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FY-4闪电成像仪实时事件处理器(RTEP)的FPGA设计研究 总被引:1,自引:0,他引:1
闪电是中尺度,特别是中-γ尺度天气系统研究的有力工具。闪电成像仪主要利用4种方法组合来实现闪电信号的增强与探测。这4种方法是:光谱滤波、空间滤波、时间滤波、帧一帧背景去除。实时事件处理器(RTEP)是实现帧一帧背景去除的最为有效的手段,它是提取闪电信号的重要途径。实时事件处理器是一个实时数字信号处理系统,在2ms的时间内要完成12bit量化的512x512个像素的信号数据处理,探测出闪电信号。文章论述了实时事件处理器RTEP的必要性,实现原理,以及FPGA实现方案。 相似文献
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S.A. Haider Jayesh P. Pabari J. Masoom Siddhi Y. Shah 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(7):2260-2266
We have solved the Maxwellian equations of electromagnetic waves which oscillate within the cavity formed in the lower ionosphere of Mars between 0 and 70?km. The electrical conductivity and Schumann Resonance (SR) frequencies are calculated in the lower ionosphere of Mars, in the presence of a major dust storm that occurred in Martian Year (MY) 25 at low latitude region (25°–35°S). It is found that the atmospheric conductivity reduced by one to two orders of magnitude in the presence of a dust storm. It represents a small dust layer at about 25–30?km altitudes where lightning can occur. We also found that the SR frequencies peak at?~18?km with values 19.9, 34.5 and 48.8?Hz for the modes l?=?1, 2 and 3, respectively, in the non-homogeneous medium. Our results indicate that practical or measurable values of SR are dependent on the altitudes. 相似文献
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Caitano Luiz da Silva Fernanda T. São Sabbas 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
We present the results of a streamer-fluid model used to investigate the electrodynamical coupling between the troposphere and upper atmosphere due to the penetration of lightning electric fields into the mesosphere and the lower ionosphere, generating sprites. The model solves the continuity equation for electrons and ions coupled to Poisson equation. The dominant physical response of the atmosphere is the formation of a screening-ionization wave. The wave shields the atmosphere above it from the action of the lightning field and, together with the conductivity reduction below it due to attachment, the wave amplifies the total field below it, allowing for the penetration of intense electric fields in the mesosphere as it propagates downwards into regions of higher density that compress the wave. This is the key physical mechanism for sprite inception. We evaluated the effects of the thundercloud charge geometry, lightning current waveshape, atmospheric conductivity, via different electron density profiles, and the effect of ionization, attachment and electron mobility coefficients in the electrical breakdown process, related to halo production, and sprite streamer initiation. The results showed that electrons with higher mobility are more efficient in shielding the lightning electric field before breakdown, causing delay, and they contribute to the formation of the streamer seed after breakdown, anticipating the sprite streamer inception. Similarly, a higher effective ionization rate, produced by modifications in the attachment and ionization coefficients, anticipates sprite inception. The simulations with 6 different electron density profiles, and therefore conductivities, spanning 4 orders of magnitude, showed that the altitude of breakdown and sprite initiation, as well as their time delays from the lightning discharge are directly related to atmospheric conductivity: higher conductivities produce halo and sprite inception at lower altitudes with longer delays and may hinder sprite formation. We document that variations of 30 times in the lightning current leads to sprite initiation altitudes in the range 66.0–73.5 km, with delays between 1.550 and 34.500 ms, while variations of 4 orders of magnitude in the conductivity profile lead to initiation altitudes 61.0–70.6 km, with delays in the range 3.825–9.825 ms. Consequently, we suggest that lightning characteristics dominate over atmospheric parameters in determining sprites’ initiation altitude and delay. The simulation of a −CG, with a constant current of 30 kA, did not produce a sprite seed, confirming an asymmetry in the response of the atmosphere to positive and negative lightning. This is due to the free electron drift direction that is away from the screening ionization wave, preventing the formation of the streamer seed for the great majority of −CGs. The same does not apply to halos, which depend on the occurrence of breakdown and can be produced by discharges of both polarities. 相似文献
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周小春 《民用飞机设计与研究》2015,(2):6
讨论闪电间接效应和高强度辐射场的飞机传递函数的同步测量与分析计算,论述飞机系统设备对闪电间接效应或高强度辐射场响应的分析预测方法,说明系统定义中电磁兼容及设备电磁防护的设计方法。 相似文献
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《中国航空学报》2020,33(4):1242-1251
Lightning strike is a complicated process involving multi-field coupling. In order to investigate the thermal damage mechanism of carbon fiber reinforced composites subject to lightning swept stroke, a complete numerical method is presented. Numerical model of lightning discharge is established based on Magneto Hydro Dynamics (MHD) and calculated by FLUENT secondary development technology. Considering aerodynamic flow effect, channel formation and evolution process during lightning discharge is analyzed for lightning current waveform A. Thermal-electric Coupling model is presented according to Radial Basis Function (RBF) interpolation theory, which is implemented by compiling program to make lightning current and heat energy inject into composite laminate. Consequently, damage mechanism of composite laminate under lightning swept stroke is studied based on the coupled numerical model and element deletion method. Ablation damage morphology of composite laminate is analyzed to understand plasma expansion and reattachment in arc root. The results show that aerodynamic flow makes the lightning channel move fast and composite laminate is deteriorated due to thermal damage. 相似文献
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概述了闪电间接效应定义,飞机级闪电间接效应(IEL)防护试验的必要性,分析了IEL耦合机理,并对飞机级IEL防护试验方法进行了初步介绍。 相似文献