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Recognition of Opposite-in-sign Orbital Angular Momenta of Laser Beams in a Turbulent Atmosphere with Neural Networks 湍流大气中激光束反符号轨道角动量的神经网络识别
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700216
E. A. Bogach, E. V. Adamov, V. V. Dudorov, V. V. Kolosov

An approach to increasing the communication channel capacity by amplitude and phase modulation almost reaches its limits. An increase in the information capacity of data communication channels by using the orbital angular momentum (OAM) of laser beams for information encoding is currently an urgent problem. The use of this approach in atmospheric optical communication systems is limited by the distorting effect of atmospheric turbulence, which makes decoding difficult and reduces the data transfer rate. In addition, the intensity distributions of vortex beams with OAMs opposite in sign are identical in a homogeneous medium, which also limits the use of OAM sign for encoding information. This work analyzes fundamental possibility of neural networks for recognizing opposite in sign OAMs of vortex beams in a turbulent atmosphere only by intensity distributions. The study is based on numerical simulation of Laguerre-Gaussian beam propagation in a turbulent atmosphere and use of the derived intensity distributions for training and testing neural networks. It is been shown for the first time that neural networks enables recognizing opposite in sign OAMs of Laguerre-Gaussian beams propagation through a turbulent atmosphere by intensity distributions with an accuracy of more than 90%. The results can be useful for developers and researchers of atmospheric optical communication systems where OAMs of vortex beams are used.

一种通过幅度和相位调制来增加通信信道容量的方法几乎达到了极限。利用激光束的轨道角动量(OAM)进行信息编码,提高数据通信信道的信息容量是当前迫切需要解决的问题。这种方法在大气光通信系统中的应用受到大气湍流的扭曲效应的限制,这使得解码困难,降低了数据传输速率。此外,在均匀介质中,具有相反符号OAM的涡旋光束的强度分布是相同的,这也限制了使用OAM符号编码信息。本文分析了神经网络仅通过强度分布识别湍流大气中涡旋光束的反符号oam的基本可能性。该研究基于湍流大气中拉盖尔-高斯光束传播的数值模拟,并使用导出的强度分布来训练和测试神经网络。研究首次表明,神经网络能够通过强度分布识别拉盖尔-高斯光束在湍流大气中传播的反符号OAMs,精度超过90%。研究结果对大气光通信系统的开发和研究人员具有一定的参考价值。
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引用次数: 0
Effect of Gas Pressure on Spatial and Spectral Characteristics of a Femtosecond Laser Pulse during Its Filamentation 气体压力对飞秒激光成丝过程空间和光谱特性的影响
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700253
D. V. Apeksimov, P. A. Babushkin, Yu. E. Geints, A. M. Kabanov, V. K. Oshlakov, A. V. Petrov, A. A. Udalov, E. E. Khoroshaeva

Filamentation of high-power femtosecond pulses in a gas is of great theoretical and practical interest with relation to the study of large-scale spectral and temporal transformations of laser radiation in a medium and generation of extra-wide (supercontinuum) radiation. This radiation is of interest in nonlinear femtosecond diagnostics of environment, optical data transmission through an atmospheric channel, and modern optical material processing techniques. This paper experimentally studies the effect of gas medium (nitrogen) pressure in an optical cell on the characteristics of femtosecond laser radiation propagating under filamentation conditions. It is found that high nitrogen pressure (up to 11 atm) and sharp geometric focusing of femtosecond radiation result in its Kerr self-focusing, which transforms from the single filamentation mode into multiple post filamentation as the gas pressure increases. Due to the phase self-modulation of a femtosecond pulse and plasma generation in the gas, the radiation spectrum is significantly enriched and the pulse spectrum near-linearly broadens with an increase in the gas pressure in the cell. It is ascertained for the first time that the pulse spectrum asymmetrically broadens mainly to the long-wave region while the initial beam focusing sharpness is increasing. The average size of high-intensity post-filaments formed inside a beam decreases as the gas pressure increases in the optical cell and can be fractions of a millimeter.

