脉冲星:走向无处不在的可见光定位

Chi Zhang, Xinyu Zhang
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引用次数: 3

摘要

近十年来可见光定位技术的研究已经达到了厘米级的定位精度。然而,现有的VLP系统要么需要专门的led,这阻碍了大规模部署,要么需要摄像头,因为功耗和覆盖范围短,无法实现连续定位。我们提出脉冲星,它使用一个紧凑的光电二极管传感器来区分现有的天花板灯基于其固有的光学发射特征。为了克服光电二极管缺乏空间分辨率的问题,我们设计了一种新的稀疏摄影测量机制,该机制可以解决光的到达角,并对设备的3D位置和方向进行三角测量。为了方便无处不在的部署,我们进一步开发了一种光注册机制,可以自动在建筑物的地板地图上注册天花板灯的位置。实验表明,脉冲星在连续覆盖下可以可靠地达到分米精度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Pulsar: Towards Ubiquitous Visible Light Localization
The past decade's research in visible light positioning (VLP) has achieved centimeter location precision. However, existing VLP systems either require specialized LEDs which hinder large-scale deployment, or cameras which preclude continuous localization due to power consumption and short coverage. We propose Pulsar, which uses a compact photodiode sensor to discriminate existing ceiling lights based on their intrinsic optical emission features. To overcome the photodiode's lack of spatial resolution, we design a novel sparse photogrammetry mechanism, which resolves the light's angle-of-arrival, and triangulates the device's 3D location and orientation. To facilitate ubiquitous deployment, we further develop a light registration mechanism that automatically registers ceiling lights' locations on a building's floor map. Our experiments demonstrate that Pulsar can reliably achieve decimeter precision with continuous coverage.
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