排序方式: 共有75条查询结果,搜索用时 15 毫秒
61.
62.
针对短码DSSS(Direct Sequence Spread Spectrum,直接序列扩频)信号扩频码MLE(Maximum Likelihood Estimation,最大似然估计)问题,提出了一种基于Viterbi算法的扩频码搜索方法,并将其应用到同步CDMA(Code Division Multiple Access,码分多址)信号的扩频码估计中.该算法利用了扩频码码元为±1的先验知识,以向量的2-范数平方或1-范数作为度量值;每次判决扩频码码元时,计算2条可能路径的度量值,并选择使度量值最大的那条路径作为幸存路径,最终的幸存路径即为估计的扩频码;所提算法不仅计算复杂度低,而且能同时估计扩频信号的扩频码和信息序列.仿真实验表明,本算法在低信噪比时同样具有较好的性能. 相似文献
63.
K.D. Moloto N.E. Engelbrecht R.D. Strauss D.M. Moeketsi J.P. van den Berg 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):626-639
Three-dimensional studies of the transport and modulation of cosmic ray particles in turbulent astrospheres require large-scale simulations using specialized scientific codes. Essentially, a multi-dimensional Fokker-Planck type equation (a parabolic diffusion equation) must be integrated numerically. One such approach is to convert the relevant transport equation into a set of stochastic differential equations (SDEs), with the latter much easier to handle numerically. Due to the growing demand for high performance computing resources, research into the application of effective and suitable numerical algorithms to solve such equations is needed. We present a case study of the performance of a custom-written FORTRAN SDE numerical solver on the CHPC (Centre for High Performance Computing) Lengau cluster in South Africa for a realistic test problem with different set-ups. It is shown that SDE codes can scale very well on large parallel computing platforms. Finally, we consider an extremely computationally expensive application of the SDE approach to cosmic ray modulation, studying the behaviour of galactic cosmic ray proton latitude gradients and relative amplitudes in a physics-first manner. This is done using a modulation code that employs diffusion coefficients derived from first principles, which in turn are functions of turbulence quantities in reasonable agreement with spacecraft observations and modelled using a two-component turbulence transport model (TTM). We show that this approach leads to reduced latitude gradients qualitatively in line with spacecraft observations of the same, without making ad hoc assumptions as to anisotropic perpendicular diffusion coefficients as are often made in many cosmic ray modulation studies. 相似文献
64.
A novel range-Doppler imaging algorithm with OFDM radar 总被引:1,自引:1,他引:0
《中国航空学报》2016,(2):492-501
Traditional pulse Doppler radar estimates the Doppler frequency by taking advantage of Doppler modulation over different pulses and usually it requires a few pulses to estimate the Doppler frequency. In this paper, a novel range-Doppler imaging algorithm based on single pulse with orthogonal frequency division multiplexing(OFDM) radar is proposed, where the OFDM pulse is composed of phase coded symbols. The Doppler frequency is estimated using one single pulse by utilizing Doppler modulation over different symbols, which remarkably increases the data update rate. Besides, it is shown that the range and Doppler estimations are completely independent and the well-known range-Doppler coupling effect does not exist. The effects of target movement on the performances of the proposed algorithm are also discussed and the results show that the algorithm is not sensitive to velocity. Performances of the proposed algorithm as well as comparisons with other range-Doppler algorithms are demonstrated via simulation experiments. 相似文献
65.
66.
Rui Tu Hongping Zhang Maorong Ge Guanwen Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
This paper proposes a method of real-time monitoring and modeling the ionospheric Total Electron Content (TEC) by Precise Point Positioning (PPP). Firstly, the ionospheric TEC and receiver’s Differential Code Biases (DCB) are estimated with the undifferenced raw observation in real-time, then the ionospheric TEC model is established based on the Single Layer Model (SLM) assumption and the recovered ionospheric TEC. In this study, phase observations with high precision are directly used instead of phase smoothed code observations. In addition, the DCB estimation is separated from the establishment of the ionospheric model which will limit the impacts of the SLM assumption impacts. The ionospheric model is established at every epoch for real time application. The method is validated with three different GNSS networks on a local, regional, and global basis. The results show that the method is feasible and effective, the real-time ionosphere and DCB results are very consistent with the IGS final products, with a bias of 1–2 TECU and 0.4 ns respectively. 相似文献
67.
FFT在高动态扩频信号捕获中的应用 总被引:13,自引:0,他引:13
讨论了采用FFT算法实现高动态扩频信号快捕的一种方法。该方法根据帕斯瓦尔定理,以频域多点能量之和作为观测量,对伪码同步和载波多普勒频点位置进行判断,消除了数据符号跳变和栅栏效应对FFT分析的影响。实验结果表明,该方法可以很好地实现高动态扩频信号的捕获,并可以有效地节省硬件资源。 相似文献
68.
讨论了一种伪随机码跟踪环的特性,分析了码相关间隔、预检积分时间、环路带宽及信噪比等参数对码跟踪性能的影响。该方案不仅能够对PN码相位的变化作出调整,同时对PN码多普勒进行跟踪,较适合于测控应答机中PN码跟踪环的应用。 相似文献
69.
70.
为解决时分数据调制(TDDM)方式而引发的信息码位符号翻转模糊问题,提出了一种基于影响因子的模糊抑制同步算法。首先通过搜索引导处理快速地解决伪码搜索范围大的问题;进一步,通过建立影响因子及分段处理,解决信息码符号翻转位置模糊问题。通过理论推导及仿真分析表明,新算法的翻转位置估计精度可以达到> 98.8% ;新算法与传统的PN算法比较,不但提高了估计精度,而且能够适应更低信噪比环境,同时降低了处理复杂度。 相似文献