Study on the breakup lengths of free round liquid jets

IntroductionBreakup and atomization of roundliquidjetshad been widely used in internal combustion en-gines,gas turbines,and liquid rocket engines.Recently,with the development of scramjet en-gines and the deepening of fuel atomization re-search,it attract…     

航空发动机双转子系统的拍振分析

 在双转子航空发动机中,由于转子系统不可避免地存在不平衡量,当两个转子的转速比较接近时,发动机会出现拍振现象,拍振将引起振动强度过大问题。对双转子系统的拍振进行了研究,分析了拍振的周期性、信号强度及其反向转子特性,阐明了拍振产生的机理和特征,并采用数值仿真和试验对拍振进行了定量分析和验证。研究表明,拍振与双转子转速差和不平衡量的相位因素有关,当转速差小于工作转速的20%时,双转子系统拍振信号的强度较大。     

时序信号设计的一种新方法

文章结合高速时序工作的特点,从实现的角度提出了一种利用软件调整时序的新方法。在可编程逻辑器件中,利用数字时钟管理器(DCM),通过模块化和增量式设计思想达到对高速时序信号的精确调节。最终实现了一个20MHz速率的时序控制,调节精度达到100ps。     

高速旋转部件在载人航天器热控系统中的应用

文章阐述了高速旋转部件在载人航天器热控系统中的应用现状,提出了增长部件寿命、改进系统可靠性的建议并介绍了磁悬浮技术。     

用激光干涉技术测量转速的研究

叙述了一种新型转速激光干涉测量方法,详细分析了这种方法的工作原理,确定了本测量方法的转速测量范围,给出了实验结果。     

机载移动端场面引导软件设计与仿真研究

为了减轻飞行员在繁忙机场场面运行的工作负荷,提升场面运行安全与效率,设计了一种基于移 动电子设备运行的场面引导软件。其采用可扩展架构和模块化功能设计,通过无线通信网络与综合场面监视系 统交联,实现场面引导功能。仿真测试表明,机载移动端场面引导软件能够为飞机在场面滑行操作提供路径引 导信息和冲突告警提示,可提升运行效率和安全性,具有一定的使用价值。     

Planetary protection issues related to human missions to Mars

In accordance with the United Nations Outer Space Treaties [United Nations, Agreement Governing the Activities of States on the Moon and Other Celestial Bodies, UN doc A/RES/34/68, resolution 38/68 of December 1979], currently maintained and promulgated by the Committee on Space Research [COSPAR Planetary Protection Panel, Planetary Protection Policy accepted by the COSPAR Council and Bureau, 20 October 2002, amended 24 March 2005, http://www.cosparhq.org/scistr/PPPolicy.htm], missions exploring the Solar system must meet planetary protection requirements. Planetary protection aims to protect celestial bodies from terrestrial contamination and to protect the Earth environment from potential biological contamination carried by returned samples or space systems that have been in contact with an extraterrestrial environment. From an exobiology perspective, Mars is one of the major targets, and several missions are currently in operation, in transit, or scheduled for its exploration. Some of them include payloads dedicated to the detection of life or traces of life. The next step, over the coming years, will be to return samples from Mars to Earth, with a view to increasing our knowledge in preparation for the first manned mission that is likely to take place within the next few decades. Robotic missions to Mars shall meet planetary protection specifications, currently well documented, and planetary protection programs are implemented in a very reliable manner given that experience in the field spans some 40 years. With regards to sample return missions, a set of stringent requirements has been approved by COSPAR [COSPAR Planetary Protection Panel, Planetary Protection Policy accepted by the COSPAR Council and Bureau, 20 October 2002, amended 24 March 2005, http://www.cosparhq.org/scistr/PPPolicy.htm], and technical challenges must now be overcome in order to preserve the Earth’s biosphere from any eventual contamination risk. In addition to the human dimension of the mission, sending astronauts to Mars will entail meeting all these constraints. Astronauts present huge sources of contamination for Mars and are also potential carriers of biohazardous material on their return to Earth. If they were to have the misfortune of being contaminated, they themselves would become a biohazard, and, as a consequence, in addition to the technical constraints, human and ethical considerations must also be taken into account.     

