Geodesic lenses applied to nonimaging optics

J. Miñano, P. Benítez, Bill Parkyn, D. Grabovičkić, Fernando García, J. Blen, A. Santamaria, J. Chaves, W. Falicoff
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Abstract

A novel waveguide-optical integrator is introduced for applications to LEDs. The concept is based upon a Kohler illuminator made of Luneburg lenses. Typical Kohler illuminators are formed by pairs of thin lenses, and perform badly when the paraxial approximation is rough, i.e., when the angular span of the incoming rays is wide. In contrast, the new illuminator performs ideally for angular spans up to 90o (±45o), and has only a 3% loss for a 180o angular span. In general such an illuminator cannot be made in 3D, because adjacent Luneburg lenses overlap. It can, however, be implemented in planar optics, by using Rinehart geodesic lenses, which moreover do not use gradient index material. This waveguide device has application in illumination engineering as a light mixer, particularly for LEDs. Another light mixer using a combination of two kaleidoscopes with a geodesic lens is also presented. Irradiance at the exit of a kaleidoscope has good light mixing if the kaleidoscope is long enough, but the intensity is never well mixed, irrespective of the length. Inserting a Rinehart geodesic lens produces a 90-degree phase-space rotation of the rays, i.e., it exchanges irradiance and intensity. A further kaleidoscope assures complete mixing in both irradiance and intensity.
用于非成像光学的测地线透镜
介绍了一种应用于led的新型波导光积分器。这个概念是基于由卢讷堡透镜制成的科勒照明器。典型的科勒照明器是由一对薄透镜组成的,当近轴近似粗糙时,即入射光线的角跨度很宽时,照明器的性能很差。相比之下,新的照明执行理想的角跨度高达90度(±45度),只有3%的损失为180度角跨度。一般来说,这样的照明器不能在3D中制作,因为相邻的吕讷堡透镜重叠。然而,它可以在平面光学中实现,通过使用莱因哈特测地线透镜,而且不使用梯度折射率材料。该波导器件在照明工程中作为混光器,尤其适用于led。另一种混合光使用两个万花筒与测地线镜头的组合也被提出。如果万花筒足够长,则万花筒出口的辐照度具有良好的光混合,但无论长度如何,其强度都不能很好地混合。插入莱因哈特测地线透镜会产生光线的90度相空间旋转,即它交换辐照度和强度。进一步的万花筒保证了辐照度和强度的完全混合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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