2013
DOI: 10.1016/j.infrared.2012.12.026
|View full text |Cite
|
Sign up to set email alerts
|

Multispectral and polarimetric imaging in the LWIR: Intersubband detectors as a versatile solution

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

0
4
0

Year Published

2014
2014
2019
2019

Publication Types

Select...
6
1
1

Relationship

0
8

Authors

Journals

citations
Cited by 13 publications
(4 citation statements)
references
References 29 publications
0
4
0
Order By: Relevance
“…For instance, according to the diffraction limit theory proposed by Ernest Abbe and Lord Rayleigh in 1873 and 1879, a higher resolution of microscope and telescope requires either the reduction of operational wavelength or the increase of aperture size. For many specific objects such as molecules and star dust, the smallest operational wavelength is limited by the absorption/scattering process, thus a larger aperture becomes the only possible choice (for ground-based telescope, adaptive optics is required to eliminate the influence of atmosphere turbulence). , However, the increase in telescope aperture requires much higher cost and longer manufacturing time for both ground-based and space-based telescopes. In microscopes and lithographic systems, the highest numerical aperture is ultimately limited by the immersion materials and hardly to be further improved beyond 1.4.…”
mentioning
confidence: 99%
“…For instance, according to the diffraction limit theory proposed by Ernest Abbe and Lord Rayleigh in 1873 and 1879, a higher resolution of microscope and telescope requires either the reduction of operational wavelength or the increase of aperture size. For many specific objects such as molecules and star dust, the smallest operational wavelength is limited by the absorption/scattering process, thus a larger aperture becomes the only possible choice (for ground-based telescope, adaptive optics is required to eliminate the influence of atmosphere turbulence). , However, the increase in telescope aperture requires much higher cost and longer manufacturing time for both ground-based and space-based telescopes. In microscopes and lithographic systems, the highest numerical aperture is ultimately limited by the immersion materials and hardly to be further improved beyond 1.4.…”
mentioning
confidence: 99%
“…In visible range of the spectrum the extinction ratio of micro-polarizers has reached ~60 6 . In infrared (IR) range, however, the extinction ratio is only 2.3 for IR detectors 7 (expressed as contrast ratio (diattenuation) = (Rx-Ry)/(Rx+Ry) > 40% in the referenced paper), and will saturate to only about 10 (responsivity contrast ~82%) even when the pixel size is enlarged to 100 μm 8 . The reason might be attributed to the cross-talks between neighbor pixels or the wave-leakage through pixel edges that contaminates the polarization as for imaging FPAs the detecting pixel is completely exposed within the light beam and the longer wavelength in IR range will make the cross-talk/wave-leakage much easier.…”
mentioning
confidence: 99%
“…Targets under tree cover received relatively diffuse illumination and exhibited considerably weaker polarisation. Thales have also explored the feasibility of developing a tri-spectral polarimetric QWIP array to enhance the location of sites harbouring potential IEDs [20].…”
Section: Dtc Research On Eo Systemsmentioning
confidence: 99%