用电介质镜像法计算线电荷与介质圆柱所形成的电场

利用电介质镜像法计算线电荷与介质圆柱体所形成的电场,给出电势与场强的解析表达式,进一步得出等势线与电场线方程,并利用软件MATLAB绘制出电场线和等势线(面)图予以验证.     

由接地导体限定的无限深槽内线电荷的电场

利用复数坐标系z上的施瓦茨-克利斯多菲变换和镜像法,计算由接地导体限定的无限深槽内线电荷电场中的电势分布和场强分布,给出电场线与等势线方程,并利用数学软件Matlab绘制出其电势分布三维图、电场线和等势线(面)图.     

半圆柱壳电容器内的电场及其电容

利用复数坐标系z上的保角变换,计算半圆柱壳电容器内的电势、场强分布,给出其电场线和等势线方程,绘制出电场线和等势线图,并计算其电容量.     

二维复杂静电场的电场线方程求解及其数值模拟

在保角变换的基础上,给出由C-R条件及静电场的复势求解二维复杂静电场的电场线方程的方法,并利用MATLAB软件绘制出其电场线与等势线(面)分布图.     

线电荷与接地半无限大导体板所形成的电场

将镜像法和保角变换法相结合,计算由线电荷与接地半无限大导体板所形成的电场,给出其电势分布和场强分布,进一步得出等势线方程和电场线方程,并利用数学软件MATLAB绘制出等势线图和电场线图.     

静电场的描绘等势线测试的新方法

“静电场的描绘”实验中,通常采用方法是用一对电极产生的恒定电流模拟一对等量异种电荷产生的静电场．传统测试方法如图１,是用电压表直接测出电场中的几条等势线,根据等势线和电场线垂直的关系画出电场线．但是,这种方法,无论测量如何准确,其所测出的等势线总是发...     

关于《有限长带电导体直线的电荷分布》的商榷

本文指出了一篇文献中有限长带电直线导体的电荷分布线密度公式的错误,用多种方法证明了带电线段的电荷分布是均匀的.推导了均匀带电线段的等势线方程和电场方程,证明带电线段就是等势线,电场线与线段垂直.证明了线段外的电势满足三维拉普拉斯方程,从而证明均匀带电线段是导体.     

均匀带电线与接地导体薄圆筒内的等势线与电场线方程

利用电象法和解析函数的规律,得出均匀带电线与接地薄导体圆筒内的电势和电场强度表达式,并给出了等势线与电场线方程.     

两维电场和电流的可视化

文章利用保角变换和镜像电荷,借助数学软件画出了正方形和正三角形上点电荷和电流对等的等势线和电场线的图形.从上半复平面到矩形或三角形上的保角变换可以用第一类不完全椭圆积分或不完全贝塔函数表示.满足Dirichlet或Neumann边界条件上半复平面上的等势线和电场线可以用镜像电荷(流)方法求得,它们是一系列垂直正交的圆.选取特殊参数,保角变换把这些等势线和电场线映射到正方形或正三角形上,点电荷映射到对称中心,电流映射到顶点.     

线电荷与介质圆柱所形成的电场

在线电荷电场的电势调和展开式的基础上,得出线电荷电场内存在介质圆柱时电势的级数解.并以此来分析长直线电荷与介质圆柱所形成的电场的电像,从而给出电势与电像有关的解析表达式,进一步得出等势线(面)与电场线方程,并利用软件MATLAB绘制出电场线和等势线图予以验证.     

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...