关于厚薄板弯曲分析的内位移杂交元法

 本文通过引入单元内位移和优化处理的单元应力场,以计入剪切变形的板弯曲能量泛函为基础,导出适用于厚、薄板分析的四边形杂交应力元。内力场和内位移的合理选择避免了单元零能模式的出现、避免了解的剪切自锁现象。该优化单元显示了较好的通用性和收敛性。对关于剪切自锁的RCI判据提出了反例、说明了它的局限性。     

环氧基复合材料的混合模式分层

 采用混合模式弯曲试验研究了Ｔ３００／Ｍ１０和ＨＴＡ／６３７６两种复合材料静态和疲劳加载的分层断裂行为。在不同α／Ｌ比和混合模式比条件下加载,两种材料呈现脆性不稳定或脆性稳定的裂纹扩展。在疲劳加载中,裂纹扩展始终是稳定的。混合模式比对分层韧性、疲劳裂纹扩展速率和疲劳门槛值均有明显影响。     

氢燃料的特性与应用前景

本文论述了氢作为动力燃料的特性,介绍了氢能利用技术方面的概况。讨论了由烃燃料向氢燃料过渡的几种方式,目前氢燃料存在的问题以及氢能的应用前景。     

高能氧化剂二硝酰胺铵的热分解研究

为深入了解二硝酰胺铵(ADN)的热分解，为该氧化剂在推进剂中应用提供必要的技术保障和实验依据，采用热重分析法(TG)及差示扫描量热法(DSC)，实验研究了氮气流量、合成中间体烷基羰基N-硝酰胺铵(AUN)及硝酸铵(AN)对ADN热分解过程的影响，并利用model-free isoconversional方法模ADN热分解过程的活化能曲线。结果表明：氮气流量和硝酸铵(AN)对ADN的热分解过程有显著影响，而AUN可使ADN热分解曲线产生肩峰，但基本不影响ADN的热分解过程。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

一种新的空间飞行器再入制导律研究

基于阻力与能量关系的优化剖面,以该再入剖面作为基准轨迹,给出了跟踪这一基准轨迹的空间飞行器再入制导律与控制律,将基准轨迹转化为相应的迎角剖面和滚转角剖面,设计了相应的结构配置。仿真结果表明,基于阻力与能量关系剖面设计的制导律满足了各项约束条件,并能成功地控制飞行器到达所要求的位置。     

粒子云侵蚀问题实验研究中动能通量模拟的意义

本文首先将粒子云侵蚀条件下的驻点表面后退分解为无粒子烧蚀部分、粒子云引起的烧蚀增量部分和粒子撞击物面引起的直接侵蚀部分。然后研究了表面能量平衡关系,给出了粒子云引起的烧蚀增量表达式。最后分三类讨论粒子与飞行器的碰撞:(1)完全弹性碰撞(不符合实际);(2)完全非弹性碰撞;(3)部分弹性碰撞。对于后两种碰撞,本文分析了动能通量模拟适用的条件。     

含非对称裂纹三维有限大体应力强度因子能量释放率方法的封闭解

 本文提出一种新的半工程半解析的方法,导出含非对称裂纹三维有限大体应力强度因子的封闭解。根据此方法,只需少量的机时,即可获得一系列结果。本方法及所得结果在工程上有实际应用价值。     

复合固体推进剂的高能化

本文评述了国外固体推进剂近年来向高能化方向发展的三个主要动向:HTPB推进剂的高固体及硝胺化;丁羟之后的新品种——NEPE推进剂;Be、B、叠氮化物等高能组分的研究等.对我国固体推进剂的发展方向提出了建议.     

先进的变载吸能器

传统的定载吸能器以50百分位男性乘员满足95％生存率为条件设计，它不能为全体乘员提供保护，变载吸能器能够根据乘员重量而调节动作载荷，为全体乘员提供最合理的保护，同时可以大大降低吸能器的冲击行程。