共轴式小型直升机操纵系统动态特性分析研究

对某共轴式小型遥控直升机纵向系统建立了工程实用的数学模型,分析研究了该系 统动态特性和参数变化对其动特性的影响.通过与试验、试飞比较,证明该模型是正确的、 可信的、其精度符合工程要求.     

热暴露对B/Al复合材料性能的影响

对经300℃、500℃高温热暴露的B／Al（LF6）复合材料的力学性能进行了研究，实验结果表明材料在300℃下热暴露时，性能下降速度较慢，100h后强度保留率约为76％，延伸率保留率为74％。而在500℃下热暴露时，5h以上强度就有明显降低。高温长时间热暴露后复合材料的断裂也从积累型转变为典型的非累积型断裂。通过透射电镜（TEM）及扫描电镜（SEM）对固态热压制造态和主温热暴露的界面状况进行了分析，认为界面反应是造成B／Al复合材料力学性能下降的主要原因。     

Phase Space Density Analysis of Energy Transport in the Earth’s Magnetotail

Two energetic events in the Earth’s magnetotail detected by Geotail are examined with detailed analysis of three-dimensional velocity phase space density. It is found that the occurrence of multiple ion components is high during these dynamic episodes. Different populations evolve independently of each other, suggesting particles from multiple activity sites contributing to the observed phase space density. The transport properties with consideration of multiple components are evaluated, with the result showing significant differences from those based on a single fluid approach. This comparison indicates that precise evaluation of the energy and magnetic flux transport of energetic events in the magnetotail requires resolving individual populations in the phase space density.     

300M钢纯洁度磁粉检验磁痕现象的分析

采用交、直流磁粉检验并结合金相试验、电子探针试验及微量元素含量分析的方法，对３００Ｍ钢磁痕现象的本质进行了分析。结果表明，采用磁粉检验方法对航空优质钢进行纯洁度检验是可信的。     

Variations of the magnetic fields in large solar flares

We present preliminary results from high resolution observations obtained with the Michelson Doppler Imager (MDI) instrument on the SOHO of two large solar flares of 14 July 2000 and 24 November 2000. We show that rapid variations of the line-of-sight magnetic field occured on a time scale of a few minutes during the flare explosions. The reversibility/irreversibility of the magnetic field of both active regions is a very good tool for understanding how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system. This revised version was published online in August 2006 with corrections to the Cover Date.     

磁制动对地壳板块运动影响的理论分析与实证研究

太阳和木星的自转是不均匀的，纬度愈高，自转愈慢。据此，作者推测液态外地核的自转，也存在类似的不均匀性，而这种不均匀自转将对地壳板块运动产生影响。利用磁流体力学理论，阐明这类星球自转的不均匀性，是磁制动的不均匀性引起的。研究了磁制动对地壳板块运动影响的途径及表现方式，并举出实例证明这些表现方式的确存在，从而证明磁制动是影响地壳板块运动的一个极为重要的因素。     

TC21钛合金的微观组织对力学性能的影响

研究了两相钛合金TC21关于两种不同微观组织(片状组织和网篮组织)的拉伸性能、断裂韧性和疲劳裂纹扩展性能.结果显示:片状组织相比网篮组织有相近的拉伸强度,但塑性较差;两者的韧性相差不大,但增韧机理不同;网篮组织在中低速扩展区的扩展速率和片状组织几乎相同,但在较高速扩展区显示略低的扩展速率;加载方向对两种组织的疲劳裂纹扩展速率基本无影响;和其他钛合金类似,TC21在Paris区存在转折.     

腰形柱壳的有限条元解

本文用考虑了曲率影响的两结线低阶有限板条元分析了腰形柱壳的力学性能这种条元位移参数少,能较好地体现壳体的几何特性。     

面内强磁场下铁磁板壳的自由振动

本文研究了面内强磁场环境下铁磁板壳的自由振动问题。基于Eringen-Maugin的关于磁弹性作用的理性力学模型,从理论上推导了一般壳体在磁场中的运动方程,进而求解了面内强磁场作用下的小磁化率悬臂铁磁薄板自由振动频率。数值计算结果表明,本文模型和已有的实验结果吻合很好。     

The characteristics of sharp (small-scale) boundaries of solar wind plasma and magnetic field structures

We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed.