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501.
通过对星间链路和空间态势感知系统国内外发展现状的分析,指出星间链路在空间信息有效获取、安全传输和实时应用以及保障空间态势感知系统战场生存能力等方面起着重要的作用.针对星间链路在未来空间态势感知系统中的应用需求,提出包含空间通信模型和空间导航模型在内的空间感知体系基本架构,并对该架构下星间链路的设计要求或者特点进行分析,指出星间链路应该具有灵活可变的星间路由策略和联网结构,并能够支持高速可变和安全可靠的星间数据传输.分别从空间网络和卫星节点2个层面提出了系统实现的关键技术,并给出部分关键技术的研究重点和研究方法.上述研究结果可以为星间链路及相关领域的研究工作提供一定的借鉴和帮助.  相似文献   
502.
Using low power electronic devices for space applications to reduce the mass and energy consumption has lead to electromagnetic interference (EMI) problem. Electronic enclosures are used to shield electronic devices against EMI. In the past, electromagnetic shielding has been mainly the only criteria considered in electronic enclosure design. However, there are several structural and thermal requirements for selection of shielding materials which should also be taken into account. In this research work, three quantitative materials selection methods, i.e. Digital Logic (DL), Modified Digital Logic (MDL), and Z-transformation, are employed to select the best material from among a list of candidate materials. Composite and metallic electronic enclosures are explored and the best material is selected. Z-transformation method is applicable to both of the considered case studies while DL and MDL can only be used for solving one of them. Z-transformation method ranks aluminum as the first choice among various metallic materials. The wide range of Z-transformation application and its practical results confirm the superiority of Z-transformation method over DL and MDL methods.  相似文献   
503.
受快速傅里叶变换(fast Fourier transform,FFT)的影响,基于FFT和压缩感知(compressive sensing, CS)的脉冲星周期快速估计算法的计算量大。为进一步减小计算量并提高计算精度,利用离散余弦变换(discrete cosine transform,DCT)取代FFT,提出了一种基于DCT-CS的脉冲星周期超快速估计算法。在该方法中,利用DCT提取脉冲星信号的低频部分构建低频DCT矩阵;构建畸变轮廓字典并获取累积轮廓;提出了利用最大值超分辨率稀疏恢复估计脉冲星周期的方法。仿真结果表明,DCT-CS的脉冲星周期估计精度达到了3.82×10-12 s,计算时间达到了9.31 ms。与FFT-CS相比,周期估计精度提高了约16%,计算时间缩短了约37.5%,实现了实时高精度的脉冲星周期估计。  相似文献   
504.
To evaluate the effects of ionizing radiation (IR) on murine preosteoblastic cell differentiation, we directed OCT-1 cells to the osteoblastic lineage by treatment with a combination of β-glycerophosphate (β-GP), ascorbic acid (AA), and dexamethasone (Dex). In vitro mineralization was evaluated based on histochemical staining and quantification of the hydroxyapatite content of the extracellular bone matrix. Expression of mRNA encoding Runx2, transforming growth factor β1 (TGF-β1), osteocalcin (OCN), and p21CDKN1A was analyzed. Exposure to IR reduced the growth rate and diminished cell survival of OCT-1 cells under standard conditions. Notably, calcium content analysis revealed that deposition of mineralized matrix increased significantly under osteogenic conditions after X-ray exposure in a time-dependent manner. In this study, higher radiation doses exert significant overall effects on TGF-β1, OCN, and p21CDKN1A gene expression, suggesting that gene expression following X-ray treatment is affected in a dose-dependent manner. Additionally, we verified that Runx2 was suppressed within 24 h after irradiation at 2 and 4 Gy. Although further studies are required to verify the molecular mechanism, our observations strongly suggest that treatment with IR markedly alters the differentiation and mineralization process of preosteoblastic cells.  相似文献   
505.
This paper reviews the medical operations performed on six European astronauts during seven space missions on board the space station Mir. These missions took place between November 1988 and August 1999, and their duration ranged from 14 days to 189 days. Steps of pre-flight medical selection and flight certification are presented. Countermeasures program used during the flight, as well as rehabilitation program following short and long-duration missions are described. Also reviewed are medical problems encountered during the flight, post-flight physiological changes such as orthostatic intolerance, exercise capacity, blood composition, muscle atrophy, bone density, and radiation exposure.  相似文献   
506.
Why the draft Treaty on the Prevention of the Placement of Weapons in Outer Space, the Threat or Use of Force Against Outer Space Objects (PPWT) will not work - whereas the Code of Conduct for Outer Space Activities may.  相似文献   
507.
Poland has a long-standing tradition in space activities. Polish institutions have participated as co-investigators in almost all European Space Agency (ESA) science projects, as well as on many other missions. However, the first Polish satellite (PW-SAT) was only launched in 2012. Poland was one of the first Eastern European countries to conclude a Cooperation Agreement with ESA in the peaceful use of outer space; it was signed in 1994 and followed by a second in January 2002. Negotiations on Polish membership in the ESA were started in autumn of 2011, and ended in April 2012. Following ratification of the agreement, Poland officially became the 20th Member State of ESA on 19 November 2012. This article examines how Poland is setting its way as a space nation. It describes recent developments in the Polish space programme, including the road to Poland's full membership in the European Space Agency.  相似文献   
508.
简介了国外月球和火星等探测器软着陆缓冲机构"触地"敏感技术与应用,提出了采用冲击加速度检测的探测器软着陆缓冲机构(足垫)触月敏感触发方案,阐述了敏感触发装置的设计思想,分析了探测器软着陆触月过程的动力学响应,论述了触发装置的冲击加速度敏感检测方式与原理以及电路单元设计。该装置比较适合月球探测器软着陆缓冲机构的结构和工作特点,可以满足制导、导航与控制(GNC)主控系统设计要求。  相似文献   
509.
In 2012 a working group was established to formulate the African space policy and strategy which would lead to the establishment of an African Space Agency (ASA). Dr Peter Martinez asserts in his article “Is there a need for an African Space Agency?” [1] that the arguments that have been posited in support of an ASA are flawed; namely the arguments of the existing example of the European Space Agency (ESA), and that an ASA would lead to fostering competition, synergy, industrial development and capacity building. While this viewpoint agrees that all the perfect conditions may not exist at present for the creation of an ASA, it addresses some of the issues raised by Martinez, and proposes ideas to foster intra-regional cooperation.  相似文献   
510.
This paper describes the experimental and computational analyses of a high velocity aluminum projectile impact on an Al6061-T6 spacecraft inner wall at different oblique angles. Al2017-T4 spherical projectiles of 5.56 mm in diameter and 0.25 g in weight were chosen within the velocity range of 1000±200 m/s due to the limitation of the light gas gun. The energy absorbed was calculated by measuring the velocities before and after impact on the inner wall. The energy absorbed by the wall and the remaining energy carried by the projectile helped to estimate the severity of further damage to inner components. Afterwards, validation was done by using the commercially available software LS-DYNA with a dedicated SPH. On average, a 10% energy absorption difference between experimentation and simulation was found. By using C-SCAN, the damage area proportion of the total inner wall to impact penetration hole area was found to be on average 6%, 26% and 53% greater than the projectile cross sectional area for the oblique angle impacts of 30°, 45°, and 60°, respectively. These findings helped to understand the relationship between the oblique impact event and the damage area on a spacecraft inner wall along with space debris cloud propagation and comparison with experimental results using LS-DYNA.  相似文献   
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