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Understanding Infrared Thermography Reading 7 Part 2 of 2.pdf

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Staring Array<br />

A staring array, staring-plane array, focal-plane array (FPA), or focal-plane is<br />

an image sensing device consisting <strong>of</strong> an array (typically rectangular) <strong>of</strong> lightsensing<br />

pixels at the focal plane <strong>of</strong> a lens. FPAs are used most commonly for<br />

imaging purposes (e.g. taking pictures or video imagery), but can also be<br />

used for non-imaging purposes such as spectrometry, LIDAR, and wave-front<br />

sensing.<br />

In radio astronomy the term "FPA" refers to an array at the focus <strong>of</strong> a radiotelescope<br />

(see full article on Focal Plane Arrays). At optical and infrared<br />

wavelengths it can refer to a variety <strong>of</strong> imaging device types, but in common<br />

usage it refers to two-dimensional devices that are sensitive in the infrared<br />

spectrum. Devices sensitive in other spectra are usually referred to by other<br />

terms, such as CCD (charge-coupled device) and CMOS image sensor in the<br />

visible spectrum. FPAs operate by detecting photons at particular<br />

wavelengths and then generating an electrical charge, voltage, or resistance<br />

in relation to the number <strong>of</strong> photons detected at each pixel. This charge,<br />

voltage, or resistance is then measured, digitized, and used to construct an<br />

image <strong>of</strong> the object, scene, or phenomenon that emitted the photons.<br />

Charlie Chong/ Fion Zhang<br />

http://military.wikia.com/wiki/Staring_arrayc

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