The Light Field
Light field = radiance function on rays Surface and field radiance Conservation of radiance Measurement Irradiance from area sources Measuring rays Form factors and throughput Conservation of throughput
From London and Upton
CS348B Lecture 5 Pat Hanrahan, 2004
Light Field = Radiance(Ray)
Page 1 Incident Surface Radiance
Definition: The incoming surface radiance (luminance) is the power per unit solid angle per unit projected area arriving at a receiving surface dω dA dx2Φ (,ω ) Lx(,ω )≡ i i ddAωi
CS348B Lecture 5 Pat Hanrahan, 2004
Exitant Surface Radiance
Definition: The outgoing surface radiance (luminance) is the power per unit solid angle per unit projected area leaving at surface dω dA dx2Φ (,ω ) Lx(,ω )≡ o o ddAωi
Alternatively: the intensity per unit projected area leaving a surface
CS348B Lecture 5 Pat Hanrahan, 2004
Page 2 Field Radiance
Definition: The field radiance (luminance) at a point in space in a given direction is the power per unit solid angle per unit area perpendicular to the direction
dω dA Lx(,ω )
CS348B Lecture 5 Pat Hanrahan, 2004
Environment Maps
L(,θ ϕ )
Miller and Hoffman, 1984
CS348B Lecture 5 Pat Hanrahan, 2004
Page 3 Spherical Gantry ⇒ Light Field
Lxy(,,,θ ϕ ) (,θ ϕ )
Capture all the light leaving an object - like a hologram
CS348B Lecture 5 Pat Hanrahan, 2004
Two-Plane Light Field
2D Array of Cameras 2D Array of Images L(,,,)uvst CS348B Lecture 5 Pat Hanrahan, 2004
Page 4 Multi-Camera Array ⇒ Light Field
CS348B Lecture 5 Pat Hanrahan, 2004
Properties of Radiance
Page 5 Properties of Radiance
1. Fundamental field quantity that characterizes the distribution of light in an environment. ∴ Radiance is a function on rays ∴ All other field quantities are derived from it 2. Radiance invariant along a ray. ∴ 5D ray space reduces to 4D 3. Response of a sensor proportional to radiance.
CS348B Lecture 5 Pat Hanrahan, 2004
1st Law: Conversation of Radiance
The radiance in the direction of a light ray remains constant as the ray propagates
2 2 22 d Φ1 d Φ2 ddΦ12=Φ
dA1 dω1 2 L1 dLddAΦ=1111ω
dω2 dA2 2 L2 dLddAΦ=2222ω r dA dA ddAωω==12 ddA 11r 2 2 2
∴L12= L
CS348B Lecture 5 Pat Hanrahan, 2004
Page 6 Radiance: 2nd Law
The response of a sensor is proportional to the radiance of the surface visible to the sensor.
Ω Aperture A Sensor
RLddALT==∫∫ ω TddA= ∫∫ ω A Ω A Ω
L is what should be computed and displayed. T quantifies the gathering power of the device.
CS348B Lecture 5 Pat Hanrahan, 2004
Quiz
Does the brightness that a wall appears to the sensor depend on the distance?
No!! CS348B Lecture 5 Pat Hanrahan, 2004
Page 7 Irradiance from a Uniform Surface Source
Irradiance from the Environment
2 dxΦ=ii(,ω ) Lx (,ωθ )cos dAd ω Lxi (,ω ) dE( x ,ω )= Li ( x ,ωθω )cos d dω θ
dA E()xLxd= (,ω )cosθω ∫ i H2 CS348B Lecture 5 Pat Hanrahan, 2004
Page 8 Irradiance from an Area Source
A
E()xLd= ∫ cosθ ω H2 Ω = Ld∫cosθ ω Ω =ΩL Ω
CS348B Lecture 5 Pat Hanrahan, 2004
Projected Solid Angle
dω θ
cosθ dω ∫ cosθ dωπ= H2 CS348B Lecture 5 Pat Hanrahan, 2004
Page 9 Uniform Disk Source
Geometric Derivation Algebraic Derivation cosαπ 2 r Ω= ∫∫cosθφdd cosθ 10 cosα α cos2 θ = 2π 2 h 1 = παsin2 sinα r 2 = π rh22+ Ω= π sin2 α
CS348B Lecture 5 Pat Hanrahan, 2004
Spherical Source
Geometric Derivation Algebraic Derivation
r Ω= ∫ cosθ dω R = π sin2 α α r 2 = π R2
Ω= π sin2 α CS348B Lecture 5 Pat Hanrahan, 2004
Page 10 The Sun
Solar constant (normal incidence at zenith) Irradiance 1353 W/m2 Illuminance 127,500 lm/m2 = 127.5 kilolux Solar angle α = .25 degrees = .004 radians (half angle) 22 Ω= π sin απα ≈ = 6 x 10-5 steradians Solar radiance EWm1.353× 1032 / W L == =2.25 × 107 Ω× 610−52sr m ⋅ sr
CS348B Lecture 5 Pat Hanrahan, 2004
Polygonal Source
CS348B Lecture 5 Pat Hanrahan, 2004
Page 11 Polygonal Source
CS348B Lecture 5 Pat Hanrahan, 2004
Polygonal Source
CS348B Lecture 5 Pat Hanrahan, 2004
Page 12 Lambert’s Formula