疲劳S-N曲线预测的三维断裂力学方法

根据旋转弯典圆棒疲劳断口分析,给出了裂纹几何参量及应用强度因子随裂纹扩展的变化规律,采用考虑三维应力约束效应的断裂力学理论及常幅载荷下材料的疲劳裂纹扩展da/dN-ΔK曲线,得到了独立于试件几何形状和应力比的材料da/dN-ΔKeff基准数据,结合断口分析所得的应力强度因子以及材料da/dN-Δkeff数据,以三种旋转弯曲圆棒S－N（应力－疲劳寿命）曲线进行了预测,结果表明,本文预测的疲劳S－N曲线和试验的结果较为吻合,本文的S－N曲线断裂力学预测方法对确定结构全寿命具有实际指导意义,同时也揭示了发展疲劳断裂统一理论的可行性。     

雷达监视下程序管制短期冲突告警算法研究

本文研究了一种基于航空器飞行轨迹线性外推冲突预测的短期冲突告警（STCA）算法,并给出算法的具体实现方案。仿真实验结果证明了算法的有效性,适用于雷达监视下的程序管制间隔标准和管制体制。     

广汉WAFS数值预报资料再分析研究

本文结合广汉地方气候特点。对WAFS数值预报资料进行整理、诊断,转换GRIB数据,并根据WAFS资料计算了露点温度的预报值,由此得出一些预报产品,如降水预报、形势场预报、K指数、假相当位温、结冰指数等。在实际工作中,使用WAFS预报产品多次准确预报了广汉机场的大风、降水等重要天气过程。同时,也发现WAFS资料在强度预报和长期预报中的不足。     

T639、ECMWF数值预报产品对积冰预报的释用

本文主要利用T639资料、ECMWF数值预报、卫星云图、天气图分析及地形分析对中低空飞行时频繁出现积冰的原因进行分析,着重对T639数值预报、欧洲中心数值预报产品所含的温度、湿度、相对湿度在航路积冰预报中的释用进行了分析。结论得出欧洲中心预报24小时、48小时预报风场、湿度场和实况吻合很好。T639数值预报风场、湿度场、温度场12小时预报效果很好,和实况吻合。二者结合利用,对积冰预报效果更好。     

LC4铝合金预腐蚀损伤疲劳寿命预测

在不同的腐蚀时间条件下,按ASTM标准对试验件进行预腐蚀试验,产生腐蚀坑,获得了腐蚀损伤的数据,然后进行疲劳加载试验,建立了不同腐蚀时间与疲劳寿命之间的关系。用AFGROW软件预测不同腐蚀时间对试件疲劳寿命影响,预测值与试验值对比偏保守。建立了预腐蚀损伤试件的疲劳寿命预测的方法。     

广州地磁Z分量日变幅的谱特征

利用1972—1993年广州地磁资料，分析了Z分量日变幅的年平均、年变化和半年变化等低频成分的逐年变化，以及小于60天的短周期变化特征．同时对1972—1993年的F10.7日均值进行了谱分析．结果指出，广州地磁Z分量日变幅的年平均与太阳活动指数F10．7的年平均存在良好的线性相关；具有幅度大约5nT夏季极大的年变化，与太阳活动没有明显相关，是一种季节效应；存在春秋分极大的半年变化，幅度与太阳活动有关，高年的幅度明显大于低年；具有明显的与太阳自转相关的27天左右的变化和明显的与行星波有关的接近16日、10日、5日、2日等短周期变化．广州地磁Z分量日变幅的这些谱特征，有助于更深入地了解中低层大气对电离层影响的物理机制．     

空间碎片碰撞预警研究

介绍了空间碎片的分布和危害，阐明了航天器进行碎片预警规避的必要性，讨论了碎片碰撞预警技术中的关键问题，用已有的碰撞和规避实例对自行研制的软件进行了计算检验，结果证明了软件的正确性，也说明了国内进行碎片预警工作的可行性．     

Interplanetary shocks and sudden impulses during solar maximum (2000) and solar minimum (1995–1996)

In this work a study is performed on the correlation between fast forward interplanetary shock parameters at 1 Astronomical Unit and sudden impulse (SI) amplitudes in the H-component of the geomagnetic field, for periods of solar activity maximum (year 2000) and minimum (year 1995–1996). Solar wind temperature, density and speed, and total magnetic field, were taken to calculate the static pressures (thermal and magnetic) both in the upstream and downstream sides of the shocks. The variations of the solar wind parameters and pressures were then correlated with SI amplitudes. The solar wind speed variations presented good correlations with sudden impulses, with correlation coefficients larger than 0.70 both in solar maximum and solar minimum, whereas the solar wind density presented very low correlation. The parameter better correlated with SI was the square root dynamic pressure variation, showing a larger correlation during solar maximum (r = 0.82) than during solar minimum (r = 0.77). The correlations of SI with square root thermal and magnetic pressure were smaller than with the dynamic pressure, but they also present a good correlation, with r > 0.70 during both solar maximum and minimum. Multiple linear correlation analysis of SI in terms of the three pressure terms have shown that 78% and 85% of the variance in SI during solar maximum and minimum, respectively, are explained by the three pressure variations. Average sudden impulse amplitude was 25 nT during solar maximum and 21 nT during solar minimum, while average square root dynamic pressure variation is 1.20 and 0.86 nPa^1/2 during solar maximum and minimum, respectively. Thus on average, fast forward interplanetary shocks are 33% stronger during solar maximum than during solar minimum, and the magnetospheric SI response has amplitude 20% higher during solar maximum than during solar minimum. A comparison with theoretical predictions (Tsyganenko’s model corrected by Earth’s induced currents) of the coefficient of sudden impulse change with solar wind dynamic pressure variation showed excellent agreement, with values around 17 nT/nPa^1/2.     

Research on a complex CME event including Hα, LASCO, radio and MDI observations

We present our research on a fast and decelerating partial halo coronal mass ejection (CME) event detected in multi-wavelengths in the chromosphere and the corona on 14 October, 1999. The event involved a whole complex active area which spanned more than 40° of heliolongitude. It included a strong solar flare (XI/1N) and a complex eruptive filament within an active region of the entire complex. Especially, several radio sources were detected in the decimetric range prior to the CME by the Nançay Radioheliograph (NRH). A linear force-free field extrapolation of the Michelson Doppler Imager (MDI) magnetogram was performed to calculate the magnetic topology of the complex prior to the triggering of the event. The presence of a coronal null point combined with the occurrence of two distant and nearly simultaneous radio sources put strong arguments in favor of the generalized breakout model for the triggering of the eruption. The analysis of the subsequent development of the event suggests that large interconnecting loops were ejected together with the CME.     

SOME RESULTS OF UPPER ATMOSPHERIC COMPOSITION MEASUREMENTS BY A MASS-SPECTROMETER ON BOARD "SZ-2":CHANGE OF COMPOSITIONS DURING SOLAR AND GEOMAGNETIC DISTURBANCES

Upper atmosphere composition data were obtained for the last half year with a quadruple mass spectrometer on board spacecraft "SZ-2" launched on 10 Jan uary 2001. Based on the analysis of these data, the variations of atmospheric compositions in solar and geomagnetic quiet conditions are reported first, then a detailed discussion on the atmospheric composition variations under the so lar and geomagnetic disturbed conditions is given. The results show that near the altitude of 400 km the variations of main atmospheric compositions corre sponding to solar disturbances are more remarkable in the sunlit area than in the shade area. On the contrary, in geomagnetic disturbance events the corre sponding variations are more obvious in the shade area, an evident increase of N2 density at relatively higher latitudes was observed.