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Diffraction model of a plenoptic camera for in-situ space exploration

机译:用于空间探索的全光相机的衍射模型

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This paper provides a detailed system theoretical model of a plenoptic camera with the aim to provide in-depth understanding of the plenoptic data recording concept and its effects. Plenoptic cameras, also known as light field cameras, were firstly thought of in the beginning of the 20th century and became recently possible thanks to rapid development of processing hardware and the increase of camera sensor resolution. Despite being a new type of sensor, they are operated in the same way as conventional cameras, but offer several advantages. A plenoptic camera consists of a main lens and a lenslet array (microlens array) right in front of the detector. The microlens array causes not only the recording of the incident location of a light ray on the sensor, as it is done by a conventional camera, but also the incident direction. Such a record can be represented by a 4-D data set known as the light field. In fact, by inserting a microlens array any conventional camera can be transformed into a plenoptic camera. The plenoptic recording concept and the 4-D light field provide multiple advantages over conventional cameras. For example, a single recorded light field allows first, to reconstruct novel views with small changes in viewpoint, second, to create a depth map, and third, to refocus images after the data capture. Hence, the process of focusing is shifted from hardware to software. Last, but not least, plenoptic cameras allow an extended depth of field in comparison to a conventional camera and the use of a bigger camera aperture. Most of the mentioned advantages become particularly effective at close-range to an object. The German Aerospace Center performs research on plenoptic cameras for close-range imaging in space. Possible applications are for example robot vision with plenoptic cameras for robotic arm operations during on-orbit servicing missions or the use of plenoptic cameras on rovers in the course of exploration missions to other planets. Those application scenarios and the demanding conditions in space require thorough comprehension of plenoptic cameras. For this purpose, this paper shall provide a detailed model of plenoptic cameras, which allows to derive camera parameters and optimize them with particular attention to the user requirements and to generate synthetic data. The latter can be utilized to assess the evaluation algorithms, which are not mentioned in detail in this paper. The modeling of the plenoptic camera is mainly based on the theory of geometric optics expanded by elements of diffraction optics.
机译:本文提供了详细的全光相机系统理论模型,旨在深入了解全光数据记录概念及其效果。全光相机,也称为光场相机,最早是在20世纪初想到的,由于处理硬件的飞速发展和相机传感器分辨率的提高,最近才成为可能。尽管是新型传感器,但它们的操作方式与传统相机相同,但具有许多优点。全光摄像机由一个主透镜和一个位于检测器正前方的小透镜阵列(微透镜阵列)组成。微透镜阵列不仅导致记录光线在传感器上的入射位置(如通过常规照相机完成的记录),而且导致入射方向的记录。这样的记录可以由称为光场的4-D数据集表示。实际上,通过插入微透镜阵列,可以将任何常规相机转换为全光相机。全光记录概念和4-D光场提供了优于常规相机的多项优势。例如,单个记录的光场首先允许重建视点变化很小的新颖视图,其次可以创建深度图,其次可以在数据捕获后重新聚焦图像。因此,关注的过程从硬件转移到了软件。最后但并非最不重要的是,与传统摄像机相比,全光摄像机可以扩展景深,并且可以使用更大的摄像机光圈。提到的大多数优点在靠近对象时变得特别有效。德国航空航天中心对全光相机进行太空近距离成像研究。可能的应用是,例如在维修任务期间使用全光相机进行机器人手臂操作的机器人视觉,或在对其他行星进行探索任务的过程中在车上使用全光相机。那些应用场景和太空中的苛刻条件要求全面了解全光相机。为此,本文将提供全光相机的详细模型,该模型允许导出相机参数并对其进行优化,并特别注意用户要求并生成合成数据。后者可用于评估评估算法,本文将不对其进行详细介绍。全光相机的建模主要基于由衍射光学元件扩展的几何光学理论。

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