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Hyperspectral imaging: history and prospects 高光谱成像:历史与展望
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-09-12 DOI: 10.1007/s10043-025-01001-x
Motoki Yako

Hyperspectral (HS) imaging, which acquires the detailed spectral information of an object, has attracted extensive interest in various fields, such as remote sensing, agriculture, and biomedicine. In the dawn of HS imaging, HS imaging relied primarily on time-consuming scanning techniques to achieve high spatial and spectral resolution, limiting its applicability. Subsequently, snapshot (non-scanning) HS imaging emerged, enabling high-speed capturing. The snapshot method captures HS images in a single exposure, but it has the drawback of lower spatial resolution. With recent advancements in computational technology, high-efficiency HS imaging has been pursued in cooperation with image post-processing. In this review, the historical evolution of HS imaging is described focusing on spectroscopic techniques. An up-to-date HS imaging technique, computational HS imaging using a spatial-spectral random coded mask, is introduced with a brief explanation of its working principle. The HS imaging technique demonstrates outstanding characteristics in terms of sensitivity, spatial resolution, spectral accuracy, and frame rate. Several applications of HS imaging are introduced showing improved accuracy of image analysis compared to traditional RGB image analysis. Finally, the remaining challenges and prospects are discussed.

高光谱成像是一种获取物体详细光谱信息的技术,在遥感、农业、生物医学等领域引起了广泛的关注。在HS成像的初期,HS成像主要依靠耗时的扫描技术来实现高空间和光谱分辨率,限制了其适用性。随后,快照(非扫描)HS成像出现,实现了高速捕获。快照方法在一次曝光中捕获高分辨率图像,但其缺点是空间分辨率较低。随着计算机技术的进步,高效的HS成像与图像后处理相结合。本文综述了HS成像的历史演变,重点介绍了光谱技术。介绍了一种最新的HS成像技术——基于空间光谱随机编码掩模的计算HS成像技术,并简要说明了其工作原理。HS成像技术在灵敏度、空间分辨率、光谱精度和帧率等方面具有突出的特点。介绍了HS成像的几个应用,表明与传统的RGB图像分析相比,HS成像的图像分析精度得到了提高。最后,对未来面临的挑战和前景进行了展望。
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引用次数: 0
Performance analysis of 450/520 nm LD-PS based UOWC systems for IoUT applications across various water conditions using opti-system 使用opti-system对450/520 nm基于LD-PS的UOWC系统进行了性能分析,该系统可用于各种水条件下的IoUT应用
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-09-12 DOI: 10.1007/s10043-025-01002-w
M. Mokhtar Zayed, Mona Shokair

Underwater Optical Wireless Communication (UOWC) is a key enabler of the Internet of Underwater Things (IoUT), offering high-speed and low-latency data transmission in aquatic environments. However, system performance is highly sensitive to environmental factors such as absorption, scattering, turbulence, and noise. This study presents a comprehensive, simulation-based performance analysis and optimization of UOWC systems using Opti-System software, focusing on laser diodes operating at 450 nm and 520 nm. Four representative water types—pure seawater, clear ocean, coastal ocean, and turbid harbor—are examined to evaluate key performance metrics, including received power, Q-factor, eye diagrams, signal-to-noise ratio (SNR), bit error rate (BER), and transmission range. An environment-aware optimization framework is proposed, correlating wavelength selection and system configurations with the optical properties of each water type. The impact of transmitter power, beam divergence, photodetector sensitivity, and modulation (OOK) is assessed to identify optimal design choices for robust communication. Simulation results reveal that shorter wavelengths perform better in clearer waters, while adaptive tuning strategies significantly enhance reliability in highly scattering or turbulent conditions. This work provides practical design insights and optimization strategies to support scalable, efficient, and resilient UOWC systems for real-world IoUT applications.

