Based on the ERA-40 reanalysis data from the European Centre for Medium-Range Weather Forecasts and the output of ECHAM5/MPI-OM, this study investigated the interactions between the quasi-stationary planetary wave （...Based on the ERA-40 reanalysis data from the European Centre for Medium-Range Weather Forecasts and the output of ECHAM5/MPI-OM, this study investigated the interactions between the quasi-stationary planetary wave （SPW） and mean flow, and their responses to E1 Nifio-Southern Oscillation （ENSO） events in the northern hemispheric stratosphere. Results show that the activity of SPW is the strongest in winter, when the SPW propagates along the polar waveguide into the stratosphere and along the low-latitude waveguide to the subtropical tropopause. The analysis of three dimensional SPW structure indicates that the main sources of SPW activity are located over the Eurasian continent and the North Pacific north of 45°N. On the one hand, the two waveguides of the SPW reflect the influence of mean flow on the propagation of the SPW. On the other hand, the upward propagating SPW can interact with the stratospheric mean flow, leading to deceleration of the zonal mean westerly. Furthermore, the SPW exhibits clear responses to ENSO events. During E1 Nifio winters, the SPW in the strat- osphere tends to propagate more upward and poleward. Its interactions with mean flow can induce a dipole pattern in zonal mean zonal winds, with accelerated westerly winds at low-middle latitudes and decelerated westerly winds at high latitudes. The ECHAM5/MPI-OM model reproduces the climatology of the SPW well. Although the simulated SPW is slightly weaker than the observations in the stratosphere, the model＇s performance has significant improvements compared with other GCMs used in previous studies. However, there are still some problems in the responses of the SPW to ENSO in the model. Although the model reproduces the responses of both the amplitude and the SPW-mean flow interactions to ENSO well in the troposphere, the stratospheric responses are quite weak. Therefore, further studies are needed to improve the simulation of the stratospheric atmospheric circulation and related dynamical processes.展开更多
Based on the traditional theory of wave mean flow interaction, an improved quasi-geostrophic Eliassen-Palm flux with diabatic heating included is deduced. It is shown that there exists an intrinsic relation between th...Based on the traditional theory of wave mean flow interaction, an improved quasi-geostrophic Eliassen-Palm flux with diabatic heating included is deduced. It is shown that there exists an intrinsic relation between the atmospheric energy cycle derived by Lorenz and the wave energy transfer derived by Eliassen and Palm. From this relation it becomes clear that the energy propagation process of large-scale stationary wave is indeed a part of Lorenz energy cycle, and the energy transform from mean flow to wave equals the global mass integral of the divergence of local wave energy flux or the global integral of local wave energy. The diagnostic results by using NCEP/NCAR reanalysis data suggest that the classical adiabatic Eliassen-Palm flux relation can present only the wintertime wave energy transformation. For other seasons, however, the diabatic effect must be taken into account.展开更多
针对传统波方程全波形反演步骤繁琐、计算量大和难度高等问题,提出一种基于全连接神经网络的早至波反演方法。实验结果表明,所提方法在早至波反演中交并比IoU(Intersection over Union)和平均精度均值mAP(mean Average Precision)分别达...针对传统波方程全波形反演步骤繁琐、计算量大和难度高等问题,提出一种基于全连接神经网络的早至波反演方法。实验结果表明,所提方法在早至波反演中交并比IoU(Intersection over Union)和平均精度均值mAP(mean Average Precision)分别达到74.01%和73.72%,可对速度模型进行有效重构。展开更多
