现代谱分析技术综述

本文综述了最近20年推出的有关离散时序谱分析的新方法。对每个方法所假设的基本时序模型作的分析,构成本文了解各种谱分析方法之间差别的共同基础。所讨论的方法包括经典的周期图法、经典的 Blackman-Tukey 法、自回归(最大熵)法、滑动平均法、自回归滑动平均法、最大似然法、Prony 法和 Pisarenko 法。正文中的一览表对所有方法作了简要的评述,包括基本的参考文献和计算每一谱估计的相应公式     

Research priorities and plans for the International Space Station-results of the 'REMAP' Task Force

Recent events in the International Space Station (ISS) Program have resulted in the necessity to re-examine the research priorities and research plans for future years. Due to both technical and fiscal resource constraints expected on the International Space Station, it is imperative that research priorities be carefully reviewed and clearly articulated. In consultation with OSTP and the Office of Management and budget (OMB), NASA's Office of Biological and Physical Research (OBPR) assembled an ad-hoc external advisory committee, the Biological and Physical Research Maximization and Prioritization (REMAP) Task Force. This paper describes the outcome of the Task Force and how it is being used to define a roadmap for near and long-term Biological and Physical Research objectives that supports NASA's Vision and Mission. Additionally, the paper discusses further prioritizations that were necessitated by budget and ISS resource constraints in order to maximize utilization of the International Space Station. Finally, a process has been developed to integrate the requirements for this prioritized research with other agency requirements to develop an integrated ISS assembly and utilization plan that maximizes scientific output.     

Climate model studies of synchronously rotating planets

M stars constitute 75% of main sequence stars though, until recently, their star systems have not been considered suitable places for habitable planets to exist. In this study the climate of a synchronously rotating planet around an M dwarf star is evaluated using a three-dimensional global atmospheric circulation model. The presence of clouds and evaporative cooling at the surface of the planet result in a cooler surface temperature at the subsolar point. Water ice forms at the polar regions and on the dark side, where the minimum temperature lies between -30 degrees C and 0 degrees C. As expected, rainfall is extremely high on the starlit side and extremely low on the dark side. The presence of a dry continent causes higher temperatures on the dayside, and allows accumulation of snow on the nightside. The absence of any oceans leads to higher day-night temperature differences, consistent with previous work. The present study reinforces recent conclusions that synchronously rotating planets within the circumstellar habitable zones of M dwarf stars should be habitable, and therefore M dwarf systems should not be excluded in future searches for exoplanets.     

用于大型固体推进剂火箭发动机的独特点火系统试验

本文介绍了用于大型固体推进剂火箭发动机的组合式无喷管、无壳体点火器方案的设计、分析及试验结果。该点火方案的主要优点是可以把60%左右的点火器消极重量变成药柱有效载荷。点火系统的主装药由点火器周围的发动机前段装药所构成。这段装药又是发动机推进剂药柱的一部分,设计成象一个小的低压无喷管火箭发动机,给主发动机推进剂段提供足够的压力和热流输出以实现发动机点火。前段推进剂的点火由一个比较小的径向排气的BKNO_3烟火剂药片点火器来实现。试验计划需验证三个方面的设计问题:     

用X射线系统检测三叉戟火箭发动机

洛克希德公司研制了一种X射线实时显像系统,用于检测海军C4三叉戟固体火箭发动机。此法比普通X射线系统检测更完全、更均匀、效率高且费用明显降低。这一看法为生产三叉戟导弹第一级发动机的赛奥科尔公司、生产该导弹第二、三级发动机的赫克利斯公司和航空喷气战术系统公司的实验所证明。航空喷气公司利用该系统检测了陆军的霍克导弹发动机和海军通用动力标准导弹发动机。     

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。     

固体推进剂发动机的比冲予示

实际比冲的理论予示方法大家是比较熟悉的.这些方法包括计算由于两相流、扩散、边界层、动能、喷管潜入和不完全燃烧造成的损失。在典型的加铝推进剂中最大的计算损失是两相流损失;由于粒子的大小和分布是不能精确知道的,因此这种计算也就具有最大的不精确性.本文中把由试验数据获得的平均粒子直径与喉径的关系用在固体火箭性能予示程序(SPP)方面,以便予示一系列发动机的推进剂比冲。这些予示与试验结果进行比较。结果指出比冲效率可认为与推进剂的本质有关.此外,试验比冲和比冲效率对发动机和推进剂变量是统计地相关的。这些相关性与较复杂的、较昂贵的理论分析一样准确.除比冲予示外,相关方程在发动机设计最佳化中是有用的。     

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.     

中国航天发展政策和展望

航天技术是人类开展空间活动，探索、开发和利用外层空间的综合性工程技术，是当今世界高科技群体中最具影响力的科学技术之一。它使人类活动范围从地面扩展到太空，从根本上改变了人们的思维方式、生产方式和生活方式。自第一颗人造卫星上天以来，空间技术不断渗透到人类活动的各个领域，空间应用成为现代信息社会不可缺少的重要组成部分，而空间科学的发展则带给世界科学技术发展以崭新的视角。航天技术的发展历程表明，它已不仅是振奋人心的科学成就，而且是提高人类生活质量，扩展人类生存空间，开发新的资源的重要途径。同时，航天技术…     

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.