也谈刚体在固定曲面上作纯滚动时接触点的加速度

用矢量分析的方法求出刚体在固定曲面上作纯滚动时接触点、即速度瞬心的加速度的表示式.     

对平面运动刚体加速度瞬心问题的进一步讨论

讨论了与加速度瞬心相关的几个问题,进一步深化了对加速度瞬心概念的理解．     

平面运动刚体加速度瞬心的确定及应用

给出在特殊情况下,确定刚体平面运动加速度瞬心的方法以实例说明加速度瞬心在运动学以及动力学中的应用,可使一些问题求解大为简化．     

关于加速度瞬时中心

本文主要内容包括加速度瞬心的关系式的推导，加速度瞬心的作法简介以及一些有关结论。这些内容在一般教科书上是欠缺的。     

用自然坐标分析平面运动刚体上各点的加速度

介绍了用自然坐标分析平面运动刚体上各点加速度的方法,并用该方法直是明地讨论了瞬心的加速度和刚体绕瞬心的转动方程。     

一道易错的力学习题

指出在确定刚体平面运动的加速度瞬心时一个易犯的错误。     

刚体平面运动的教学设计与讨论

刚体平面运动是理论力学课程刚体力学部分的重点教学内容。本文根据平面运动的特点和学生的认知习惯,在该内容的教学中,首先采用对比教学法分析平面运动与平动的不同,使学生的认识能从简单的平动顺利过渡到复杂的平面运动;然后增加了作平面运动的刚体运动情况能以一个平面的运动情况来代表的证明,让学生对该代表的因果关系达到理论上的认识;接着在介绍速度瞬心的时候补充加速度瞬心的介绍,加深学生对速度瞬心的特点及作用的理解;最后分析了平面运动在讨论运动学问题和动力学问题时的不同分解要求,为进一步讨论刚体平面运动的动力学方程建立作铺垫。     

圆轮在固定面纯滚动时加速度瞬心的轨迹分析

推导了圆轮在固定面上纯滚动时其上任意点的加速度计算公式,数值分析了圆轮在固定面纯滚动时加速度瞬心轨迹的分布规律,可加深理解圆轮纯滚动时的运动规律,为平面运动图形上点的加速度分析提供了另一种有效方法.     

圆周运动加速度一种新的推导方法

主要从加速度的基本定义出发, 给出了一种新的推导方法, 用以推导圆周运动的加速度. 这种推导方法 紧扣加速度的基本定义, 浅显易懂, 有助于学生加深对加速度的理解     

相切型传递的加速度表现

圆盘/摇杆类相切型传递机构是复合运动训练的典型题目,但是传统所用的动点/动系的做法无法推广到边缘曲线为任意形状的情形。为了分析相切型传递的加速度关系,笔者直接使用加速度的定义式,其中速度用基点法获得。通过分析弧长变化率、割线方向、公切线单位矢量导数等极限,最终获得了沿公切向和公法向的加速度分量关系。     

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...