低速风洞半模实验壁压法洞壁干扰修正

 <正> 1.前言 低速风洞半模实验有许多优点,但伴随而来的是洞壁干扰修正问题。大迎角、大堵塞度情况洞壁干扰修正值相当大。如某后掠大展弦比机翼半模,迎角90°时堵塞度达18％,阻力系数洞壁干扰修正值可达真实值的70％。又如某农机机翼半模,迎角40°时堵塞度达8％。压力系数洞壁干扰修正值达真实值的30％。因此,在进行半模实验时,洞壁干扰修正的准确性十分重要。     

MESSENGER: Exploring Mercury’s Magnetosphere

The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission to Mercury offers our first opportunity to explore this planet’s miniature magnetosphere since the brief flybys of Mariner 10. Mercury’s magnetosphere is unique in many respects. The magnetosphere of Mercury is among the smallest in the solar system; its magnetic field typically stands off the solar wind only ∼1000 to 2000 km above the surface. For this reason there are no closed drift paths for energetic particles and, hence, no radiation belts. Magnetic reconnection at the dayside magnetopause may erode the subsolar magnetosphere, allowing solar wind ions to impact directly the regolith. Inductive currents in Mercury’s interior may act to modify the solar wind interaction by resisting changes due to solar wind pressure variations. Indeed, observations of these induction effects may be an important source of information on the state of Mercury’s interior. In addition, Mercury’s magnetosphere is the only one with its defining magnetic flux tubes rooted beneath the solid surface as opposed to an atmosphere with a conductive ionospheric layer. This lack of an ionosphere is probably the underlying reason for the brevity of the very intense, but short-lived, ∼1–2 min, substorm-like energetic particle events observed by Mariner 10 during its first traversal of Mercury’s magnetic tail. Because of Mercury’s proximity to the sun, 0.3–0.5 AU, this magnetosphere experiences the most extreme driving forces in the solar system. All of these factors are expected to produce complicated interactions involving the exchange and recycling of neutrals and ions among the solar wind, magnetosphere, and regolith. The electrodynamics of Mercury’s magnetosphere are expected to be equally complex, with strong forcing by the solar wind, magnetic reconnection, and pick-up of planetary ions all playing roles in the generation of field-aligned electric currents. However, these field-aligned currents do not close in an ionosphere, but in some other manner. In addition to the insights into magnetospheric physics offered by study of the solar wind–Mercury system, quantitative specification of the “external” magnetic field generated by magnetospheric currents is necessary for accurate determination of the strength and multi-polar decomposition of Mercury’s intrinsic magnetic field. MESSENGER’s highly capable instrumentation and broad orbital coverage will greatly advance our understanding of both the origin of Mercury’s magnetic field and the acceleration of charged particles in small magnetospheres. In this article, we review what is known about Mercury’s magnetosphere and describe the MESSENGER science team’s strategy for obtaining answers to the outstanding science questions surrounding the interaction of the solar wind with Mercury and its small, but dynamic, magnetosphere.     

基于惯性定位定向的高铁轨检仪研究

根据高铁轨道静态检测的测量需求,设计了一种利用定位定向技术的0级轨检仪,详细阐述了其构成和工作原理,介绍了其特点。通过对比性分析论证,优选了一种测量精度高、操作方法简单且可大幅度提高测量效率的设计方案。理论仿真表明,本系统测量精度能够达到优于13mm/km水平。根据理论仿真结果搭建了原理简易验证设备,结合高铁测控网的测量基准,在一段高铁的弯道铁轨上进行了验证测试。从测试结果看,样机测量精度的重复性可以到达1mm/500m（1σ）的水平,10次测量效率优于500m/2h,表明采用定位定向技术的0级轨检仪具备实际工程化的潜力,以及提高测量效率和精度的能力。