火星探测着陆系统开伞控制方法研究

文章通过对火星探测进入轨道的分析，提出了一种以动压为控制目标的开伞控制方法，并借鉴过载-时间控制法的相关思想，结合火星探测进入轨道的特点，研究了该开伞控制法的原理和实现方法。根据火星探路者的实际进入条件，采用该方法的分析结果与实际飞行中的开伞情况基本吻合。     

风力机组叶片的先进翼型族设计

大型风力机组叶片设计需要专用的翼型族,以满足风力机组运行的环境要求。高升阻比、低粗糙度影响是该翼型族的气动性能特点。为了发展我国具有自主知识产权的风力机专用翼型族,在科技部863项目的支持下,北京航空航天大学联合国内气动研究单位,通过理论分析、数值模拟和风洞试验等技术途径,开发了两个适用于大型风力机组叶片的先进翼型族。理论分析和风洞试验表明,设计结果基本达到了预先设定的气动性能指标。     

飞机退租检的常见问题浅析

从维修记录、合同签署、结构修理、沟通谈判等方面分析了飞机在退租检工作中遇到的常见问题,总结出相应的解决方法,提出改进措施。     

复合材料抗冲击性能和结构压缩设计许用值

 从复合材料结构压缩设计许用值的概念和复合材料的冲击后压缩强度性能出发,讨论按NASA标准得到的CAI值与它们的关系,指出传统的CAI值不能充分反映复合材料体系的抗冲击性能,且与结构压缩设计许用值无任何联系。在对复合材料结构完整性要求和作者的试验研究,和对国外文献总结的基础上,提出复合材料抗冲击性能应包括损伤阻抗和损伤容限两方面。大量的试验数据证实复合材料层压板抗冲击性能存在拐点现象,在对拐点附近复合材料层压板的破坏机理研究基础上,建议用拐点附近的性能建立复合材料层压板抗冲击性能的评定体系,即可以用表面层在冲击下保持其完整性的最大能力(最大接触力)来表征复合材料体系的损伤阻抗(韧性);用出现拐点后基本不变的压缩强度(破坏应变)门槛值来表征复合材料体系的损伤容限。     

火星车转移坡道柔顺性优化设计及动力学分析

对一种抽展式火星车转移坡道开展柔顺性优化设计和动力学分析。首先,分析火星车与存在异面角的坡道的挤压几何原理。然后,设计坡道的间隙机构和限位机构,并计算出机构关键设计参数的最优值,以自适应调整两侧坡道的距离,〖JP2〗减小火星车与坡道护栏之间的相互作用力。最后,对坡道下落过程和火星车在坡道上的行驶过程进行动力学仿真,验证坡道柔顺性优化设计的效果。结果表明：优化后的坡道柔顺性大幅提高,坡道可以自适应调整两侧的距离;使用优化后的坡道,可以有效降低火星车与坡道护栏的作用力,实现火星车在坡道上的安全行驶。     

大跨时空任务背景下的太阳能无人机任务规划技术研究进展

通过任务规划技术合理的优化太阳能无人机的飞行轨迹和动力学参数,能够有效提高太阳能无人机的能量利用率,使其胜任许多大范围跨时间跨空间飞行任务。从能量建模、续航评估和能量管理策略3个方面对大跨时空任务背景下太阳能无人机任务规划技术的研究进展进行了综述。在能量建模方面,介绍了当前主流的太阳辐射模型和能量生产基本框架;在续航评估方面,分析了目前的指标设计和应用方法;在能量管理策略方面,从能量综合应用、风力滑翔机制、轨迹优化方法和面向特定任务的应用4个角度,梳理了当前的研究现状。最后,对该领域未来可能的研究方向进行了展望。     

浅析航天型号计量保证工作

计量保证工作是航天型号任务质量保障的基础,关系着型号任务的成败。主要介绍了航天型号任务中计量保证工作的现状和不足,结合航天型号任务的全流程工作,提出在型号任务各环节的计量保证工作建议。     

Survival and death of the haloarchaeon Natronorubrum strain HG-1 in a simulated martian environment

