可见光CMOS探测器星上逐点自适应成像方法及验证

    Visible spectrum CMOS detector on-board pixel-by-pixel adaptive imaging method and verification

    • 为解决海洋光学遥感中高动态范围与高信噪比难以兼顾的难题,提出了基于可见光互补金属氧化物半导体(complementary metal-oxide-semiconductor,CMOS)探测器的星上逐点自适应成像方法。该方法由定制探测器、星上处理算法和地面定标实现。开发了以高性能现场可编程门阵列(field-programmable gate array,FPGA)为载体的星上处理软件,并设计了逐点逐级增益的实时判断逻辑,使每个像元能够动态选择并输出其最高且未饱和的增益数据。通过地面辐射定标,精确确定了高增益、中增益、低增益和超低增益四档最优线性工作区间及切换阈值。在轨验证表明:该方法显著提升了HY-3A中分辨率成像光谱仪的性能。在信噪比满足观测要求的条件下,最大辐亮度为典型辐亮度的8.9倍以上,有效解决了高灵敏度与大动态范围之间的固有矛盾,为高精度海洋水色遥感提供了可靠技术途径。

       

      Abstract: To address the challenge of balancing high dynamic range and high signal-to-noise ratio (SNR) in marine optical remote sensing, an on-board pixel-by-pixel adaptive imaging method based on a visible spectrum complementary metal-oxide-semiconductor (CMOS) detector was proposed. The implementation of this method involved a customized detector, an on-board processing algorithm, and ground calibration. The on-board processing software was developed using a high-performance field-programmable gate array (FPGA) platform, and a real-time decision logic for pixel-by-pixel and stage-by-stage gain was designed, enabling each pixel to dynamically select and output the highest gain that remained unsaturated. Through ground radiation calibration, the optimal linear operating ranges and switching gain thresholds for the four gain stages, including high, medium, low, and ultra-low, were precisely determined. On-orbit verification demonstrates that this method significantly improves the performance of the HY-3A medium resolution imaging spectrometer. Under the condition that the SNR satisfies the observation requirements, the maximum radiance is at least 8.9 times the typical radiance, by which the inherent conflict between high sensitivity and large dynamic range is effectively resolved, providing a reliable technical approach for high-precision ocean color remote sensing.

       

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