共查询到17条相似文献,搜索用时 281 毫秒
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一种轴对称变几何进气道设计方法 总被引:4,自引:2,他引:2
对带凹腔的圆锥流动进行了数值分析,就流场结构和总压分布与实验结果进行了比较,数值模拟结果与实验数据吻合较好,结果可信.数值模拟研究了不同几何构型的凹腔对圆锥流动的影响,分析并揭示了凹腔与圆锥流场的耦合流动特征.据此,对一种圆锥头部可移动的轴对称变几何进气道开展了方案设计及气动性能分析,并与相应定几何进气道进行了对比.结果表明:当来流马赫数高于设计马赫数时,后退圆锥头部可以调节进气道外压缩波系,保证流量系数达到0.99以上,采用该变几何技术,在不改变进气道内通道几何形状的前体下,可明显提高进气道的流量系数. 相似文献
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F. Simões M. Rycroft N. Renno Y. Yair K. L. Aplin Y. Takahashi 《Space Science Reviews》2008,137(1-4):455-471
The propagation of extremely low frequency (ELF, 3 Hz to 3 kHz) radio waves and resonant phenomena in the spherical Earth-ionosphere cavity has been studied for almost fifty years. When such a cavity is excited by naturally occurring broadband electromagnetic radiation, resonances can develop if the equatorial circumference is approximately equal to an integral number of wavelengths of the propagating electromagnetic waves; these are termed Schumann resonances. They provide information not only about thunderstorm and lightning activity on the Earth, and their relation to climate, but also on the properties of the low ionosphere. Similar investigations can be performed for any other planet or satellite, provided that it has an ionosphere. There are important differences between the Earth and other celestial bodies regarding, for example, the surface conductivity, the atmospheric conductivity profile, the geometry of the ionospheric cavity, and the sources of excitation. To a first approximation, the size of the cavity defines the fundamental resonant frequency, the atmospheric electron density profile controls the wave attenuation, the nature of the sources influences the electromagnetic field distribution in the cavity, and the body surface conductivity indicates to what extent the subsurface can be explored. The frequencies and attenuation rates of the principal eigenmodes depend upon the electrical properties of the cavity. Instruments that monitor the electromagnetic environment in the ELF range on the surface, on balloons, or on descent probes provide unique information on the cavity. In this paper, we present Schumann resonance models for selected inner planets, some gaseous giant planets and a few of their satellites. We review the crucial parameters of ELF electromagnetic waves in their atmospheric cavities, namely the electric and magnetic field spectra, their eigenfrequencies, and the associated Q-factors (damping factors). Then we present important information on theoretical developments, on a general model that uses the finite element method and on the parameterization of the cavity. Next we show the distinctiveness of each planetary environment, and discuss how ELF radio wave propagation can contribute to an assessment of the major characteristics of those planetary environments. 相似文献
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射线追踪法在球面收敛调节片喷管RCS计算中的应用 总被引:1,自引:0,他引:1
结合射线追踪法的原理,利用自主开发的电磁散射特性计算程序,对具有不同尾缘修型的球面收敛调节片喷管进行了数值模拟计算,分别得到了不同喷管内部腔体散射场和喷管出口边缘绕射场的雷达散射截面积(RCS),并且通过计算获得了不同入射方位角上喷管腔体内壁面上的感应电流,通过对感应电流的分析,从本质上解释了RCS的变化规律.研究结果表明:对喷管出口尾缘所采用的修型措施在降低喷管出口边缘绕射场的RCS和改善喷管电磁隐身性能方面效果显著;相对于普通的遮挡算法,射线追踪法将计算周期缩短了21%以上,明显地提高了计算效率;利用感应电流的分析方法能够清晰直观地从本质上解释RCS的变化规律,并且具有较高的可靠性. 相似文献
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电磁学中麦克斯韦方程组和流体力学中无粘流动欧拉方程一样,都是具有实特征值的双曲型偏微分方程组,相同的数学特性使得计算流体力学(CFD)技术能够在计算电磁学(CEM)中得以应用。采用MUSCL格式结合Steger-Warming分裂计算电磁通量,采用4阶Runge-Kutta法计算非定常时间推进,借鉴CFD方法计算电磁场边界条件;采用时域有限体积法(FVTD)数值模拟宽带脉冲波、完全导电体、含吸波材料涂层介质/金属混合体以及复杂外形目标的电磁散射。结果表明:基于CFD的FVTD方法能够高精度地计算目标的电磁特性。 相似文献
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翼剖面介质构形的隐身缩比模型数值计算研究 总被引:1,自引:0,他引:1
结构型吸波材料以全角度、多方位的有效性和不改变飞行器原有形状设计的特点,在隐身技术领域占有重要的技术地位,开展全尺度结构的隐身效能与其技术参数影响作用的研究需要较大的测试空间与经费支持,由此限制了试验技术在更大范围内的应用。结合试验技术与参数研究的应用需求,探讨缩比介质体电磁散射规律可提供于大型结构隐身技术的计算与试验应用研究参考。采用复杂介质体的二维电磁散射有限元数值计算方法,对介质体机翼剖面的缩比模型电磁散射规律进行了数值计算研究,发现若介质体阻抗比大于0.5,则缩比模型的雷达散射截面(RCS)试验结论不能按照导体修正原理还原,必须修正才能作为原构形介质体的电磁散射特性,这对于大型结构体小型化隐身技术测试具有实用价值与意义。 相似文献