微波后射特性测量实验的研究

利用普通微波分光仪研究微波的反射特性,能够出不同材料和不同厚度平板在不同入射角时对微波的反射强度。原理直观,物理规律明显,简单且实用。     

测量介质微波吸收的实验研究

利用微波分光仪测量介质板的微波吸收系数,考虑了接收器和介质板对微波的反射影响.沿波传播方向移动介质板的位置来测量微波强度的极大值和极小值,以它们的平均值作为透射波的强度.还考虑了介质板两个界面的反射对入射波强度的影响.     

量子微波制备方法与实验研究进展

量子微波信号既保留了经典微波信号的空间远距离传播能力,又具有非经典的量子特性,为微波频段量子通信、量子导航及量子雷达等基于大尺度动态空间环境无线传输的量子信息技术提供了可资利用的重要信号源.按照腔量子电动力学系统、超导电路量子电动力学系统和腔–光(电)–力学系统三大类型实验平台,归纳、分析了微波单光子、纠缠微波光子以及压缩微波场和纠缠微波场的产生原理、方法和相关典型实验的进展,并探讨了非经典微波场在量子导航等自由空间传输系统应用中需重点解决的若干关键问题.     

相对论速调管放大器中微波的相位抖动研究

相位抖动对于相对论速调管放大器来讲是一个重要参数,同微波器件的物理过程密切联系,论文从影响器件相位抖动的物理过程出发,结合模拟程序,研究不同条件下放大器的微波相位抖动,给出影响器件微波相位抖动的物理因素.当微波器件实现稳定放大工作时,输出微波相对于注入微波的相位抖动主要由电子束束压波形的抖动和纹波引起,在一定范围内相位抖动与这种波动成线性关系. 关键词： 相对论速调管放大器 相位抖动 微波器件     

任意时间分布电子束同单间隙微波腔的非线性自洽过程

在高功率微波（HPM）的研究中，电子束同微波腔中微波场相互作用是大家所关心的问题，微波腔中电子束与微波场的相互作用，是一个闭环过程，微波场影响电子的运动，同时电子束作为电流源也产生辐射，影响微波场。不同微波腔的微波场不同，电子束同微波场的相互作用形式也不相同，但是在微波场作用下电子束群聚，群聚的电子束反过来影响微波场的自洽过程。     

压缩空气微波等离子体发射光谱的实验研究

利用微波等离子体发生装置,以压缩空气为工作气体,在1～5 atm气压下激发了微波等离子体。使用光谱测量系统,对不同气压和不同入射微波功率情况下的压缩空气微波等离子体的发射光谱进行了实验研究。结果显示,在其他条件不变时,随着气压升高,压缩空气微波等离子体的带状连续谱特征逐渐减弱;随着入射微波功率降低,带状连续谱强度逐渐减弱而带状连续谱特征依然显著。实验结果为了解压缩空气微波等离子体的光谱特性和NO活性基团的产生条件提供了实验依据。     

微波谐振腔中电子与微波作用的非稳态过程研究

 在微波腔中微波场影响电子的运动，同时电子束作为电流源也产生辐射，影响微波场，这种相互作用包含线性和非线性过程。根据Maxwell理论，微波腔中的实际微波场可以按微波腔的模式展开，而且不同模式与电子束之间的相互作用不同。将电子束作为激励源，根据Maxwell方程和电子受到的洛伦兹力，建立不同模式在电子束作用下的激励方程和电子束电子在不同模式作用下的运动方程（即微波谐振腔中电子束与微波场相互作用的自洽方程组），并由此进一步分析一维情况下单间隙微波腔中微波建场、辐射场呈指数增长和饱和等非稳态作用过程，该过程涉及到电子束与微波作用的线性和非线性过程。     

基于可调光延迟线的光子学微波频率测量

提出了一种基于可调光延迟线的光子学微波频率测量方法.经同一微波信号调制的两个不同波长光载波在经过一段可调色散介质传输后,解调输出两路具有不同相位的微波信号,得到的相干微波功率随着色散量的改变出现周期性变化,由此周期可得到输入微波频率值.采用由8个磁光开关和1.6 km单模光纤构成的7-bit光纤延迟线实现色散量的调节....     

开槽管微波腔中微波场分布初步研究

开槽管微波腔已被用于铷原子频标,但是其中的微波场分布尚不清楚. 利用高频结构仿真软件(HFSS)获得了开槽管微波腔内微波场的分布,利用激光-微波双共振方法实现了微波腔场分布的实验测量,所得结果与理论结果一致. 研究结果表明,腔内微波场磁力线呈轴向分布,这表明该种微波腔是适用于原子频标的. 研究结果还表明,腔内微波场存在明显的空间不均匀性,这会导致一些区域的原子不能充分利用,限制原子的钟跃迁信号强度. 因此,现有的开槽管腔结构还有改进的余地.     

基于纠缠见证的路径纠缠微波检测方法

提出了一种基于纠缠见证的路径纠缠微波信号检测方法.路径纠缠微波是微波频段上的连续变量纠缠,介绍了利用微波压缩态和微波分束器制备路径纠缠微波的方法.根据部分转置正定判据以及2?2纠缠态密度矩阵的部分转置具有负本征值的性质,分别对常见的两种2?2纠缠进行了纠缠见证算符的构造,用于对两路信号是否为纠缠态进行判定.将连续变量纠缠的路径纠缠微波分解为大量2?2纠缠子系统叠加的纠缠态,证明其能够利用所构造的2?2纠缠见证算符来检测路径纠缠微波.同时分析了微波分束器的作用,并利用微波分束器设计了一种用于检测路径纠缠微波信号的实验方案,并在理论上分析了纠缠检测所得到的结果.结果表明,该方法能够有效检测路径纠缠微波信号,降低了检测的复杂度和计算量.本文的研究为纠缠微波的检测提供了思路.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...