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handbook of modern sensors

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108 3 Physical Principles <strong>of</strong> Sensing<br />

(A)<br />

(B)<br />

Fig. 3.45. Spatial emissivities for a nonmetal (A) and a polished metal (B).<br />

All nonmetals are very good diffusive emitters <strong>of</strong> thermal radiation with a remarkably<br />

constant emissivity defined by Eq. (3.139) within a solid angle <strong>of</strong> about ±70 ◦ . Beyond<br />

that angle, emissivity begins to decrease rapidly to zero with the angle approaching<br />

90 ◦ . Near 90 ◦ , emissivity is very low. A typical calculated graph <strong>of</strong> the directional<br />

emissivity <strong>of</strong> nonmetals into air is shown in Fig. 3.45A. It should be emphasized<br />

that the above considerations are applicable only to wavelengths in the far-infrared<br />

spectral range and are not true for the visible light, because emissivity <strong>of</strong> thermal<br />

radiation is a result <strong>of</strong> electromagnetic effects which occur at an appreciable depth.<br />

Metals behave quite differently. Their emissivities greatly depend on the surface<br />

finish. Generally, polished metals are poor emitters within the solid angle <strong>of</strong> ±70 ◦ ,<br />

and their emissivity increases at larger angles (Fig. 3.45B). This implies that even a<br />

very good metal mirror reflects poorly at angles approaching 90 ◦ to normal. Table<br />

A.18 in the Appendix gives typical emissivities <strong>of</strong> some materials in a temperature<br />

range between 0 ◦ C and 100 ◦ C.<br />

Unlike most solid bodies, gases in many cases are transparent to thermal radiation.<br />

When they absorb and emit radiation, they usually do so only in certain narrow spectral<br />

bands. Some gases, such as N 2 ,O 2 , and others <strong>of</strong> nonpolar symmetrical molecular<br />

structure, are essentially transparent at low temperatures, whereas CO 2 ,H 2 O, and<br />

various hydrocarbon gases radiate and absorb to an appreciable extent. When infrared<br />

light enters a layer <strong>of</strong> gas, its absorption has an exponential decay pr<strong>of</strong>ile, governed<br />

by Beer’s law:<br />

x<br />

= e −αλx , (3.140)<br />

0<br />

where 0 is the incident thermal flux, x is the flux at thickness x, and α λ is the<br />

spectral coefficient <strong>of</strong> absorption. The above ratio is called a monochromatic transmissivity<br />

γ λ at a specific wavelength λ. If gas is nonreflecting, then its emissivity is<br />

defined as<br />

ε λ = 1 − γ λ = 1 − e −αλx . (3.141)<br />

It should be emphasized that because gases absorb only in narrow bands, emissivity<br />

and transmissivity must be specified separately for any particular wavelength. For<br />

instance, water vapor is highly absorptive at wavelengths <strong>of</strong> 1.4, 1.8, and 2.7 µm and<br />

is very transparent at 1.6, 2.2, and 4 µm.

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