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Understanding Infrared Thermography Reading 3

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Figure 1.8: Spectral distribution of a blackbody, graybody and nongraybody<br />

100<br />

Blackbody at 300 K<br />

Q)<br />

Q)<br />

..<br />

><br />

Ctl<br />

- Q)<br />

90<br />

u<br />

c: 80<br />

.!!:!<br />

"0<br />

ns 70<br />

a:<br />

- ns 60<br />

...<br />

u<br />

c. 50<br />

en<br />

Q)<br />

40<br />

a:<br />

...<br />

...<br />

30<br />

Q) 20<br />

r::n<br />

ns<br />

1- 10<br />

L<br />

-I ~<br />

Graybody at 300 K<br />

H-<br />

Nongray(body at 300 K<br />

1 5 10 15 20<br />

Wavelength (llm)<br />

Charlie Chong/ Fion Zhang

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