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Light

Visible electromagnetic radiation

Power spectrum

Freq uency (H er tz)



2 4 6 8 10 12 14 16 18 20 22 24 26

1 10 10 10 10 10 10 10 10 10 10 10 10 10



Pow er H ea t Ra d io Infra - Ultra - X -Ra y s Ga m m a Cosm ic

Red V iolet Ra y s Ra y s



16 14 12 10 8 6 4 2 -2 -4 -6 -8

10 10 10 10 10 10 10 10 1 10 10 10 10

W a velength (N M )



IR R G B UV



700 600 500 400









Polarization From London and Upton



Photon (quantum effects)

Wave (interference, diffraction)

Topics

Light sources and illumination

Radiometry and photometry

Quantify spatial energy distribution

 Radiant intensity

 Irradiance

 Inverse square law and cosine law

 Radiance

 Radiant exitance (radiosity)

Illumination calculations

 Irradiance from environment

Radiometry and Photometry

Radiant Energy and Power



Power: Watts vs. Lumens

 Energy efficiency



 Spectral efficacy







Energy: Joules vs. Talbot

 Exposure Luminance

 Film response

Y   V ( ) L ( )d 

 Skin - sunburn

Radiometry vs. Photometry

Radiometry [Units = Watts]

 Physical measurement of electromagnetic energy

Photometry and Colorimetry [Lumen]

 Sensation as a function of wavelength

 Relative perceptual measurement

1

Brightness [Brils] B Y 3



 Sensation at different brightness levels

 Absolute perceptual measurement

 Obeys Steven’s Power Law

Radiant Intensity

The Invention of Photometry

Bouguer’s classic experiment

Compare a light source and a

candle

Intensity is proportional to ratio

of distances squared



Definition of a candela

Originally a “standard” candle

Currently 550 nm laser w/ 1/683

W/sr

1 of 6 fundamental SI units

Radiant Intensity



Definition: The radiant (luminous) intensity

is the power per unit solid angle emanating

from a point source.

d

I ( ) 

d

 W   lm 

 sr   sr  cd  candela 

  

683 lumens/watt @ 555nm

Angles and Solid Angles



l

Angle 

r

circle has 2p radians



A

Solid angle  2

R



sphere has 4p steradians

Differential Solid Angles



r sin



d dA  (r d )(r sin  d )

r

d  r 2 sin  d d





 dA

d  2

 sin  d d

r

Differential Solid Angles



dA

r sin d  2

 sin  d d

r

d r



d   d

S2

p 2p

   sin  d d

 0 0

1 2p

   d cos

1 0

d



 4p

Isotropic Point Source



  I d

S2



 4p I







I

4p

Warn’s Spotlight





 ˆ

A

ˆ )s

I ( )  cos   (  A

s









2p 1

   I ( ) d cos d

0 0

Warn’s Spotlight



 ˆ

A

ˆ )s

I ( )  cos   (  A

s







2p

2p

1 1

    I ( ) d cos d  2p  cos  d cos 

s



0 0 0

s 1

s 1 s

I ( )   cos 

2p

Light Source Goniometric

Diagrams

Radiance

Radiance



Definition: The surface radiance (luminance) is

the intensity per unit (projected) area leaving a

surface

L ( x,  ) dI ( x,  )

L( x,  ) 

dA

d d ( x,  )

2



d dA

 W   cd lm 

 sr m2   m2  sr m 2  nit 

  

dA

Typical Values of Luminance

[cd/m2]

Surface of the sun 2,000,000,000 nit

Sunlight clouds 30,000

Clear day 3,000

Overcast day 300

Moon 0.03

The Sky Radiance Distribution









From Greenler, Rainbows, halos and glories

Environment Maps









Interface, Chou and Williams (ca. 1985)

Gazing Ball  Environment

Maps









 Photograph of mirror ball Miller and Hoffman, 1984

 Maps all spherical directions to a to circle

 Reflection direction indexed by normal

 Resolution function of orientation

Irradiance

Irradiance

Definition: The irradiance (illuminance) is the

power per unit area incident on a surface.

d i

E( x) 

dA

 W   lm 

 m2   m2  lux 

   



Sometimes referred to as the radiant (luminous)

incidence.

Lambert’s Cosine Law

A



  EA







E

A

Lambert’s Cosine Law

A A / cos











 

E  cos

A / cos A

Irradiance: Isotropic Point Source





 h



r I

4p

Irradiance: Isotropic Point Source



d

 h



r I

4p

dA



d  I d

Irradiance: Isotropic Point Source



d

 h



r I

4p

dA

cos

d  2 dA

r

Irradiance: Isotropic Point Source



d

 h



r I

4p

dA

 cos

I d  dA

4p r 2

Irradiance: Isotropic Point Source



d

 h



r I

4p

dA

 cos  cos

I d  dA  E dA E 

4p r 2

4p r 2

Irradiance: Isotropic Point Source



d

 h  r cos



r I

4p

dA

 cos   cos  3

E 

4p r 2

4p h 2

Directional Power Arriving at a

Surface



Li ( x,  )

d

dA

d  i ( x,  )  Li ( x,  ) cos  dAd

2





cos  dAd  dA d



d  i ( x,  )

2

Irradiance from the Environment

Li ( x,  )

d 2  i ( x,  )  Li ( x,  )cos  dA d  dEdA

d

dE ( x,  )  Li ( x,  )cos d 







dA



Light meter E( x)   L ( x,)cos d

i

H2

Typical Values of Illuminance

[lm/m2]

Sunlight plus skylight 100,000 lux

Sunlight plus skylight (overcast) 10,000

Interior near window (daylight) 1,000

Artificial light (minimum) 100

Moonlight (full) 0.02

Starlight 0.0003

Blackbody Radiation

Tungsten Lamp

Fluorescent Bulb

Sunlight

Irradiance Environment Maps

L( ,  ) R

E( , ) N









Radiance Irradiance

Environment Map Environment Map

Irradiance Map or Light Map









Isolux contours

Radiant Exitance

(Radiosity)

Radiant Exitance



Definition: The radiant (luminous) exitance is the

energy per unit area leaving a surface.

d o

M ( x) 

dA

 W   lm 

m  m

2  2

 lux 

 

In computer graphics, this quantity is often

referred to as the radiosity (B)

Directional Power Leaving a

Surface

Lo ( x ,  )

d

dA

d  o ( x,  )  Lo ( x,  ) cos  dAd

2







d  o ( x,  )

2

Uniform Diffuse Emitter



Lo ( x,  )

M L o cos  d

H2

d

 Lo  cos d 

H2







dA

Projected Solid Angle

d











cos d

  cos  d  p

H2

Uniform Diffuse Emitter



M L 2

o cos  d

Lo ( x,  )

H



 Lo  cos  d d

H2 

 p Lo

M

Lo  dA

p

Radiometry and Photometry

Summary

Radiometric and Photometric

Terms



Physics Radiometry Photometry



Energy Radiant Energy Luminous Energy



Flux (Power) Radiant Power Luminous Power



Flux Density Irradiance Illuminance



Radiosity Luminosity



Angular Flux Density Radiance Luminance



Intensity Radiant Intensity Luminous Intensity

Photometric Units

Photometry Units



MKS CGS British



Luminous Energy Talbot



Luminous Power Lumen



Illuminance Lux Phot Footcandle

Luminosity

Luminance Nit Stilb

Apostilb, Blondel Lambert Footlambert



Luminous Intensity Candela (Candle, Candlepower, Carcel, Hefner)



“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


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