CBERS-1卫星IRMSS数据在冀中地区应用评价研究

通过冀中保定—廊坊地区典型研究中采用的CBERS_1卫星IRMSS数据 ,对数据图像的质量、图像信息的处理方法和专业应用潜力进行评价。通过快速评价 ,以评估IRMSS不同波段数据的应用效果 ,加速IRMSS数据的推广应用。     

双星定位法与北斗1号卫星导航系统

简要介绍了基于双星定位法的北斗 1号卫星导航系统的原理。     

民用飞机最小风险炸弹位置适航符合性验证方法研究

民用飞机最小风险炸弹位置(LRBL)是航空运营面对炸弹爆炸恐怖袭击的最后一道安全屏障,对民用飞机的安全性有重要意义。针对国内民用飞机LRBL工作缺乏适航符合性验证方法研究的现状,以AC25.795 6为指导,以满足FAR 25.795(c)(1)中有关LRBL的适航要求为目标,首次对LRBL的适航符合性验证方法进行研究;通过该工作,一方面明确了LRBL周围设备的系统安全性适航符合性验证方法,增强LRBL相关系统安全性分析工作在型号设计中的可操作性;另一方面,通过开展爆炸物在LRBL发生爆炸对飞机结构的安全性影响分析,得出了LRBL周围结构设计的适航符合性验证方法。该研究建立了面向FAR25.795(c)(1)的LRBL适航符合性验证体系,为提高产品的安全性和适航性提供了更为详实、可操作的设计方法。     

VARIABLE STRUCTURE MODEL－FOLLOWING ADAPTIVE CONTROL DESIGN FOR ROBOT MANIPULATORS

ＶＡＲＩＡＢＬＥＳＴＲＵＣＴＵＲＥＭＯＤＥＬ－ＦＯＬＬＯＷＩＮＧＡＤＡＰＴＩＶＥＣＯＮＴＲＯＬＤＥＳＩＧＮＦＯＲＲＯＢＯＴＭＡＮＩＰＵＬＡＴＯＲＳＺｈａｏＤｏｎｇｂｉａｏ；ＺｈｕＪｉａｎｙｉｎｇ（ＤｅｐａｒｔｍｅｎｔｏｆＭｅｃｈａｎｉｃａｌＥｎｇｉｎ...     

复合氧化物LaM1—xNixO3（M=Fe,Ni）的晶体结构及电性的研究

采用柠檬酸络合法、固相反应法分别制备ＬａＦｅ１ｘＮｉｘＯ３和ＬａＭｎ１ｘＮｉｘＯ３。用差热分析法、Ｘ射线法、四探针电阻测量法对化合物的晶体结构、电性进行研究。结果表明：ｘ〈０．５时化合物为单相的钙钛矿结构，ＬａＦｅ１ｘＮｉｘＯ３的导电性比ＬａＭｎ１ｘＮｉｘＯ３差，导电通道为－（Ｍ、Ｎｉ）－０－；ｘ≥０．５时化合物为畸变的钙钛矿结构，两者的电性相近，通道为－（０－Ｎｉ－）－。     

大扩张通道超音高载荷对转涡轮动叶三维设计方法研究

 为设计一种SRR结构具有大扩张通道的超音高载荷对转涡轮高压动叶，论文提出了一种更符合三维真实流动状态的S1流面三维造型法，详细阐述了三维造型方法基本原理，并用之设计了一个出口马赫数1.33，通道扩张角37.3°的超音高载荷对转涡轮动叶。三维数值模拟结果显示对转涡轮动叶流场参数分布合理，没有出现分离，滞止效率达到92.57%。实例表明三维造型法由于充分考虑涡轮流场三维性，对于通道扩张度大，流线曲率变化剧烈的涡轮叶片，比传统二维柱面造型法更精确、更实效。     

MIDAS – The Micro-Imaging Dust Analysis System for the Rosetta Mission

The International Rosetta Mission is set for a rendezvous with Comet 67 P/Churyumov-Gerasimenko in 2014. On its 10 year journey to the comet, the spacecraft will also perform a fly-by of the two asteroids Stein and Lutetia in 2008 and 2010, respectively. The mission goal is to study the origin of comets, the relationship between cometary and interstellar material and its implications with regard to the origin of the Solar System. Measurements will be performed that shed light into the development of cometary activity and the processes in the surface layer of the nucleus and the inner coma. The Micro-Imaging Dust Analysis System (MIDAS) instrument is an essential element of Rosetta’s scientific payload. It will provide 3D images and statistical parameters of pristine cometary particles in the nm-μm range from Comet 67P/Churyumov-Gerasimenko. According to cometary dust models and experience gained from the Giotto and Vega missions to 1P/Halley, there appears to be an abundance of particles in this size range, which also covers the building blocks of pristine interplanetary dust particles. The dust collector of MIDAS will point at the comet and collect particles drifting outwards from the nucleus surface. MIDAS is based on an Atomic Force Microscope (AFM), a type of scanning microprobe able to image small structures in 3D. AFM images provide morphological and statistical information on the dust population, including texture, shape, size and flux. Although the AFM uses proven laboratory technology, MIDAS is its first such application in space. This paper describes the scientific objectives and background, the technical implementation and the capabilities of MIDAS as they stand after the commissioning of the flight instrument, and the implications for cometary measurements.     

氪气和氙气中四氟化碳杂质分析

介绍了CF4定性定量分析方法,探讨了CF4的来源及清除.     

Deep Impact: The Anticipated Flight Data

A comprehensive observational sequence using the Deep Impact (DI) spacecraft instruments (consisting of cameras with two different focal lengths and an infrared spectrometer) will yield data that will permit characterization of the nucleus and coma of comet Tempel 1, both before and after impact by the DI Impactor. Within the constraints of the mission system, the planned data return has been optimized. A subset of the most valuable data is planned for return in near-real time to ensure that the DI mission success criteria will be met even if the spacecraft should not survive the comet’s closest approach. The remaining prime science data will be played back during the first day after the closest approach. The flight data set will include approach observations spanning the 60 days prior to encounter, pre-impact data to characterize the comet at high resolution just prior to impact, photos from the Impactor as it plunges toward the nucleus surface (including resolutions exceeding 1 m), sub-second time sampling of the impact event itself from the Flyby spacecraft, monitoring of the crater formation process and ejecta outflow for over 10 min after impact, observations of the interior of the fully formed crater at spatial resolutions down to a few meters, and high-phase lookback observations of the nucleus and coma for 60 h after closest approach. An inflight calibration data set to accurately characterize the instruments’ performance is also planned. A ground data processing pipeline is under development at Cornell University that will efficiently convert the raw flight data files into calibrated images and spectral maps as well as produce validated archival data sets for delivery to NASA’s Planetary Data System within 6 months after the Earth receipt for use by researchers world-wide.     

电离层峰下结构的数值模拟

在考虑由扩散与中性风引起的动力学输运与有原子离子Ｏ＾＋（＾４Ｓ），Ｏ＾＋（＾２Ｄ）与Ｏ＾＋（＾２Ｐ）以及分子离子Ｏ２＾＋，ＮＯ＾＋，Ｎ２＾＋参加光化学反应的电离层－热层体系中，提出一个一维时变的电离层剖面数值模型，通过数值计算着重讨论了武昌地区Ｆ２层峰以下，尤其是Ｅ／Ｆ与Ｆ１／Ｆ２谷区的电离层形态与有关过程，得到如下结论：（１）对于原子离子，单一成分Ｏ＾＋（＾４Ｓ）的光化学反应与输运，也有助于形成