Chapter 1:
An Overview of Uncooled Thermal Imaging Detection Mechanisms and Their Figures of Merit
Authors(s): Paul W. Kruse
Published: 2001
DOI: 10.1117/3.415351.ch1
The subject of this book is uncooled thermal imaging focal plane arrays and systems. In this context, "€œuncooled"€ refers to not employing artificial means of reducing the temperature of the infrared array, such as by means of cryogenic solids or liquids, mechanical refrigerators, thermoelectric coolers, or Joule-Thomson coolers. The infrared array operates at the ambient temperature, whatever that might be. If unstated, the temperature is assumed to be "room temperature," generally considered to be 295 K or 300 K. Some detection mechanisms require the use of temperature stabilizers upon which are mounted the thermal imaging arrays. Although their construction is similar to that of thermoelectric coolers, they maintain the array at or very near room temperature; thus they are not considered to be coolers. The term "€œthermal imaging"€ refers to the ability of the array in its system to image room temperature scenes. Here again, “room temperature” implies 295 K or 300 K. A thermal image of a scene refers to an image of that scene made entirely by detecting the thermal (infrared) radiation emitted by everything in the scene. Thus there is no use of artificial (lamps, lasers) or natural (sunlight, moonlight, starlight, airglow) illumination of the scene. Because “room temperature” radiation has its spectral peak emittance at about 10-μm wavelength, this implies that the spectral response of the thermal imaging array extends beyond 3-μm wavelength; such arrays are usually designed to operate in the 3-€“5-μm or 8-14-μm atmospheric windows.
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