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面向星地激光通信的大气湍流预报研究进展(特邀)

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激光通信系统在大气环境下应用的性能受到严重制约,当激光在大气湍流中传输时,其波面会发生畸变.在激光通信系统中,对大气湍流相关参数进行预报可以提前对星地数据传输链路进行调度,避免建立无效的通信任务.此外,大气湍流预报在天文选址、光学遥感等领域也有重要价值.随着国内外相关工作的长期积累以及算力、观测设备等硬件的能力提升,当前科研人员已经提出了一些大气湍流预报方案.文中主要综述了国内外学者在大气湍流预报方面的研究进展,首先详细介绍了 目前应用比较广泛的中尺度数值预报技术,列举了使用中尺度数值预报方法对国内外典型区域的大气湍流进行预报的相关工作;然后介绍了深度学习方法在大气湍流预报中的应用情况,对其优势与局限性进行了讨论;最后介绍了 一种面向星地激光通信的大气相干长度短时预报方法.
Atmospheric optical turbulence prediction method for satellite-ground laser communication(invited)
Significance The prediction of atmospheric turbulence has great significance both in science and engineering,which provides key parameters and references for domains like astronomical observation,site selection,satellite-ground laser communication,and remote sensing.Especially in satellite-ground laser communication,predicting key parameters of atmospheric turbulence can schedule satellite-ground data transmission links in advance,and pre-deploy adaptive optical schemes to compensate turbulence effects,so as to establish effective communication links and suppress the performance degradation of data transmission.Therefore,atmospheric turbulence prediction is crucial and become an important issue,which needs to be addressed for most of laser scenarios in atmosphere.Progress This review consists of three sections.In the first section,firstly,the widely used meso-scale numerical prediction scheme to forecast atmospheric turbulence is introduced in detail.This scheme is accomplished by turbulence parameterization schemes,which establishes the relationship between the turbulence characteristics and the conventional meteorological parameters output from mesoscale meteorological model.Mesoscale meteorological model has been well developed,the most representative models include Meso-Nh(Non-hydrostatic mesoscale atmospheric model),MM5(Mesoscale Model 5),WRF(Weather Research & Forecasting Model)and Polar WRF.Many achievements have been made in turbulence parameterization schemes,including Hufmagel model,Tatarski model.Then,the relevant work of using mesoscale numerical prediction method to forecast atmospheric turbulence in typical regions is reviewed.The second section presents recent advances regarding deep learning in atmospheric turbulence prediction,and discusses its advantages and limitations.This section first introduces the research achievements of deep learning in meteorological forecasting,and then introduces the research advances of deep learning in atmospheric turbulence forecasting.Based on a large amount of data,deep learning scheme can establish a relationship between the input data and the target label without any prior formula.In atmospheric turbulence prediction,deep learning is used to establish the relationship between meteorological parameters and atmospheric turbulence parameters,but the prediction accuracy is also limited by the accuracy of meteorological parameters.In the third section,a short-time atmospheric coherence length prediction method called TsVMD-AR is introduced.TsVMD-AR model uses VMD(variational mode decomposition)algorithm and AR(autoregression)algorithm to forecast the short-term atmospheric coherence length.This scheme reduces the interference and coupling between the multi-scale feature information in the dataset,makes the complex internal features of the dataset easier to obtain.The results show that the established TsVMD-AR model is obviously superior to other models and is suitable for daily atmospheric turbulence prediction.Prospects We hope this review will provide more valuable information for people who is working in scenarios of laser applications in atmosphere turbulence,and inspire more wonderful ideas towards abilities of more accurate and faster turbulence grasp.

atmospheric turbulenceturbulence predictionC2n profileatmospheric coherent length

郭盈池、李浪、李晨、高春清、付时尧

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北京理工大学光电学院,北京 100081

光电成像技术与系统教育部重点实验室,北京 100081

信息光子技术工信部重点实验室,北京 100081

大气湍流 湍流预报 C2n廓线 大气相干长度

国家自然科学基金项目国家自然科学基金项目国家自然科学基金项目国家自然科学基金项目国家重点研发计划北京市自然科学基金项目

623750146235001111834001619050122022YFB36077001232031

2024

红外与激光工程
中国航天科工集团公司第三研究院第八三五八研究所

红外与激光工程

CSTPCD北大核心
影响因子:0.754
ISSN:1007-2276
年,卷(期):2024.53(3)
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