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排序方式: 共有127条查询结果,搜索用时 93 毫秒
1.
相关系数平稳过程时频分析方法 总被引:9,自引:6,他引:9
相关系数平稳过程是从非平稳过程中分离出的一类工程上常见且便于研究的随机过程,其均值和方差都可随时间变化,传统的平稳随机过程是它的一个特例。本文提出了相关系数AR(p),MA(q)和ARMA(p,q)序列的概念,建立了相关系数平稳过程的时频分析方法。该方法首先在时域进行全程分析,得到相关系数平稳过程的均值函数、方差函数和相关系数函数,然后可以对其进行傅里叶变换、短时傅里叶变换或小波变换,给出相关系数平稳过程的谱密度,同时提出了随机项谱密度和趋势项谱密度的概念。文中还讨论了线性系统对相关系数平稳过程输入的响应。 相似文献
2.
本文提出了一种ARMAX模型参数估计的新两步法。这种方法与其它递推估计方法(如增广矩阵法,极大似然法,Durbin两步法、三步法等)比较,具有较好的收敛特性,对参数的估计,特别是对C参数的估计比较精确,这是利用其它方法,一直未能很好解决的一个难题。 相似文献
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战斗机对地攻击作战效能分析 总被引:13,自引:2,他引:13
运用马尔柯夫过程理论,建立了战斗机攻击地面目标的战场想定和数学模型.通过分析战斗机的作战生存特征、打击能力和所使用的进攻战术以及各种战场防空武器系统的物理特性和损伤机理,评估了任务成功率、目标被毁率、飞机损失率以及与费用相关的最优战斗时间等作战效能指标.给出了战斗机对地攻击作战效能的计算实例.结果表明所建模型客观地描述了对地攻击作战的实质. 相似文献
5.
Hamdi Habacha 《Spatial Cognition & Computation》2019,19(2):130-145
The involvement of motor processes in mental rotation is experience-dependent: different levels of expertise in sensorimotor interactions lead to different strategies in mental rotation. In the present study, wrestlers, gymnasts, and nonathletes physically rotated objects that were either light (wooden) or heavy (lead) but otherwise having the same sizes and shapes. They then performed a mental rotation task using photographs of these objects in which the material and therefore the weight was visible. I hypothesized that wrestlers would rely more heavily on experience-based sensorimotor strategies in performing mental rotation because during their athletic practice they not only manipulate external “objects” (i.e., their opponent) but also have to plan future actions taking into account past experience of these “objects” (for example their weight). All participants reported that lead objects were harder to physically rotate than wooden ones. However, only wrestlers mentally rotated lead objects more slowly than wooden ones—as they would if they were physically rotating them—suggesting the involvement of motor processes. These findings show that the involvement of motor processes in mental rotation depends on specific rather than mere sensorimotor experience. 相似文献
6.
J.J. Podesta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):148-152
Solar wind data is used to estimate the autocorrelation function for the stochastic process x(τ) = y(t + τ) − y(t), considered as a function of τ, where y(t) is any one of the quantities B2(t), np(t)V2(t), or np(t). This process has stationary increments and a variance that increases like a power law τ2γ where γ is the scaling exponent. For the kinetic energy density and the proton density the scaling exponent is close to the Kolmogorov value γ = 1/3, for the magnetic energy density it is slightly larger. In all three cases, it is shown that the autocorrelation function estimated from the data agrees with the theoretical autocorrelation function for a self-similar stochastic process with stationary increments and finite variance. This is far from proof, but it suggests that these stochastic processes may be self-similar for time scales in the small scale inertial range of the turbulence, that is, from approximately 10 to 103 s. 相似文献
7.
U.W. Langner M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(2):368-372
A numerical model, based on Parker’s transport equation, describing the modulation of anomalous cosmic rays and containing diffusive shock acceleration is applied. The role of radial perpendicular diffusion at the solar wind termination shock, and as the dominant diffusion coefficient in the outer heliosphere, is studied, in particular the role it plays in the effectiveness of the acceleration of anomalous protons and helium when its latitude dependence is changed. It is found that the latitudinal enhancement of radial perpendicular diffusion towards the heliospheric poles and along the termination shock has a prominent effect on the acceleration of these particles. It results in a ‘break’ in the energy spectrum for anomalous protons at ∼6.0 MeV, causing the spectral index to change from E−1.38 to E−2.23, but for anomalous helium at ∼3.0 MeV, changing the spectral index from E−1.38 to E−2.30. When approaching the simulated TS, the changes in the modulated spectra as they unfold to a ‘steady’ power law shape at energies below 50 MeV are much less prominent as a function of radial distances when radial perpendicular diffusion is increased with heliolatitude. 相似文献
8.
网格计算是一种新兴的解决大规模复杂问题的应用技术,充分利用现有资源提供高性能的计算能力。现在的生产过程越来越向大规模复杂化方向发展,过程控制需要新的控制模型和控制方法来解决这些问题。但现有的计算能力无疑又限制了控制技术的应用,将高性能的网格计算运用到过程控制当中可以提高控制模型和控制算法的计算速度,也将大大提高其控制品质和应用范围。 相似文献
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S.V. Veretenenko V.A. DergachevP.B. Dmitriyev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Long-term changes of the Arctic frontal zone characteristics near the south-eastern coasts of Greenland were considered, the NCEP/NCAR reanalysis data being used. It was found that in the cold half of the year the temperature gradients in the layer 1000–500 hPa in the region under study reveal strong ∼10-yr and ∼22-yr periodicities that seem to be related to solar activity cycles. The results obtained suggest the influence of solar activity and cosmic ray variations on the structure of the temperature field of the troposphere resulting in the changes of the temperature contrasts in the Arctic frontal zone that, in turn, may affect the intensity of cyclogenesis at middle latitudes. The detected effects seem to indicate an important part of frontal zones in the mechanism of solar activity and cosmic ray variation influence on the development of extratropical baric systems. It is suggested that the variations of the temperature gradients revealed in the Arctic frontal zone are due to the radiative forcing of cloudiness changes which may be associated with geomagnetic activity and cosmic ray variations. 相似文献