基于FPGA的校准器星载太阳闪烁快速检测方法

Yuhao Li, F. Ji, Yadong Hu, Gaojun Chi, Zhenwei Qiu, Zhuoran Li, Feinan Chen
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引用次数: 0

摘要

太阳闪烁是被动光学遥感成像的一个严重障碍。由于太阳光在水面上的镜面反射,太阳闪烁具有很强的线偏振特性,通常通过增加偏振器来抑制。为此,研制了星载太阳闪烁偏振参数测量系统,实时计算在轨太阳闪烁参数。首先,分析了太阳闪烁的偏振辐射分布模型,根据星载偏振成像仪的原理,研制了太阳闪烁偏振角的实时检测系统。系统采用Xilinx V5 FPGA作为星上处理平台,采用高级综合(high-level synthesis, HLS)工具进行算法硬件描述开发。通过在HLS中使用数据流、流水线等优化方法,大大缩短了计算时间,减少了FPGA资源的使用。最后,我们利用它在670nm下通过粒度为25×25的三通道数据计算太阳闪烁偏振角,仿真结果表明,在100M时钟下,消耗了54%的片和DSP48 FPGA资源,可以在8ms时间内计算出太阳闪烁偏振角,满足了太阳闪烁快速检测的设计要求。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Fast detection method of calibrator spaceborne sun glint based on FPGA
Sun glint is a serious obstacle to passive optical remote sensing images. As is the specular reflection of sunlight from the facets of the water surface, sun glint has great linear polarization characteristics, and it is usually suppressed by adding polarizers. Therefore, a spaceborne sun glint polarization parameter measurement system is developed to calculate the on-orbit sun glint parameters in real time. Firstly, we analyzed the polarizing radiation distribution model of sun glint and developed a real time detection system for polarization angle of sun glint according to the principle of spaceborne polarization imager. The system is using Xilinx V5 FPGA as the on-the-satellite processing platform, and we use high-level synthesis (HLS) tools for algorithm hardware description development. By using dataflow, pipeline and other optimization methods in HLS, we greatly reducing computing time and reducing the FPGA resource use. Finally, we use it to calculate the sun glint polarization angle through a three-channel data with a granularity of 25×25 in 670nm, the simulation results show that under the 100M clock, 54% of the slice and DSP48 FPGA resources are consumed, and the sun glint polarization angle can be calculated in 8ms time, which meets the design requirements of rapid sun glint detection.
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