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331.
针对目前隐身飞行器外形雷达散射截面(RCS)难以准确计算的问题,提出了一种基于目标外形几何特征和矩量法的飞行器RCS算法.通过对矩量法阻抗矩阵元的理论分析,研究了物面感应电流随散射体表面曲率的变化规律,指出感应电流之间的耦合已成为影响隐身飞行器物面电流分布的重要因素,并且指出根据飞行器物面曲率分布可以预知强的感应电流耦合区域,利用这些强的电流耦合能够组成稀疏化的阻抗矩阵,从而实现飞行器RCS的快速求解.以金属双弧柱和典型隐身飞机外形为例,分析验证了物面曲率几何信息对计算结果精度的影响以及在提高计算效率方面的作用.数值结果表明该方法保持了与传统矩量法基本一致的计算精度,但计算时间仅为矩量法的7.2%. 相似文献
332.
介绍了某型卫星测控雷达的校飞设备以及这些设备在某型飞机上的安装方案,并对方案进行了分析,确保方案的可行性。 相似文献
333.
Jan Dousa Pavel Vaclavovic 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The Geodetic Observatory Pecný (GOP) routinely estimates near real-time zenith total delays (ZTD) from GPS permanent stations for assimilation in numerical weather prediction (NWP) models more than 12 years. Besides European regional, global and GPS and GLONASS solutions, we have recently developed real-time estimates aimed at supporting NWP nowcasting or severe weather event monitoring. While all previous solutions are based on data batch processing in a network mode, the real-time solution exploits real-time global orbits and clocks from the International GNSS Service (IGS) and Precise Point Positioning (PPP) processing strategy. New application G-Nut/Tefnut has been developed and real-time ZTDs have been continuously processed in the nine-month demonstration campaign (February–October, 2013) for selected 36 European and global stations. Resulting ZTDs can be characterized by mean standard deviations of 6–10 mm, but still remaining large biases up to 20 mm due to missing precise models in the software. These results fulfilled threshold requirements for the operational NWP nowcasting (i.e. 30 mm in ZTD). Since remaining ZTD biases can be effectively eliminated using the bias-reduction procedure prior to the assimilation, results are approaching the target requirements in terms of relative accuracy (i.e. 6 mm in ZTD). Real-time strategy and software are under the development and we foresee further improvements in reducing biases and in optimizing the accuracy within required timeliness. The real-time products from the International GNSS Service were found accurate and stable for supporting PPP-based tropospheric estimates for the NWP nowcasting. 相似文献
334.
A. Borgazzi A. Lara G. Paz J.P. Raulin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
In order to detect and study the ionospheric response to solar flares (transient high energy solar radiation), we have constructed a radio receiver station at Mexico City, which is part of the “Latin American Very low frequency Network” (LAVNet-Mex). This station extends to the northern hemisphere the so called “South American VLF Network”. 相似文献
335.
First results of operational ionospheric dynamics prediction for the Brazilian Space Weather program
Adriano Petry Jonas Rodrigues de Souza Haroldo Fraga de Campos Velho André Grahl Pereira Graham John Bailey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
It is shown the development and preliminary results of operational ionosphere dynamics prediction system for the Brazilian Space Weather program. The system is based on the Sheffield University Plasmasphere–Ionosphere Model (SUPIM), a physics-based model computer code describing the distribution of ionization within the Earth mid to equatorial latitude ionosphere and plasmasphere, during geomagnetically quiet periods. The model outputs are given in a 2-dimensional plane aligned with Earth magnetic field lines, with fixed magnetic longitude coordinate. The code was adapted to provide the output in geographical coordinates. It was made referring to the Earth’s magnetic field as an eccentric dipole, using the approximation based on International Geomagnetic Reference Field (IGRF-11). During the system operation, several simulation runs are performed at different longitudes. The original code would not be able to run all simulations serially in reasonable time. So, a parallel version for the code was developed for enhancing the performance. After preliminary tests, it was frequently observed code instability, when negative ion temperatures or concentrations prevented the code from continuing its processing. After a detailed analysis, it was verified that most of these problems occurred due to concentration estimation of simulation points located at high altitudes, typically over 4000 km of altitude. In order to force convergence, an artificial exponential decay for ion–neutral collisional frequency was used above mentioned altitudes. This approach shown no significant difference from original code output, but improved substantially the code stability. In order to make operational system even more stable, the initial altitude and initial ion concentration values used on exponential decay equation are changed when convergence is not achieved, within pre-defined values. When all code runs end, the longitude of every point is then compared with its original reference station longitude, and differences are compensated by changing the simulation point time slot, in a temporal adjustment optimization. Then, an approximate neighbor searching technique was developed to obtain the ion concentration values in a regularly spaced grid, using inverse distance weighting (IDW) interpolation. A 3D grid containing ion and electron concentrations is generated for every hour of simulated day. Its spatial resolution is 1° of latitude per 1° of longitude per 10 km of altitude. The vertical total electron content (VTEC) is calculated from the grid, and plotted in a geographic map. An important feature that was implemented in the system is the capacity of combining observational data and simulation outputs to obtain more appropriate initial conditions to the ionosphere prediction. Newtonian relaxation method was used for this data assimilation process, where ionosonde data from four different locations in South America was used to improve the system accuracy. The whole process runs every day and predicts the VTEC values for South America region with almost 24 h ahead. 相似文献
336.
