客机起落架件号和改装标识分析

针对客机起落架件号不同的OEM标识规则进行对比分析,明确了起落架在进行翻修和改装的件号标识规则,提出了起落架组件和零件的标识方法,对于起落架日常维护、改装、翻修以及让步修理工作进行规范的刻号和标识具有重要参考价值,为相关人员快速识别起落架构型和改装状态提供了工具,同时也给互换性评估人员对起落架的识别提供了一定思路。     

基于动力学边界的结冰飞机安全预警方法

结冰严重破坏飞机的动力学特性，使飞机的非线性和动力学耦合特性表现明显，导致传统的安全预警方法无法准确有效地评估飞行存在的潜在风险，易引发飞行事故。为解决此问题，提出了一种基于动力学边界的新型安全预警方法，该方法可综合考虑飞机的动力学耦合特性，可为结冰飞机的实时安全预警系统的构建提供有力的理论支撑。首先，基于微分流形理论确定结冰飞机精确的动力学边界，并详细分析了飞机结冰对动力学边界的影响；其次，利用动力学边界相对距离对飞行风险进行量化，结合动力学边界的特性确定了安全预警的方法；最后，搭建了飞行仿真训练系统，并以着陆为训练科目，通过与传统迎角安全预警方法对比，得到基于动力学边界安全预警方法的优越性。研究结果表明，相比于传统迎角限制方法，动力学边界安全预警方法可提前发现飞行中存在的潜在风险，且基于此方法的飞行训练系统可对驾驶员进行结冰安全操纵训练可提高结冰飞机的飞行安全。     

着陆姿态对地外天体表层采样的影响研究

表层采样技术是获得地外天体特性的重要手段,是完成地外天体采样任务的一项关键技术。文章结合4自由度表层采样装置的特点,建立了表层采样装置的逆运动学模型,分析了极限着陆姿态下表层采样装置安装位置在当地参考坐标系中的变化,并针对一次封装与二次封装过程中表层采样装置的位置和姿态要求,明确了末端采样器姿态补偿方法,提出了着陆姿态对表层采样影响的分析算法。仿真结果表明,该算法能有效分析着陆姿态对表层采样的影响,可为表层采样装置适应性设计提供支持。     

On the planetary ionospheric vortex electric fields

The paper presents a physical mechanism of large-scale vortex electric field generation in the ionospheric E- and F-layers. It shows that the planetary-scale, synoptic short-period (from several second to several hours) and fast processes (with propagation velocity higher than 1 km/s) produce a planetary-scale internal vortex electric field. Its value may far exceed that of the dynamo-field generated in the same ionospheric layer by local wind motion. We found, that an ionospheric source of the vortex electric field is spatial inhomogeneity of the geomagnetic field.     

Antiparticle content in the magnetosphere

In the present work we assess the stable and transient antiparticle content of planetary magnetospheres, and subsequently we consider their capture and application to high delta-v space propulsion. We estimate the total antiparticle mass contained within the Earth’s magnetosphere to assess the expediency of such usage. Using Earth’s magnetic field region as an example, we have considered the various source mechanisms that are applicable to a planetary magnetosphere, the confinement duration versus transport processes, and the antiparticle loss mechanisms. We have estimated the content of the trapped population of antiparticles magnetically confined following production in the exosphere due to nuclear interactions between high energy cosmic rays (CR) and constituents of the residual planetary upper atmosphere.The galactic antiprotons that directly penetrate into the Earth’s magnetosphere are themselves secondary by its nature, i.e. produced in nuclear reactions of the cosmic rays passing through the interstellar matter. These antiproton fluxes are modified, dependent on energy, when penetrating into the heliosphere and subsequently into planetary magnetospheres. During its lifetime in the Galaxy, CR pass through the small grammage of the interstellar matter where they produce secondary antiprotons. In contrast to this, antiprotons generated by the same CR in magnetosphere are locally produced at a path length of several tens g/cm² of matter in the ambient planetary upper atmosphere. Due to the latter process, the resulting magnetically confined fluxes significantly exceed the fluxes of the galactic antiprotons in the Earth’s vicinity by up to two orders of magnitude at some energies.The radiation belt antiparticles can possibly be extracted with an electromagnetic-based “scoop” device. The antiparticles could be concentrated by and then stored within the superimposed magnetic field structure of such a device. In future developments, it is anticipated that the energy of the captured antiparticles (both rest energy and kinetic energy) can be adapted for use as a fuel for propelling spacecraft to high velocities for remote solar system missions.     

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.     

“阿波罗”登月舱的软着陆支架

登月舱的软着陆支架是确保月面探测活动及宇航员返回地球的关键装置。文章对“阿波罗”登月舱软着陆支架进行了介绍,描述了其技术指标、功能要求和基本组成,并对“阿波罗”登月舱软着陆支架的构型设计,主支柱、辅助支柱、足垫、展开架、收拢释放机构、展开锁定机构、触杆高度器以及铝蜂窝缓冲元件的设计方案进行了说明。鉴于“阿波罗”登月舱软着陆支架的设计通过了多次飞行试验的验证,文章结合“阿波罗”登月舱软着陆支架的方案,提出了中国载人登月工程中登月舱软着陆支架研制的建议。     

行星着陆复杂形貌特征匹配与自主导航研究进展

基于行星定点软着陆探测任务的需求,围绕复杂形貌行星着陆过程环境特点,首先分析了行星着陆复杂形貌特征匹配与自主导航所面临的主要技术挑战,随后综述了行星着陆复杂形貌特征匹配与自主导航的研究现状,并概括了行星着陆复杂形貌特征匹配与自主导航所涉及的关键技术。最后对未来行星着陆探测复杂形貌特征匹配与自主导航发展方向进行了展望。     

温度对油—气式起落架缓冲性能的影响研究

油—气式缓冲器内部的油液特性及充气压力会随环境温度而变化,进而影响起落架的缓冲性能。为了探究温度对油—气式起落架缓冲性能的影响,在起落架落震试验的基础上,提出一种缓冲器环境温度模拟方法,并分析油—气式起落架缓冲器在20~80℃环境温度下的缓冲性能。结果表明：在所研究的温度范围内,缓冲器初始充气压力对温度变化敏感,随着温...     

舰载飞机着舰拦阻动力学研究综述简

 拦阻着舰过程通常被认为是舰载飞机事故率最高的阶段,因此,自从有了航空母舰和舰载飞机,拦阻着舰动力学就一直是国内外相关研究人员的研究热点。本文从拦阻钩、拦阻装置和起落架3个关键部件着手,比较详细地论述了舰载飞机着舰拦阻涉及到的关键动力学问题及其研究现状,重点对拦阻钩弹跳动力学及其载荷分析、拦阻索动力学及其载荷分析、下沉速度、非对称拦阻对起落架载荷的影响、拦阻系统动力学等方面进行了综述。最后,对着舰拦阻动力学研究的发展趋势进行了展望。