像素间距为12微米的测热计- fpa在8-12微米波段的透镜设计的挑战、限制和结果

N. Schuster, J. Franks
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引用次数: 4

摘要

在8-12微米波段,焦平面阵列(FPA)的像素间距为12微米或更小。具有VGA, XGA和SXGA分辨率的高分辨率fpa应该以合理的价格提供。这将需要新的镜头设计来提供所需的视野。光学设计师面临的挑战是,当探测器的像素间距与成像光的波长相同时,设计透镜。镜头规格将需要更多地考虑系统所需的分辨率。较小的像素间距检测器定义了对较短焦距的要求,以提供相同的视野。这将对镜头设计产生许多影响。几何像差随焦距成比例地减小。反向长焦布局将变得更加普遍,特别是当系统有快门时。像素数的增加将需要宽视场镜头,这提出了特殊的挑战。衍射效应对透镜设计的影响大大增加。快速的f值增加了系统的衍射极限,但也按立方规律增加了几何像差。因此,在衍射极限和像差极限性能之间的平衡变得更加困难。设计人员的第一种方法是重新使用最初用于17微米探测器的经过验证的设计。其中一些设计将在奈奎斯特12微米探测器的极限下具有足够的性能。甚至更小的探测器间距,如10微米,将需要新的红外透镜设计方法。传统的方法会将元素的数量迅速增加到3个甚至更多。这可能导致具有中等视场的透镜驱动系统成本。相机开发人员和镜头设计人员之间的密切合作将成为必要,以探索替代方法,如波前编码,以达到最具成本效益的解决方案。
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Challenges, constraints and results of lens design in 8-12micron waveband for bolometer-FPAs having a pixel pitch 12micron
In the 8-12 micron waveband Focal Plane Arrays (FPA) are available with a pixel pitch of 12 microns or less. High resolution FPAs with VGA, XGA and SXGA resolution should become available at a reasonable price. These will require new lens designs to give the required fields of view. The challenge for the Optical Designer is to design lenses when the pixel pitch of the detector is the same as the wavelength of the light imaged. The lens specification will need to give more thought to the resolution required by the system. A smaller pixel pitch detector defines a requirement for a shorter focal length to give the same field of view. This will have a number of effects upon the lens design. Geometrical aberrations decrease proportionally with the focal length. Reverse telephoto layouts will become more common, particularly when the system has a shutter. The increase in pixel count will require wide field of view lenses which present particular challenges. The impact of diffraction effects on the lens design is considerably increased. The fast F-number causes an increase in the diffraction limit of the system, but also increases geometric aberrations by a cube law. Therefore the balance between the diffraction limited and the aberration limited performance becomes more difficult. The first approach of the designer is to re-use proven designs originally intended for use with 17micron detectors. Some of these designs will have adequate performance at the Nyquist limit of the 12 micron detectors. Even smaller detector pitches, such as 10 micron, will demand new approaches to Infra Red lens design. The traditional approach will quickly increase the number of elements to 3 or even more. This could lead to the lenses with medium fields of view driving the system cost. A close cooperation between the camera developer and lens designer will become necessary in order to explore alternate approaches, such as wavefront coding, in order to reach the most cost effective solution.
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