水下光无线通信(UOWC)是水下物联网(IoUT)的关键推动因素,可在水下环境中提供高速、低延迟的数据传输。然而,系统性能对环境因素非常敏感,如吸收、散射、湍流和噪声。本研究使用Opti-System软件对UOWC系统进行了全面的、基于仿真的性能分析和优化,重点研究了工作在450 nm和520 nm的激光二极管。四种代表性的水类型——纯净海水、清澈海洋、沿海海洋和浑浊港口——被检查以评估关键性能指标,包括接收功率、q因子、眼图、信噪比(SNR)、误码率(BER)和传输范围。提出了一种环境感知优化框架,将波长选择和系统配置与每种水的光学性质相关联。评估了发射机功率、光束发散、光电探测器灵敏度和调制(OOK)的影响,以确定鲁棒通信的最佳设计选择。仿真结果表明,短波长在较清澈的水域中表现更好,而自适应调谐策略在高散射或湍流条件下显著提高了可靠性。这项工作提供了实用的设计见解和优化策略,以支持可扩展,高效和有弹性的UOWC系统用于现实世界的IoUT应用。
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引用次数: 0
Enhancement of spatial noise tolerance in single-pixel imaging with a feature-extended deep neural network 基于特征扩展深度神经网络的单像素图像空间噪声容忍度增强
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-09-08 DOI: 10.1007/s10043-025-00991-y
Taku Hoshizawa, Shinjiro Kodama, Chihiro Sato, Tomoaki Mizoguchi, Moe Sakurai, Eriko Watanabe

To compensate for time-fluctuating spatial noise and reconstruct an object image, a deep learning-based single-pixel imaging (SPI) system using a neural network consisting of five transposed convolutional layers and three convolutional layers has been developed. In the present study, we proposed a new image reconstruction method using deep learning with a feature-extended time-division pattern-learning (TDPL) network, which further increased the number of features in each layer to enhance the tolerance to time-fluctuating spatial noise. Simulations and experiments were performed to compare the performance of the proposed network with that of conventional methods, such as computational ghost imaging, Hadamard single-pixel imaging, deep convolutional auto-encoder network (DCAN), and TDPL network. We found that the image quality of the reconstructed image using the proposed method is superior to that of conventional methods in any environment with time-fluctuating spatial noise. For example, the quality of an object image reconstructed using the proposed method improved by − 0.037 and − 0.014 in a root-mean-square error and + 0.083 and + 0.005 in a structural similarity compared to that using the DCAN and TDPL network, respectively, under time-fluctuating spatial noise with a standard deviation of 0.5. Therefore, the proposed deep learning-based SPI system with a feature-extended TDPL network is expected to be applied to various imaging or observation in an environment where conditions are likely to change, such as astronomical observations, remote monitoring, and optical wireless communications.

为了补偿时间波动的空间噪声并重建目标图像,开发了一种基于深度学习的单像素成像(SPI)系统,该系统使用由5个转置卷积层和3个卷积层组成的神经网络。在本研究中,我们提出了一种新的图像重建方法,利用深度学习和特征扩展的时分模式学习(TDPL)网络,进一步增加每层特征的数量,以增强对时间波动空间噪声的容忍度。通过仿真和实验,比较了该网络与传统方法(如计算鬼影成像、Hadamard单像素成像、深度卷积自编码器网络(DCAN)和TDPL网络)的性能。结果表明,在任何具有时变空间噪声的环境下,采用该方法重建的图像质量都优于传统方法。例如,在标准偏差为0.5的时间波动空间噪声下,与DCAN和TDPL网络相比,使用该方法重建的目标图像的均方根误差分别提高了- 0.037和- 0.014,结构相似度分别提高了+ 0.083和+ 0.005。因此,本文提出的基于深度学习的具有特征扩展TDPL网络的SPI系统有望应用于天文观测、远程监测、光学无线通信等条件可能发生变化的环境下的各种成像或观测。
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引用次数: 0
Deep-learning-based rapid wavefront sensor using a line-scan camera 基于深度学习的快速波前传感器,采用线扫描相机
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-09-01 DOI: 10.1007/s10043-025-00999-4
Yohei Nishizaki, Katsuhisa Kitaguchi, Mamoru Saito, Jun Tanida

We present a rapid wavefront sensor based on machine learning and using a line-scan camera. The object light wave propagates through a scattering medium. In our method, the scattered light wave undergoes a series of preconditioning steps. The resultant light wave, in which only the wavefront aberration component is emphasized and the reference object light wave is removed, is captured as one-dimensional data using line focusing optics. The captured data are trained by a convolutional neural network, and the trained network can estimate the Zernike coefficients without iterative calculations. The proposed method achieves significantly faster measurement compared to a two-dimensional sensor. The proposed method was experimentally demonstrated, as a proof of concept, using a line-scan camera and a preconditioning method that we designed.

