Measuring Light: Radiometry and Cameras

Transcription

1 Lecture 11: Measuring Light: Radiometry and Cameras Computer Graphics CMU /15-662, Fall 2015 Slides credit: a majority of these slides were created by Matt Pharr and Pat Hanrahan

2 Simulating a pinhole camera Imprecise statements you ve heard me say so far in this class: What is the color of the surface visible at each sample point? How much light arrives at sensor point through pinhole? 8-pixel pinhole camera y H o, d 1 Pinhole x sensor o = H T d = H T 0.375H T

3 Radiometry System of units and measures for measuring illumination Geometric optics model of light - Photons travel in straight lines, represented by rays - Good approximation when wavelength << size of objects light interacts with - Doesn t model diffraction, interference,

4 Light is electromagnetic radiation that is visible to eye Image credit: Licensed under CC BY-SA 3.0 via Commons

5 Lights: what do they do? Physical process converts input energy into photons - Each photon carries a small amount of energy Over some amount of time, light fixture consumes some amount of energy, Joules - Some input energy is turned into heat, some into photons Energy of photons hitting an object ~ exposure - Film, sensors, sunburn, solar panels, Graphics: generally assume steady state process - Rate of energy consumption = power, Watts Cree 11 W LED light bulb ( 60 Watt incandescent replacement) (Joules/second)

6 Measuring illumination: radiant flux (power) Given a sensor, we can count how many photons reach it Sensor - Over a period of time, gives the power received by the sensor Given a light, consider counting the number of photons emitted by it - Over a period of time, gives the power emitted by the light Energy carried by a photon: Q = hc h

7 Measuring illumination: radiant flux (power) Flux: energy per unit time (Watts) received by the sensor (or emitted by Sensor the light) Q = lim!0 t = dq dt apple J s Time integral of flux is total radiant energy Z t1 Q = (t)dt t 0

8 Spectral power distribution Describes distribution of energy by wavelength Figure credit:

9 Measuring illumination: irradiance Flux: time density of energy Irradiance: area density of flux Given a sensor of with area A, we can consider the average flux over the entire sensor area: A Irradiance (E) is given by taking the limit of area at a single point on the sensor: A E(p) = lim!0 (p) A = d (p) da apple W m 2

10 Beam power in terms of irradiance Consider beam with flux incident on surface with area A E = A A = EA

11 Projected area Consider beam with flux incident on angled surface with area A A A 0 A = A 0 cos A = projected area of surface relative to direction of beam

12 Lambert s Law Irradiance at surface is proportional to cosine of angle between light direction and surface normal. A A 0 A = A 0 cos E = A 0 = cos A

13 Why do we have seasons? Sun Summer (Northern hemisphere) Winter (Northern hemisphere) Earth s axis of rotation: ~23.5 off axis [Image credit: Pearson Prentice Hall]

14 Irradiance falloff with distance Assume light is emitting flux in a uniform angular distribution r 2 Compare irradiance at surface r 1 of two spheres: E 1 = 4 r 2 1! =4 r 2 1E 1 E 2 = 4 r 2 2! =4 r 2 2E 2 E 2 E 1 = r2 1 r 2 2

15 Angles and solid angles Angle: ratio of subtended arc length on circle to radius - = l r - Circle has 2 radians r l Solid angle: ratio of subtended area on sphere to radius squared - = A r 2 - Sphere has 4 steradians r A

16 Solid angles in practice Sun and moon both subtend ~60µ sr as seen from earth Surface area of earth: ~510M km 2 Projected area: 510Mkm 2 60µsr 4 sr = km 2

17 Differential solid angle da =(r d )(r sin d ) =r 2 sin d d d! = da r 2 =sin d d

18 Differential solid angle Z Z = d! S 2 Z Z Z 2 Z = Z 0 Z 0 sin d d =4

19 ! as a direction vector! Will use! to donate a direction vector (unit length)

20 Measuring illumination: radiance Radiance is the solid angle density of irradiance L(p,!) = lim!0 E! (p)! = de!(p) d! apple W m 2 sr where denotes that the differential surface area is E!! oriented to face in the direction da d! In other words, radiance is energy along a ray defined by origin point p and direction!

21 Radiance functions Equivalently, L(p,!) = de(p) d! cos = d2 (p) da d! cos Previous slide described measuring radiance at a surface oriented in ray direction - cos(theta) accounts for different surface orientation d! da

22 Field radiance: the light field Light field = radiance function on rays Radiance is constant along rays * Spherical gantry: captures 4D light field (all light leaving object) L(x, y,, ) (, ) * in a vacuum

23 Surface radiance Need to distinguish between incident radiance and exitant radiance functions at a point on a surface L i (p 1,! 1 ) L o (p 2,! 2 ) (p 1 p 2, In general: L i (p,!) 6= L o (p,!)

