一种基于虚拟页地址映射的NAND Flash管理算法

本文提出了一种基于虚拟页地址映射的NAND Flash管理算法.该算法通过定义坏块表、对应表等结构，以及设计的坏块替换策略和虚拟页地址到实际物理页地址的转换算法，实现上层软件采用虚拟地址对NAND Flash的无坏块连续页地址访问.该算法是一种高效的地址映射算法，能高效地对数据进行索引，占用SRAM空间较少，使系统达到高性能，并使得闪存使用的更加稳定持久.     

科学计算中的高性能有限元算法

 圆周率的计算是科学计算的启示,它提供了许多信息,包括计算误差的正负、大小,以及算法的加速。在偏微分方程的计算中,有无相似的内容,这就是本文试要回答的问题。     

一类二阶三点边值问题解的存在性

运用上下解方法,研究了一类二阶混合非线性边值条件的三点边值问题,通过构造了适当的非线性辅助函数工得到了解存在的充分条件,推广和改进了某些已知的结果。     

Advances in the Studies of the Middle and Upper Atmosphere in 2004 - 2006

This paper summarizes the research results obtained by Chinese scientists and/or through international collaborations during 2004 to 2006. Within the context of COSPAR, the progresses in the studies of the middle and upper atmosphere in China in the past two years are introduced with focusing the developments in facilities and instruments, and the advancements in scientific issues, e.g., dynamics related processes, atmospheric constituents, and the coupling with the lower atmosphere.     

不确定参数结构特征值问题的概率统计方法和区间分析方法的比较

 基于区间数学理论、灵敏度分析理论、Kronecker代数理论,应用Taylor级数展开、概率摄动技术,提出了具有不确定参数结构的特征值问题的区间分析方法。结合工程实例与传统的概率分析方法进行比较,给出了两种方法的数值解法及各自解法的Kronecker代数形式。数值算例的结果显示了区间分析方法在具有不确定参数结构特征值问题分析中的价值和有效性。     

基于序列凸优化的上面级远程交会轨迹优化

针对末端时间自由的上面级远程交会问题,提出一种基于序列凸优化的上面级远程交会轨迹优化方法.首先建立了末端时间自由的上面级远程交会模型,通过约束松弛和线性化等方法将该模型转化为一组可以迭代求解的凸优化问题.其次结合上面级发动机推力较大的特点,采用双脉冲变轨的计算结果作为迭代初值,进而减少迭代次数.最后用对偶内点法求出远程...     

泵压式上面级发动机性能精度干扰因素研究

性能精度是液体火箭发动机的一项重要指标,对于上面级发动机性能精度尤其重要.以某型泵压式上面级发动机为研究对象,利用影响分析树的方法识别了发动机生产、测试、性能调整过程中影响性能精度的干扰因素;针对所识别的干扰因素,通过仿真计算,得到了其偏差对发动机推力和混合比的影响.根据统计学原理,推导得到多项干扰因素影响概率的计算模型,并利用小子样样本对计算模型和程序的正确性进行了验证.利用该概率计算模型,根据置信水平要求,确定了多项干扰因素对发动机性能的极限偏差影响.根据发动机性能精度要求,分解得到了单个干扰因素的控制目标.     

基于非连续算子广义变分不等式强解的存在性

在算子不连续的情况下,利用FKKM定理和Weierstrass定理及标量化方法得到了广义向量变分不等式的强解存在性定理.     

Numerical modeling of inhomogeneous orographic wave influence on planetary waves in the middle atmosphere

Parameterization of dynamical and thermal effects of stationary orographic gravity waves (OGWs) generated by the Earth’s surface topography is incorporated into a numerical model of general circulation of the middle and upper atmosphere. Responses of atmospheric general circulation and characteristics of planetary waves at altitudes from the troposphere up to the thermosphere to the effects of OGWs propagating from the earth surface are studied. Changes in atmospheric circulation and amplitudes of planetary waves due to variations of OGW generation and propagation in different seasons are considered. It is shown that during solstices the main OGW dynamical and heat effects occur in the middle atmosphere of winter hemispheres, where changes in planetary wave amplitudes due to OGWs may reach up to 50%. During equinoxes OGW effects are distributed more homogeneously between northern and southern hemispheres.     

Simulating planetary wave propagation to the upper atmosphere during stratospheric warming events at different mountain wave scenarios

Parameterization schemes of atmospheric normal modes (NMs) and orographic gravity waves (OGWs) have been implemented into the mechanistic Middle and Upper Atmosphere Model (MUAM) simulating atmospheric general circulation. Based on the 12-members ensemble of runs with the MUAM, a composite of the stratospheric warming (SW) has been constructed using the UK Met Office data as the lower boundary conditions. The simulation results show that OGW amplitudes increase at altitudes above 30 km in the Northern Hemisphere after the SW event. At altitudes of about 50 km, OGWs have largest amplitudes over North American and European mountain systems before and during the composite SW, and over Himalayas after the SW. Simulations demonstrate substantial (up to 50–70%) variations of amplitudes of stationary planetary waves (PWs) during and after the SW in the mesosphere-lower thermosphere of the Northern Hemisphere. Westward travelling NMs have amplitude maxima not only in the Northern, but also in the Southern Hemisphere, where these modes have waveguides in the middle and upper atmosphere. Simulated variations of PW and NM amplitudes correspond to changes in the mean zonal wind, EP-fluxes and wave refractive index at different phases of the composite SW events. Inclusion of the parameterization of OGW effects leads to decreases in amplitudes (up to 15%) of almost all SPWs before and after the SW event and their increase (up to 40–60%) after the SW in the stratosphere and mesosphere at middle and high northern latitudes. It is suggested that observed changes in NM amplitudes in the Southern Hemisphere during SW could be caused by divergence of increased southward EP-flux. This EP-flux increases due to OGW drag before SW and extends into the Southern Hemisphere.