高功率飞秒脉冲在气体中的成丝对于研究激光辐射在介质中的大尺度光谱和时间变换以及超宽(超连续统)辐射的产生具有重要的理论和实践意义。这种辐射在环境的非线性飞秒诊断、通过大气信道的光数据传输和现代光学材料处理技术中具有重要意义。实验研究了光腔内气体介质(氮气)压力对飞秒激光在成丝条件下传播特性的影响。研究发现,高氮气压力(高达11 atm)和飞秒辐射的锐利几何聚焦导致其克尔自聚焦,随着气体压力的增加,克尔自聚焦从单丝模式转变为多个后丝模式。由于飞秒脉冲的相位自调制和气体中等离子体的产生,辐射谱明显丰富,脉冲谱随着细胞内气体压力的增加而近线性变宽。首次确定了脉冲谱主要向长波区域不对称拓宽,同时初始光束聚焦锐度增大。光束内部形成的高强度后丝的平均尺寸随着光学电池中气体压力的增加而减小,可以是一毫米的几分之一。
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引用次数: 0
Energy Characteristics of a Copper Vapor Laser Pumped by a Marx Generator 马克思发生器抽运铜蒸气激光器的能量特性
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700332
H. A. Baalbaki, A. V. Malikov, N. A. Yudin

Energy characteristics of a copper vapor laser (CVL) pumped by a Marx generator are studied. The schematic of the generator is provided; features of its operational are described, since thyratrons are used as switches in the generator. It is shown that a Marx generator enables increasing the upper limit of stable operation of thyratrons (proportional to the number of thyratrons used; up to ∼ 8–10 kV of inverse voltage across the thyratron anodes for two thyratrons) and, hence, ensures active medium pumping parameters unattainable with a single thyratron. The pulse energy is shown to linearly increase with the voltage across a gas discharge tube (GDT) and decrease with the excitation pulse repetition rate. A CVL pumped by a Marx generator is a promising radiation source for high-altitude sensing of the atmosphere and creation of artificial guide stars in adaptive optics devices, active optical systems, and atmospheric bistatic communication channels.

研究了马克思发生器抽运铜蒸气激光器的能量特性。给出了该发电机的原理图;由于闸流管在发电机中用作开关,因此描述了其运行特性。研究表明,马克思发生器能够提高闸流管稳定运行的上限(与所使用的闸流管数量成正比;两个闸流管的闸流管阳极上的反向电压高达~ 8-10 kV),因此确保了单个闸流管无法实现的有效介质泵送参数。脉冲能量随气体放电管(GDT)电压的增加呈线性增加,随激励脉冲重复率的增加而减小。马克思发生器抽运的CVL是一种很有前途的辐射源,可用于自适应光学装置、有源光学系统和大气双基地通信信道的高空大气传感和人造导星的创建。
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引用次数: 0
Effect of Air Nanobubble Clusters on Optical Pulse Propagation in Water 空气纳米气泡团对光脉冲在水中传播的影响
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700204
V. F. Myshkin, V. A. Khan, S. F. Balandin, Cailun Wang, S. A. Sosnovsky

Development of mineral resources in the ocean presents the problem of high-speed communication between two underwater objects. Optical radiation provides the highest transmission rate. However, the turbidity of natural waters is strongly variable; therefore, the study of the effects of different components of water suspension on laser pulse transmission is relevant. In the work, propagation of 2-ns optical pulses at a wavelength of 0.514 μm in water containing only clusters of nanobubbles is simulated. The maximal flux of radiation scattered on nanobubble clusters at the entrance to a receiver is shown to be no higher than 10% of the radiation flux propagated without scattering along a path up to 150 m long; the pulse full width at half maximum decreases by no more than 30%. The restriction on the path length in water containing only clusters of nanobubbles is due to radiation attenuation. Our results can be used for prediction of the solar radiation penetration depth during diving operations in water bodies or analyses of images of underwater objects, as well as for the development and usage of equipment for open underwater optical telecommunication lines. The influence of organic and inorganic suspended matter on the laser radiation propagation in water is planned to be studied further.

