Ray tracing (graphics)

related topics
{math, energy, light}
{system, computer, user}
{math, number, function}
{film, series, show}
{@card@, make, design}
{car, race, vehicle}
{war, force, army}
{style, bgcolor, rowspan}

In computer graphics, ray tracing is a technique for generating an image by tracing the path of light through pixels in an image plane and simulating the effects of its encounters with virtual objects. The technique is capable of producing a very high degree of visual realism, usually higher than that of typical scanline rendering methods, but at a greater computational cost. This makes ray tracing best suited for applications where the image can be rendered slowly ahead of time, such as in still images and film and television special effects, and more poorly suited for real-time applications like computer games where speed is critical. Ray tracing is capable of simulating a wide variety of optical effects, such as reflection and refraction, scattering, and chromatic aberration.

Contents

Algorithm overview

Optical ray tracing describes a method for producing visual images constructed in 3D computer graphics environments, with more photorealism than either ray casting or scanline rendering techniques. It works by tracing a path from an imaginary eye through each pixel in a virtual screen, and calculating the color of the object visible through it.

Scenes in raytracing are described mathematically by a programmer or by a visual artist (typically using intermediary tools). Scenes may also incorporate data from images and models captured by means such as digital photography.

Typically, each ray must be tested for intersection with some subset of all the objects in the scene. Once the nearest object has been identified, the algorithm will estimate the incoming light at the point of intersection, examine the material properties of the object, and combine this information to calculate the final color of the pixel. Certain illumination algorithms and reflective or translucent materials may require more rays to be re-cast into the scene.

Full article ▸

related documents
Radio telescope
Plasma stability
Rendering (computer graphics)
Superconducting magnetic energy storage
High Frequency Active Auroral Research Program
Electrometer
Geomagnetic storm
Attenuation
Maxwell–Boltzmann distribution
Olbers' paradox
Optical isolator
Thermistor
Capacitance
Optics
Metrology
Rayleigh scattering
Very Large Telescope
Gravitational constant
Resonance
Proton decay
2 Pallas
Weak interaction
Star formation
Gravitational singularity
Potential flow
Near-Earth asteroid
Weight
Ganymede (moon)
Terrestrial planet
Hydrogen atom