Radiometry and Photometry - Computer Graphics at...

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Page 1 CS348B Lecture 4 Pat Hanrahan, Spring 2012 Light Visible electromagnetic radiation Power spectrum Polarization Photon (quantum effects) Wave (interference, diffraction) From London and Upton CS348B Lecture 4 Pat Hanrahan, Spring 2012 Radiometry and Photometry Measuring spatial properties of light ! Radiant power ! Radiant intensity ! Irradiance ! Inverse square law and cosine law ! Radiance ! Radiant exitance (radiosity) Goal is to perform lighting calculations in the physically correct way

Transcript of Radiometry and Photometry - Computer Graphics at...

Page 1: Radiometry and Photometry - Computer Graphics at …graphics.stanford.edu/courses/cs348b-12/lectures/...Page 2 Radiometry and Photometry CS348B Lecture 4 Pat Hanrahan, Spring 2012

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Light

Visible electromagnetic radiation

Power spectrum

Polarization

Photon (quantum effects)

Wave (interference, diffraction) From London and Upton

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Radiometry and Photometry

Measuring spatial properties of light

!! Radiant power

!! Radiant intensity

!! Irradiance !! Inverse square law and cosine law

!! Radiance

!! Radiant exitance (radiosity)

Goal is to perform lighting calculations in the physically correct way

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Radiometry and Photometry

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Radiant Energy and Power

Power: Watts (radiometry)

vs. Lumens (photometry)

!! Spectral efficacy

!! Energy efficiency

Energy: Joules vs. Talbot

!! Exposure !! Film response

!! Skin - sunburn

Photometric luminance

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Radiant Intensity

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Radiant Intensity

Definition: The radiant (luminous) intensity is the

power per unit solid angle emanating from

a point source.

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Angles and Solid Angles

!! Angle

!! !! !! !! !!

!! Solid angle

"" circle has 2 ## radians

"" sphere has 4 ## steradians

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Differential Solid Angles

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Differential Solid Angles

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Differential Solid Angles

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Isotropic Point Source

Sphere

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Warn’s Spotlight

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Warn’s Spotlight

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Warn’s Spotlight

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Warn’s Spotlight

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Light Source Goniometric Diagrams

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Irradiance

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Irradiance

Definition: The irradiance (illuminance) is the power per unit area incident on a surface.

Sometimes referred to as the radiant (luminous) incidence.

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

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

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Beam Power in Terms of Irradiance

Φ = EA

A

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Beam Power Falling on the Surface

A′Φ′ = E′A′

E′ =Φ′

A′

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Projected Area

A! A′

A = A′ cos θ

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Conservation of Energy

A! A′

A = A′ cos θ

Φ = Φ′

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Lambert’s Cosine Law

A! A′

A = A′ cos θ

Φ = Φ′

E�=

Φ�

A�=

Φ

Acos θ = E cos θ

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Irradiance: Isotropic Point Source

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Irradiance: Isotropic Point Source

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Irradiance: Isotropic Point Source

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Irradiance: Isotropic Point Source

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Irradiance: Isotropic Point Source

CS348B Lecture 4 Pat Hanrahan, Spring 2012

The Invention of Photometry

Bouguer’s classic experiment !! Compare a light source and a

candle !! Move until they both appear

equally bright !! Intensity is proportional to ratio

of distances squared

Definition of a candela !! Originally a “standard” candle !! Currently 550 nm laser

with 1/683 W/sr !! 1 of 6 fundamental SI units

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Radiance

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Definition: The surface radiance (luminance) is

the intensity per unit area leaving a surface

Area Lights – Surface Radiance

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Typical Values of Luminance [cd/m2]

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

Sunlight clouds 30,000

Clear sky 3,000

Overcast sky 300

Moon 0.03

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Directional Power Leaving a Surface

Same dA for all directions

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Radiant Exitance

(Radiosity)

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Radiant Exitance

Definition: The radiant (luminous) exitance is the energy per unit area leaving a surface.

In computer graphics, this quantity is usually referred to as radiosity (B)

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Area Light Source

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Area Light Source

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Area Light Source

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Area Light Source

Hemisphere

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Uniform Diffuse Emitter

Uniform means Lo is not a function of direction

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Projected Solid Angle

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CS348B Lecture 4 Pat Hanrahan, Spring 2012

Projected Solid Angle

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Uniform Diffuse Emitter

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Radiometry and Photometry

Summary

CS348B Lecture 4 Pat Hanrahan, Spring 2012

Radiometric and Photometric Terms

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Photometric Units

“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