24 Properties of radiance Radiance is a fundamental field quantity that characterizes the distribution of light in an environment - Radiance is the quantity associated with a ray - Rendering is all about computing radiance Radiance is invariant along a ray in a vacuum A pinhole camera measures radiance

25 Irradiance from the environment Computing flux per unit area on surface, due to incoming light from all directions. de(p,!) =L i (p,!) cos d! Z Contribution to irradiance from light arriving from direction! E(p,!) = H 2 L i (p,!) cos d! d! Light meter da

26 Simple case: irradiance from uniform hemispherical source E(p) = Z = L H 2 L d! Z 2 0 Z 2 0 cos sin d d = L d! da

27 Irradiance from a uniform area source (source emits radiance L) Z E(p) = L(p,!) cos d! HZ 2 O =L =L? cos d! Projected solid angle:? - Cosine-weighted solid angle - Area of object O projected onto unit d!? = cos d! sphere, then projected onto plane

28 Uniform disk source (oriented perpendicular to plane) Geometric Derivation Algebraic Derivation (using projected solid angle) Z 2 Z? = 0 0 =2 sin2 2 cos sin d d 0 = sin 2 sin? = sin 2

29 Measuring illumination: radiant intensity Power per solid angle emanating from a point source apple W I(!) = d d! sr

30 Isotropic point source Z = S 2 I d! =4 I I = 4

31 Goniometric diagrams

32 Rendering with goniometric diagrams

33 Photometry All radiometric quantities have equivalents in photometry Dark adapted eye (scoptic) Daytime adapted eye (photoptic) Photometry: accounts for response of human visual system V ( ) to electromagnetic radiation Luminance (Y) is photometric quantity that corresponds to radiance: integrate radiance over (nm) all wavelengths, weight by eye s luminous efficiacy curve, e.g.: Z 1 Y (p,!) = 0 L(p,!, ) V ( )d

34 Radiometric and photometric terms Physics Radiometry Photometry Energy Radiant Energy Luminous Energy Flux (Power) Radiant Power Luminous Power Flux Density Irradiance (incoming) Radiosity (outgoing) Illuminance (incoming) Luminosity (outgoing) Angular Flux Density Radiance Luminance Intensity Radiant Intensity Luminous Intensity

35 Photometric Units Photometry MKS CGS British Luminous Energy Talbot Talbot Talbot Luminous Power Lumen Lumen Lumen Illuminance Luminosity Lux Phot Footcandle Luminance Nit, Apostlib, Blondel Stilb Lambert Footlambert Luminous Intensity Candela Candela Candela Thus one nit is one lux per steradian is one candela per square meter is one lumen per square meter per steradian. Got it? James Kajiya

36 Modern LED light Input power: 11 W Output: 815 lumens (~ 80 lumens / Watt) Incandescent bulbs: ~15 lumens / Watt)

37 Cameras

38 Pinhole camera Infinitesimally small aperture y Pinhole x sensor

39 Real camera has lens with finite aperture Sensor plane: (X,Y) Image credit: Canon (EOS M)

40 Thin lens model lens F Focal length, F, is the distance behind Lens diameter is d=f/n, where n is the lens f-number the lens where parallel rays focus

41 Gaussian thin lens model sensor plane lens scene plane of focus Z 0 F Z Points at distance z focus at distance z behind the lens given by 1 F = 1 Z + 1 Z 0 Lenses are focused by moving them closer to/farther from the sensor plane Derivation:

42 Defocus blur Image credit: Mike Stobe/Getty Images for the USTA (link:

43 Defocus blur sensor plane Z 0 Z Z f Lens is focused at depth z f ; points at other depths image to an area (not a single point) on the sensor plane: this area is called the circle of confusion

44 How big is the circle of confusion? What is d c, the diameter of the circle of confusion of a scene point at depth z? sensor plane We know z s, the sensor plane position, and the lens diameter d d c d Compute z from F and z: 1 F = 1 Z + 1 Z 0 Z 0 Similar triangles: d c Zs 0 Z 0 = d Z 0 1 Z 0 s 1 d c = d Z 0 s Z 0 F Z

45 Depth of field is inversely proportional to aperture Plane of focus Larger aperture Image credit: Smaller aperture

46 Motion blur Camera records light over finite aperture and finite amount of time Cook et al. 1984

47 Film and sensors Camera sensors (film, CCD,...) effectively count the number of photons that hit them over small areas of the image Want to determine how much energy arrives over regions of the sensor (pixels) over a given period of time (exposure time) - Integrate irradiance over pixel area to get power (flux) - Integrate flux over time to get energy (joules) Q = Z t 1 t 0 Z A E(p 0,t 0 )dp 0 dt 0 How do we compute irradiance at a point on the image plane?

48 The measurement equation Lens aperture Sensor plane p Z E(p,t)= H 2 L i (p,! 0,t) cos d! 0

49 The measurement equation Lens aperture p 0 r 2 0 Sensor plane p E(p,t)= = Z Z A A L(p 0! p,t) L(p 0! p,t) cos cos 0 p 0 p 2 da0 cos 2 Transform integral over solid angle to integral over lens aperture p 0 p 2 da0 Assume aperture and film plane are parallel: = 0

50 The measurement equation Lens aperture p 0 r 2 p 0 p = d cos d Sensor plane E(p,t)= Z A = 1 d 2 Z Q = 1 Z t 1 d 2 t 0 Z L(p 0! p,t) A A lens p 0 cos 2 p 2 da0 L(p 0! p,t) cos 4 da 0 Z A film L(p 0! p,t) cos 4 dp dp 0 dt 0 p

51 Summary Today: - How to describe/measure light (radiant energy) - How light is measured by real sensors Next time: - How to compute all these integrals Next, next time: - Materials: how to describe the interaction of light with surfaces