放射性物质^(137)Cs对微波大气击穿特性的影响北大核心CSCD

针对现有的放射性物质探测手段有效距离近和效率较低等局限性,考虑到高功率微波(HPM)良好的空间辐射特性,研究放射性物质对微波大气击穿特性的影响,以实现利用HPM远距离探测放射性物质的设想。阐释了微波脉冲等离子体击穿原理和自由电子对击穿特性影响,分析了放射性物质^(137)Cs射线产生自由电子的过程,在此基础上分析了HPM大气击穿时间和击穿阈值。基于HPM大气击穿等离子体实验装置,分别在6000 Pa、7000 Pa和8000 Pa的低气压环境对有、无放射源存在情形开展多次HPM辐照实验。实验结果表明:放射源的存在降低了约10%的HPM大气击穿阈值,缩短约50%的击穿时间。     

FDTD结合DFT分析宽频高功率微波大气传播

联立麦克斯韦方程与电子流体方程,用时域有限差分法(FDTD)模拟高斯型和阻尼正弦型等宽频高功率微波(HPM)的大气传播.在每个时间网格上,根据窄带脉冲的电子速度,通过离散傅立叶变换(DFT)方法求解出宽频脉冲的等效电场,将等效电场和压强代入电离参数公式,使电离参数随空间网格不断更新,提高计算准确性.结果表明,宽频HPM脉冲幅值、脉宽以及海拔高度等参数对大气击穿有明显的影响;大气击穿导致尾蚀效应;随着传播距离的增加,宽频HPM脉冲的尾部衰减加剧,脉宽缩短,引起宽频脉冲的频谱出现展宽、分裂及中心频率移动等现象.     

高功率微波在低电离层中的互作用效应分析

 高功率微波在低电离层中传输时会产生非线性效应。分析了低电离层中HPM的互作用效应，推导了HPM在低电离层中传输的互作用因子同初始场强和微波频率的关系，并对不同条件下振幅交调深度同两个脉冲的延迟时间之间的关系进行了理论研究与数值模拟。结果表明：改变脉冲的延迟时间，振幅交调深度的变化规律也随之改变；为了减少吸收衰减，低电离层中传输的HPM电波的干扰波电场初始振幅与特征等离子体电场振幅的比值应保持在10以下。     

高功率微波大气击穿的光学诊断

 介绍了一种高功率微波在波导内击穿光电诊断测量装置,测得了大气击穿的光电信号,获得了HPM击穿形成的等离子体衰减常数,对击穿点向源方向移动的猜想进行了实验验证。同时进行了短脉冲HPM在自由空间击穿实验,获得了HPM在自由空间击穿的系统光学图像,分析了击穿的放电特征。     

高功率微波大气击穿区域分布

大气击穿是高功率微波(HPM)大气传输研究最主要的内容。一方面高功率微波辐射天线近场以振荡场形式存在,在某些局部点形成场强的峰值分布,导致天线近场击穿、天线口径面介质击穿等一系列复杂的问题;另一方面,随着单台微波源功率的大幅提高和功率合成技术的发展,天线远场区的大气击穿问题越来越突出。如何判别是否存在大气击穿,如何确定判断的依据,都是需要解决的问题。论文提出依据击穿阈值和天线辐射场与高度关系曲线的变化规律进行判断。当HPM初始辐射场小于该区域大气击穿阈值,且上述两条曲线之间存在交点,即说明存在HPM辐射天线未击穿而传输路径近场区或远场区可能满足大气击穿条件的情况,这一现象也在相关实验中得到了证实。     

