二维板状激光介质热效应的理论分析

利用二维模型,对固体激光器中侧面双向泵浦板状激光介质的热效应进行了理论分析,重点研究了介质热物性的温度依存性对其最高温度和最大应力的影响,给出了一种计算介质内最高温度和最大应力的简便方法,并与数值模拟结果进行了对比。结果表明,不考虑介质热物性随温度的变化,将导致计算结果特别是热应力结果偏小。考虑介质热物性随温度的变化时,应用本文提出的简便方法计算得到的最高温度和最大应力与数值模拟结果基本吻合.     

X射线在介质中的剂量分布计算

研究了放射治疗中X射线在介质中的输运过程, 编程实现了基于蒙特卡罗方法的剂量计算. 并在便于图形处理的软件Matlab中对光子输运结果进行了可视化处理. 对X射线在均匀介质和非均匀介质中的蒙特卡罗模拟结果与实测结果、其他蒙特卡罗软件模拟结果进行了比较, 结果符合较好. 实验结果表明该方法既可以获得很快的仿真速度, 又能得到精确直观的剂量计算结果, 为提高放射治疗水平具有重要的指导意义和应用价值.     

阻抗梯度飞片加载下的超高速发射二维数值模拟方法

阻抗梯度飞片准等熵加载和超高速发射的二维数值模拟,在计算方法上集中体现了多介质、多界面、大变形、高密度比等特点.采用多介质流体高精度PPM计算方法,以VOF为基础研制MFPPM2二维计算程序,数值模拟Sandia实验室的超高速发射实验模型,获得了与Sandia实验室数值计算一致的结果.     

金属圆筒内爆轰波对碰效应的欧拉数值模拟

运用基于Youngs技术的多介质欧拉方法及应用该方法研制的二维多介质弹塑性流体动力学欧拉程序meph2d对金属圆筒内爆轰波相互作用过程进行了数值模拟并获得成功，计算图像与实验照片吻合，计算结果与实验测量结果符合较好。说明采用多介质欧拉方法可以对此类爆轰波相互作用及爆轰驱动问题进行有效的数值模拟。     

热辐射输运问题的高效蒙特卡罗模拟方法

惯性约束聚变研究中,热辐射光子在介质中的输运以及热辐射光子与介质的相互作用是重要研究课题,蒙特卡罗方法是该类问题的重要研究手段之一.隐式蒙特卡罗方法虽然能正确地模拟热辐射在介质中的输运过程,但当模拟重介质(材料的吸收系数大)问题时,该方法花费的计算时间将变得很长,导致模拟效率很低.本文以离散扩散蒙特卡罗方法为基础,开发了"离散扩散蒙特卡罗方法辐射输运模拟程序",可以较好地解决重介质区的计算效率问题,但是离散扩散蒙卡罗方法在模拟轻介质区时精度不够高.辐射输运问题中通常既有轻介质也有重介质,为了能同时解决蒙特卡罗方法模拟的效率和精度问题,本文研究了离散扩散蒙特卡罗方法与隐式蒙特卡罗方法相结合的模拟方法,并提出了新的扩散区与输运区界面处理方法,研制了混合蒙特卡罗方法的辐射输运模拟程序.典型辐射输运问题模拟显示:在模拟重介质问题时,该程序能大幅缩短模拟时间,且能取得与隐式蒙特卡罗方法一致的结果;在模拟轻重介质均存在的问题时,与隐式蒙特卡罗方法相比,混合蒙特卡罗方法的模拟精度与其相当且计算效率同样能够得到显著提升.     

Lattice Boltzmann方法模拟多孔介质Klinkenberg效应

格子Boltzmann数值模拟方法是研究复杂的多孔介质结构特别是Klinkenberg效应的有效方法之一，对处理复杂边值问题尤其有效，用格子Boltzmann方法研究了气流穿越多孔介质问题，并将数值计算结果与实验结果进行了比较，结果表明格子Boltzmann方法是数值模拟气流穿越多孔介质问题的有效方法之一。     

带状电缆的直流X射线辐照响应

对真空环境下带状电缆模型直流X射线辐照响应进行了实验和数值模拟研究;研制了电缆直流X射线辐照实验系统;使用蒙特卡罗模拟软件计算了直流X光机产生的X射线能谱、通量等参数;建立了带状电缆X射线辐照响应一维计算模型,该计算模型包括电缆导体与介质层间隙和介质层电导率模型。实验测量了两个带状电缆模型的直流X射线辐照响应电流波形,并对其进行了数值模拟。结果显示,在一定的电缆导体与介质层间隙大小假设条件下,采用带状电缆X射线辐照响应计算模型计算的结果与实验测量结果在波形特征和绝对幅度方面比较接近,说明了利用该模型描述电缆直流X射线辐照响应具有其合理性。     

气体和气溶胶在多孔介质中迁移的数值模拟

为了研究多孔介质对气体和气溶胶的封闭能力,用数值方法模拟了气体和气溶胶在多孔介质中的迁移.考虑了渗透、吸附过滤、扩散、热传导等因素,在柱对称坐标下用双孔双渗模型进行了数值模拟,并与实验结果进行了比较.计算结果显示,多孔介质对气溶胶有较强的阻挡作用,模拟实验结果也证明了这一点.     

随机四参数法生成多孔介质及渗流模拟

本文基于多孔介质内流动的广泛应用背景,模拟了多孔介质渗流。采用随机四参数生长法生成了多孔介质模型,并对模型中的微小固相进行了过滤处理。将随机四参数生长法生成的多孔介质结合格子玻尔兹曼方法D2Q9模型模拟了压力驱动的多孔介质中的渗流。通过将模拟结果与著名的CK理论公式的计算结果进行比较,发现在孔隙率高时误差较小(φ=0.9时,误差约为6%)。研究表明在高孔隙率时采用文中的方法得到的多孔介质渗透率及孔隙尺度的流动结果较为准确。     

多孔介质模型在管壳式换热器数值模拟中的应用

本文详细讨论了多孔介质模型在管壳式换热器数值模拟中的应用,开发了一套能自动生成多孔介质特性参数的通用程序。该程序主要基于三维交错网格及SIMPLE算法,然后运用该模型,采用改进的κ-ε模型和壁面函数法,对换热器壳侧的湍流流动进行了数值模拟。计算结果与换热器冷态实验结果符合良好,表明该模型和计算方法是切实可行的。     

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...