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1.
以捷径法提高射线追踪效率   总被引:2,自引:0,他引:2       下载免费PDF全文
为改善计算效率,提出了一种捷径法对射线追踪法进行改进. 射线追踪的计算时间主要耗费在求交判断上. 通过实际计算并记录一条射线管的轨迹,作为其后若干条射线管求交计算的优先参考,避免了再次进行漫无目的的遍历式求交,从而大量减少进行实际计算的射线管数量,节省射线求交运算时间. 经编程计算验证,该优化算法能够在保证相当精度的前提下,大幅度提高射线追踪法的计算效率,具备一定的实用价值.   相似文献   

2.
邻域辅助径迹法提高射线追踪效率   总被引:1,自引:1,他引:1       下载免费PDF全文
针对面元形式的目标数据,从提高入射点求解的成功率着手,采用增加对参考路径上参考面元的相邻单元进行相交性判断的方法,并将普通径迹法的单参考路径改为双参考路径,提高了径迹法射线追踪的效率.对邻域辅助径迹法在样条曲面格式目标文件上的应用作了探讨.分析了该方法与其它方法的兼容性和对计算资源的占用情况,给出了该方法提高射线追踪速度的上限.以2个典型目标为例,对该方法的效果进行了测试.结果表明,该方法通过减少真实、遍历式追踪的次数,能将普通径迹法射线追踪过程的计算量减少到原来的1/3左右.该方法对目标具有很强的适应性,并克服了普通径迹法对射线管的划分密度的依赖性.   相似文献   

3.
低RCS齿形挂架参数选择研究   总被引:4,自引:2,他引:2       下载免费PDF全文
常规飞机的机翼与外挂架构成90°的二面角,成为飞机侧向的重要散射源.为求在不改变机体结构的前提下减缩飞机侧向RCS,采用齿形方案改变了挂架外形,消除了直角二面角结构,削弱了耦合效应.计算结果显示,改形的国产某型战斗机的机翼-外挂架结构的RCS在侧向重点姿态角内降低了9~13dBsm,证明了齿形改形方案能明显改善飞机侧向的耦合散射效应.在计算过程中使用了射线追踪法.   相似文献   

4.
随着移动通信技术和物联网的快速发展,预测室内短距离无线通信网络的信号覆盖情况成为当前的研究热点。基于十射线模型,自主开发了一种改进射线跟踪模型算法。该模型方法对微波室内传播提供可视化场景模拟,实现了室内短距离无线电波的传播预测和电磁波场强可视化。在多种场景测试并与其他室内电波传输模型对比,结果显示经过校准的模型均方根误差降低至5.53,准确度更高,能够更准确地预测室内环境中的信号接收功率。  相似文献   

5.
电离层短波射线追踪   总被引:10,自引:0,他引:10  
本文以电离层等离子体参量的平均背景模式计算为基础, 给出一种电离层短波射线轨迹计算方法。供短波通信系统、工作于短波段的其它系统(如HF雷达的目标定位系统)及有关研究工作使用参考。  相似文献   

6.
用射线法研究复杂目标的电磁散射特征   总被引:1,自引:0,他引:1       下载免费PDF全文
应用计算机图形学中的曲面造型方法给出目标精确的数学外形,将之离散为三角面元,并采用拓扑结构来描述几何元素之间的关系;利用射线追踪法模拟射线束的多次反射,同时求出扩散因子、磁场方向和相位差;在最终反射点处采用物理光学积分求远场散射,叠加每一射线束的贡献,进而得出耦合雷达散射截面值.为减小射线追踪过程中的计算量,采用了加速算法.给出了作为特例的翼身组合体的计算结果.  相似文献   

7.
在国际参考电离层模型和多层准抛物模型的基础上,提出了一种混合应用两种模型进行电离层建模的新方法.利用射线追踪技术,分别对混合模型和传统国际参考电离层模型下短波射线在电离层中的轨迹进行了仿真,得到了电波群路径.通过与实测电波群路径的对比,结果表明:对中国中纬度地区在电离层混合模型下的射线追踪精度优于传统国际参考电离层模型下的射线追踪精度,同时混合建模方法降低了多层准抛物模型对输入条件的要求,扩展了多层准抛物模型在射线追踪技术中的应用范围.  相似文献   