海洋矿产资源的开发提出了两个水下物体之间高速通信的问题。光辐射的传输速率最高。然而,天然水的浑浊度变化很大;因此,研究不同成分的水悬浮液对激光脉冲传输的影响是有意义的。本文模拟了波长为0.514 μm的2ns光脉冲在仅含纳米气泡簇的水中的传播。在接收器入口处的纳米气泡团簇上散射的最大辐射通量显示不高于沿150 m长的路径传播的无散射辐射通量的10%;脉冲全宽在一半最大时减小不超过30%。在仅含有纳米气泡簇的水中,路径长度受到辐射衰减的限制。我们的研究结果可用于水体潜水作业时太阳辐射穿透深度的预测或水下物体图像的分析,也可用于开放式水下光通信线路设备的开发和使用。有机悬浮物和无机悬浮物对激光在水中传播的影响有待进一步研究。
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引用次数: 0
Temperature Dependence of Water Vapor Microwave Line Broadening 水蒸气微波谱线展宽的温度依赖性
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700228
V. I. Starikov

Results of solving the problem of determining the temperature dependence of the broadening coefficient of water vapor lines by pressure of different buffer gases are presented. The broadening coefficients γ have been calculated for 18 microwave absorption lines of H2O molecule broadened by N2, O2, CO2, air, H2O, CO2, He, Ar, Kr, and Xe pressure in the temperature range 30 ≤ T ≤ 400 K. The models of rectilinear, parabolic, and exact trajectories of colliding particles are used. It is shown that the calculated dependence γ(T) for T ( lesssim ) 100 K is determined by the calculation method and model of the trajectories of colliding particles; in the case of broadening by monatomic gases, these results strongly depend on the chosen interaction potential. The results of the work can be useful for spectral calculations required by atmospheric applications.

给出了用不同缓冲气体的压力确定水蒸汽管路展宽系数与温度的关系的结果。计算了在30≤T≤400k温度范围内,N2、O2、CO2、空气、H2O、CO2、He、Ar、Kr和Xe压力下,18条H2O分子微波吸收谱线的展宽系数γ。使用了直线、抛物线和精确粒子碰撞轨迹模型。结果表明,T ( lesssim ) 100 K的计算依赖γ(T)由粒子碰撞轨迹的计算方法和模型决定;在单原子气体展宽的情况下,这些结果强烈依赖于所选择的相互作用势。这项工作的结果可用于大气应用所需的光谱计算。
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引用次数: 0
Influence of Soil Moisture and Rainfall on the Efficiency of a Near-IR Hyperspectral Oil Pollution Detection Technique 土壤湿度和降雨量对近红外高光谱石油污染检测效率的影响
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700289
Minh Bach Nguyen, Yu. V. Fedotov, N. V. Baryshnikov, M. L. Belov

Monitoring of oil pollution of the land surface is one of the pressing ecological issues today. The work is devoted to the experimental study of hyperspectral technique for detecting oil pollution on the land surface in the near-IR. The spectral brightness coefficients of soil samples contaminated with different oil product types are experimentally measured in the 1.6–2.5 μm spectral range. The influence of soil moisture and rainfall on the reflection spectra of soils (several types of sand and soil from forest and park areas) contaminated by oil products (of Moscow and Samara oil processing plants, kerosene, gas condensate, various gasoline brands, motor oils, and diesel fuel) is studied. It is shown that spectral dips near 1.73 and 2.3 μm (typical for soils contaminated with oil products) in most cases remain in the reflectance spectra under conditions of moderately moist soil, moderate rain, and even heavy rain. A specially created neural network shows the probability of detecting oil pollution on the land surface to be more than 99% under conditions of moderately moist soil and moderate rain and more than 88% under conditions of heavy rain and moist soil for 14 spectral channels 10 nm wide in the 1.6–2.4 μm range. The results can be used in the development of pipeline leak remote monitoring systems.