我们提出了一种基于机器学习和使用线扫描相机的快速波前传感器。物体光波通过散射介质传播。在我们的方法中,散射光波经过一系列预处理步骤。所得到的光波,其中只有波前像差分量被强调,参考对象光波被去除,被捕获为一维数据,使用线聚焦光学。利用卷积神经网络对捕获的数据进行训练,训练后的神经网络无需迭代计算即可估计出泽尼克系数。与二维传感器相比,该方法的测量速度明显加快。实验证明了该方法的概念,使用线扫描相机和我们设计的预处理方法。
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引用次数: 0
Pupil expansion prism and beam splitter array waveguide for high luminance and high resolution head-mounted display 用于高亮度和高分辨率头戴式显示器的瞳孔扩展棱镜和分束器阵列波导
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-08-18 DOI: 10.1007/s10043-025-00997-6
Toshiteru Nakamura, Takuma Kuno, Ryuji Ukai

Head-mounted displays (HMDs) for augmented reality (AR) require optical systems that deliver high luminance, high optical see-through performance, and high image resolution. Conventional two-directional pupil expansion using beam splitter array (BSA) waveguides often suffers from low light coupling efficiency and degraded image quality due to narrow coupling mirrors and wavefront disturbances caused by exposed mirror edges along the total internal reflection surface. We propose a novel HMD optical system that combines a pupil expansion (PE) prism with a one-directional BSA waveguide. The PE prism features an enlarged coupling surface, efficiently capturing light from the light engine. Importantly, the PE prism is designed to avoid exposed mirror edges in the optical path, thereby eliminating wavefront disturbances and enabling high-resolution virtual image projection. Within the PE prism, multiple ray paths are generated through complex reflections and transmissions via overlapping multi-mirrors. This multi-path propagation not only expands the eye-box orthogonally to the BSA waveguide, but also ensures uniform output luminance. A prototype HMD implementing the proposed method achieves high luminance (over 5000 cd/m2), high image resolution (MTF > 58% at 10 cycles/degree), high optical see-through transparency (over 94%), and luminance uniformity (over 53%). These results demonstrate significant improvements over conventional BSA waveguide approaches.

用于增强现实(AR)的头戴式显示器(hmd)需要提供高亮度、高光学透光性能和高图像分辨率的光学系统。利用分束器阵列(BSA)波导进行双向扩瞳时,由于耦合镜狭窄以及沿全内反射面暴露镜边缘引起的波前干扰,导致光耦合效率低,成像质量下降。我们提出了一种结合瞳孔扩展(PE)棱镜和单向BSA波导的新型HMD光学系统。PE棱镜具有放大的耦合表面,有效地捕获来自光引擎的光。重要的是,PE棱镜的设计避免了光路中暴露的镜像边缘,从而消除了波前干扰,实现了高分辨率的虚拟图像投影。在PE棱镜内,通过重叠的多镜反射和传输产生多种光线路径。这种多径传输不仅使眼盒与BSA波导正交扩展,而且保证了输出亮度均匀。实现该方法的HMD原型实现了高亮度(超过5000 cd/m2)、高图像分辨率(10周期/度时MTF >; 58%)、高光学透明度(超过94%)和亮度均匀性(超过53%)。这些结果表明,与传统的BSA波导方法相比,有了显著的改进。
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引用次数: 0
The interference of the evanescent mode of two Airy beams in near field 两艾里光束在近场中倏逝模式的干涉
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-08-03 DOI: 10.1007/s10043-025-00995-8
Ze Wang, Zhengling Wang

The exact analytical solution of the electric field of the Airy beam with a polarization in the x-direction is derived by the vector angular spectrum theory. And then, the evanescent interference of two symmetrically offset evanescent Airy beams is investigated by the angular spectrum theory in detail. Two separated Airy beams at the initial position will overlap and interfere due to the lateral self-acceleration. The y-axis interference field shows a superior stability and a slower decay compared to the x-axis. The interference optical field forms a spindle-shaped central optical field along the y-axis, and the intensity rapidly decays along the x-axis, and a small-scale scattered optical field is formed in the low-intensity regions on both sides. The result is useful to elucidating the formation mechanism and theoretical properties of the interference phenomenon of Airy beams.