针对目前合成孔径雷达(SAR)目标模拟器通常只能模拟点目标,且通用化程度和实时性较低的问题,提出了一种基于商用现成品或技术(COTS)的SAR分布式目标模拟方法。利用NI PXI平台构建了一个基于电磁仿真的SAR分布式目标模拟器,由电磁仿真软件模拟获取目标散射特性,并通过高速网口输入硬件设备进行采样及卷积操作得到仿真SAR回波数字信号,经数模转换模块完成对SAR数字信号的调制并输出模拟回波,可以直接用于SAR系统的数据验证。模拟器采用数字式一体化硬件设备,由NI PXIe-5646R和PXIe-5840进行信号的接收和发送,PXIe-7902作为系统核心进行高速实时数据运算。系统以现场可编程门阵列(FPGA)为核心,通过LabVIEW RT (Real Time)和FPGA模块直接进行访问,能实时、高速地采集和处理数据。经过测试,该目标模拟器可以生成分布式目标的射频回波信号,环路验证结果证明了本文提出方法的有效性。另外,本文提出的方法适用于多种雷达信号的模拟,通过设置不同的信号体制或接收外部信号输入,可以实现灵活的SAR目标模拟。 相似文献
337.
338.
Jian Huang Weidong Hu Mounir Ghogho Qin Xin Xiaoyong Du Weiwei Guo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The increase in space debris can seriously threaten regular activities in the Low Earth Orbit (LEO) environment. Therefore, it is necessary to develop robust, efficient and reliable techniques to understand the potential motions of the LEO debris. In this paper, we propose a novel signal processing approach to detect and estimate the motions of LEO space debris that is based on a fence-type space surveillance radar system. Because of the sparse distribution of the orbiting debris through the fence in our observations, we formulate the signal detection and the motion parameter estimation as a sparse signal reconstruction problem with respect to an over-complete dictionary. Moreover, we propose a new scheme to reduce the size of the original over-complete dictionary without the loss of the important information. This new scheme is based on a careful analysis of the relations between the acceleration and the directions of arrival for the corresponding LEO space debris. Our simulation results show that the proposed approach can achieve extremely good performance in terms of the accuracy for detection and estimation. Furthermore, our simulation results demonstrate the robustness of the approach in scenarios with a low Signal-to-Noise Ratio (SNR) and the super-resolution properties. We hope our signal processing approach can stimulate further work on monitoring LEO space debris. 相似文献
339.
Tanvir Islam Miguel A. Rico-RamirezDawei Han Prashant K. Srivastava 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The separation of rain types in convective and stratiform regimes has long been a goal in microwave remote sensing of precipitation research. In this essence, a dual polarized radar based indexing scheme that provides information on convective and stratiform (C/S) rain regimes has been presented in correspondence with advanced microwave scanning radiometer – earth observing system (AMSR-E) GSFC profiling algorithm estimate of convective rain percentage. The dual polarized radar based C/S indexing scheme first retrieves the normalized gamma drop size distribution parameters, median volume drop diameter (D0) and concentration parameter (Nw), from dual polarized radar measurements ZH and ZDR, representing reflectivity and differential reflectivity respectively, by means of the genetic programming approach. Next, the C/S rain index is calculated based on the formulation of an empirical relation in Nw–D0 domain. The scheme has been inspected and applied on measurements from the S-band Chilbolton dual polarized radar. A considerable number of “coincident” cases from the radar and the AMSR-E observations are investigated. It has been revealed that the dual polarized radar based C/S rain indexing is in a similar pattern with the AMSR-E GSFC profiling algorithm estimate of convective rain percentage. Generally, as C/S rain index value increases, which signifies a stratiform to convective trend, the AMSR-E convective rain percentage also increases. 相似文献
340.
从机组运行和机务维修两个方面对气象雷达失效的放行限制进行了综合的分析评估,并对气象雷达系统进行由简到繁的排故介绍,为航线放行提供参考。 相似文献