吸波Cf和SiCf的制备及其微波电磁特性

探讨吸波Cf和吸波SiCf的制备方法方法和微波电磁特性，降低Cf的碳化温度、改变Cf的截面形状和大小、对Cf进行表面改性以及对Cf进行掺杂改性能制备出吸波性能优良的Cf，采用高温处理，对纤维进行表面改性和掺杂异种元素可制备出吸波SiCf.     

钛合金TC11深孔钻削刀片材料的选择

在研究了钛舍金材料切削性能的基础上，针对钛合金的特点，选用了五种国内常用的硬质舍金刀片材料，对钛合金进行深孔钻削刀具磨损试验。结果表明，确定了适合钻削钛合金TC11的硬质合金刀片材料。     

固体火箭喷管排气中的粒子分布

1.前言 现代的固体火箭发动机为提高推进剂的能量特性及抑制不稳定燃烧，常常在推进剂中添加金属粉末，最常见的是加金属铝粉。在发动机工作时，铝粉燃烧形成凝聚相的氧化铝粒子。这些粒子在喷管中的流动过程中，温度、速度等方面的变化滞后于燃·气本身的变     

三维四向石英/酚醛复合材料烧蚀性能的实验研究

介绍了利用最短长度的轴对称拉伐尔喷管，在FD－04D电弧加热器上对三维四向石英／酚醛复合材料进行的驻点烧蚀试验，并利用多元线性回归分析的方法，拟和出材料的质量烧蚀率与气流总焓和驻点压力的关系式，即m1=aHs^bPs^c。在一定的范围内，利用此关系式，可以很方便地计算出这种石英／酚醛复合材料的质量烧蚀率。     

微量碳化硅纤维/环氧树脂复合吸波材料研究

研究微量碳化硅纤维／环氧树脂复合吸波材料不同排布的吸波性能。结果表明：碳化硅纤维吸波性能与纤维的排布间距和纤维含量密切相关；正交排布试样的吸波效果总体上优于平行排布试样；间距为4mm、纤维含量为1600根／束时的正交排布方式获得大于8GHz、-10dB以下的反射衰减。     

CVD过程中温度对SiC涂层沉积速率及组织结构的影响

以CH3SiCl3 H2体系在1000～1300℃沉积了SiC涂层,研究了温度对涂层沉积速率的影响,应用自发形核理论解释了不同沉积温度下CVDSiC涂层的组织结构。结果表明,随着沉积温度的提高,CVDSiC涂层的沉积速率相应增大;1000～1200℃沉积过程为化学动力学控制过程,1200～1300℃沉积过程为质量转移控制,1000℃和1100℃沉积的SiC涂层表面光滑、致密;1200℃和1300℃沉积的SiC涂层表面粗糙、多孔;随着沉积温度的提高,CVDSiC涂层的晶体结构趋于完整,当温度超过1150℃时,涂层中除β SiC外还出现了少量α SiC。     

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.     

碳化铬／Ni3Al复合材料的高温抗氧化性能

对比研究碳化铬/Ni3Al复合材料和传统高温耐磨材料Stellite 12合金在1000℃时的高温氧化行为.结果表明,Stellite 12合金表面形成以Cr2O3为主的氧化膜,并发生明显剥落;而碳化铬/Ni3Al复合材料表面形成以α-Al2O3为主的致密氧化膜,其空气中的氧化速率仅为Stellite 12合金的1/2,碳化铬具有良好的抗氧化稳定性并与Ni3Al基体有较好的氧化协同性.分析认为,碳化铬在堆焊过程中发生溶解导致部分Cr固溶于Ni3Al合金基体中,促进α-Al2O3的形成,从而改善复合材料的抗氧化性.而材料表面所形成的氧化膜类型是两种材料抗氧化性差异的主要原因.     

涂层硬质合金刀具加工镍基合金的应用

本文在对镍基合金进行系统车削实验基础上，研究了多种先进硬质合金刀片的切削性能。并对涂层硬质合金刀片独特的优良性能进行了论述。文中从抗磨料磨损、抗扩散磨损及抗氧化磨损几方面，对涂层刀具的切削机理进行了分析研究。     

基于光滑粒子流体动力学方法的液滴蒸发问题数值模拟研究

基于光滑粒子流体动力学方法（Smoothed Particle Hydrodynamics，SPH），开展了SPH新算法在蒸发燃烧领域的研究。建立了适用于SPH方法的蒸发数值模型，推导了基于傅立叶热传导公式和菲克扩散定律的SPH离散方程；借鉴VOF方法（Volume of Fluid）的思想，提出了SPH粒子的液相质量分数的概念，以有效表征蒸发过程中的相变问题。采用SPH方法对高温环境中单个液滴的蒸发过程进行数值模拟，结果符合D2定律，与理论模型相一致；在强迫对流环境中，液滴的蒸发过程受到对流作用及表面张力的影响，蒸发速率加快；进一步对双液滴在静止、对流环境中的蒸发过程进行数值模拟研究。结果表明，液滴的间距、滴径对多个液滴的蒸发过程影响至关重要，液滴间距至少在两倍的液滴直径以上，相互之间的影响才可以近似忽略。通过本文研究，拓宽了SPH方法在蒸发相变领域的应用范围，研究结果也能够为进一步的燃烧问题研究奠定基础。