长株潭红色旅游区域协作问题探讨

红色旅游是新兴的文化旅游项目,悠久厚重的历史文化酝酿了长、株、潭丰富的红色旅游资源,论文从长株潭旅游资源的特色、共性、共享优势进行分析,提出了协作的六点思路和方法。     

与航天员共度116小时

昨天，入住北京航天飞行控制中心新闻中心。我和13名女记者被安排在一间教室大小的房间里。大家都非常兴奋，一夜没怎么睡。     

关于热量与质量传递的湍流模式问题

本文发展了一个新的热量与质量传递的标量—压力相关模式。讨论了局部平衡湍流的标量脉动与速度脉动相关。同时将所得理论结果和自由射流中关于温度脉动的测量数据进行了比较。     

小展弦比飞机非线性气动特性风洞与飞行相关性研究

在较大迎角范围，如何由风洞试验数据预计全尺寸小展弦比飞机的非线性气动特性，并与飞行值相关，始终是国际航空界致力解决的重大问题，本项研究采用风洞试验与工程计算相结合的方法，对支架，洞壁、进气，喷流，雷诺数及静弹性等影响相关性的诸因素予以修正，并计及配平影响，从而比较准确地预计出全尺寸收音机的非线性气动特性，预计值与试飞值相比较结果验证了本项研究的可靠性和实用性。     

Multi-objective Optimization of Differential Steering System of Electric Vehicle with Motorized Wheels

A differential steering system is presented for electric vehicle with motorized wheels and a dynamic model of three-freedom car is built. Based on these models, the quantitative expressions of the road feel, sensitivity, and operation stability of the steering are derived. Then, according to the features of multi-constrained optimization of multi-objective function, a multi-island genetic algorithm （MIGA） is designed. Taking the road feel and the sensi- tivity of the steering as optimization objectives and the operation stability of the steering as a constraint, the system parameters are optimized. The simulation results show that the system optimized with MIGA can improve the steering road feel, and guarantee the operation stability and steering sensibility.     

网络安全体系结构研究

详细讨论了基于防火墙的Ｉｎｔｅｒｎｅｔ网络信息安全体系结构,并指出了防火墙自身的局限性以及未来安全体系结构的发展趋势。     

Interplanetary origin of geomagnetic storms

Around solar maximum, the dominant interplanetary phenomena causing intense magnetic storms (Dst<−100 nT) are the interplanetary manifestations of fast coronal mass ejections (CMEs). Two interplanetary structures are important for the development of storms, involving intense southward IMFs: the sheath region just behind the forward shock, and the CME ejecta itself. Whereas the initial phase of a storm is caused by the increase in plasma ram pressure associated with the increase in density and speed at and behind the shock (accompanied by a sudden impulse [SI] at Earth), the storm main phase is due to southward IMFs. If the fields are southward in both of the sheath and solar ejecta, two-step main phase storms can result and the storm intensity can be higher. The storm recovery phase begins when the IMF turns less southward, with delays of ≈1–2 hours, and has typically a decay time of 10 hours. For CMEs involving clouds the intensity of the core magnetic field and the amplitude of the speed of the cloud seems to be related, with a tendency that clouds which move at higher speeds also posses higher core magnetic field strengths, thus both contributing to the development of intense storms since those two parameters are important factors in genering the solar wind-magnetosphere coupling via the reconnection process. During solar minimum, high speed streams from coronal holes dominate the interplanetary medium activity. The high-density, low-speed streams associated with the heliospheric current sheet (HCS) plasma impinging upon the Earth's magnetosphere cause positive Dst values (storm initial phases if followed by main phases). In the absence of shocks, SIs are infrequent during this phase of the solar cycle. High-field regions called Corotating Interaction Regions (CIRs) are mainly created by the fast stream (emanating from a coronal hole) interaction with the HCS plasma sheet. However, because the B_z component is typically highly fluctuating within the CIRs, the main phases of the resultant magnetic storms typically have highly irregular profiles and are weaker. Storm recovery phases during this phase of the solar cycle are also quite different in that they can last from many days to weeks. The southward magnetic field (B_s) component of Alfvén waves in the high speed stream proper cause intermittent reconnection, intermittent substorm activity, and sporadic injections of plasma sheet energy into the outer portion of the ring current, prolonging its final decay to quiet day values. This continuous auroral activity is called High Intensity Long Duration Continuous AE Activity (HILDCAAs). Possible interplanetary mechanisms for the creation of very intense magnetic storms are discussed. We examine the effects of a combination of a long-duration southward sheath magnetic field, followed by a magnetic cloud B_s event. We also consider the effects of interplanetary shock events on the sheath plasma. Examination of profiles of very intense storms from 1957 to the present indicate that double, and sometimes triple, IMF B_s events are important causes of such events. We also discuss evidence that magnetic clouds with very intense core magnetic fields tend to have large velocities, thus implying large amplitude interplanetary electric fields that can drive very intense storms. Finally, we argue that a combination of complex interplanetary structures, involving in rare occasions the interplanetary manifestations of subsequent CMEs, can lead to extremely intense storms. This revised version was published online in June 2006 with corrections to the Cover Date.     

自适应变结构神经网络在航空发动机故障诊断上的应用

根据样本空间的内积特性,提出一种无需迭代学习的自适应变结构神经网络。它的特点是学习速度快,准确性高,且能根据出现的新样本,随时改变结构。在对某型航空发动机故障诊断中,比原软件包采用的方法在准确性方面有显着提高,而且维护工作量减少,并具有实时处理能力,因此有着良好的推广应用前景。      

JL8飞机航炮吊舱卡链故障分析

通过对JL8飞机航炝吊舱供弹系统及弹带结构的分析,结合弹带在供弹道内的运动特性,找出了航炮吊舱卡停射故障产笺原因,并通过计算,提出了改进措施。     

快速加热恒应力试验方法的初步研究

短时高温试验是适应现代高速飞行器的发展而建立起来的一种新型的力学性能试验方法。目前已有多种试验方案, 其中快速加热恒应力拉伸试验是在某恒定应力下, 以一定的速率加热试件, 测定合金的应变与温度的关系, 并从而求得材料在试验条件下的屈服温度(通常以引起0.2%的残余应变为准)。本文简要地评述了短时高温试验方法的现状; 介绍了为进行快速加热恒应力拉伸试验而建立的试验装置, 并提供了国产Д16AT及B95AT合金的初步试验数据;最后还对所得数据进行处理和分析。