预移相型恒温热线(膜)流速计的动态响应方程

分析传统恒温热线热膜流速计(简称 HWFA)动态方程后,提出了一种新型HWFA 线路模型——主电桥预移相模型,推导出真实条件下小扰动动态响应方程,并按此原理设计制造了崭新的高性能 IFV—900型 HWFA 样机。该机全部革除了传统HWFA 的三个调节参量,大大地简化了调节步骤;不自激振荡的范围明显增宽,极大地减少了使用上的麻烦;频带宽度比当今世界流行的 HWFA 增宽了2～5倍;加上一系列智能化功能后使自动化程度达到了新的高度。这一新型 HWFA 的问世将可能导至 HWFA技术的重大改进和新的变革。首先阐明主电桥预移相模型的提出和真实条件下小扰动动态响应方程的推导。随后将用若干姐妹篇阐明动态方程频率响应调节元物理值的解析解,频率特性实验分析手段的电扰动试验响应情况的理论分析等内容。     

屋面现浇板裂缝的防治

从设计、施工、材料、气候等多方面分析现浇板裂缝产生的原因,并总结一些防治措施。     

低温热水分户计量采暖系统共用立管水力平衡分析

本文分析了重力作用压头对低温热水计量采暖系统共用立管形式的影响,通过运用基尔霍夫定律分析了下分异程式双管系统和下分同程式双管系统的水力平衡状况,得出了下分异程式双管系统更适用于低温热水采暖系统的结论,并确定了立管经济比摩阻的范围和下分异程式双管可以负担的楼层数。     

燃气推力矢量控制发动机内流场数值模拟

采用基于Favre平均的三维N-S方程,对燃气推力矢量控制发动机全内流场进行了数值仿真,研究了燃气引流、燃气二次喷射及与发动机内主流相互作用等复杂流动。研究结果表明,流场内包含复杂的涡系结构和波系结构,还存在着边界层与激波的相互干扰、自由剪切层、激波、膨胀波和大尺寸分离。通过数值模拟,对试验中的异常现象进行了定性分析,得出了与试验一致的结论。     

高强度铝合金中氢传输的研究

采用化学镀镍层作为铝合金LC4上防护层,应用电化学氢渗透技术研究了氢在LC4中的静态传输规律以及在不同热处理状态下,氢在LC4中的传输对其应力腐蚀敏感性的影响。实验结果表明:常温下氢在LC4中的静态传输是以扩散为控制步骤的过程。氢扩散系数为10~(-9)cm~2·s~(-1)数量级,为同条件下氢在纯铝中扩散系数的四分之一;LC4材料的DCB试样在常温下的3.5％NaCl溶液中的应力腐蚀断裂不遵循氢脆机理。     

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.     

航空航天结构复合材料湿热老化机理的研究

通过研究T300／5405和T300／NT9200复合材料以及基体树脂5405和NY9200的浇注料在80℃水浸中的吸水动力学，红外光谱，动态力学性能和表达形态的变化，分析了复合材料的湿热老化机理，结果表明：在80℃水浸的加速湿热老化条件下，两种复合材料的老化机理主要是吸入水分对基体的塑化／溶胀作用以及因树脂与纤维湿膨胀的不匹配所产生的内应力引起的微观开裂。     

用慢拉伸法研究GC-4超高强度钢的应力腐蚀开裂敏感性

 本文采用慢拉伸试验法研究了GC-4超高强度钢（40CrMnSiMoVA）的应力腐蚀开裂敏感性。结果表明,三种热处理的GC-4钢在典型模拟环境3％NaCl溶液和蒸馏水中都对应力腐蚀开裂敏感。环境介质的存在使该钢的抗拉强度、总应变和断裂能大大降低,而且,阴极极化和阳极极化都使其应力腐蚀开裂敏感性显著提高。分析表明,氢脆和阳极溶解都是导致GC-4钢应力腐蚀开裂的重要原因。     

机械合金化＋热压制备Laves相NbCr2合金及其组织性能研究

采用机械合金化 热压工艺路线来制备化学配比成分的单相Laves相NbCr2合金.研究了Cr,Nb元素粉经20h球磨后在1200℃,1250℃和1300℃不同时间热压所获得的Laves相NbCr2合金的组织和性能.结果表明:1250℃×0.5h热压获得的Laves相NbCr2合金组织均匀,晶粒尺寸达到微/纳米级,致密度达到97.1%,室温断裂韧性高于5.07MPa·m1/2.与熔铸工艺制备的单相Laves相NbCr2合金的断裂韧性1.50MPa·m1/2相比,所制备的单相Laves相NbCr2合金的室温断裂韧性大大提高,充分实现了细晶韧化的效果.     

高温富油燃气作引导火焰的煤油超燃研究

对采用高温富油燃气作引导火焰的煤油超声速燃烧进行了研究。根据试验测得的壁面静压分布，采用一维简化模型处理与分析数据，得出了不同试验条件下的燃烧效率与总压恢复系数；对超声速燃烧室内的静压分布特点作出了分析；对超声速燃烧室人口处的气流总温，燃料喷射位置，以及燃烧总体当时比对燃烧室内静压分布、燃烧效率与总压恢复系数的影响进行了讨论。