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221.
袁玉亮 《华北航天工业学院学报》2008,(6):22-25
空气悬架以其优良的减振性能,在汽车振动控制中得到越来越广泛的应用。本文以空气悬架为研究对象,构建了带附加空气室空气悬架系统的1/4车辆振动模型;分析了空气悬架刚度调节原理和控制特性,本文采用了不依赖于被控对象精确数学模型的模糊控制策略进行空气悬架控制器的设计。 相似文献
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建立了基于遥测视加速度的推力及比冲计算模型,模型中考虑了附加质量对发动机推力的影响,对固体火箭发动机飞行试验推力及比冲进行了计算,并与利用标准内弹道预示程序重新预示的发动机推力及比冲进行了对比,两种方法计算结果一致。算例表明,利用飞行试验遥测视加速度计算发动机推力及比冲的计算模型正确,有关参数的选取和处理方法可行;该方法可准确再现发动机飞行过程的实时推力和比冲;可有效用于发动机飞行试验结果的快速分析与评估。 相似文献
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稳态加速度模拟试验设备:离心机设计(3) 总被引:1,自引:0,他引:1
文章分3篇10章详细介绍了稳态加速度模拟试验设备--离心机的设计.上篇对稳态加速度环境及其效应、相关试验方法和国家标准作了阐述;中篇(上)系统介绍了国内外离心机发展的历史,提供了较为全面具体的离心机结构概况,并对它们逐一进行小结与点评;中篇(下)对离心机进行基本理论分析,研究总体设计和部件设计问题,提出离心机设计原则及其计算方法;下篇通过一个国家"七五"科技攻关项目的实践作为实例,提供读者作设计参考.在文章中,作者对多年来积累的技术资料和实践心得进行了系统的整理和归纳,梳理出一条在离心机研制中科学的设计思路和实用的工作程序.该文章对相关领域的研究人员和技术人员会有启发和帮助,同时对其他同类设备的设计也有触类旁通的作用.文章主要探讨的对象是中型,大型、特大型航空航天物体离心机,土工离心机和载人离心机. 相似文献
226.
Volodymyr Kryvdyk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Formation of relativistic jets in the magnetosphere of collapsing stars is considered. These jets will be formed in the polar caps of magnetosphere of collapsing star, where the stellar magnetic field increases during the collapse and the charged particles are accelerated. The jets will generate non-thermal radiation. The analysis of dynamics and emission of particles in the stellar magnetosphere under collapse shows that collapsing stars can be powerful sources of relativistic jets. 相似文献
227.
M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(2):245-258
Voyager 1 crossed the solar wind termination shock on December 16, 2004 at a distance of 94 AU from the Sun, to become the first spacecraft to explore the termination shock region and to enter the heliosheath, the final heliospheric frontier. By the end of 2006, Voyager 1 will be at ∼101 AU, with Voyager 2 at ∼81 AU and still approaching the termination shock. Both spacecraft have been observing the modulation of galactic and anomalous cosmic rays since their launch in 1977. The recent observations close to or inside the heliosheath have provided several interesting ‘surprises’ with subsequent theoretical and modeling challenges. Examples are: what does the modulation of galactic cosmic rays amount to in this region?; how do the anomalous cosmic rays get accelerated and modulated?; why are there ‘breaks’ in the power-law slopes of the spectra of accelerated particles? Several numerical models have been applied to most of these topics over the years and comprehensive global predictions have been made the past decade, thought to be based on reasonable assumptions about the termination shock and the heliosheath. Examples of these predictions and assumptions are concisely discussed within the context of the main observed features of cosmic rays in the vicinity of the termination shock, ending with a discussion of some of the issues and challenges to cosmic ray modeling in particular. 相似文献
228.
A. W. Hood 《Space Science Reviews》1999,87(1-2):79-92
Theories and observations of energy input, heating and acceleration mechanisms in the low corona were presented and discussed.
The main topics of discussion were large-scale solar wind simulations, theoretical heating mechanisms, observational constraints,
confronting theory with observations and observational issues.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
229.
E.E. Antonova N.O. Ermakova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The problem of auroral particle acceleration is analyzed taking into account the filling of the magnetosphere by accelerated particles of ionospheric origin and the trapping of particles between the magnetic and electrostatic barriers. It is taken into account that kappa distributions describe experimentally measured distribution functions better than do maxwellians. The existence of conjugate field-aligned potential drops in the north and south hemispheres is suggested. Field-aligned potential drops are formed if the value of field-aligned current is higher than the threshold determined by the free gazodynamic flow of electrons along field lines. Results of experimental observations showing the possibility of field-aligned potential drop concentration in double layers are summarized. The theory of kinetic double layers is developed taking into account the nonmaxwellian forms of distribution functions. It is shown that the kinetic treatment and the existence of nonmaxwellian distributions lead to real changes in the criteria required for double-layer formation. 相似文献
230.