8.
研究和分析了脉冲星定位方法中的绝对定位法。通过一系列的公式和图表详细分析了定位算法的理论依据,同时还对整周模糊度问题的解算进行了研究。最后,利用MATLAB建立了一个简单模型,对定位算法进行仿真。结果表明定位准确度与星载原子钟准确度、脉冲星相位模型准确度以及相位观测误差有直接联系。  相似文献   

9.
针对现有的ORB特征匹配算法在图像模糊、光照变化、图像压缩、噪声条件下,匹配准确率下降问题,提出了一种改进的ORB特征匹配算法。首先,在提取特征点过程中,对图像进行网格化处理,并引入四叉树结构,使提取的特征点在图像中均匀分布,解决传统的特征提取方法遇到的特征点集中问题。然后,利用暴力匹配进行初步匹配,并采用交叉验证的方式,剔除部分误匹配,改善暴力匹配的结果。最后,利用高斯核对网格运动统计的结果做加权处理,优化统计结果,进一步剔除误匹配,得到准确率更高的匹配集合。实验结果表明:改进后的算法在图像模糊、光照变化、图像压缩和噪声条件下,平均准确率分别提高了3.5%、4.2%、2.2%和6%。   相似文献   

10.
一种新颖的ICT扫描方式及其FBP重构算法   总被引:2,自引:2,他引:2       下载免费PDF全文
计算机层析成像检测的突出问题是获取一幅图像的时间太长.为了缩短较大尺寸构件层析成像检测的二代(TR,Transverse Rotation)扫描时间,讨论了一种准三代(RR,Rotation and Rotation)扫描的概念,推导了它的滤波反投影算法. 计算机模拟结果证明了该算法的正确性. 分析表明,在同样检测条件下,它的扫描速度将比TR提高3倍以上.   相似文献   

11.
    
Poor angular resolution of present day gamma ray telescopes (1° at 100 MEV) together with the complicated gamma ray sky structures at compareable angular extents and poor statistics available necessitate the selection of those gammas which will increase the observable signal from a suspected source. A method for such a selection using the pre-known time signature of the source as its signal, has been developed (Özel and Mayer-Haβelwander, 1983). In an iterative procedure based on the improvement of source signal, generalized zones around the source are defined, from which gamma rays should be accepted to construct the optimum light curve of the source. These zones depend on the energy of the probed gamma rays, on the spatial structure and intensity of the background around the source, on the (estimated and/or tentative) intetnsity of the source and finally on the observing instrument's angular and energy response functions. The method, when applied to simulated and observed COS-B data demonstrated its feasibility and merits over the previonsly used circular event-acceptance cones method which was the basis of searches for gamma ray emission from radio pulsars (see for example Kniffen et al., 1974; Ögelman, et al. 1976; Kanbach, et al., 1977; and references therein). Present method does not introduce “trials” which usually reduce the significance of the results obtained, fully accounts the available knowledge on the topography of gamma ray sky, makes use of all the information about the sky, source and the instrument and therefore is the proper way of handling gamma ray data in pulsar-type searches.Presently, method is applied in the analyses of COS-B data in the context of searches for gamma ray emitting X-ray and radio pulsars. Results will be published elsewhere.  相似文献   

12.
    
A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs during transient events at different space/time scales. In this paper we present the detector and analyze observations made during one full year. After the analysis and correction of the GCR flux variability due to the atmospheric conditions (pressure and temperature), a study of the periodicities is performed in order to analyze modulations due to heliospheric phenomena. We can observe two periods: (a) 1 day, associated with the Earth’s rotation combined with the spatial anisotropy of the GCR flux; and (b) 30 days due to solar impact of stable solar structures combined with the rotation of the Sun. From a superposed epoch analysis, and considering the geomagnetic effects, the mean diurnal amplitude is 0.08% and the maximum flux is observed in 15 h local time (LT) direction in the interplanetary space. In such a way, we determine the capability of Neurus to observe anisotropies and other interplanetary modulations on the GCR flux arriving at the Earth.  相似文献   

