2012
DOI: 10.1117/12.928564
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Real-time transmission-type terahertz microscope with palm size terahertz camera and compact quantum cascade laser

Abstract: This paper describes a real-time transmission-type Terahertz (THz) microscope, with palm-size THz camera and compact quantum cascade laser (QCL). The THz camera contains 320x240 microbolometer focal plane array which operates at 30 Hz frame rate and has lock-in imaging function as well as integration functions such as frame integration and spatial filter. These functions are found very powerful in improving signal-to-noise ratio. QCL is installed in compact Stirling cycle cooler. A variety of QCLs covers frequ… Show more

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Cited by 9 publications
(8 citation statements)
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“…The shape of the blade is easily recognizable. Note that there is no fringe pattern in the image, which is often observed in images obtained when using a detector array [19], [22]. In Fig.…”
Section: -D Imagingmentioning
confidence: 78%
See 2 more Smart Citations
“…The shape of the blade is easily recognizable. Note that there is no fringe pattern in the image, which is often observed in images obtained when using a detector array [19], [22]. In Fig.…”
Section: -D Imagingmentioning
confidence: 78%
“…Real-time imaging with a QCL was realized using a commercial focal-plane array microbolometer camera for detection [19]- [22]. However, these systems seem to suffer from fringe patterns, which appear in the THz image.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…It is found in Fig.9(b) that the lock-in imaging function increases SNR as a function of square root of the number of frame-integration, while frame integration without lock-in function does not so much increase SNR as expectation, because low frequency noise is predominant in microbolometer FPAs. [41] . Figures 11(a) and (b) show THz images of tablet put into an envelope and metallic clip put under flours, respectively.…”
Section: Lock-in Imaging Functionmentioning
confidence: 95%
“…Such imaging systems are already built on commercial basis and can be used for specific practical tasks [19]. Judged by their noise equivalent power (NEP), a single pixel of such a detector array (typical NEPs are spanning from 10 -9 W Hz -1/2 [19] over 10 -11 W Hz -1/2 [20] up to 0.5 10 -12 W Hz -1/2 [21]) is less sensitive than very sensitive single-pixel detectors (typical NEP~10 -14 W Hz -1/2 [22]). Some detectors used for space applications do have even lower NEPs (e.g.…”
mentioning
confidence: 99%