谈我院综合教学楼的设计

本文简明扼要地介绍了我院新建综合教学楼在有限的建筑用地范围内，为满足各项功能要求的建筑设计思路及结构上的处理方法。     

空间积分声光相关器

论述空间积分声光相关器的系统设计，给出了单器件和双器件声光信号处理器的光学系统，提出了两种新型的外差检测方法，并推志了处理器输出的数学模型，利用这两种检测方法分别对１３位巴克码ＢＰＳＫ（二进制相移键控）信号进行了相关检测，得出了与理论分析相一致的实验结果。     

复合材料叠层结构剖面翘曲修正理论

 首先假设复合材料叠层结构的面内位移沿厚度方向为直线分布,然后根据剪切变形进行连续修正,获得逐步升高的各阶翘曲位移分布函数。文中以叠层梁为例,应用最小势能原理导出其静力方程和力的边界条件。在长度方向则采用升阶谱位移函数,进行了数值计算。所得叠层梁的位移和应力分布的数值结果与精确解相比,表明本文方法有很好的收敛性。     

加入增益介质的F-P干涉仪和衍射光栅光谱仪的光谱特性对比

对加入增益介质的F—P干涉仪的光谱特性与衍射光栅光谱仪的光谱特性作了定量对比。结果表明，加入增益介质的F—P干涉仪的光谱特性要明显优于衍射光栅光谱仪的光谱特性。这为光谱精细结构分析提供了更为理想的选择。     

两种镁合金的化学处理

对AZ91D和AM50合金进行化学处理，用SEM和电化学方法来分析化学转化膜的表面形貌及在腐蚀性电解质中的稳定性。结果表明，铬酸盐处理时，AM50合金较AZ91D合金的成膜反应容易进行，成膜均匀，在3．5％NaCI水溶液中耐蚀性能好；而磷酸盐处理时，结果恰恰相反，AZ91D合金转化膜的性能优于AM50合金的膜。     

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.     

基于超纯水电解加工的水解离机理研究

介绍了一种以超纯水为电解液的电解加工工艺方法,即超纯水电解加工技术.研究了阳离子交换膜在超纯水中的水解离机理及工作特性,分析其在超纯水电解加工过程中的作用机理,并进行了水解离试验研究.结果表明：电流密度达到了3.7 A/cm^2,电场强度约为2 MV/m,已进入微细电解加工去除材料要求范围,为超纯水微细电解加工的应用奠定了基础.     

浇注温度和细化剂对K4169高温合金微观组织的影响

研究了降低浇注温度或加入细化剂后 ,K4 16 9合金晶粒细化的微观组织、夹杂及缩松等的变化。发现同样加或不加细化剂条件下 ,浇注温度越低 ,一次枝晶主轴长度和二次枝晶臂距越小。而同一浇注温度下 ,化学法细晶试样一次枝晶主轴长度较普通试样的短 ,而二者的二次枝晶臂距无明显差别。晶粒细化后 ,晶粒形态由普通铸造组织中的树枝晶向细晶组织中的粒状晶转变 ,且合金中主要元素的偏析减轻 ,这均有利于提高细晶铸件机械性能。MC型碳化物和Laves相的尺寸、数量和形貌在晶粒细化前后变化不大。铸件中加入微量细化剂不形成夹杂 ,不改变合金相组成。此外 ,加细化剂不仅可使晶粒细化 ,同时铸件中的缩松大大减少     

彩色三维激光快速成型技术的研究

目前逆向工程采用线结构激光和一个彩色面阵CCD摄像机构成三维彩色扫描系统,彩色CCD摄像机分两次对被测物体成像,首先摄取物体的彩色图片,然后加用滤光片再摄取激光光平面上的三维信息.最后将两次获取的信息重叠,便可得到三维彩色信息.提出了激光光平面方程式三维测量方法,建立了相应的数学模型.研制成一套适用于彩色逆向工程流程,并进行了实验研究,给出了实验结果.     

声光相关技术在电子战中的应用

介绍了声光相关技术原理及其在现代战争,特别是在电子战及扩频通信等方面的应用,比较了体波及其表面波、声光及声电技术在应用中的不同特点,并具体探讨了声光相关器应用子通信信号的解调及同步中的可行性,分析表明,声光相关技术是很有发展前景的一项技术,将越来越多地应用于各个不同的领域。