RDX/AP 复合推进剂中声不稳定性的微粒抑制

为了说明微粒对于环三甲撑三硝胺(RDX)/过氯酸铵(AP)复合推进剂燃烧时观察到的高频燃烧不稳定的抑制作用,进行了本项实验研究。实验中看到了很高频率的燃烧不稳定,它是在推进剂药柱的圆形孔道中发生的10-30KH_2范围的横向波。这种不稳定性可以通过添加少量固体微粒而被有效地消除。燃烧不稳定区已确定为微粒大小和浓度的函数。在压力—微粒浓度曲线上确定了发生不稳定燃烧的临界范围。根据 Horton 和 McGie 的微粒抑制理论计算出临界条件下的抑制常数(α_(p.(?))),并由假设(α_(p.(?)))=-α_g 求出推进剂的增长常数(α_g)。     

固体推进剂药柱结构安全裕度预测方法述评

当前,各工业公司用来预测固体推进剂药柱结构安全裕度的方法各不相同。虽然他们所用的计算公式均很相似,但针对具体问题算得的安全裕度值却是有正有负。事实上,这一问题已成为发动机药柱设计结构完整性评定工作产生混乱的根源。本文评论了影响安全裕度计算的各项参数,即破坏准则、结构分析方法、推进剂响应和破坏特性。本文还鉴别和讨论了与上述参数有关的技术问题,提出了今后研究工作中应予关注的问题。     

火箭发动机壳体爆破实验时的声发射

1.引言用声发射(AE)技术对压力容器和压力边界进行结构评价是声发射的应用中很有吸引力的领域之一。本文介绍了由NAIS系统最先提出的评价缺陷程度的方法应用于东京大学的M—13火箭发动机壳体的爆破实验的情况,目的是为了评价由于水压压力上升时该发动机壳体的有害度,而且讨论了断口特征和得到的声发射结果之间的关系。更进一步讨论了在高压     

The dynamics of blood biochemical parameters in cosmonauts during long-term space flights

Most of the previously obtained data on cosmonauts' metabolic state concerned certain stages of the postflight period. In this connection, all conclusions, as to metabolism peculiarities during the space flight, were to a large extent probabilistic. The purpose of this work was study of metabolism characteristics in cosmonauts directly during long-term space flights. In the capillary blood samples taken from a finger, by "Reflotron IV" biochemical analyzer, "Boehringer Mannheim" GmbH, Germany, adapted to weightlessness environments, the activity of GOT, GPT, CK, gamma-GT, total and pancreatic amylase, as well as concentration of hemoglobin, glucose, total bilirubin, uric acid, urea, creatinine, total, HDL- and LDL cholesterol, triglycerides had been determined. HDL/LDL-cholesterol ratio also was computed. The crewmembers of 6 main missions to the "Mir" orbital station, a total of 17 cosmonauts, were examined. Biochemical tests were carried out 30-60 days before launch, and in the flights different stages between the 25-th and the 423-rd days of flights. In cosmonauts during space flight had been found tendency to increase, in compare with basal level, GOT, GPT, total amylase activity, glucose and total cholesterol concentration, and tendency to decrease of CK activity, hemoglobin, HDL-cholesterol concentration, and HDL/LDL - cholesterol ratio. Some definite trends in variations of other determined biochemical parameters had not been found. The same trends of mentioned biochemical parameters alterations observed in majority of tested cosmonauts, allows to suppose existence of connection between noted metabolic alterations with influence of space flight conditions upon cosmonaut's body. Variations of other studied blood biochemical parameters depends on, probably, pure individual causes.     

CASH 2021: commercial access and space habitation

Issues about commercialization of space have been a growing concern in the past decade for the space community. This paper focuses on the work from a team of 51 students attending the Summer Session Program of the International Space University in Bremen, Germany. CASH 2021 (Commercial Access and Space Habitation) documents a plan that identifies commercial opportunities for space utilization that will extend human presence in space, and will chart the way forward for the next 20 years. The group selected four commercial sectors that show the most promise for the future: tourism, entertainment, space system service, assembly and debris removal, and research and development/production. The content of this document presents the results of their research. Historical activities in each of the commercial sectors are reviewed along with the current market situation. To provide a coherent background for future commercialization possibilities a scenario has been developed. This scenario includes a postulated upon ideal future and includes social, political and economic factors that may affect the space industry over the timeline of the study. The study also presents a roadmap, within the limited optimistic scenario developed, for the successful commercialization of space leading to future human presence in space. A broad range of commercially viable opportunities, not only within the current limits of the International Space Station, but also among the many new developments that are expected by 2021 are discussed.     

