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基于Solid Works和Cosmos的模具结构三维设计及有限元分析 总被引:2,自引:0,他引:2
复杂结构注塑模具的设计和强度、刚度分析是注塑行业的重要难题。利用Solid Works三维设计软件实现了注塑模具的三维实体建模,并运用COSMOS/Works软件对注塑模具的典型部件进行了有限元分析,验证设计的零件是否符合实际工作情况是实现注塑模具现代化设计的重要途径。通过GearTrax2001Plus、Toolbox等外挂、内挂插件的使用.大大地简化了建模过程,克服了原有设计方法的不足.为解决较复杂的结构设计和理论分析问题提供了一种新的途径。 相似文献
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S. M. Krimigis D. G. Mitchell D. C. Hamilton S. Livi J. Dandouras S. Jaskulek T. P. Armstrong J. D. Boldt A. F. Cheng G. Gloeckler J. R. Hayes K. C. Hsieh W.-H. Ip E. P. Keath E. Kirsch N. Krupp L. J. Lanzerotti R. Lundgren B. H. Mauk R. W. McEntire E. C. Roelof C. E. Schlemm B. E. Tossman B. Wilken D. J. Williams 《Space Science Reviews》2004,114(1-4):233-329
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. 相似文献
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以某型整体叶轮数控电解加工为例,基于UG软件平台,通过二次开发实现其加工工艺过程的模拟,验证数控轨迹,检查工件和阴极间的间隙以及判断是否发生干涉,为数控代码和阴极设计的改进提供依据,减少试验次数。 相似文献
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真实气体流动的相似规律 总被引:8,自引:0,他引:8
本文从具有化学反应的NS方程出发导出了真实气体流动的相似律,分别给出了高温空气非平衡流、平衡流和冻结流的相似参数。文中还讨论了航天飞机轨道器各种Mach数范围内的真实气体流动的相似参数和实验模拟问题。 相似文献
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逆向射流多斜孔气膜冷却的数值模拟 总被引:1,自引:0,他引:1
为了使航空燃气轮机燃烧室在高于燃烧室材料许用温度的前提下能够正常工作,需对燃烧室内壁采取冷却措施,并对变吹风比和变角度下的逆向射流多斜孔气膜冷却进行了数值模拟。在贴体坐标下划分网格,采用k-ε模型模拟湍流流动,求解气膜冷却过程的数学模型。分别改变逆向射流同主流的夹角,使其为20°、30°、45°和60,°改变吹风比的变化范围为0.5到1.5等多种条件下,对多斜孔气膜冷却效果进行了数值模拟。在所研究的范围内得到了符合规律的结论。研究结果表明,当吹风比不变的情况下,减小逆向射流角度,用有效温比表示的冷却效果相应提高。当逆向射流角度不变时,增加吹风比,冷却效果也相应提高。 相似文献
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用透射电子显微镜重点研究了Fe-10Ni-14Co钢的标准处理状态(830℃风冷+—73℃+510℃Sh)的微观组织结构。510℃回火不同时间,由于M2C的析出状态发生变化,钢也由峰时效(510℃/10min)→过时效(510℃/5h)→明显过时效转变。510℃5h合会开始发生逆转变。 相似文献