Halophilic archaea are of interest to astrobiology due to their survival capabilities in desiccated and high salt environments. The detection of remnants of salty pools on Mars stimulated investigations into the response of haloarchaea to martian conditions. Natronorubrum sp. strain HG-1 is an extremely halophilic archaeon with unusual metabolic pathways, growing on acetate and stimulated by tetrathionate. We exposed Natronorubrum strain HG-1 to ultraviolet (UV) radiation, similar to levels currently prevalent on Mars. In addition, the effects of low temperature (4, −20, and −80 °C), desiccation, and exposure to a Mars soil analogue from the Atacama desert on the viability of Natronorubrum strain HG-1 cultures were investigated. The results show that Natronorubrum strain HG-1 cannot survive for more than several hours when exposed to UV radiation equivalent to that at the martian equator. Even when protected from UV radiation, viability is impaired by a combination of desiccation and low temperature. Desiccating Natronorubrum strain HG-1 cells when mixed with a Mars soil analogue impaired growth of the culture to below the detection limit. Overall, we conclude that Natronorubrum strain HG-1 cannot survive the environment currently present on Mars. Since other halophilic microorganisms were reported to survive simulated martian conditions, our results imply that survival capabilities are not necessarily shared between phylogenetically related species.     

火星磁层顶形成和变化的理论研究

考虑太阳风动压与行星电离层中的带电粒子热压及磁压之和平衡,建立了有大气（电离层）的行星磁层顶形成的理论模型,结合卫星对火星的观测数据,对子午面内向日侧火星磁层顶位形进行了数值计算和分析,研究了火星磁层顶位形及其与太阳风动压之间的变化关系．结果认为,火星磁层顶位形与地球磁层顶相似．太阳风动压越大,火星磁层顶越靠近火星;太阳风动压越弱,火星磁层顶越远离火星．根据火星内秉磁矩从古到今逐渐减小的观点,探索了大尺度磁场（内禀磁矩）对火星磁层顶的贡献作用,结果认为大尺度磁场越强,火星磁层顶越远离行星．这对于进一步研究火星磁层的长期演化以及其他行星磁层的位形变化都具有重要的意义．     

Planetary protection issues related to human missions to Mars

In accordance with the United Nations Outer Space Treaties [United Nations, Agreement Governing the Activities of States on the Moon and Other Celestial Bodies, UN doc A/RES/34/68, resolution 38/68 of December 1979], currently maintained and promulgated by the Committee on Space Research [COSPAR Planetary Protection Panel, Planetary Protection Policy accepted by the COSPAR Council and Bureau, 20 October 2002, amended 24 March 2005, http://www.cosparhq.org/scistr/PPPolicy.htm], missions exploring the Solar system must meet planetary protection requirements. Planetary protection aims to protect celestial bodies from terrestrial contamination and to protect the Earth environment from potential biological contamination carried by returned samples or space systems that have been in contact with an extraterrestrial environment. From an exobiology perspective, Mars is one of the major targets, and several missions are currently in operation, in transit, or scheduled for its exploration. Some of them include payloads dedicated to the detection of life or traces of life. The next step, over the coming years, will be to return samples from Mars to Earth, with a view to increasing our knowledge in preparation for the first manned mission that is likely to take place within the next few decades. Robotic missions to Mars shall meet planetary protection specifications, currently well documented, and planetary protection programs are implemented in a very reliable manner given that experience in the field spans some 40 years. With regards to sample return missions, a set of stringent requirements has been approved by COSPAR [COSPAR Planetary Protection Panel, Planetary Protection Policy accepted by the COSPAR Council and Bureau, 20 October 2002, amended 24 March 2005, http://www.cosparhq.org/scistr/PPPolicy.htm], and technical challenges must now be overcome in order to preserve the Earth’s biosphere from any eventual contamination risk. In addition to the human dimension of the mission, sending astronauts to Mars will entail meeting all these constraints. Astronauts present huge sources of contamination for Mars and are also potential carriers of biohazardous material on their return to Earth. If they were to have the misfortune of being contaminated, they themselves would become a biohazard, and, as a consequence, in addition to the technical constraints, human and ethical considerations must also be taken into account.