中国空间碎片防护研究工作进展

回顾了2006年中国空间碎片防护研究工作的情况,简要介绍了MODAOST软件研究的相关活动,以及风险评估及防护结构优化技术、超高速撞击横向校验、部件/分系统和空间碎片撞击感知技术。     

酚醛树脂基纳米多孔材料的制备及结构调控

酚醛树脂基纳米多孔材料（Phenolic Resin-based Nanoporous Materials,PNM）是满足新一代航天飞行器轻质、高效隔热需求的新型热防护材料,传统制备方法中需使用超临界干燥技术,制备周期长、成本高。本研究通过两步法,即先合成线性酚醛树脂,再进行溶胶-凝胶的方法,实现了常压干燥PNM的制备。系统研究了固化剂含量、固化温度和固化时间对材料结构的影响和调控作用,分析了影响材料收缩率和热稳定性的因素。结果表明,PNM的微观纳米结构的变化会影响材料干燥后的收缩率,制备大颗粒、大孔径的微观结构更有利于降低材料的收缩率。而PNM的热稳定性主要受交联反应过程形成的化学结构的影响,通过优化固化剂的含量可提高PNM的热稳定性。当固化剂含量为10%,固化温度提高至150℃,固化时间延长至48 h的条件下,获得的PNM有最高的热稳定性（900℃下的残碳率为54.2%）、最发达的孔结构（比表面积为264.0 m²/g、孔容为2.67 cm³/g、平均孔径为40.0 nm）和最小的收缩率（0%）。此PNM制备方法简单、性能优异,在未来航天飞行器上有广阔的应用前景。     

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.     

航空永磁发电机的火灾保护

介绍一种应用于航空永磁发电机绕组短路保护的脱开机构，并为此脱开机构设计了测试电路，通过对脱开时间的测试，证明了这种脱开机构是有效的，最后对测试误差进行了分析。     

分区和有限容积法计算长尾喷管中的湍流流动

为了给长尾喷管热防护结构设计提供热边界条件，从轴对称二维雷诺平均N－S方程出发，采用分区算法和有限容积法计算了长尾喷管中的湍流流动，分析了流场的结构特性，提出了长尾喷管中燃气温度，压强和马赫数分布的某些规律以及燃气温度沿壁面的分布，计算和分析结果提出了长尾喷管热防护结构设计应注意的事项。     

可重复使用热防护系统防热结构及材料的研究现状

在对国外有关各类航天器的防热结构和材料进行广泛调研的基础上，对陶瓷瓦、柔性毡、盖板等防热结构及材料进行了介绍，并总结了防热结构和防热材料的发展现状及趋势。     

Linux 2．6内存保护机制研究

基于Intel i386平台处理器和Linux 2.6内核源代码,从硬件内存保护和虚拟内存保护两个方面分析了最新的Linux内存保护机制,其中硬件内存保护机制包括段式映射阶段的访问控制、页式映射阶段的访问控制以及最新内存保护NX(No eXecute)技术,虚拟内存保护机制包括虚拟区间保护、虚拟区间加锁和Hole技术.最后进一步讨论了增强Linux内存保护的方案.     

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.     

热障涂层在涡轮叶片应用中的热防护有效性

建立了含热障涂层的涡轮叶片简化传热模型,通过理论推导建立了热障涂层的有效性判据,并基于此进行了热防护有效性分析。理论分析与数值实验表明:由热障涂层带来的复合传热表面传热系数的变化会显著影响热障涂层的热防护效果;在发动机典型工况下,对于处于高温区的高压涡轮叶片前缘处,热障涂层引起的复合传热表面传热系数变化率最大值的范围为1.25%~10.83%以满足热防护有效性要求。在工程中应特别注意由于热障涂层的应用带来的复合传热表面传热系数的变化,否则会导致热防护失效,甚至产生反效果。      

新型一体化热防护系统热力分析与试验研究

高速飞行器对结构效率的苛刻要求使得热防护系统不断趋于向轻质化、集成化方向发展,新型的力热耦合一体化热防护系统(ITPS)极具发展潜力.首先阐释了一种新型一体化热防护方案的概念与特点,总结了一体化结构设计的基本原则,数值分析了结构参数对背面温度响应、屈曲临界载荷的影响,结果表明腹板厚度对背面温度以及屈曲临界载荷的影响最大.然后设计并加工制备了ITPS的面板与单胞试验样件,分别展开了800℃的高温防隔热性能试验考核和屈曲性能的力学试验研究;试验表明腹板结构是引发热短路效应和屈曲的关键因素,屈曲试验与模拟结果吻合,高温屈曲分析表明温度梯度对屈曲特征有较大影响.