横向加强构件作用下的开口薄壁梁等效建模方法

卫星结构中通常有大量横向加强构件作用下的开口薄壁杆件,横向加强构件一般沿杆件轴向均匀分布,通过对这类结构研究,理论上证明了这种结构的振动微分方程与普通的开口薄壁梁振动微分方程有相同的形式,因此可以用开口薄壁梁单元进行等效计算。本文建立了开口薄壁梁的3种数学模型:有限元模型、传递矩阵模型和解析模型。采用优化理论中序列二次规划对等效截面参数进行辨识,同时分析了不同目标函数对辨识结果的影响,并且提出了一种对截面初始参数进行估计的方法。对于有限元模型,提出采用MATLAB与ABAQUS交互式参数优化方法,充分结合二者优点可以快速高效地对截面参数进行优化辨识,具有较强的通用性。通过实验验证了这种等效建模方法的正确性与精确性。所提出的等效建模方法可以减少90%以上的单元数量。通过建立这种简化模型,可以大幅度提高整星结构模型修正与结构重分析的效率。      

超磁致伸缩作动器小回线动态J-A模型

超磁致伸缩作动器（GMA）输入输出之间存在着磁滞非线性关系,当研究其中高频输出特性时,为了降低材料自身迟滞非线性特性的影响,往往选用零点与饱和状态之间线性度较好的不饱和小回线,因此很有必要开展动态不饱和小回线数学模型的研究。首先在综合研究磁致伸缩材料（GMM）和GMA结构动力学特性的基础上结合安培环路定理提出以励磁电流为输入、应变为输出的动态Jiles-Atherton（J-A）模型,然后在引入磁滞回线特性变量的基础上得出J-A模型关键模型参数对其特性的影响规律,根据不饱和小回线仿真与实验波形的偏离特性提出模型参数的修正方法得到不饱和小回线动态J-A模型。最后,在不同频率和不同饱和幅值下通过实验验证该数学模型的正确性。      

运动基航天飞行模拟器信号缩比策略

对于大幅值的输入信号,三阶多项式缩比法易产生信号畸变且参数配置复杂;而Hermite缩比函数法的触发速度较慢.提出两种改进的缩比方法:基于三阶多项式缩比法的最优参数配置法和加入线性缩比的非线性缩比法.前一种方法通过参数的优化配置最大化稳定区,以防止信号的畸变;后一种方法则利用线性缩比的特性将缩比度限制在稳定区内.仿真结果表明:线性缩比的加入可以防止三阶多项式缩比法信号的畸变;最优配置参数法应用方便且整体效果较好.为航天飞行模拟提供了更有效的缩比策略.     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).     

抑制复原图像振铃波纹的频域循环边界算法

提出了一种基于Wiener滤波的频域循环边界复原算法,并给出了有效的规整化表达式和信噪比估算方法.复原算法首先将原观测图像按反射对称的方式延拓,形成一个新的观测图像(称为延拓图像);然后,用Wiener滤波算法复原延拓图像,并取延拓图像的复原图像的主值序列作为原观测图像的复原图像.对延拓图像在频域进行复原处理时,需要使用FFT(Fast Fourier Transform)技术,将延拓图像进行周期延拓,因其结合边界在垂直方向上的梯度为零,且边界平滑满足微分条件,抑制了复原图像的振铃波纹.复原过程中,将噪声与原始图像的功率谱之比规整化为原观测图像信噪比的函数.实验结果表明,该算法对周边区域梯度变化较大的观测图像复原效果较好.      

齿轮测量中心测头数据采集系统

提出了齿轮测量中心电感测头的新型数据采集系统,包括以集成开关构成的新型相敏检波器和以单片机为核心的数据采集系统,可以应用于各种电感信号的处理,具有较强的通用性。     

Estimation of optical maturity parameter for lunar soil characterization using Moon Mineralogy Mapper (M3)

Prolonged exposure of the microscopic outer layer of the lunar surface to the space environment leads to the maturation of the surface. Maturation can be quantified and it may be expressed in terms of optical maturity (OMAT). Optical maturity estimations are very much helpful in the identification and mapping of the major minerals present on the lunar regolith. Estimation of the maturation and mineral mapping using remote sensing techniques are achieved, by coupling spectral reflectance of the lunar surface with an optimized origin. The present work estimates the optical maturity and Ferrous oxide content of the Goldschmidt and Schrodinger craters, through the recalibration of the classical method of Lucey et al. (2000a) with an origin of (0.08, 1.18) and Moon Mineralogy Mapper (M3) data. The overall recalibration results assure that the craters are highly matured.     

大气紊流环境下的纵向飞行参数响应分析

介绍了大气紊流环境下飞机纵向飞行参数的计算与匹配方法.由于紊流的随机性特征,飞行参数响应分析采用时域与频域相结合的方式,对某型飞机紊流环境下的纵向飞行参数进行了计算分析.采用所介绍的方法,可以获得比较合理的飞行情况来指导型号设计工作.     

CMH模型中部分参数对磁滞回线形状影响的研究

研究了Complete Moving Hysteresis模型计算公式中部分参数对磁滞回线形状的影响 ,发现饱和磁化强度Ms 和移动参数α对回线形状的影响并不显著 ,但参量γ的影响却是明显的 ,随着γ值的增加 ,回线的斜率增加 ,突变性增强     

二元外压式进气道斜板和唇口参数选择的风洞试验研究

在几何不可调的二元外压式斜板进气道的设计中，选择合理的斜板和唇口几何能数是最重要的问题之一。本文对一个设计马赫数为１．８的这类进气道的斜板和唇口参数进行了风洞试验研究。用缩尺模型风洞试验，对比分析了不同斜板角和不同外侧唇口内唇角，唇缘半径对进气道内流特性的影响，结果表明，对确定的进气道布局，斜板角小的变化对进气道超音速内流总压恢复系数，稳态出口流场周向畸变指数及喘振裕度的影响很大，唇口参数小的改变