陆地表面石油污染监测是当今最紧迫的生态问题之一。本文对近红外高光谱技术在陆地表面石油污染检测中的应用进行了实验研究。实验测量了不同油品污染土壤样品在1.6 ~ 2.5 μm光谱范围内的光谱亮度系数。研究了土壤湿度和降雨对被石油产品(莫斯科和萨马拉石油加工厂、煤油、凝析油、各种汽油品牌、机油和柴油)污染的土壤(来自森林和公园地区的几种沙子和土壤)反射光谱的影响。结果表明,在中等湿润土壤、中雨甚至暴雨条件下,反射光谱在1.73和2.3 μm附近(油品污染土壤的典型特征),大部分情况下仍保持在反射光谱中。特别建立的神经网络显示,在1.6 ~ 2.4 μm范围内,14个10 nm宽的光谱通道,在土壤中湿润和中雨条件下,对陆地表面油污的检测概率大于99%,在大雨和土壤潮湿条件下,检测概率大于88%。研究结果可用于管道泄漏远程监测系统的开发。
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引用次数: 0
Creation of an Extended Continuous Ionization Region in Atmospheric Aerosol by Laser Radiation 激光辐射在大气气溶胶中产生扩展连续电离区
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700265
S. F. Balandin, V. A. Donchenko, V. F. Myshkin, V. A. Pogodaev, V. A. Khan

To form plasma antennas in different radio and telecommunication devices it is necessary to increase the relaxation time of laser breakdown centers. To solve this problem, processes running in aerodisperse media with solid microparticles during interaction with laser radiation are considered. The decay time of plasma with aerosol particles under the action of nanosecond and microsecond laser pulses is analyzed. The effect of the electron shell around solid microparticles on the creation of a continuous ionization zone in an aerosol atmosphere formed by overlapping plasma halos around microparticles has been estimated. The conditions necessary for the generation of a long ionized channel by breakdown centers during explosive evaporation of atmospheric microparticles in the zone of action of a nanosecond CO2 laser pulse and the further maintenance of the generated plasma by microsecond laser radiation are considered. A scheme of an experimental setup for creating a long ionized channel in an aerosol atmosphere is suggested. The results can be used for creation of wireless communication channels in the atmosphere.

为了在不同的无线电和通信设备中形成等离子体天线,必须增加激光击穿中心的弛豫时间。为了解决这一问题,考虑了固体微粒在空气分散介质中与激光辐射相互作用的过程。分析了纳秒和微秒激光脉冲作用下气溶胶粒子等离子体的衰减时间。在微粒周围重叠的等离子体晕形成的气溶胶大气中,固体微粒周围的电子壳层对连续电离区产生的影响已被估计。讨论了纳秒级CO2激光脉冲作用区内大气微粒爆炸蒸发时击穿中心产生长电离通道的必要条件和微秒级激光辐射对等离子体的进一步维持。提出了在气溶胶大气中建立长电离通道的实验装置方案。研究结果可用于在大气中建立无线通信信道。
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引用次数: 0
Correction of Numerical Forecasts of Wind Gusts Using Artificial Neural Networks and Observations 利用人工神经网络和观测资料修正阵风数值预报
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700320
I. V. Del, A. V. Starchenko

In 2023, more than a third of dangerous weather events in the Siberian Federal District were associated with strong wind, which emphasizes the importance of improving the accuracy and timing of its forecasting. Modern numerical simulation and machine learning methods make it possible to improve forecasts; however, the task of direct calculation of wind gusts remains topical due to the limited resolution of models. An original method is proposed for correcting the results of short-term forecast of wind gusts obtained on the basis of mesoscale models of numerical weather forecasting using advance measurements and artificial neural networks. The results show that the proposed correction method makes it possible to improve the forecast of wind gusts by various semiempirical methods. The results can be applied in meteorology, energy engineering, transportation, and other industries to minimize damage from dangerous weather events.

2023年,西伯利亚联邦区超过三分之一的危险天气事件与强风有关,这强调了提高预报准确性和时间的重要性。现代数值模拟和机器学习方法使改进预测成为可能;然而,由于模型的分辨率有限,直接计算阵风的任务仍然是热门话题。提出了一种利用超前测量和人工神经网络对数值天气预报中尺度模式的短期阵风预报结果进行校正的新方法。结果表明,所提出的修正方法可以改进各种半经验方法对阵风的预报。研究结果可以应用于气象学、能源工程、交通运输和其他行业,以尽量减少危险天气事件造成的损害。
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引用次数: 0
Non-photochemical Formation of Atmospheric Hazes and Rate of Sulphate Accumulation in Them 大气雾霾的非光化学形成及其中硫酸盐积累速率
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S102485602570023X
G. B. Pronchev, A. N. Yermakov

