钛合金表面抗激光涂层损伤特性及热效应影响研究

实验研究了钛合金和高反射型陶瓷涂层材料抗连续型激光烧蚀的损伤及温度分布特性，并从热效应影响角度对比分析了二者在抗激光损伤效果方面的差异性。研究结果表明：相比于钛合金，高反射型陶瓷涂层材料能有效增强钛合金基底抗激光损伤的能力；在同等激光功率密度辐照下，陶瓷涂层材料能有效提升钛合金基底耐受激光辐照的时间长度。实验结果表明该陶瓷涂层材料的激光损伤阈值比钛合金高约5.8倍。实验发现陶瓷涂层温升速率高于钛合金，但由于陶瓷材料具有较高的反射特性，以及良好的热吸收和热传导特性，因此能使由激光辐照产生的热量在其表面较快地扩散，而降低向基底方向传导的程度，最终提升陶瓷涂层的抗激光损伤阈值。     

RFID技术在物流配送中的应用模型研究

文章阐述RFID物流配送系统的构成及其信息处理过程,探讨RFID电子标签在物流配送全过程中的信息识别作用,提出了RFID技术在现代物流配送中的一种新型应用模型和方法。     

MX导弹喷管用先进材料评论

目前正在进行研制石墨材料,准备用于MX 第一级和第二级固体火箭喷管的入口部,喉部,后喉部,出口锥和可延伸出口锥。这些材料必须经受住新型洲际弹道导弹(ICBM)喷管系统的苛刻的结构、化学侵蚀,粒子冲刷和高温环境。该系统的燃烧室压力可达127公斤/厘米~2,火焰温度为3700°K 至3922°K。叙述了第一级和第二级全尺寸试验喷管的现状。还提出了在喷管设计、石墨材料研制以及预期性能改进方面进一步工作的方向。     

传导、对流和辐射传热对火箭发动机使用寿命的影响

在存放场地,固体发动机会由于各种瞬时热应力而产生累积性损伤。引起这些瞬时热应力的是环境温度、风、太阳辐照等与地理位置有关的所有一切因素的作用。业已表明,与最大损伤发生在大应力值的假设相反,推进剂的粘弹特性使其在低应力值下出现显著的损伤。因此,防护性贮存对发动机的使用寿命并不总是有利的。     

The Interplanetary Internet: a communications infrastructure for Mars exploration

A strategy is being developed whereby the current set of internationally standardized space data communications protocols can be incrementally evolved so that a first version of an operational "Interplanetary Internet" is feasible by the end of the decade. This paper describes its architectural concepts, discusses the current set of standard space data communications capabilities that exist to support Mars exploration and reviews proposed new developments. We also speculate that these current capabilities can grow to support future scenarios where human intelligence is widely distributed across the Solar System and day-to-day communications dialog between planets is routine.     

MX导弹喷管用先进材料评论 Ⅱ 第一级喷管的先进材料

本文是评论MX导弹喷管先进材料的三篇文章中的第二篇。第一篇文章于1977年4月在SAMPE季刊中发表(译文见“固体火箭技术”1978年第二期第99—105页),综述了MX导弹喷管对材料的要求,叙述了石墨材料的结构、性质和性能之间的关系。本文继续对MX的第一级和第二级发动机喷管所用先进材料进一步进行评价。     

基于MATLAB的现代优化算法在飞行器气动外形设计中的应用

本文发展了MATLAB语言环境下的现代优化算法，包括遗传算法、模拟退火算法和基于分支联赛选择的多目标遗传算法，并用来求解高超声速飞行器气动外形参数优化问题。所研究的气动外形为带控制舵飞行器和可变弯体飞行器。在MATLAB环境下，求解了最大化升阻比的单目标优化问题和具体有两个冲突目标（最小化铰链力矩并且最大化平均操纵效率）的多目标优化问题。实际算例表明，在快速有效的气动力分析方法辅助之下，本文所发展的MATLAB现代优化算法可以在飞行器初始设计中发挥作用。本文所提供的现代优化算法是对MATLAB优化工具箱的一个有益的扩展。     

Production of neutrons from interactions of GCR-like particles

In order to help assess the risk to astronauts due to the long-term exposure to the natural radiation environment in space, an understanding of how the primary radiation field is changed when passing through shielding and tissue materials must be obtained. One important aspect of the change in the primary radiation field after passing through shielding materials is the production of secondary particles from the breakup of the primary. Neutrons are an important component of the secondary particle field due to their relatively high biological weighting factors, and due to their relative abundance, especially behind thick shielding scenarios. Because of the complexity of the problem, the estimation of the risk from exposure to the secondary neutron field must be handled using calculational techniques. However, those calculations will need an extensive set of neutron cross section and thicktarget neutron yield data in order to make an accurate assessment of the risk. In this paper we briefly survey the existing neutron-production data sets that are applicable to the space radiation transport problem, and we point out how neutron production from protons is different than neutron production from heavy ions. We also make comparisons of one the heavy-ion data sets with Boltzmann-Uehling-Uhlenbeck (BUU) calculations.     

ESA's Biopan 1--"Vitamin" experiment preliminary results

The purpose of “Vitamin” experiment is to study the efficiency of protective substances on three biological acellular systems aqueous solutions exposed to cosmic radiation in space. The first system “LDL”is a low density lipoprotein. The second is “E2-TeBG complexe” in which estradiol (E2) is bound to its plasmatic carrier protein, testosterone-estradiol binding globulin (TeBG). The third is “pBR 322”, a plasmid. “Vitamin” experiment was accomodated in the Biopan which had been mounted on the outer surface of a Foton retrievable satellite. The experiment was exposed to space environment during 15 days. A stable temperature of about 20 °C was maintained throughout the flight. “Vitamin” experiment preliminary results are presented and discussed.