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地面目标的中波红外高光谱成像特性测量

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利用Telops公司设计的Hyper-Cam中波高光谱成像仪对水泥地上某坦克模型进行3~5 μm波段的红外高光谱成像测量.对实验数据进行了逐像素点的大气校正.基于矫正后的实验数据,分析了仪器误差、随机误差、大气校正传递误差等对测试不确定度的影响.分析了该坦克模型在不同谱段上的亮度分布和模型上不同部位的光谱分布特性.结果表明:在波数为2 000~3 000 cm-1波段,其相对不确定度一直稳定在10%以内,但是在大于3 000 cm-1的波段,其误差迅速上升,主要因为常温物体的中波辐射低,在该波段目标辐射与大气路程辐射接近,而引起的噪声增大,造成的测试信噪比降低.该坦克模型光谱辐射亮度测试数据的平均相对不确定度在20%以内,整体误差较低.光谱分布上,坦克各部分特征点和水泥地表的光谱辐射亮度在波长为4.2~5 μm波段时的差异性比波长为3.0~4.2μm波段时的差异性更大,且探测器接收到的4.2~5μm波段的光谱辐射亮度要大于3.0~4.2 μm的光谱辐射亮度.由于4.3 μm波段处于大气吸收带,大气透射率几乎为0,以至于无法获得目标的光谱辐射亮度的真实测量值.空间分布上,模型的辐射亮度主要集中在侧边涂层上,炮口处和履带处的辐射亮度较小.目标各部位辐射亮度分布与周边水泥地表的辐射亮度有着明显差异性.在3~5 μm的辐射亮度中,4.4~4.8 μm波段的辐射亮度占比较高,该波段成像效果最好.3.2~3.8μm波段的辐射亮度占比较低,该波段成像效果较差.处于大气吸收带的4.2~4.4μm波段,由于大气透射率几乎为0,无法获得其准确的空间辐射亮度分布.研究表明该拓展中波高光谱成像仪在地面目标的中波红外高光谱成像特性研究上具有目标区分精确、误差小、"图像光谱合一"的特点,测试数据可以应用于目标的红外高光谱隐身设计、目标的分类与识别等领域.
Measurement of Mid-Wave Infrared Hyperspectral Imaging Characteristics of Ground Targets
The Hyper-Cam medium-wave hyperspectral imager designed by Telops was used to measure the infrared hyperspectral imaging of a tank model on the cement floor in the 3~5 μm band.Atmospheric correction is performed on a pixel-by-pixel basis of the experimental data.Finally,according to the corrected experimental data,the effects of instrument,random,and atmospheric correction transmission errors on the test uncertainty were analyzed.The luminance distribution of the tank model on different spectral bands and the spectral distribution characteristics of different parts of the model were also analyzed.The results show that the relative uncertainty of the wavenumber in the band of 2 000~3 000 cm 1 has been stable w ithin 10%,but in the band greater than 3 000 cm-1,the error rises rapidly.The error is mainly because the medium-wave radiation of the normal temperature object is low,and the target radiation in this band is close to the atmospheric radiation of the distance,and the noise caused by the increase of the noise caused by the decrease of the test signal-to-noise ratio is reduced.The average relative uncertainty of the tank model's spectral radiation brightness test data is within 17%,and the overall error is low,which has reached the advanced level in China.In terms of spectral distribution,the difference in the spectral radiation brightness of the characteristic points of each part of the tank and the cement surface in the wavelength of 4.2~5 μm is greater than that in the wavelength of 3.0~4.2 μm,and the spectral radiation brightness in the 4.2~5 μm band emitted by the detector is greater than the spectral radiation brightness of 3.0~4.2 μm in the shorter band.Since the 4.3 μm band is in the atmospheric absorption band,the average transmittance calculated by Modtran is almost 0,so a true measurement of the spectral radiation brightness on the target cannot be obtained.Regarding spatial distribution,the radiation brightness of the model is mainly concentrated on the side coating,and the radiation brightness at the muzzle and track is small.The radiant brightness distribution of typical target parts is significantly different from that of the surrounding cement surface.Among them,4.4~4.8μm occupies a high radiation brightness ratio,and this band's imaging effect is the best.The proportion of radiation brightness occupied by 3.2~3.8 μm is low,and the imaging effect in this band is poor.In the 4.2~4.4 μm band under the atmospheric absorption zone,because the atmospheric transmittance is almost 0,the accurate spatial radiation brightness distribution cannot be obtained.The results show that the extended medium-wave hyperspectral imager has the characteristics of accurate target discrimination,small error and"image spectrum integration"in the study of the medium-wave infrared hyperspectral imaging characteristics of ground targets,and the test data can be applied to the infrared hyperspectral stealth design of the target.

Infrared radiation characteristic measurementMedium wave hyperspectral imagingAtmospheric correctionUncertainty analysis

江岳鹏、曹运华、吴振森、曹轶森、胡绥靖

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西安电子科技大学物理学院,陕西西安 710071

红外辐射特性测量 中波高光谱成像 大气校正 不确定度分析

国家自然科学基金

61875156

2024

光谱学与光谱分析
中国光学学会

光谱学与光谱分析

CSTPCD北大核心
影响因子:0.897
ISSN:1000-0593
年,卷(期):2024.44(4)
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