X波段长脉冲高功率微波产生的实验研究

 获得长脉冲高功率微波（HPM）输出是HPM源技术追求的重要目标之一。从物理机理上分析了影响慢波结构HPM器件实现长脉冲HPM输出的因素,并利用长脉冲脉冲功率源和过模慢波结构HPM器件,开展了X波段长脉冲HPM产生实验。实验中,采用介质-铜阴极,并在慢波结构表面镀Cr,在导引磁场约0.7 T、二极管电压约400 kV、电流约10 kA、束流脉宽200 ns的条件下,获得了功率500 MW、脉宽约100 ns、主模为TM₀₁的X波段长脉冲HPM输出。对实验结果的分析表明,脉冲功率源与HPM器件的阻抗不匹配,是导致HPM器件输出微波脉宽比电子束脉宽短、以及HPM器件输出微波功率效率较低的主要原因。     

大气信道对激光脉冲延迟时间影响的仿真研究

分析了大气散射和吸收特性,并进一步研究了大气散射所引起的激光脉冲延迟效应,定量分析了在不同能见度、不同脉冲传输距离、不同散射系数和单程散射反照率的条件下,大气信道所产生激光脉冲传输延迟时间,为探测误差的校正提供了理论依据.通过对仿真结果的分析可知,在衰减系数不变的条件下,大气信道的散射越严重,散射所造成的路径延迟就越大,激光脉冲传输延迟时间也就越长;而大气的吸收效应越明显,激光脉冲传输延迟时间越短.     

FDTD方法分析高功率微波对大气的电离与击穿

 应用麦克斯韦方程和电子流体方程,利用时域有限差分方法(FDTD)计算模拟了高功率微波(HPM)对大气的电离与击穿;该方法用瞬时电场代替等效电场,时刻更新大气电离击穿过程中的电离频率和碰撞频率,消除了近似解析法未考虑大气电离击穿过程中电场幅度衰减而引起的误差,计算得到击穿阈值大小随海拔高度的变化趋势与文献所得的变化趋势相吻合,其值略大于近似解析解;并通过仿真计算分析了HPM脉冲幅值、脉宽以及海拔高度等参数对大气击穿的影响。     

高功率微波天线增益测试方法研究

介绍了几种天线增益的测试方法,并根据高功率微波(HPM)天线的特殊性,提出了一种窄脉冲激励下HPM天线增益测试方法。利用直接功率测量方法,将窄脉冲信号源作为发射信号源,通过标定不同脉冲宽度下接收天线的最大接收功率,开展实验研究,测得窄脉冲条件下天线的增益值。测试结果表明:在脉冲宽度大于25 ns的微波脉冲激励HPM天线时,天线增益测试结果与连续波条件下天线增益测试结果相同。     

电磁波在非均匀碰撞等离子体中的透射增强效应

为研究碰撞等离子体对电磁波传输性质的影响,基于电磁波在介质中的传输特性,将等离子体作为一种特殊的介质,针对一定实验条件下的高功率微波（HPM）大气等离子体与一定范围电磁波的透射特性开展了实验、理论及仿真研究。研究发现:S波段HPM在50 Pa真空下形成的等离子体对不同频率的电磁波透射特性具有较大影响,且在一定频率范围内有规律地出现电磁波透射信号增强效应现象;获取了一系列不同频率连续电磁波穿过HPM等离子体区域的透射波形,并对波形进行了归一化处理,在32.4 GHz下,连续电磁波穿过有无等离子体区域的透射系数约有2倍的差异。建立了仿真模型,获得31.5～32.5 GHz范围内透射系数分布曲线图,穿过等离子体的电磁波出现透射增强效应,且在某些频点上出现了约1.9倍的透射增强。该研究成果为HPM大气等离子体在隐身、应急通讯、黑障通讯等方面的应用提供了重要的技术支撑。     

基于极化强度叠加模型的高功率微波混合气体传播特性

 基于气体极化强度叠加模型,推导了混合气体的介电常数,得到了高功率微波在混合气体中传播时的折射指数和衰减系数。研究发现,高功率微波大气电离产生的混合气体是快速时变的色散有耗介质。根据其色散性分析了微波在混合气体中的传播速度以及微波脉冲在其中的展宽效应,同时,根据其有耗性对微波脉冲在混合气体中传播时的缩短效应进行了研究。研究结果均能自洽地过渡到对流层或电离层电波传播理论。     

