression  Use anti-aliasing (within reason)  Don’t raytrace if you can avoid it!

6. Simple shading  We’ve already considered this in the simplest sense: Flat, Gouraud and Phong shading  None of these consider inter-face reflections or shadows.  We need these for visual realism.  For these we need global illumination algorithms

7. Global illumination  This simulates the interaction of light with the entire environment rather than individual surfaces.  Light is tracked from emitters to sensors.  Shadows are automatically generated, as are interactions between surfaces.  There are two common approaches: ray tracing and radiosity  Before we look at these in detail, we should look at some general features of global illumination

8. Global illumination (2)  Ignoring the fact that the calculations (as we shall see later) are complex, the solution to global illumination is simple:  Start at a light source  Trace every light path through the environment it either: * hits the eye point * has its energy reduced below a threshold * travels out of the environment

9. A first attempt: the rendering equation where I(x,x’) is the transport intensity g(x, x') is the visibility function  (x, x') transfer emittance  (x, x', x'') is the scattering term  Describes what happens at point x on a surface due to light travelling from it

10. Another attempt: surface-surface interactions  We can also model the way one surface interacts with another  This is easier to consider non-mathematically  Four different interactions: diffuse to diffuse specular to diffuse diffuse to specular specular to specular

11. Mechanisms of light transport Diffuse to diffuseSpecular to diffuse Specular to specularDiffuse to specular

12. Mechanisms of light transport (2)  Specular-specular transfer can be calculated using ray-tracing  Diffuse-diffuse transfer can be calculated using radiosity  Specular-diffuse and diffuse-specular need a combination  We can categorise the type of transfer so that we know how to handle a given situation

13. Categories of light transfer  Light-Diffuse-Diffuse-Eye (LDDE)  Light-Specular-Diffuse-Eye (LSDE)  Light-Diffuse-Specular-Eye (LDSE)  Light-Specular-Specular-Eye (LSSE) ……

14. Examples of light transfer

15. Ray tracing Initial ray Transmitted ray Reflected ray Transmitted ray Eye Initial ray Transmitted ray Reflected ray

16. Including a local model

17. A classic ray-traced scene 1 2 3 4 5 6 7

18. 1 2 3 4 5 6 7 1 2 3 4 5 6 7

20. Radiosity  This implements diffuse-diffuse transfer.  Instead of following individual rays, interaction between patches in a scene are considered.  This is different from other global illumination algorithms in two important ways: * the solution is view independent * the scene must be divided into patches

21. Radiosity (2)  Consider a light source as an array of emitting patches  Light is shot from these into the scene and we consider the diffuse-diffuse interaction between the light patch and the first hit patch  The energy arriving at the hit patch is then re- emitted according to the surface properties, hitting other patches…  This process iterates until there are no further significant changes in energy distribution

22. Radiosity example 20 250 5000