具有应变梯度的复合推进剂中裂纹扩展的特性

本文研究在具有应变梯度、填充密度大的复合推进剂中裂纹扩展的特性。采用中心有楔形裂纹的双轴试样。在室温、恒定十字头速度下进行试验。考虑了两种裂纹长度。通过分析试验数据来研究初始裂纹长度和非均匀总应变场对推进剂裂纹扩展特性的影响,还研究了测量裂纹长度所用时间间隔对裂纹扩展速率计算精度的影响。     

军用精密声表面波振荡器的研制

近年来,美国雷声公司已经有研制300～600MHz可军用的声表面波振荡器的课题;此种振荡器在频率调节能力和稳定性两方面均达当代最高水平。本文不讨论这种振荡器的详细用途。对它的要求一般为:(1)噪声本底必需至少为-160dBc/Hz;(2)振动灵敏度至少应与AT切体波器件一样好;(3)振荡器频率应能在大致±10ppm频率窗内进行调节并加以保持。在某些情况还要求加热时间小于3分钟。在满足这些要求方面,雷声公司已取得明显进展。本文将对这种进展加以讨论。在频谱纯度方面,文中讨论了二个题目:其一是低噪声放大器。实验证明,当它与310MHz声表面波谐振器联用时,噪声本底可达-176dBc/Hz。其二主要讨论了外部振动对噪声边带的影响。研制声表面波振荡器最重要的方面之一就是它的频率调节能力。利用金衬微调技术被证实既适用于延迟线也适用于谐振器。文中给出了实验结果,也讨论了在焊封过程中产生频移(约100ppm数量级)这一复杂情况。但已提出一种外部牵引频率技术来重调频率。在很多应用场合要求用恒溫箱以保持常温,于是就要求快速加热,而给出的数据要能显示出3分钟加热周期的频率稳定度。最后,除上述要求外,还要求声表面波振荡器的长稳保持在～1ppm/年的水平。利用提供的数据来确定冷焊密封在TO-8型外壳中的器件的基本老化率,同时也示出微调器件以及低振动灵敏度器件的变化率。     

分时移相调制的多路光纤陀螺仪

本文提出一上实现多路多轴光纤陀螺仪的新方法。Ｎ个Ｓａｇｎａｃ干涉仪通过一个２×Ｎ个耦合器共用一个光源。这些干涉仪都以通常的方法相位调制来进行调制然而，这些调制都在时间上有τ／Ｎ的延尺，τ是进入光纤环圈的平均传输时间。     

A status report on the characterization of the microgravity environment of the International Space Station

A primary objective of the International Space Station is to provide a long-term quiescent environment for the conduct of scientific research for a variety of microgravity science disciplines. Since continuous human presence on the space station began in November 2000 through the end of Increment-6, over 1260 hours of crew time have been allocated to research. However, far more research time has been accumulated by experiments controlled on the ground. By the end of the time period covered by this paper (end of Increment-6), the total experiment hours performed on the station are well over 100,000 hours (Expedition 6 Press Kit: Station Begins Third Year of Human Occupation, Boeing/USA/NASA, October 25, 2002). This paper presents the results of the on-going effort by the Principal Investigator Microgravity Services project, at NASA Glenn Research Center, in Cleveland, Ohio, to characterize the microgravity environment of the International Space Station in order to keep the microgravity scientific community apprised of the reduced gravity environment provided by the station for the performance of space experiments. This paper focuses on the station microgravity environment for Increments 5 and 6. During that period over 580 Gbytes of acceleration data were collected, out of which over 34,790 hours were analyzed. The results presented in this paper are divided into two sections: quasi-steady and vibratory. For the quasi-steady analysis, over 7794 hours of acceleration data were analyzed, while over 27,000 hours were analyzed for the vibratory analysis. The results of the data analysis are presented in this paper in the form of a grand summary for the period under consideration. For the quasi-steady acceleration response, results are presented in the form of a 95% confidence interval for the station during "normal microgravity mode operations" for the following three attitudes: local vertical local horizontal, X-axis perpendicular to the orbit plane and the Russian torque equilibrium attitude. The same analysis was performed for the station during "non-microgravity mode operations" to assess the station quasi-steady acceleration environment over a long period of time. The same type of analysis was performed for the vibratory, but a 95th percentile benchmark was used, which shows the overall acceleration magnitude during Increments 5 and 6. The results, for both quasi-steady and vibratory acceleration response, show that the station is not yet meeting the microgravity requirements during the microgravity mode operations. However, it should be stressed that the requirements apply only at assembly complete, whereas the results presented below apply up to the station's configuration at the end of Increment-6.