Dispersive distortions of a radio-wave pulse in a double-resonance gaseous medium

The problem on dispersive distortions of an electromagnetic pulse in a gaseous medium with two isolated resonant frequencies is solved analytically. The solution is obtained directly in the time region and, thus, is not the result of calculations of the Fourier integral. Without introducing additional assumptions, it is possible to study the regularities and the features of the process of propagation of pulses caused by variations of both their initial characteristics and the parameters of the propagation medium. As an example, the solution is applied to describe the distortions of the two-frequency pulse of subnanosecond duration in the terrestrial atmosphere.     

大气环境下用于瞄准的激光波束传播特性研究

针对激光瞄准过程中的光斑偏移现象,结合修正的Von Karman谱的折射指数起伏和Hufnagel-Vally湍流模型上的近似积分,研究了高斯脉冲光束在湍流大气中远场水平以及斜程传播时的脉冲展宽和闪烁指数,分析了强湍流条件下1.06 μm准单色光斜程大气传输光强分布与脉冲展宽的关系,对数值结果进行比较,发现远距离传输中波长和距离对波束瞄准偏差影响较大.从理论和实验上对大气环境下激光光斑瞄准偏差进行了分析研究,研究结果表明:将激光光斑全场数据及分析结果应用到现有偏差补偿算法中,可以实现激光瞄准偏差的有效补偿,在大气能见度1 km～3 km范围内,激光瞄准偏差测量误差σA≤0.1 mrad.     

带宽对脉冲贝塞尔光束传输的影响

从惠更斯-菲涅耳衍射积分公式出发得到具有高斯型频谱分布的脉冲贝塞尔光束频率域的传输表示式,并使用傅里叶变换最后推导了脉冲贝塞尔光束时间域的传输公式。根据得到的公式通过具体数值计算对脉冲贝塞尔光束在自由空间中的传输进行了研究。计算结果表明脉冲光束的带宽对脉冲贝塞尔光束传输中的脉冲时间延迟和脉冲宽度产生影响。具体表现为脉冲光束带宽的增宽使脉冲时间延迟增大,并使脉冲时间波形的后沿拖长,从而导致脉冲宽度增宽。脉冲时间延迟和脉冲宽度还随传输距离发生变化。脉冲光束传输距离越大,脉冲时间延迟越大,脉冲宽度变得越宽。     

On the theory of short light pulse propagation in a turbulent medium

We consider the problem of propagation of light pulses in a turbulent medium. Within the framework of the used approximation, we obtain a formula for the average intensity of the pulsed signal. Using this formula, we estimate the time delay of the pulse and its broadening. We find the characteristic time scales determining the light pulse transformation in a turbulent medium. The physical meaning of these time scales is explained qualitatively. The quantitative estimates for the Earth’s atmosphere show that the phenomena in question are significant only for very short, picosecond pulses. a. M. Obukhov Institute of the Physics of Atmosphere, Moscow, Russia Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 43, No. 7, pp. 456–467, September, 2000.     

重复频率高功率微波脉冲的大气击穿

 理论研究了重复频率高功率微波脉冲在大气中的传输特性，推导了n个高功率微波脉冲之后空间某点的电子密度，数值模拟并给出了在不同微波频率、大气压强、脉冲宽度以及脉冲间隔的条件下，大气击穿时，透射过去的脉冲个数与微波功率的关系。模拟结果表明：当微波脉冲参数一定时，压强越小，透射过去的脉冲个数越少，大气越容易发生击穿；当压强一定时，脉宽越宽,微波频率越小，透射过去的脉冲个数越少，大气越容易发生击穿。     

高功率光子晶体光纤放大器内超短脉冲的放大传输特性

由速率方程和功率传输方程得到信号脉冲平均功率和增益系数随脉冲传输距离的变化关系.利用Ginzburg-landau方程,在信号脉冲功率的不断增强和增益系数的不断变化的情况下,研究超短脉冲的传输演化特性,发现信号脉冲平均功率、能量和增益系数等参量受到色散和非线性效应的影响相对较小,而信号脉冲的峰值功率、时域和频域特性则易受到色散和非线性效应的影响.探讨了在非线性作用下,脉冲分裂和展宽等所导致的脉宽不稳定性对传输特性的影响,表明研究脉冲传输问题时,引入脉宽不稳定性有利于提高数值模拟准确度.     

