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。     

Mineralogical biosignatures and the search for life on Mars

If life ever existed, or still exists, on Mars, its record is likely to be found in minerals formed by, or in association with, microorganisms. An important concept regarding interpretation of the mineralogical record for evidence of life is that, broadly defined, life perturbs disequilibria that arise due to kinetic barriers and can impart unexpected structure to an abiotic system. Many features of minerals and mineral assemblages may serve as biosignatures even if life does not have a familiar terrestrial chemical basis. Biological impacts on minerals and mineral assemblages may be direct or indirect. Crystalline or amorphous biominerals, an important category of mineralogical biosignatures, precipitate under direct cellular control as part of the life cycle of the organism (shells, tests, phytoliths) or indirectly when cell surface layers provide sites for heterogeneous nucleation. Biominerals also form indirectly as by-products of metabolism due to changing mineral solubility. Mineralogical biosignatures include distinctive mineral surface structures or chemistry that arise when dissolution and/or crystal growth kinetics are influenced by metabolic by-products. Mineral assemblages themselves may be diagnostic of the prior activity of organisms where barriers to precipitation or dissolution of specific phases have been overcome. Critical to resolving the question of whether life exists, or existed, on Mars is knowing how to distinguish biologically induced structure and organization patterns from inorganic phenomena and inorganic self-organization. This task assumes special significance when it is acknowledged that the majority of, and perhaps the only, material to be returned from Mars will be mineralogical.     

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。     

欧洲同步科学卫星用的远地点发动机

意大利斯尼亚粘胶公司和法国“欧洲推进公司”于1973年5月开始联合研制“GEOS”欧洲同步科学卫星的远地点发动机,前者负责计划管理,发动机设计,推进剂和绝热层研制,发动机的装配和试验;后者负责壳体、喷管和点火器的设计、制造和试验。计划于1976年1月完成,将成为欧洲首创的远地点发动机。发动机长1130毫米,直径684毫米,装端羧聚丁二烯推进剂267公斤,壳体材料用 Ti—6A1—4V 钛合金,绝热层用石棉乙丙橡胶,采用半潜入喷管,喉径67毫米,膨胀比37,高密度石墨喉衬,碳布缠绕扩散段。发动机总重303公斤,燃烧室平均压力23公斤/厘米~2,真空最大推力2360公斤,真空比冲286秒,使用温度范围-10~℃～+40℃,相应的燃烧时间为51和47秒。研制工作分初步设计、金属件设计,组件鉴定,研制试验,鉴定试验和验收试验六个阶段。研制、鉴定试验中全尺寸发动机试车4发,验收批4发,其中试车2发,交货2发,提出这个报告时,正进行鉴定试验工作,已经取得的试验结果都很好,但研制试验有一台发动机经 X 射线检查,发现装药有缺陷而未进行试车。     

导引头实物仿真技术

讨论了美国陆军导弹司令部在研制面空导弹时采用的导引头实物仿真技术.目前在导弹系统的研制过程中,人们受到很多限制,例如经费有限,需要进行可靠的系统试验,要求在逼真的环境,包括电磁干扰和抗干扰环境中评价系统等.导引头实物仿真试验能为解决上述问题发挥重要作用.介绍和讨论了射频、非红外成像和电-光波段的现有仿真设备及其性能;举例介绍了最近完成的仿真试验结果及其对降低导弹系统研制成本所起的作用.最后介绍了主要的仿真技术和美国陆军提高仿真器能力的未来计划.     

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。     

通过聚集探测SAR图像中的动目标

本文介绍的是一种在合成孔径雷达（SAR）图像中探测动目标的方法。这种方法是将SAR复图像分成若干分区，分别对各个分区进行聚焦，然后测量聚焦区域中锐度的增长情况，这种方法能敏锐地检测到目标的方位速度，对目标径向加速度的检测尤为敏锐，还能对任意方向的运动进行检测，对于只能检测快速运动目标径向速度的传统多普勒传感动目标指示器而言，这种方法是一种有效的补充。     

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.     

Effect of weightlessness on posture and movement control during a whole body reaching task

Here are reported preliminary results of the “Synergy” experiment performed aboard the Russian orbital station “MIR” in July 1993 (Altaïr Mission). The experiment was carried out before, during, and after the space flight of two astronauts (S1 and S2). The duration of the flight was 21 days for S1 and 6 month for S2. The subjects were tested during preflight, inflight and postflight. The astronaut subjects were fixed on the ground by the feet. They were asked to pick up a box in front of them on the ground. Two velocities of movement and two distances of the target to be reached were tested. The movement of several small markers placed on the body was recorded on video tape.

Results show that the shape of head and hand trajectories in the sagittal plane remains roughly the same during the flight in spite of the modification of mechanical constraints. Trajectory invariance does not result in joint angular displacement invariance. These data indicate that the planning of the movement takes place in terms of head and hand trajectories rather than joint rotations as it was previously suggested for simple arm reaching movement.     

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.