1975
DOI: 10.1117/12.954526
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<title>Far Infrared Imagery</title>

Abstract: Imaging experiments in the far infrared are described. Transmission data are presented for several common media. Far infrared pictures of metallic objects are presented. The practicality of a far infrared imaging system is discussed.

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Cited by 17 publications
(3 citation statements)
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“…It is likely that the better agreement for the tooth results is related to the low levels of hydration in the tooth samples, while measurements in skin are likely to vary substantially without careful control of measuring conditions. Absorption coefficient results obtained were of the same order of magnitude as the early, incoherent, measurements reported by Barker et al 20 , and rank in the same order. Although reflection losses were included in their attenuation coefficients, the values for bone and fat are lower than those reported here, and not higher as might be expected.…”
Section: Discussionsupporting
confidence: 75%
“…It is likely that the better agreement for the tooth results is related to the low levels of hydration in the tooth samples, while measurements in skin are likely to vary substantially without careful control of measuring conditions. Absorption coefficient results obtained were of the same order of magnitude as the early, incoherent, measurements reported by Barker et al 20 , and rank in the same order. Although reflection losses were included in their attenuation coefficients, the values for bone and fat are lower than those reported here, and not higher as might be expected.…”
Section: Discussionsupporting
confidence: 75%
“…The potential of technical imaging in the veryfar-infrared (FIR) range has been considered as early as 1975. Owing to the lack of easy-to-use sources at that time this topic had not been pursued past an initial proof of principle [9]. Recent advancements in ultrashort electromagnetic pulse generation has revived this subject [10,11].…”
Section: Chemical Recognition In Terahertz Imagingmentioning
confidence: 99%
“…All objects at temperatures above absolute zero radiate energy in the form of electromagnetic waves and absorb and reflect energy that is incident upon them. A perfect absorber is calied a blackbody which is a perfect radiator and has an omission spectrum completely governed by the absolute physical temperature T. The brightness of the radiation is given by Planck's radiation law as follows: 2hv 3 (1) In Fig. 1, several brightness curves are plotted as a function of frequency and temperature using Eq.…”
Section: Radiometry Fundamentalsmentioning
confidence: 99%