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Radiometry Sung-Eui Yoon ( ) ( ) C Course URL: URL - PowerPoint PPT Presentation

CS680: CS680: Radiometry Sung-Eui Yoon ( ) ( ) C Course URL: URL http://jupiter.kaist.ac.kr/~sungeui/SGA/ Announcements Announcements 2 papers for each student 2 papers for each student Choose 4 papers from the


  1. CS680: CS680: Radiometry Sung-Eui Yoon ( 윤성의 ) ( 윤성의 ) C Course URL: URL http://jupiter.kaist.ac.kr/~sungeui/SGA/

  2. Announcements Announcements ● 2 papers for each student 2 papers for each student ● Choose 4 papers from the paper list ● Send them (titles of 4 papers) to TA (Bochang ● Send them (titles of 4 papers) to TA (Bochang Moon) by Oct-11 (Mon) ● Look at videos and talk files (captured talk Look at videos and talk files (captured talk video or presentation files) ● Schedule of student presentations ● Will be decided on Oct-12 (Tue) ( ) ● Presentations will start after the mid-term 2

  3. Motivation Motivation Eye ??? 3

  4. Light and Material Interactions Light and Material Interactions ● Physics of light Physics of light ● Radiometry ● Material properties From kavita’s slides ● Rendering equation 4

  5. Models of Light Models of Light ● Quantum optics Quantum optics ● Fundamental model of the light ● Explain the dual wave particle nature of light ● Explain the dual wave-particle nature of light ● Wave model ● Simplified quantum optics ● Simplified quantum optics ● Explains diffraction, interference, and polarization polarization ● Geometric optics Geometric optics ● Most commonly used model in CG ● Size of objects >> wavelength of light j g g ● Light is emitted, reflected, and transmitted 5

  6. Radiometry Radiometry ● Measurement of light energy Measurement of light energy ● Critical component for photo-realistic rendering ● Light energy flows through space ● Varies with time position and direction ● Varies with time, position, and direction ● Radiometric quantities ● Radiometric quantities ● Densities of energy at particular places in time, space, and direction space, and direction ● Photometry Photometry ● Quantify the perception of light energy 6

  7. Hemispheres Hemispheres ● Hemisphere Hemisphere ● Two-dimensional surfaces ● Direction Direction ● Point on (unit) sphere From kavita’s slides 7

  8. Solid Angles Solid Angles 2D 2D 3D 3D Full circle Full circle F ll Full sphere h = 2pi radians = 4pi steradians 8

  9. Solid Angles Solid Angles 2D 2D 3D 3D Full circle Full sphere = 2pi radians 2pi radians = 4pi steradians = 4pi steradians 9

  10. Hemispherical Coordinates Hemispherical Coordinates Direction   ● Direction, ● Point on (unit) sphere From kavita’s slides 10

  11. Hemispherical Coordinates Hemispherical Coordinates ● Differential solid angle Differential solid angle 11

  12. Hemispherical Integration Hemispherical Integration ● Area of hemispehre: Area of hemispehre: 12

  13. Energy Energy ● Symbol: Q Symbol: Q ● # of photons in this context ● Unit: Joules ● Unit: Joules From Steve Marschner’s talk 13

  14. Power (or Flux) Power (or Flux) ● Symbol, P or Φ Symbol P or Φ ● Total amount of energy through a surface per unit time dQ/dt unit time, dQ/dt ● Radiant flux in this context ● Unit: Watts (=Joules / sec.) Unit: Watts ( Joules / sec.) ● Other quantities are derivatives of P ● Example ● A light source emits 50 ● A light source emits 50 watts of radiant power ● 20 watts of radiant power is p incident on a table 14

  15. Irradiance Irradiance ● Incident radiant power per unit Incident radiant power per unit area (dP/dA) ● Area density of power ● Area density of power ● Symbol: E unit: W/ m 2 ● Symbol: E, unit: W/ m ● Area power density existing a surface is called radiance exitance (M) or radiosity (B) ● For example ● A light source emitting 100 W of area 0.1 m 2 0 1 2 ● Its radiant exitance is 1000 W/ m 2 15

  16. Irradiance Example Irradiance Example ● Uniform point source illuminates a small Uniform point source illuminates a small surface dA from a distance r ● Power P is uniformly spread over the area of ● Power P is uniformly spread over the area of the sphere 16

  17. Irradiance Example Irradiance Example ● Uniform point source illuminates a small Uniform point source illuminates a small surface dA from a distance r ● Power P is uniformly spread over the area of ● Power P is uniformly spread over the area of the sphere θ 17

  18. Radiance Radiance ● Radiant power at x in direction θ Radiant power at x in direction θ : 5D function   ● L x ( ) ● Per unit area ● Per unit area ● Per unit solid angle ● Important quantity for rendering 18

  19. Radiance Radiance ● Radiant power at x in direction θ Radiant power at x in direction θ : 5D function   ● L x ( ) ● Per unit area ● Per unit area ● Per unit solid angle ● Units: Watt / (m 2 sr) ● Irradiance per unit solid angle ● 2 nd derivative of P ● Most commonly used term 19

  20. Radiance: Projected Area Radiance: Projected Area 2 d P      d d dA dA cos cos  ● Why per unit projected surface area y p p j 20

  21. Properties of Radiance Properties of Radiance ● Invariant along a straight line (in vacuum) Invariant along a straight line (in vacuum) From kavita’s slides 21

  22. Invariance of Radiance Invariance of Radiance W We can prove it based it b d on the assumption the conservation of energy conservation of energy. 22

  23. Sensitivity to Radiance Sensitivity to Radiance ● Responses of sensors (camera, human eye) Responses of sensors (camera human eye) is proportional to radiance From kavita’s slides ● Pixel values in image proportional to radiance received from that direction di i d f h di i 23

  24. Relationships Relationships ● Radiance is the fundamental quantity Radiance is the fundamental quantity ● Power: ● Radiosity: ● Radiosity: 24

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  33. Light and Material Interactions Light and Material Interactions ● Physics of light Physics of light ● Radiometry ● Material properties From kavita’s slides ● Rendering equation 33

  34. Materials Materials Ideal diffuse (Lambertian) Ideal specular Glossy Glossy From kavita’s slides 34

  35. Bidirectional Reflectance Distribution Function (BRDF) Distribution Function (BRDF) 35

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  39. Homework Homework 39

  40. Next Time Next Time ● Rendering equation Rendering equation 40

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