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随着航空航天高分辨率观测手段的逐步成熟,定量遥感在有效解决了光学地表多尺度效应后,更高分辨率的光学偏振效应在地表、大气、仪器3大要素方面逐步全面凸显出来,并直接决定或影响高分辨率观测系统的定量遥感效能实现和质量保障。例如,植被冠层极其微弱的多次散射反射偏振效应,如果不加扣除其模型误差达到136%;大气衰减本质是大气偏振效应,是遥感反演的最大误差源,误差达到5%—30%,偏振手段扣除大气误差目前已可以降低一半以上的误差;观测仪器扣除多次散射透射偏振光后,可以实现5 nm分辨率下0.1—0.3 nm高光谱定标能力,并借助偏振强化光噪声分离出中心波长偏移和带宽退化的误差根源。借助偏振"强光弱化,弱光强化",能够实现稳定度达10~(-8)月球辐亮度基准观测,为遥感辐亮度定标不确定度由7%到1%—2%跨越提供可能。 相似文献
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光的偏振信息在当前快速发展的光电子学和光学研究中是缺失的,利用偏振特征不仅可以提取探测物和研究对象的额外信息,而且延伸了探测的维度和提高了灵敏度。本文主要从基础研究和应用研究两个方面分析讨论红外偏振效应测量技术及红外遥感的若干进展,期望从不同的角度来考察偏振效应所带来的潜在应用。在上述背景下,本文介绍了红外椭圆偏振光谱技术及其在探测无机和有机薄膜体系光学性质的应用,并且归纳了红外偏振光学仪器理论及相关进展,特别是在空间遥感上的应用潜力。 相似文献
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Based on our previous work, the influence of annealing conditions on impurity species in in-situ arsenic (As)-doped Hg1-xCdxTe (x≈ 0.3) grown by molecular beam epitaxy has been systematically investigated by modulated photoluminescence spectra. The results show that (i) the doped-As acting as undesirable shallow/deep levels in as-grown can be optimized under proper annealing conditions and the physical mechanism of the disadvantage of high activation temperature, commonly assumed to be more favourable for As activation, has been discussed as compared with the reports in the As-implanted HgCdTe epilayers (x≈ 0.39), (ii) the density of V_textrmHg has an evident effect on the determination of bandgap (or composition) of epilayers and the excessive introduction of VHg will lead to a short-wavelength shift of epilayers, and (iii) the V_textrmHg prefers forming the VHg-AsHg complex when the inactivated-As (AsHg or related) coexists in a certain density, which makes it difficult to annihilate VHg in As-doped epilayers. As a result, the bandedge electronic structures of epilayers under different conditions have been drawn as a brief guideline for preparing extrinsic p-type epilayers or related devices. 相似文献
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