Wave-Particle-Electric Field Synergetic Auroral Electron Acceleration

Space Science Reviews - We discuss afresh the problem of the auroral electron acceleration based on the controversy reports of Bryant, D. A. et al.: 1992, Phys. Rev. Lett. 68, 37, and Borovsky, J.:...     

关于平面激波在凹两段楔面上的传播

众所周知,当一平面激波同任意形状的障碍物相互作用时,将产生十分复杂的波系,其中激波在曲面壁上的绕射和反射,将产生非定常波系。关于平面激波在凹圆柱壁面上的传播,我们可以用一连串、长度为无限小的楔面所构成的多边形来近似和代替凹圆柱面,因此分析和研究激波在两段楔面上反射和绕射的目的在于得出激波在圆柱壁面以及其它较复杂形状壁面上的传播规律。本文采用马赫-曾德干涉仪在激波管上进行光测模型实验。根据所拍摄的流场干涉图像,以分析其波系的演变过程及传播规律,得到有关流场的密度分布和压力分布,更为重要的是给出流场参数的定量结果。     

燃气的基准表及图制定

本文在阐述基准的热力学概念基础上,提出了燃气基准的计算方法,应用CHAPPELL推荐的有关燃气热力性质表达式,导出计算燃气基准的公式,通过微机计算,将结果整理成燃气基准的有关表、图。     

独立函数的表达式及完备性

给出独立函数的逻辑表达式和递推关系式。证明了独立函数系的线性完备性。讨论逻辑函数关于独立函数系的展开式、不同极性独立函数系展式之间的关系,以及与Reed-Muller展式之间的关系。这些问题的结论为建立新型的通用逻辑模块奠定了理论基础。     

一种基于事件序列的故障树最小割集算法

在系统分析故障树最小割集各种求解算法的基础上，提出了一种故障树事件序列的数据结构，并针对该数据结构，设计了一种高效的故障树最小割集求解算法，并对其替换子算法、复制子算法和消减子算法进行了形式化描述。算法可有效降低最小割集生成中的“组合爆炸”问题，实验结果表明算法具有较好的计算性能。     

平面形状误差分离方法的比较分析

就十种典型的精密平面形状误差测量－分离方法的权函数及其零点，作了分析比较。按形状误差谐波抑制最小准则，论证了五点式正交逐次三点法、九点式正交逐次三点法、复合三点法、不对称二维混合法和不对称四点法优于其他方法，不对称四点法则较为理想。     

含有任意多个椭圆孔弹性板的应力场计算

本文应用弹性力学的复变函数理论,用多保角变换的方法,导出了含有任意多个椭圆孔的无限大弹性板多复变量应力函数的表达式。每个孔的大小、位置和孔边作用的载荷均为任意指定。板的无限远处作用有和坐标轴方向一致的均匀拉压载荷P_x,P_y和均匀剪切载荷P_(xy)。并在孔边进行复Fourier级数展开,用待定系数法确定应力函数的未知系数,从而计算弹性板的应力场。编制了相应的FORTRAN77标准化程序,进行了考题和算例分析,给出了级数的收敛状况和孔边周向应力的分布图。     

对地定向三轴稳定卫星的圆锥扫描地球敏感器的数学模型

本文介绍了对地定向三轴稳定卫星的圆锥扫描式地球敏感器的姿态测量原理、输出几何关系和数学模型，并以实际例子说明大角度姿态控制时必须注意敏感器输出的轴间耦合问题     

Solar and Heliospheric Modulation of Galactic Cosmic Rays

The significance of external influences on the environment of Earth and its atmosphere has become evident during recent years. Especially, on time scales of several hundred years, the cosmogenic isotope concentration during the Wolf-, Spoerer-, Maunder- and Dalton-Minimum indicates an increased cosmic ray flux. Because these grand minima of solar activity coincide with cold periods, a correlation of the Earth climate with the cosmic ray intensities is plausible. Any quantitative study of the effects of energetic particles on the atmosphere and environment of the Earth must address their transport to Earth and their interactions with the Earth’s atmosphere including their filtering by the terrestrial magnetosphere. The first problem is one of the fundamental problems in modern cosmic ray astrophysics, and corresponding studies began in the 1960s based on Parker’s cosmic ray modulation theory taking into account diffusion, convection, adiabatic deceleration, and (later) the drift of energetic particles in the global heliospheric magnetic field. It is well established that all of these processes determining the modulation of cosmic rays are depending on parameters that are varying with the solar magnetic cycle. Therefore, the galactic cosmic ray intensities close to Earth is the result of a complex modulation of the interstellar galactic spectrum within the heliosphere. The modern view of this cosmic ray modulation is summarized in our contribution.     

Phase coherence of foreshock MHD waves: wavelet analysis

The earth's foreshock is a region where particularly large amplitude MHD waves are commonly observed. They exhibit various waveforms, suggesting that nonlinear interaction between the waves is in progress. In a previous paper (Hada et al., 2003) we have introduced a method to quantitatively evaluate the strength of phase coherence among the waves from a given time series data. Here we further develop our method by applying wavelet filtering technique. From the analysis it was found that, although the turbulence is consisted of waves with a wide range of plasma rest frame frequencies, only those frequencies lower than the ion gyrofrequency are responsible for generating the phase coherence. This revised version was published online in August 2006 with corrections to the Cover Date.