低纬地磁Z分量的半年变化

利用武汉、广州、泉州和琼中等4个低纬地磁站连续多年的地磁资料，计算了各月5个磁静日Z分量日均值与中午1100---1300时段平均值之差(Dz)，对每年12个Dz采用多元回归分析方法，得到各年的半年变化幅度和相位．结果表明：4个站的Dz每年都有半年变化现象；半年变化幅度与太阳活动有关，一般来说，太阳活动高年Dz半年变化幅度明显大于太阳活动低年；太阳活动本身的半年变化，对Dz半年变化幅度有显著的调制作用；Dz半年变化的相位在3—4月(或9—10月)，即极大值出现在分季；低纬地区地磁Z分量存在显著的半年变化，能够反映赤道电急流也有明显的半年变化，这再一次证明，赤道电急流幅度的半年变化，通过“喷泉效应”使得电离层，f0F2产生半年变化，其是产生，f0F2半年变化的一个主要因素．     

神舟2号大气密度探测器的探测结果(Ⅰ)日照和阴影区域热层大气密度变化

选用了神舟2号（SZ-2）大气密度探测器在2001年2—4月间的探测数据,进行日照和阴影区域热层大气密度变化的探讨.结果表明:在高度410km附近,日照和阴影区域大气密度变幅为2—3倍,变幅的大小与地磁活动程度呈负相关关系.日照面大气密度峰区位于星下点地方时1400—1500LT的纬度处,峰值大小与太阳活动程度呈正相关关系.阴影面大气密度谷区位于星下点地方时0400-0500的纬度处,同时在±10°纬度区域中还出现了阴影面峰区.     

线阵CCD平场校正及FPGA实现的研究

为了消除由于照明光源的非均匀性、镜头渐晕及CCD传感器噪声对图像质量造成的不良影响,首先从理论上分析了线阵CCD固定模式噪声和像素光电响应非均匀性的数学模型和产生的原因;对像素光电响应非均匀性这一主要影响因素,根据其光电响应模型提出了CCD像素光电响应非均匀性的两点校正方法,即求解出各个像素光电响应不均匀性的校正因子和暗偏置量系数,进而用以计算各个像素的校正量,实现逐点校正;针对校正算法大数据量、实时计算的要求,设计了基于现场可编程逻辑门阵列FPGA快速实现校正算法的硬件处理结构。最后,通过仿真和实验表明,两点校正方法可以有效地减小CCD像素光电响应不均匀性的图像噪声,提高图像质量,以便做后续精确处理。     

静止轨道卫星通信链路的预算与分析

星地链路计算作为卫星通信的重要技术，是卫星通信系统设计的基础和理论依据，直接决定了卫星通信系统的链路通信质量。由于影响卫星链路的因素很多，设计中存在一处不合理即使得整条星地链路不可用，造成巨大的损失。而且在实际设计中无法做到最理想的链路状态，往往需要在某方面有所取舍，这也是链路计算中的一大难点。基于目前国际通用的链路计算方法，将星地链路上下行拆分，独立计算，综合分析，再结合实际工程经验，分析和计算实际工程案例，针对不同的链路配置给出相应合理的设计方法，可作为静止轨道通信卫星星地链路计算分析的参考。     

Application of small-size antennas for estimation of angles of arrival of HF signals scattered by ionospheric irregularities

A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network.     

Aircraft nonlinear stability analysis and multidimensional stability region estimation under icing conditions

Icing is one of the crucial factors that could pose great threat to flight safety,and thus research on stability and stability region of aircraft safety under icing conditions is significant for control and flight.Nonlinear dynamical equations and models of aerodynamic coefficients of an air craft are set up in this paper to study the stability and stability region of the aircraft under an icing condition.Firstly,the equilibrium points of the iced aircraft system are calculated and analyzed based on the theory of differential equation stability.Secondly,according to the correlation theory about equilibrium points and the stability region,this paper estimates the multidimensional stability region of the aircraft,based on which the stability regions before and after icing are compared.Finally,the results are confirmed by the time history analysis.The results can give a reference for stability analysis and envelope protection of the nonlinear system of an iced aircraft.     

阵风载荷减缓系统故障分析

阵风引起的额外载荷会引起飞机结构疲劳,降低结构使用寿命。采用非定常气动力有理函数拟合方法建立时域状态空间下的动力学系统,设计了阵风载荷减缓系统。研究了阵风载荷减缓系统3种典型故障模式(副翼偏转饱和、舵机卡死、副翼偏转延时)的力学建模方法,并对机翼在阵风减缓系统故障模式下的阵风响应进行分析。仿真结果表明,3种故障模式均不利于阵风载荷减缓系统对阵风载荷的减缓,对于一些特定情况,故障模式下的阵风载荷减缓系统不仅不能减缓阵风载荷,还会带来由副翼偏转不当引起的额外负载。     

Avoid online radiation risk: Theoretical simulation of chromosome breaks in cells exposed to heavy ions

In this study, we report an easy and quick method on simulating chromosome breaks in cells exposed to heavy charged particles. The theoretical value of chromosome break was calculated, and validated comparison with experimental value by using premature chromosome condensation technique. A good consistency was found between theoretical and experimental value. This suggested that higher relative biological effectiveness of heavy ions was closely correlated with its physical characteristics. Also, a safe approach on predicting chromosome breaks in cells exposed to heavy ions at off-line environment can be considered. Furthermore, three key factors influencing the theoretical simulation was investigated and discussed.     

EPDM包覆层热解状态下的力学行为及本构模型

为了准确描述固体火箭发动机三元乙丙(EPDM)包覆层在不同热解状态下的力学特性,通过热重分析的方法得到EPDM的热解温度范围,并采用准静态单轴拉伸实验的方法获得EPDM在不同热解温度下的应力-应变曲线。以Ogden(n=2)模型为基础,分别对不同热解状态下的力学曲线进行建模,并通过对实验数据的拟合获得模型参数。结果表明,在初始热解状态下,材料只发生了少量的失水和气体的逃逸,其力学行为可通过粘超弹本构模型进行描述;随着材料热解程度增加,基体材料和填充纤维均遭到破坏,其力学行为表现为超弹脆性材料特性。