Propagation Characteristics of Infrared Pulse Waves through Windblown Sand and Dust Atmosphere

The physics characteristics of the windblown sand and dust atmosphere at the sand bench of Yellow River in China are discussed. The pulse distortion and time delay of infrared nanosecond pulse propagating through the atmosphere having sand and dust particles are investigated at 1.06 and 3.8 μm, respectively. It is shown that the delay of 10 ns laser pulse propagating through 5 km windblown sand and dust atmosphere are over 1 ns and 10 ns at 1.06 and 3.8 μm, respectively. The pulse spread increases slightly with wavelength increase. The pulse spread of a 10 ns laser pulse is over 40 ns at 3.8 μm. The pulse delay and spread increase rapidly with the sand particle density increasing in atmosphere. The narrower the pulse width is, the more the pulse distortion is. Hence, at infrared band, for a laser pulse propagating in sand and dust atmosphere, the pulse delay and spread are quite severe and need be taken into account for a narrower pulse laser system.     

Time-dependent propagation of high energy laser beams through the atmosphere

The computation of time-dependent three-space-dimensional laser beam propagation is described. The methods are applicable to the propagation of high energy laser beams through the atmosphere in the presence of a horizontal wind and turbulence for most situations of interest. Possible cases are propagation of cw beams through stagnation zones, multi-pulse propagation, including the self-consistent treatment of pulse self-blooming, and propagation involving transonic slewing. The solution of the Maxwell wave equation in Fresnel approximation is obtained by means of a discrete Fourier transform method, which, surprisingly, gives excellent results for diffraction problems. The latter provide a stringent test for the accuracy of any solution method. Considerable use is also made of discrete Fourier transform methods in solving the hydrodynamic equations. The treatment of turbulence is based on the generation of random phase screens at each calculation step along the propagation path. In a time-dependent calculation the random phase screens can be either made to move with the wind at a given propagation position or generated anew for each successive time. This work was done under contract to the Advanced Research Projects Agency of the Department of Defense, the Army Missile Command, Huntsville, Alabama, and the U.S. Energy Research and Development Administration.     

Statistical temporal behaviour of pulse wave propagation through continuous random media

Pulse waves propagating through random media suffer distortions, such as fluctuation of arrival time, temporal broadening, and alteration of skewness and kurtosis, due to both the background medium and embedded irregularities. We carry out a study on the temporal behaviour of electromagnetic pulses propagating through random media using temporal moments and an analytic solution of a two-frequency mutual coherence function recently obtained by iteration. We treat the temporal characteristics sequentially, with general expressions obtained first. Then the concise forms are given for pulse propagation in the turbulent non-dispersive atmosphere and the ionosphere, with numerical calculations for the latter. The results show that the mean arrival time is dominated by the term propagating at group velocity, and small corrections arise from higher-order dispersion of the background medium and random scattering of irregularities, but the correction from dispersion of irregularities is neglected as it is so small. As for pulse broadening in trans-ionospheric propagation, the results show that contributions are mainly from the dispersion of the background ionosphere and scattering of electron density irregularities in most cases, and the contribution of dispersion of irregularities is so small that it can be neglected. Finally, we find that the temporal skewness of a trans-ionospheric pulse is negative and its energy is shifted to the leading edge, and the contributions from scattering and dispersion of irregularities dominate over those of background, so the latter can be neglected in most cases.