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DigitalVideoAndHDTVAlgorithmsAndInterfaces.pdf

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Eq B.1<br />

Radiant exitance sums emitted and<br />

reflected light. The former term<br />

emittance excludes reflected light.<br />

Some thermal engineers use the<br />

term radiosity for radiant exitance.<br />

In computer graphics, radiosity<br />

refers to a specialized technique to<br />

compute illumination; it does not<br />

refer to any particular quantity.<br />

In photography, the symbol I<br />

is often used for irradiance or<br />

illuminance, instead of intensity.<br />

Radiometry and photometry involve light, in space. No<br />

surface is necessary! Light properties may be described<br />

at a real or imaginary surface; however, they are not<br />

properties of a surface. Absorptance (α), reflectance (ρ),<br />

and transmittance (τ) are intrinsic properties of surfaces,<br />

not properties of light.<br />

In what follows, I use the usual physics convention of<br />

writing letter symbols in italics and units in Roman type.<br />

Radiometry<br />

Radiometry starts with energy (symbol Q) at wavelengths<br />

between 100 nm and 1 mm. Energy is<br />

expressed in units of joules, J. A photon’s energy (Qp ) is<br />

related to its wavelength (λ):<br />

Qp h<br />

The rate of flow – or formally, the time-derivative – of<br />

radiant energy is power (P), also known as radiant flux<br />

(F, or preferably, Φ), expressed in units of watts, W.<br />

c −34<br />

h ≈ 6. 6260755⋅10 J⋅s (Planck's constant)<br />

= ;<br />

λ<br />

-1<br />

c ≡ 299972458 m ⋅s<br />

(speed of light)<br />

Radiant flux per unit area – that is, flux density – arriving<br />

at a real or imaginary surface, throughout all directions<br />

in a hemisphere, is irradiance (E). Irradiance is<br />

expressed in units of watts per meter squared, W·m -2<br />

(or W/m 2). Solar irradiance (insolation) at noon is about<br />

1 kW·m -2.<br />

Radiant flux per unit area leaving a surface, in all directions,<br />

is radiant exitance (M). Formally, this is the derivative<br />

of radiant flux with respect to area. Radiant<br />

exitance is expressed in units of watts per meter<br />

squared, W·m -2 . Radiant exitance from a nonemissive<br />

surface is simply its irradiance times its reflectance.<br />

Radiant flux in a specified direction – or formally, radiant<br />

flux per unit solid angle – is radiant intensity<br />

(symbol I ). The unit for intensity is watts per steradian,<br />

W·sr -1 (or W/sr). Intensity must be specified in<br />

a particular direction; it is independent of the<br />

observer’s location.<br />

602 DIGITAL VIDEO AND HDTV ALGORITHMS AND INTERFACES

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