镉镍电池在武器回收系统中的应用探讨

文章对镉镍电池在武器回收系统中的应用进行了探讨 ,得到了在武器回收系统中可以用镉镍充电电池取代银锌蓄电池的结论     

翼柱型装药发动机点火升压过程计算

利用实验获得的翼槽内火焰传播规律经验公式,在Ｐ（ｔ）模型的基础上,建立了翼柱型发动机的点火升压计算模型。计算结果与实测数据吻合较好。同时就点火器流量、推进剂燃速、喷管堵盖打开压强等设计参数对发动机点火升压过程的影响进行了分析。     

固体火箭发动机点火药量的计算

通过对点火过程及数学模型的描述，以气体状态方程计算点火药量的公式为基础，提出了一个新的点火药量计算经验公式，并讨论了公式的应用情况和使用范围。     

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.     

隐身外形飞行器用埋入式进气道的设计与风洞实验研究

本文为隐身外形飞行器用埋入式进气道发展了一套设计方法。该方法的理论基础是埋入式进气道进气机理和气动S弯概念,其关键技术包含通道中心线设计、横截面面积变化规律设计以及横截面形状设计等,各技术可以方便地用数学方法加以描述,整个方法易于编程实现。并结合一种隐身外形无人机提出了埋入式进气道方案,通过实验得到了此类隐身外形飞行器用埋入式进气道的气动特性。结果表明,所提出的埋入式进气道方案可行,所设计的模型进气道性能良好,所发展的设计方法合理。同时验证了埋入式进气道进气机理的正确性,也表明隐身外形飞行器与埋入式进气道的组合方案具有十分光明的应用前景。     

一种高亚音速弹用S弯进气道设计及其特性

针对导弹进气道的结构特点，在前人的工作基础上总结出一种适合导弹使用的大偏距、短扩压S弯进气道的设计方法。该方法通过变更中心线、面积规律、唇口形状和喉道位置等参数完成进气道的设计。应用本文中使用的S弯进气道的数学描述方法，可以方便地完成S弯进气道的几何造型工作，实现此类导弹用S弯进气道的参数化设计，生成的造型数据也可以为CFD和CAM使用。此外，作为验证，文中应用此方法设计了一个椭圆进口的S弯进气道，并进行了模型的风洞实验。实验结果表明，使用本文方法设计的弹用S弯进气道可以达到较好的气动性能，能够满足应用需要。     

APPLICATION OF HOT-PRESS SINTERING TECHNIQUE TO EXPLOSIVE CHARGE LINER OF PETROLEUM PERFORATION BULLET

介绍了一种制备石油射孔弹的药形罩的新方法，采用粉末冶金技术，热压烧结工艺制备石油射孔弹的药形罩，并对药形罩的烧结工艺进行了研究。实验结果表明，采用该工艺制备的石油射孔弹药形罩可以满足要求。     

扩展型面排孔气膜冷却的实验研究

本文设计了三种型面的气膜孔扩展结构，研究了气膜冷却效率、壁面换热系数及流量系数随吹风比的变化规律。研究结果表明，与典型的圆柱形气膜孔相比，有后向扩展型面的气膜孔具有相对较高的冷却效率和换热系数，流量系数略有降低。扩展型面的流向扩展角α对冷却效率和换热系数的影响大于侧向扩展角 的影响。侧向扩展角 只在特定吹风比下才对提高气膜的侧向覆盖率、进而提高气膜冷却效率起作用，它使得位于二次流出流下游的低压区域范围增大，流量系数减小。     

Investigations into sensing characteristics of circular thin-plate electrostatic sensors for gas path monitoring

Circular thin-plate electrostatic sensors are promising in gas path monitoring due to their advantages of non-intrusiveness and easy installation. The spatial sensitivity and filtering effect are two important performance parameters. In this paper, an analytically mathematical model of induced charge on a circular thin-plate electrode is first derived. Then the spatial sensitivity and filtering effect of the circular electrostatic sensor are investigated by numerical calculations. Finally,experimental studies are performed to testify the theoretical results. Both theoretical and experimental results demonstrate that circular thin-plate electrostatic sensors act as a low-pass filter in the spatial frequency domain, and both the spatial filtering effect and the temporal frequency response characteristics depend strongly on the spatial position and velocity of the charged particle. These conclusions can provide guidelines for the optimal design of circular thin-plate electrostatic sensors.     

环型与线型聚能装药射流成型机理对比

环型聚能装药药型罩2侧在挤压汇聚形成射流过程中存在不对称性,不能完全套用线型聚能装药射流成型的现有理论。利用DYNA3D软件对相同剖面结构的环型、线型聚能装药射流成型过程进行数值模拟,通过比较分析得出了环型聚能装药形成杵体及射流参数的分布特性,为进一步理论研究及工程应用提供参考。