短波通信原理简单,已广泛应用于大型无线通信系统。但在实际应用中,很多因素会影响短波通信,造成数据干扰,因此应采取有效的控制措施。基于此,分析短波通信的基本内容与主要特点,并在剖析短波通信干扰的基础上,分别从短波通信信号特征...短波通信原理简单,已广泛应用于大型无线通信系统。但在实际应用中,很多因素会影响短波通信,造成数据干扰,因此应采取有效的控制措施。基于此,分析短波通信的基本内容与主要特点,并在剖析短波通信干扰的基础上,分别从短波通信信号特征提取、干扰数据识别、数据干扰控制及实验测试4个方面,探讨基于最小均方(Least Mean Square,LMS)的短波通信数据干扰控制技术。展开更多
基金supported by National Basic Research Program of China(Grant No. 2010CB428603)National Natural Science Foundation of China (Grant Nos. 41025017 and 40775035)
文摘Based on the ERA-40 reanalysis data from the European Centre for Medium-Range Weather Forecasts and the output of ECHAM5/MPI-OM, this study investigated the interactions between the quasi-stationary planetary wave （SPW） and mean flow, and their responses to E1 Nifio-Southern Oscillation （ENSO） events in the northern hemispheric stratosphere. Results show that the activity of SPW is the strongest in winter, when the SPW propagates along the polar waveguide into the stratosphere and along the low-latitude waveguide to the subtropical tropopause. The analysis of three dimensional SPW structure indicates that the main sources of SPW activity are located over the Eurasian continent and the North Pacific north of 45°N. On the one hand, the two waveguides of the SPW reflect the influence of mean flow on the propagation of the SPW. On the other hand, the upward propagating SPW can interact with the stratospheric mean flow, leading to deceleration of the zonal mean westerly. Furthermore, the SPW exhibits clear responses to ENSO events. During E1 Nifio winters, the SPW in the strat- osphere tends to propagate more upward and poleward. Its interactions with mean flow can induce a dipole pattern in zonal mean zonal winds, with accelerated westerly winds at low-middle latitudes and decelerated westerly winds at high latitudes. The ECHAM5/MPI-OM model reproduces the climatology of the SPW well. Although the simulated SPW is slightly weaker than the observations in the stratosphere, the model＇s performance has significant improvements compared with other GCMs used in previous studies. However, there are still some problems in the responses of the SPW to ENSO in the model. Although the model reproduces the responses of both the amplitude and the SPW-mean flow interactions to ENSO well in the troposphere, the stratospheric responses are quite weak. Therefore, further studies are needed to improve the simulation of the stratospheric atmospheric circulation and related dynamical processes.
基金the Chinese Academy of Sciences(Grant No.ZKCX2-SW-210) the National Natural Science Foundation of China(Grant Nos.40405016,40475027,40135020,40221503 , 40023001).
文摘Based on the traditional theory of wave mean flow interaction, an improved quasi-geostrophic Eliassen-Palm flux with diabatic heating included is deduced. It is shown that there exists an intrinsic relation between the atmospheric energy cycle derived by Lorenz and the wave energy transfer derived by Eliassen and Palm. From this relation it becomes clear that the energy propagation process of large-scale stationary wave is indeed a part of Lorenz energy cycle, and the energy transform from mean flow to wave equals the global mass integral of the divergence of local wave energy flux or the global integral of local wave energy. The diagnostic results by using NCEP/NCAR reanalysis data suggest that the classical adiabatic Eliassen-Palm flux relation can present only the wintertime wave energy transformation. For other seasons, however, the diabatic effect must be taken into account.
文摘针对传统波方程全波形反演步骤繁琐、计算量大和难度高等问题,提出一种基于全连接神经网络的早至波反演方法。实验结果表明,所提方法在早至波反演中交并比IoU(Intersection over Union)和平均精度均值mAP(mean Average Precision)分别达到74.01%和73.72%,可对速度模型进行有效重构。
文摘短波通信原理简单,已广泛应用于大型无线通信系统。但在实际应用中,很多因素会影响短波通信,造成数据干扰,因此应采取有效的控制措施。基于此,分析短波通信的基本内容与主要特点,并在剖析短波通信干扰的基础上,分别从短波通信信号特征提取、干扰数据识别、数据干扰控制及实验测试4个方面,探讨基于最小均方(Least Mean Square,LMS)的短波通信数据干扰控制技术。