Causes of occurrence of dense non-photochemical haze (smog) over Beijing in winter are still poorly understood. The purpose of the work is to study the catalytic oxidation of sulfur dioxide with molecular oxygen in aerosol particles and origination of dense non-photochemical haze. The rapid accumulation of ({text{SO}}_{4}^{{2 - }}) (tens of micrograms per m3 per h) is shown to occur only at high humidity and moisture acidity in particles (рН = 3.7–4.8) due to a transition of the catalytic (non-photochemical) air oxidation of SO2 with participation of Fe and Mn ions into a fast degenerate branched mode. Origination of hazard atmospheric haze should necessarily be simulated accounting this catalytic reaction. The results can be used in forecasting the occurrence of dense atmospheric hazes with the aim of minimizing their dangerous consequences for human health and environment.

北京冬季非光化学雾霾的成因尚不清楚。本研究的目的是研究二氧化硫在气溶胶颗粒中与分子氧的催化氧化和密集非光化学雾霾的起源。由于Fe和Mn离子参与的SO2的催化(非光化学)空气氧化转变为快速简并支链模式,({text{SO}}_{4}^{{2 - }})(数十微克每立方米每小时)的快速积累仅发生在颗粒(рН = 3.7-4.8)的高湿度和湿酸性条件下。考虑到这种催化反应,必须模拟有害大气霾的产生。这些结果可用于预测大气浓霾的发生,目的是尽量减少其对人类健康和环境的危险后果。
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引用次数: 0
Vertical Wind Speed Variations in the Polar Stratosphere of Northern Hemisphere from ERA5 Reanalysis Data and their Correlation with the Lunar Tide ERA5再分析资料的北半球极地平流层垂直风速变化及其与月潮的相关性
IF 0.9 Q4 OPTICS Pub Date : 2025-09-04 DOI: 10.1134/S1024856025700290
D. S. Khabituev, O. S. Zorkaltseva

The NH Earth polar stratospheric vortex significantly varies from year to year in winter, which periodically leads to the occurrence of sudden stratospheric warmings (SSWs). Such events significantly disturb the circulation and chemical composition of the polar stratosphere. Our understanding of the wave processes that are recorded in the stratosphere and are directly involved in the occurrence of SSWs remains incomplete to date. Oscillations of the polar stratosphere of the Northern Hemisphere in the period from 1979 to 2023 are studied based on ERA5 reanalysis data. The method of current spectra is used to study the variations in the periodicity of wave processes in the polar stratosphere for different time intervals. As the main indicator of the wave properties of the stratosphere, we use the field of the vertical component of the wind velocity in the region between 60° and 90° N. It is shown that in some years, oscillations of the stratosphere coincide with or are close to the periods of the main waves of the fortnightly and monthly lunar gravitational tide. The causes and consequences of the oscillatory processes synchronization in the polar stratosphere with the lunar gravitational tide are discussed. The results can be useful for improving the understanding of the mechanisms of occurrence of SSWs, as well as for improving the forecast of such events.

冬季北半球极地平流层涡旋的年际变化显著,周期性地导致平流层突然变暖的发生。这些事件极大地扰乱了极地平流层的环流和化学成分。迄今为止,我们对记录在平流层并直接参与ssw发生的波过程的理解仍然不完整。利用ERA5再分析资料,研究了1979 ~ 2023年北半球极地平流层的振荡。本文采用电流谱法研究了极地平流层波浪过程在不同时间间隔内的周期性变化。我们利用60°~ 90°n区域的风速垂直分量场作为平流层波动特性的主要指标。结果表明,在某些年份,平流层的振荡与两周和每月的月球引力潮的主波周期重合或接近。讨论了极地平流层振荡过程与月球引力潮同步的原因和后果。研究结果可用于提高对ssw发生机制的认识,以及改进此类事件的预报。
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引用次数: 0
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Atmospheric and Oceanic Optics
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