利用矢量角谱理论,导出了具有x方向偏振的艾里光束电场的精确解析解。然后,利用角谱理论详细研究了对称偏移的两束倏逝Airy光束的倏逝干涉。两个分离的艾里梁在初始位置将重叠和干扰由于横向自加速度。与x轴相比,y轴干涉场具有更好的稳定性和更慢的衰减。干涉光场沿y轴方向形成纺锤形中心光场,强度沿x轴方向快速衰减,两侧低强度区域形成小尺度散射光场。该结果有助于阐明艾里光束干涉现象的形成机理和理论性质。
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引用次数: 0
Tailoring plasmonic and nonlinear optical response in ZnSe-based core–shell nanocomposites: influence of shell thickness and host matrix permittivity znse基核-壳纳米复合材料的等离子体和非线性光学响应:壳层厚度和基体介电常数的影响
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-08-01 DOI: 10.1007/s10043-025-00996-7
Shewa Getachew Mamo

This study presents a theoretical and numerical investigation of local field enhancement and optical bistability in ZnSe-based core–shell nanocomposites, providing insights for photonic applications. The structures consist of a ZnSe dielectric core and a metallic shell of either silver ((textrm{Ag})) or gold ((textrm{Au})), embedded in oxide matrices ((textrm{SiO}_2), (textrm{ZnO}), or (textrm{HFO}_2)) with varying permittivities. Using the quasi-static approximation and the Lorentz–Drude model, we analyze how variations in the core radius (keeping the outer radius fixed) influence spectral response and local field enhancement. Results show that smaller cores (thicker shells) yield stronger local field enhancement factors ((textrm{LFEF})) due to increased plasmonic confinement. Ag shells produce sharper, more intense resonances than Au, attributed to lower damping and superior plasmonic performance. The dielectric environment also plays a key role: low-permittivity matrices like (textrm{SiO}_2) support higher field localization, while high-permittivity ones such as (textrm{HFO}_2) weaken confinement and blue-shift the resonances. Nonlinear analysis reveals that thicker shells and lower matrix permittivity enhance bistability and reduce switching thresholds, particularly in Ag-based systems. These findings highlight the critical influence of geometry and material choice on both linear and nonlinear optical responses. The results offer practical guidance for engineering core–shell nanocomposites tailored for applications in photonic devices, optical sensors, and all-optical switching.

本研究对znse基核壳纳米复合材料的局部场增强和光学双稳定性进行了理论和数值研究,为光子应用提供了见解。该结构由ZnSe介电芯和银(Agtextrm{Ag})或金(Autextrm{Au})的金属壳组成,嵌入具有不同介电常数的氧化物基体(SiO2textrm{SiO}_2, ZnOtextrm{ZnO}或HFO2textrm{HFO}_2)中。利用准静态近似和洛伦兹-德鲁德模型,我们分析了核半径的变化(保持外半径固定)如何影响谱响应和局部场增强。结果表明,由于等离子体约束的增加,较小的核(较厚的壳)产生更强的局域场增强因子(LFEFtextrm{LFEF})。银壳比金壳产生更尖锐、更强烈的共振,这归因于较低的阻尼和优越的等离子体性能。介质环境也起着关键作用:低介电常数矩阵如SiO2textrm{SiO}_2支持较高的场局域化,而高介电常数矩阵如HFO2textrm{HFO}_2削弱约束和蓝移共振。非线性分析表明,更厚的壳层和更低的基体介电常数增强了双稳性,降低了开关阈值,特别是在银基系统中。这些发现突出了几何形状和材料选择对线性和非线性光学响应的关键影响。研究结果为工程核壳纳米复合材料在光子器件、光学传感器和全光开关中的应用提供了实际指导。
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引用次数: 0
New periodic wave solution for time-fractional perturbed nonlinear Schrödinger equation arising in optical fiber via newly extended mapping scheme 光纤中时间分数阶摄动非线性Schrödinger方程的新周期波解
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-07-31 DOI: 10.1007/s10043-025-00994-9
Loubna Ouahid, M. A. Abdou, Dhafer O. Alshahrani, Ali Akgül

In this study, we investigate the time-fractional perturbed nonlinear Schrödinger equation in the context of optical fibers using the newly extended mapping scheme. As a result, many types of traveling wave solutions are obtained, including novel solitary wave solutions, triangular, hyperbolic, and periodic wave solutions expressed in terms of Jacobi elliptic functions. Solutions are obtained as well in the limiting cases for (ell) approach 0 or 1. By assigning specific values to the free parameters, the physical significance of the 2D and 3D geometric shapes of the derived solutions is discussed, and the corresponding physical variations are illustrated. This work demonstrates the applicability of the proposed method to a broader class of nonlinear evolution equations in physics and engineering.

