共查询到16条相似文献,搜索用时 92 毫秒
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在反射面尺寸一定的情况下,优化设计了 TEM喇叭馈源与共面馈源脉冲辐射天线,并对比了两种天线的辐射性能。分析了反射面型脉冲辐射天线的工作机理,通过准静态近似,分别得到了两种天线的远区辐射场解析解。通过理论求解,得到了两种馈源在反射面口径造成的场分布,为天线结构设计提供参考。通过分析不同脉冲宽度时两种天线的辐射情况,比较了这两种馈源性能的优劣。完成了上述两种GW级高功率高效率馈源的研制,并开展了对比实验,实验结果与理论分析相吻合。 相似文献
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对高功率超宽带脉冲辐射实验装置的理论分析、工程设计及实验等分别进行了介绍。高功率超宽带脉冲辐射实验装置主要由脉冲充电电源、超宽带脉冲产生装置及超宽带脉冲发射天线三部分组成。脉冲充电电源为脉冲产生装置提供充足的前级能源;超宽带脉冲产生装置包括高压储能电容、高压开关、充电电感、低阻脉冲形成线、亚纳秒开关和高功率负载等部分;超宽带脉冲发射天线包括阻抗变换、传输线、同轴到平板过渡段、TEM喇叭馈源、透镜及密封腔、4.5m抛物面等部分。 相似文献
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设计了一种椭圆形柱面透镜天线阵列。为改善天线的辐射性能,考虑到高功率应用中的高压击穿问题,提出在横截面为椭圆形组合矩形的天线罩内填充变压器油的方法,并将三元刀型天线阵列密封其内,形成介质透镜天线阵。利用椭圆的几何聚焦能力和介质的缩波效应,提高天线阵列的主瓣增益,并增加天线阵列的电尺寸。通过调整天线阵列的单元间距,相较于不加透镜的阵列结构,该结构的轴向远场电压峰峰值增加41%,远场辐射波束宽度变窄,前后比也得到改善,且增益提高了4.96 dB,功率容量提高338倍,达9.63 GW。 相似文献
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设计了一种椭圆形柱面透镜天线阵列。为改善天线的辐射性能,考虑到高功率应用中的高压击穿问题,提出在横截面为椭圆形组合矩形的天线罩内填充变压器油的方法,并将三元刀型天线阵列密封其内,形成介质透镜天线阵。利用椭圆的几何聚焦能力和介质的缩波效应,提高天线阵列的主瓣增益,并增加天线阵列的电尺寸。通过调整天线阵列的单元间距,相较于不加透镜的阵列结构,该结构的轴向远场电压峰峰值增加41%,远场辐射波束宽度变窄,前后比也得到改善,且增益提高了4.96 dB,功率容量提高338倍,达9.63 GW。 相似文献
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V. V. Alexandrov E. V. Grabovsky M. V. Zurin I. V. Krasovsky K. N. Mitrofanov S. L. Nedoseev G. M. Oleinik I. Yu. Porofeev A. A. Samokhin P. V. Sasorov V. P. Smirnov M. V. Fedulov I. N. Frolov 《Journal of Experimental and Theoretical Physics》2004,99(6):1150-1172
A qualitative model of the dynamics of a multiterawatt radiating Z-pinch with cold start and high rate of current rise is proposed. The model is used to analyze discharges with currents I ~ 2–5 MA (with dI/dt > 1013 A/s) through uniform or structured plasma-producing loads, including wire arrays. The most important consequence of cold start is that spatially nonuniform plasma production is prolonged to almost the entire current rise time. Under these conditions, the Ampére force begins to play a dominant role in the plasma dynamics before the plasma-producing load is completely transformed into an accelerated plasma. The results of computations of wire-array vaporization are presented. A formula is proposed for estimating the highest attainable velocity of plasma flow into a heterogeneous liner driven by the Ampére force. It is shown that local imbalance between radial motion of the produced plasma and supply of the plasma-producing substance to be ionized leads to axially nonuniform breakthrough of magnetic flux into the liner, which precedes plasma collapse. The magnetic-flux breakthrough gives rise to a chaotic azimuthal-axial plasma structure consisting of radial plasma jets of relatively small diameter, which is called a radial plasma rainstorm. The breaking-through azimuthal magnetic flux obstructs further current flow in the breakthrough region. Analyses of Z-pinch implosion based on the theory of Rayleigh-Taylor instability or the snowplow model are incorrect under the plasma-rainstorm conditions. The processes taking place in a stagnant Z-pinch include conversion of the energy carried by the current-generated magnetic field into turbulent MHD flow of the ion component of the plasma, its convective mixing with magnetic field, heating, energy transfer from ions to electrons, and emission from the plasma. Under typical experimental conditions, emission plays a key role in the energy balance in an imploding pinch. Z-pinch is modeled by an electric-circuit component that has a time-dependent nonlinear impedance and consumes the magnetic energy supplied by a generator through a magnetically insulated transmission line (MITL). The peak power reached in the circuit is comparable to the peak soft X-ray power output emitted by the pinch in terms of magnitude and timing. Optimum matching conditions are formulated for the generator-MITL-pinch circuit. 相似文献