表一偶数为二素数之二进伪和

大量的计算机计算的结果,支持我们提出如下猜想:每个正偶数,均可表示成两个奇素数的二进伪和,且其表法有无穷多种.     

Data fusion algorithm based on state and attribute parameter

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Simulation Techniques for Cosmological Simulations

Modern cosmological observations allow us to study in great detail the evolution and history of the large scale structure hierarchy. The fundamental problem of accurate constraints on the cosmological parameters, within a given cosmological model, requires precise modelling of the observed structure. In this paper we briefly review the current most effective techniques of large scale structure simulations, emphasising both their advantages and shortcomings. Starting with basics of the direct N-body simulations appropriate to modelling cold dark matter evolution, we then discuss the direct-sum technique GRAPE, particle-mesh (PM) and hybrid methods, combining the PM and the tree algorithms. Simulations of baryonic matter in the Universe often use hydrodynamic codes based on both particle methods that discretise mass, and grid-based methods. We briefly describe Eulerian grid methods, and also some variants of Lagrangian smoothed particle hydrodynamics (SPH) methods.     

UDu~T分解滤波算法及其应用

本文介绍UDU~T 分解滤波算法;用工程师容易理解的方法重新推导时间修正和量测修正滤波公式,并给出标准通用的UDU~T 分解滤波子程序。本算法子程序已实际用于工程估计器中。本算法具有高的数字稳定性。作为UDU~T 分解滤波算法理论和工程应用之间桥梁的本通用标准子程序具有良好性能,使用方便,极易推广应用。     

固定影响平行数据模型参数的偏最小二乘估计及应用

当平行数据的解释变量之间存在严重的多重共线性,或者样本点个数与解释变量个数相比较少时,用经典方法求解模型(如最小二乘法等)误差偏大,难以满足实际要求.针对这种情况提出了用偏最小二乘法思想求解固定影响平行数据模型,并且实例表明误差明显减少,可以满足建模和预报的要求.     

New evidence for strong non-thermal effects in Tycho’s supernova remnant

For the case of Tycho’s supernova remnant (SNR), we present the relation between the blast wave and contact discontinuity radii calculated within the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is demonstrated that these radii are confirmed by recently published Chandra measurements which show that the observed contact discontinuity radius is very close to the shock radius. Therefore a consistent explanation of these observations can be given in terms of efficient CR acceleration which makes the medium more compressible.     

混凝土靶侵彻计算的半经验法

在球形空腔膨胀理论基础上,通过不同强度混凝土材料的侵彻实验数据直接识别建立混凝土材料综合动态强度参数psd与混凝土材料无侧限压缩强度σ-b的经验关系式;从应力波表层损伤理论分析了混凝土表层“开坑区”的侵彻特性,提出“简化等效阻力线”的计算方法;指出球形空腔膨胀理论的阻力算式中取动阻力项系数B=1.5的合理性。理论分析和侵彻实验表明:本文方法适用于小弹侵彻混凝土靶、大弹侵彻混凝土靶和以混凝土材料为面层的部分多层复合靶的侵彻计算,克服了Forrestal半经验法的不足。     

金融服务滞后产业发展的成因及对策——以航空业为例

分析了在战略产业发展过程中金融业服务滞后的各种表现，从战略产业经济结构调整本身、风险约束和金融宏观政策传导三个方面剖析了金融服务滞后的原因。以民用航空制造业的发展为例，用博弈论对金融在支持战略产业发展过程中的两难状况作了理论和实证分析，提出金融支持战略产业的发展是金融发展的最优选择的观点。最后从金融体系、资金投入和金融服务等方面提出相应的对策建议。     

Non-Thermal Processes in Cosmological Simulations

Non-thermal components are key ingredients for understanding clusters of galaxies. In the hierarchical model of structure formation, shocks and large-scale turbulence are unavoidable in the cluster formation processes. Understanding the amplification and evolution of the magnetic field in galaxy clusters is necessary for modelling both the heat transport and the dissipative processes in the hot intra-cluster plasma. The acceleration, transport and interactions of non-thermal energetic particles are essential for modelling the observed emissions. Therefore, the inclusion of the non-thermal components will be mandatory for simulating accurately the global dynamical processes in clusters. In this review, we summarise the results obtained with the simulations of the formation of galaxy clusters which address the issues of shocks, magnetic field, cosmic ray particles and turbulence.     

增升状态下的全机位流数值模拟

研究了势流理论下的全机增升装置复杂外形气动力数值计算方法,该方法以低阶面元法为基础,具有计算量小、速度快的优点.复杂流动的粘性效应主要通过附面层粘性修正技术加以体现.采用该方法对某增升装置翼身组合体外形压力分布特性进行计算,并和风洞实验数据相比较,验证了方法的正确性和实用性.在此基础上对某型飞机真实复杂外形的压力分布特性进行了计算,为复杂外形飞行器增升装置的初步设计、方案选型与评估提供了非常理想的工程技术手段.