13.
Launched from McMurdo (Antarctica) in December 2005, the balloon experiment CREAM (cosmic ray energetics and mass) collected about 15 million triggers during its second flight of 28 days. Redundant charge identification, by two pixelated silicon arrays and a time resolved pulse shaping technique from a scintillator system, allowed a clear signature of the primary nuclei. The energy was measured with a tungsten/SciFi calorimeter preceded by a graphite target. Preliminary results from the analysis of the data of the second flight are presented.  相似文献   

14.
This paper researches on Synthetic Aperture Radar (SAR) ocean wind retrieval approach, evaluates the method of Damped Newton VARiational method (DNVAR) and the direct method (DIRECT) using two years’ real SAR data and different background winds. Experiments are carried out using SENTINEL-1 SAR information as observation, National Data Buoy Center (NDBC) buoy data as in-situ data, Global Forecast System (GFS), Advanced SCATterometer (ASCAT), WindSAT, and Cross-Calibrated Multi-Platform (CCMP) wind products as background data. Thousands of match-ups are extracted. Results show that DNVAR can improve the wind field accuracy when the background data is ASCAT and CCMP. Especially, DNVAR wind speed results are much better than the official product of SENTINEL-1 wind data. The background data is crucial to the wind field retrieval results, so high accuracy of background data could lead to high accuracy results.  相似文献   

15.
    
The discovery of direct evidences for the acceleration of high energetic particles at the shell supernova remnant RXJ1713.7-3946 underlined the need to calculate the cosmic ray (CR) distribution in the Galaxy on a spatial grid fine enough to resolve the changes in the CR density due to these kind of objects. It was shown before by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005] that the discrete nature (both in space and time) of super novae (SN) as sources of Galactic CR leads to CR spectra changing in space and time, resulting in a range of possible CR spectra at a given location in the Galaxy. As the most frequent SN types Ib and II are found within spiral arms, one can expect a significant difference of the range of possible spectra in and outside spiral arms. We investigate the variability of the local interstellar CR proton spectrum during the motion of the Sun in and out of spiral arms in its journey around the Galactic center. Using the code described by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005], the proton CR density in the Galaxy is calculated with high spatial and temporal resolution (75 pc in galactocentric radius r and azimuth φ at the position of the Sun and 20 pc in z (perpendicular to the galactic plane), with a time step of 1 kyr), assuming stochastically distributed point sources with a probability distribution that resembles the spiral structure of our Galaxy. We find the averaged CR flux outside the spiral arm to be about 50% of that inside a spiral arm. We further find spatial and temporal variations of the CR flux inside spiral arms.  相似文献   

16.
The deramp range migration algorithm (DRMA) for space-borne spotlight synthetic aperture radar (SAR) is presented, which is based on the two-step algorithm and range migration algorithm. The presented algorithm combines the advantages of SPECAN algorithm and range migration algorithm. Firstly, the presented algorithm performs a bulk azimuth raw data compression to achieve a pixel spacing no larger than the expected azimuth resolution of the fully focused image. Therefore, the azimuth spectral folding phenomenon is overcome. Secondly, the residual and precise focusing of the synthetic aperture radar data is achieved by applying the range migration algorithm. The space-borne SAR focusing parameters’ computation is also described in the paper. At the end of this paper, results are presented which confirm the validity of the presented algorithm.  相似文献   

17.
为了解决低轨SAR卫星对观测区域成像幅宽小、重访时间长的问题;研制了陆地探测四号01星。其是世界首颗高轨SAR卫星;利用地球同步轨道的轨位优势;对同一地点的重访周期由低轨SAR的天级提升为小时级;幅宽由低轨SAR的百千米级提升为千千米级;可为及时、有效实施灾害应急响应提供有力支持。围绕高轨微波成像的新体制;解决了高轨微波成像、超大功率星载微波发射、超大口径星载天线、多体大挠性高精度姿态稳定控制、万瓦级强脉冲高品质电源、载荷与平台一体化高效热管理、高轨星地一体化精密定轨等一系列关键技术;实现了快重访、大幅宽、全天时、全天候的观测能力。通过分析在轨测试数据;卫星获取的高轨SAR图像纹理清晰;质量良好;可满足防灾减灾、国土资源勘查等领域使用需求。  相似文献   

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