FLIR C3 User Manual

Theory of thermography
18
For highly polished materials ε
λ
approaches zero, so that for a perfectly reflecting material
(i.e. a perfect mirror) we have:
For a graybody radiator, the Stefan-Boltzmann formula becomes:
This states that the total emissive power of a graybody is the same as a blackbody at the
same temperature reduced in proportion to the value of ε from the graybody.
Figure 18.8 Spectral radiant emittance of three types of radiators. 1: Spectral radiant emittance; 2: Wave-
length; 3: Blackbody; 4: Selective radiator; 5: Graybody.
Figure 18.9 Spectral emissivity of three types of radiators. 1: Spectral emissivity; 2: Wavelength; 3: Black-
body; 4: Graybody; 5: Selective radiator.
#T559918; r. AN/42281/42281; en-US
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FLIR C3 Specifications

General

Temperature Range	-10°C to 150°C (14°F to 302°F)
Field of View	41° x 31°
Thermal Sensitivity	<0.10°C
Accuracy	±2 °C or ±2% of reading
Resolution	80 x 60 pixels
Image Storage	Internal memory
Connectivity	Wi-Fi
Display	3-inch touchscreen
Image Modes	Thermal, MSX, Picture-in-Picture
Digital Camera	640 x 480 pixels
File Format	JPEG
Battery Life	4 hours
Dimensions	125 x 80 x 24 mm (4.9 x 3.1 x 0.94 in)
Operating Temperature	-10°C to +50°C