在这项研究中,我们使用新的扩展映射格式研究了光纤背景下的时间分数阶摄动非线性Schrödinger方程。结果,得到了多种类型的行波解,包括新颖的孤波解、三角形、双曲和以Jacobi椭圆函数表示的周期波解。在极限情况下,也得到了解。通过赋予自由参数特定的值,讨论了导出解的二维和三维几何形状的物理意义,并说明了相应的物理变化。这项工作证明了所提出的方法在物理和工程中更广泛的非线性演化方程中的适用性。
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引用次数: 0
Self-supervised neural reconstructions for lensless imaging 无透镜成像的自监督神经重建
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-07-30 DOI: 10.1007/s10043-025-00992-x
Jose Reinaldo Cunha Santos Aroso Vieira Silva Neto, Hodaka Kawachi, Yasushi Yagi, Tomoya Nakamura

Recent advances in lensless imaging reconstruction have primarily relied on supervised neural models trained using target images captured by lensed cameras via a beam splitter. However, we argue that using reference images from a different optical system introduces bias into the reconstruction process. To mitigate this issue, we propose a self-supervised approach that leverages data-fidelity guidance, similar to deep image prior, to train neural models for single-iteration lensless reconstruction. Through simulations and prototype camera experiments, we demonstrate that combining simple convex optimization methods with a denoising UNet improves perceptual quality (LPIPS), accelerates inference compared to traditional optimization techniques, and reduces potential unwanted biases in the reconstruction network.

无透镜成像重建的最新进展主要依赖于有监督的神经模型,该模型使用由有透镜相机通过分束器捕获的目标图像进行训练。然而,我们认为使用来自不同光学系统的参考图像会在重建过程中引入偏差。为了缓解这个问题,我们提出了一种自监督方法,利用数据保真度指导,类似于深度图像先验,训练神经模型进行单次迭代无透镜重建。通过模拟和原型相机实验,我们证明了将简单的凸优化方法与去噪UNet相结合可以提高感知质量(LPIPS),与传统优化技术相比可以加速推理,并减少重建网络中潜在的不必要的偏差。
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引用次数: 0
Design and performance of photon counting detector with charge coupling delay-line readout 电荷耦合延迟线读出光子计数探测器的设计与性能
IF 0.9 4区 物理与天体物理 Q4 OPTICS Pub Date : 2025-07-29 DOI: 10.1007/s10043-025-00982-z
Yalong Zhang, Yongan Liu, Xianghui Yang, Zhe Liu, Lizhi Sheng, Yue Li

Detectors based on cross delay-line (XDL) anodes with charge induction are widely applicable in space astronomical telescopes, deep space exploration, and fluorescence lifetime measurements. In this article, a three-dimensional structure XDL anode based on Printed Circuit Board (PCB) technology is proposed, which can conveniently realize high-resolution detection with a simple process and low cost. We theoretically studied the charge induction principle and established a model of the XDL anode through the finite element method. The model allows us to determine anode parameters, such as anode strip width, inter-strip distance, and substrate thickness, to optimize the output signal on the XDL anode, thereby indirectly affecting the resolution of the detector. Based on the experimental platform, we systematically characterized the key performance parameters of the detector. We conclude that the spatial resolution of the detector is better than 50 (upmu)m and the non-linearity is less than 5(%).

基于电荷感应交叉延迟线(XDL)阳极的探测器广泛应用于空间天文望远镜、深空探测和荧光寿命测量等领域。本文提出了一种基于印刷电路板(PCB)技术的三维结构XDL阳极,以简单的工艺和低廉的成本方便地实现高分辨率检测。从理论上研究了电荷感应原理,并通过有限元方法建立了XDL阳极的模型。该模型允许我们确定阳极参数,如阳极带宽度、带间距离和衬底厚度,以优化XDL阳极上的输出信号,从而间接影响检测器的分辨率。在实验平台的基础上,对探测器的关键性能参数进行了系统表征。结果表明,该探测器的空间分辨率优于50 μμ upmum,非线性小于5%。
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引用次数: 0
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Optical Review
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