周边固支环扇形板静力学问题的小波方法

根据相关文献，将拟Shannon小波配置法应用到环扇形板的混合状态方程中，构造出了环扇形板平面方向离散，而厚度方向是解析的混合状态方程。因为用拟Shannon小波张量积表示的近似解是离散形式的，所以固支边界的未知应力可以近似地用内点的应力和位移来表示。数值实例验证了本文方法的正确性。     

Diurnal and seasonal variations of F2 layer characteristics over Irkutsk during the decrease in solar activity in 2003–2006: Observations and IRI-2001 model predictions

The diurnal and seasonal variations of F2 layer characteristics (critical frequency, peak height and bottomside thickness) over Irkutsk, Russia (52.3 N and 104.3 E) are studied by the method of running medians. The comparison with the IRI-2001 model during the decrease in solar activity in 2003–2006 revealed cases of both close agreement and systematic differences between predictions and observations. The systematic difference is not the only reason for disagreement between IRI and observations; there are also intrayear variations which are not associated with seasonal behavior. The period of observation was too short to make conclusions about solar activity dependence of the noon bottomside thickness and the modification of its diurnal behavior with decreasing solar activity.     

Physical mechanism of the vertical electric field generation over active tectonic faults

The concept of the Global Electric Circuit (GEC) provides an explanation of the existence of a vertical atmospheric electric field and coupling between the ground and ionosphere. Presently, ionospheric physics pays more attention to electric fields and coupling processes in the polar and auroral regions, whereas in other areas the potential difference between the ground and ionosphere usually is not taken into account. Regional processes exist, however, that are able to significantly affect the GEC parameters and through modification of the ionospheric potential to create plasma density irregularities of different scales within the ionosphere. One such source of ionosphere modification is air ionization in the vicinity of active tectonic faults, which takes place due to increased radon emanation. This paper considers the process of local modification of the GEC and corresponding ionospheric variability due to tectonic activity.     

弹道快速解法-样条边值法

本文提出了一种弹道计算的新方法，样条边值法，它具有精度高，收敛快的优点。     

NUMERICAL SIMULATION ON MULTI-FLUID INTERFACES

INTRODUCTIONThe study on phenomenon of multi- fluid in-terface driven by shock waves include:( 1 ) totrack the motion of multimaterial interfaces;( 2 )to simulate the chemical reaction on the inter-faces. As the pioneering work,chemical reactionis neglected in this paper. The objective is totrack the interfaces. Of course,the fluids aretreated as compressible medium under such ahigh impact.Although Eulerian schemes workwell for most gas flows,they have been shownto be too dissipative nea…     

计算机翼跨声速绕流的全速位积分方程数值解

本文利用格林定理将全速位方程转换为全速位积分方程，应用高斯定理对沿激波面的显式积分进行简化。将全速位积分方程的解表示成为面元项和场元项之和，然后离散进行数值求解。本文将激波捕捉方法和激波装配技术结合起来，对机翼跨声速绕流进行数值实验，计算结果令人满意。     

超声速平面钝体流动的快速解法

本文介绍了一种平面流动的快速欧拉方程解法。该方法将原参数非定常欧拉方程组重新组合成以广义称曼变量表示的欧拉方程组，再用二点二步迎风格式离散解。针对钝体流动，本文先建立了动网格下的方程，构造了动网格下的算法。提出了一种简单的激波处理方法。计算结果表明，该方法速度快，稳定性好，对初场不敏感。     

双组尾翼弹气动特性计算与分析

本文根据双组尾翼弹的外形特点，选用了代数网格生成方法，通过求角N－S方程，对其气动特性进行了数值计算，并对其计算结果进行了分析。由计算结果可知，此种弹的双尾翼可以为其提供一定的转速和升力，提高其静稳定性。并且此种弹已经用于型号设计。     

Thermal cyclotron radiation from a hot coronal loop with helical magnetic field

The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field.     

高超声速边界层的转捩及预测

首先描述了边界层转捩的基本过程及研究内容。在此基础上,指出了高超声速边界层不同于不可压缩边界层的流动不稳定性特性,并介绍了边界层的转捩机理与感受性特征;给出了高超声速三维边界层中预测转捩的常用方法,并着重介绍了多用于工程实际的e N方法以及对e N方法的理性改进,同时列举了在高超声速三维边界层中应用e N方法实现转捩预测的多个实例。最后,分析并总结了高超声速边界层转捩预测所存在的困难及需要解决的问题。